diff --git a/.github/workflows/swift.yml b/.github/workflows/swift.yml
index 7b195ac..fc01ce5 100644
--- a/.github/workflows/swift.yml
+++ b/.github/workflows/swift.yml
@@ -2,32 +2,75 @@ name: Swift
on:
push:
- branches: [ main ]
+ branches: [main]
pull_request:
- branches: [ main ]
+ branches: [main]
+
+permissions:
+ contents: read
jobs:
- macos:
- runs-on: macos-13
- steps:
- - name: Checkout
- uses: actions/checkout@v3
- - name: Setup Swift
- uses: swift-actions/setup-swift@v1
- - name: Build
- run: swift build -v
- - name: Run tests
- run: swift test -v
- linux:
- runs-on: ubuntu-latest
- container:
- image: swift:5.9
+ build-and-test:
+ name: Swift 6.4 on ${{ matrix.os }}
+ runs-on: ${{ matrix.os }}
+ strategy:
+ fail-fast: false
+ matrix:
+ include:
+ - os: macos-latest
+ build-system: swiftbuild
+ # Use the previous backend while investigating opaque Linux/Windows failures.
+ - os: ubuntu-24.04
+ build-system: native
+ - os: windows-latest
+ build-system: native
steps:
- - name: Checkout
- uses: actions/checkout@v3
- - name: Setup Swift
- uses: swift-actions/setup-swift@v1
- - name: Build
- run: swift build -v
- - name: Run tests
- run: swift test -v
+ - name: Checkout
+ uses: actions/checkout@v6
+ - name: Set up Swift 6.4
+ if: runner.os != 'Windows'
+ uses: swift-actions/setup-swift@v3
+ with:
+ swift-version: "6.4"
+ - name: Set up Swift 6.4 on Windows
+ if: runner.os == 'Windows'
+ uses: SwiftyLab/setup-swift@v1.14.0
+ with:
+ swift-version: "6.4"
+ - name: Show Swift version
+ run: swift --version
+ - name: Build
+ shell: bash
+ run: |
+ set -o pipefail
+ status=0
+ swift build --build-system "${{ matrix.build-system }}" --very-verbose --no-color-diagnostics 2>&1 | tee swift-build.log || status=$?
+ if [ "$status" -ne 0 ]; then
+ echo "::group::Swift build error summary"
+ grep -n -m 30 -E '(fatal )?error:|[Ss]ignal [0-9]+|[Kk]illed|[Cc]rash' swift-build.log || true
+ echo "::endgroup::"
+ fi
+ exit "$status"
+ - name: Run tests
+ shell: bash
+ run: |
+ set -o pipefail
+ status=0
+ swift test --build-system "${{ matrix.build-system }}" --very-verbose --no-color-diagnostics 2>&1 | tee swift-test.log || status=$?
+ if [ "$status" -ne 0 ]; then
+ echo "::group::Swift test error summary"
+ grep -n -m 30 -E '(fatal )?error:|[Ss]ignal [0-9]+|[Kk]illed|[Cc]rash' swift-test.log || true
+ echo "::endgroup::"
+ fi
+ exit "$status"
+ - name: Upload failure diagnostics
+ if: failure()
+ uses: actions/upload-artifact@v4
+ with:
+ name: swift-diagnostics-${{ runner.os }}
+ retention-days: 7
+ include-hidden-files: true
+ path: |
+ swift-build.log
+ swift-test.log
+ .build/**/*.dia
diff --git a/.gitignore b/.gitignore
index 95c4320..6ba4f9e 100644
--- a/.gitignore
+++ b/.gitignore
@@ -3,3 +3,11 @@
/Packages
/*.xcodeproj
xcuserdata/
+
+# Optional local JPL exports; never package multi-gigabyte ephemerides.
+/Data/DE441/
+
+# Reproducible JPL extraction caches and optional local kernel collections.
+/Data/JPL/cache/
+/Data/JPL/SPK/
+/Tools/SmallBodies/__pycache__/
diff --git a/.swiftpm/xcode/package.xcworkspace/contents.xcworkspacedata b/.swiftpm/xcode/package.xcworkspace/contents.xcworkspacedata
deleted file mode 100644
index 706eede..0000000
--- a/.swiftpm/xcode/package.xcworkspace/contents.xcworkspacedata
+++ /dev/null
@@ -1,7 +0,0 @@
-
-
-
-
-
diff --git a/Data/JPL/pois-smoke-enriched.json b/Data/JPL/pois-smoke-enriched.json
new file mode 100644
index 0000000..158de2c
--- /dev/null
+++ b/Data/JPL/pois-smoke-enriched.json
@@ -0,0 +1,42350 @@
+{
+ "schema": 1,
+ "generated_at": "2026-10-13T18:44:34.354112+00:00",
+ "manifest": {
+ "schema": 1,
+ "mandatory_asteroids": [
+ {
+ "designation": "1",
+ "reason": "Dwarf planet Ceres"
+ },
+ {
+ "designation": "134340",
+ "reason": "Dwarf planet Pluto; retain existing provider when selected"
+ },
+ {
+ "designation": "136108",
+ "reason": "Dwarf planet Haumea"
+ },
+ {
+ "designation": "136199",
+ "reason": "Dwarf planet Eris"
+ },
+ {
+ "designation": "136472",
+ "reason": "Dwarf planet Makemake"
+ }
+ ],
+ "comet_seeds": [
+ {
+ "designation": "1P",
+ "reason": "Historical prominence: Halley"
+ },
+ {
+ "designation": "2P",
+ "reason": "Short-period archetype: Encke"
+ },
+ {
+ "designation": "9P",
+ "reason": "Spacecraft target: Tempel 1"
+ },
+ {
+ "designation": "19P",
+ "reason": "Spacecraft target: Borrelly"
+ },
+ {
+ "designation": "21P",
+ "reason": "Meteor-stream association: Giacobini-Zinner"
+ },
+ {
+ "designation": "26P",
+ "reason": "Unusual activity: Grigg-Skjellerup; spacecraft target"
+ },
+ {
+ "designation": "29P",
+ "reason": "Outbursting distant comet: Schwassmann-Wachmann 1"
+ },
+ {
+ "designation": "55P",
+ "reason": "Meteor-stream association: Tempel-Tuttle"
+ },
+ {
+ "designation": "67P",
+ "reason": "Spacecraft target: Churyumov-Gerasimenko"
+ },
+ {
+ "designation": "73P",
+ "reason": "Fragmentation: Schwassmann-Wachmann 3; parent only"
+ },
+ {
+ "designation": "81P",
+ "reason": "Spacecraft target: Wild 2"
+ },
+ {
+ "designation": "103P",
+ "reason": "Spacecraft target: Hartley 2"
+ },
+ {
+ "designation": "109P",
+ "reason": "Meteor-stream association: Swift-Tuttle"
+ },
+ {
+ "designation": "153P",
+ "reason": "Bright apparition: Ikeya-Zhang"
+ },
+ {
+ "designation": "1995 O1",
+ "reason": "Bright historical apparition: Hale-Bopp"
+ },
+ {
+ "designation": "1996 B2",
+ "reason": "Bright historical apparition: Hyakutake"
+ },
+ {
+ "designation": "2006 P1",
+ "reason": "Bright historical apparition: McNaught"
+ },
+ {
+ "designation": "2011 W3",
+ "reason": "Sungrazing survivor: Lovejoy"
+ },
+ {
+ "designation": "2012 S1",
+ "reason": "Sungrazing disruption: ISON"
+ },
+ {
+ "designation": "2014 Q2",
+ "reason": "Bright apparition: Lovejoy"
+ },
+ {
+ "designation": "2020 F3",
+ "reason": "Bright apparition: NEOWISE"
+ },
+ {
+ "designation": "2023 A3",
+ "reason": "Bright apparition: Tsuchinshan-ATLAS"
+ },
+ {
+ "designation": "2019 Q4",
+ "alias": "2I/Borisov",
+ "reason": "Interstellar comet: Borisov"
+ }
+ ]
+ },
+ "selection": {
+ "asteroids_by_known_diameter": 1000,
+ "additional_trojan_quota": 50,
+ "comets": 100,
+ "comet_policy": "Curated seeds then orbit-family diversity; not an objective interest ranking"
+ },
+ "units": {
+ "diameter": "km",
+ "GM": "km^3/s^2",
+ "density": "g/cm^3",
+ "rot_per": "hours",
+ "orbital_distances": "AU",
+ "orbital_angles": "degrees",
+ "epoch_and_tp": "JD TDB"
+ },
+ "sources": {
+ "2fe70281d3bb13aeed4cb733b75b0a1f45a9608aa1d84e23b1391d8e89b5af32": {
+ "url": "https://ssd-api.jpl.nasa.gov/sbdb_query.api?fields=spkid%2Cpdes%2Cfull_name%2Cname%2Cprefix%2Cclass%2Cdiameter%2Cdiameter_sigma%2Calbedo%2CH%2CGM%2Cdensity%2Crot_per%2Cpole%2Cspec_B%2Cspec_T%2Cepoch%2Ce%2Ca%2Cq%2Ci%2Com%2Cw%2Cma%2Ctp%2Ccondition_code%2Corbit_id&full-prec=true&limit=1000&sb-cdata=%7B%22AND%22%3A%5B%22diameter%7CDF%22%5D%7D&sb-kind=a&sort=-diameter%2Cspkid",
+ "fetched_at": "2026-10-13T18:40:09.253960+00:00",
+ "response_sha256": "6b17716e2f490b6cb49db2fa30cf3133596392e39d2baff1e23f4b8eb8efe778"
+ },
+ "3a6723261a8682c8aafa650f1c169d12cd902510125d20a8c92a9c384e01ed48": {
+ "url": "https://ssd-api.jpl.nasa.gov/sbdb_query.api?fields=spkid%2Cpdes%2Cfull_name%2Cname%2Cprefix%2Cclass%2Cdiameter%2Cdiameter_sigma%2Calbedo%2CH%2CGM%2Cdensity%2Crot_per%2Cpole%2Cspec_B%2Cspec_T%2Cepoch%2Ce%2Ca%2Cq%2Ci%2Com%2Cw%2Cma%2Ctp%2Ccondition_code%2Corbit_id&full-prec=true&sb-cdata=%7B%22AND%22%3A%5B%22pdes%7CEQ%7C134340%22%5D%7D&sb-kind=a",
+ "fetched_at": "2026-10-13T18:40:09.752346+00:00",
+ "response_sha256": "80a27707f8c3a822a03208786224e1ed4ae13d13eab9ceec457d57c0c6a700f2"
+ },
+ "783c49f01f7e4e10f7988667279c5951a639b62a778b93d6d5af5fa100726b4d": {
+ "url": "https://ssd-api.jpl.nasa.gov/sbdb_query.api?fields=spkid%2Cpdes%2Cfull_name%2Cname%2Cprefix%2Cclass%2Cdiameter%2Cdiameter_sigma%2Calbedo%2CH%2CGM%2Cdensity%2Crot_per%2Cpole%2Cspec_B%2Cspec_T%2Cepoch%2Ce%2Ca%2Cq%2Ci%2Com%2Cw%2Cma%2Ctp%2Ccondition_code%2Corbit_id&full-prec=true&sb-cdata=%7B%22AND%22%3A%5B%22pdes%7CEQ%7C136108%22%5D%7D&sb-kind=a",
+ "fetched_at": "2026-10-13T18:40:10.230915+00:00",
+ "response_sha256": "bbfd49c7595bf4ee6d18b3abdc2158d0cce83342a1cb2e36f2487851aef9c3f4"
+ },
+ "847805717dba74bbb57f2b16a2da96c47da16648f2ed6111c13c279eecfa17eb": {
+ "url": "https://ssd-api.jpl.nasa.gov/sbdb_query.api?fields=spkid%2Cpdes%2Cfull_name%2Cname%2Cprefix%2Cclass%2Cdiameter%2Cdiameter_sigma%2Calbedo%2CH%2CGM%2Cdensity%2Crot_per%2Cpole%2Cspec_B%2Cspec_T%2Cepoch%2Ce%2Ca%2Cq%2Ci%2Com%2Cw%2Cma%2Ctp%2Ccondition_code%2Corbit_id&full-prec=true&sb-cdata=%7B%22AND%22%3A%5B%22pdes%7CEQ%7C136199%22%5D%7D&sb-kind=a",
+ "fetched_at": "2026-10-13T18:40:10.728374+00:00",
+ "response_sha256": "9496e5de9e2ac9e8ff6a7fba1596bc118e904891ea76091682deecac92fd5324"
+ },
+ "de3f70b52206977e28ace58045e46763574028a11339feb496adfa0db0ef956a": {
+ "url": "https://ssd-api.jpl.nasa.gov/sbdb_query.api?fields=spkid%2Cpdes%2Cfull_name%2Cname%2Cprefix%2Cclass%2Cdiameter%2Cdiameter_sigma%2Calbedo%2CH%2CGM%2Cdensity%2Crot_per%2Cpole%2Cspec_B%2Cspec_T%2Cepoch%2Ce%2Ca%2Cq%2Ci%2Com%2Cw%2Cma%2Ctp%2Ccondition_code%2Corbit_id&full-prec=true&sb-cdata=%7B%22AND%22%3A%5B%22pdes%7CEQ%7C136472%22%5D%7D&sb-kind=a",
+ "fetched_at": "2026-10-13T18:40:11.237486+00:00",
+ "response_sha256": "4c7e463dfa2772b0d6af3d427e3c60473bc0047c051142ab5a9b7947d98acb52"
+ },
+ "1089f716bfd4421489d69990c7adcbbd78c58ddadef672cb99d5f9eceb5f4de9": {
+ "url": "https://ssd-api.jpl.nasa.gov/sbdb_query.api?fields=spkid%2Cpdes%2Cfull_name%2Cname%2Cprefix%2Cclass%2Cdiameter%2Cdiameter_sigma%2Calbedo%2CH%2CGM%2Cdensity%2Crot_per%2Cpole%2Cspec_B%2Cspec_T%2Cepoch%2Ce%2Ca%2Cq%2Ci%2Com%2Cw%2Cma%2Ctp%2Ccondition_code%2Corbit_id&full-prec=true&limit=50&sb-cdata=%7B%22AND%22%3A%5B%22diameter%7CDF%22%5D%7D&sb-class=TJN&sb-kind=a&sort=-diameter%2Cspkid",
+ "fetched_at": "2026-10-13T18:40:11.865905+00:00",
+ "response_sha256": "2ed66feec07ce6a8854597d2851059b023265d540cc975a8fdaea2dec304fc7d"
+ },
+ "015a3eb2f9d4d145c4c0dff277eb89004f0ac8b2764f58f7dd3e7b84d150f6df": {
+ "url": "https://ssd-api.jpl.nasa.gov/sbdb_query.api?fields=spkid%2Cpdes%2Cfull_name%2Cname%2Cprefix%2Cclass%2Cdiameter%2Cdiameter_sigma%2Calbedo%2CH%2CGM%2Cdensity%2Crot_per%2Cpole%2Cspec_B%2Cspec_T%2Cepoch%2Ce%2Ca%2Cq%2Ci%2Com%2Cw%2Cma%2Ctp%2Ccondition_code%2Corbit_id%2CM1%2CK1%2CM2%2CK2%2CA1%2CA2%2CA3&full-prec=true&sb-kind=c&sb-xfrag=true",
+ "fetched_at": "2026-10-13T18:40:13.326169+00:00",
+ "response_sha256": "6b146f463eb11d80454898446502b906c33211a2644cf37e92a10cf5246426a4"
+ },
+ "d1662a0ab8931ebfef89c68a117f344a470d08142fb3c01a0532c285e5068ff3": {
+ "url": "https://ssd-api.jpl.nasa.gov/sbdb.api?alt-des=true&full-prec=true&phys-par=true&spk=20000001",
+ "fetched_at": "2026-10-13T18:41:33.854491+00:00",
+ "response_sha256": "afeab7061610cb5b2b9a6091edf38d6d67a543cef30ce21b330bebb9b3b4a9ac"
+ },
+ "449f5848c27b6f588cc91c3e3bb2ac3fc3568be56c75caa25241a98bf7879041": {
+ "url": "https://ssd-api.jpl.nasa.gov/sbdb.api?alt-des=true&full-prec=true&phys-par=true&spk=20000002",
+ "fetched_at": "2026-10-13T18:41:34.355930+00:00",
+ "response_sha256": "1644c1fcddc101c582cef98f075ff7e4ae2b228e183c161f58ea3511b5926e6f"
+ }
+ },
+ "bodies": [
+ {
+ "spkid": "20000001",
+ "kind": "asteroid",
+ "data": {
+ "spkid": "20000001",
+ "pdes": "1",
+ "full_name": " 1 Ceres (A801 AA)",
+ "name": "Ceres",
+ "prefix": null,
+ "class": "MBA",
+ "diameter": 939.4,
+ "diameter_sigma": "0.2",
+ "albedo": 0.09,
+ "H": 3.34,
+ "GM": 62.6284,
+ "density": 2.162,
+ "rot_per": 9.07417,
+ "pole": "291.421/66.758",
+ "spec_B": "C",
+ "spec_T": "G",
+ "epoch": 2461200.5,
+ "e": 0.07969229514816586,
+ "a": 2.765552595034094,
+ "q": 2.545159361382861,
+ "i": 10.58802780183462,
+ "om": 80.24862682043221,
+ "w": 73.29421453021587,
+ "ma": 274.4193463761342,
+ "tp": 2461599.841466614,
+ "condition_code": "0",
+ "orbit_id": "48",
+ "source_cache_key": "2fe70281d3bb13aeed4cb733b75b0a1f45a9608aa1d84e23b1391d8e89b5af32"
+ },
+ "selection_reasons": [
+ "Diameter ranking among cataloged values: 1",
+ "Dwarf planet Ceres"
+ ],
+ "sbdb_details": {
+ "orbit": {
+ "pe_used": "DE441",
+ "soln_date": "2021-04-13 11:04:44",
+ "cov_epoch": "2458849.5",
+ "data_arc": "9520",
+ "orbit_id": "48",
+ "last_obs": "2021-01-28",
+ "equinox": "J2000",
+ "rms": ".43153",
+ "epoch": "2461200.5",
+ "first_obs": "1995-01-05",
+ "n_dop_obs_used": 0,
+ "sb_used": "SB441-N373",
+ "model_pars": [],
+ "t_jup": "3.310",
+ "n_del_obs_used": 60,
+ "condition_code": "0",
+ "elements": [
+ {
+ "name": "e",
+ "title": "eccentricity",
+ "units": null,
+ "label": "e",
+ "sigma": "4.7755E-12",
+ "value": ".07969229514816586"
+ },
+ {
+ "sigma": "1.0134E-11",
+ "value": "2.765552595034094",
+ "label": "a",
+ "units": "au",
+ "title": "semi-major axis",
+ "name": "a"
+ },
+ {
+ "sigma": "1.9113E-11",
+ "value": "2.545159361382861",
+ "label": "q",
+ "units": "au",
+ "title": "perihelion distance",
+ "name": "q"
+ },
+ {
+ "label": "i",
+ "sigma": "4.6124E-9",
+ "value": "10.58802780183462",
+ "title": "inclination; angle with respect to x-y ecliptic plane",
+ "name": "i",
+ "units": "deg"
+ },
+ {
+ "title": "longitude of the ascending node",
+ "name": "om",
+ "units": "deg",
+ "label": "node",
+ "value": "80.24862682043221",
+ "sigma": "6.1807E-8"
+ },
+ {
+ "label": "peri",
+ "sigma": "6.6076E-8",
+ "value": "73.29421453021587",
+ "name": "w",
+ "title": "argument of perihelion",
+ "units": "deg"
+ },
+ {
+ "sigma": "6.1728E-9",
+ "value": "274.4193463761342",
+ "label": "M",
+ "units": "deg",
+ "title": "mean anomaly",
+ "name": "ma"
+ },
+ {
+ "sigma": "2.8446E-8",
+ "value": "2461599.841466614066",
+ "label": "tp",
+ "units": "TDB",
+ "name": "tp",
+ "title": "time of perihelion passage"
+ },
+ {
+ "units": "d",
+ "name": "per",
+ "title": "sidereal orbital period",
+ "sigma": "9.2333E-9",
+ "value": "1679.853119758983",
+ "label": "period"
+ },
+ {
+ "units": "deg/d",
+ "name": "n",
+ "title": "mean motion",
+ "sigma": "1.1779E-12",
+ "value": ".21430445064843",
+ "label": "n"
+ },
+ {
+ "sigma": "1.0942E-11",
+ "value": "2.985945828685327",
+ "label": "Q",
+ "units": "au",
+ "name": "ad",
+ "title": "aphelion distance"
+ }
+ ],
+ "not_valid_after": null,
+ "comment": null,
+ "source": "JPL",
+ "moid_jup": "2.0967",
+ "n_obs_used": 1075,
+ "producer": "Davide Farnocchia",
+ "moid": "1.58107",
+ "not_valid_before": null,
+ "two_body": null
+ },
+ "signature": {
+ "source": "NASA/JPL Small-Body Database (SBDB) API",
+ "version": "1.3"
+ },
+ "object": {
+ "orbit_class": {
+ "code": "MBA",
+ "name": "Main-belt Asteroid"
+ },
+ "orbit_id": "48",
+ "pha": false,
+ "des_alt": [
+ {
+ "des": "1943 XB"
+ },
+ {
+ "des": "A899 OF"
+ },
+ {
+ "pri": "A801 AA"
+ }
+ ],
+ "spkid": "20000001",
+ "des": "1",
+ "prefix": null,
+ "shortname": "1 Ceres",
+ "kind": "an",
+ "fullname": "1 Ceres (A801 AA)",
+ "neo": false
+ },
+ "phys_par": [
+ {
+ "units": null,
+ "title": "absolute magnitude",
+ "desc": "absolute magnitude (magnitude at 1 au from Sun and observer)",
+ "name": "H",
+ "sigma": null,
+ "value": "3.34",
+ "notes": "IRAS observations used: 15",
+ "ref": "MPO980521"
+ },
+ {
+ "units": null,
+ "name": "G",
+ "title": "magnitude slope",
+ "desc": "magnitude slope parameter used in the standard asteroid H/G magnitude law",
+ "ref": "PDS3 (MPC 17257)",
+ "notes": "Fit",
+ "sigma": null,
+ "value": "0.12"
+ },
+ {
+ "value": "939.4",
+ "sigma": "0.2",
+ "notes": null,
+ "ref": "Nature vol. 537, pp515-517 (22 September 2016)",
+ "title": "diameter",
+ "desc": "effective body diameter",
+ "name": "diameter",
+ "units": "km"
+ },
+ {
+ "sigma": "0.2 x 0.2 x 0.2",
+ "value": "964.4 x 964.2 x 891.8",
+ "ref": "Nature vol. 537, pp515-517 (22 September 2016)",
+ "notes": "fit w.r.t. center of mass and in body-fixed frame",
+ "desc": "tri(or bi)-axial body dimensions",
+ "title": "extent",
+ "name": "extent",
+ "units": "km"
+ },
+ {
+ "name": "GM",
+ "desc": "standard gravitational parameter: product of the mass (M) and gravitational constant (G)",
+ "title": "GM",
+ "units": "km^3/s^2",
+ "notes": null,
+ "ref": "Nature vol. 537, pp515-517 (22 September 2016)",
+ "sigma": "0.0009",
+ "value": "62.6284"
+ },
+ {
+ "value": "2.162",
+ "sigma": "0.008",
+ "notes": null,
+ "ref": "Nature vol. 537, pp515-517 (22 September 2016)",
+ "units": "g/cm^3",
+ "desc": "bulk density",
+ "title": "bulk density",
+ "name": "density"
+ },
+ {
+ "name": "rot_per",
+ "desc": "body rotation period (synodic)",
+ "title": "rotation period",
+ "units": "h",
+ "notes": "derived from published value: 952.1532 +/- 0.0001 deg./day",
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+ "Diameter ranking among cataloged values: 383",
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+ "Diameter ranking among cataloged values: 453",
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+}
diff --git a/Data/JPL/pois.json b/Data/JPL/pois.json
new file mode 100644
index 0000000..2e0f09e
--- /dev/null
+++ b/Data/JPL/pois.json
@@ -0,0 +1,41777 @@
+{
+ "schema": 1,
+ "generated_at": "2026-10-13T18:44:34.354112+00:00",
+ "manifest": {
+ "schema": 1,
+ "mandatory_asteroids": [
+ {
+ "designation": "1",
+ "reason": "Dwarf planet Ceres"
+ },
+ {
+ "designation": "134340",
+ "reason": "Dwarf planet Pluto; retain existing provider when selected"
+ },
+ {
+ "designation": "136108",
+ "reason": "Dwarf planet Haumea"
+ },
+ {
+ "designation": "136199",
+ "reason": "Dwarf planet Eris"
+ },
+ {
+ "designation": "136472",
+ "reason": "Dwarf planet Makemake"
+ }
+ ],
+ "comet_seeds": [
+ {
+ "designation": "1P",
+ "reason": "Historical prominence: Halley"
+ },
+ {
+ "designation": "2P",
+ "reason": "Short-period archetype: Encke"
+ },
+ {
+ "designation": "9P",
+ "reason": "Spacecraft target: Tempel 1"
+ },
+ {
+ "designation": "19P",
+ "reason": "Spacecraft target: Borrelly"
+ },
+ {
+ "designation": "21P",
+ "reason": "Meteor-stream association: Giacobini-Zinner"
+ },
+ {
+ "designation": "26P",
+ "reason": "Unusual activity: Grigg-Skjellerup; spacecraft target"
+ },
+ {
+ "designation": "29P",
+ "reason": "Outbursting distant comet: Schwassmann-Wachmann 1"
+ },
+ {
+ "designation": "55P",
+ "reason": "Meteor-stream association: Tempel-Tuttle"
+ },
+ {
+ "designation": "67P",
+ "reason": "Spacecraft target: Churyumov-Gerasimenko"
+ },
+ {
+ "designation": "73P",
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+ "Bright apparition: Tsuchinshan-ATLAS"
+ ]
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+ },
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+ "Representative orbit family JFc; ranked by catalog M1, then diameter"
+ ]
+ },
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+ },
+ "selection_reasons": [
+ "Representative orbit family HYP; ranked by catalog M1, then diameter"
+ ]
+ },
+ {
+ "spkid": "1003974",
+ "kind": "comet",
+ "data": {
+ "spkid": "1003974",
+ "pdes": "2024 C2",
+ "full_name": " C/2024 C2 (PANSTARRS)",
+ "name": "PANSTARRS",
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+ },
+ "selection_reasons": [
+ "Representative orbit family CTc; ranked by catalog M1, then diameter"
+ ]
+ },
+ {
+ "spkid": "1004011",
+ "kind": "comet",
+ "data": {
+ "spkid": "1004011",
+ "pdes": "2024 N1",
+ "full_name": " C/2024 N1 (PANSTARRS)",
+ "name": "PANSTARRS",
+ "prefix": "C",
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+ },
+ "selection_reasons": [
+ "Representative orbit family HYP; ranked by catalog M1, then diameter"
+ ]
+ },
+ {
+ "spkid": "1004013",
+ "kind": "comet",
+ "data": {
+ "spkid": "1004013",
+ "pdes": "2024 N3",
+ "full_name": " C/2024 N3 (Sarneczky)",
+ "name": "Sarneczky",
+ "prefix": "C",
+ "class": "HYP",
+ "diameter": null,
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+ "albedo": null,
+ "H": null,
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+ "epoch": 2460834.5,
+ "e": 1.001357062473293,
+ "a": -3695.175295400575,
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+ },
+ "selection_reasons": [
+ "Representative orbit family HYP; ranked by catalog M1, then diameter"
+ ]
+ },
+ {
+ "spkid": "1004072",
+ "kind": "comet",
+ "data": {
+ "spkid": "1004072",
+ "pdes": "2023 RS61",
+ "full_name": " C/2023 RS61 (PANSTARRS)",
+ "name": "PANSTARRS",
+ "prefix": "C",
+ "class": "CTc",
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+ },
+ "selection_reasons": [
+ "Representative orbit family CTc; ranked by catalog M1, then diameter"
+ ]
+ },
+ {
+ "spkid": "1004086",
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+ "data": {
+ "spkid": "1004086",
+ "pdes": "2024 XK14",
+ "full_name": " C/2024 XK14 (Bok)",
+ "name": "Bok",
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+ "A3": null,
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+ },
+ "selection_reasons": [
+ "Representative orbit family HTC; ranked by catalog M1, then diameter"
+ ]
+ }
+ ]
+}
diff --git a/Documentation/README.md b/Documentation/README.md
new file mode 100644
index 0000000..282c64e
--- /dev/null
+++ b/Documentation/README.md
@@ -0,0 +1,73 @@
+# Documentation
+
+Public documentation is authored in seven DocC catalogs, alongside the module sources:
+
+| Module | Catalog |
+| --- | --- |
+| CelMek | [CelMek.docc](../Sources/CelMek/CelMek.docc/CelMek.md) |
+| Math | [Math.docc](../Sources/Math/Math.docc/Math.md) |
+| FluidDynamics | [FluidDynamics.docc](../Sources/FluidDynamics/FluidDynamics.docc/FluidDynamics.md) |
+| Hydrodynamics | [Hydrodynamics.docc](../Sources/Hydrodynamics/Hydrodynamics.docc/Hydrodynamics.md) |
+| Aerodynamics | [Aerodynamics.docc](../Sources/Aerodynamics/Aerodynamics.docc/Aerodynamics.md) |
+| Atmospheres | [Atmospheres.docc](../Sources/Atmospheres/Atmospheres.docc/Atmospheres.md) |
+| MagneticFields | [MagneticFields.docc](../Sources/MagneticFields/MagneticFields.docc/MagneticFields.md) |
+
+The module landing pages curate conceptual guides and API symbols. Internal article
+links use DocC references; repository code links point to the GitHub source tree.
+Roadmaps, working audits, fixture notes and developer architecture policy remain
+repository documents. The former Antora source pages/configuration have been replaced;
+the original bibliography and ERFA license notice remain in this directory.
+
+## Build one module
+
+Use the existing Swift-DocC package plugin:
+
+```sh
+mkdir -p .build/documentation
+swift package generate-documentation --target CelMek --disable-indexing \
+ --output-path .build/documentation/CelMek.doccarchive
+```
+
+In Xcode, select the package scheme and use Product → Build Documentation.
+
+## Build the package archive
+
+With a Swift toolchain that includes `docc merge` (Xcode 16 or newer):
+
+```sh
+python3 Tools/Documentation/build.py
+```
+
+This generates one archive for each library module and merges them into
+`.build/documentation/Physics.doccarchive`, with a package landing page. Build logs
+are retained next to the archives. DocC warnings are treated as build failures.
+The script selects the navigator-index option supported by the installed DocC toolchain. Open the combined archive in Xcode to browse it.
+Output stays under `.build`; no generated archives are checked into the repository.
+
+## Browse in a web browser
+
+Serve the archive over HTTP:
+
+```sh
+python3 Tools/Documentation/preview.py
+```
+
+Open [the local documentation](http://127.0.0.1:8080/documentation). The preview binds
+only to localhost; stop it with Ctrl-C. Use `--port 8081` if the default port is busy,
+or `--archive /path/to/Physics.doccarchive` for another combined archive.
+
+Opening the archive's `index.html` directly with `file://` produces a blank page:
+the DocC web viewer needs HTTP to load its JavaScript and JSON assets from the
+archive root. Open the archive itself in Xcode, or use this browser preview.
+
+When running inside an existing restricted sandbox, pass `--disable-sandbox` to
+avoid nesting SwiftPM's plugin sandbox. Use `--output /path/to/directory` to select
+another output directory. The script grants the plugin write access only to that
+selected output directory.
+
+## Editing guides
+
+Add articles to the owning module's `.docc` catalog and curate them under a `## Topics`
+section on its module landing page. Use `` for conceptual guides and
+double-backtick symbol links for API references. Build the affected module and check
+its DocC diagnostics before submitting changes.
diff --git a/Documentation/antora.yml b/Documentation/antora.yml
deleted file mode 100644
index 492afbc..0000000
--- a/Documentation/antora.yml
+++ /dev/null
@@ -1,8 +0,0 @@
-name: celmek
-version: latest
-nav:
- - modules/ROOT/nav.adoc
-asciidoc:
- attributes:
- bibtex-file: ../attachments/bibliography.bib
- bibtex-style: ieee
diff --git a/Documentation/licenses/ERFA.txt b/Documentation/licenses/ERFA.txt
new file mode 100644
index 0000000..d19fad0
--- /dev/null
+++ b/Documentation/licenses/ERFA.txt
@@ -0,0 +1,56 @@
+The Swift Earth-orientation implementation and series are adapted from ERFA 2.0.1.
+This is a modified Swift implementation, not the official SOFA library.
+
+Copyright (C) 2013-2023, NumFOCUS Foundation.
+All rights reserved.
+
+This library is derived, with permission, from the International
+Astronomical Union's "Standards of Fundamental Astronomy" library,
+available from http://www.iausofa.org.
+
+The ERFA version is intended to retain identical
+functionality to the SOFA library, but made distinct through
+different function and file names, as set out in the SOFA license
+conditions. The SOFA original has a role as a reference standard
+for the IAU and IERS, and consequently redistribution is permitted only
+in its unaltered state. The ERFA version is not subject to this
+restriction and therefore can be included in distributions which do not
+support the concept of "read only" software.
+
+Although the intent is to replicate the SOFA API (other than replacement of
+prefix names) and results (with the exception of bugs; any that are
+discovered will be fixed), SOFA is not responsible for any errors found
+in this version of the library.
+
+If you wish to acknowledge the SOFA heritage, please acknowledge that
+you are using a library derived from SOFA, rather than SOFA itself.
+
+
+TERMS AND CONDITIONS
+
+Redistribution and use in source and binary forms, with or without
+modification, are permitted provided that the following conditions are met:
+
+1 Redistributions of source code must retain the above copyright
+ notice, this list of conditions and the following disclaimer.
+
+2 Redistributions in binary form must reproduce the above copyright
+ notice, this list of conditions and the following disclaimer in the
+ documentation and/or other materials provided with the distribution.
+
+3 Neither the name of the Standards Of Fundamental Astronomy Board, the
+ International Astronomical Union nor the names of its contributors
+ may be used to endorse or promote products derived from this software
+ without specific prior written permission.
+
+THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS
+IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED
+TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A
+PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE COPYRIGHT
+HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL,
+SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED
+TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR
+PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF
+LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING
+NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS
+SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE.
diff --git a/Documentation/modules/ROOT/attachments/bibliography.bib b/Documentation/modules/ROOT/attachments/bibliography.bib
deleted file mode 100644
index 389483e..0000000
--- a/Documentation/modules/ROOT/attachments/bibliography.bib
+++ /dev/null
@@ -1,21 +0,0 @@
-@BOOK{meeus,
- author = {{Meeus}, J.},
- title = "{Astronomical Algorithms: Second Edition}",
- year = 1998,
- publisher = "Willmann-Bell, Inc.",
- isbn = "0-943396-61-1"
-}
-
-@ARTICLE{goffin,
- author = {{Goffin}, E. and {Meeus}, J. and {Steyaert}, C.},
- title = "{An accurate representation of the motion of Pluto}",
- journal = {aap},
- keywords = {Celestial Mechanics, Pluto (Planet), Solar Orbits, Astronomical Coordinates, Least Squares Method, Long Term Effects, Position Errors, Time Series Analysis, PLUTO, MOTION, CELESTIAL MECHANICS, CALCULATIONS, COORDINATES, LONGITUDE, LATITUDE, PROCEDURE, TECHNIQUES, PERTURBATIONS, PARAMETERS, ASTRONOMY, Astronomy; Pluto},
- year = 1986,
- month = feb,
- volume = {155},
- number = {2},
- pages = {323-325},
- adsurl = {https://ui.adsabs.harvard.edu/abs/1986A&A...155..323G},
- adsnote = {Provided by the SAO/NASA Astrophysics Data System}
-}
diff --git a/Documentation/modules/ROOT/nav.adoc b/Documentation/modules/ROOT/nav.adoc
deleted file mode 100644
index 703e461..0000000
--- a/Documentation/modules/ROOT/nav.adoc
+++ /dev/null
@@ -1,3 +0,0 @@
-* xref::index.adoc[]
-* xref::algorithms.adoc[]
-* xref::copyright.adoc[]
diff --git a/Documentation/modules/ROOT/pages/algorithms.adoc b/Documentation/modules/ROOT/pages/algorithms.adoc
deleted file mode 100644
index 322a857..0000000
--- a/Documentation/modules/ROOT/pages/algorithms.adoc
+++ /dev/null
@@ -1,16 +0,0 @@
-= Algorithms
-:bibtex-file: ../attachments/bibliography.bib
-:bibtex-style: ieee
-
-[bibliography]
-== Bibliography
-
-bibliography::[]
-
-== Goffin 2000
-
-Goffin 2000 is described in cite:[goffin] and cite:[meeus].
-
-== VSOP87
-
-
diff --git a/Documentation/modules/ROOT/pages/copyright.adoc b/Documentation/modules/ROOT/pages/copyright.adoc
deleted file mode 100644
index db67ee7..0000000
--- a/Documentation/modules/ROOT/pages/copyright.adoc
+++ /dev/null
@@ -1,10 +0,0 @@
-= Copyright
-
-== CelMek
-
-The CelMek library is copyright to Mattias Holm.
-
-== Third Party
-
-No third party libraries are used at this time.
-
diff --git a/Documentation/modules/ROOT/pages/index.adoc b/Documentation/modules/ROOT/pages/index.adoc
deleted file mode 100644
index f64ea40..0000000
--- a/Documentation/modules/ROOT/pages/index.adoc
+++ /dev/null
@@ -1,3 +0,0 @@
-= CelMek Documentation
-
-
diff --git a/Examples/AttitudeDynamicsDemo/main.swift b/Examples/AttitudeDynamicsDemo/main.swift
new file mode 100644
index 0000000..4ece537
--- /dev/null
+++ b/Examples/AttitudeDynamicsDemo/main.swift
@@ -0,0 +1,47 @@
+// SPDX-License-Identifier: Apache-2.0
+import Foundation
+import CelMek
+import Math
+
+// swift run --disable-sandbox AttitudeDynamicsDemo
+// Newtonian Earth-orbit example with a continuously firing, off-centre engine.
+let reference = Frame(name: "Earth inertial",pseudoInertial: true)
+let body = Frame(parent: reference,name: "Spacecraft axes",pseudoInertial: false)
+let tree = try FrameTree(root: reference)
+let gm = try GravitationalParameter(cubicMetresPerSecondSquared: 3.986004418e14,
+ convention: .newtonian,provenance: PhysicalDataProvenance(source: "Earth game model",version: "1"))
+let context = try RotationalEvaluationContext(inertia: RigidBodyInertia(xx: 200,yy: 300,zz: 400),bodyFrame: body,
+ referenceContext: ForceEvaluationContext(frame: reference,origin: .earth))
+let spacecraft = try SpacecraftState(cartesian: CartesianState(epoch: .j2000,frame: reference,
+ position: SIMD3(7e6,0,0),velocity: SIMD3(0,sqrt(gm.cubicMetresPerSecondSquared/7e6),0)),
+ mass: SpacecraftMassProperties(dryMassKilograms: 1000,propellantMassKilograms: 100))
+let attitude = try AttitudeState(epoch: .j2000,referenceFrame: reference,bodyFrame: body,
+ bodyToReference: Quaternion(angle: .pi/2,axis: SIMD3(0,0,1)))
+let engine = try BodyMountedThruster(bodyFrame: body,thrustNewtons: 1,directionBody: SIMD3(1,0,0),
+ positionBodyMetres: SIMD3(0,1,0),effectiveExhaustVelocityMetresPerSecond: 3000)
+let dynamics = try CoupledSpacecraftDynamics(context: context,
+ forceModels: [CentralGravity(body: .earth,gravitationalParameter: gm)],wrenchModels: [engine])
+let trajectory = try CoupledSpacecraftPropagator(initialState: CoupledSpacecraftState(spacecraft: spacecraft,attitude: attitude),
+ dynamics: dynamics,attitudeOptions: .preset(for: .full),numericalOptions: .preset(for: .full))
+try tree.registerSpacecraftFrame(spacecraft: trajectory.spacecraftProvider,attitude: trajectory.attitudeProvider)
+struct Sample: Encodable {
+ let seconds: Double
+ let positionMetres: [Double]
+ let forceReferenceNewtons: [Double]
+ let angularVelocityBodyRadiansPerSecond: [Double]
+ let quaternionBodyToReferenceXYZW: [Double]
+ let totalMassKilograms: Double
+}
+func array(_ vector: SIMD3) -> [Double] { [vector.x,vector.y,vector.z] }
+let samples = try [0.0,5,10,20].map { seconds in
+ let epoch = try Epoch.j2000.advanced(by: CelMek.Duration(seconds: seconds))
+ let state = try trajectory.state(at: epoch), force = try engine.contribution(for: state,in: context)
+ let q = state.attitude.bodyToReference
+ return Sample(seconds: seconds,positionMetres: array(state.spacecraft.cartesian.position),
+ forceReferenceNewtons: array(force.forceReferenceNewtons),
+ angularVelocityBodyRadiansPerSecond: array(state.attitude.angularVelocityBodyRadiansPerSecond),
+ quaternionBodyToReferenceXYZW: [q.x,q.y,q.z,q.w],totalMassKilograms: state.spacecraft.mass.totalMassKilograms)
+}
+let encoder = JSONEncoder()
+encoder.outputFormatting = [.prettyPrinted,.sortedKeys]
+print(String(decoding: try encoder.encode(samples),as: UTF8.self))
diff --git a/Examples/FluidPhysicsDemo/EntryComparison.swift b/Examples/FluidPhysicsDemo/EntryComparison.swift
new file mode 100644
index 0000000..c604334
--- /dev/null
+++ b/Examples/FluidPhysicsDemo/EntryComparison.swift
@@ -0,0 +1,76 @@
+// SPDX-License-Identifier: Apache-2.0
+import FluidDynamics
+import Foundation
+import Aerodynamics
+import Atmospheres
+
+// Prescribed-attitude, planar entry harness owned by the example, not Aerodynamics.
+// Synthetic capsule coefficients and an ideal pressure-only flat wing are illustrative.
+struct EntryDemoReport {
+ let speed: Double
+ let peakDeceleration: Double
+ let peakDynamicPressure: Double
+ let peakHeatFlux: Double
+ let heatLoad: Double
+}
+
+func entryComparison(winged: Bool, step: Double) throws -> EntryDemoReport {
+ let alpha = winged ? 0.35 : 0.2, mass = winged ? 2000.0 : 1500.0
+ let atmosphere = ISAAtmosphere()
+ let geometry = try FluidReferenceGeometry(areaSquareMetres: 5,momentLengthsMetres: SIMD3(repeating: 2))
+ let capsule = try WholeBodyAerodynamics(geometry: geometry,reynoldsReferenceLengthMetres: 2,
+ model: ConstantBodyCoefficients(value: WindForceCoefficients(drag: 1.4,lift: 0.3)
+ .bodyCoefficients(angleOfAttackRadians: alpha,sideslipRadians: 0),
+ source: "Synthetic entry demonstration",version: "1"))
+ let panels = try (0..<8).map { i in
+ try FluidSurfacePanel(areaSquareMetres: 1.5,centreMetres: SIMD3(0,Double(i)-3.5,0),outwardNormal: SIMD3(0,0,1))
+ }
+ let wing = try SurfacePressureIntegration(panels: panels,referenceLengthMetres: 2,
+ model: ModifiedNewtonianPressure(specificHeatRatio: 1.4,machRange: 5...25))
+ let heating = SuttonGravesHeating(parameters: .earthAirColdWall,coverage: try StagnationHeatingCoverage(
+ speedMetresPerSecond: 1500...8000,densityKilogramsPerCubicMetre: 1e-6...1,
+ noseRadiusMetres: 0.05...1,machNumber: 5...25))
+ let leadingEdge = try SweptCylinderStagnationHeating(referenceSphereModel: heating,
+ referenceSphereRadiusMetres: 1,coverage: heating.coverage)
+ // state = altitude, horizontal speed, downward speed, externally integrated heat per unit area.
+ var state = SIMD4(70000,5000*cos(0.18),5000*sin(0.18),0)
+ var peakDeceleration = 0.0, peakQ = 0.0, peakHeat = 0.0
+ func derivative(_ s: SIMD4) throws -> SIMD4 {
+ let properties = try atmosphere.properties(at: s.x), speed = hypot(s.y,s.z)
+ // Explicit illustrative mean-free-path approximation; not a transport dataset.
+ let path = 6.6e-8*1.225/properties.densityKilogramsPerCubicMetre
+ let flow = try FluidFlow(relativeVelocityMetresPerSecond: SIMD3(speed*cos(alpha),0,speed*sin(alpha)),
+ properties: properties,meanFreePathMetres: path)
+ guard let mach = flow.machNumber, (5...25).contains(mach) else { throw FluidError.outsideCoverage }
+ let loads = try winged ? wing.evaluate(flow: flow).loads : capsule.evaluate(flow: flow)
+ let theta = atan2(s.z,s.y)-alpha
+ let horizontalForce = cos(theta)*loads.forceNewtons.x-sin(theta)*loads.forceNewtons.z
+ let downwardForce = sin(theta)*loads.forceNewtons.x+cos(theta)*loads.forceNewtons.z
+ let query = try StagnationHeatingQuery(flow: flow,gasIdentifier: "earth-air",noseRadiusMetres: winged ? 0.1 : 1,
+ surfacePositionMetres: .zero)
+ let heat = try winged ? leadingEdge.heatFlux(for: query,effectiveSweepRadians: 0.4) : heating.heatFlux(for: query)
+ peakDeceleration = max(peakDeceleration,-(horizontalForce*s.y+downwardForce*s.z)/(mass*speed))
+ peakQ = max(peakQ,flow.dynamicPressurePascals); peakHeat = max(peakHeat,heat.wattsPerSquareMetre)
+ return SIMD4(-s.z,horizontalForce/mass,9.80665+downwardForce/mass,heat.wattsPerSquareMetre)
+ }
+ let count = Int((25/step).rounded())
+ for _ in 0.. TabulatedDragCoefficients {
+ try TabulatedDragCoefficients(samples: [0.0,0.5].flatMap { mach in
+ [1e4,1e8].map { DragCoefficientSample(machNumber: mach,reynoldsNumber: $0,dragCoefficient: coefficient) }
+ },source: "Synthetic steady drag",version: "1")
+}
+let descentFlow = try FluidFlow(relativeVelocityMetresPerSecond: SIMD3(0,0,10),
+ properties: ISAAtmosphere().properties(at: 0))
+let parachute = ParachuteAerodynamics(drag: try DragAreaForces(areaSquareMetres: 20,
+ referenceLengthMetres: 5,forceApplicationPointMetres: SIMD3(0,0,-2),model: demoDragTable(1.5)))
+print("Steady parachute force: \(try parachute.evaluate(flow: descentFlow).forceNewtons) N")
+let balloon = BalloonAerodynamics(buoyancy: try Buoyancy(displacedVolumeCubicMetres: 100),
+ drag: try DragAreaForces(areaSquareMetres: 5,referenceLengthMetres: 5,model: demoDragTable(0.5)))
+let balloonLoads = try balloon.evaluate(flow: descentFlow,
+ field: .hydrostaticGravityMetresPerSecondSquared(SIMD3(0,0,9.80665)))
+print("Balloon gross buoyancy plus drag (weight external): \(balloonLoads.forceNewtons) N")
+
+let molecularGas = try FreeMolecularGas(identifier: "Synthetic single-species example",
+ specificGasConstantJoulesPerKilogramKelvin: 300,source: "Demonstration assumptions")
+let molecularModel = try MaxwellianFreeMolecularTraction(gas: molecularGas,
+ surface: GasSurfaceReflection(specularFraction: 0.2,wallTemperatureKelvin: 300))
+let molecularPanel = try FluidSurfacePanel(areaSquareMetres: 1,
+ centreMetres: SIMD3(1,0,0),outwardNormal: SIMD3(1,0,0))
+let molecularFlow = try FluidFlow(relativeVelocityMetresPerSecond: SIMD3(7000,0,0),
+ densityKilogramsPerCubicMetre: 1e-8,temperatureKelvin: 200,meanFreePathMetres: 20)
+let molecularLoads = try SurfaceTractionIntegration(panels: [molecularPanel],referenceLengthMetres: 1,
+ model: molecularModel).evaluate(flow: molecularFlow).loads
+print("Free-molecular example panel force: \(molecularLoads.forceNewtons) N")
+
+// Nonlinear section/wake coupling; do not wrap the section polar in a separate
+// finite-wing correction, which would count induced drag twice.
+let wakeSegments = try SegmentedWing.rectangular(spanMetres: 8,chordMetres: 2,
+ incidenceRadians: 0.08,model: AirfoilWingSectionModel(airfoil: airfoil)).segments
+let wakeSolver = try NonlinearLiftingLine(segments: wakeSegments,wakeLengthMetres: 800,vortexCoreRadiusMetres: 0.001)
+let wakeResult = try wakeSolver.evaluate { _ in wingFlow }
+print("Nonlinear fixed wake: \(wakeResult.iterations) iterations; residual \(wakeResult.maximumNormalizedCirculationResidual); force \(wakeResult.loads.forceNewtons) N")
+try runEntryComparison()
+try runPropwashExample()
+if CommandLine.arguments.contains("--cfd") { try runCFDBenchmark() }
+try runLiquidExamples()
+if CommandLine.arguments.contains("--compressible") { try runCompressibleExample() }
diff --git a/Examples/TwoBodyGameDemo/main.swift b/Examples/TwoBodyGameDemo/main.swift
new file mode 100644
index 0000000..24f2401
--- /dev/null
+++ b/Examples/TwoBodyGameDemo/main.swift
@@ -0,0 +1,46 @@
+// SPDX-License-Identifier: Apache-2.0
+import Foundation
+import CelMek
+
+// swift run --disable-sandbox TwoBodyGameDemo
+// The output is SI state data suitable for an application's rendering adapter.
+let start = Epoch.j2000
+let end = try start.advanced(by: Duration(seconds: 600))
+let tree = try CelestialFrames.makeTree()
+let planets = try VSOP87Ephemeris(body: earth, coverage: start...end,
+ tdbModel: FairheadTDBModel(), accuracy: .low)
+let centre = try FrameConvertedStateProvider(planets, in: CelestialFrames.icrf, using: tree)
+// The prescribed origin lacks acceleration; this policy is chosen explicitly.
+let inertial = try tree.makeGCRF(earth: centre, accelerationPolicy: .assumeZero)
+let spin = try FixedAxisOrientationProvider(referenceFrame: CelestialFrames.icrf,
+ axis: SIMD3(0,0,1), rate: 7.292115e-5)
+let rotating = try tree.makeBodyFixedFrame(name: "Game Earth spin", centre: centre,
+ orientation: spin, accelerationPolicy: .assumeZero)
+// Explicit Newtonian game model; no relativistic scaling of catalogue GM is inferred.
+let gm = try GravitationalParameter(cubicMetresPerSecondSquared: 3.986004418e14,
+ convention: .newtonian, provenance: PhysicalDataProvenance(source: "Earth game model",
+ version: "1", reference: "ORBITAL_MECHANICS.md"))
+let seed = try CartesianState(epoch: start, frame: inertial, position: SIMD3(7e6,0,0),
+ velocity: SIMD3(0,sqrt(gm.cubicMetresPerSecondSquared/7e6),0))
+let coast = try TwoBodyPropagator(initialState: seed, centralBody: .earth, gravitationalParameter: gm)
+let burn = try ImpulsiveManeuver(epoch: start.advanced(by: Duration(seconds: 300)), frame: inertial,
+ deltaVelocityMetresPerSecond: SIMD3(0,20,0))
+let trajectory = try ManeuveredTwoBodyPropagator(base: coast, maneuvers: [burn])
+let samples = try TrajectorySampler.sample(trajectory, from: start, through: end,
+ step: Duration(seconds: 120), in: rotating, using: tree)
+struct Sample: Encodable {
+ let secondsFromStart: Double
+ let earthBarycentricPositionMetres: [Double]
+ let spacecraftEarthRotatingPositionMetres: [Double]
+ let spacecraftEarthRotatingVelocityMetresPerSecond: [Double]
+}
+let output = try samples.map { sample -> Sample in
+ let earthState = try planets.state(at: sample.epoch, in: CelestialFrames.icrf, using: tree)
+ return Sample(secondsFromStart: try sample.epoch.duration(since: start).seconds,
+ earthBarycentricPositionMetres: [earthState.position.x,earthState.position.y,earthState.position.z],
+ spacecraftEarthRotatingPositionMetres: [sample.position.x,sample.position.y,sample.position.z],
+ spacecraftEarthRotatingVelocityMetresPerSecond: [sample.velocity.x,sample.velocity.y,sample.velocity.z])
+}
+let encoder = JSONEncoder()
+encoder.outputFormatting = [.prettyPrinted, .sortedKeys]
+print(String(decoding: try encoder.encode(output), as: UTF8.self))
diff --git a/Examples/Voyager2GameDemo/README.md b/Examples/Voyager2GameDemo/README.md
new file mode 100644
index 0000000..379c09a
--- /dev/null
+++ b/Examples/Voyager2GameDemo/README.md
@@ -0,0 +1,119 @@
+# Voyager 2 inspired game planning example
+
+Run from the repository root:
+
+```sh
+swift run Voyager2GameDemo > /tmp/voyager2-report.json
+```
+
+In a restricted development sandbox use the same module-cache configuration as the
+other demos:
+
+```sh
+env CLANG_MODULE_CACHE_PATH=/tmp/celmek-clang-cache \
+ SWIFTPM_MODULECACHE_OVERRIDE=/tmp/celmek-swift-cache \
+ swift run --disable-sandbox Voyager2GameDemo > /tmp/voyager2-report.json
+```
+
+No DE/SPICE assets, network service, or CSPICE installation are required. The example
+uses full VSOP87E and the injected Fairhead TDB model, plus an explicit built-in
+leap-second table for historical UTC input/output. It subtracts the Sun's barycentric
+position and velocity to form Sun-relative states in the same ecliptic J2000 axes.
+No metre/AU or barycentric/heliocentric relabelling is implicit.
+
+## What it plans
+
+The [NASA mission fact sheet](https://science.nasa.gov/mission/voyager/fact-sheet/)
+records launch on 1977-08-20 and Jupiter/Saturn/Uranus/Neptune encounters on
+1979-07-09, 1981-08-25, 1986-01-24 and 1989-08-25. The
+[NASA Voyager 2 mission page](https://science.nasa.gov/mission/voyager/voyager-2/)
+supplies launch time 14:29:44 UT. The example uses that launch timestamp and **noon
+UTC** on the encounter reference days, rather than exact historical closest-approach
+instants.
+
+It searches all 81 combinations of -30, 0 and +30 days around the four encounter
+dates. Thirty precomputed zero-revolution, prograde Lambert connectors join Earth,
+Jupiter, Saturn, Uranus and Neptune in the Sun's two-body field. Candidate ranking
+minimizes illustrative parking-orbit injection delta-v plus unresolved encounter
+velocity mismatches. The dates are constraints with a small search window, so matching
+the historical flight time is not an independent prediction of the mission schedule.
+
+A 200 km circular Earth parking orbit is converted into a local hyperbolic departure
+with the Lambert leg's outgoing excess vector. The example samples the actual
+Earth-centred parking/burn/escape propagator and translates those states into the
+heliocentric plotting frame. Its departure calculation includes injection delta-v
+and C3; it does not simulate the launch vehicle, ascent, launch-site plane or staging.
+
+At Jupiter, Saturn and Uranus, incoming/outgoing Lambert velocities are measured
+relative to the moving body. A local unpowered flyby preserves incoming excess speed,
+turns toward the next connector, and respects the configured spherical periapsis
+limit. If the requested turn exceeds that limit, the model clamps it. The report
+shows requested/achieved turn, signed excess-speed mismatch, inferred periapsis altitude
+and the remaining outgoing vector mismatch. That mismatch is **not an implemented
+maneuver or a periapsis burn cost**, and is not silently assigned to spacecraft fuel.
+
+Neptune has no following Lambert endpoint. A final local flyby targets a chosen
+out-of-ecliptic departure at approximately the demo's 5,000 km minimum altitude.
+This demonstrates a fourth flyby without inventing a historical interstellar target.
+
+## Expected result and practical limits
+
+On the development run the chosen dates are the reference encounter days: total
+flight time is about **4,387.90 days (12.01 Julian years)**. The illustrative Earth
+injection is about **7.19 km/s**, with **C3 103.01 km²/s²**. Jupiter/Saturn/Uranus
+connector velocity residuals are approximately **102 / 134 / 13 m/s**. Propagating
+each solar Lambert leg independently reaches its requested endpoint within about
+0.1 m on that run; that is solver agreement, not a bound on mission-model error.
+These are diagnostics, not historical reference fixtures or cross-platform exact values.
+
+The output declares `isContinuousMissionTrajectory: false`. Local flyby, parking/escape
+and solar coast samples are separate views. Finite sphere-of-influence patch times,
+positions and velocities are not solved, and transitions may have discontinuities.
+The solar coasts reach system barycentres; local flybys approximate those as planetary
+centres. Satellite motion, atmospheric/ring constraints, planetary perturbations during
+coasts, navigation corrections and historical spacecraft mass/propellant are omitted.
+Rounded Newtonian GM and spherical equatorial radii are explicit illustrative constants.
+The arbitrary parking plane, terminal turn and safety altitudes are not recovered mission
+parameters. Do not interpret this example as a continuous Voyager reconstruction.
+
+The library's finite encounter-sequence and numerical verification APIs can be used
+for the next refinement: optimize B-plane geometry and dates, connect finite local arcs
+with explicit residual/correction constraints, and propagate the resulting itinerary
+under chosen perturbing forces. The current example intentionally exposes the residuals
+that refinement must resolve.
+
+## Using the samples in a game
+
+The JSON includes legs, flyby diagnostics, flight-time comparison, clock playback and sampled SI
+position/velocity states. Solar coasts contain 49 uniformly spaced samples each;
+parking/departure and local encounters have their own labelled sample groups. Separate
+`phase` values before drawing: joining all rows as one polyline would connect unrelated
+local views and discontinuous patches. Encounter dates are not rest stops or rendezvous.
+
+For playback, retain each leg's `TwoBodyPropagator` and query `state(at:)` at the atomic
+simulation epoch advanced by your time-warp scale. Use the same epoch for body ephemeris
+queries. For prediction query a future covered epoch without mutating the current state;
+choose the appropriate coast segment and display transition residuals explicitly. The
+returned solar propagator itself is not coverage-limited, so the example/application
+must enforce each leg's departure/arrival bounds. Avoid linearly interpolating distant
+render samples as a replacement for orbital propagation.
+
+Rendering can subtract the camera's **Double** position before converting to `Float`,
+with an explicit scene scale. The sample coordinates are Sun-relative metres, not
+camera-relative graphics units; a separate renderer adapter remains roadmap work.
+The `playback` rows exercise the reusable `SimulationClock`: one real second advances
+one 365-day simulation year, followed by pause, reverse and a seek to the Jupiter patch.
+Each row queries the spacecraft and all five prescribed planets at the same epoch.
+A 30-day future query leaves the clock untouched; predictions beyond Neptune are
+omitted instead of extrapolating the itinerary. Segment selection uses the following
+coast at an exact patch epoch, so velocity jumps remain explicit. Orbital display
+samples use `TrajectorySampler` rather than hidden interpolation.
+
+See [time guide](../../Sources/CelMek/CelMek.docc/TimeGuide.md) for clock semantics, bounds and floating-point limits.
+Renderer adapters, persistence and the remaining release-readiness work are separate
+Milestone 9 items.
+
+Playback also exports `spacecraftCentredPlanetPositionsRenderUnits`: five planet
+positions relative to the spacecraft, converted to `Float` after subtracting in
+`Double`, at 1e9 metres per render unit. Axes remain right-handed heliocentric
+axes; the spacecraft renders at zero. See [rendering contracts](../../Sources/CelMek/CelMek.docc/GAME_INTEGRATION.md).
diff --git a/Examples/Voyager2GameDemo/main.swift b/Examples/Voyager2GameDemo/main.swift
new file mode 100644
index 0000000..083cdab
--- /dev/null
+++ b/Examples/Voyager2GameDemo/main.swift
@@ -0,0 +1,238 @@
+// SPDX-License-Identifier: Apache-2.0
+import Foundation
+import CelMek
+import Math
+
+// An asset-free, bounded date search and patched-conic diagnostic, not a mission reconstruction.
+func norm(_ v: SIMD3) -> Double { hypot(hypot(v.x,v.y),v.z) }
+func cross(_ a: SIMD3,_ b: SIMD3) -> SIMD3 {
+ SIMD3(a.y*b.z-a.z*b.y,a.z*b.x-a.x*b.z,a.x*b.y-a.y*b.x)
+}
+func array(_ v: SIMD3) -> [Double] { [v.x,v.y,v.z] }
+func utc(_ y: Int,_ m: Int,_ d: Int,_ seconds: Double = 43200) throws -> Epoch {
+ try Epoch(utc: UTCDate(modifiedJulianDay: GregorianDay(year: y,month: m,day: d).modifiedJulianDay,
+ secondOfDay: CelMek.Duration(seconds: seconds)),using: .iersBulletinC72)
+}
+func label(_ epoch: Epoch) throws -> String {
+ let date = try epoch.utc(using: .iersBulletinC72), day = try GregorianDay(modifiedJulianDay: date.modifiedJulianDay)
+ return String(format: "%04d-%02d-%02d UTC",day.year,day.month,day.day)
+}
+let provenance = try PhysicalDataProvenance(source: "Rounded Newtonian demo constants; spherical body model",version: "Voyager2-demo-1")
+func gm(_ value: Double) throws -> GravitationalParameter {
+ try GravitationalParameter(cubicMetresPerSecondSquared: value,convention: .newtonian,provenance: provenance)
+}
+let launch = try utc(1977,8,20,14*3600+29*60+44)
+let anchors = try [utc(1979,7,9),utc(1981,8,25),utc(1986,1,24),utc(1989,8,25)]
+let coverage = try launch.advanced(by: CelMek.Duration(seconds: -86400))...anchors.last!.advanced(by: CelMek.Duration(seconds: 400*86400))
+let tdb = try FairheadTDBModel()
+let coefficients = [earth,jupiter,saturn,uranus,neptune]
+let ephemerides = try coefficients.map { try VSOP87Ephemeris(body: $0,coverage: coverage,tdbModel: tdb,accuracy: .full) }
+let sunEphemeris = try VSOP87Ephemeris(body: sun,coverage: coverage,tdbModel: tdb,accuracy: .full)
+let heliocentric = Frame(name: "Sun origin; VSOP87E native axes",pseudoInertial: true)
+@MainActor
+func bodyState(_ body: Int,_ epoch: Epoch) throws -> CartesianState {
+ let planet = try ephemerides[body].checkedState(at: epoch), centre = try sunEphemeris.checkedState(at: epoch)
+ guard planet.frame === centre.frame else { throw EphemerisError.frameMismatch }
+ return try CartesianState(epoch: epoch,frame: heliocentric,position: planet.position-centre.position,velocity: planet.velocity-centre.velocity)
+}
+let solarGM = try gm(1.32712440018e20), earthGM = try gm(3.986004418e14)
+let bodies: [BodyIdentifier] = [.jupiterBarycentre,.saturnBarycentre,.uranusBarycentre,.neptuneBarycentre]
+let names = ["Jupiter","Saturn","Uranus","Neptune"]
+let mus = try [1.26686534e17,3.7931187e16,5.793939e15,6.836529e15].map(gm)
+let radii = [71_492e3,60_268e3,25_559e3,24_764e3]
+let minAltitudes = [100_000e3,60_000e3,25_000e3,5_000e3] // Demo limits, not historical closest approaches.
+let offsets = [-30.0,0,30]
+let dates = try anchors.map { date in try offsets.map { try date.advanced(by: CelMek.Duration(seconds: $0*86400)) } }
+let endpoints = try dates.enumerated().map { index,options in try options.map { try bodyState(index+1,$0) } }
+let departure = try bodyState(0,launch)
+struct LegKey: Hashable { let leg,from,to: Int }
+var connectors: [LegKey:LambertSolution] = [:]
+for leg in 0..<4 {
+ for from in 0..<(leg == 0 ? 1 : 3) { for to in 0..<3 {
+ let a = leg == 0 ? departure : endpoints[leg-1][from], b = endpoints[leg][to]
+ connectors[LegKey(leg: leg,from: from,to: to)] = try LambertSolver.solve(
+ departurePosition: a.position,arrivalPosition: b.position,departureEpoch: a.epoch,arrivalEpoch: b.epoch,
+ frame: heliocentric,centralBody: .sun,gravitationalParameter: solarGM,
+ referencePole: SIMD3(0,0,1),direction: .positive)
+ } }
+}
+struct FlybyDiagnostic {
+ let result: UnpoweredFlybyResult
+ let residual: Double
+ let requestedTurn: Double
+ let speedMismatch: Double
+}
+func flyby(_ index: Int,_ epoch: Epoch,_ incoming: SIMD3,_ desired: SIMD3) throws -> FlybyDiagnostic {
+ let speed = norm(incoming), desiredSpeed = norm(desired), u = incoming/speed, w = desired/desiredSpeed
+ let angle = acos(max(-1,min(1,(u*w).sum())))
+ let maximum = 2*asin(1/(1+(radii[index]+minAltitudes[index])*speed*speed/mus[index].cubicMetresPerSecondSquared))
+ let turn = min(angle,maximum*(1-1e-10))
+ let perpendicular = w-u*(u*w).sum(), length = norm(perpendicular)
+ guard length > 1e-12, turn > 1e-12 else { throw FlybyError.degenerateTurn }
+ let outgoing = (u*cos(turn)+perpendicular/length*sin(turn))*speed
+ let frame = Frame(name: "\(names[index]) system origin; VSOP87E native axes",pseudoInertial: true)
+ let request = try FlybyEncounterRequest(body: bodies[index],periapsisEpoch: epoch,frame: frame,
+ gravitationalParameter: mus[index],bodyRadiusMetres: radii[index],minimumPeriapsisAltitudeMetres: minAltitudes[index],
+ incomingExcessVelocityMetresPerSecond: incoming,outgoingExcessVelocityMetresPerSecond: outgoing)
+ let result = try UnpoweredFlyby.solve(request)
+ return FlybyDiagnostic(result: result,residual: norm(result.outgoingExcessVelocityMetresPerSecond-desired),
+ requestedTurn: angle,speedMismatch: desiredSpeed-speed)
+}
+struct Candidate {
+ let indices: [Int]
+ let legs: [LambertSolution]
+ let flybys: [FlybyDiagnostic]
+ let escape: ParkingOrbitTransfer
+ let score: Double
+}
+var best: Candidate?
+for j in 0..<3 { for s in 0..<3 { for u in 0..<3 { for n in 0..<3 {
+ let indices = [j,s,u,n]
+ let legs = (0..<4).map { connectors[LegKey(leg: $0,from: $0 == 0 ? 0 : indices[$0-1],to: indices[$0])]! }
+ var flybys: [FlybyDiagnostic] = []
+ for i in 0..<3 {
+ let centre = endpoints[i][indices[i]]
+ flybys.append(try flyby(i,centre.epoch,legs[i].arrivalState.velocity-centre.velocity,legs[i+1].departureState.velocity-centre.velocity))
+ }
+ let escape = try ParkingOrbitTransfer(parkingRadiusMetres: 6_378_137+200_000,bodyRadiusMetres: 6_378_137,
+ hyperbolicExcessSpeedMetresPerSecond: norm(legs[0].departureState.velocity-departure.velocity),gravitationalParameter: earthGM)
+ let score = escape.deltaVelocityMetresPerSecond+flybys.reduce(0) { $0+$1.residual }
+ if best == nil || score < best!.score { best = Candidate(indices: indices,legs: legs,flybys: flybys,escape: escape,score: score) }
+} } } }
+let selected = best!
+let earthFrame = Frame(name: "Earth origin; VSOP87E native axes",pseudoInertial: true)
+let excess = selected.legs[0].departureState.velocity-departure.velocity
+let normal = cross(excess,SIMD3(0,0,1)); let unitNormal = normal/norm(normal)
+let injection = try selected.escape.plan(kind: .escape,periapsisEpoch: launch,frame: earthFrame,centralBody: .earth,
+ hyperbolicExcessVelocityMetresPerSecond: excess,orbitalNormal: unitNormal)
+// Neptune terminal local flyby targets a chosen out-of-plane departure; no fifth Lambert leg.
+let lastCentre = endpoints[3][selected.indices[3]]
+let lastIncoming = selected.legs[3].arrivalState.velocity-lastCentre.velocity
+let away = lastIncoming/norm(lastIncoming)
+let downward = SIMD3(0,0,-1)+away*away.z
+let terminalTurn = 2*asin(1/(1+(radii[3]+minAltitudes[3])*norm(lastIncoming)*norm(lastIncoming)/mus[3].cubicMetresPerSecondSquared))*(1-1e-10)
+let terminalDesired = (away*cos(terminalTurn)+downward/norm(downward)*sin(terminalTurn))*norm(lastIncoming)
+let terminal = try flyby(3,lastCentre.epoch,lastIncoming,terminalDesired)
+let allFlybys = selected.flybys+[terminal]
+
+struct Sample: Encodable {
+ let phase,utc: String
+ let secondsFromLaunch: Double
+ let heliocentricPositionMetres,heliocentricVelocityMetresPerSecond: [Double]
+}
+var samples: [Sample] = []
+@MainActor
+func append(_ state: CartesianState,_ phase: String) throws {
+ samples.append(Sample(phase: phase,utc: try label(state.epoch),secondsFromLaunch: try state.epoch.duration(since: launch).seconds,
+ heliocentricPositionMetres: array(state.position),heliocentricVelocityMetresPerSecond: array(state.velocity)))
+}
+// Initial orbit and escape are genuine Earth-centred propagated states, translated for plotting.
+for (seconds,phase) in [(-5400.0,"parking orbit"),(-3600,"parking orbit"),(-1800,"parking orbit"),(0,"injection"),(3600,"Earth escape") ] {
+ let e = try launch.advanced(by: CelMek.Duration(seconds: seconds)), local = try injection.trajectory.state(at: e), earth = try bodyState(0,e)
+ try append(CartesianState(epoch: e,frame: heliocentric,position: earth.position+local.position,velocity: earth.velocity+local.velocity),phase)
+}
+struct LegReport: Encodable { let from,to,departureUTC,arrivalUTC: String; let days,endpointResidualMetres: Double }
+var reports: [LegReport] = []
+for i in 0..<4 {
+ let leg = selected.legs[i], coast = try leg.trajectory(), duration = try leg.arrivalState.epoch.duration(since: leg.departureState.epoch).seconds
+ let epochs = try (0...48).map { k in
+ k == 48 ? leg.arrivalState.epoch : try leg.departureState.epoch.advanced(by: CelMek.Duration(seconds: duration*Double(k)/48))
+ }
+ for state in try TrajectorySampler.sample(coast,at: epochs) { try append(state,"Lambert coast \(i+1)") }
+ reports.append(LegReport(from: i == 0 ? "Earth" : names[i-1],to: names[i],departureUTC: try label(leg.departureState.epoch),
+ arrivalUTC: try label(leg.arrivalState.epoch),days: duration/86400,
+ endpointResidualMetres: norm(try coast.state(at: leg.arrivalState.epoch).position-leg.arrivalState.position)))
+}
+struct FlybyReport: Encodable {
+ let body,utc: String
+ let incomingExcessKilometresPerSecond,requestedSpeedMismatchMetresPerSecond,connectorVelocityResidualMetresPerSecond: Double
+ let requestedTurnDegrees,achievedTurnDegrees,periapsisAltitudeKilometres: Double
+ let referenceDateOffsetDays: Double
+}
+let encounters = try allFlybys.enumerated().map { i,f in
+ FlybyReport(body: names[i],utc: try label(f.result.request.periapsisEpoch),incomingExcessKilometresPerSecond: f.result.excessSpeedMetresPerSecond/1000,
+ requestedSpeedMismatchMetresPerSecond: f.speedMismatch,connectorVelocityResidualMetresPerSecond: f.residual,
+ requestedTurnDegrees: f.requestedTurn*180 / .pi,achievedTurnDegrees: f.result.turningAngleRadians*180 / .pi,
+ periapsisAltitudeKilometres: f.result.periapsisAltitudeMetres/1000,
+ referenceDateOffsetDays: try f.result.request.periapsisEpoch.duration(since: anchors[i]).seconds/86400)
+}
+// Local flyby samples are separate views; they are not silently substituted into Lambert legs.
+for (i,f) in allFlybys.enumerated() {
+ for seconds in [-21600.0,-10800,0,10800,21600] {
+ let e = try f.result.request.periapsisEpoch.advanced(by: CelMek.Duration(seconds: seconds))
+ let local = try f.result.trajectory.state(at: e), planet = try bodyState(i+1,e)
+ try append(CartesianState(epoch: e,frame: heliocentric,position: planet.position+local.position,velocity: planet.velocity+local.velocity),"local \(names[i]) flyby")
+ }
+}
+// Playback selects a bounded coast explicitly; exact patch epochs use the following leg.
+let playbackCoasts = try selected.legs.map { try $0.trajectory() }
+@MainActor
+func spacecraft(at epoch: Epoch) throws -> CartesianState {
+ guard epoch >= launch, epoch <= lastCentre.epoch else { throw LambertTransferPlanningError.outsideFlight }
+ for i in 0..<4 where epoch < selected.legs[i].arrivalState.epoch || i == 3 {
+ return try playbackCoasts[i].state(at: epoch)
+ }
+ throw LambertTransferPlanningError.outsideFlight
+}
+struct Playback: Encodable {
+ let mode,utc: String
+ let simulationSecondsFromLaunch,simulationSecondsPerRealSecond: Double
+ let isPaused: Bool
+ let spacecraftPositionMetres: [Double]
+ let prescribedPlanetPositionsMetres: [[Double]]
+ let spacecraftCentredPlanetPositionsRenderUnits: [[Float]]
+ let predictionUTC: String?
+ let predictedSpacecraftPositionMetres: [Double]?
+}
+var clock = try SimulationClock(epoch: launch,rate: 365*86400,coverage: launch...lastCentre.epoch)
+var playback: [Playback] = []
+@MainActor
+func capture(_ mode: String) throws {
+ let epoch = clock.epoch, remaining = try lastCentre.epoch.duration(since: epoch)
+ let lookAhead = try CelMek.Duration(seconds: 30*86400)
+ let future = remaining >= lookAhead ? try clock.prediction(after: lookAhead) : nil
+ let renderAdapter = try RendererAdapter(origin: spacecraft(at: epoch), metresPerRenderUnit: 1e9)
+ let renderPlanets = try (0..<5).map { index in
+ let position = try renderAdapter.adapt(bodyState(index,epoch)).position
+ return [position.x,position.y,position.z]
+ }
+ playback.append(Playback(mode: mode,utc: try label(epoch),simulationSecondsFromLaunch: try epoch.duration(since: launch).seconds,
+ simulationSecondsPerRealSecond: clock.rate,isPaused: clock.isPaused,spacecraftPositionMetres: array(try spacecraft(at: epoch).position),
+ prescribedPlanetPositionsMetres: try (0..<5).map { array(try bodyState($0,epoch).position) },
+ spacecraftCentredPlanetPositionsRenderUnits: renderPlanets,
+ predictionUTC: try future.map(label),predictedSpacecraftPositionMetres: try future.map { array(try spacecraft(at: $0).position) }))
+}
+try capture("start")
+for _ in 0..<12 { try clock.advance(realDuration: CelMek.Duration(seconds: 1)); try capture("forward warp") }
+clock.setPaused(true); try clock.advance(realDuration: CelMek.Duration(seconds: 100)); try capture("paused")
+try clock.setRate(-365*86400); clock.setPaused(false)
+try clock.advance(realDuration: CelMek.Duration(seconds: 1)); try capture("reverse warp")
+try clock.seek(to: selected.legs[0].arrivalState.epoch); try capture("seek Jupiter patch")
+
+struct Output: Encodable {
+ let model,axes,nativeEphemerisAxes,referenceURL: String
+ let flightDays,referenceFlightDays,flightTimeDifferenceDays,injectionDeltaVelocityMetresPerSecond,departureC3SquareKilometresPerSquareSecond: Double
+ let searchedCandidates: Int
+ let isContinuousMissionTrajectory: Bool
+ let assumptions: [String]
+ let legs: [LegReport]; let flybys: [FlybyReport]; let samples: [Sample]; let playback: [Playback]
+}
+let output = Output(model: "Voyager 2 inspired bounded-date Lambert / unpowered flyby diagnostic",axes: heliocentric.name,
+ nativeEphemerisAxes: ephemerides[0].frame.name,referenceURL: "https://science.nasa.gov/mission/voyager/fact-sheet/",
+ flightDays: try lastCentre.epoch.duration(since: launch).seconds/86400,
+ referenceFlightDays: try anchors[3].duration(since: launch).seconds/86400,
+ flightTimeDifferenceDays: try lastCentre.epoch.duration(since: anchors[3]).seconds/86400,
+ injectionDeltaVelocityMetresPerSecond: selected.escape.deltaVelocityMetresPerSecond,
+ departureC3SquareKilometresPerSquareSecond: selected.escape.characteristicEnergySquareMetresPerSquareSecond/1e6,
+ searchedCandidates: 81,isContinuousMissionTrajectory: false,
+ assumptions: ["Encounter reference dates use noon UTC, not exact closest-approach times.",
+ "Search uses -30/0/+30 days around each historical date; timing agreement is constrained, not a free prediction.",
+ "Full VSOP87E positions; system barycentres approximate outer planet centres for local spherical flybys.",
+ "Zero-revolution prograde solar two-body Lambert legs; no planetary perturbations during coasts.",
+ "200 km circular parking orbit is illustrative; no launch vehicle ascent or historical fuel model.",
+ "Rank by injection delta-v plus connector velocity residuals. Residuals are unresolved asymptotic mismatches, not implemented burns.",
+ "Independent local flyby arcs and Earth escape are not finitely patched to coasts; their positions and velocities can differ at transitions.",
+ "Neptune departure is a chosen out-of-plane local flyby, not a reconstructed interstellar trajectory."],
+ legs: reports,flybys: encounters,samples: samples,playback: playback)
+let encoder = JSONEncoder(); encoder.outputFormatting = [.prettyPrinted,.sortedKeys]
+print(String(decoding: try encoder.encode(output),as: UTF8.self))
diff --git a/Experiments/MPCCulling/Catalog.swift b/Experiments/MPCCulling/Catalog.swift
new file mode 100644
index 0000000..32da229
--- /dev/null
+++ b/Experiments/MPCCulling/Catalog.swift
@@ -0,0 +1,132 @@
+// SPDX-License-Identifier: Apache-2.0
+import Foundation
+import CelMek
+import Math
+
+let au = 149_597_870_700.0
+// Explicit experimental Newtonian convention, not a precision ephemeris.
+let solarMu = 1.32712440018e20
+let catalogFrame = Frame(name: "MPC heliocentric ecliptic J2000 experiment", pseudoInertial: true)
+let catalogGM = try! GravitationalParameter(cubicMetresPerSecondSquared: solarMu, convention: .newtonian,
+ provenance: PhysicalDataProvenance(source: "Experimental nominal solar GM", version: "1"))
+enum ExperimentError: Error { case malformed(String), invalidQuery, outsideIndexWindow }
+
+func calendarEpoch(_ year: Int, _ month: Int, _ day: Double) throws -> Epoch {
+ guard (1...9999).contains(year), (1...12).contains(month), day.isFinite else {
+ throw ExperimentError.malformed("calendar date")
+ }
+ let leap = year % 4 == 0 && (year % 100 != 0 || year % 400 == 0)
+ let days = [31, leap ? 29 : 28, 31, 30, 31, 30, 31, 31, 30, 31, 30, 31]
+ guard day >= 1, day < Double(days[month - 1] + 1) else {
+ throw ExperimentError.malformed("calendar date")
+ }
+ let y = month <= 2 ? year - 1 : year
+ let m = month <= 2 ? month + 12 : month
+ let a = floor(Double(y) / 100)
+ let jd = floor(365.25 * Double(y + 4716)) + floor(30.6001 * Double(m + 1)) + day + 2 - a + floor(a / 4) - 1524.5
+ return try Epoch(julianDate: jd, scale: .tt)
+}
+func packedEpoch(_ value: String) throws -> Epoch {
+ let chars = Array(value.utf8)
+ func digit(_ c: UInt8) throws -> Int {
+ if (48...57).contains(c) { return Int(c - 48) }
+ if (65...90).contains(c) { return Int(c - 65) + 10 }
+ throw ExperimentError.malformed("packed epoch \(value)")
+ }
+ guard chars.count == 5 else { throw ExperimentError.malformed("packed epoch \(value)") }
+ return try calendarEpoch(digit(chars[0]) * 100 + digit(chars[1]) * 10 + digit(chars[2]),
+ digit(chars[3]), Double(digit(chars[4])))
+}
+struct OrbitRecord {
+ let id: String
+ let elementEpoch: Epoch? // Comets can omit this; perihelion time remains available.
+ let orbit: TwoBodyPropagator
+ let perihelion: Double
+ let aphelion: Double
+ let maximumSpeed: Double
+ init(id: String, epoch: Epoch, elementEpoch: Epoch?, q: Double, e: Double,
+ inclination: Double, node: Double, peri: Double, anomaly: Double) throws {
+ let elements = try OsculatingOrbitalElements(epoch: epoch, frame: catalogFrame, centralBody: .sun,
+ gravitationalParameter: catalogGM, semiLatusRectumMetres: q * (1 + e), eccentricity: e,
+ inclination: inclination, longitudeOfAscendingNode: node, argumentOfPeriapsis: peri, trueAnomaly: anomaly)
+ self.id = id; self.elementEpoch = elementEpoch
+ orbit = try TwoBodyPropagator(initialState: elements.cartesianState(), centralBody: .sun, gravitationalParameter: catalogGM)
+ perihelion = q; aphelion = e < 1 ? q * (1 + e) / (1 - e) : .infinity
+ maximumSpeed = sqrt(solarMu / q * (1 + e))
+ }
+}
+
+// Bounded-buffer line reader: never creates a String for the entire MPCORB file.
+func readLines(_ url: URL, consume: (String, Int) throws -> Void) throws {
+ let file = try FileHandle(forReadingFrom: url)
+ defer { try? file.close() }
+ var pending = Data(), number = 0
+ while let chunk = try file.read(upToCount: 1 << 20), !chunk.isEmpty {
+ pending.append(chunk)
+ var start = pending.startIndex
+ while let end = pending[start...].firstIndex(of: 10) {
+ number += 1
+ try consume(String(decoding: pending[start.. [OrbitRecord] {
+ var records = [OrbitRecord](), inData = false
+ let radians = Double.pi / 180
+ try readLines(url) { line, number in
+ if !inData { if line.hasPrefix("----------") { inData = true }; return }
+ if line.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty { return }
+ if let limit, records.count >= limit { return }
+ let bytes = Array(line.utf8)
+ guard bytes.count >= 103 else { throw ExperimentError.malformed("MPCORB line \(number): short record") }
+ func field(_ lo: Int, _ hi: Int) -> String {
+ String(decoding: bytes[(lo-1).. Double {
+ guard let x = Double(field(lo, hi)), x.isFinite else { throw ExperimentError.malformed("MPCORB line \(number), columns \(lo)-\(hi)") }
+ return x
+ }
+ let epoch = try packedEpoch(field(21, 25))
+ let e = try numeric(71, 79), a = try numeric(93, 103) * au
+ guard a > 0, e >= 0, e < 1 else { throw ExperimentError.malformed("unsupported asteroid conic at line \(number)") }
+ let anomaly = try ConicAnomaly.from(meanAnomaly: numeric(27, 35) * radians, eccentricity: e).trueAnomaly(eccentricity: e)
+ records.append(try OrbitRecord(id: "mpc:asteroid:" + field(1, 7), epoch: epoch, elementEpoch: epoch,
+ q: a * (1 - e), e: e, inclination: numeric(60, 68) * radians,
+ node: numeric(49, 57) * radians, peri: numeric(38, 46) * radians, anomaly: anomaly))
+ }
+ guard inData else { throw ExperimentError.malformed("missing MPCORB header separator") }
+ return records
+}
+struct CometInput: Decodable {
+ let Orbit_type: String
+ let Designation_and_name: String
+ let Comet_num: Int?
+ let Provisional_packed_desig: String?
+ let Year_of_perihelion: Int, Month_of_perihelion: Int
+ let Day_of_perihelion: Double
+ let Perihelion_dist: Double, e: Double, Peri: Double, Node: Double, i: Double
+ let Epoch_year: Int?, Epoch_month: Int?, Epoch_day: Int?
+}
+func loadComets(_ url: URL) throws -> [OrbitRecord] {
+ try JSONDecoder().decode([CometInput].self, from: Data(contentsOf: url)).map { c in
+ guard let designation = c.Comet_num.flatMap({ _ in c.Designation_and_name.split(separator: "/").first.map(String.init) }) ?? c.Provisional_packed_desig else {
+ throw ExperimentError.malformed("comet without designation")
+ }
+ let epoch = try calendarEpoch(c.Year_of_perihelion, c.Month_of_perihelion, c.Day_of_perihelion)
+ let elementEpoch: Epoch?
+ if let y = c.Epoch_year, let m = c.Epoch_month, let d = c.Epoch_day {
+ elementEpoch = try calendarEpoch(y, m, Double(d))
+ } else {
+ guard c.Epoch_year == nil, c.Epoch_month == nil, c.Epoch_day == nil else {
+ throw ExperimentError.malformed("partial comet element epoch")
+ }
+ elementEpoch = nil
+ }
+ return try OrbitRecord(id: "mpc:comet:" + c.Orbit_type + ":" + designation,
+ epoch: epoch, elementEpoch: elementEpoch, q: c.Perihelion_dist * au, e: c.e,
+ inclination: c.i * .pi / 180, node: c.Node * .pi / 180, peri: c.Peri * .pi / 180, anomaly: 0)
+ }
+}
diff --git a/Experiments/MPCCulling/Checks.swift b/Experiments/MPCCulling/Checks.swift
new file mode 100644
index 0000000..717e336
--- /dev/null
+++ b/Experiments/MPCCulling/Checks.swift
@@ -0,0 +1,31 @@
+// SPDX-License-Identifier: Apache-2.0
+import Foundation
+import CelMek
+
+func checkSyntheticCases() throws {
+ guard try packedEpoch("K2669") == calendarEpoch(2026, 6, 9) else { throw ExperimentError.malformed("packed epoch check") }
+ let records = try [0.0, 0.8, 0.999999, 1.0, 1.2].enumerated().map { i, e in
+ try OrbitRecord(id: "synthetic:\(i)", epoch: .j2000, elementEpoch: .j2000,
+ q: au * 0.1, e: e, inclination: 0.3, node: 0.4, peri: 0.5, anomaly: 0)
+ }
+ let index = try CullingIndex(records: records, epoch: .j2000, halfWindowSeconds: 86400, cellWidth: 0.01 * au)
+ for seconds in [-86400.0, -43200, 0, 43200, 86400] {
+ let epoch = try Epoch.j2000.advanced(by: CelMek.Duration(seconds: seconds))
+ for record in records {
+ let position = try record.orbit.state(at: epoch).position
+ // Zero-radius queries exactly on a body exercise cell crossings and closed bounds.
+ for radius in [0.0, 0.01 * au, au] {
+ let oracle = try matches(records, indices: Array(records.indices), observer: position, radius: radius, epoch: epoch)
+ for spatial in [false, true] {
+ let candidates = try index.candidates(observer: position, radius: radius, epoch: epoch, spatial: spatial)
+ guard oracle.isSubset(of: Set(candidates)) else { throw ExperimentError.malformed("synthetic false negative") }
+ }
+ }
+ }
+ }
+ do {
+ _ = try index.candidates(observer: .zero, radius: -1, epoch: .j2000, spatial: true)
+ throw ExperimentError.malformed("negative radius accepted")
+ } catch ExperimentError.invalidQuery {}
+ print("Synthetic circular/eccentric/near-parabolic/parabolic/hyperbolic checks PASS")
+}
diff --git a/Experiments/MPCCulling/Index.swift b/Experiments/MPCCulling/Index.swift
new file mode 100644
index 0000000..8d52ddb
--- /dev/null
+++ b/Experiments/MPCCulling/Index.swift
@@ -0,0 +1,79 @@
+// SPDX-License-Identifier: Apache-2.0
+import Foundation
+import CelMek
+
+struct Cell: Hashable { let x, y, z: Int }
+struct Bounds {
+ var low = SIMD3(repeating: .infinity)
+ var high = SIMD3(repeating: -.infinity)
+ mutating func include(_ p: SIMD3, padding: Double) {
+ for axis in 0..<3 { low[axis] = min(low[axis], p[axis] - padding); high[axis] = max(high[axis], p[axis] + padding) }
+ }
+ func intersects(_ p: SIMD3, radius: Double) -> Bool {
+ var squared = 0.0
+ for axis in 0..<3 {
+ let d = max(low[axis] - p[axis], max(0, p[axis] - high[axis]))
+ squared += d * d
+ }
+ return squared <= radius * radius
+ }
+}
+struct Bucket {
+ var indices = [Int]()
+ var bounds = Bounds()
+ var radialLow = Double.infinity, radialHigh = -Double.infinity
+}
+struct CullingIndex {
+ let centerEpoch: Epoch
+ let halfWindowSeconds: Double
+ let buckets: [Bucket]
+ let radialBounds: [(Double, Double)]
+ init(records: [OrbitRecord], epoch: Epoch, halfWindowSeconds: Double, cellWidth: Double) throws {
+ guard halfWindowSeconds.isFinite, halfWindowSeconds >= 0, cellWidth.isFinite, cellWidth > 0 else { throw ExperimentError.invalidQuery }
+ centerEpoch = epoch; self.halfWindowSeconds = halfWindowSeconds
+ var cells = [Cell: Bucket](), radial = [(Double, Double)]()
+ radial.reserveCapacity(records.count)
+ for (index, record) in records.enumerated() {
+ let position = try record.orbit.state(at: epoch).position
+ // Perihelion speed is a global speed bound for elliptic, parabolic and hyperbolic two-body motion.
+ // Numerical guard is experimental, not a certified floating-point error bound.
+ let padding = record.maximumSpeed * halfWindowSeconds + 1000 + norm(position) * 1e-12
+ let r = norm(position)
+ let lower = max(0, max(min(record.perihelion, r) - 1000, r - padding))
+ let upper = min(max(record.aphelion, r) + 1000, r + padding)
+ radial.append((lower, upper))
+ let coordinates = (0..<3).map { floor(position[$0] / cellWidth) }
+ guard coordinates.allSatisfy({ $0.isFinite && $0 > Double(Int.min) && $0 < Double(Int.max) }) else { throw ExperimentError.invalidQuery }
+ let cell = Cell(x: Int(coordinates[0]), y: Int(coordinates[1]), z: Int(coordinates[2]))
+ // Mutate through Dictionary's default subscript to avoid copying the bucket's array on every insertion.
+ cells[cell, default: Bucket()].indices.append(index)
+ cells[cell, default: Bucket()].bounds.include(position, padding: padding)
+ cells[cell, default: Bucket()].radialLow = min(cells[cell]!.radialLow, lower)
+ cells[cell, default: Bucket()].radialHigh = max(cells[cell]!.radialHigh, upper)
+ }
+ buckets = Array(cells.values); radialBounds = radial
+ }
+ func candidates(observer: SIMD3, radius: Double, epoch: Epoch, spatial: Bool) throws -> [Int] {
+ guard radius.isFinite, radius >= 0, (0..<3).allSatisfy({ observer[$0].isFinite }) else { throw ExperimentError.invalidQuery }
+ guard abs(try epoch.duration(since: centerEpoch).seconds) <= halfWindowSeconds else { throw ExperimentError.outsideIndexWindow }
+ let r = norm(observer), low = max(0, r - radius), high = r + radius
+ var selected = [Int]()
+ for bucket in buckets {
+ guard bucket.radialLow <= high, bucket.radialHigh >= low else { continue }
+ if spatial && !bucket.bounds.intersects(observer, radius: radius) { continue }
+ for i in bucket.indices {
+ let bounds = radialBounds[i]
+ if bounds.0 <= high && bounds.1 >= low { selected.append(i) }
+ }
+ }
+ return selected
+ }
+}
+func norm(_ p: SIMD3) -> Double { hypot(hypot(p.x, p.y), p.z) }
+func matches(_ records: [OrbitRecord], indices: [Int], observer: SIMD3, radius: Double, epoch: Epoch) throws -> Set {
+ var result = Set()
+ for i in indices {
+ if norm(try records[i].orbit.state(at: epoch).position - observer) <= radius { result.insert(i) }
+ }
+ return result
+}
diff --git a/Experiments/MPCCulling/README.md b/Experiments/MPCCulling/README.md
new file mode 100644
index 0000000..b1b626a
--- /dev/null
+++ b/Experiments/MPCCulling/README.md
@@ -0,0 +1,62 @@
+# MPC culling experiment
+
+Run from the repository root:
+
+```sh
+swift run -c release MPCCullingExperiment
+swift run -c release MPCCullingExperiment --limit 10000
+```
+
+Options: `--data Data/MPC`, `--half-window-days 1`, `--cell-au 0.25`.
+`--limit` limits asteroids only (the text reader still scans the file); all comets are included.
+Requires the caller-supplied MPCORB.DAT and cometels.json, which are not packaged as library resources.
+
+This standalone experiment streams fixed-width asteroid records and decodes comet JSON.
+It prepares Newtonian Sun-centered two-body propagators in ecliptic J2000 axes.
+Asteroids start at their packed TT element epoch; comets start at perihelion, retaining
+optional element epochs separately. Dates are interpreted as TT for this experiment.
+It does not include planetary perturbations or comet nongravitational forces and is
+not a precision replacement for MPC/JPL ephemerides. No source GM/time-scale conversion
+is asserted. Names, photometry and full source metadata are not yet imported.
+
+The index groups positions at a center epoch into Cartesian grid cells. Bounds are
+expanded by perihelion speed times the half-window duration, plus a numerical guard.
+This global two-body speed bound covers motion throughout the window, including
+hyperbolic and parabolic orbits, without relying on endpoint samples. Per-body radial
+bounds intersect swept-radius bounds with whole-orbit perihelion/aphelion bounds.
+Queries scan cell radial bounds, optionally reject sphere/AABB nonintersection, then
+filter individual radial intervals before evaluating selected states. Spatial indexing
+therefore avoids propagation per query but requires one full pass when rebuilt.
+Cell scans are linear in occupied cells; this is a baseline for a future BVH.
+
+The benchmark reports load/preparation, build, selection and evaluation separately.
+Four sphere queries at both window endpoints and its center are checked against
+brute-force exact queries. It also checks stale-index rejection. All geometric
+coordinates and query radii use metres in the same heliocentric axes.
+Bounds are conservative for the chosen ideal two-body model; the floating-point
+padding is pragmatic and not a formally certified error bound. Wide windows or
+small-perihelion comets loosen bounds. Bodies are not truncated or silently skipped
+on loader/evaluator failures. Rebuild after jumps outside the window.
+
+Source data credit: Minor Planet Center. Preserve the complete MPCORB header,
+per-record references and orbit-computer attribution when redistributing source or
+derived datasets. Update information is in Data/MPC/MPCORB.DAT's header. This
+experiment does not write or redistribute a compiled dataset.
+
+## Preliminary full-catalog measurement
+
+2026-10-13, local arm64 release executable, after compilation completed.
+These are indicative single-run measurements, not repeated benchmark medians.
+The full transcript is in `results/full-catalog.txt` (timings recorded to microseconds).
+
+- 1,574,501 records; asteroid load/preparation 6.014 s, comet load/preparation 0.008 s.
+- One-day half-window, 0.25 AU cells: 25,832 occupied cells; build 2.977 s.
+- Full evaluation oracle: 2.403–2.643 s per sphere query (includes distance checks/output collection).
+- Belt probe at (2.7, 0, 0) AU with radius 0.1 AU: 294,308 radial candidates,
+ 5,276 spatial candidates, 535 exact hits at center epoch. Spatial candidate
+ evaluation took 0.021 s at center epoch and 0.009–0.021 s across the three epochs.
+- All 12 full-catalog queries matched brute force; synthetic cases and stale-index rejection passed.
+
+This baseline deliberately uses prepared existing propagators per record, rather
+than the eventual compact structure-of-arrays catalog. It measures the existing
+solver and prioritizes verifying culling correctness before memory optimization.
diff --git a/Experiments/MPCCulling/main.swift b/Experiments/MPCCulling/main.swift
new file mode 100644
index 0000000..1723cf3
--- /dev/null
+++ b/Experiments/MPCCulling/main.swift
@@ -0,0 +1,61 @@
+// SPDX-License-Identifier: Apache-2.0
+import Foundation
+import CelMek
+
+func timed(_ name: String, _ body: () throws -> T) rethrows -> T {
+ let start = DispatchTime.now().uptimeNanoseconds
+ let result = try body()
+ print(String(format: "%@: %.6f s", name, Double(DispatchTime.now().uptimeNanoseconds - start) / 1e9))
+ return result
+}
+let args = Array(CommandLine.arguments.dropFirst())
+func argument(_ key: String, default fallback: String) -> String {
+ guard let i = args.firstIndex(of: key), i + 1 < args.count else { return fallback }
+ return args[i + 1]
+}
+do {
+ try checkSyntheticCases()
+ let root = URL(fileURLWithPath: argument("--data", default: "Data/MPC"))
+ let limit: Int?
+ if args.contains("--limit") {
+ guard let n = Int(argument("--limit", default: "")), n > 0 else { throw ExperimentError.invalidQuery }; limit = n
+ } else { limit = nil }
+ guard let halfDays = Double(argument("--half-window-days", default: "1")),
+ let cellAU = Double(argument("--cell-au", default: "0.25")),
+ halfDays >= 0, halfDays.isFinite, cellAU > 0, cellAU.isFinite else { throw ExperimentError.invalidQuery }
+ let records = try timed("Load/prepare asteroids") { try loadAsteroids(root.appendingPathComponent("MPCORB.DAT"), limit: limit) }
+ + timed("Load/prepare comets") { try loadComets(root.appendingPathComponent("cometels.json")) }
+ guard Set(records.map(\.id)).count == records.count else { throw ExperimentError.malformed("duplicate identities") }
+ print("Records: \(records.count); missing element epochs: \(records.filter { $0.elementEpoch == nil }.count)")
+ let epoch = try calendarEpoch(2026, 10, 13)
+ let index = try timed("Build swept radial/spatial index (includes full evaluation)") {
+ try CullingIndex(records: records, epoch: epoch, halfWindowSeconds: halfDays * 86400, cellWidth: cellAU * au)
+ }
+ print("Cells: \(index.buckets.count); half-window: \(halfDays) days; cell width: \(cellAU) AU")
+ // Fixed locations in the index's heliocentric ecliptic axes; these are query probes, not planet states.
+ let probes: [(String, SIMD3, Double)] = [
+ ("inner", SIMD3(1, 0, 0) * au, 0.1 * au),
+ ("belt", SIMD3(2.7, 0, 0) * au, 0.1 * au),
+ ("Jupiter distance", SIMD3(5.2, 0, 0) * au, 0.25 * au),
+ ("outer", SIMD3(40, 0, 0) * au, au)]
+ for offset in [-halfDays, 0, halfDays] {
+ let queryEpoch = try epoch.advanced(by: CelMek.Duration(seconds: offset * 86400))
+ for (name, observer, radius) in probes {
+ print("Query \(name), offset \(offset) days")
+ let radial = try timed(" Radial selection") { try index.candidates(observer: observer, radius: radius, epoch: queryEpoch, spatial: false) }
+ let spatial = try timed(" Radial + spatial selection") { try index.candidates(observer: observer, radius: radius, epoch: queryEpoch, spatial: true) }
+ let hits = try timed(" Evaluate spatial candidates") { try matches(records, indices: spatial, observer: observer, radius: radius, epoch: queryEpoch) }
+ let oracle = try timed(" Full evaluation oracle") { try matches(records, indices: Array(records.indices), observer: observer, radius: radius, epoch: queryEpoch) }
+ guard hits == oracle, oracle.isSubset(of: Set(radial)) else { throw ExperimentError.malformed("culling missed bodies") }
+ print(" Candidates radial=\(radial.count), spatial=\(spatial.count), exact=\(hits.count); oracle PASS")
+ }
+ }
+ let outside = try epoch.advanced(by: CelMek.Duration(seconds: halfDays * 86400 + 1))
+ do {
+ _ = try index.candidates(observer: .zero, radius: au, epoch: outside, spatial: true)
+ throw ExperimentError.malformed("stale index accepted")
+ } catch ExperimentError.outsideIndexWindow { print("Stale-index rejection PASS") }
+} catch {
+ FileHandle.standardError.write(Data("MPCCullingExperiment: \(error)\n".utf8))
+ exit(1)
+}
diff --git a/Experiments/MPCCulling/results/full-catalog.txt b/Experiments/MPCCulling/results/full-catalog.txt
new file mode 100644
index 0000000..066d51c
--- /dev/null
+++ b/Experiments/MPCCulling/results/full-catalog.txt
@@ -0,0 +1,79 @@
+Synthetic circular/eccentric/near-parabolic/parabolic/hyperbolic checks PASS
+Load/prepare asteroids: 6.013611 s
+Load/prepare comets: 0.007549 s
+Records: 1574501; missing element epochs: 5
+Build swept radial/spatial index (includes full evaluation): 2.977311 s
+Cells: 25832; half-window: 1.0 days; cell width: 0.25 AU
+Query inner, offset -1.0 days
+ Radial selection: 0.000222 s
+ Radial + spatial selection: 0.000033 s
+ Evaluate spatial candidates: 0.001007 s
+ Full evaluation oracle: 2.412656 s
+ Candidates radial=6422, spatial=496, exact=74; oracle PASS
+Query belt, offset -1.0 days
+ Radial selection: 0.006130 s
+ Radial + spatial selection: 0.000152 s
+ Evaluate spatial candidates: 0.009077 s
+ Full evaluation oracle: 2.416895 s
+ Candidates radial=294308, spatial=5276, exact=543; oracle PASS
+Query Jupiter distance, offset -1.0 days
+ Radial selection: 0.000363 s
+ Radial + spatial selection: 0.000059 s
+ Evaluate spatial candidates: 0.000003 s
+ Full evaluation oracle: 2.408638 s
+ Candidates radial=11412, spatial=1, exact=0; oracle PASS
+Query outer, offset -1.0 days
+ Radial selection: 0.000131 s
+ Radial + spatial selection: 0.000038 s
+ Evaluate spatial candidates: 0.000005 s
+ Full evaluation oracle: 2.642510 s
+ Candidates radial=1044, spatial=1, exact=1; oracle PASS
+Query inner, offset 0.0 days
+ Radial selection: 0.003728 s
+ Radial + spatial selection: 0.000047 s
+ Evaluate spatial candidates: 0.001135 s
+ Full evaluation oracle: 2.550600 s
+ Candidates radial=6422, spatial=496, exact=84; oracle PASS
+Query belt, offset 0.0 days
+ Radial selection: 0.018802 s
+ Radial + spatial selection: 0.000324 s
+ Evaluate spatial candidates: 0.020513 s
+ Full evaluation oracle: 2.533168 s
+ Candidates radial=294308, spatial=5276, exact=535; oracle PASS
+Query Jupiter distance, offset 0.0 days
+ Radial selection: 0.000940 s
+ Radial + spatial selection: 0.000059 s
+ Evaluate spatial candidates: 0.000003 s
+ Full evaluation oracle: 2.443741 s
+ Candidates radial=11412, spatial=1, exact=0; oracle PASS
+Query outer, offset 0.0 days
+ Radial selection: 0.000111 s
+ Radial + spatial selection: 0.000037 s
+ Evaluate spatial candidates: 0.000003 s
+ Full evaluation oracle: 2.413231 s
+ Candidates radial=1044, spatial=1, exact=1; oracle PASS
+Query inner, offset 1.0 days
+ Radial selection: 0.000275 s
+ Radial + spatial selection: 0.000034 s
+ Evaluate spatial candidates: 0.001022 s
+ Full evaluation oracle: 2.411541 s
+ Candidates radial=6422, spatial=496, exact=89; oracle PASS
+Query belt, offset 1.0 days
+ Radial selection: 0.008174 s
+ Radial + spatial selection: 0.000155 s
+ Evaluate spatial candidates: 0.009183 s
+ Full evaluation oracle: 2.411376 s
+ Candidates radial=294308, spatial=5276, exact=522; oracle PASS
+Query Jupiter distance, offset 1.0 days
+ Radial selection: 0.000419 s
+ Radial + spatial selection: 0.000059 s
+ Evaluate spatial candidates: 0.000003 s
+ Full evaluation oracle: 2.402999 s
+ Candidates radial=11412, spatial=1, exact=0; oracle PASS
+Query outer, offset 1.0 days
+ Radial selection: 0.000147 s
+ Radial + spatial selection: 0.000039 s
+ Evaluate spatial candidates: 0.000004 s
+ Full evaluation oracle: 2.405266 s
+ Candidates radial=1044, spatial=1, exact=1; oracle PASS
+Stale-index rejection PASS
diff --git a/MODULES.md b/MODULES.md
new file mode 100644
index 0000000..b4c66b6
--- /dev/null
+++ b/MODULES.md
@@ -0,0 +1,125 @@
+# Module boundaries
+
+The package is `swift-physics`. Seven public modules share physical contracts
+without importing vehicle systems or rendering. There are no compatibility
+re-exports or old aerodynamic names for the shared fluid APIs.
+
+## Package products and imports
+
+| SwiftPM product | Module dependencies |
+| --- | --- |
+| `FluidDynamics` | None |
+| `Hydrodynamics` | `FluidDynamics` |
+| `Aerodynamics` | `FluidDynamics`, `Atmospheres`, `Yams` |
+| `CelMek` | `Math`, `ERFASwift` (internal), `Atmospheres`, `MagneticFields`, `FluidDynamics` |
+| `Math` | None |
+| `Atmospheres` | None |
+| `MagneticFields` | None |
+| `Physics` | Bundles all seven module targets |
+
+`Physics` is a product name, not a module. Import each module whose APIs are used;
+importing Aerodynamics does not re-export FluidDynamics or Atmospheres. A consumer
+using hull and sail models imports Hydrodynamics, Aerodynamics and FluidDynamics.
+CelMek's `FluidWrench` accepts shared loads without linking Aerodynamics or Yams.
+SwiftPM still resolves package-level dependencies independently of product selection.
+
+For a local development dependency:
+
+```swift
+.package(path: "/path/to/swift-celmek")
+// Target dependencies; the package identity here follows the local folder name.
+.product(name: "CelMek", package: "swift-celmek"),
+.product(name: "FluidDynamics", package: "swift-celmek"),
+.product(name: "Hydrodynamics", package: "swift-celmek")
+```
+
+## Responsibilities and dependency direction
+
+**Math** owns general numerical and geometric operations: quaternions, matrices,
+coordinate representations, angle utilities, and the existing frame identity/parent
+primitive. It does not depend on CelMek or Aerodynamics. Astronomical frame names,
+epochs, units of physical state, ephemerides, and orientation models belong above it.
+Existing astronomical coordinate structs and the legacy `Transformation` remain
+here for compatibility; that is not a requirement to place new astronomy models here.
+
+**ERFASwift** is an internal target, with no standalone product or public API.
+It isolates the ERFA-derived Earth-orientation and full Fairhead TDB routines and
+tables under their BSD terms, retained in `Sources/ERFASwift/LICENSE.txt`.
+It depends only on Math; CelMek adapts epochs, coverage, frames, and errors at the
+boundary using package-scoped entry points.
+
+**CelMek** owns astronomical time, shared physical states and conventions, the frame
+tree and epoch-dependent transforms, celestial properties, orientations, ephemerides,
+and orbital mechanics. New force, propagation and attitude interfaces initially live
+here because they share epochs, states and frames. Keep the following conceptual
+layers within the module rather than immediately introducing more targets:
+
+| Layer | Responsibilities / allowed dependencies |
+| --- | --- |
+| Time | Epochs, durations, time-scale and calendar adapters, injected time data; independent of body catalogues and dynamics. |
+| State and frames | SI Cartesian states, provider interfaces, frame composition and named physical frames; depends on time and Math. |
+| Bodies and models | Body identities/properties, ephemeris and orientation implementations, coefficient/file evaluation; uses shared states and frames. |
+| Orbits and dynamics | Propagators, force/torque interfaces, trajectories and maneuvers; consumes prescribed models through interfaces. |
+| Data adapters | Parsers/loaders and storage; produce validated model/provider data with coverage and provenance. |
+
+These are development boundaries, not separately importable submodules. Provider
+interfaces may reference shared types without depending on concrete implementations.
+For example, a third-body force should consume an ephemeris interface; it should not
+require a particular DE reader or analytic series. Ephemerides must not depend on the
+spacecraft integrator. Frames consume origin/orientation providers without owning a
+simulation clock. Data loading remains separate from evaluating a provider.
+
+**Atmospheres** owns atmospheric profiles, body lookup, units and coverage. It is a
+dependency-free target exposed through the `Atmospheres` product.
+
+**MagneticFields** owns magnetic-field queries, vectors, coverage, provenance,
+dipole models and nominal body-centre lookup. It is a target without
+dependencies. WMM/IGRF coefficient loaders and Swift harmonic evaluators implement the same provider interface.
+CelMek adds body identity, epoch-to-calendar injection and orientation adapters;
+magnetic evaluators do not depend on ephemerides or spacecraft integration.
+
+**FluidDynamics** owns medium-neutral flow, force/moment/reference geometry,
+surface traction integration, displacement buoyancy, scalar tables, propeller
+slipstreams and shared Cartesian numerical infrastructure. Incompressible projection
+and compressible conservative solvers are separate formulations. Gas EOS and
+transport contracts are providers rather than atmosphere/body catalogues. It has
+no dependency on other package modules, YAML, clocks or rigid-body state.
+
+**Aerodynamics** owns gas/airfoil/wing physics, aerodynamic coefficient data,
+finite-wing models, rarefied gas traction and entry heating correlations. It consumes
+FluidDynamics and explicit Atmospheres samples, without owning generic fluid contracts.
+
+**Hydrodynamics** owns liquid property providers, calm-surface partial-immersion
+geometry, hydrostatic/restoring loads, submerged-body damping/added inertia and
+liquid-specific CFD pressure calibration. It reuses FluidDynamics propeller/CFD
+machinery without importing Aerodynamics. Fully filled liquid CFD is distinct from
+future evolving free-surface/wave/two-phase support.
+
+Vehicle assembly, deployment, ballast/flooding/gas management, actuators, failures
+and coupled subsystem evolution belong to a separate systems package. Fluid models
+may own fluid field state, geometric interfaces and their numerical timesteps;
+consumers own scheduling, rigid-body integration and frame/state orchestration.
+
+**Game/renderer adapters** belong in consumer applications or future optional targets.
+They consume CelMek and optionally Aerodynamics. Engine clocks, rendering axes,
+origin shifting, Float conversion and engine objects must not become core dependencies.
+All shared physical coordinates remain right-handed; engine conversion is an explicit
+adapter boundary.
+
+## When to extract another target
+
+Extract a target when there is a concrete consumer or build/data-cost benefit and
+its interface and dependency direction are understood. Likely candidates are large
+optional ephemeris assets/file readers, spacecraft dynamics, game-engine bridges,
+and atmosphere-to-force adapters. Such a split must preserve one shared definition
+of epoch, state and frame identity; it must not duplicate frame singletons or require
+mutual imports.
+
+Extract shared contracts before implementations and preserve acyclic dependencies. Until then, keep numerical implementations
+in Swift and avoid adding runtime dependencies to compensate for missing algorithms.
+Reference tools may use external implementations for independent fixture generation;
+they are developer tooling rather than linked library dependencies.
+
+Shared vector helpers use package visibility; implementation helpers are not promoted
+to public APIs solely to cross a target boundary. New public APIs expose validated
+physical contracts rather than vehicle-system ownership.
diff --git a/Package.resolved b/Package.resolved
new file mode 100644
index 0000000..557e9ac
--- /dev/null
+++ b/Package.resolved
@@ -0,0 +1,32 @@
+{
+ "pins" : [
+ {
+ "identity" : "swift-docc-plugin",
+ "kind" : "remoteSourceControl",
+ "location" : "https://github.com/apple/swift-docc-plugin",
+ "state" : {
+ "revision" : "26ac5758409154cc448d7ab82389c520fa8a8247",
+ "version" : "1.3.0"
+ }
+ },
+ {
+ "identity" : "swift-docc-symbolkit",
+ "kind" : "remoteSourceControl",
+ "location" : "https://github.com/apple/swift-docc-symbolkit",
+ "state" : {
+ "revision" : "b45d1f2ed151d057b54504d653e0da5552844e34",
+ "version" : "1.0.0"
+ }
+ },
+ {
+ "identity" : "yams",
+ "kind" : "remoteSourceControl",
+ "location" : "https://github.com/jpsim/Yams.git",
+ "state" : {
+ "revision" : "a27b21e0c81c5bf42049b897a62aaf387e80f279",
+ "version" : "6.2.2"
+ }
+ }
+ ],
+ "version" : 2
+}
diff --git a/Package.swift b/Package.swift
index 4188599..463cad9 100644
--- a/Package.swift
+++ b/Package.swift
@@ -1,20 +1,30 @@
-// swift-tools-version:5.9
+// swift-tools-version:6.4
// The swift-tools-version declares the minimum version of Swift required to build this package.
import PackageDescription
let package = Package(
name: "swift-physics",
+ platforms: [
+ .macOS(.v15), .iOS(.v18), .tvOS(.v18), .watchOS(.v11), .visionOS(.v2),
+ ],
products: [
// Products define the executables and libraries produced by a package, and make them visible to other packages.
.library(
name: "Physics",
- targets: ["CelMek", "Aerodynamics", "Math"]),
+ targets: ["CelMek", "Aerodynamics", "FluidDynamics", "Hydrodynamics", "Math", "Atmospheres", "MagneticFields"]),
+ .library(name: "CelMek", targets: ["CelMek"]),
+ .library(name: "Atmospheres", targets: ["Atmospheres"]),
+ .library(name: "MagneticFields", targets: ["MagneticFields"]),
+ .library(name: "Math", targets: ["Math"]),
+ .library(name: "Aerodynamics", targets: ["Aerodynamics"]),
+ .library(name: "FluidDynamics", targets: ["FluidDynamics"]),
+ .library(name: "Hydrodynamics", targets: ["Hydrodynamics"]),
],
dependencies: [
// Dependencies declare other packages that this package depends on.
// .package(url: /* package url */, from: "1.0.0"),
- .package(url: "https://github.com/jpsim/Yams.git", from: "5.0.6"),
+ .package(url: "https://github.com/jpsim/Yams.git", from: "6.2.2"),
.package(url: "https://github.com/apple/swift-docc-plugin", from: "1.1.0"),
],
targets: [
@@ -22,19 +32,55 @@ let package = Package(
// Targets can depend on other targets in this package, and on products in packages which this package depends on.
.target(
name: "CelMek",
- dependencies: ["Math"]),
+ dependencies: ["Math", "ERFASwift", "Atmospheres", "FluidDynamics",
+ "MagneticFields"]),
+ .target(name: "MagneticFields", resources: [.process("Resources")]),
+ .target(name: "ERFASwift", dependencies: ["Math"], exclude: ["LICENSE.txt", "README.md"]),
+ .target(name: "Atmospheres"),
+ .target(name: "FluidDynamics"),
+ .target(name: "Hydrodynamics", dependencies: ["FluidDynamics"]),
.target(
name: "Math",
dependencies: []),
.target(
name: "Aerodynamics",
- dependencies: ["Yams"]),
+ dependencies: ["Yams", "Atmospheres", "FluidDynamics"]),
+ .executableTarget(name: "FluidPhysicsDemo", dependencies: ["Aerodynamics", "Atmospheres", "FluidDynamics", "Hydrodynamics"],
+ path: "Examples/FluidPhysicsDemo"),
+ .executableTarget(
+ name: "TwoBodyGameDemo",
+ dependencies: ["CelMek"],
+ path: "Examples/TwoBodyGameDemo"),
+ .executableTarget(
+ name: "AttitudeDynamicsDemo",
+ dependencies: ["CelMek", "Math"],
+ path: "Examples/AttitudeDynamicsDemo"),
+ .executableTarget(
+ name: "Voyager2GameDemo",
+ dependencies: ["CelMek", "Math"],
+ path: "Examples/Voyager2GameDemo",
+ exclude: ["README.md"]),
+ .executableTarget(
+ name: "GameIntegrationBenchmark",
+ dependencies: ["CelMek", "Math"],
+ path: "Tools/GameIntegrationBenchmark"),
+ .executableTarget(
+ name: "VSOP87Characterization",
+ dependencies: ["CelMek", "Math"],
+ path: "Tools/VSOP87Characterization"),
+ .executableTarget(name: "MPCCullingExperiment", dependencies: ["CelMek", "Math"],
+ path: "Experiments/MPCCulling", exclude: ["README.md", "results"]),
.testTarget(
name: "CelMekTests",
- dependencies: ["CelMek"]),
+ dependencies: ["CelMek", "FluidDynamics", "Atmospheres"],
+ resources: [.copy("Fixtures")]),
.testTarget(
name: "AerodynamicsTests",
- dependencies: ["Aerodynamics"]),
+ dependencies: ["Aerodynamics", "FluidDynamics", "Atmospheres"], resources: [.process("Resources")]),
+ .testTarget(name: "FluidDynamicsTests", dependencies: ["FluidDynamics"]),
+ .testTarget(name: "HydrodynamicsTests", dependencies: ["Hydrodynamics", "FluidDynamics"]),
+ .testTarget(name: "AtmospheresTests", dependencies: ["Atmospheres"]),
+ .testTarget(name: "MagneticFieldsTests", dependencies: ["MagneticFields"], resources: [.copy("Fixtures")]),
.testTarget(
name: "MathTests",
dependencies: ["Math"]),
diff --git a/README.md b/README.md
index bb829e2..413da72 100644
--- a/README.md
+++ b/README.md
@@ -1,6 +1,6 @@
-# swift-celmek
+# swift-physics
-A port of the celmek library to swift.
+Swift physics libraries for celestial mechanics, gas and liquid dynamics, atmospheres and magnetic fields.
The celmek library implements several astronomical algorithms.
@@ -20,10 +20,90 @@ A companion app for interactivelly working with this library is developed here:
## Evolution
-In addition to the celestial mechanics algorithms,
-various functionality related to Aerodynamics have been added.
-It is probable that we will rename the package `swift-physics` at some point.
+The package has grown beyond the original CelMek port. Shared fluid physics now
+lives in FluidDynamics, with dedicated Aerodynamics and Hydrodynamics modules.
+
+## Requirements
+
+Swift 6.4 or newer. Apple deployment targets are macOS 15, iOS 18, tvOS 18,
+watchOS 11, and visionOS 2 or newer, matching `Synchronization.Mutex` availability.
+Linux and Windows builds are covered by CI.
+
+## Modules
+
+Use the `CelMek`, `Math`, `FluidDynamics`, `Aerodynamics`, `Hydrodynamics`,
+`Atmospheres`, or `MagneticFields` product for the modules your application needs.
+The `Physics` product bundles all seven.
+Import the corresponding module names. See [MODULES.md](MODULES.md) for responsibilities and dependency rules.
+
+## Documentation
+
+The public guides and API references use DocC. See [documentation build instructions](Documentation/README.md)
+for the seven module catalogs and the combined package archive.
+
+```sh
+python3 Tools/Documentation/build.py
+python3 Tools/Documentation/preview.py
+```
+
+Browse the result at [localhost:8080/documentation](http://127.0.0.1:8080/documentation).
+
+## Time API
+
+Precise epochs, durations, UTC leap seconds, and calendar readings with explicit
+TAI/TT/TDB/UTC scales are documented in [time guide](Sources/CelMek/CelMek.docc/TimeGuide.md).
+
+Coordinate handedness, quaternion and angle conventions, transform direction, and
+error handling are documented in [CONVENTIONS.md](Sources/CelMek/CelMek.docc/CONVENTIONS.md).
+
+## Testing
+
+The tests use Swift Testing and require a Swift 6.4 or newer toolchain. Run all
+test targets with:
+
+```sh
+swift test
+```
## License
-Apache 2.0
+Apache 2.0 for the package's original code. ERFA-derived Earth-orientation and
+Fairhead TDB numerical code is isolated in the internal `ERFASwift` module under
+its [BSD terms and attribution](Sources/ERFASwift/LICENSE.txt). See the
+[module README](Sources/ERFASwift/README.md) for its scope.
+
+Shared Cartesian states use metres and metres per second, with explicit unit conversion and a VSOP87 provider adapter. See [STATES.md](Sources/CelMek/CelMek.docc/STATES.md).
+
+Time-dependent frame trees, rotating transforms, and their conventions are documented in [FRAMES.md](Sources/CelMek/CelMek.docc/FRAMES.md).
+
+The IAU coefficient review, updated data, and independent SPICE reference tests are documented in [IAU_ROTATION_AUDIT.md](IAU_ROTATION_AUDIT.md).
+
+Body identities, sourced SI properties, and the injectable JPL GM catalogue are documented in [BODIES.md](Sources/CelMek/CelMek.docc/BODIES.md).
+
+The common ephemeris contract, validating state-provider adapter, and body-query collection are documented in [EPHEMERIDES.md](Sources/CelMek/CelMek.docc/EPHEMERIDES.md).
+
+Shared accuracy intent and each adapter's supported levels are documented in [ACCURACY.md](Sources/CelMek/CelMek.docc/ACCURACY.md).
+
+Reduced VSOP87 error and query-cost measurements, with a reproducible release tool, are in [VSOP87_ACCURACY_CHARACTERIZATION.md](Sources/CelMek/CelMek.docc/VSOP87_ACCURACY_CHARACTERIZATION.md).
+
+Atmospheric profiles are provided by the [Atmospheres target](Sources/Atmospheres/Atmospheres.docc/Guide.md),
+shared by CelMek and Aerodynamics. It includes Earth ISA, nominal planetary/moon
+profiles, and gas-giant pressure during descent below the 1-bar level.
+
+The [MagneticFields target](Sources/MagneticFields/MagneticFields.docc/Guide.md) supplies
+pluggable magnetic-field models, ideal dipoles and CelMek body/orientation adapters.
+It also includes Swift WMM/IGRF evaluators, coefficient-file loaders and bundled
+WMM2025/IGRF-14 datasets with explicit date coverage.
+
+## Fluid physics examples
+
+```sh
+swift run FluidPhysicsDemo
+swift run -c release -debug-info-format none FluidPhysicsDemo --cfd --compressible
+```
+
+The example includes dedicated Earth/Titan liquid displacement and pressure cases,
+optional incompressible rotor/body CFD and a compressible Sod reference problem.
+Liquid properties and vehicle coefficients in these examples are illustrative.
+See the FluidDynamics and Hydrodynamics DocC guides for coverage, numerical cost,
+pressure-reference rules and the remaining real-gas/free-surface fidelity work.
diff --git a/Scripts/generate_spice_oracle.py b/Scripts/generate_spice_oracle.py
new file mode 100644
index 0000000..523ba81
--- /dev/null
+++ b/Scripts/generate_spice_oracle.py
@@ -0,0 +1,103 @@
+#!/usr/bin/env python3
+"""Optional black-box fixture generator. Requires binary SpiceyPy/CSPICE and NumPy.
+Uses public writer/query APIs only; do not consult toolkit implementation source.
+Run with PYTHONPATH pointing to an optional external binary-wheel installation.
+"""
+from pathlib import Path
+import hashlib, json, math, platform
+import numpy as np
+import spiceypy as s
+
+out = Path(__file__).resolve().parents[1] / 'Tests/CelMekTests/Fixtures/spice-oracle'
+out.mkdir(parents=True, exist_ok=True)
+s.kclear()
+for name in ['states.bsp','attitudes.bc','rotation.bpc']:
+ (out/name).unlink(missing_ok=True)
+refs = dict(schema=1, toolkit=s.tkvrsn('TOOLKIT'), wrapper=s.__version__,
+ generator='Scripts/generate_spice_oracle.py', platform=platform.platform(),
+ basis='Public NAIF format/behavior/API documentation; binary oracle only',
+ spk=[], ck=[], pck=[], utc=[], sclk=[])
+# Position coefficients deliberately differ from supplied type-3 velocity coefficients.
+p = np.array([[2,.3,-.2],[4,-.1,.05],[-1,.2,.01]])
+v = np.array([[.4,.02,0],[.1,0,.003],[-.2,.01,0]])
+h = s.spkopn(str(out/'states.bsp'),'CELMEK ORACLE SPK',0)
+for body,kind in [(399,2),(499,3)]:
+ coeff = p if kind == 2 else np.vstack([p,v])
+ s.__getattribute__('spkw%02d'%kind)(h,body,3,'J2000',-20,20,'TYPE %d'%kind,20,2,2,
+ np.vstack([coeff,coeff+0.01]).ravel(),-20)
+s.spkw02(h,3,0,'J2000',-20,20,'CENTRE CHAIN',40,1,1,[10,.5,-3,.2,2,-.1],-20)
+s.spkcls(h); s.furnsh(str(out/'states.bsp'))
+for body in [399,499]:
+ for t in [-20,-17.125,-0.000001,0,6.25,20]:
+ state, _ = s.spkez(body,t,'J2000','NONE',0)
+ refs['spk'].append(dict(body=body,centre=0,t=t,state=state.tolist()))
+
+h = s.ckopn(str(out/'attitudes.bc'),'CELMEK ORACLE CK',0)
+times = np.array([0.,20.,60.,80.,100.]); angles=[.3,.7,1.1,1.4,1.6]
+# Use oracle matrix-to-quaternion conversion to avoid sharing Swift quaternion assumptions.
+quats=np.array([s.m2q(s.rotate(a,3) @ s.rotate(.4,1)) for a in angles])
+av=np.array([[i*.01,.02,-.03] for i in range(5)])
+s.ckw01(h,0,100,-77001,'J2000',True,'TYPE 1',5,times,quats,av)
+s.ckw02(h,0,100,-77002,'J2000','TYPE 2',2,np.array([0.,60.]),np.array([40.,100.]),
+ quats[[0,2]],av[[0,2]],np.array([2.,3.]))
+s.ckw03(h,0,100,-77003,'J2000',True,'TYPE 3',5,times,quats,av,3,np.array([0.,60.,100.]))
+s.ckw03(h,0,100,-77004,'J2000',False,'TYPE 3 NO RATE',5,times,quats,av,3,np.array([0.,60.,100.]))
+s.ckcls(h); s.furnsh(str(out/'attitudes.bc'))
+for inst,queries in [(-77001,[(0,0),(20,0),(19,2),(100,0)]),
+ (-77002,[(0,0),(15,0),(40,0),(60,0),(77,0),(100,0)]),
+ (-77003,[(0,0),(7,0),(20,0),(35,16),(60,0),(73,0),(100,0)]),
+ (-77004,[(7,0),(73,0)])]:
+ for tick,tol in queries:
+ if inst == -77004:
+ matrix,selected=s.ckgp(inst,tick,tol,'J2000'); rate=None
+ else:
+ matrix,rate,selected=s.ckgpav(inst,tick,tol,'J2000'); rate=rate.tolist()
+ refs['ck'].append(dict(instrument=inst,tick=tick,tolerance=tol,selected=selected,matrix=matrix.tolist(),rate=rate))
+
+h=s.pckopn(str(out/'rotation.bpc'),'CELMEK ORACLE PCK',0)
+s.pckw02(h,3000,'J2000',-20,20,'PCK TYPE 2',20,2,2,np.vstack([p*.1,p*.1+.01]).ravel(),-20)
+s.pckcls(h)
+(out/'frames.tf').write_text("""KPL/FK
+\\begindata
+FRAME_ORACLE_PCK = 13000
+FRAME_13000_NAME = 'ORACLE_PCK'
+FRAME_13000_CLASS = 2
+FRAME_13000_CLASS_ID = 3000
+FRAME_13000_CENTER = 301
+""")
+s.furnsh(str(out/'frames.tf')); s.furnsh(str(out/'rotation.bpc'))
+for t in [-20,-17.125,-.000001,0,6.25,20]:
+ refs['pck'].append(dict(t=t,matrix=s.pxform('J2000','ORACLE_PCK',t).tolist()))
+
+(out/'time.tls').write_text("""KPL/LSK
+\\begindata
+DELTET/DELTA_T_A=32.184
+DELTET/K=1.657D-3
+DELTET/EB=1.671D-2
+DELTET/M=(6.239996 1.99096871D-7)
+DELTET/DELTA_AT=(10 @1972-JAN-1 11 @1972-JUL-1 12 @1973-JAN-1)
+""")
+s.furnsh(str(out/'time.tls'))
+for label,mjd,seconds in [('1972 JAN 01 00:00:00 UTC',41317,0),('1972 JUN 30 23:59:59 UTC',41498,86399),
+ ('1972 JUN 30 23:59:60 UTC',41498,86400),('1972 JUL 01 00:00:00 UTC',41499,0),
+ ('1973 JAN 01 00:00:00 UTC',41683,0)]:
+ refs['utc'].append(dict(label=label,mjd=mjd,seconds=seconds,tt=s.unitim(s.str2et(label),'ET','TT')))
+(out/'clock.tsc').write_text("""KPL/SCLK
+\\begindata
+SCLK_DATA_TYPE_77=1
+SCLK01_N_FIELDS_77=2
+SCLK01_MODULI_77=(1000 10)
+SCLK01_OFFSETS_77=(0 0)
+SCLK01_OUTPUT_DELIM_77=2
+SCLK01_TIME_SYSTEM_77=1
+SCLK_PARTITION_START_77=(0 0)
+SCLK_PARTITION_END_77=(1000 1000)
+SCLK01_COEFFICIENTS_77=(0 0 20 1000 2000 10)
+""")
+s.furnsh(str(out/'clock.tsc'))
+for tick in [0,17.125,999.5,1000,1000.5,1750,2000]:
+ refs['sclk'].append(dict(tick=tick,tdb=s.sct2e(-77,tick)))
+refs['assets']={p.name:hashlib.sha256(p.read_bytes()).hexdigest() for p in sorted(out.iterdir()) if p.suffix in ['.bsp','.bc','.bpc','.tf','.tls','.tsc']}
+(out/'reference.json').write_text(json.dumps(refs,indent=2)+'\n')
+s.kclear()
+print('Wrote pinned oracle fixtures:',out)
diff --git a/Scripts/generate_spk21_oracle.py b/Scripts/generate_spk21_oracle.py
new file mode 100644
index 0000000..86ab17b
--- /dev/null
+++ b/Scripts/generate_spk21_oracle.py
@@ -0,0 +1,85 @@
+#!/usr/bin/env python3
+"""Optional binary CSPICE oracle; public SPKW21/SPKE21 contracts only, no toolkit source.
+PYTHONPATH=/path/to/binary/spiceypy python3 Scripts/generate_spk21_oracle.py
+"""
+import ctypes
+import hashlib
+import json
+from pathlib import Path
+import numpy as np
+import spiceypy as spice
+from spiceypy.utils.libspicehelper import libspice
+
+out = Path(__file__).resolve().parents[1] / 'Tests/CelMekTests/Fixtures/spk21'
+out.mkdir(parents=True, exist_ok=True)
+refs = dict(schema=1, toolkit=spice.tkvrsn('TOOLKIT'), wrapper=spice.__version__,
+ basis='Published API contracts; binary oracle only', files=[], states=[])
+for dimension, count in [(15, 201), (25, 2)]:
+ size = 4 * dimension + 11
+ epochs = np.arange(count, dtype=np.float64) * 10 + 10
+ lines = np.zeros((count, size), dtype=np.float64)
+ rng = np.random.default_rng(21000 + dimension)
+ for i, end in enumerate(epochs):
+ line = lines[i]
+ line[0] = end - 4
+ line[1:dimension+1] = np.cumsum(rng.uniform(8, 12, dimension))
+ line[1+dimension:7+dimension] = [1e8+i*100, 2, -2e8+i*200, -3, 3e7-i*300, 4]
+ line[7+dimension:7+4*dimension] = rng.uniform(-0.02, 0.02, 3*dimension)
+ line[7+4*dimension] = dimension+1
+ line[8+4*dimension:11+4*dimension] = [dimension, dimension-4, dimension-7]
+ path = out / f'dimension{dimension}.bsp'
+ path.unlink(missing_ok=True)
+ h = spice.spkopn(str(path), 'CELMEK TYPE21 BINARY ORACLE', 0)
+ # No CSPICE C wrapper exists; call the documented Fortran writer entry point.
+ ints = [ctypes.c_int(x) for x in [h, 900000+dimension, 0, count, size]]
+ first, last = ctypes.c_double(0), ctypes.c_double(epochs[-1])
+ libspice.spkw21_(ctypes.byref(ints[0]), ctypes.byref(ints[1]), ctypes.byref(ints[2]),
+ ctypes.c_char_p(b'J2000'), ctypes.byref(first), ctypes.byref(last), ctypes.c_char_p(b'TYPE21 ORACLE'),
+ ctypes.byref(ints[3]), ctypes.byref(ints[4]), lines.ctypes.data_as(ctypes.POINTER(ctypes.c_double)),
+ epochs.ctypes.data_as(ctypes.POINTER(ctypes.c_double)), ctypes.c_int(5), ctypes.c_int(13))
+ if spice.failed():
+ message = spice.getmsg('LONG'); spice.reset(); raise RuntimeError(message)
+ spice.spkcls(h)
+ spice.furnsh(str(path))
+ queries = sorted(set([0., 1.25, 6., 9.9, 10., np.nextafter(10., np.inf), float(epochs[-1])] +
+ ([990., 1000., np.nextafter(1000., np.inf), 1999., 2000., np.nextafter(2000., np.inf)] if count > 100 else [])))
+ for t in queries:
+ state, _ = spice.spkez(900000+dimension, t, 'J2000', 'NONE', 0)
+ refs['states'].append(dict(file=path.name, t=float(t), record=int(np.searchsorted(epochs,t)), state=state.tolist()))
+ refs['files'].append(dict(name=path.name, dimension=dimension, count=count,
+ sha256=hashlib.sha256(path.read_bytes()).hexdigest()))
+ spice.unload(str(path))
+(out/'reference.json').write_text(json.dumps(refs, indent=2)+'\n')
+print('Generated', len(refs['states']), 'type 21 oracle states')
+
+# Optionally pin a real small-body kernel obtained by the extraction script.
+# Existing real fixtures are retained when this argument is omitted.
+if len(__import__('sys').argv) == 3 and __import__('sys').argv[1] == '--horizons':
+ source = Path(__import__('sys').argv[2])
+ destination = out / 'horizons-ceres.bsp'
+ destination.write_bytes(source.read_bytes())
+ h = spice.dafopr(str(destination)); spice.dafbfs(h)
+ if not spice.daffna(): raise RuntimeError('Empty real kernel')
+ descriptor = spice.dafgs(5)
+ body, center, frame, kind, start, end, first, last = spice.spkuds(descriptor)
+ if kind != 21 or body != 20000001: raise RuntimeError('Expected Ceres type 21')
+ dimension, count = map(int, spice.dafgda(h, last-1, last))
+ size = 4*dimension+11
+ epochs = spice.dafgda(h, first+size*count, first+size*count+count-1)
+ spice.dafcls(h); spice.furnsh(str(destination))
+ queries = [start, start+(end-start)/7, (start+end)/2, end]
+ for boundary in epochs:
+ if start < boundary < end:
+ queries += [float(np.nextafter(boundary, -np.inf)), float(boundary), float(np.nextafter(boundary, np.inf))]
+ rows = []
+ for t in sorted(set(queries)):
+ state, _ = spice.spkez(body,t,'J2000','NONE',center)
+ rows.append(dict(t=t, record=int(np.searchsorted(epochs,t)), state=state.tolist()))
+ reference = dict(schema=1, toolkit=spice.tkvrsn('TOOLKIT'), wrapper=spice.__version__,
+ file=destination.name, body=body, center=center, frame=frame,
+ sha256=hashlib.sha256(destination.read_bytes()).hexdigest(),
+ origin='NASA/JPL Horizons API; Ceres; requested 2000-01-01 through 2000-01-03 TDB',
+ states=rows)
+ (out/'horizons-reference.json').write_text(json.dumps(reference,indent=2)+'\n')
+ spice.unload(str(destination))
+ print('Generated',len(rows),'real Horizons oracle states')
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/Aerodynamics.md b/Sources/Aerodynamics/Aerodynamics.docc/Aerodynamics.md
new file mode 100644
index 0000000..2bb7318
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/Aerodynamics.md
@@ -0,0 +1,116 @@
+# ``Aerodynamics``
+
+Local flow, coefficient data, airfoil geometry and physical aerodynamic loads.
+
+Aerodynamics provides parametric and thin-airfoil models, NACA geometry and YAML
+coefficient input. Atmospheric profiles live in Atmospheres. Shared flow, load, propeller and CFD
+contracts live in [FluidDynamics](/documentation/fluiddynamics); import those modules explicitly.
+
+## Topics
+
+### Physics foundations
+-
+- ``GasFlowCoverage``
+- ``CoveredBodyCoefficients``
+- ``MachRegimeBodyCoefficients``
+-
+
+### Checked coefficient models
+- ``AirfoilCoefficientModel``
+- ``AirfoilPolar``
+- ``TabulatedAirfoil``
+- ``AirfoilTableLoader``
+- ``CoefficientBoundaryPolicy``
+
+### Wing and whole-body evaluation
+-
+-
+- ``FiniteWingAirfoil``
+- ``FiniteWingSolution``
+-
+- ``NonlinearLiftingLine``
+- ``NonlinearLiftingLineResult``
+-
+- ``LiftingLineWing``
+- ``LiftingLineSection``
+- ``LiftingLineResult``
+- ``LiftingLineStationResult``
+- ``SegmentedWing``
+- ``WingSegment``
+- ``WingSectionAxes``
+- ``WingSectionCoefficientModel``
+- ``AirfoilWingSectionModel``
+- ``WholeBodyAerodynamics``
+- ``BodyAerodynamicCoefficientModel``
+- ``TabulatedBodyCoefficients``
+- ``WindForceCoefficients``
+-
+- ``BodyAerodynamicRateReference``
+- ``BodyAerodynamicRateDerivatives``
+- ``BodyAerodynamicRateDerivativeModel``
+- ``ConstantBodyRateDerivatives``
+- ``LinearBodyRateAerodynamics``
+-
+- ``ControlSurfaceSetting``
+- ``TabulatedControlSurface``
+- ``ControlSurfaceTableLoader``
+
+### Airfoil models
+- ``Airfoil``
+- ``AirfoilCoefficients``
+- ``ParametricAirfoil``
+- ``ThinSymetricAirfoil``
+- ``ThinCamberedAirfoil``
+- ``NACA4``
+
+### Hypersonic surface pressure
+-
+- ``ModifiedNewtonianPressure``
+-
+- ``FreeMolecularGas``
+- ``GasSurfaceReflection``
+- ``MaxwellianFreeMolecularTraction``
+- ``TabulatedRarefiedTraction``
+
+### Aerothermal physics
+-
+- ``SurfaceHeatingQuery``
+- ``SurfaceConvectiveHeatingModel``
+- ``SurfaceConvectionResult``
+- ``LaminarFlatPlateHeating``
+- ``TurbulentFlatPlateHeating``
+-
+- ``AerothermalBoundaryLayer``
+- ``EnthalpySurfaceHeatingCoverage``
+- ``EnthalpySurfaceHeatingQuery``
+- ``EnthalpySurfaceHeatingResult``
+- ``EnthalpySurfaceHeatingModel``
+- ``TabulatedEnthalpySurfaceHeating``
+- ``LeadingEdgeHeatingQuery``
+- ``LeadingEdgeConvectiveHeatingModel``
+- ``SweptCylinderStagnationHeating``
+- ``TabulatedRadiativeHeating``
+-
+- ``StagnationHeatingQuery``
+- ``AerothermalWallState``
+- ``ConvectiveHeatingModel``
+- ``RadiativeHeatingModel``
+- ``SuttonGravesParameters``
+- ``StagnationHeatingCoverage``
+- ``SuttonGravesHeating``
+-
+- ``StagnationGasState``
+- ``SuttonGravesBaseGas``
+- ``SuttonGravesMixtureParameters``
+- ``SuttonGravesMixtureHeating``
+- ``HydrogenHeliumHeatingMixture``
+- ``HydrogenHeliumColdWallHeating``
+- ``HydrogenHeliumHeatingResult``
+
+### Optional airflow simulation
+- [shared propwash/CFD guide](/documentation/fluiddynamics/propellersandcfd)
+
+### Parachutes and balloons
+-
+- ``ParachuteAerodynamics``
+- ``BalloonAerodynamics``
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/Aerothermal.md b/Sources/Aerodynamics/Aerodynamics.docc/Aerothermal.md
new file mode 100644
index 0000000..b090e8d
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/Aerothermal.md
@@ -0,0 +1,78 @@
+# Stagnation-point heating
+
+``ConvectiveHeatingModel`` and ``RadiativeHeatingModel`` accept a
+``StagnationHeatingQuery`` and return incoming heat flux in W/m² at an explicit
+surface position. They are separate contributions: no radiative model means
+radiation is unavailable, not zero. ``TabulatedRadiativeHeating`` accepts supplied cold-wall radiation data; no default radiative correlation is inferred.
+Wall radiation emission, temperature evolution, conduction and ablation belong to
+external thermal models. These interfaces do not advance a clock or mutate vehicle
+state. Richer gas chemistry or catalytic-surface data can be supplied through a
+replacement model's provider; these initial contracts are for stagnation heating.
+
+``SuttonGravesHeating`` supplies a laminar cold-wall convective estimate for an
+axisymmetric blunt body:
+
+`qConvective = k sqrt(ρ / Rnose) V³`
+
+Density is kg/m³, nose radius is metres, relative speed is m/s and output is W/m².
+The coefficient `k` has SI dimensions kg^0.5/m. Its numerical value depends on
+the gas and the coefficient's unit convention; a W/cm² coefficient cannot be used
+unchanged with the W/m² interface.
+
+``SuttonGravesParameters`` requires a gas identifier, coefficient, source and
+version. ``SuttonGravesParameters/earthAirColdWall`` explicitly selects the Earth-air
+value `1.7415e-4` used in the NASA TFAWS 2012 course. No planet or atmosphere lookup
+selects it automatically. The query's gas identifier must match the parameters;
+this is a dataset identity check, not composition analysis. Custom parameter sets
+allow independently justified approximations for other gas mixtures.
+
+```swift
+let coverage = try StagnationHeatingCoverage(
+ speedMetresPerSecond: 1000...8000,
+ densityKilogramsPerCubicMetre: 1e-6...0.01,
+ noseRadiusMetres: 0.1...5, machNumber: 5...40)
+let model = SuttonGravesHeating(parameters: .earthAirColdWall, coverage: coverage)
+let flow = try FluidFlow(relativeVelocityMetresPerSecond: SIMD3(3535, 0, 0),
+ densityKilogramsPerCubicMetre: 3.1459e-4, speedOfSoundMetresPerSecond: 300,
+ meanFreePathMetres: 1e-4)
+let query = try StagnationHeatingQuery(flow: flow, gasIdentifier: "earth-air",
+ noseRadiusMetres: 1, surfacePositionMetres: SIMD3(1, 0, 0))
+let heat = try model.heatFlux(for: query)
+```
+
+These example bounds are declared simulation coverage, not experimentally validated
+limits. The caller must establish that the correlation suits the gas, geometry and
+entry conditions. The model restricts declared Mach coverage to hypersonic flow
+(Mach ≥ 5) and continuum coverage to Kn ≤ 0.01, using nose radius as the reference
+length. Missing sound speed or mean free path throws for nonzero speed. Speed,
+density, radius, Mach and Knudsen coverage are checked before evaluating the
+correlation. Zero speed produces zero aerodynamic convective flux after checking
+gas identity, wall assumptions and radius, without requiring Mach or mean free path.
+Zero density at nonzero speed is outside the declared positive-density coverage.
+Low density alone does not establish continuum applicability.
+
+The stagnation point and effective nose radius are caller-supplied. The model does
+not locate a stagnation point or extrapolate a capsule value over a wing. Local flow
+must already account for atmospheric co-rotation and winds, as described in
+. Use consistent thermodynamic and transport inputs; current
+atmosphere profiles do not supply mean free path automatically.
+
+This cold-wall approximation does not account for finite wall temperature. A query
+with ``AerothermalWallState`` therefore throws `unsupportedQuery`; a different
+correlation must use that state. No turbulent multiplier, catalytic correction,
+radiative contribution or species-equilibrium solver is inferred. The estimate
+may be integrated externally as heat load in J/m², but does not itself predict
+wall temperature or protection-system survival.
+
+See for a Mars preset, explicit Venus mixture parameters
+and a separate hydrogen/helium cold-wall correlation with different wall assumptions.
+
+Tests reproduce the NASA course's rounded shuttle-like reference of 13.6 W/cm²,
+check cubic velocity, square-root density and inverse-square-root radius scaling,
+and exercise gas mismatch, custom coefficients, rest and coverage boundaries.
+
+Sources: [Sutton and Graves, NASA TR R-376](https://ntrs.nasa.gov/citations/19720003329)
+and [NASA TFAWS 2012 Aerothermodynamics Course](https://tfaws.nasa.gov/TFAWS12/Proceedings/Aerothermodynamics%20Course.pdf).
+
+See for enthalpy-based surface data and swept leading-edge
+stagnation-line heating, and for low-speed plate convection.
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/BodyRates.md b/Sources/Aerodynamics/Aerodynamics.docc/BodyRates.md
new file mode 100644
index 0000000..192d9b7
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/BodyRates.md
@@ -0,0 +1,71 @@
+# Body angular-rate aerodynamics
+
+``LinearBodyRateAerodynamics`` adds supplied small-rate derivatives to an existing
+whole-body coefficient model. It preserves static lift and trim/restoring moments:
+
+`C = Cstatic + Droll pHat + Dpitch qHat + Dyaw rHat`
+
+The normalization is `rateHat[i] = angularVelocity[i] momentLength[i] / (2 speed)`.
+Aircraft typically use span/chord/span; capsule datasets must use their stated
+reference dimensions. ``BodyAerodynamicRateDerivatives`` holds three columns of
+six signed body-axis coefficient derivatives, allowing force, moment and cross-axis
+effects. A negative diagonal moment derivative provides damping in the selected
+convention; arbitrary derivatives are not assumed to imply a stable vehicle.
+
+``BodyAerodynamicRateDerivativeModel`` permits flow-dependent derivative datasets.
+``ConstantBodyRateDerivatives`` supplies prescribed derivatives with explicit
+Mach, Reynolds, incidence and sideslip ranges and source/version metadata. It also
+checks the query's moment lengths and Reynolds reference length against its dataset.
+Area, axes and moment reference point must match the static coefficient dataset and
+the supplied geometry; the query cannot independently certify those conventions.
+No real capsule or aircraft derivative database is bundled here.
+
+The wrapper requires a minimum speed and per-axis absolute normalized-rate limits.
+These are declared applicability limits, not measured accuracy guarantees. It queries
+both the static and derivative providers with zero angular rates, then adds one rate
+increment. Do not wrap another rate-corrected model or add these loads to a second
+provider representing the same effect. Missing properties and unsupported ranges
+throw instead of silently extrapolating.
+
+## Rate reference and rotating air
+
+``BodyAerodynamicRateReference`` explicitly distinguishes inertial-reference rates
+from rates relative to a rigidly rotating medium. The query tag must match the
+wrapper's configured convention. For inertial-reference data, supply the attitude's
+inertial angular velocity expressed in body axes. For medium-relative data, subtract
+the atmosphere's angular velocity, also expressed in body axes, then tag the query
+as `rigidlyRotatingMedium`. The wrapper does not transform axes or infer atmospheric
+rotation. The underlying linear flow remains vehicle-relative-to-air in either case.
+Do not subtract atmospheric rotation again from an already medium-relative rate.
+
+Pass the convention through ``WholeBodyAerodynamics``:
+
+```swift
+let loads = try body.evaluate(flow: flow,
+ angularVelocityRadiansPerSecond: vehicleRateBody - atmosphereRateBody,
+ angularRateReference: .rigidlyRotatingMedium)
+```
+
+Here `body` uses a wrapper configured for that same medium-relative convention.
+CelMek's aerodynamic wrench adapter consumes the returned force and moment as usual;
+the caller chooses the rate convention required by the dataset.
+
+## Limits and validation
+
+This is a local linear angular-rate model. It does not implement incidence/sideslip
+time derivatives, hysteresis, dynamic stall, oscillatory-frequency corrections or
+unsteady wakes. Some experimental pitch-damping datasets combine pitch-rate and
+incidence-rate derivatives; they cannot be imported as a pure pitch-rate derivative
+without a justified conversion.
+
+Direct coefficient queries below the minimum speed throw. Whole-body evaluation
+continues to return zero loads at zero dynamic pressure without querying a model.
+This does not estimate spin drag when a body rotates in otherwise stationary air;
+surface/segment methods with sampled local velocities are needed for that case.
+
+Tests check an analytic three-axis damping torque, negative rotational power for
+the supplied stable diagonal example, reversal and velocity scaling, preservation
+of static lift/moment, zero-rate provider queries, reference tags and coverage.
+The demo's derivative values are synthetic rather than validated capsule data.
+
+Reference: [NASA body-axis dynamic derivative conventions](https://ntrs.nasa.gov/api/citations/20040090578/downloads/20040090578.pdf).
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/ControlSurfaces.md b/Sources/Aerodynamics/Aerodynamics.docc/ControlSurfaces.md
new file mode 100644
index 0000000..a52be6b
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/ControlSurfaces.md
@@ -0,0 +1,71 @@
+# Wing and tail control-surface data
+
+``TabulatedControlSurface`` implements the existing section coefficient contract
+for caller-supplied geometric control deflection. It uses a set of
+``ControlSurfaceSetting`` datasets, each containing a checked incidence/Reynolds/Mach
+``TabulatedAirfoil``. Lift, drag and pitching moment interpolate linearly across
+deflection after evaluating the neighboring polars. No incidence offset or assumed
+control-effectiveness factor is substituted for measured or computed data.
+
+Deflection coordinates are finite radians within ±π, sorted on construction, with
+duplicates rejected. All settings share the same Reynolds and Mach coordinate grid;
+incidence samples may differ. Intermediate deflections require coverage in both
+neighboring polars. Exact deflection settings use only their own dataset, avoiding
+irrelevant neighboring coverage restrictions. A single setting represents one
+supported deflection, not an assumed constant response at all deflections.
+
+The deflection boundary policy defaults to rejection. Explicit clamping affects
+only the deflection coordinate; each underlying airfoil retains its own declared
+incidence/Re/Mach policy. Clamping is a caller-selected numerical approximation,
+not a calibrated extrapolation. No transition or smoothing beyond piecewise linear
+interpolation is inferred.
+
+## Conventions and integration
+
+Source/version, deflection sign and moment-reference descriptions are mandatory.
+For example, positive deflection may mean trailing edge down and CM may refer to
+quarter chord. All datasets must share reference chord/area conventions, section
+axes and moment origin. Metadata records those assumptions but cannot verify the
+physical meaning of externally supplied data.
+
+Pass the model directly to ``WingSegment`` or ``SegmentedWing``. Segments already
+accept their own `controlDeflectionRadians`, so an external caller can supply
+differential aileron, elevator or rudder geometry without adding actuator state here.
+Horizontal and vertical tail surfaces use the same section/strip contracts with
+the appropriate supplied section axes and positions. Do not apply another incidence
+or camber correction for the same deflection when the dataset already includes it.
+
+```swift
+let controlled = try TabulatedControlSurface(settings: [
+ ControlSurfaceSetting(deflectionRadians: -0.1, airfoil: negativeDeflectionData),
+ ControlSurfaceSetting(deflectionRadians: 0, airfoil: neutralData),
+ ControlSurfaceSetting(deflectionRadians: 0.1, airfoil: positiveDeflectionData)
+], source: "Caller-supplied control polar database", version: "1",
+ deflectionConvention: "Positive trailing edge down",
+ momentReferenceDescription: "Quarter chord in section axes")
+let segment = try WingSegment(positionMetres: SIMD3(-3, 1, 0),
+ axes: WingSectionAxes(incidenceRadians: 0), chordMetres: 1, areaSquareMetres: 1,
+ controlDeflectionRadians: 0.05, model: controlled)
+let loads = try segment.evaluate(bodyFlow: flow).loads
+```
+
+The example datasets and local flow are provided by the caller. No measured flap,
+rudder or tail database is bundled. Section moments include the dataset CM plus
+the existing force lever arm, with no separate centre-of-pressure addition.
+Independent strips still do not compute spanwise circulation, wake interaction or
+finite-wing control effectiveness automatically.
+
+## Stall and data loading
+
+Nonlinear lift curves, rising drag and post-stall pitching moments can be represented
+by supplied polar samples. They are preserved rather than replaced by a lift-slope
+formula. This is a quasi-steady interpolation model, not a dynamic-stall, hysteresis,
+hinge-moment, flutter or unsteady separation model. Sparse sampling can miss extrema;
+coverage does not itself prove accuracy. The low-speed attached-flow limits of
+``FiniteWingAirfoil`` must not be extended simply because a control polar has
+post-stall samples.
+
+``ControlSurfaceTableLoader`` reads JSON. Codable decoding revalidates the table,
+deflection settings and nested airfoil grids. Tests cover four-coordinate affine
+interpolation, exact settings, different incidence coverage, rejection/clamping,
+duplicate coordinates, invalid decoded data and a supplied post-stall curve.
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/EntryHeating.md b/Sources/Aerodynamics/Aerodynamics.docc/EntryHeating.md
new file mode 100644
index 0000000..5214378
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/EntryHeating.md
@@ -0,0 +1,77 @@
+# Entry surface and leading-edge heating
+
+Use explicit recovery/chemistry data for local surface heating and a bounded swept-cylinder approximation at the leading-edge stagnation line.
+
+## Enthalpy-based surface data
+
+``EnthalpySurfaceHeatingModel`` is separate from low-speed temperature-difference
+convection. ``EnthalpySurfaceHeatingQuery`` requires local edge flow, streamline
+distance, gas identity and wall/adiabatic-wall enthalpies sharing the dataset's
+reference. Adiabatic-wall enthalpy includes recovery; it is not automatically the
+edge static or total enthalpy. Real-gas chemistry and catalytic-wall assumptions
+must be supplied with the data rather than replaced by a constant cp times temperature.
+
+``TabulatedEnthalpySurfaceHeating`` evaluates
+`q = rho_edge V_edge St (h_adiabaticWall - h_wall)` in W/m². The sign preserves
+convective cooling. Its dimensionless Stanton table uses, in order, axes named
+`mach`, `log10Re` and `wallEnthalpyRatio`, each with units `1`. Reynolds uses edge
+viscosity/density and the supplied streamline distance. The last coordinate is
+wall enthalpy divided by adiabatic-wall enthalpy, so the chosen enthalpy reference
+must remain consistent. Positive adiabatic-wall enthalpy is required.
+
+A dataset explicitly declares laminar or turbulent boundary layer; selection and
+transition detection remain caller responsibilities. Each table needs gas identity,
+source, version and assumptions covering geometry, pressure gradient, chemistry
+and catalytic state. Its rectangle must be wholly supported by the data, including
+intermediate interpolated conditions. There is no extrapolation, automatic
+laminar/turbulent switch or built-in calibrated high-enthalpy surface dataset.
+``EnthalpySurfaceHeatingCoverage`` also bounds edge temperature, edge pressure,
+absolute adiabatic-wall enthalpy and streamline distance. These checks prevent
+a Mach/Reynolds match from silently admitting an unsupported thermochemical state.
+Kn must not exceed the declared continuum limit (at most 0.01). Missing edge temperature/pressure, local sound
+speed, viscosity or mean free path throws. Rest/zero Reynolds is outside coverage.
+
+## Swept leading edge
+
+``LeadingEdgeConvectiveHeatingModel`` accepts a ``LeadingEdgeHeatingQuery`` so
+higher-fidelity geometry/chemistry models can replace the initial provider.
+``SweptCylinderStagnationHeating`` implements the idealized laminar **Earth-air**
+geometry approximation `q_line = q_sphere / sqrt(2) * sqrt(Rsphere/RleadingEdge)
+* cos(effectiveSweep)^1.1`. Its reference sphere evaluator and radius are explicit;
+the query radius denotes the actual leading-edge radius. The sphere provider
+retains its own gas, wall and flow restrictions. Effective sweep is relative to
+incident flow. Declared speed/density/radius/Mach/Kn limits are checked using the
+actual leading-edge radius; implementation sweep is restricted to at most ±60°.
+This restriction is not an experimental accuracy guarantee. It does not calculate
+sweep from vehicle attitude or discover the stagnation line. Other gases require
+separately justified models or data.
+
+The source geometry approximation is [NASA CR-181922, equation 1](https://ntrs.nasa.gov/api/citations/19900007739/downloads/19900007739.pdf).
+Its implementation is verified against unswept and 60° reference calculations.
+It predicts a stagnation **line**, with no circumferential distribution, shock
+interaction, transition or acreage distribution. Do not use a small leading-edge
+radius with a sphere model's Kn check alone: the smaller radius can be rarefied
+while the reference sphere is still in continuum flow.
+
+## Incoming radiation
+
+``TabulatedRadiativeHeating`` implements ``RadiativeHeatingModel`` using a supplied
+cold-wall shock-layer dataset. Its axes are `speed` (`m/s`), `density` (`kg/m^3`)
+and spherical nose `radius` (`m`), in that order, with values in `W/m^2`. Gas identity,
+provenance, version, assumptions, freestream-temperature range and declared
+continuum coverage are mandatory.
+It accepts cold-wall queries without additional stagnation-gas state. It does not
+infer radiative equilibrium, chemistry, optical thickness or wall emissivity, and
+no universal planetary radiation correlation is bundled. Missing radiation data
+still means unknown, not zero. Convective and radiative contributions can be
+combined externally only when they describe the same state and position.
+
+All these evaluations are stateless. Temperature evolution, radiative emission,
+conduction, ablation and changes in geometry/mass belong to external thermal and
+systems packages. The supplied-data tests use analytic synthetic fixtures to
+verify interpolation, units, signs, identity and coverage; they do not validate a
+real vehicle database. See for the runnable entry harness and
+its distinction between integration error and physical-model error.
+
+The enthalpy/Stanton formulation is described in
+[NPTEL compressible boundary-layer heat transfer](https://archive.nptel.ac.in/content/storage2/courses/101103003/module5/lec26/4.html).
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/FiniteWing.md b/Sources/Aerodynamics/Aerodynamics.docc/FiniteWing.md
new file mode 100644
index 0000000..96d3da9
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/FiniteWing.md
@@ -0,0 +1,78 @@
+# Equivalent finite-wing correction
+
+Add bounded induced-angle and induced-drag corrections to a supplied section polar.
+
+``FiniteWingAirfoil`` implements ``AirfoilCoefficientModel`` and can wrap a
+``TabulatedAirfoil`` or another checked polar. This is a steady equivalent-wing
+approximation for attached, low-speed flow. It is not a spanwise lifting-line solver,
+a wake model or a hypersonic correction.
+
+## Physical model
+
+For aspect ratio `AR = span² / area` and supplied span efficiency `e`, solve:
+
+```text
+alpha = alphaEffective + CL(alphaEffective) / (pi e AR)
+alphaInduced = CL / (pi e AR)
+CDinduced = CL² / (pi e AR)
+CDtotal = CDprofile(alphaEffective) + CDinduced
+```
+
+The underlying polar supplies profile drag only. Do not wrap data that already
+contains finite-wing induced drag, combine this correction with a second induced-drag
+model, or also apply its induced angle as a separate local-flow correction.
+Moment is the underlying polar's moment at effective incidence, about its original
+moment reference. This simple model does not predict finite-wing changes to that
+moment reference or spanwise pressure distribution.
+
+For a linear polar with slope `a0`, the resulting wing lift slope is
+`a = a0 / (1 + a0 / (pi e AR))`. Cambered polars retain their zero-lift offset through
+the implicit solution rather than simply multiplying all coefficients by a factor.
+The induced-drag basis is [NASA's induced-drag coefficient relation](https://www1.grc.nasa.gov/beginners-guide-to-aeronautics/induced-drag-coefficient/).
+
+## Explicit coverage and solver limits
+
+The caller declares an attached-flow effective-angle bracket covered by the polar,
+and a separate geometric operating-angle interval. The implementation restricts
+aspect ratio to at least four, Mach to at most 0.3, and both angle intervals to
+±0.35 radians. These are deliberately chosen model limits, not an accuracy certificate.
+Calibrating efficiency and confirming attached flow remain responsibilities of the
+supplied aerodynamic data; the model does not detect stall or separation.
+
+Bisection solves the angle residual with a configurable tolerance and iteration
+budget. ``FiniteWingSolution`` returns effective angle, induced angle, induced drag,
+coefficients, residual and iterations. Input coverage errors from the polar propagate.
+An unbracketed solution or exhausted budget throws ``FiniteWingError``; there is no
+silent fallback to infinite-wing coefficients. Multiple/post-stall roots are outside
+the intended physical assumptions, and numerical convergence does not prove uniqueness.
+
+```swift
+import Aerodynamics
+// `polar` is a caller-supplied checked, attached-flow airfoil model.
+let corrected = try FiniteWingAirfoil(airfoil: polar,
+ aspectRatio: 8, spanEfficiency: 0.8,
+ effectiveAngleRangeRadians: -0.2...0.2,
+ operatingAngleRangeRadians: -0.15...0.15)
+let solution = try corrected.solve(angleOfAttackRadians: 0.1,
+ reynoldsNumber: 1_000_000, machNumber: 0.2)
+```
+
+## Use with wing strips
+
+For uniform geometry and flow, the equivalent coefficient model can be wrapped in
+``AirfoilWingSectionModel`` and supplied to ``SegmentedWing``. Use the **whole wing's**
+aspect ratio on every strip, never the individual strip's aspect ratio. Uniform-wing
+forces then do not depend on segmentation resolution.
+
+Applying this equivalent model separately to arbitrary twisted, controlled or
+nonuniformly loaded strips is not a true coupled finite-wing calculation. Such cases
+require spanwise circulation/induced-flow coupling or validated finite-wing datasets.
+Tail interference and downstream wake velocities are not generated by this model.
+
+`swift run FluidPhysicsDemo` demonstrates the correction on a uniform rectangular
+wing with synthetic data. Tests compare with the analytic linear-polar result,
+cambered and infinite-aspect-ratio limits, signed lift and positive induced drag,
+explicit coverage/bracketing/budget failures and uniform strip-count independence.
+
+For a straight wing with supplied linear polars and spanwise incidence/chord
+variation, see for the bounded coupled solver.
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/Foundations.md b/Sources/Aerodynamics/Aerodynamics.docc/Foundations.md
new file mode 100644
index 0000000..6f8f62e
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/Foundations.md
@@ -0,0 +1,132 @@
+# Flow, coefficient data and physical loads
+
+Evaluate aerodynamic physics from supplied local flow and geometry, independently of vehicle systems.
+
+Aerodynamics owns coefficients, section geometry and physical loads. Vehicle assembly,
+actuator commands, deployment/reefing sequences, gas management and thermal/structural
+state evolution belong to external consumers. Wing strips and whole-body coefficient evaluators build on this foundation; see
+. A bounded equivalent finite-wing correction is available; spanwise wake flow, vehicle-specific entry datasets and
+heating correlations remain follow-up work.
+
+## Coefficient datasets
+
+``AirfoilPolar`` preserves explicit angle samples at one Reynolds/Mach condition.
+``TabulatedAirfoil`` interpolates linearly in angle, Reynolds number and Mach number.
+The Reynolds/Mach grid must be rectangular and contain exactly one polar at every
+condition. Different polars may have different angle spacing. For a query, only
+contributing polars must cover the requested angle. A singleton axis covers only its
+one value under the default rejecting policy; it does not imply Reynolds/Mach independence.
+
+```swift
+import Aerodynamics
+let samples = [
+ AirfoilSample(angleOfAttackRadians: -0.1,
+ coefficients: AirfoilCoefficients(lift: -0.5, drag: 0.02, moment: 0)),
+ AirfoilSample(angleOfAttackRadians: 0.1,
+ coefficients: AirfoilCoefficients(lift: 0.5, drag: 0.02, moment: 0))
+]
+let polar = try AirfoilPolar(reynoldsNumber: 1_000_000, machNumber: 0.2, samples: samples)
+let model = try TabulatedAirfoil(polars: [polar], source: "Example synthetic polar", version: "1")
+let coefficients = try model.coefficients(
+ angleOfAttackRadians: 0.05, reynoldsNumber: 1_000_000, machNumber: 0.2)
+```
+
+Tables reject malformed/nonfinite coefficients, nonpositive Reynolds numbers,
+negative Mach numbers, duplicate or unordered angles, duplicate conditions and missing
+grid cells. Coefficient signs are preserved; validation does not certify scientific
+accuracy or a nonnegative measured drag. Codable decoding revalidates the data.
+Out-of-coverage queries throw by default. ``CoefficientBoundaryPolicy/clamp`` explicitly
+uses the nearest boundary value instead; this is not a physical extrapolation model.
+
+``AirfoilTableLoader`` reads the existing XFOIL-style YAML columns: angle in degrees,
+CL, CD, CDp and CM. Every `data` entry is retained; optional `mach-number` defaults to
+zero. File I/O is separate from evaluation and source/version metadata is explicit.
+Malformed rows or conditions fail before constructing the evaluator.
+
+The legacy ``ParametricAirfoil`` remains available. Its scalar queries use radians,
+query Mach zero and explicitly clamp to dataset boundaries. Invalid queries return
+NaN. It now interpolates between loaded Reynolds datasets and preserves irregular
+angle samples. Prefer the throwing table API when coverage matters. Existing 361-sample
+Codable degree grids are readable, as are older 362-sample grids with −181° padding;
+new encoding retains the validated table, coordinate samples and provenance.
+
+## Flow conventions and missing properties
+
+`FluidFlow` uses right-handed body or section axes: X forward, Y right,
+Z down. Its velocity is the body's motion relative to the atmosphere. Positive
+angle of attack is `atan2(vz, vx)`; sideslip is `atan2(vy, hypot(vx, vz))`.
+Angle of attack is absent when the X/Z velocity projection is zero; sideslip is absent
+at zero speed. All vectors must be expressed in the same axes by the caller.
+
+Atmospheric rest depends on the reference frame. In a planet-centred inertial frame
+(for example, with ICRF-aligned axes), a rigidly co-rotating atmosphere has velocity
+`vAir = ΩPlanet × r + wind`. Here `wind` is motion relative to the rotating planet,
+expressed in the inertial axes. In the planet-fixed rotating frame, the co-rotation
+term disappears and `vAir = wind`; a still atmosphere therefore has zero velocity.
+This does not imply that the vehicle's relative velocity is zero.
+
+Compute `vRelative = vVehicle − vAir` at the same position in a common frame,
+then rotate that difference into vehicle or section axes. A full velocity transform
+to rotating coordinates includes the frame's `Ω×r` term; rotating vector components
+alone does not perform that transform. Since both velocities acquire the same frame
+term, it cancels in their difference. Atmospheric co-rotation must be included once.
+CelMek's `SphericalBodyAtmosphere` already supplies it for planet-centred inertial
+states. Atmospheric profiles themselves supply thermodynamic properties, not frames
+or wind velocities.
+
+Dynamic pressure uses `q = ρ V² / 2`. Mach, Reynolds and Knudsen numbers require
+speed of sound, dynamic viscosity and mean free path respectively. Missing properties
+remain unavailable; they never become zero. Reference lengths must be positive.
+Atmospheres profiles can directly supply ambient properties:
+
+```swift
+import Aerodynamics
+import Atmospheres
+let ambient = try ISAAtmosphere().properties(at: 0)
+let flow = try FluidFlow(
+ relativeVelocityMetresPerSecond: SIMD3(100, 0, 0), properties: ambient)
+let reynolds = try flow.reynoldsNumber(referenceLengthMetres: 1)
+let local = try flow.atLocalPoint(
+ offsetMetres: SIMD3(0, 2, 0), angularVelocityRadiansPerSecond: SIMD3(0, 0, 0.1))
+```
+
+Local velocity adds `(ωVehicle − ωMedium)×offset` for a rigidly rotating medium.
+The optional `mediumAngularVelocityRadiansPerSecond` defaults to zero for uniform air. Callers supply actual winds,
+atmospheric gradients and coordinate transformations; no orientation or ephemeris is
+inferred. Measure both rates relative to the same frame and express them in the same axes as
+the offset. In an inertial frame, supply the planet's rate as the medium rate. In a
+planet-fixed frame, supply the vehicle's rate relative to the planet and zero medium
+rate. The flow at the reference point must already subtract atmospheric velocity. Alternatively, sample vehicle and air
+velocities at every strip, including atmospheric co-rotation and wind gradients.
+The units and definitions follow [NASA dynamic pressure](https://www1.grc.nasa.gov/beginners-guide-to-aeronautics/dynamic-pressure-2/)
+and [Reynolds number](https://www.grc.nasa.gov/WWW/K-12/airplane/reynolds.html).
+
+## Forces and moments
+
+`FluidCoefficients` carries three signed force and three moment components.
+`FluidReferenceGeometry` states area, three moment reference lengths and a
+moment reference point. Aircraft moment lengths typically use span/chord/span.
+`FluidLoads` contains force in N and moment in N m in the same caller-selected
+axes. Coefficient conversion uses `F = q S C` and `M = q S L Cmoment`.
+The moment already includes the full coefficient moment about its stated reference
+point; do not add a second centre-of-pressure moment for the same load.
+
+Transferring the moment to another point uses `Mnew = Mold + (rold−rnew)×F`.
+Load addition first transfers the other moment to the receiving load's reference
+point. This operation aggregates physics without owning a vehicle assembly.
+Reference points and force/moment vectors must use the same origin and axes;
+the types do not perform frame transforms or certify coordinate compatibility.
+
+`SurfaceHeatFlux` provides a surface position and positive inward heat flux in
+W/m² for correlations and external thermal integration. See for
+the initial stagnation-point evaluator. The value itself does not evolve temperature
+or manage ablation.
+
+## NACA geometry
+
+``NACA4`` computes thickness offsets normal to the actual camber-line tangent,
+including a zero-camber limit without division by zero. Coordinates are normalized
+by chord; evaluation covers `0...1`. The conventional thickness polynomial retains
+a finite trailing-edge gap. Use the throwing geometry initializer and
+`surfaceCoordinates(atChordFraction:)` for recoverable input validation; legacy
+methods retain preconditions. The basis is [NASA-TM-X-3284](https://ntrs.nasa.gov/citations/19760003945).
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/LiftingLine.md b/Sources/Aerodynamics/Aerodynamics.docc/LiftingLine.md
new file mode 100644
index 0000000..bb2cafe
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/LiftingLine.md
@@ -0,0 +1,77 @@
+# Coupled spanwise lifting line
+
+``LiftingLineWing`` solves a straight, unswept planar wing in uniform incident
+flow. Unlike independent strips or an equivalent whole-wing correction, its
+circulation and induced incidence are coupled across the span. It accepts supplied
+linear section polars with spanwise chord, incidence and zero-lift-angle variation.
+
+Use it for attached, low-speed flow: aspect ratio ≥ 4, Mach ≤ 0.3, zero sideslip
+within numerical tolerance, speed ≥ 1 m/s and small angles. Every station must
+satisfy its declared effective-incidence and Reynolds coverage. Lift slopes are
+positive and bounded to 0.01…20 per radian; geometric/zero-lift angles and declared
+effective-incidence bounds stay within ±0.35 rad. These implementation limits do
+not constitute validated accuracy bounds for a particular wing.
+
+## Geometry and section inputs
+
+The reference line lies along body Y, with a supplied centre in body axes. All
+section moments refer to that same straight line; positions of swept or staggered
+quarter-chord lines are not represented. The constructor samples
+`sectionAtSpanFraction` at cosine-spaced stations, from left (−1) to right (+1).
+``LiftingLineSection`` supplies chord, lift slope, zero-lift angle, incidence,
+constant profile drag, pitching moment and coverage. Profile drag excludes induced
+drag. Supplied control/camber changes may alter these parameters externally; no
+control-effectiveness factor or actuator state is inferred.
+
+Reference area sets coefficient normalization and must match the geometry/dataset.
+Rectangular area is span times chord; elliptical area is π span rootChord / 4.
+Stations do not include the tips, where circulation vanishes. Chord/span ratios at
+sampled stations must lie within 1e-6…1. Station count is configurable from 2 to 64,
+with eight as the initial default rather than an accuracy claim.
+
+```swift
+let wing = try LiftingLineWing(spanMetres: 8,
+ referenceAreaSquareMetres: 4 * .pi, stationCount: 16,
+ source: "Ideal elliptical wing", version: "1") { fraction in
+ try LiftingLineSection(chordMetres: 2 * sqrt(1 - fraction * fraction),
+ liftSlopePerRadian: 2 * .pi, profileDragCoefficient: 0.02,
+ effectiveAngleRangeRadians: -0.2...0.2, reynoldsRange: 1e3...1e8)
+}
+let result = try wing.evaluate(flow: flow)
+```
+
+The example parameters are idealized. Flow supplies sound speed and viscosity for
+coverage checks, and is already relative to the atmosphere in the stated body axes.
+This model does not sample local rotation, varying incident speed or wind gradients.
+Those require a more general lifting-line/wake formulation; the independent-strip
+sampler remains available for externally prescribed local flow.
+
+## Solution and loads
+
+The sine-series collocation system is solved with a pivoted factorization cached
+at construction. Setup costs O(N³) and each query O(N²). ``LiftingLineResult`` returns
+Fourier coefficients, per-station circulation/effective incidence, lift, profile
+and induced drag coefficients, span efficiency and maximum equation residual.
+Numerically zero total lift has undefined span efficiency, even when asymmetric
+circulation produces nonzero induced drag.
+
+Lift, induced drag and the spanwise lift moment use Fourier integrals. Profile drag,
+section pitching moments and the spanwise drag moment use numerical quadrature;
+increase station count to check their convergence. Local induced-drag allocation
+uses the small-angle lifting-line approximation. The returned force/moment are
+about an explicit point and can feed CelMek's aerodynamic wrench adapter.
+
+Do not add another finite-wing correction or induced-drag load for the same wing.
+The linear section data does not supply nonlinear stall, dynamic stall, compressibility,
+surface interference, multiple-wing wakes or a validated control database.
+`FiniteWingAirfoil` remains the cheaper equivalent uniform-wing option.
+
+Tests reproduce elliptical lift slope and minimum induced drag at several station
+counts, an analytic second-harmonic twist/rolling moment, rectangular convergence,
+constant profile drag, reference-point transfer and unsupported coverage.
+
+References: [classical lifting-line Fourier formulation](https://www.mdpi.com/2076-3417/15/6/3383)
+and [NASA induced-drag relationship](https://www1.grc.nasa.gov/beginners-guide-to-aeronautics/induced-drag-coefficient/).
+
+For supplied nonlinear polars, nonuniform incident flow and coupled fixed wakes
+between surfaces, see .
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/ModelCoverage.md b/Sources/Aerodynamics/Aerodynamics.docc/ModelCoverage.md
new file mode 100644
index 0000000..4120f17
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/ModelCoverage.md
@@ -0,0 +1,107 @@
+# Model coverage and validation
+
+Select the physical approximation and data coverage explicitly, then assess numerical convergence separately.
+
+## Selection and cost
+
+| Provider | Supported approximation / required data | Evaluation cost |
+| --- | --- | --- |
+| Checked airfoil/control/body tables | Supplied rectangular incidence, Mach, Reynolds and optional control grid; no implied validity between different regimes | Up to 16 body-grid corners; section/angle lookup also searches samples |
+| SegmentedWing | Independent strips and sampled local flow; no automatic wake | O(N) |
+| FiniteWingAirfoil | Uniform equivalent attached low-speed wing, AR ≥ 4 | Iterative scalar root |
+| LiftingLineWing | Straight planar unswept wing, linear sections, uniform Mach ≤ 0.3 flow | O(N³) setup, O(N²) evaluation |
+| NonlinearLiftingLine | Supplied nonlinear sections, nonuniform flow, unswept fixed wakes and mutual surface coupling, Mach ≤ 0.3 | O(N²) setup/memory, O(I N²) solve |
+| ModifiedNewtonianPressure | Windward calorically perfect gas, declared Mach ≥ 5 and Kn ≤ 0.01 | O(1) per panel |
+| MaxwellianFreeMolecularTraction | Single-species Maxwellian, specified reflection/wall temperature, Kn ≥ 10 | O(1) per panel |
+| TabulatedRarefiedTraction | Supplied consistent gas/surface data across declared Kn/incidence/speed/wall-temperature range | At most 16 corners per pressure/shear lookup |
+| LaminarFlatPlateHeating / TurbulentFlatPlateHeating | Low-Mach isothermal attached zero-pressure-gradient plate; explicit film properties and boundary-layer choice | O(1) per point |
+| TabulatedEnthalpySurfaceHeating | Supplied gas/geometry/recovery/catalytic assumptions, explicit laminar/turbulent Stanton data, Kn ≤ 0.01 | At most 8 corners |
+| SuttonGravesHeating / mixture / H₂-He | Distinct gas-specific stagnation correlations with their own bounds and wall assumptions | O(1) per point |
+| SweptCylinderStagnationHeating | Idealized laminar Earth-air stagnation line, supplied sphere model, bounded effective sweep | One sphere evaluation plus O(1) |
+| TabulatedRadiativeHeating | Supplied cold-wall shock-layer radiation data and gas-specific continuum coverage | At most 8 corners |
+| ActuatorDiskSlipstream | Prescribed axial thrust/torque, ideal contracting top-hat slipstream and swirl; no body deflection | O(1) per point |
+| IncompressibleFlowGrid | Constant-density incompressible MAC grid, Mach ≤ 0.3, caller-established continuum applicability, fixed free-slip solids and prescribed box boundary velocities | O(substeps × cells × pressureIterations) |
+| DragAreaForces / buoyancy | Supplied current drag area/coefficient and displaced volume/local pressure gradient | Provider cost plus O(1) |
+
+Tables carry source, version and assumptions. `FluidScalarTable` supports
+1–8 named/unit-labelled axes, strict ordering, finite values and complete grids,
+with last-axis-fastest storage, multilinear interpolation and no extrapolation.
+JSON decoding revalidates structure. Physical wrappers additionally check axis
+names, units, signs and gas/geometry conventions. A rectangular interpolation grid
+must not span an unsupported hole in the physical dataset. Single-node dimensions
+are exact constraints, not unconstrained coordinates. Floating-point query values
+must remain within the declared endpoints.
+
+``CoveredBodyCoefficients`` binds a provider to reference lengths and explicit
+Mach/Reynolds/incidence/sideslip/Kn coverage. ``MachRegimeBodyCoefficients``
+dispatches by caller-chosen thresholds to bounded providers. A threshold belongs
+to the upper interval; it does not blend, extrapolate or hide discontinuities.
+Transonic/high-incidence support therefore comes from appropriate supplied body
+data, rather than a low-speed or hypersonic approximation stretched across all
+Mach numbers. No validated generic capsule/spaceplane database is bundled.
+
+## Gas and transport
+
+`PerfectGasMixture` stores explicit mass fractions of `PerfectGasSpecies` and
+mass-weights cp and R. Each species declares a constant-cp temperature range; the
+mixture uses their intersection. It supplies ideal-gas density and sound speed and
+can construct film transport properties with **caller-supplied** viscosity and
+conductivity. There is no viscosity/conductivity averaging rule or high-temperature
+chemistry inferred from composition. Species identifiers must be unique, positive
+mass fractions must sum to one, and property queries outside the shared temperature
+interval throw. Use a richer provider for dissociation, ionization, variable cp,
+non-equilibrium or multicomponent diffusion. A mixture-average R is not a resolved
+multispecies free-molecular model.
+
+## Failure and zero-flow behavior
+
+Checked constructors reject invalid geometry/nonfinite coefficients and incomplete
+data. Unsupported physical regimes throw `outsideCoverage`; missing state throws
+`missingFlowProperty`; incompatible identities/conventions throw `unsupportedQuery`.
+The nonlinear wake and CFD pressure solvers additionally report `nonConvergence`.
+CFD state updates are transactional; budget/coverage failure leaves the original grid unchanged.
+
+Whole-body/strip/drag-area evaluators return zero aerodynamic load at zero dynamic
+pressure without querying undefined incidence. The steady lifting-line solvers,
+forced-convection plate models and supplied enthalpy/radiation datasets reject
+rest when it lies outside their declared domains. Free-molecular traction retains
+thermal molecular impacts at zero bulk speed. Sutton–Graves cold-wall stagnation
+models retain their documented zero-speed convention. There is no universal
+zero-density-to-vacuum shortcut, fallback model or assumed zero heat flux when a
+provider is unavailable. Buoyancy is evaluated independently of airspeed.
+
+## Runnable entry comparison
+
+Run `swift run FluidPhysicsDemo`. In addition to wing/control/parachute/balloon
+examples it integrates 25 seconds of planar prescribed-attitude entry for a
+lifting capsule and a pressure-panel wing. The harness owns RK4, gravity, mass,
+attitude prescription and heat-load integration. Aerodynamics only returns loads
+and flux. It uses ISA below 86 km, explicitly approximate mean free path,
+synthetic capsule coefficients and an idealized pressure-only flat wing. Heating
+uses Earth-air Sutton–Graves and a swept-cylinder stagnation-line estimate.
+
+It reports peak deceleration, dynamic pressure, local heat flux and integrated
+local heat load, plus final-speed/heat-load changes when halving the step from
+0.2 to 0.1 seconds. The starting altitude is 70 km: the small leading-edge radius
+would fail continuum coverage at 80 km. Coverage checks remain active throughout
+the run. Heat load is J/m² at the chosen local point, not total vehicle energy or
+a thermal-protection temperature/survival prediction. Attitude is prescribed;
+this harness does not assess trim, structural response or closed-loop guidance.
+
+Step refinement measures integration sensitivity, not physical accuracy. Other
+tests separately compare spanwise convergence, classical lifting-line references,
+independent molecular quadrature, published stagnation-heating CFD and similarity
+heat-transfer values. The shared fluid implementations and their numerical tests now belong to FluidDynamics.
+Supplied-data tests establish interpolation and contracts;
+real vehicle data still needs independent calibration/validation.
+
+## Deliberate limits and later fidelity
+
+The initial physics/API workstream includes replaceable providers for the remaining
+regimes. The optional local incompressible solver is described in [shared propwash/CFD guide](/documentation/fluiddynamics/propellersandcfd).
+It does not include a general compressible CFD/DSMC/radiation solver or universal
+validated vehicle datasets. Free-wake rollup, swept/separated-wing fidelity,
+chemistry-resolved transport and high-enthalpy/transitional/radiative databases
+remain specialist extensions. Atmosphere coverage above ISA, thermal response and
+vehicle systems are separate workstreams, not missing state machines to place in
+Aerodynamics. See , and .
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/NonlinearWakes.md b/Sources/Aerodynamics/Aerodynamics.docc/NonlinearWakes.md
new file mode 100644
index 0000000..727a758
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/NonlinearWakes.md
@@ -0,0 +1,72 @@
+# Nonlinear sections and coupled wakes
+
+Solve a bounded fixed-wake lifting-line problem across supplied aerodynamic strips.
+
+``NonlinearLiftingLine`` accepts ``WingSegment`` geometry and the existing
+``WingSectionCoefficientModel`` contract, including tabulated nonlinear/control
+polars. Strips from separate wings or tails may share a solve. The caller samples
+incident flow at each strip, including local rotation, atmosphere gradients,
+external body interference or prescribed winds. No vehicle assembly is owned.
+
+Each strip is a constant-circulation horseshoe: a bound vortex along the supplied
+section span through its moment-reference point, with width `area/chord`, and two
+straight finite trailing legs. Use quarter-chord geometry and a matching section
+moment convention. Wake direction is physical air motion (normally body −X).
+It must be perpendicular to each strip's span; the model supports unswept lifting
+lines with incidence/dihedral and separated surfaces, rather than arbitrary swept
+or intersecting lifting lines. Distinct control points alone do not establish a
+well-resolved geometry. Avoid other bound/wake vortex cores and endpoints.
+
+The solver sums regularized Biot–Savart air velocity, subtracts it from each
+incident body-relative velocity, queries the section model and relaxes toward
+`Gamma = 0.5 V_section chord CL`. It reports circulation, induced air velocities,
+section results, loads, iteration count and maximum circulation residual normalized
+by incident `0.5 V chord`. A failed solve throws `nonConvergence`; it never returns
+an unconverged best guess. Multiple nonlinear roots or convergence from a zero
+initial state do not establish uniqueness or post-stall physical accuracy.
+
+```swift
+let sections = try SegmentedWing.rectangular(spanMetres: 8, chordMetres: 1,
+ model: sectionModel).segments
+let solver = try NonlinearLiftingLine(segments: sections,
+ wakeLengthMetres: 800, vortexCoreRadiusMetres: 0.0001)
+let result = try solver.evaluate { segment in
+ try incidentFlow.atLocalPoint(offsetMetres: segment.positionMetres,
+ angularVelocityRadiansPerSecond: suppliedBodyRate)
+}
+let airWake = try solver.inducedAirVelocity(at: downstreamBodyPoint,
+ circulation: result.circulationSquareMetresPerSecond)
+let downstreamFlow = try incidentFlow.replacingRelativeVelocity(
+ incidentFlow.relativeVelocityMetresPerSecond - airWake)
+```
+
+Both vectors must share axes, units and frame. `FluidFlow/replacingRelativeVelocity(_:)`
+also works with body, panel and parachute providers. For mutually interacting
+lifting surfaces, put all their strips in one solver; successive isolated solves
+provide only one-way interaction. Body shielding, wake deficits and arbitrary
+interference may be supplied through the flow sampler; they are not inferred.
+
+Loads use the converged effective flow, so its tilted lift already produces induced
+drag. Supply **section profile drag**; do not wrap the polar in ``FiniteWingAirfoil``
+or add another induced-drag force. Section moments and force lever arms are summed
+once about the requested reference point.
+
+Limits are Mach ≤ 0.3, incident speed ≥ 1 m/s, incident alignment within 0.35 rad
+of the upstream wake axis, incident spanwise speed ≤ 10% of speed, section incidence
+within ±0.35 rad and |CL| ≤ 2. Provider coverage also applies at every iterate.
+No 3-D separation, transonic shocks, dynamic stall, free-wake rollup or ground
+images are inferred. A supplied post-stall polar remains an approximation of local
+2-D behavior. Zero density/rest are outside this steady circulation solver's coverage.
+
+At most 256 strips are accepted. Setup/memory cost O(N²), evaluation O(I N²).
+Relaxation, residual tolerance, iteration cap, wake length and core radius are
+explicit. Core radius is limited to 2% of the narrowest strip; this is a numerical
+restriction, not a vortex-physics model. Refine strip count, increase wake length
+and decrease core radius independently to assess numerical sensitivity.
+
+Tests compare a single horseshoe against an independent semi-infinite-vortex/scalar
+root solution, check 8/16/32/64-strip convergence against Fourier lifting line, and
+exercise nonlinear polar response, two-way wing/tail coupling, nonuniform flow,
+reference-point transfer and explicit failures.
+
+Background: [CN-AeroModels nonlinear lifting-line formulation](https://lheea.gitlab.io/CN-AeroModels/nonlinear_lifting_line.html).
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/ParachutesAndBalloons.md b/Sources/Aerodynamics/Aerodynamics.docc/ParachutesAndBalloons.md
new file mode 100644
index 0000000..52f05fc
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/ParachutesAndBalloons.md
@@ -0,0 +1,76 @@
+# Parachute and balloon loads
+
+These evaluators compute steady physical loads for caller-supplied geometry and
+local flow. They do not own a vehicle, deployment sequence, inflation state,
+opening shock, gas inventory or thermal evolution.
+
+## Steady drag
+
+`DragAreaForces` applies `F = −velocityDirection q Cd area` at an explicit
+force application point and transfers the resulting moment to the requested point.
+``ParachuteAerodynamics`` uses this contract for a supplied current canopy.
+Area must follow the coefficient dataset's definition, such as nominal canopy area
+or projected area. Supply shape, reefing and wake effects through the current area
+or a calibrated coefficient provider; count each correction once.
+
+`DragCoefficientModel` permits custom providers. `TabulatedDragCoefficients`
+validates a complete rectangular Mach/Reynolds grid, nonnegative coefficients,
+source and version, and interpolates linearly in each coordinate. It rejects queries
+outside the grid and requires sound speed and viscosity. A supplied axis points
+along positive vehicle-relative-to-air motion at zero incidence; its angle with
+that velocity is available to custom providers. The table may restrict that angle
+but does not invent orientation dependence inside the permitted range. Without an
+angle limit it declares orientation-invariant coefficients. It does not project the
+area automatically or generate lift, pitching moment or canopy stability.
+
+```swift
+let data = try TabulatedDragCoefficients(samples: [
+ DragCoefficientSample(machNumber: 0, reynoldsNumber: 1e4, dragCoefficient: 1.5),
+ DragCoefficientSample(machNumber: 0, reynoldsNumber: 1e6, dragCoefficient: 1.5),
+ DragCoefficientSample(machNumber: 0.5, reynoldsNumber: 1e4, dragCoefficient: 1.5),
+ DragCoefficientSample(machNumber: 0.5, reynoldsNumber: 1e6, dragCoefficient: 1.5)
+], source: "Synthetic demonstration coefficients", version: "1")
+let drag = try DragAreaForces(areaSquareMetres: 20, referenceLengthMetres: 5,
+ forceApplicationPointMetres: SIMD3(0, 0, -2), model: data)
+let parachute = ParachuteAerodynamics(drag: drag)
+let loads = try parachute.evaluate(flow: flow)
+```
+
+The example coefficients are synthetic, not canopy performance data. Flow is
+sampled at the drag resultant location and must already include vehicle/atmosphere
+rotation and winds. All positions and vectors use common axes and origin. A canopy
+resultant and a force transmitted to a payload attachment are different physical
+loads: the external tether/multibody model establishes transmission. This evaluator
+does not move a canopy force to an attachment by assumption.
+
+Zero dynamic pressure or zero supplied area produces zero drag without querying
+coefficients. Area cannot be negative; reference length stays positive. A zero area
+can represent externally supplied collapsed geometry, but this contract provides
+no transient inflation loads or opening-load prediction.
+
+## Displaced-volume buoyancy
+
+`Buoyancy` accepts volume in m³ and centre of buoyancy in metres. Under local
+hydrostatic conditions, it returns `F = −ρ volume gravity`. Alternatively, with an
+approximately uniform pressure gradient, it returns `F = −volume gradientPressure`.
+`BuoyancyField` selects one description. The gradient includes the full ambient
+pressure field and is not added to a second hydrostatic buoyancy force. Density is
+used by the gravity form; the gradient form uses the supplied gradient directly.
+For significant atmospheric rotation or other departures from static hydrostatic
+conditions, supply the actual pressure gradient rather than substituting vehicle
+acceleration for gravity. Large bodies spanning significant gradients need a
+distributed pressure integration instead of the local uniform approximation.
+
+``BalloonAerodynamics`` adds this pressure force to optional supplied-shape drag,
+retaining each force's moment arm. It returns gross buoyancy, without subtracting
+lifting-gas, envelope or payload weight. External dynamics must use the full mass
+and apply gravity once. Volume, lifting-gas mass, gas heating/expansion, venting and
+envelope constraints remain external.
+
+Tests verify terminal parachute descent against external weight, oblique drag,
+force moment arms, buoyancy equilibrium, equivalent hydrostatic/gradient inputs,
+coefficient interpolation and supplied-state limits. Results can feed CelMek's
+existing aerodynamic wrench adapter without adding systems logic here.
+
+References: [NASA parachute recovery forces](https://www.grc.nasa.gov/www/k-12/VirtualAero/BottleRocket/airplane/rktvrecv.html)
+and [NASA balloon design](https://www.grc.nasa.gov/www/k-12/Numbers/Math/Mathematical_Thinking/designing_a_high_altitude.htm).
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/PlanetaryHeating.md b/Sources/Aerodynamics/Aerodynamics.docc/PlanetaryHeating.md
new file mode 100644
index 0000000..c87f0e9
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/PlanetaryHeating.md
@@ -0,0 +1,79 @@
+# Planetary heating parameters
+
+Heating parameters are explicit gas datasets, independent of the atmosphere
+catalogue. Density and temperature profiles alone do not identify a heating model.
+Use a query gas identifier matching the chosen parameter set.
+
+## Mars
+
+``SuttonGravesParameters/marsCarbonDioxideNitrogenColdWall`` supplies
+`k = 1.83e-4` for an idealized 97% CO₂ / 3% N₂ mixture **by mass**. Use it with
+``SuttonGravesHeating`` and caller-declared coverage. It is the simple cold-wall
+estimate, not the newer CFD correlation in the same paper.
+
+Source: [West and Brandis, 2020, equation 2](https://ntrs.nasa.gov/api/citations/20200002354/downloads/20200002354.pdf).
+
+## Venus and explicit mixtures
+
+``SuttonGravesMixtureParameters`` accepts mass or mole fractions of nine base
+gases. It derives the enthalpy-form coefficient using equation 42 and the rounded
+transport products in table I. Mole fractions are converted to mass fractions.
+``SuttonGravesMixtureParameters/venusCarbonDioxideNitrogen`` assumes 96.5% CO₂ /
+3.5% N₂ by mole, ignoring trace species. This is a derived mixture approximation,
+not a fitted Venus flight dataset.
+
+``SuttonGravesMixtureHeating`` requires ``StagnationGasState`` in the query:
+stagnation pressure in Pa and boundary-layer-edge specific enthalpy in J/kg.
+It uses `q = K sqrt((pStag/101325)/Rnose) hEdge`, neglecting wall enthalpy.
+The coefficient's source units contain atm and differ from the velocity-cubed
+coefficient; the evaluator performs the pressure conversion. Wall state must be
+absent for this cold-wall estimate. Flow and continuum coverage are also checked.
+Pressure and edge enthalpy are limited to the original study's 0.001…100 atm and
+2.3…116.2 MJ/kg ranges. These bounds do not establish the cold-wall approximation's
+accuracy for every state. The model does not solve equilibrium chemistry or infer
+shock-layer properties from an ISA-like profile.
+
+Sources: [Sutton–Graves report](https://ntrs.nasa.gov/citations/19720003329) and
+[NASA Venus composition](https://nssdc.gsfc.nasa.gov/planetary/factsheet/venusfact.html).
+
+## Hydrogen and helium
+
+``HydrogenHeliumColdWallHeating`` implements the separate nonlinear cold-wall
+fit. Its baseline is 81.55% H₂ / 18.45% He by mole, with a fully catalytic,
+non-ablating spherical wall at 300 K and freestream temperature 141.2 K. A missing
+wall adopts 300 K; other wall temperatures and inconsistent freestream temperature
+are rejected. It requires Mach ≥ 5, Kn ≤ 0.003, radius 0.2…1 m and density
+1e-5…0.1 kg/m³. Speed coverage follows a log-density interpolation of table-2
+boundary points rather than a full 7…45 km/s rectangle.
+
+``HydrogenHeliumHeatingMixture`` provides the Neptune baseline and Saturn/Uranus
+approximations. Their factors 0.952/0.980 originate in hot-wall composition studies
+and were also applied by the authors to cold-wall comparisons. They are not
+independent cold-wall fits. The model preserves the published branch switch at
+29 km/s, including an approximately 5–9% downward step for supported radii near
+that boundary; it does not smooth or extrapolate it.
+Diagnostics expose fitted pressure, enthalpy difference, K₂ and selected branch.
+Tests compare both flux and K₂ with all 180 Appendix-B CFD cases within 20%; this
+checks implementation against the dataset, not arbitrary trajectories.
+
+Source: [Carroll and Brandis, 2022](https://ntrs.nasa.gov/api/citations/20220018610/downloads/AIAA_Aviation_2022_Paper-6.pdf).
+
+## Example
+
+```swift
+let mixture = HydrogenHeliumHeatingMixture.neptuneReference
+let model = HydrogenHeliumColdWallHeating(mixture: mixture)
+let flow = try FluidFlow(relativeVelocityMetresPerSecond: SIMD3(19000, 0, 0),
+ densityKilogramsPerCubicMetre: 1e-4, temperatureKelvin: 141.2,
+ speedOfSoundMetresPerSecond: 1000, meanFreePathMetres: 1e-5)
+let query = try StagnationHeatingQuery(flow: flow, gasIdentifier: mixture.gasIdentifier,
+ noseRadiusMetres: 0.4, surfacePositionMetres: SIMD3(1, 0, 0),
+ wall: AerothermalWallState(temperatureKelvin: 300))
+let result = try model.evaluate(query)
+```
+
+Example sound speed and mean free path are supplied assumptions. No radiative flux
+is included. Jupiter, Titan and tenuous-moon heating presets remain unsupported.
+Current nominal atmosphere profiles also do not establish upper-atmosphere or
+transport coverage for these entry calculations. See for the
+external thermal-integration boundary.
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/RarefiedFlow.md b/Sources/Aerodynamics/Aerodynamics.docc/RarefiedFlow.md
new file mode 100644
index 0000000..035df34
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/RarefiedFlow.md
@@ -0,0 +1,113 @@
+# Free-molecular surface loads
+
+`SurfaceTractionModel` returns signed gauge pressure and tangential stress in Pa.
+`SurfaceTractionIntegration` integrates these over supplied surface panels,
+including force lever arms and moment-reference transfer. It validates that shear
+is tangential to each panel. `PressureOnlyTraction` adapts existing continuum
+pressure laws into the same contract with zero shear; it is an alternative evaluator,
+not an additional force to count alongside pressure-only integration.
+
+## Gas and surface inputs
+
+``MaxwellianFreeMolecularTraction`` describes independent impacts from an ideal
+single-species Maxwellian gas. ``FreeMolecularGas`` supplies specific gas constant
+in J/(kg K), identity and provenance. Flow supplies density, temperature, local
+vehicle-relative-to-air velocity and mean free path. Sound speed and viscosity are
+not required. Ambient pressure is computed as `ρ R T`; any supplied flow pressure
+must be consistent with those inputs. A mixture-average R is an additional
+approximation, not a species-resolved mixture treatment.
+
+``GasSurfaceReflection`` sets the specular fraction and wall temperature. Specular
+reflection transfers normal momentum without shear. The remaining fraction is fully
+accommodated diffuse re-emission at wall temperature, with outgoing molecular flux
+balancing incoming flux. This reflection fraction is not a general independent
+normal/tangential accommodation law, and is not inferred from material name.
+
+For outward normal `n`, let `U = vehicleVelocity · n`, `σ = sqrt(R T)` and `a = U/σ`.
+Incoming mass and normal momentum fluxes follow Gaussian half-space moments:
+
+`J = ρ σ [φ(a) + a Φ(a)]`
+
+`Pincident = ρ σ² [(a² + 1) Φ(a) + a φ(a)]`
+
+The diffuse outgoing pressure is `J sqrt(π R Twall / 2)`. The model combines that
+pressure with specular reflection, subtracts ambient pressure, and supplies diffuse
+shear opposite the tangential vehicle velocity. Thermal molecules can hit leeward
+faces, so they are not discarded by an incidence sign test. Deep leeward Gaussian
+tails use an asymptotic expansion to avoid subtraction cancellation.
+
+## Coverage and geometry
+
+The evaluator requires Kn ≥ 10 using the supplied reference length and mean free
+path. Missing temperature or mean free path throws, including at rest; low density
+does not imply vacuum or select a regime. A separate numerical bound requires
+`abs(U/σ) ≤ 1e6`. Zero speed does not necessarily mean zero pressure load when wall
+and gas temperatures differ. At equal temperatures, stationary gas produces zero
+gauge pressure and shear. A uniform closed body at rest has no net pressure force.
+
+Normals point outward. Gauge pressure may be negative on leeward panels; absolute
+surface pressure is obtained by adding `ρ R T`. Gauge subtraction removes the
+local ambient contribution, so these loads do not supply a separate hydrostatic
+buoyancy force. Sample consistent flow and any needed buoyancy separately.
+
+The exposure flag is a caller-supplied inclusion mask. A false flag skips the panel's
+traction; it does not solve molecular occlusion, reflected-particle reimpact or
+thermal-view geometry. Independent panels suit externally exposed geometry;
+concavities and nearby interacting surfaces need a more complete model. All flow,
+stress and location vectors use the same axes, with atmospheric co-rotation already
+included in relative flow. The panel sampling overload supports local rotation and
+external gradients.
+
+## Example
+
+```swift
+let gas = try FreeMolecularGas(identifier: "Supplied single-species gas",
+ specificGasConstantJoulesPerKilogramKelvin: 300, source: "Caller gas dataset")
+let surface = try GasSurfaceReflection(specularFraction: 0.2, wallTemperatureKelvin: 300)
+let model = try MaxwellianFreeMolecularTraction(gas: gas, surface: surface)
+let panel = try FluidSurfacePanel(areaSquareMetres: 1,
+ centreMetres: SIMD3(1, 0, 0), outwardNormal: SIMD3(1, 0, 0))
+let evaluator = try SurfaceTractionIntegration(panels: [panel],
+ referenceLengthMetres: 1, model: model)
+let flow = try FluidFlow(relativeVelocityMetresPerSecond: SIMD3(7000, 0, 0),
+ densityKilogramsPerCubicMetre: 1e-8, temperatureKelvin: 200, meanFreePathMetres: 20)
+let loads = try evaluator.evaluate(flow: flow).loads
+```
+
+These are demonstration inputs, not an atmosphere or material preset. No chemical
+reactions, ablation, heat flux or gas inventory is evolved. Do not extrapolate either endpoint model into slip/transitional flow.
+``TabulatedRarefiedTraction`` accepts a supplied consistent transition dataset
+through the same integration contract; no universal endpoint blend is inferred.
+
+Tests compare molecular fluxes with independent Simpson quadrature, equal-temperature
+rest and hot-wall limits, thermal leeward impacts, specular high-speed pressure,
+force/moment transfer and equivalence of the continuum pressure adapter.
+
+References: [NASA free-molecular pressure/shear formulation](https://ntrs.nasa.gov/api/citations/19890015753/downloads/19890015753.pdf)
+and [NASA rarefied-flow regime definitions](https://www.nas.nasa.gov/assets/nas/pdf/ams/2022/AMS_20220802_Singh.pdf).
+
+
+## Supplied transitional traction
+
+``TabulatedRarefiedTraction`` uses matched pressure/shear `FluidScalarTable`
+axes, ordered `log10Kn`, `incidenceCosine`, `speedRatio`, `wallTemperatureRatio`,
+all dimensionless. Incidence cosine is outward normal dotted with body-relative
+velocity direction; speed ratio is `V / sqrt(R T)`, and temperature ratio is
+`Tw / T`. Pressure values are gauge pressure divided by `rho R T`; nonnegative
+shear magnitudes use the same normalization and oppose tangential relative velocity.
+This normalization differs from conventional dynamic-pressure coefficients.
+Normals/rest have no tangential direction and must have zero interpolated shear;
+inconsistent data throws. Nonzero molecular thermal pressure at rest can remain.
+
+Gas R and wall temperature are explicit; source/version/assumptions must identify
+the gas composition, surface accommodation, geometry and data method (for example
+DSMC or a calibrated bridge). A complete rectangular dataset may include continuum,
+slip, transition and free-molecular conditions, with continuous multilinear output
+inside its stated coverage. The model never changes mean free path to trick the
+asymptotic evaluators into accepting unsupported states. Missing temperature/path
+or an out-of-range coordinate throws; no density-based vacuum fallback exists.
+Caller exposure flags remain the only shielding input.
+
+Tests use a synthetic affine dataset to verify log-Kn interpolation/continuity,
+normalization, shear direction and integrated moments. These tests do not validate
+a physical transition law; no calibrated transition dataset ships by default.
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/SurfaceHeating.md b/Sources/Aerodynamics/Aerodynamics.docc/SurfaceHeating.md
new file mode 100644
index 0000000..3137352
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/SurfaceHeating.md
@@ -0,0 +1,66 @@
+# Local surface convection
+
+Evaluate bounded laminar or fully turbulent flat-plate heat transfer separately from capsule stagnation heating.
+
+``SurfaceConvectiveHeatingModel`` accepts local boundary-layer-edge flow, distance
+along the streamline from the leading edge, a supplied wall temperature and
+`ThermalTransportProperties`. The latter carries gas identity/provenance and
+film-temperature density, viscosity, conductivity and specific heat. No body-specific
+transport defaults or chemistry are inferred. Film temperature is `(Te + Tw)/2`;
+the evaluator checks the supplied property temperature.
+
+``LaminarFlatPlateHeating`` implements the isothermal, zero-pressure-gradient,
+attached parallel-flow approximation `Nu_x = 0.332 sqrt(Re_x) Pr^(1/3)`, with
+`Re_x = rho_f V_edge x / mu_f`, `Pr = mu_f cp_f / k_f` and `h_x = Nu_x k_f / x`.
+The edge-flow density/viscosity are not used in place of film properties.
+``SurfaceConvectionResult`` retains signed `q = h_x (Te - Tw)`: positive heats the
+wall and negative cools it. This differs deliberately from the incoming-only
+`SurfaceHeatFlux` used by stagnation correlations. Do not clamp cooling to
+zero or add this flux to a stagnation correlation at the same point.
+
+Implementation bounds are Mach ≤ 0.3, local Reynolds 1,000–500,000, Prandtl
+0.6–15, local Knudsen ≤ 0.01 and wall/edge temperature ratio 0.8–1.25.
+These conservative limits are restrictions, not an accuracy guarantee or a
+transition detector. The caller must establish an attached laminar boundary layer,
+parallel edge flow and approximately uniform wall temperature and properties.
+Shock interactions, pressure gradients, sweep, separation, automatic turbulent transition,
+compressible recovery temperature and high-enthalpy chemistry need other models.
+Zero speed is outside forced-convection coverage; no natural-convection estimate
+is substituted. The singular leading edge at x=0 is rejected.
+
+```swift
+let transport = try ThermalTransportProperties(
+ gasIdentifier: "supplied-air", source: "caller property dataset",
+ temperatureKelvin: 315, densityKilogramsPerCubicMetre: 1.12,
+ dynamicViscosityPascalSeconds: 1.92e-5,
+ thermalConductivityWattsPerMetreKelvin: 0.0274,
+ specificHeatJoulesPerKilogramKelvin: 1007)
+let edge = try FluidFlow(relativeVelocityMetresPerSecond: SIMD3(10, 0, 0),
+ densityKilogramsPerCubicMetre: 1.07, temperatureKelvin: 330,
+ speedOfSoundMetresPerSecond: 364, meanFreePathMetres: 7e-8)
+let result = try LaminarFlatPlateHeating().evaluate(SurfaceHeatingQuery(
+ edgeFlow: edge, distanceFromLeadingEdgeMetres: 0.1,
+ surfacePositionMetres: SIMD3(0.1, 0, 0),
+ wall: AerothermalWallState(temperatureKelvin: 300), transport: transport))
+```
+
+Evaluation costs O(1) per point. Callers sample a surface distribution and integrate
+flux over area externally; no surface mesh, thermal evolution or assembly is owned
+by the model. Position is an output label, not a substitute for streamline distance.
+This establishes a surface-convection extension point and a low-speed reference
+model. Use for supplied high-enthalpy surface data and a bounded
+swept-cylinder stagnation-line approximation.
+
+The correlation and independent numerical similarity coefficients are given in
+[NPTEL External Flows, lecture 8, table 2.2](https://archive.nptel.ac.in/content/storage2/courses/112104159/module2/Lec8.pdf).
+Tests compare those coefficients, integrate the local distribution over a bounded
+plate interval and exercise heating/cooling, coverage and property requirements.
+
+
+``TurbulentFlatPlateHeating`` explicitly selects a fully turbulent boundary layer
+from the leading edge, with `Nu_x = 0.0296 Re_x^0.8 Pr^(1/3)` and Reynolds
+500,000–10,000,000. It retains the same Mach, Kn, Pr and temperature-ratio limits,
+film-property requirements and signed flux. It does not locate transition or model
+an initially laminar region. The different spatial dependence is tested alongside
+heating/cooling and out-of-range rejection. Source:
+[NPTEL External Flows, lecture 12](https://archive.nptel.ac.in/content/storage2/courses/112104159/module2/Lec12.pdf).
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/SurfacePressure.md b/Sources/Aerodynamics/Aerodynamics.docc/SurfacePressure.md
new file mode 100644
index 0000000..63d2443
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/SurfacePressure.md
@@ -0,0 +1,66 @@
+# Hypersonic surface pressure
+
+`SurfacePressureIntegration` integrates gauge pressure over supplied flat
+`FluidSurfacePanel` elements. Each panel has area in m², an outward normal,
+a centre in metres and a caller-supplied exposure flag. Geometry and flow use the
+same body axes. Subdivision is caller-selected; evaluation costs O(panel count).
+It returns per-panel pressure coefficients and gauge pressures plus force and
+moment about an explicit point, ready for CelMek's aerodynamic wrench adapter.
+
+`SurfacePressureCoefficientModel` permits replacement pressure laws. The initial
+``ModifiedNewtonianPressure`` approximation uses a calorically perfect gas with
+explicit specific-heat ratio γ. It computes downstream normal-shock Mach and static
+pressure, then isentropically decelerates to obtain stagnation pressure. The law is:
+
+`CpMax = (pStagnationBehindShock/pFreeStream − 1)/(γ Mach²/2)`
+
+`Cp = CpMax max(0, outwardNormal · vehicleRelativeVelocityDirection)²`
+
+Vehicle-relative velocity points into the windward outward normal. The pressure
+force is inward: `F = −normal Cp q area`. Panel moments use the force lever arm;
+ambient pressure is subtracted. For an open surface, these are aerodynamic gauge
+loads, not total structural pressure loads. Leeward, tangent and explicitly
+unexposed panels have zero pressure coefficient in this approximation.
+
+```swift
+let panel = try FluidSurfacePanel(areaSquareMetres: 1,
+ centreMetres: SIMD3(2, 0, 0), outwardNormal: SIMD3(1, 0, 0))
+let pressureModel = try ModifiedNewtonianPressure(specificHeatRatio: 1.4)
+let surface = try SurfacePressureIntegration(panels: [panel],
+ referenceLengthMetres: 1, model: pressureModel)
+let flow = try FluidFlow(relativeVelocityMetresPerSecond: SIMD3(1000, 0, 0),
+ densityKilogramsPerCubicMetre: 0.02, speedOfSoundMetresPerSecond: 100,
+ meanFreePathMetres: 0.001)
+let result = try surface.evaluate(flow: flow)
+```
+
+This synthetic example supplies γ and sound speed consistently with the chosen gas
+approximation. Thermodynamic profiles do not yet supply mean free path; it must be
+provided independently. The model requires known Mach and Knudsen numbers for
+nonzero speed, defaults to Mach 5…25 and Kn ≤ 0.01, and allows narrower caller
+coverage within Mach 5…50. Reference length must be positive and should represent
+the relevant body or local geometry scale. These are implementation coverage
+bounds, not guarantees of accuracy or proof that perfect-gas behavior applies.
+Zero speed returns zero aerodynamic pressure load without requiring gas properties.
+Unsupported coverage and missing properties throw even for unexposed panels.
+
+Use the panel-flow sampling overload to account for vehicle and atmospheric
+rotation, winds or gradients at each panel centre. Uniform-flow evaluation assumes
+the same flow everywhere. No geometry shadowing or shock interaction is inferred.
+Normals are normalized during construction; outward orientation and correct areas
+remain the caller's responsibility.
+
+The approximation is intended for idealized blunt-body windward pressure. It does
+not model viscous skin friction, base suction, expansion pressures, heating,
+dissociation or variable heat capacity. Add separately supported contributions
+without counting pressure drag twice; do not silently extrapolate it into another
+flight regime or treat constant γ as a real-gas entry model.
+
+Tests check a normal-shock stagnation reference, inclined-panel force and lever-arm
+moment, coverage and rest behavior, and convergence to the analytic unit-sphere
+result `CD = CpMax/2` based on projected area. This validates the implementation of
+the approximation, not a particular vehicle's flight accuracy.
+
+The formulation follows [NASA normal-shock relations](https://www.grc.nasa.gov/WWW/BGH/normal.html)
+and the modified Newtonian coefficient discussed in
+[NASA TR R-127](https://ntrs.nasa.gov/citations/19630006549).
diff --git a/Sources/Aerodynamics/Aerodynamics.docc/WingsAndBodies.md b/Sources/Aerodynamics/Aerodynamics.docc/WingsAndBodies.md
new file mode 100644
index 0000000..e6eb33b
--- /dev/null
+++ b/Sources/Aerodynamics/Aerodynamics.docc/WingsAndBodies.md
@@ -0,0 +1,117 @@
+# Segmented wings and whole-body loads
+
+Evaluate aerodynamic loads for supplied wing or capsule geometry and coefficient data.
+
+These evaluators remain pure aerodynamic physics. They do not integrate motion,
+assemble vehicles, manage control systems or calculate reentry heating. All body
+vectors use the same caller-selected origin and X-forward/Y-right/Z-down axes.
+
+## Wing strips
+
+``SegmentedWing`` aggregates ``WingSegment`` loads about a supplied moment reference.
+A rectangular helper defaults to eight strips; other counts and arbitrary segment
+geometry are supported. ``WingSectionAxes`` defines the segment's chord/span/down
+basis, allowing twist, dihedral, sweep or a vertical tail orientation through explicit
+orthonormal directions. Positive incidence raises the leading edge.
+
+Each strip samples body-relative-to-air velocity at its own reference location,
+projects that velocity into the chord plane and evaluates its section coefficients.
+This independent-strip approximation discards spanwise velocity: dynamic pressure,
+Mach and Reynolds number use the chord-plane speed. It is not a complete swept-wing
+or finite-wing model.
+
+Positive lift is perpendicular to chord-plane velocity, toward section-up; drag
+opposes that velocity. Positive CM rotates about section +span. Force is `q S C`;
+section moment is `q S chord CM`. The segment position must match the polar's moment
+reference, such as quarter chord. Summation adds the lever-arm moment exactly once.
+See [NASA aerodynamic-center conventions](https://www1.grc.nasa.gov/beginners-guide-to-aeronautics/aerodynamic-center/).
+
+```swift
+import Aerodynamics
+let ambient = try ISAAtmosphere().properties(at: 0)
+let flow = try FluidFlow(relativeVelocityMetresPerSecond: SIMD3(40, 0, 0), properties: ambient)
+// `airfoil` is a caller-supplied AirfoilCoefficientModel with appropriate coverage.
+let wing = try SegmentedWing.rectangular(spanMetres: 8, chordMetres: 2,
+ incidenceRadians: 0.08, model: AirfoilWingSectionModel(airfoil: airfoil))
+let result = try wing.evaluate(flow: flow,
+ angularVelocityRadiansPerSecond: SIMD3(0.1, 0, 0))
+```
+
+The uniform-flow convenience adds `ω×r`, with offsets from an explicit velocity
+reference point. A separate sampler overload accepts local flow for each segment,
+allowing atmosphere gradients, winds and prescribed induced-flow corrections.
+Results include each strip's section flow, coefficients and physical loads as well
+as the total. Zero chord-plane dynamic pressure yields zero loads and nil coefficients
+without querying an undefined incidence/Reynolds number.
+
+``WingSectionCoefficientModel`` receives flow, chord and caller-supplied control
+surface deflection. A calibrated provider may use deflection to select/interpolate
+its aerodynamic data. ``AirfoilWingSectionModel`` adapts existing checked polars;
+it rejects nonzero deflection and missing Mach/Reynolds inputs instead of ignoring
+them. No generic flap effectiveness, stall or wake field is invented. The optional
+ correction supplies equivalent uniform-wing induced angle/drag
+under explicitly bounded conditions; it does not couple arbitrary strips.
+Use a provider and dataset appropriate to the flight regime; this API does not
+extend low-speed airfoil data to hypersonic entry automatically.
+
+## Capsule and fuselage models
+
+``WholeBodyAerodynamics`` consumes ``BodyAerodynamicCoefficientModel`` and reference
+geometry. It uses full freestream dynamic pressure, scales all six body-axis
+coefficients and transfers the resulting moment to the requested point if needed.
+It never adds a second centre-of-pressure moment to a complete coefficient moment.
+
+``BodyAerodynamicQuery`` carries flow, Reynolds reference length, moment reference
+lengths and body angular velocity. The normalized angular rates are
+`(p span, q chord, r span)/(2 V)` when speed is nonzero. A custom provider can use
+these for calibrated damping. No damping is applied by the static table provider.
+
+``TabulatedBodyCoefficients`` linearly interpolates a complete rectangular grid of
+angle of attack, sideslip, Mach and Reynolds conditions. Up to 16 corner coefficients
+contribute to a query. All axes default to rejecting out-of-coverage requests;
+explicit clamping uses their nearest boundary values. A singleton axis covers its
+single value rather than implying independence. Empty, duplicate, malformed or
+incomplete grids are rejected, including during Codable decoding.
+
+``BodyCoefficientTableLoader`` reads the Codable JSON table format from supplied data
+or files; I/O is separate from evaluation. The JSON fields are `samples`,
+`boundaryPolicy`, `source` and `version`. Samples contain `angleOfAttackRadians`,
+`sideslipRadians`, `machNumber`, `reynoldsNumber` and `coefficients`; coefficients
+contain three-element `force` and `moment` arrays. Source/version identify supplied
+data. Geometry dimensions and moment references must match that dataset; the
+caller is responsible for this compatibility.
+
+``WindForceCoefficients`` converts positive drag, signed side force and positive
+lift into body-axis force coefficients using incidence and sideslip. Wind X is along
+the body's relative velocity, wind Y is right and wind Z is down; force components
+in wind axes are `(-CD, CY, -CL)`. Moments are supplied separately in body axes,
+with body-axis moment reference lengths. The conversion convention is consistent
+with [NASA's component/velocity-axis definitions](https://rotorcraft.arc.nasa.gov/Publications/files/NDARCTheory_v1_6_938.pdf).
+
+``ConstantBodyCoefficients`` provides explicitly fixed body-axis coefficients for
+controlled scenarios. It does not represent wind-aligned drag at arbitrary incidence.
+For zero dynamic pressure the whole-body evaluator returns zero loads without
+querying coefficients. A table query with undefined incidence (pure spanwise flow)
+or missing Mach/Reynolds properties fails explicitly.
+
+No capsule-specific flight database is bundled. A lifting or ballistic capsule
+must supply measured, computed or explicitly idealized data and geometry. Heat flux,
+aerodynamic damping, rarefied-flow transitions and hypersonic surface-pressure
+models remain separate workstreams.
+
+## Runnable example and verification
+
+```sh
+swift run FluidPhysicsDemo
+```
+
+The example evaluates an eight-strip wing using Earth sea-level ISA and a lifting
+capsule using ISA at 50 km. Its coefficients are synthetic demonstrations of the
+interfaces, not validated flight or entry predictions.
+
+Tests compare uniform strip loads with analytic `q S C` totals, validate moment
+reference transfers, examine rotational local flow and check midpoint convergence
+against an independently integrated spanwise drag distribution. Body tests use an
+exact affine four-dimensional coefficient field, checked JSON round trips and
+wind-axis transformations. These checks validate implementation conventions;
+vehicle-specific physical accuracy requires independent aerodynamic datasets.
diff --git a/Sources/Aerodynamics/AerothermalHeating.swift b/Sources/Aerodynamics/AerothermalHeating.swift
new file mode 100644
index 0000000..73f842f
--- /dev/null
+++ b/Sources/Aerodynamics/AerothermalHeating.swift
@@ -0,0 +1,153 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// Caller-supplied wall state for correlations which require it. No thermal evolution.
+public struct AerothermalWallState: Sendable {
+ public let temperatureKelvin: Double
+ public init(temperatureKelvin: Double) throws {
+ guard temperatureKelvin.isFinite, temperatureKelvin > 0 else { throw FluidError.invalidParameter }
+ self.temperatureKelvin = temperatureKelvin
+ }
+}
+
+/// Flow at a caller-identified stagnation point of an axisymmetric blunt body.
+/// Gas identifier names the parameter dataset/composition, not an astronomical body.
+/// Richer gas/surface state can be carried by a replacement model's own provider.
+public struct StagnationHeatingQuery: Sendable {
+ public let flow: FluidFlow
+ public let gasIdentifier: String
+ public let noseRadiusMetres: Double
+ public let surfacePositionMetres: SIMD3
+ public let wall: AerothermalWallState?
+ public let gasState: StagnationGasState?
+ public init(flow: FluidFlow, gasIdentifier: String, noseRadiusMetres: Double,
+ surfacePositionMetres: SIMD3, wall: AerothermalWallState? = nil,
+ gasState: StagnationGasState? = nil) throws {
+ guard !gasIdentifier.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty,
+ noseRadiusMetres.isFinite, noseRadiusMetres > 0, fluidFinite(surfacePositionMetres) else {
+ throw FluidError.invalidParameter
+ }
+ self.flow = flow; self.gasIdentifier = gasIdentifier; self.noseRadiusMetres = noseRadiusMetres
+ self.surfacePositionMetres = surfacePositionMetres; self.wall = wall
+ self.gasState = gasState
+ }
+}
+
+/// Incoming convective flux only; wall response and emitted radiation are external.
+public protocol ConvectiveHeatingModel: Sendable {
+ func heatFlux(for query: StagnationHeatingQuery) throws -> SurfaceHeatFlux
+}
+/// Incoming shock-layer radiative flux only. Absence of a model means unknown,
+/// not zero radiation; this interface does not provide a radiative correlation.
+public protocol RadiativeHeatingModel: Sendable {
+ func heatFlux(for query: StagnationHeatingQuery) throws -> SurfaceHeatFlux
+}
+
+/// Parameter k for q = k sqrt(ρ/Rn) V³ with kg/m³, metres, m/s and W/m².
+/// k has SI dimensions kg^0.5/m. Gas and provenance are mandatory.
+public struct SuttonGravesParameters: Sendable {
+ public let gasIdentifier: String
+ public let coefficientSI: Double
+ public let source: String
+ public let version: String
+ public init(gasIdentifier: String, coefficientSI: Double, source: String, version: String) throws {
+ guard [gasIdentifier,source,version].allSatisfy({ !$0.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty }),
+ coefficientSI.isFinite, coefficientSI > 0 else { throw FluidError.invalidParameter }
+ self.gasIdentifier = gasIdentifier; self.coefficientSI = coefficientSI; self.source = source; self.version = version
+ }
+ /// Explicit Earth-air cold-wall approximation from NASA's 2012 TFAWS course.
+ /// Selection does not establish accuracy or coverage for a given trajectory.
+ public static var earthAirColdWall: Self {
+ try! Self(gasIdentifier: "earth-air", coefficientSI: 1.7415e-4,
+ source: "https://tfaws.nasa.gov/TFAWS12/Proceedings/Aerothermodynamics%20Course.pdf",
+ version: "TFAWS 2012")
+ }
+ /// Published cold-wall approximation for a 97% CO₂ / 3% N₂ Mars mixture by mass.
+ public static var marsCarbonDioxideNitrogenColdWall: Self {
+ try! Self(gasIdentifier: "mars-co2-n2-97-3-mass", coefficientSI: 1.83e-4,
+ source: "https://ntrs.nasa.gov/api/citations/20200002354/downloads/20200002354.pdf",
+ version: "West and Brandis 2020, equation 2")
+ }
+}
+
+/// Supplied stagnation pressure and boundary-layer-edge enthalpy for mixture
+/// correlations. Neither is inferred from an ideal-gas atmosphere profile.
+public struct StagnationGasState: Sendable {
+ public let pressurePascals: Double
+ public let edgeSpecificEnthalpyJoulesPerKilogram: Double
+ public init(pressurePascals: Double, edgeSpecificEnthalpyJoulesPerKilogram: Double) throws {
+ guard pressurePascals.isFinite, pressurePascals > 0,
+ edgeSpecificEnthalpyJoulesPerKilogram.isFinite, edgeSpecificEnthalpyJoulesPerKilogram > 0 else {
+ throw FluidError.invalidParameter
+ }
+ self.pressurePascals = pressurePascals
+ self.edgeSpecificEnthalpyJoulesPerKilogram = edgeSpecificEnthalpyJoulesPerKilogram
+ }
+}
+
+/// Caller-declared applicability bounds, not a calibrated accuracy guarantee.
+public struct StagnationHeatingCoverage: Sendable {
+ public let speedMetresPerSecond: ClosedRange
+ public let densityKilogramsPerCubicMetre: ClosedRange
+ public let noseRadiusMetres: ClosedRange
+ public let machNumber: ClosedRange
+ public let maximumKnudsenNumber: Double
+ public init(speedMetresPerSecond: ClosedRange, densityKilogramsPerCubicMetre: ClosedRange,
+ noseRadiusMetres: ClosedRange, machNumber: ClosedRange,
+ maximumKnudsenNumber: Double = 0.01) throws {
+ guard [speedMetresPerSecond,densityKilogramsPerCubicMetre,noseRadiusMetres,machNumber]
+ .allSatisfy({ $0.lowerBound.isFinite && $0.lowerBound > 0 && $0.upperBound.isFinite }),
+ machNumber.lowerBound >= 5, maximumKnudsenNumber.isFinite,
+ maximumKnudsenNumber > 0, maximumKnudsenNumber <= 0.01 else { throw FluidError.invalidParameter }
+ self.speedMetresPerSecond = speedMetresPerSecond; self.densityKilogramsPerCubicMetre = densityKilogramsPerCubicMetre
+ self.noseRadiusMetres = noseRadiusMetres; self.machNumber = machNumber; self.maximumKnudsenNumber = maximumKnudsenNumber
+ }
+}
+
+/// Laminar cold-wall stagnation-point estimate, not a surface heating distribution.
+/// No wall-temperature correction, catalytic-state correction or turbulent multiplier.
+public struct SuttonGravesHeating: ConvectiveHeatingModel {
+ public let parameters: SuttonGravesParameters
+ public let coverage: StagnationHeatingCoverage
+ public init(parameters: SuttonGravesParameters, coverage: StagnationHeatingCoverage) {
+ self.parameters = parameters; self.coverage = coverage
+ }
+ public func heatFlux(for query: StagnationHeatingQuery) throws -> SurfaceHeatFlux {
+ guard query.gasIdentifier == parameters.gasIdentifier else { throw FluidError.unsupportedQuery }
+ // A supplied finite-temperature wall needs a different correlation.
+ guard query.wall == nil else { throw FluidError.unsupportedQuery }
+ let flow = query.flow
+ guard coverage.noseRadiusMetres.contains(query.noseRadiusMetres) else { throw FluidError.outsideCoverage }
+ if flow.speedMetresPerSecond == 0 {
+ return try SurfaceHeatFlux(wattsPerSquareMetre: 0, surfacePositionMetres: query.surfacePositionMetres)
+ }
+ guard let mach = flow.machNumber,
+ let kn = try flow.knudsenNumber(referenceLengthMetres: query.noseRadiusMetres) else {
+ throw FluidError.missingFlowProperty
+ }
+ guard coverage.speedMetresPerSecond.contains(flow.speedMetresPerSecond),
+ coverage.densityKilogramsPerCubicMetre.contains(flow.densityKilogramsPerCubicMetre),
+ coverage.machNumber.contains(mach), kn <= coverage.maximumKnudsenNumber else { throw FluidError.outsideCoverage }
+ let v = flow.speedMetresPerSecond
+ let flux = ((parameters.coefficientSI*sqrt(flow.densityKilogramsPerCubicMetre)/sqrt(query.noseRadiusMetres))*v)*v*v
+ guard flux.isFinite else { throw FluidError.nonFiniteResult }
+ return try SurfaceHeatFlux(wattsPerSquareMetre: flux, surfacePositionMetres: query.surfacePositionMetres)
+ }
+}
diff --git a/Sources/Aerodynamics/Airfoil.swift b/Sources/Aerodynamics/Airfoil.swift
index 5d6ca26..e03ef74 100644
--- a/Sources/Aerodynamics/Airfoil.swift
+++ b/Sources/Aerodynamics/Airfoil.swift
@@ -16,6 +16,7 @@
// limitations under the License.
//
+import FluidDynamics
import Foundation
import Yams
@@ -26,133 +27,78 @@ public protocol Airfoil {
func coefficients(at alpha: Double, for reynoldsNumber: Double) -> AirfoilCoefficients
}
-public struct AirfoilCoefficients : Codable {
+public struct AirfoilCoefficients: Codable, Sendable {
public let lift: Double
public let drag: Double
public let moment: Double
+ public init(lift: Double, drag: Double, moment: Double) {
+ self.lift = lift; self.drag = drag; self.moment = moment
+ }
+ internal var isFinite: Bool { [lift,drag,moment].allSatisfy(\.isFinite) }
}
-public struct ParametricAirfoil : Airfoil, Codable {
- let reynoldsNumber: Double
- let coefficients: [AirfoilCoefficients]
+/// Legacy scalar facade. Queries use radians and explicitly clamp to the loaded
+/// angle/Reynolds/Mach coverage with a Mach-zero query. Invalid queries return NaN; prefer the
+/// throwing TabulatedAirfoil API for coverage-sensitive physics.
+public struct ParametricAirfoil: Airfoil, Codable, Sendable {
+ private let model: TabulatedAirfoil
+ private init(model: TabulatedAirfoil) { self.model = model }
+ /// Coefficients at one-degree intervals from −180° through +180°, inclusive.
+ /// Use validatingReynoldsNumber for recoverable validation errors.
public init(reynoldsNumber: Double, coefficients: [AirfoilCoefficients]) {
- self.reynoldsNumber = reynoldsNumber
- self.coefficients = coefficients
+ do { try self.init(validatingReynoldsNumber: reynoldsNumber, coefficients: coefficients) }
+ catch { preconditionFailure("Invalid coefficient table: \(error)") }
}
- public init?(withString string: String) {
- guard let foil = try? Yams.load(yaml: string) as? [String: Any] else {
- print("Yams load failed")
- return nil
- }
-
- //guard let name = foil["name"] as? String else {
- // print("no name")
- // return nil
- //}
- //guard let generator = foil["generated-with"] as? String else {
- // print("Generated with missing")
- // return nil
- //}
- guard let foilData = foil["data"] as? [[String : Any]] else {
- print("Data missing")
- return nil
- }
- let foilDataEntry = foilData[0]
-
- guard let reynoldsNumber = foilDataEntry["reynolds-number"] as? Double else {
- return nil
- }
-
- guard let coefficientsInFile = foilDataEntry["coefficients"] as? [[Double]] else {
- return nil
- }
-
- var coefficients = [AirfoilCoefficients]()
-
- guard let firstCoeef = coefficientsInFile.first else {
- return nil
- }
-
- var preFill = -181.0
- while preFill < firstCoeef[0] {
- coefficients.append(AirfoilCoefficients(lift: firstCoeef[1],
- drag: firstCoeef[2],
- moment: firstCoeef[4]))
- preFill += 1.0
- }
- for coef in coefficientsInFile {
- coefficients.append(AirfoilCoefficients(lift: coef[1], drag: coef[2], moment: coef[4]))
- }
-
- guard let lastCoef = coefficientsInFile.last else {
- return nil
- }
- var postFill = lastCoef[0] + 1
- while postFill < 181.0 {
- coefficients.append(AirfoilCoefficients(lift: lastCoef[1],
- drag: lastCoef[2],
- moment: lastCoef[4]))
- postFill += 1.0
+ public init(validatingReynoldsNumber reynoldsNumber: Double, coefficients: [AirfoilCoefficients]) throws {
+ guard coefficients.count == 361 else { throw FluidError.invalidCoefficients }
+ let samples = coefficients.enumerated().map {
+ AirfoilSample(angleOfAttackRadians: Double($0.offset-180) * .pi/180, coefficients: $0.element)
}
+ model = try TabulatedAirfoil(polars: [AirfoilPolar(reynoldsNumber: reynoldsNumber,samples: samples)],
+ boundaryPolicy: .clamp,source: "Caller-supplied degree grid",version: "1")
+ }
- self.reynoldsNumber = reynoldsNumber
- self.coefficients = coefficients
+ public init?(withString string: String) {
+ guard let parsed = try? AirfoilTableLoader.yaml(string,boundaryPolicy: .clamp) else { return nil }
+ model = parsed
}
public init?(withFile file: String) {
- guard let data = try? String(contentsOfFile: file) else {
- return nil
- }
-
- self.init(withString: data)
+ guard let parsed = try? AirfoilTableLoader.yamlFile(URL(fileURLWithPath: file),boundaryPolicy: .clamp) else { return nil }
+ model = parsed
}
-
public func liftCoefficient(at alpha: Double, for reynoldsNumber: Double) -> Double {
- let alphaDeg = alpha * 180 / .pi
- let alphaInt = Int(alphaDeg)
- assert(abs(alphaInt) <= 180)
- let c0 = coefficients[alphaInt + 180]
- let sub = alphaInt < 0
- let c1 = coefficients[alphaInt + 180 + (sub ? -1 : 1)]
- let fraction = fmod(alpha, 1.0)
- return c0.lift * fraction + c1.lift * (1-fraction)
+ return coefficients(at: alpha,for: reynoldsNumber).lift
}
public func dragCoefficient(at alpha: Double, for reynoldsNumber: Double) -> Double {
- let alphaDeg = alpha * 180 / .pi
- let alphaInt = Int(alphaDeg)
- assert(abs(alphaInt) <= 180)
- let c0 = coefficients[alphaInt + 180]
- let sub = alphaInt < 0
- let c1 = coefficients[alphaInt + 180 + (sub ? -1 : 1)]
- let fraction = fmod(alpha, 1.0)
- return c0.drag * fraction + c1.drag * (1-fraction)
+ return coefficients(at: alpha,for: reynoldsNumber).drag
}
public func momentCoefficient(at alpha: Double, for reynoldsNumber: Double) -> Double {
- let alphaDeg = alpha * 180 / .pi
- let alphaInt = Int(alphaDeg)
- assert(abs(alphaInt) <= 180)
- let c0 = coefficients[alphaInt + 180]
- let sub = alphaInt < 0
- let c1 = coefficients[alphaInt + 180 + (sub ? -1 : 1)]
- let fraction = fmod(alpha, 1.0)
- return c0.moment * fraction + c1.moment * (1-fraction)
+ return coefficients(at: alpha,for: reynoldsNumber).moment
+ }
+ public func coefficients(at alpha: Double, for reynoldsNumber: Double) -> AirfoilCoefficients {
+ guard alpha.isFinite, abs(alpha) <= .pi else {
+ return AirfoilCoefficients(lift: .nan,drag: .nan,moment: .nan)
+ }
+ return (try? model.coefficients(angleOfAttackRadians: alpha,reynoldsNumber: reynoldsNumber,machNumber: 0))
+ ?? AirfoilCoefficients(lift: .nan,drag: .nan,moment: .nan)
}
- public func coefficients(at alpha: Double, for reynoldsNumber: Double) -> AirfoilCoefficients
- {
- let alphaDeg = alpha * 180 / .pi
- let alphaInt = Int(alphaDeg)
- assert(abs(alphaInt) <= 180)
- let c0 = coefficients[alphaInt + 181]
- let sub = alphaInt < 0
- let c1 = coefficients[alphaInt + 181 + (sub ? -1 : 1)]
- let fraction = fmod(alpha, 1.0)
- let resultingCoefficient = AirfoilCoefficients(
- lift: c0.lift * fraction + c1.lift * (1-fraction),
- drag: c0.drag * fraction + c1.drag * (1-fraction),
- moment: c0.moment * fraction + c1.moment * (1-fraction))
- return resultingCoefficient
+ private enum CodingKeys: String, CodingKey { case model, reynoldsNumber, coefficients }
+ public init(from decoder: Decoder) throws {
+ let c = try decoder.container(keyedBy: CodingKeys.self)
+ if c.contains(.model) { try self.init(model: c.decode(TabulatedAirfoil.self,forKey: .model)) }
+ else {
+ var values = try c.decode([AirfoilCoefficients].self,forKey: .coefficients)
+ // The original YAML loader added an unused −181° padding sample.
+ if values.count == 362 { values.removeFirst() }
+ try self.init(validatingReynoldsNumber: c.decode(Double.self,forKey: .reynoldsNumber),coefficients: values)
+ }
+ }
+ public func encode(to encoder: Encoder) throws {
+ var c = encoder.container(keyedBy: CodingKeys.self)
+ try c.encode(model,forKey: .model)
}
}
diff --git a/Sources/Aerodynamics/AirfoilTables.swift b/Sources/Aerodynamics/AirfoilTables.swift
new file mode 100644
index 0000000..f82bb7d
--- /dev/null
+++ b/Sources/Aerodynamics/AirfoilTables.swift
@@ -0,0 +1,183 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+import Yams
+
+/// Explicit boundary behavior; no automatic physical extrapolation beyond measured samples.
+public enum CoefficientBoundaryPolicy: String, Codable, Sendable { case reject, clamp }
+
+/// One measured/computed angle sample. Angles are radians and moment reference is dataset-defined.
+public struct AirfoilSample: Sendable, Codable {
+ public let angleOfAttackRadians: Double
+ public let coefficients: AirfoilCoefficients
+ public init(angleOfAttackRadians: Double, coefficients: AirfoilCoefficients) {
+ self.angleOfAttackRadians = angleOfAttackRadians; self.coefficients = coefficients
+ }
+}
+
+/// Validated section polar at one Reynolds/Mach condition, preserving irregular angle spacing.
+public struct AirfoilPolar: Sendable, Codable {
+ public let reynoldsNumber: Double
+ public let machNumber: Double
+ public let samples: [AirfoilSample]
+ public var angleRangeRadians: ClosedRange { samples.first!.angleOfAttackRadians...samples.last!.angleOfAttackRadians }
+ public init(reynoldsNumber: Double, machNumber: Double = 0, samples: [AirfoilSample]) throws {
+ guard reynoldsNumber.isFinite, reynoldsNumber > 0, machNumber.isFinite, machNumber >= 0,
+ !samples.isEmpty, samples.allSatisfy({ $0.angleOfAttackRadians.isFinite && abs($0.angleOfAttackRadians) <= .pi && $0.coefficients.isFinite }),
+ zip(samples,samples.dropFirst()).allSatisfy({ $0.angleOfAttackRadians < $1.angleOfAttackRadians }) else {
+ throw FluidError.invalidCoefficients
+ }
+ self.reynoldsNumber = reynoldsNumber; self.machNumber = machNumber; self.samples = samples
+ }
+ public func coefficients(at angle: Double, boundaryPolicy: CoefficientBoundaryPolicy = .reject) throws -> AirfoilCoefficients {
+ let a = try boundedCoefficientCoordinate(angle, range: angleRangeRadians, policy: boundaryPolicy)
+ let lower = samples.lastIndex(where: { $0.angleOfAttackRadians <= a })!
+ guard lower+1 < samples.count else { return samples[lower].coefficients }
+ let first = samples[lower], next = samples[lower+1]
+ let weight = (a-first.angleOfAttackRadians)/(next.angleOfAttackRadians-first.angleOfAttackRadians)
+ return try blendCoefficients(first.coefficients,next.coefficients,weight: weight)
+ }
+ private enum CodingKeys: String, CodingKey { case reynoldsNumber, machNumber, samples }
+ public init(from decoder: Decoder) throws {
+ let c = try decoder.container(keyedBy: CodingKeys.self)
+ try self.init(reynoldsNumber: c.decode(Double.self,forKey: .reynoldsNumber),
+ machNumber: c.decode(Double.self,forKey: .machNumber),samples: c.decode([AirfoilSample].self,forKey: .samples))
+ }
+}
+
+/// Checked section model interface, independent of motion integration and vehicle systems.
+public protocol AirfoilCoefficientModel: Sendable {
+ func coefficients(angleOfAttackRadians: Double, reynoldsNumber: Double, machNumber: Double) throws -> AirfoilCoefficients
+}
+
+/// Rectangular Reynolds/Mach grid of polars, with linear interpolation in each coordinate.
+/// Angle grids may differ; all contributing polars must cover a query unless clamping is selected.
+public struct TabulatedAirfoil: AirfoilCoefficientModel, Sendable, Codable {
+ public let polars: [AirfoilPolar]
+ public let boundaryPolicy: CoefficientBoundaryPolicy
+ public let source: String
+ public let version: String
+ private let reynoldsGrid: [Double]
+ private let machGrid: [Double]
+ private let grid: [AirfoilPolar]
+ public init(polars: [AirfoilPolar], boundaryPolicy: CoefficientBoundaryPolicy = .reject,
+ source: String, version: String) throws {
+ guard !polars.isEmpty, !source.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty,
+ !version.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty else { throw FluidError.invalidParameter }
+ let re = Array(Set(polars.map(\.reynoldsNumber))).sorted(), ma = Array(Set(polars.map(\.machNumber))).sorted()
+ var ordered = [AirfoilPolar]()
+ for m in ma {
+ for r in re {
+ let matching = polars.filter { $0.reynoldsNumber == r && $0.machNumber == m }
+ guard matching.count <= 1 else { throw FluidError.duplicateCondition }
+ guard let polar = matching.first else { throw FluidError.incompleteGrid }
+ ordered.append(polar)
+ }
+ }
+ self.polars = polars; self.boundaryPolicy = boundaryPolicy; self.source = source; self.version = version
+ reynoldsGrid = re; machGrid = ma; grid = ordered
+ }
+ public func coefficients(angleOfAttackRadians: Double, reynoldsNumber: Double, machNumber: Double) throws -> AirfoilCoefficients {
+ guard reynoldsNumber.isFinite, reynoldsNumber > 0, machNumber.isFinite, machNumber >= 0 else {
+ throw FluidError.invalidParameter
+ }
+ let re = try bracket(reynoldsNumber,grid: reynoldsGrid), ma = try bracket(machNumber,grid: machGrid)
+ func evaluate(_ r: Int, _ m: Int) throws -> AirfoilCoefficients {
+ try grid[m*reynoldsGrid.count+r].coefficients(at: angleOfAttackRadians,boundaryPolicy: boundaryPolicy)
+ }
+ func atMach(_ m: Int) throws -> AirfoilCoefficients {
+ let first = try evaluate(re.0,m)
+ guard re.0 != re.1 else { return first }
+ return try blendCoefficients(first,evaluate(re.1,m),weight: re.2)
+ }
+ let first = try atMach(ma.0)
+ guard ma.0 != ma.1 else { return first }
+ return try blendCoefficients(first,atMach(ma.1),weight: ma.2)
+ }
+ private func bracket(_ value: Double, grid: [Double]) throws -> (Int,Int,Double) {
+ let v = try boundedCoefficientCoordinate(value,range: grid.first!...grid.last!,policy: boundaryPolicy)
+ let lower = grid.lastIndex(where: { $0 <= v })!
+ guard lower+1 < grid.count, v != grid[lower] else { return (lower,lower,0) }
+ return (lower,lower+1,(v-grid[lower])/(grid[lower+1]-grid[lower]))
+ }
+ private enum CodingKeys: String, CodingKey { case polars, boundaryPolicy, source, version }
+ public init(from decoder: Decoder) throws {
+ let c = try decoder.container(keyedBy: CodingKeys.self)
+ try self.init(polars: c.decode([AirfoilPolar].self,forKey: .polars),
+ boundaryPolicy: c.decode(CoefficientBoundaryPolicy.self,forKey: .boundaryPolicy),
+ source: c.decode(String.self,forKey: .source),version: c.decode(String.self,forKey: .version))
+ }
+ public func encode(to encoder: Encoder) throws {
+ var c = encoder.container(keyedBy: CodingKeys.self)
+ try c.encode(polars,forKey: .polars); try c.encode(boundaryPolicy,forKey: .boundaryPolicy)
+ try c.encode(source,forKey: .source); try c.encode(version,forKey: .version)
+ }
+}
+
+/// Loader for the existing XFOIL-style YAML: degrees, CL, CD, CDp, CM.
+/// Every `data` entry is retained, with optional `mach-number` (default zero).
+public enum AirfoilTableLoader {
+ public static func yaml(_ text: String, boundaryPolicy: CoefficientBoundaryPolicy = .reject,
+ source: String = "Caller-supplied airfoil YAML", version: String = "1") throws -> TabulatedAirfoil {
+ let file: YAMLAirfoilFile
+ do { file = try YAMLDecoder().decode(YAMLAirfoilFile.self,from: text) }
+ catch { throw FluidError.malformedData }
+ guard !file.data.isEmpty else { throw FluidError.malformedData }
+ var polars = [AirfoilPolar]()
+ for entry in file.data {
+ let re = entry.reynoldsNumber, mach = entry.machNumber ?? 0, rows = entry.coefficients
+ guard !rows.isEmpty else { throw FluidError.malformedData }
+ var samples = [AirfoilSample]()
+ for row in rows {
+ guard row.count == 5, row.allSatisfy(\.isFinite), (-180.0...180.0).contains(row[0]) else {
+ throw FluidError.malformedData
+ }
+ samples.append(AirfoilSample(angleOfAttackRadians: row[0] * .pi/180,
+ coefficients: AirfoilCoefficients(lift: row[1],drag: row[2],moment: row[4])))
+ }
+ polars.append(try AirfoilPolar(reynoldsNumber: re,machNumber: mach,samples: samples))
+ }
+ return try TabulatedAirfoil(polars: polars,boundaryPolicy: boundaryPolicy,source: source,version: version)
+ }
+ public static func yamlFile(_ url: URL, boundaryPolicy: CoefficientBoundaryPolicy = .reject) throws -> TabulatedAirfoil {
+ try yaml(String(contentsOf: url,encoding: .utf8),boundaryPolicy: boundaryPolicy,source: url.absoluteString)
+ }
+}
+
+internal func boundedCoefficientCoordinate(_ value: Double, range: ClosedRange, policy: CoefficientBoundaryPolicy) throws -> Double {
+ guard value.isFinite else { throw FluidError.invalidParameter }
+ guard policy == .clamp || range.contains(value) else { throw FluidError.outsideCoverage }
+ return min(range.upperBound,max(range.lowerBound,value))
+}
+internal func blendCoefficients(_ first: AirfoilCoefficients, _ last: AirfoilCoefficients, weight: Double) throws -> AirfoilCoefficients {
+ let result = AirfoilCoefficients(lift: first.lift*(1-weight)+last.lift*weight,
+ drag: first.drag*(1-weight)+last.drag*weight,moment: first.moment*(1-weight)+last.moment*weight)
+ guard result.isFinite else { throw FluidError.nonFiniteResult }
+ return result
+}
+
+private struct YAMLAirfoilFile: Decodable { let data: [YAMLAirfoilEntry] }
+private struct YAMLAirfoilEntry: Decodable {
+ let reynoldsNumber: Double
+ let machNumber: Double?
+ let coefficients: [[Double]]
+ private enum CodingKeys: String, CodingKey {
+ case reynoldsNumber = "reynolds-number", machNumber = "mach-number", coefficients
+ }
+}
diff --git a/Sources/Aerodynamics/Atmosphere.swift b/Sources/Aerodynamics/Atmosphere.swift
deleted file mode 100644
index 184dcea..0000000
--- a/Sources/Aerodynamics/Atmosphere.swift
+++ /dev/null
@@ -1,124 +0,0 @@
-//
-// SPDX-License-Identifier: Apache-2.0
-//
-// Copyright 2023 Mattias Holm
-//
-// Licensed under the Apache License, Version 2.0 (the "License");
-// you may not use this file except in compliance with the License.
-// You may obtain a copy of the License at
-//
-// http://www.apache.org/licenses/LICENSE-2.0
-//
-// Unless required by applicable law or agreed to in writing, software
-// distributed under the License is distributed on an "AS IS" BASIS,
-// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
-// See the License for the specific language governing permissions and
-// limitations under the License.
-//
-import Foundation
-
-public protocol Atmosphere {
- func pressure(at altitude: Double) -> Double
- func temperature(at altitude: Double) -> Double
- func density(at altitude: Double) -> Double
- func speedOfSound(at altitude: Double) -> Double
- func dynamicViscosity(at altitude: Double) -> Double
-}
-
-public extension Atmosphere {
- func kinematicViscosity(at altitude: Double) -> Double {
- return dynamicViscosity(at: altitude)/density(at: altitude)
- }
-}
-
-public struct EarthAtmosphere: Atmosphere {
- // Very simplified model from:
- // https://www.grc.nasa.gov/www/k-12/airplane/atmosmet.html
- public init() {
-
- }
- public func density(at altitude: Double) -> Double {
- //let hc = altitude
- let h = altitude
- //let h = hc - 6371.0e3 // Distance from surface
- let T = temperature(at: h)
-
- if h < 11000 { // Troposphere
- let p = 101.29 * pow(((T + 273.1) / 288.08), 5.256)
- return p
- } else if h < 25000 { // Lower stratosphere
- let p = 22.65 * exp(1.73 - 0.000157 * h)
- return p
- } else { // Upper stratosphere
- let p = 2.488 * pow((T + 273.1)/216.6, -11.388)
- return p
- }
- }
-
- public func pressure(at altitude: Double) -> Double {
- let p = density(at: altitude)
- let T = temperature(at: altitude)
- let pressure = p / (0.2869 * (T + 273.1))
- return pressure
- }
- public func temperature(at altitude: Double) -> Double {
- //let hc = altitude
- //let h = hc - 6371.0e3 // Distance from surface
- let h = altitude
- if h < 11000 { // Troposphere
- let T = 15.04 - 0.00649 * h
- return T
- } else if h < 25000 { // Lower stratosphere
- let T = -56.46
- return T
- } else { // Upper stratosphere
- let T = -131.21 + 0.00299 * h
- return T
- }
- }
-
- public func speedOfSound(at altitude: Double) -> Double {
- let adibiaticIndex = 1.4
- return sqrt(adibiaticIndex * pressure(at: altitude) / density(at: altitude))
- }
- public func dynamicViscosity(at altitude: Double) -> Double {
- // Tables from https://www.engineeringtoolbox.com/standard-atmosphere-d_604.html
- // -1k to 10k, 1k steps
- let dynamicViscosityTable10k = [
- 1.821, 1.789, 1.758, 1.726, 1.694, 1.661, 1.628, 1.595, 1.561, 1.527,
- 1.493, 1.458]
- // 10k to 30k, 5k steps
- let dynamicViscosityTable30k = [1.458, 1.422, 1.422, 1.448, 1.475]
-
- // 30k to 80k, 10 steps
- let dynamicViscosityTable80k = [1.475, 1.601, 1.704, 1.584, 1.438, 1.321]
-
- if altitude < 10000 {
- let index = Int(altitude + 1000) / 1000
- let weight = fmod(altitude + 1000, 1000) / 1000
- return dynamicViscosityTable10k[index] * (1 - weight) +
- dynamicViscosityTable10k[index + 1] * (weight)
- } else if altitude < 30000 {
- let index = Int(altitude - 10000) / 5000
- let weight = fmod(altitude - 10000, 5000) / 5000
- return dynamicViscosityTable30k[index] * (1 - weight) +
- dynamicViscosityTable30k[index + 1] * weight
-
- } else if altitude < 80000 {
- let index = Int(altitude - 30000) / 10000
- let weight = fmod(altitude - 30000, 10000) / 10000
- return dynamicViscosityTable80k[index] * (1 - weight) +
- dynamicViscosityTable80k[index + 1] * weight
-
- }
-
- return 0.0
- }
-}
-
-extension Atmosphere {
- func reynoldsNumber(at altitude: Double, forLength length: Double, atVelocity velocity: Double) -> Double {
- // Re = density * velocity * length / viscosity
- return self.density(at: altitude) * velocity * length / self.dynamicViscosity(at: altitude)
- }
-}
diff --git a/Sources/Aerodynamics/AtmosphericFlow.swift b/Sources/Aerodynamics/AtmosphericFlow.swift
new file mode 100644
index 0000000..9c8bac7
--- /dev/null
+++ b/Sources/Aerodynamics/AtmosphericFlow.swift
@@ -0,0 +1,30 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Atmospheres
+
+public extension FluidFlow {
+ init(relativeVelocityMetresPerSecond: SIMD3, properties: AtmosphericProperties,
+ meanFreePathMetres: Double? = nil) throws {
+ try self.init(relativeVelocityMetresPerSecond: relativeVelocityMetresPerSecond,
+ densityKilogramsPerCubicMetre: properties.densityKilogramsPerCubicMetre,
+ pressurePascals: properties.pressurePascals,temperatureKelvin: properties.temperatureKelvin,
+ speedOfSoundMetresPerSecond: properties.speedOfSoundMetresPerSecond,
+ dynamicViscosityPascalSeconds: properties.dynamicViscosityPascalSeconds,meanFreePathMetres: meanFreePathMetres)
+ }
+}
diff --git a/Sources/Aerodynamics/BalloonAerodynamics.swift b/Sources/Aerodynamics/BalloonAerodynamics.swift
new file mode 100644
index 0000000..e7f3903
--- /dev/null
+++ b/Sources/Aerodynamics/BalloonAerodynamics.swift
@@ -0,0 +1,35 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+/// Combine displaced-volume buoyancy and optional supplied-shape drag exactly once.
+/// Weight of envelope, lifting gas and payload is handled by external mass/gravity.
+public struct BalloonAerodynamics: Sendable {
+ public let buoyancy: Buoyancy
+ public let drag: DragAreaForces?
+ public init(buoyancy: Buoyancy, drag: DragAreaForces? = nil) {
+ self.buoyancy = buoyancy; self.drag = drag
+ }
+ public func evaluate(flow: FluidFlow, field: BuoyancyField,
+ momentReferencePointMetres: SIMD3 = .zero) throws -> FluidLoads {
+ let pressureLoads = try buoyancy.evaluate(densityKilogramsPerCubicMetre: flow.densityKilogramsPerCubicMetre,
+ field: field, momentReferencePointMetres: momentReferencePointMetres)
+ guard let drag else { return pressureLoads }
+ return try pressureLoads.adding(drag.evaluate(flow: flow, momentReferencePointMetres: momentReferencePointMetres))
+ }
+}
diff --git a/Sources/Aerodynamics/BodyAerodynamics.swift b/Sources/Aerodynamics/BodyAerodynamics.swift
new file mode 100644
index 0000000..4a8b172
--- /dev/null
+++ b/Sources/Aerodynamics/BodyAerodynamics.swift
@@ -0,0 +1,219 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// Rates must match the convention used to identify the coefficient derivatives.
+public enum BodyAerodynamicRateReference: Sendable, Equatable {
+ case inertialReference
+ case rigidlyRotatingMedium
+}
+
+/// Whole-body inputs in X-forward/Y-right/Z-down axes. Angular rates are carried
+/// for providers with calibrated damping; no damping coefficient is invented.
+public struct BodyAerodynamicQuery: Sendable {
+ public let flow: FluidFlow
+ public let reynoldsReferenceLengthMetres: Double
+ public let momentLengthsMetres: SIMD3
+ public let angularVelocityRadiansPerSecond: SIMD3
+ public let angularRateReference: BodyAerodynamicRateReference
+ public var angleOfAttackRadians: Double? { flow.angleOfAttackRadians }
+ public var sideslipRadians: Double? { flow.sideslipRadians }
+ public var machNumber: Double? { flow.machNumber }
+ public func reynoldsNumber() throws -> Double? { try flow.reynoldsNumber(referenceLengthMetres: reynoldsReferenceLengthMetres) }
+ public var nondimensionalAngularRates: SIMD3? {
+ guard flow.speedMetresPerSecond > 0 else { return nil }
+ return ((angularVelocityRadiansPerSecond*momentLengthsMetres)/flow.speedMetresPerSecond)*0.5
+ }
+ public init(flow: FluidFlow, reynoldsReferenceLengthMetres: Double,
+ momentLengthsMetres: SIMD3, angularVelocityRadiansPerSecond: SIMD3 = .zero,
+ angularRateReference: BodyAerodynamicRateReference = .inertialReference) throws {
+ guard reynoldsReferenceLengthMetres.isFinite, reynoldsReferenceLengthMetres > 0,
+ [momentLengthsMetres.x,momentLengthsMetres.y,momentLengthsMetres.z].allSatisfy({ $0.isFinite && $0 > 0 }),
+ fluidFinite(angularVelocityRadiansPerSecond) else { throw FluidError.invalidParameter }
+ self.flow = flow; self.reynoldsReferenceLengthMetres = reynoldsReferenceLengthMetres
+ self.momentLengthsMetres = momentLengthsMetres; self.angularVelocityRadiansPerSecond = angularVelocityRadiansPerSecond
+ self.angularRateReference = angularRateReference
+ guard nondimensionalAngularRates.map(fluidFinite) ?? true else { throw FluidError.nonFiniteResult }
+ }
+}
+public protocol BodyAerodynamicCoefficientModel: Sendable {
+ var source: String { get }
+ var version: String { get }
+ /// Six coefficients in body axes, with moments about the supplied geometry's
+ /// reference point. Dataset dimensions must match that geometry.
+ func coefficients(for query: BodyAerodynamicQuery) throws -> FluidCoefficients
+}
+
+/// Prescribed coefficients for controlled scenarios; no capsule geometry or
+/// scientific validity is implied. Coefficients are fixed in body axes, not wind axes.
+public struct ConstantBodyCoefficients: BodyAerodynamicCoefficientModel {
+ public let value: FluidCoefficients
+ public let source: String
+ public let version: String
+ public init(value: FluidCoefficients, source: String, version: String) throws {
+ guard !source.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty,
+ !version.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty else { throw FluidError.invalidParameter }
+ self.value = value; self.source = source; self.version = version
+ }
+ public func coefficients(for query: BodyAerodynamicQuery) throws -> FluidCoefficients { value }
+}
+
+/// Wind axes X along body-relative-to-air velocity, Y to wind-right, Z wind-down.
+/// Converts drag, side force and lift into signed body force coefficients.
+/// Moments remain separate body-axis coefficients supplied by the dataset.
+public struct WindForceCoefficients: Sendable {
+ public let drag: Double
+ public let side: Double
+ public let lift: Double
+ public init(drag: Double, side: Double = 0, lift: Double) throws {
+ guard [drag,side,lift].allSatisfy(\.isFinite), drag >= 0 else { throw FluidError.invalidCoefficients }
+ self.drag = drag; self.side = side; self.lift = lift
+ }
+ public func bodyCoefficients(angleOfAttackRadians alpha: Double, sideslipRadians beta: Double,
+ momentBody: SIMD3 = .zero) throws -> FluidCoefficients {
+ guard alpha.isFinite, beta.isFinite, abs(alpha) <= .pi, abs(beta) <= .pi/2 else { throw FluidError.invalidParameter }
+ let ca = cos(alpha), sa = sin(alpha), cb = cos(beta), sb = sin(beta)
+ let x = SIMD3(ca*cb,sb,sa*cb), y = SIMD3(-ca*sb,cb,-sa*sb), z = SIMD3(-sa,0,ca)
+ return try FluidCoefficients(force: -drag*x+side*y-lift*z,moment: momentBody)
+ }
+}
+
+/// Generic capsule/fuselage/whole-body evaluator driven by a supplied coefficient
+/// model. No automatic model selection, heating, deployment or motion integration.
+public struct WholeBodyAerodynamics: Sendable {
+ public let geometry: FluidReferenceGeometry
+ public let reynoldsReferenceLengthMetres: Double
+ public let model: any BodyAerodynamicCoefficientModel
+ public init(geometry: FluidReferenceGeometry, reynoldsReferenceLengthMetres: Double,
+ model: any BodyAerodynamicCoefficientModel) throws {
+ guard reynoldsReferenceLengthMetres.isFinite, reynoldsReferenceLengthMetres > 0 else { throw FluidError.invalidGeometry }
+ self.geometry = geometry; self.reynoldsReferenceLengthMetres = reynoldsReferenceLengthMetres; self.model = model
+ }
+ public func evaluate(flow: FluidFlow, angularVelocityRadiansPerSecond: SIMD3 = .zero,
+ angularRateReference: BodyAerodynamicRateReference = .inertialReference,
+ momentReferencePointMetres: SIMD3? = nil) throws -> FluidLoads {
+ let query = try BodyAerodynamicQuery(flow: flow,reynoldsReferenceLengthMetres: reynoldsReferenceLengthMetres,
+ momentLengthsMetres: geometry.momentLengthsMetres,angularVelocityRadiansPerSecond: angularVelocityRadiansPerSecond,
+ angularRateReference: angularRateReference)
+ let loads: FluidLoads
+ if flow.dynamicPressurePascals == 0 {
+ loads = try FluidLoads(forceNewtons: .zero,momentNewtonMetres: .zero,
+ referencePointMetres: geometry.momentReferencePointMetres)
+ } else {
+ loads = try model.coefficients(for: query).loads(dynamicPressurePascals: flow.dynamicPressurePascals,geometry: geometry)
+ }
+ return try momentReferencePointMetres.map { try loads.referred(to: $0) } ?? loads
+ }
+}
+
+/// One whole-body coefficient sample. Conditions use radians and dimensionless Mach/Reynolds.
+public struct BodyCoefficientSample: Sendable, Codable {
+ public let angleOfAttackRadians: Double
+ public let sideslipRadians: Double
+ public let machNumber: Double
+ public let reynoldsNumber: Double
+ public let coefficients: FluidCoefficients
+ public init(angleOfAttackRadians: Double, sideslipRadians: Double, machNumber: Double,
+ reynoldsNumber: Double, coefficients: FluidCoefficients) {
+ self.angleOfAttackRadians = angleOfAttackRadians; self.sideslipRadians = sideslipRadians
+ self.machNumber = machNumber; self.reynoldsNumber = reynoldsNumber; self.coefficients = coefficients
+ }
+}
+
+/// Validated rectangular incidence/sideslip/Mach/Reynolds grid, linearly interpolated
+/// across up to 16 corners. Static coefficients: supplied angular rates are not used.
+public struct TabulatedBodyCoefficients: BodyAerodynamicCoefficientModel, Sendable, Codable {
+ public let samples: [BodyCoefficientSample]
+ public let boundaryPolicy: CoefficientBoundaryPolicy
+ public let source: String
+ public let version: String
+ private let axes: [[Double]]
+ private let values: [[Double]: FluidCoefficients]
+ public init(samples: [BodyCoefficientSample], boundaryPolicy: CoefficientBoundaryPolicy = .reject,
+ source: String, version: String) throws {
+ guard !samples.isEmpty, !source.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty,
+ !version.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty else { throw FluidError.invalidParameter }
+ var records: [[Double]: FluidCoefficients] = [:]
+ for sample in samples {
+ let key = [sample.angleOfAttackRadians,sample.sideslipRadians,sample.machNumber,sample.reynoldsNumber]
+ guard key.allSatisfy(\.isFinite), abs(key[0]) <= .pi, abs(key[1]) <= .pi/2,
+ key[2] >= 0, key[3] > 0 else { throw FluidError.invalidCoefficients }
+ guard records[key] == nil else { throw FluidError.duplicateCondition }
+ records[key] = sample.coefficients
+ }
+ let grids = (0..<4).map { coordinate in Array(Set(records.keys.map { $0[coordinate] })).sorted() }
+ var expected = 1
+ for grid in grids {
+ let product = expected.multipliedReportingOverflow(by: grid.count)
+ guard !product.overflow, product.partialValue <= samples.count else { throw FluidError.incompleteGrid }
+ expected = product.partialValue
+ }
+ guard expected == records.count else { throw FluidError.incompleteGrid }
+ self.samples = samples; self.boundaryPolicy = boundaryPolicy; self.source = source; self.version = version
+ axes = grids; values = records
+ }
+ public func coefficients(for query: BodyAerodynamicQuery) throws -> FluidCoefficients {
+ guard let alpha = query.angleOfAttackRadians, let beta = query.sideslipRadians else { throw FluidError.unsupportedQuery }
+ guard let mach = query.machNumber, let re = try query.reynoldsNumber() else { throw FluidError.missingFlowProperty }
+ return try coefficients(angleOfAttackRadians: alpha,sideslipRadians: beta,machNumber: mach,reynoldsNumber: re)
+ }
+ public func coefficients(angleOfAttackRadians: Double, sideslipRadians: Double,
+ machNumber: Double, reynoldsNumber: Double) throws -> FluidCoefficients {
+ let coordinates = [angleOfAttackRadians,sideslipRadians,machNumber,reynoldsNumber]
+ guard coordinates.allSatisfy(\.isFinite), abs(angleOfAttackRadians) <= .pi,
+ abs(sideslipRadians) <= .pi/2, machNumber >= 0, reynoldsNumber > 0 else { throw FluidError.invalidParameter }
+ let brackets = try zip(coordinates,axes).map { try bracket($0,grid: $1) }
+ func interpolate(_ dimension: Int, key: [Double]) throws -> FluidCoefficients {
+ if dimension == 4 { return values[key]! }
+ let (lower,upper,weight) = brackets[dimension]
+ let first = try interpolate(dimension+1,key: key+[lower])
+ guard lower != upper else { return first }
+ let last = try interpolate(dimension+1,key: key+[upper])
+ return try FluidCoefficients(force: first.force*(1-weight)+last.force*weight,
+ moment: first.moment*(1-weight)+last.moment*weight)
+ }
+ return try interpolate(0,key: [])
+ }
+ private func bracket(_ value: Double, grid: [Double]) throws -> (Double,Double,Double) {
+ guard boundaryPolicy == .clamp || (grid.first!...grid.last!).contains(value) else { throw FluidError.outsideCoverage }
+ let v = min(grid.last!,max(grid.first!,value)), lower = grid.lastIndex(where: { $0 <= v })!
+ guard lower+1 < grid.count, v != grid[lower] else { return (grid[lower],grid[lower],0) }
+ return (grid[lower],grid[lower+1],(v-grid[lower])/(grid[lower+1]-grid[lower]))
+ }
+ private enum CodingKeys: String, CodingKey { case samples, boundaryPolicy, source, version }
+ public init(from decoder: Decoder) throws {
+ let c = try decoder.container(keyedBy: CodingKeys.self)
+ try self.init(samples: c.decode([BodyCoefficientSample].self,forKey: .samples),
+ boundaryPolicy: c.decode(CoefficientBoundaryPolicy.self,forKey: .boundaryPolicy),
+ source: c.decode(String.self,forKey: .source),version: c.decode(String.self,forKey: .version))
+ }
+ public func encode(to encoder: Encoder) throws {
+ var c = encoder.container(keyedBy: CodingKeys.self)
+ try c.encode(samples,forKey: .samples); try c.encode(boundaryPolicy,forKey: .boundaryPolicy)
+ try c.encode(source,forKey: .source); try c.encode(version,forKey: .version)
+ }
+}
+
+/// JSON I/O is separate from coefficient evaluation; decoding revalidates every sample/grid.
+public enum BodyCoefficientTableLoader {
+ public static func json(_ data: Data) throws -> TabulatedBodyCoefficients {
+ try JSONDecoder().decode(TabulatedBodyCoefficients.self,from: data)
+ }
+ public static func jsonFile(_ url: URL) throws -> TabulatedBodyCoefficients { try json(Data(contentsOf: url)) }
+}
diff --git a/Sources/Aerodynamics/BodyRateAerodynamics.swift b/Sources/Aerodynamics/BodyRateAerodynamics.swift
new file mode 100644
index 0000000..c2280cf
--- /dev/null
+++ b/Sources/Aerodynamics/BodyRateAerodynamics.swift
@@ -0,0 +1,119 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// Columns of the six-coefficient derivative with respect to pHat, qHat, rHat.
+/// Signed derivatives may describe damping or excitation; no stability is inferred.
+public struct BodyAerodynamicRateDerivatives: Sendable {
+ public let rollRate: FluidCoefficients
+ public let pitchRate: FluidCoefficients
+ public let yawRate: FluidCoefficients
+ public init(rollRate: FluidCoefficients, pitchRate: FluidCoefficients,
+ yawRate: FluidCoefficients) {
+ self.rollRate = rollRate; self.pitchRate = pitchRate; self.yawRate = yawRate
+ }
+ public func increment(nondimensionalRates rates: SIMD3) throws -> FluidCoefficients {
+ guard fluidFinite(rates) else { throw FluidError.invalidParameter }
+ return try FluidCoefficients(force: rollRate.force*rates.x+pitchRate.force*rates.y+yawRate.force*rates.z,
+ moment: rollRate.moment*rates.x+pitchRate.moment*rates.y+yawRate.moment*rates.z)
+ }
+}
+
+/// Derivatives may depend on the static flow state, but are queried at zero rates.
+public protocol BodyAerodynamicRateDerivativeModel: Sendable {
+ var source: String { get }
+ var version: String { get }
+ func derivatives(for query: BodyAerodynamicQuery) throws -> BodyAerodynamicRateDerivatives
+}
+
+/// Prescribed derivatives within explicit Mach/Re/incidence/sideslip coverage.
+/// Reference dimensions must match the dataset; values are not a capsule database.
+public struct ConstantBodyRateDerivatives: BodyAerodynamicRateDerivativeModel {
+ public let value: BodyAerodynamicRateDerivatives
+ public let source: String
+ public let version: String
+ public let machRange: ClosedRange
+ public let reynoldsRange: ClosedRange
+ public let incidenceRangeRadians: ClosedRange
+ public let sideslipRangeRadians: ClosedRange
+ public let momentLengthsMetres: SIMD3
+ public let reynoldsReferenceLengthMetres: Double
+ public init(value: BodyAerodynamicRateDerivatives, source: String, version: String,
+ machRange: ClosedRange, reynoldsRange: ClosedRange,
+ incidenceRangeRadians: ClosedRange, sideslipRangeRadians: ClosedRange,
+ momentLengthsMetres: SIMD3, reynoldsReferenceLengthMetres: Double) throws {
+ guard [source,version].allSatisfy({ !$0.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty }),
+ machRange.lowerBound.isFinite, machRange.lowerBound >= 0, machRange.upperBound.isFinite,
+ reynoldsRange.lowerBound.isFinite, reynoldsRange.lowerBound > 0, reynoldsRange.upperBound.isFinite,
+ [incidenceRangeRadians.lowerBound,incidenceRangeRadians.upperBound].allSatisfy({ $0.isFinite && abs($0) <= .pi }),
+ [sideslipRangeRadians.lowerBound,sideslipRangeRadians.upperBound].allSatisfy({ $0.isFinite && abs($0) <= .pi/2 }),
+ [momentLengthsMetres.x,momentLengthsMetres.y,momentLengthsMetres.z].allSatisfy({ $0.isFinite && $0 > 0 }),
+ reynoldsReferenceLengthMetres.isFinite, reynoldsReferenceLengthMetres > 0 else { throw FluidError.invalidParameter }
+ self.value = value; self.source = source; self.version = version; self.machRange = machRange; self.reynoldsRange = reynoldsRange
+ self.incidenceRangeRadians = incidenceRangeRadians; self.sideslipRangeRadians = sideslipRangeRadians
+ self.momentLengthsMetres = momentLengthsMetres; self.reynoldsReferenceLengthMetres = reynoldsReferenceLengthMetres
+ }
+ public func derivatives(for query: BodyAerodynamicQuery) throws -> BodyAerodynamicRateDerivatives {
+ guard query.momentLengthsMetres == momentLengthsMetres,
+ query.reynoldsReferenceLengthMetres == reynoldsReferenceLengthMetres else { throw FluidError.invalidGeometry }
+ guard let mach = query.machNumber, let re = try query.reynoldsNumber(),
+ let alpha = query.angleOfAttackRadians, let beta = query.sideslipRadians else { throw FluidError.missingFlowProperty }
+ guard machRange.contains(mach), reynoldsRange.contains(re), incidenceRangeRadians.contains(alpha),
+ sideslipRangeRadians.contains(beta) else { throw FluidError.outsideCoverage }
+ return value
+ }
+}
+
+/// C = Cstatic + D[pHat,qHat,rHat], with rate_i = ω_i L_i/(2V).
+/// Small-rate linearization only; no alphaDot, betaDot, time-history or unsteady lift.
+public struct LinearBodyRateAerodynamics: BodyAerodynamicCoefficientModel {
+ public let staticModel: any BodyAerodynamicCoefficientModel
+ public let derivativeModel: any BodyAerodynamicRateDerivativeModel
+ public let rateReference: BodyAerodynamicRateReference
+ public let minimumSpeedMetresPerSecond: Double
+ public let maximumAbsoluteNondimensionalRates: SIMD3
+ public var source: String { "Static: \(staticModel.source); rate derivatives: \(derivativeModel.source)" }
+ public var version: String { "\(staticModel.version) / \(derivativeModel.version)" }
+ public init(staticModel: any BodyAerodynamicCoefficientModel,
+ derivativeModel: any BodyAerodynamicRateDerivativeModel,
+ rateReference: BodyAerodynamicRateReference,
+ minimumSpeedMetresPerSecond: Double,
+ maximumAbsoluteNondimensionalRates: SIMD3) throws {
+ guard minimumSpeedMetresPerSecond.isFinite, minimumSpeedMetresPerSecond > 0,
+ fluidFinite(maximumAbsoluteNondimensionalRates),
+ [maximumAbsoluteNondimensionalRates.x,maximumAbsoluteNondimensionalRates.y,
+ maximumAbsoluteNondimensionalRates.z].allSatisfy({ $0 >= 0 }) else { throw FluidError.invalidParameter }
+ self.staticModel = staticModel; self.derivativeModel = derivativeModel; self.rateReference = rateReference
+ self.minimumSpeedMetresPerSecond = minimumSpeedMetresPerSecond
+ self.maximumAbsoluteNondimensionalRates = maximumAbsoluteNondimensionalRates
+ }
+ public func coefficients(for query: BodyAerodynamicQuery) throws -> FluidCoefficients {
+ guard query.angularRateReference == rateReference else { throw FluidError.unsupportedQuery }
+ guard query.flow.speedMetresPerSecond >= minimumSpeedMetresPerSecond,
+ let rates = query.nondimensionalAngularRates else { throw FluidError.outsideCoverage }
+ let bounds = maximumAbsoluteNondimensionalRates
+ guard abs(rates.x) <= bounds.x, abs(rates.y) <= bounds.y, abs(rates.z) <= bounds.z else { throw FluidError.outsideCoverage }
+ let staticQuery = try BodyAerodynamicQuery(flow: query.flow,
+ reynoldsReferenceLengthMetres: query.reynoldsReferenceLengthMetres,
+ momentLengthsMetres: query.momentLengthsMetres, angularRateReference: rateReference)
+ let base = try staticModel.coefficients(for: staticQuery)
+ let increment = try derivativeModel.derivatives(for: staticQuery).increment(nondimensionalRates: rates)
+ return try FluidCoefficients(force: base.force+increment.force, moment: base.moment+increment.moment)
+ }
+}
diff --git a/Sources/Aerodynamics/ControlSurfaceAerodynamics.swift b/Sources/Aerodynamics/ControlSurfaceAerodynamics.swift
new file mode 100644
index 0000000..47c3cb2
--- /dev/null
+++ b/Sources/Aerodynamics/ControlSurfaceAerodynamics.swift
@@ -0,0 +1,104 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// A checked incidence/Re/Mach dataset at one supplied geometric deflection.
+public struct ControlSurfaceSetting: Sendable, Codable {
+ public let deflectionRadians: Double
+ public let airfoil: TabulatedAirfoil
+ public init(deflectionRadians: Double, airfoil: TabulatedAirfoil) throws {
+ guard deflectionRadians.isFinite, abs(deflectionRadians) <= .pi else { throw FluidError.invalidParameter }
+ self.deflectionRadians = deflectionRadians; self.airfoil = airfoil
+ }
+ private enum CodingKeys: String, CodingKey { case deflectionRadians, airfoil }
+ public init(from decoder: Decoder) throws {
+ let c = try decoder.container(keyedBy: CodingKeys.self)
+ try self.init(deflectionRadians: c.decode(Double.self,forKey: .deflectionRadians),
+ airfoil: c.decode(TabulatedAirfoil.self,forKey: .airfoil))
+ }
+}
+
+/// Linear interpolation across geometric control deflection, using checked polars
+/// for incidence/Re/Mach. No incidence offset, thin-airfoil effectiveness factor,
+/// actuator response, hinge moment or dynamic-stall behavior is inferred.
+public struct TabulatedControlSurface: WingSectionCoefficientModel, Sendable, Codable {
+ public let settings: [ControlSurfaceSetting]
+ public let deflectionBoundaryPolicy: CoefficientBoundaryPolicy
+ public let source: String
+ public let version: String
+ public let deflectionConvention: String
+ public let momentReferenceDescription: String
+ public var deflectionRangeRadians: ClosedRange {
+ settings.first!.deflectionRadians...settings.last!.deflectionRadians
+ }
+ public init(settings: [ControlSurfaceSetting], deflectionBoundaryPolicy: CoefficientBoundaryPolicy = .reject,
+ source: String, version: String, deflectionConvention: String,
+ momentReferenceDescription: String) throws {
+ guard !settings.isEmpty, [source,version,deflectionConvention,momentReferenceDescription]
+ .allSatisfy({ !$0.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty }) else { throw FluidError.invalidParameter }
+ let ordered = settings.sorted { $0.deflectionRadians < $1.deflectionRadians }
+ guard zip(ordered,ordered.dropFirst()).allSatisfy({ $0.deflectionRadians < $1.deflectionRadians }) else {
+ throw FluidError.duplicateCondition
+ }
+ // Keep the Re/Mach coordinate grid consistent across deflections. Angle
+ // sampling can differ; interpolation uses the coverage of both neighbors.
+ let reference = ordered[0].airfoil.polars
+ let re = Set(reference.map(\.reynoldsNumber)), mach = Set(reference.map(\.machNumber))
+ guard ordered.allSatisfy({ Set($0.airfoil.polars.map(\.reynoldsNumber)) == re
+ && Set($0.airfoil.polars.map(\.machNumber)) == mach }) else { throw FluidError.incompleteGrid }
+ self.settings = ordered; self.deflectionBoundaryPolicy = deflectionBoundaryPolicy
+ self.source = source; self.version = version; self.deflectionConvention = deflectionConvention
+ self.momentReferenceDescription = momentReferenceDescription
+ }
+ public func coefficients(for query: WingSectionQuery) throws -> AirfoilCoefficients {
+ guard let alpha = query.angleOfAttackRadians, let mach = query.machNumber,
+ let re = try query.reynoldsNumber() else { throw FluidError.missingFlowProperty }
+ let deflection = try boundedCoefficientCoordinate(query.controlDeflectionRadians,
+ range: deflectionRangeRadians,policy: deflectionBoundaryPolicy)
+ let lower = settings.lastIndex { $0.deflectionRadians <= deflection }!
+ func evaluate(_ index: Int) throws -> AirfoilCoefficients {
+ try settings[index].airfoil.coefficients(angleOfAttackRadians: alpha,reynoldsNumber: re,machNumber: mach)
+ }
+ let first = try evaluate(lower)
+ // Exact settings query only that dataset, never an irrelevant neighbor.
+ guard settings[lower].deflectionRadians != deflection, lower+1 < settings.count else { return first }
+ let next = lower+1
+ return try blendCoefficients(first,evaluate(next),weight:
+ (deflection-settings[lower].deflectionRadians)/(settings[next].deflectionRadians-settings[lower].deflectionRadians))
+ }
+ private enum CodingKeys: String, CodingKey {
+ case settings, deflectionBoundaryPolicy, source, version, deflectionConvention, momentReferenceDescription
+ }
+ public init(from decoder: Decoder) throws {
+ let c = try decoder.container(keyedBy: CodingKeys.self)
+ try self.init(settings: c.decode([ControlSurfaceSetting].self,forKey: .settings),
+ deflectionBoundaryPolicy: c.decode(CoefficientBoundaryPolicy.self,forKey: .deflectionBoundaryPolicy),
+ source: c.decode(String.self,forKey: .source),version: c.decode(String.self,forKey: .version),
+ deflectionConvention: c.decode(String.self,forKey: .deflectionConvention),
+ momentReferenceDescription: c.decode(String.self,forKey: .momentReferenceDescription))
+ }
+}
+
+public enum ControlSurfaceTableLoader {
+ public static func load(data: Data) throws -> TabulatedControlSurface {
+ do { return try JSONDecoder().decode(TabulatedControlSurface.self,from: data) }
+ catch let error as FluidError { throw error }
+ catch { throw FluidError.malformedData }
+ }
+}
diff --git a/Sources/Aerodynamics/EntrySurfaceHeating.swift b/Sources/Aerodynamics/EntrySurfaceHeating.swift
new file mode 100644
index 0000000..14d1ee0
--- /dev/null
+++ b/Sources/Aerodynamics/EntrySurfaceHeating.swift
@@ -0,0 +1,212 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+public enum AerothermalBoundaryLayer: String, Sendable, Codable { case laminar, turbulent }
+
+/// Edge and wall enthalpies share a dataset-defined reference and composition.
+/// Adiabatic-wall enthalpy includes recovery; no perfect-gas cp*T substitution is made.
+public struct EnthalpySurfaceHeatingQuery: Sendable {
+ public let edgeFlow: FluidFlow
+ public let gasIdentifier: String
+ public let distanceFromLeadingEdgeMetres: Double
+ public let adiabaticWallEnthalpyJoulesPerKilogram: Double
+ public let wallEnthalpyJoulesPerKilogram: Double
+ public let surfacePositionMetres: SIMD3
+ public init(edgeFlow: FluidFlow, gasIdentifier: String, distanceFromLeadingEdgeMetres: Double,
+ adiabaticWallEnthalpyJoulesPerKilogram: Double, wallEnthalpyJoulesPerKilogram: Double,
+ surfacePositionMetres: SIMD3) throws {
+ guard !gasIdentifier.isEmpty, distanceFromLeadingEdgeMetres.isFinite, distanceFromLeadingEdgeMetres > 0,
+ adiabaticWallEnthalpyJoulesPerKilogram.isFinite, adiabaticWallEnthalpyJoulesPerKilogram > 0,
+ wallEnthalpyJoulesPerKilogram.isFinite, wallEnthalpyJoulesPerKilogram >= 0,
+ fluidFinite(surfacePositionMetres) else { throw FluidError.invalidParameter }
+ self.edgeFlow = edgeFlow; self.gasIdentifier = gasIdentifier
+ self.distanceFromLeadingEdgeMetres = distanceFromLeadingEdgeMetres
+ self.adiabaticWallEnthalpyJoulesPerKilogram = adiabaticWallEnthalpyJoulesPerKilogram
+ self.wallEnthalpyJoulesPerKilogram = wallEnthalpyJoulesPerKilogram
+ self.surfacePositionMetres = surfacePositionMetres
+ }
+}
+public struct EnthalpySurfaceHeatingResult: Sendable {
+ /// Signed heat into the surface, W/m².
+ public let wattsPerSquareMetre: Double
+ public let stantonNumber: Double
+ public let surfacePositionMetres: SIMD3
+}
+public protocol EnthalpySurfaceHeatingModel: Sendable {
+ func evaluate(_ query: EnthalpySurfaceHeatingQuery) throws -> EnthalpySurfaceHeatingResult
+}
+
+
+/// Additional thermodynamic/geometry coverage for a supplied Stanton dataset.
+/// Bounds must enclose only states established by the dataset's assumptions.
+public struct EnthalpySurfaceHeatingCoverage: Sendable {
+ public let edgeTemperatureKelvin: ClosedRange
+ public let edgePressurePascals: ClosedRange
+ public let adiabaticWallEnthalpyJoulesPerKilogram: ClosedRange
+ public let distanceFromLeadingEdgeMetres: ClosedRange
+ public init(edgeTemperatureKelvin: ClosedRange, edgePressurePascals: ClosedRange,
+ adiabaticWallEnthalpyJoulesPerKilogram: ClosedRange, distanceFromLeadingEdgeMetres: ClosedRange) throws {
+ guard [edgeTemperatureKelvin,edgePressurePascals,adiabaticWallEnthalpyJoulesPerKilogram,distanceFromLeadingEdgeMetres]
+ .allSatisfy({ $0.lowerBound.isFinite && $0.lowerBound > 0 && $0.upperBound.isFinite }) else {
+ throw FluidError.invalidParameter
+ }
+ self.edgeTemperatureKelvin = edgeTemperatureKelvin; self.edgePressurePascals = edgePressurePascals
+ self.adiabaticWallEnthalpyJoulesPerKilogram = adiabaticWallEnthalpyJoulesPerKilogram
+ self.distanceFromLeadingEdgeMetres = distanceFromLeadingEdgeMetres
+ }
+}
+
+/// Compressible/high-enthalpy local convection from supplied Stanton data, not a
+/// universal gas correlation. Axes: Mach, log10(Re_x), wall/adiabatic-wall enthalpy.
+/// q = rho_edge V_edge St (h_aw - h_wall). Recovery, chemistry, catalytic state,
+/// pressure-gradient and geometry assumptions must be identified in the dataset.
+public struct TabulatedEnthalpySurfaceHeating: EnthalpySurfaceHeatingModel {
+ public let gasIdentifier: String
+ public let boundaryLayer: AerothermalBoundaryLayer
+ public let stanton: FluidScalarTable
+ public let coverage: EnthalpySurfaceHeatingCoverage
+ public let maximumKnudsenNumber: Double
+ public init(gasIdentifier: String, boundaryLayer: AerothermalBoundaryLayer,
+ stanton: FluidScalarTable, coverage: EnthalpySurfaceHeatingCoverage, maximumKnudsenNumber: Double = 0.01) throws {
+ guard !gasIdentifier.isEmpty, stanton.valueUnits == "1", stanton.values.allSatisfy({ $0 >= 0 }),
+ stanton.axes.map(\.name) == ["mach","log10Re","wallEnthalpyRatio"],
+ stanton.axes.allSatisfy({ $0.units == "1" }),
+ stanton.axes[0].coordinates.first! >= 0, stanton.axes[2].coordinates.first! >= 0,
+ maximumKnudsenNumber.isFinite, maximumKnudsenNumber > 0, maximumKnudsenNumber <= 0.01 else {
+ throw FluidError.malformedData
+ }
+ self.gasIdentifier = gasIdentifier; self.boundaryLayer = boundaryLayer
+ self.stanton = stanton; self.coverage = coverage; self.maximumKnudsenNumber = maximumKnudsenNumber
+ }
+ public func evaluate(_ query: EnthalpySurfaceHeatingQuery) throws -> EnthalpySurfaceHeatingResult {
+ guard query.gasIdentifier == gasIdentifier else { throw FluidError.unsupportedQuery }
+ let flow = query.edgeFlow, x = query.distanceFromLeadingEdgeMetres
+ guard let temperature = flow.temperatureKelvin, let pressure = flow.pressurePascals,
+ let mach = flow.machNumber, let re = try flow.reynoldsNumber(referenceLengthMetres: x),
+ let kn = try flow.knudsenNumber(referenceLengthMetres: x) else { throw FluidError.missingFlowProperty }
+ guard re > 0, flow.speedMetresPerSecond > 0, kn <= maximumKnudsenNumber,
+ coverage.edgeTemperatureKelvin.contains(temperature), coverage.edgePressurePascals.contains(pressure),
+ coverage.adiabaticWallEnthalpyJoulesPerKilogram.contains(query.adiabaticWallEnthalpyJoulesPerKilogram),
+ coverage.distanceFromLeadingEdgeMetres.contains(x) else { throw FluidError.outsideCoverage }
+ let st = try stanton.value(at: [mach,log10(re),query.wallEnthalpyJoulesPerKilogram/query.adiabaticWallEnthalpyJoulesPerKilogram])
+ let flux = flow.densityKilogramsPerCubicMetre*flow.speedMetresPerSecond*st
+ * (query.adiabaticWallEnthalpyJoulesPerKilogram-query.wallEnthalpyJoulesPerKilogram)
+ guard flux.isFinite else { throw FluidError.nonFiniteResult }
+ return EnthalpySurfaceHeatingResult(wattsPerSquareMetre: flux,stantonNumber: st,surfacePositionMetres: query.surfacePositionMetres)
+ }
+}
+
+/// Leading-edge stagnation state plus effective sweep relative to incident flow.
+public struct LeadingEdgeHeatingQuery: Sendable {
+ public let stagnation: StagnationHeatingQuery
+ public let effectiveSweepRadians: Double
+ public init(stagnation: StagnationHeatingQuery, effectiveSweepRadians: Double) throws {
+ guard effectiveSweepRadians.isFinite, abs(effectiveSweepRadians) < .pi/2 else {
+ throw FluidError.invalidGeometry
+ }
+ self.stagnation = stagnation; self.effectiveSweepRadians = effectiveSweepRadians
+ }
+}
+public protocol LeadingEdgeConvectiveHeatingModel: Sendable {
+ func heatFlux(for query: LeadingEdgeHeatingQuery) throws -> SurfaceHeatFlux
+}
+
+/// Idealized laminar swept-cylinder stagnation line from a supplied sphere reference.
+/// NASA CR-181922 eq. 1: qSL=qSphere/sqrt(2)*sqrt(RSphere/RLE)*cos(sweep)^1.1.
+/// Earth-air only. Only the stagnation line, not a circumferential distribution or wing acreage.
+public struct SweptCylinderStagnationHeating: LeadingEdgeConvectiveHeatingModel {
+ public let referenceSphereModel: any ConvectiveHeatingModel
+ public let referenceSphereRadiusMetres: Double
+ public let coverage: StagnationHeatingCoverage
+ public let maximumSweepRadians: Double
+ public var source: String { "https://ntrs.nasa.gov/api/citations/19900007739/downloads/19900007739.pdf" }
+ public init(referenceSphereModel: any ConvectiveHeatingModel, referenceSphereRadiusMetres: Double,
+ coverage: StagnationHeatingCoverage, maximumSweepRadians: Double = .pi/3) throws {
+ guard referenceSphereRadiusMetres.isFinite, referenceSphereRadiusMetres > 0,
+ maximumSweepRadians.isFinite, maximumSweepRadians >= 0, maximumSweepRadians <= .pi/3 else {
+ throw FluidError.invalidParameter
+ }
+ self.referenceSphereModel = referenceSphereModel; self.referenceSphereRadiusMetres = referenceSphereRadiusMetres
+ self.coverage = coverage; self.maximumSweepRadians = maximumSweepRadians
+ }
+ public func heatFlux(for query: LeadingEdgeHeatingQuery) throws -> SurfaceHeatFlux {
+ try heatFlux(for: query.stagnation,effectiveSweepRadians: query.effectiveSweepRadians)
+ }
+ /// Query nose radius denotes the actual leading-edge radius. Effective sweep is
+ /// relative to the incident flow, not automatically the planform sweep angle.
+ public func heatFlux(for query: StagnationHeatingQuery, effectiveSweepRadians: Double) throws -> SurfaceHeatFlux {
+ // The published geometry correction is an Earth-air approximation.
+ guard query.gasIdentifier == "earth-air" else { throw FluidError.unsupportedQuery }
+ let flow = query.flow
+ guard effectiveSweepRadians.isFinite, abs(effectiveSweepRadians) <= maximumSweepRadians,
+ coverage.noseRadiusMetres.contains(query.noseRadiusMetres),
+ coverage.speedMetresPerSecond.contains(flow.speedMetresPerSecond),
+ coverage.densityKilogramsPerCubicMetre.contains(flow.densityKilogramsPerCubicMetre) else {
+ throw FluidError.outsideCoverage
+ }
+ guard let mach = flow.machNumber, let kn = try flow.knudsenNumber(referenceLengthMetres: query.noseRadiusMetres) else {
+ throw FluidError.missingFlowProperty
+ }
+ guard coverage.machNumber.contains(mach), kn <= coverage.maximumKnudsenNumber else { throw FluidError.outsideCoverage }
+ let sphereQuery = try StagnationHeatingQuery(flow: flow,gasIdentifier: query.gasIdentifier,
+ noseRadiusMetres: referenceSphereRadiusMetres,surfacePositionMetres: query.surfacePositionMetres,
+ wall: query.wall,gasState: query.gasState)
+ let reference = try referenceSphereModel.heatFlux(for: sphereQuery)
+ let flux = reference.wattsPerSquareMetre/sqrt(2)*sqrt(referenceSphereRadiusMetres/query.noseRadiusMetres)
+ * pow(cos(effectiveSweepRadians),1.1)
+ return try SurfaceHeatFlux(wattsPerSquareMetre: flux,surfacePositionMetres: query.surfacePositionMetres)
+ }
+}
+
+/// Incoming shock-layer radiation from supplied gas-specific data; no radiation
+/// transport solver or empirical universal planetary coefficient is implied.
+/// Axes: speed (m/s), density (kg/m^3), sphere nose radius (m). Cold-wall queries only.
+public struct TabulatedRadiativeHeating: RadiativeHeatingModel {
+ public let gasIdentifier: String
+ public let flux: FluidScalarTable
+ public let freestreamTemperatureKelvin: ClosedRange
+ public let coverage: StagnationHeatingCoverage
+ public init(gasIdentifier: String, flux: FluidScalarTable, coverage: StagnationHeatingCoverage,
+ freestreamTemperatureKelvin: ClosedRange) throws {
+ guard freestreamTemperatureKelvin.lowerBound.isFinite, freestreamTemperatureKelvin.lowerBound > 0,
+ freestreamTemperatureKelvin.upperBound.isFinite, !gasIdentifier.isEmpty, flux.valueUnits == "W/m^2", flux.values.allSatisfy({ $0 >= 0 }),
+ flux.axes.map(\.name) == ["speed","density","radius"],
+ flux.axes.map(\.units) == ["m/s","kg/m^3","m"],
+ flux.axes.allSatisfy({ $0.coordinates.first! > 0 }) else { throw FluidError.malformedData }
+ self.gasIdentifier = gasIdentifier; self.flux = flux; self.coverage = coverage
+ self.freestreamTemperatureKelvin = freestreamTemperatureKelvin
+ }
+ public func heatFlux(for query: StagnationHeatingQuery) throws -> SurfaceHeatFlux {
+ guard query.gasIdentifier == gasIdentifier, query.wall == nil, query.gasState == nil else {
+ throw FluidError.unsupportedQuery
+ }
+ let flow = query.flow
+ guard let temperature = flow.temperatureKelvin, let mach = flow.machNumber,
+ let kn = try flow.knudsenNumber(referenceLengthMetres: query.noseRadiusMetres) else {
+ throw FluidError.missingFlowProperty
+ }
+ guard freestreamTemperatureKelvin.contains(temperature), coverage.speedMetresPerSecond.contains(flow.speedMetresPerSecond),
+ coverage.densityKilogramsPerCubicMetre.contains(flow.densityKilogramsPerCubicMetre),
+ coverage.noseRadiusMetres.contains(query.noseRadiusMetres), coverage.machNumber.contains(mach),
+ kn <= coverage.maximumKnudsenNumber else { throw FluidError.outsideCoverage }
+ return try SurfaceHeatFlux(wattsPerSquareMetre: flux.value(at: [flow.speedMetresPerSecond,
+ flow.densityKilogramsPerCubicMetre,query.noseRadiusMetres]),surfacePositionMetres: query.surfacePositionMetres)
+ }
+}
diff --git a/Sources/Aerodynamics/FiniteWingAirfoil.swift b/Sources/Aerodynamics/FiniteWingAirfoil.swift
new file mode 100644
index 0000000..bda3531
--- /dev/null
+++ b/Sources/Aerodynamics/FiniteWingAirfoil.swift
@@ -0,0 +1,115 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+public enum FiniteWingError: Error, Equatable { case unbracketedSolution, iterationLimit }
+
+public struct FiniteWingSolution: Sendable {
+ public let coefficients: AirfoilCoefficients
+ public let effectiveAngleOfAttackRadians: Double
+ public let inducedAngleRadians: Double
+ public let inducedDragCoefficient: Double
+ public let angleResidualRadians: Double
+ public let iterations: Int
+}
+
+/// Equivalent-wing lifting-line approximation for steady, attached, low-speed flow.
+/// Solves alpha = alphaEffective + CL(alphaEffective)/(pi e AR), then adds
+/// CDi = CL²/(pi e AR). The input polar must contain profile drag only.
+/// This is a uniform-wing approximation, not a spanwise wake/interference solver.
+public struct FiniteWingAirfoil: AirfoilCoefficientModel {
+ public let airfoil: any AirfoilCoefficientModel
+ public let aspectRatio: Double
+ public let spanEfficiency: Double
+ public let effectiveAngleRangeRadians: ClosedRange
+ public let operatingAngleRangeRadians: ClosedRange
+ public let angleToleranceRadians: Double
+ public let maximumIterations: Int
+ public let maximumMachNumber: Double
+ private let inducedFactor: Double
+
+ /// The caller declares an attached-flow effective-angle bracket covered by the
+ /// polar. This approximation restricts AR>=4, Mach<=0.3 and incidence to ±0.35 rad.
+ /// A calibrated span efficiency is explicit; it is not inferred from segmentation.
+ public init(airfoil: any AirfoilCoefficientModel, aspectRatio: Double, spanEfficiency: Double,
+ effectiveAngleRangeRadians: ClosedRange,
+ operatingAngleRangeRadians: ClosedRange,
+ maximumMachNumber: Double = 0.3, angleToleranceRadians: Double = 1e-10,
+ maximumIterations: Int = 64) throws {
+ guard aspectRatio.isFinite, aspectRatio >= 4, spanEfficiency.isFinite,
+ spanEfficiency > 0, spanEfficiency <= 1,
+ maximumMachNumber.isFinite, maximumMachNumber >= 0, maximumMachNumber <= 0.3,
+ angleToleranceRadians.isFinite, angleToleranceRadians > 0,
+ maximumIterations > 0, maximumIterations <= 256,
+ [effectiveAngleRangeRadians.lowerBound,effectiveAngleRangeRadians.upperBound,
+ operatingAngleRangeRadians.lowerBound,operatingAngleRangeRadians.upperBound].allSatisfy({ $0.isFinite && abs($0) <= 0.35 }),
+ effectiveAngleRangeRadians.lowerBound < effectiveAngleRangeRadians.upperBound,
+ operatingAngleRangeRadians.lowerBound < operatingAngleRangeRadians.upperBound else {
+ throw FluidError.invalidParameter
+ }
+ self.airfoil = airfoil; self.aspectRatio = aspectRatio; self.spanEfficiency = spanEfficiency
+ self.effectiveAngleRangeRadians = effectiveAngleRangeRadians; self.operatingAngleRangeRadians = operatingAngleRangeRadians
+ self.maximumMachNumber = maximumMachNumber; self.angleToleranceRadians = angleToleranceRadians
+ self.maximumIterations = maximumIterations
+ inducedFactor = (1/aspectRatio)/spanEfficiency/Double.pi
+ guard inducedFactor.isFinite, inducedFactor > 0 else { throw FluidError.invalidParameter }
+ }
+ public func coefficients(angleOfAttackRadians: Double, reynoldsNumber: Double, machNumber: Double) throws -> AirfoilCoefficients {
+ try solve(angleOfAttackRadians: angleOfAttackRadians,reynoldsNumber: reynoldsNumber,machNumber: machNumber).coefficients
+ }
+ /// Bisection requires a bracketed root, not a promise of a unique solution.
+ /// Use a monotone attached-flow polar; post-stall branches are outside this model.
+ public func solve(angleOfAttackRadians alpha: Double, reynoldsNumber: Double, machNumber: Double) throws -> FiniteWingSolution {
+ guard alpha.isFinite, reynoldsNumber.isFinite, reynoldsNumber > 0, machNumber.isFinite, machNumber >= 0 else {
+ throw FluidError.invalidParameter
+ }
+ guard operatingAngleRangeRadians.contains(alpha), machNumber <= maximumMachNumber else {
+ throw FluidError.outsideCoverage
+ }
+ func evaluate(_ effective: Double) throws -> (AirfoilCoefficients,Double) {
+ let coefficients = try airfoil.coefficients(angleOfAttackRadians: effective,reynoldsNumber: reynoldsNumber,machNumber: machNumber)
+ guard coefficients.isFinite, coefficients.drag >= 0 else { throw FluidError.invalidCoefficients }
+ let residual = effective+coefficients.lift*inducedFactor-alpha
+ guard residual.isFinite else { throw FluidError.nonFiniteResult }
+ return (coefficients,residual)
+ }
+ func result(_ effective: Double, _ value: (AirfoilCoefficients,Double), _ iterations: Int) throws -> FiniteWingSolution {
+ let inducedAngle = value.0.lift*inducedFactor, inducedDrag = value.0.lift*inducedAngle
+ let coefficients = AirfoilCoefficients(lift: value.0.lift,drag: value.0.drag+inducedDrag,moment: value.0.moment)
+ guard inducedDrag.isFinite, coefficients.isFinite else { throw FluidError.nonFiniteResult }
+ return FiniteWingSolution(coefficients: coefficients,effectiveAngleOfAttackRadians: effective,
+ inducedAngleRadians: inducedAngle,inducedDragCoefficient: inducedDrag,
+ angleResidualRadians: value.1,iterations: iterations)
+ }
+ var lower = effectiveAngleRangeRadians.lowerBound, upper = effectiveAngleRangeRadians.upperBound
+ var lowerValue = try evaluate(lower)
+ let upperValue = try evaluate(upper)
+ if abs(lowerValue.1) <= angleToleranceRadians { return try result(lower,lowerValue,0) }
+ if abs(upperValue.1) <= angleToleranceRadians { return try result(upper,upperValue,0) }
+ guard (lowerValue.1 < 0) != (upperValue.1 < 0) else { throw FiniteWingError.unbracketedSolution }
+ for iteration in 1...maximumIterations {
+ let effective = lower+(upper-lower)*0.5
+ let value = try evaluate(effective)
+ if abs(value.1) <= angleToleranceRadians { return try result(effective,value,iteration) }
+ if (lowerValue.1 < 0) == (value.1 < 0) { lower = effective; lowerValue = value }
+ else { upper = effective }
+ }
+ throw FiniteWingError.iterationLimit
+ }
+}
diff --git a/Sources/Aerodynamics/FreeMolecularAerodynamics.swift b/Sources/Aerodynamics/FreeMolecularAerodynamics.swift
new file mode 100644
index 0000000..4b4e522
--- /dev/null
+++ b/Sources/Aerodynamics/FreeMolecularAerodynamics.swift
@@ -0,0 +1,96 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// Ideal single-species Maxwellian gas parameter, with R in J/(kg K).
+/// Using a mixture-average R is an additional approximation, not a resolved mixture.
+public struct FreeMolecularGas: Sendable {
+ public let identifier: String
+ public let specificGasConstantJoulesPerKilogramKelvin: Double
+ public let source: String
+ public init(identifier: String, specificGasConstantJoulesPerKilogramKelvin: Double, source: String) throws {
+ guard [identifier,source].allSatisfy({ !$0.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty }),
+ specificGasConstantJoulesPerKilogramKelvin.isFinite, specificGasConstantJoulesPerKilogramKelvin > 0 else {
+ throw FluidError.invalidParameter
+ }
+ self.identifier = identifier; self.specificGasConstantJoulesPerKilogramKelvin = specificGasConstantJoulesPerKilogramKelvin
+ self.source = source
+ }
+}
+/// Maxwell reflection mixture: a specified fraction reflects specularly; the remainder
+/// is fully accommodated diffuse re-emission at wall temperature, with zero net mass flux.
+public struct GasSurfaceReflection: Sendable {
+ public let specularFraction: Double
+ public let wallTemperatureKelvin: Double
+ public init(specularFraction: Double, wallTemperatureKelvin: Double) throws {
+ guard specularFraction.isFinite, (0...1).contains(specularFraction),
+ wallTemperatureKelvin.isFinite, wallTemperatureKelvin > 0 else { throw FluidError.invalidParameter }
+ self.specularFraction = specularFraction; self.wallTemperatureKelvin = wallTemperatureKelvin
+ }
+}
+
+/// Independent single-collision Maxwellian pressure and shear, including leeward
+/// thermal impacts. Requires Kn≥10; no intermolecular collisions, chemistry,
+/// multiple reflections, shielding calculation, ablation or continuum bridging.
+public struct MaxwellianFreeMolecularTraction: SurfaceTractionModel {
+ public let gas: FreeMolecularGas
+ public let surface: GasSurfaceReflection
+ public let minimumKnudsenNumber: Double
+ public init(gas: FreeMolecularGas, surface: GasSurfaceReflection, minimumKnudsenNumber: Double = 10) throws {
+ guard minimumKnudsenNumber.isFinite, minimumKnudsenNumber >= 10 else { throw FluidError.invalidParameter }
+ self.gas = gas; self.surface = surface; self.minimumKnudsenNumber = minimumKnudsenNumber
+ }
+ public func traction(panel: FluidSurfacePanel, flow: FluidFlow,
+ referenceLengthMetres: Double) throws -> SurfaceTraction {
+ guard let temperature = flow.temperatureKelvin,
+ let kn = try flow.knudsenNumber(referenceLengthMetres: referenceLengthMetres) else { throw FluidError.missingFlowProperty }
+ guard kn >= minimumKnudsenNumber else { throw FluidError.outsideCoverage }
+ let r = gas.specificGasConstantJoulesPerKilogramKelvin
+ let sigma = sqrt(r)*sqrt(temperature), wallSigma = sqrt(r)*sqrt(surface.wallTemperatureKelvin)
+ guard sigma.isFinite, sigma > 0, wallSigma.isFinite else { throw FluidError.nonFiniteResult }
+ let normalVelocity = (flow.relativeVelocityMetresPerSecond*panel.outwardNormal).sum()
+ let a = normalVelocity/sigma
+ // Explicit numerical coverage bound; not a Mach or physical gas validity limit.
+ guard a.isFinite, abs(a) <= 1e6 else { throw FluidError.outsideCoverage }
+ if !panel.exposedToFlow { return try SurfaceTraction(gaugePressurePascals: 0,shearPascals: .zero) }
+ let phi = exp(-0.5*a*a)/sqrt(2*Double.pi)
+ let massMoment: Double, pressureMoment: Double
+ if a < -10 {
+ // Stable Gaussian-tail expansion avoids cancellation on deep leeward faces.
+ let x = -a, t = 1/(x*x)
+ massMoment = phi*t*(1-3*t+15*t*t-105*t*t*t+945*t*t*t*t)
+ pressureMoment = phi*(t/x)*(2-12*t+90*t*t-840*t*t*t+9450*t*t*t*t)
+ } else {
+ let probability = 0.5*erfc(-a/sqrt(2))
+ massMoment = max(0,phi+a*probability)
+ pressureMoment = max(0,(a*a+1)*probability+a*phi)
+ }
+ let rho = flow.densityKilogramsPerCubicMetre
+ let incidentMassFlux = (rho*sigma)*massMoment
+ let ambientPressure = (rho*sigma)*sigma
+ let incidentPressure = ambientPressure*pressureMoment
+ let specular = surface.specularFraction, diffuse = 1-specular
+ let reflectedDiffusePressure = incidentMassFlux*wallSigma*sqrt(Double.pi/2)
+ let pressure = (1+specular)*incidentPressure+diffuse*reflectedDiffusePressure-ambientPressure
+ let tangentVelocity = fluidCross(panel.outwardNormal,
+ fluidCross(flow.relativeVelocityMetresPerSecond,panel.outwardNormal))
+ let shear = -tangentVelocity*(diffuse*incidentMassFlux)
+ return try SurfaceTraction(gaugePressurePascals: pressure,shearPascals: shear)
+ }
+}
diff --git a/Sources/Aerodynamics/HydrogenHeliumHeating.swift b/Sources/Aerodynamics/HydrogenHeliumHeating.swift
new file mode 100644
index 0000000..d258dff
--- /dev/null
+++ b/Sources/Aerodynamics/HydrogenHeliumHeating.swift
@@ -0,0 +1,110 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// Published baseline and approximate composition scalings from Carroll–Brandis 2022.
+/// Saturn/Uranus factors were derived with hot-wall CFD and also used by the authors
+/// for cold-wall trajectory comparisons; they are not independent cold-wall fits.
+public enum HydrogenHeliumHeatingMixture: Sendable {
+ case neptuneReference, saturnApproximation, uranusApproximation
+ public var gasIdentifier: String {
+ switch self {
+ case .neptuneReference: "h2-he-81.55-18.45-mole"
+ case .saturnApproximation: "h2-he-saturn-11-percent-he-mole"
+ case .uranusApproximation: "h2-he-uranus-15-percent-he-mole"
+ }
+ }
+ public var heliumMoleFraction: Double {
+ switch self { case .neptuneReference: 0.1845; case .saturnApproximation: 0.11; case .uranusApproximation: 0.15 }
+ }
+ var scaling: Double {
+ switch self { case .neptuneReference: 1; case .saturnApproximation: 0.952; case .uranusApproximation: 0.980 }
+ }
+}
+
+public struct HydrogenHeliumHeatingResult: Sendable {
+ public let heatFlux: SurfaceHeatFlux
+ public let fittedStagnationPressurePascals: Double
+ public let fittedEnthalpyDifferenceJoulesPerKilogram: Double
+ /// K₂, with source units kg/(s m^1.5 atm^0.5).
+ public let enthalpyCoefficient: Double
+ public let usesHighSpeedFit: Bool
+}
+
+/// Carroll–Brandis 2022 cold-wall nonlinear correlation, equations 4–6, table 3.
+/// Fully catalytic, laminar, non-ablating spherical surface at 300 K; freestream
+/// temperature 141.2 K. No radiation. There is no implicit Jupiter extrapolation.
+public struct HydrogenHeliumColdWallHeating: ConvectiveHeatingModel {
+ public let mixture: HydrogenHeliumHeatingMixture
+ public let source = "https://ntrs.nasa.gov/api/citations/20220018610/downloads/AIAA_Aviation_2022_Paper-6.pdf"
+ public let version = "Carroll–Brandis 2022 cold-wall fit"
+ public init(mixture: HydrogenHeliumHeatingMixture) { self.mixture = mixture }
+
+ /// Conservative piecewise log-density envelope through table-2 end points.
+ /// Interior values interpolate coverage, not CFD data or a certified accuracy bound.
+ public func supportedSpeedRange(densityKilogramsPerCubicMetre density: Double) throws -> ClosedRange {
+ guard density.isFinite, (1e-5...0.1).contains(density) else { throw FluidError.outsideCoverage }
+ let levels: [(Double, Double, Double)] = [(-5,15000,45000),(-4,7000,45000),
+ (-3,7000,27000),(-2,7000,23000),(-1,7000,23000)]
+ let logarithm = log10(density)
+ for i in 0.. SurfaceHeatFlux {
+ try evaluate(query).heatFlux
+ }
+ public func evaluate(_ query: StagnationHeatingQuery) throws -> HydrogenHeliumHeatingResult {
+ guard query.gasIdentifier == mixture.gasIdentifier else { throw FluidError.unsupportedQuery }
+ // Nil explicitly adopts the model's fixed 300 K wall. A specified wall must match.
+ guard query.wall.map({ abs($0.temperatureKelvin-300) <= 1e-6 }) ?? true,
+ query.gasState == nil else { throw FluidError.unsupportedQuery }
+ let flow = query.flow, v = flow.speedMetresPerSecond, rho = flow.densityKilogramsPerCubicMetre
+ guard (0.2...1).contains(query.noseRadiusMetres) else { throw FluidError.outsideCoverage }
+ guard let temperature = flow.temperatureKelvin, let mach = flow.machNumber,
+ let kn = try flow.knudsenNumber(referenceLengthMetres: query.noseRadiusMetres) else {
+ throw FluidError.missingFlowProperty
+ }
+ guard abs(temperature-141.2) <= 1e-6 else { throw FluidError.unsupportedQuery }
+ guard try supportedSpeedRange(densityKilogramsPerCubicMetre: rho).contains(v),
+ mach >= 5, kn <= 0.003 else { throw FluidError.outsideCoverage }
+ let u = v/45000, radius = query.noseRadiusMetres, densityTerm = log10(rho)/(-5)
+ let high = v >= 29000
+ let scaledFlux: Double
+ if high {
+ scaledFlux = 59.084*(u-0.2199)*pow(radius,-0.0429)*pow(densityTerm,-0.0287)
+ } else {
+ scaledFlux = 73.180*(u*u-0.0583*u)*pow(radius,-0.0184)*pow(densityTerm,-0.0254)
+ }
+ let pressure = 0.9474*rho*v*v // Figure 3a; Pa before converting to source atm.
+ let difference = 0.5024*v*v-166.9*v
+ let coefficient = scaledFlux/difference*1e6*mixture.scaling
+ let flux = scaledFlux*1e6*sqrt((pressure/101325)/radius)*mixture.scaling
+ guard flux.isFinite, coefficient.isFinite, flux >= 0 else { throw FluidError.nonFiniteResult }
+ return HydrogenHeliumHeatingResult(heatFlux: try SurfaceHeatFlux(wattsPerSquareMetre: flux,
+ surfacePositionMetres: query.surfacePositionMetres), fittedStagnationPressurePascals: pressure,
+ fittedEnthalpyDifferenceJoulesPerKilogram: difference,
+ enthalpyCoefficient: coefficient, usesHighSpeedFit: high)
+ }
+}
diff --git a/Sources/Aerodynamics/LiftingLineWing.swift b/Sources/Aerodynamics/LiftingLineWing.swift
new file mode 100644
index 0000000..84b21dc
--- /dev/null
+++ b/Sources/Aerodynamics/LiftingLineWing.swift
@@ -0,0 +1,200 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// Supplied linear attached-flow polar at one span station; profile drag excludes
+/// induced drag. Positive geometric incidence raises the leading edge.
+public struct LiftingLineSection: Sendable {
+ public let chordMetres: Double
+ public let liftSlopePerRadian: Double
+ public let zeroLiftAngleRadians: Double
+ public let geometricIncidenceRadians: Double
+ public let profileDragCoefficient: Double
+ public let pitchingMomentCoefficient: Double
+ public let effectiveAngleRangeRadians: ClosedRange
+ public let reynoldsRange: ClosedRange
+ public init(chordMetres: Double, liftSlopePerRadian: Double, zeroLiftAngleRadians: Double = 0,
+ geometricIncidenceRadians: Double = 0, profileDragCoefficient: Double = 0,
+ pitchingMomentCoefficient: Double = 0, effectiveAngleRangeRadians: ClosedRange,
+ reynoldsRange: ClosedRange) throws {
+ guard chordMetres.isFinite, chordMetres > 0, liftSlopePerRadian.isFinite,
+ (0.01...20).contains(liftSlopePerRadian),
+ [zeroLiftAngleRadians,geometricIncidenceRadians].allSatisfy({ $0.isFinite && abs($0) <= 0.35 }),
+ profileDragCoefficient.isFinite, profileDragCoefficient >= 0, pitchingMomentCoefficient.isFinite,
+ [effectiveAngleRangeRadians.lowerBound,effectiveAngleRangeRadians.upperBound]
+ .allSatisfy({ $0.isFinite && abs($0) <= 0.35 }),
+ reynoldsRange.lowerBound.isFinite, reynoldsRange.lowerBound > 0, reynoldsRange.upperBound.isFinite else {
+ throw FluidError.invalidParameter
+ }
+ self.chordMetres = chordMetres; self.liftSlopePerRadian = liftSlopePerRadian; self.zeroLiftAngleRadians = zeroLiftAngleRadians
+ self.geometricIncidenceRadians = geometricIncidenceRadians; self.profileDragCoefficient = profileDragCoefficient
+ self.pitchingMomentCoefficient = pitchingMomentCoefficient; self.effectiveAngleRangeRadians = effectiveAngleRangeRadians
+ self.reynoldsRange = reynoldsRange
+ }
+}
+public struct LiftingLineStationResult: Sendable {
+ public let spanPositionMetres: Double
+ public let circulationSquareMetresPerSecond: Double
+ public let sectionLiftCoefficient: Double
+ public let inducedAngleRadians: Double
+ public let effectiveAngleRadians: Double
+}
+public struct LiftingLineResult: Sendable {
+ public let stations: [LiftingLineStationResult]
+ public let fourierCoefficients: [Double]
+ public let liftCoefficient: Double
+ public let inducedDragCoefficient: Double
+ public let profileDragCoefficient: Double
+ /// Undefined at numerically zero total lift, including antisymmetric loading.
+ public let spanEfficiency: Double?
+ public let maximumEquationResidualRadians: Double
+ public let loads: FluidLoads
+}
+
+/// Classical linear lifting line for one straight, unswept planar wing along body Y.
+/// Uniform incident flow only, zero sideslip, Mach≤0.3, AR≥4, small attached angles.
+/// Geometry matrix is factored once (O(N³)); queries cost O(N²). No wake interaction
+/// with other surfaces, nonuniform incident speed, body rotation or stall solver.
+public struct LiftingLineWing: Sendable {
+ public let spanMetres: Double
+ public let referenceAreaSquareMetres: Double
+ public let momentReferenceLineCentreMetres: SIMD3
+ public let sections: [LiftingLineSection]
+ public let source: String
+ public let version: String
+ public var aspectRatio: Double { (spanMetres/referenceAreaSquareMetres)*spanMetres }
+ private let theta: [Double]
+ private let widths: [Double]
+ private let matrix: [Double]
+ private let factor: LiftingLineFactor
+ /// sectionAtSpanFraction receives −cos(theta), from left (−1) to right (+1).
+ /// Reference area is the dataset's normalization area; it must suit the geometry.
+ public init(spanMetres: Double, referenceAreaSquareMetres: Double, stationCount: Int = 8,
+ momentReferenceLineCentreMetres: SIMD3 = .zero, source: String, version: String,
+ sectionAtSpanFraction: (Double) throws -> LiftingLineSection) throws {
+ guard spanMetres.isFinite, spanMetres > 0, referenceAreaSquareMetres.isFinite, referenceAreaSquareMetres > 0,
+ (2...64).contains(stationCount), fluidFinite(momentReferenceLineCentreMetres),
+ [source,version].allSatisfy({ !$0.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty }) else { throw FluidError.invalidGeometry }
+ let ar = (spanMetres/referenceAreaSquareMetres)*spanMetres
+ guard ar.isFinite, ar >= 4 else { throw FluidError.outsideCoverage }
+ let angles = (1...stationCount).map { Double($0)*Double.pi/Double(stationCount+1) }
+ let local = try angles.map { try sectionAtSpanFraction(-cos($0)) }
+ guard local.allSatisfy({ (1e-6...1).contains($0.chordMetres/spanMetres) }) else { throw FluidError.outsideCoverage }
+ var entries = [Double](), weights = [Double]()
+ for (j,t) in angles.enumerated() {
+ let section = local[j]
+ for n in 1...stationCount {
+ entries.append(sin(Double(n)*t)*(4*spanMetres/(section.liftSlopePerRadian*section.chordMetres)+Double(n)/sin(t)))
+ }
+ // Fejer second-rule weights over x=−cos(theta), then dy=span/2 dx.
+ var sum = 0.0
+ for k in stride(from: 1,through: stationCount,by: 2) { sum += sin(Double(k)*t)/Double(k) }
+ weights.append(spanMetres*2*sin(t)*sum/Double(stationCount+1))
+ }
+ guard entries.allSatisfy(\.isFinite), weights.allSatisfy({ $0.isFinite && $0 > 0 }) else { throw FluidError.nonFiniteResult }
+ factor = try LiftingLineFactor(matrix: entries,count: stationCount)
+ self.spanMetres = spanMetres; self.referenceAreaSquareMetres = referenceAreaSquareMetres
+ self.momentReferenceLineCentreMetres = momentReferenceLineCentreMetres; sections = local; theta = angles
+ matrix = entries; widths = weights; self.source = source; self.version = version
+ }
+ public func evaluate(flow: FluidFlow, momentReferencePointMetres: SIMD3 = .zero) throws -> LiftingLineResult {
+ guard let mach = flow.machNumber, let alpha = flow.angleOfAttackRadians,
+ let beta = flow.sideslipRadians else { throw FluidError.missingFlowProperty }
+ guard flow.speedMetresPerSecond >= 1, mach <= 0.3, abs(alpha) <= 0.35, abs(beta) <= 1e-12 else { throw FluidError.outsideCoverage }
+ for section in sections {
+ guard let re = try flow.reynoldsNumber(referenceLengthMetres: section.chordMetres) else { throw FluidError.missingFlowProperty }
+ guard section.reynoldsRange.contains(re), abs(alpha+section.geometricIncidenceRadians) <= 0.35 else { throw FluidError.outsideCoverage }
+ }
+ let rhs = sections.map { alpha+$0.geometricIncidenceRadians-$0.zeroLiftAngleRadians }
+ let a = try factor.solve(rhs)
+ let n = sections.count, speed = flow.speedMetresPerSecond, q = flow.dynamicPressurePascals
+ var stations = [LiftingLineStationResult](), profileDrag = 0.0, dragSpanMoment = 0.0, pitch = 0.0, residual = 0.0
+ for j in 0.. 0 && abs(a[0]) > 1e-14 ? a[0]*a[0]/sum : nil,
+ maximumEquationResidualRadians: residual,loads: loads)
+ }
+}
+
+private struct LiftingLineFactor: Sendable {
+ let count: Int
+ let lu: [Double]
+ let swaps: [Int]
+ init(matrix: [Double], count: Int) throws {
+ var m = matrix, pivots = [Int]()
+ let scale = matrix.map { abs($0) }.max()!
+ for k in 0.. scale*1e-12 else { throw FluidError.invalidGeometry }
+ pivots.append(row)
+ if row != k { for j in 0.. [Double] {
+ var result = rhs
+ for k in 0..
+ public let reynoldsNumber: ClosedRange
+ public let angleOfAttackRadians: ClosedRange
+ public let sideslipRadians: ClosedRange
+ public let knudsenNumber: ClosedRange
+ public init(machNumber: ClosedRange, reynoldsNumber: ClosedRange,
+ angleOfAttackRadians: ClosedRange, sideslipRadians: ClosedRange,
+ knudsenNumber: ClosedRange) throws {
+ guard [machNumber,reynoldsNumber,angleOfAttackRadians,sideslipRadians,knudsenNumber]
+ .allSatisfy({ $0.lowerBound.isFinite && $0.upperBound.isFinite }),
+ machNumber.lowerBound >= 0, reynoldsNumber.lowerBound > 0, knudsenNumber.lowerBound >= 0,
+ angleOfAttackRadians.lowerBound >= -.pi, angleOfAttackRadians.upperBound <= .pi,
+ sideslipRadians.lowerBound >= -.pi/2, sideslipRadians.upperBound <= .pi/2 else {
+ throw FluidError.invalidParameter
+ }
+ self.machNumber = machNumber; self.reynoldsNumber = reynoldsNumber
+ self.angleOfAttackRadians = angleOfAttackRadians; self.sideslipRadians = sideslipRadians
+ self.knudsenNumber = knudsenNumber
+ }
+ public func validate(flow: FluidFlow, referenceLengthMetres: Double) throws {
+ guard let mach = flow.machNumber, let re = try flow.reynoldsNumber(referenceLengthMetres: referenceLengthMetres),
+ let kn = try flow.knudsenNumber(referenceLengthMetres: referenceLengthMetres),
+ let alpha = flow.angleOfAttackRadians, let beta = flow.sideslipRadians else {
+ throw FluidError.missingFlowProperty
+ }
+ guard machNumber.contains(mach), reynoldsNumber.contains(re), knudsenNumber.contains(kn),
+ angleOfAttackRadians.contains(alpha), sideslipRadians.contains(beta) else {
+ throw FluidError.outsideCoverage
+ }
+ }
+}
+
+/// Binds a coefficient provider to its reference dimensions and stated flow coverage.
+/// Particularly useful for measured/CFD tables across transonic and high-incidence flow.
+public struct CoveredBodyCoefficients: BodyAerodynamicCoefficientModel {
+ public let model: any BodyAerodynamicCoefficientModel
+ public let coverage: GasFlowCoverage
+ public let reynoldsReferenceLengthMetres: Double
+ public let momentLengthsMetres: SIMD3
+ public var source: String { model.source }
+ public var version: String { model.version }
+ public init(model: any BodyAerodynamicCoefficientModel, coverage: GasFlowCoverage,
+ reynoldsReferenceLengthMetres: Double, momentLengthsMetres: SIMD3) throws {
+ guard reynoldsReferenceLengthMetres.isFinite, reynoldsReferenceLengthMetres > 0,
+ [momentLengthsMetres.x,momentLengthsMetres.y,momentLengthsMetres.z].allSatisfy({ $0.isFinite && $0 > 0 }) else {
+ throw FluidError.invalidGeometry
+ }
+ self.model = model; self.coverage = coverage
+ self.reynoldsReferenceLengthMetres = reynoldsReferenceLengthMetres; self.momentLengthsMetres = momentLengthsMetres
+ }
+ public func coefficients(for query: BodyAerodynamicQuery) throws -> FluidCoefficients {
+ guard query.reynoldsReferenceLengthMetres == reynoldsReferenceLengthMetres,
+ query.momentLengthsMetres == momentLengthsMetres else { throw FluidError.unsupportedQuery }
+ try coverage.validate(flow: query.flow,referenceLengthMetres: reynoldsReferenceLengthMetres)
+ return try model.coefficients(for: query)
+ }
+}
+
+/// Explicit ordered Mach dispatch. Threshold belongs to the higher interval.
+/// Gaps and other coverage checks are owned by the selected bounded provider.
+/// Discontinuous databases remain discontinuous; this does not invent a transition blend.
+public struct MachRegimeBodyCoefficients: BodyAerodynamicCoefficientModel {
+ public let models: [any BodyAerodynamicCoefficientModel]
+ public let machThresholds: [Double]
+ public let source: String
+ public let version: String
+ public init(models: [any BodyAerodynamicCoefficientModel], machThresholds: [Double],
+ source: String, version: String) throws {
+ guard !models.isEmpty, models.count == machThresholds.count+1,
+ machThresholds.allSatisfy({ $0.isFinite && $0 > 0 }),
+ zip(machThresholds,machThresholds.dropFirst()).allSatisfy({ $0 < $1 }),
+ !source.isEmpty, !version.isEmpty else { throw FluidError.invalidParameter }
+ self.models = models; self.machThresholds = machThresholds; self.source = source; self.version = version
+ }
+ public func coefficients(for query: BodyAerodynamicQuery) throws -> FluidCoefficients {
+ guard let mach = query.machNumber else { throw FluidError.missingFlowProperty }
+ return try models[machThresholds.prefix(while: { mach >= $0 }).count].coefficients(for: query)
+ }
+}
diff --git a/Sources/Aerodynamics/NACA.swift b/Sources/Aerodynamics/NACA.swift
index 4e1dbca..abb33b6 100644
--- a/Sources/Aerodynamics/NACA.swift
+++ b/Sources/Aerodynamics/NACA.swift
@@ -17,21 +17,38 @@
//
+import FluidDynamics
import Foundation
// NACA: 4 digits describing airfoil
-public struct NACA4 {
+/// Four-digit geometry with the conventional finite trailing-edge thickness.
+/// Source: NASA-TM-X-3284, https://ntrs.nasa.gov/citations/19760003945
+public struct NACA4: Sendable {
public let camberPercentage: Int
public let maximumCamber: Int
public let maximumThicknessPercentage: Int
+ /// Four-digit NACA parameters; coordinates are normalized by chord.
public init(camberPercentage: Int, maximumCamber: Int, maximumThicknessPercentage: Int) {
+ precondition(Self.valid(camberPercentage, maximumCamber, maximumThicknessPercentage), "Invalid NACA four-digit geometry")
self.camberPercentage = camberPercentage
self.maximumCamber = maximumCamber
self.maximumThicknessPercentage = maximumThicknessPercentage
}
+ public init(validatingCamberPercentage camberPercentage: Int, maximumCamber: Int, maximumThicknessPercentage: Int) throws {
+ guard Self.valid(camberPercentage, maximumCamber, maximumThicknessPercentage) else { throw FluidError.invalidGeometry }
+ self.camberPercentage = camberPercentage; self.maximumCamber = maximumCamber
+ self.maximumThicknessPercentage = maximumThicknessPercentage
+ }
+ private static func valid(_ m: Int, _ p: Int, _ t: Int) -> Bool {
+ (0...9).contains(m) && (0...9).contains(p) && (0...99).contains(t) && (m == 0 || p > 0)
+ }
+ private func checkChord(_ x: Double) {
+ precondition(x.isFinite && (0...1).contains(x), "Normalized chord coordinate must be in 0...1")
+ }
public func thickness(_ x: Double) -> Double {
+ checkChord(x)
let t = Double(maximumThicknessPercentage)/100.0
let yt = 5 * t * (0.2969 * sqrt(x) -
0.1260 * x -
@@ -41,6 +58,8 @@ public struct NACA4 {
return yt
}
public func meanCamberLine(_ x: Double) -> Double {
+ checkChord(x)
+ if camberPercentage == 0 { return 0 }
let m = Double(camberPercentage) / 100.0
let p = Double(maximumCamber) / 10.0
@@ -53,6 +72,20 @@ public struct NACA4 {
return yc
}
+ /// Derivative of the normalized camber line with respect to normalized chord.
+ public func meanCamberSlope(_ x: Double) -> Double {
+ checkChord(x)
+ guard camberPercentage != 0 else { return 0 }
+ let m = Double(camberPercentage)/100, p = Double(maximumCamber)/10
+ return x <= p ? 2*m*(p-x)/(p*p) : 2*m*(p-x)/((1-p)*(1-p))
+ }
+
+ /// Checked surface evaluation for caller-owned geometry input.
+ public func surfaceCoordinates(atChordFraction x: Double) throws -> (SIMD2, SIMD2) {
+ guard x.isFinite, (0...1).contains(x) else { throw FluidError.invalidGeometry }
+ return surfaceCoord(x: x)
+ }
+
public func surfaceCoord(x: Double) -> (SIMD2, SIMD2) {
let yt = thickness(x)
if camberPercentage == 0 && maximumCamber == 0 {
@@ -62,7 +95,7 @@ public struct NACA4 {
}
let yc = meanCamberLine(x)
- let dyx = 0.0
+ let dyx = meanCamberSlope(x)
let theta = atan(dyx)
let xu = x - yt * sin(theta)
let xl = x + yt * sin(theta)
diff --git a/Sources/Aerodynamics/NonlinearLiftingLine.swift b/Sources/Aerodynamics/NonlinearLiftingLine.swift
new file mode 100644
index 0000000..585bfff
--- /dev/null
+++ b/Sources/Aerodynamics/NonlinearLiftingLine.swift
@@ -0,0 +1,152 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// Converged fixed-wake solution. Circulation is m²/s and induced air velocity is
+/// the medium's physical velocity, so subtract it from body-relative incident flow.
+public struct NonlinearLiftingLineResult: Sendable {
+ public let circulationSquareMetresPerSecond: [Double]
+ public let inducedAirVelocityMetresPerSecond: [SIMD3]
+ public let segments: [WingSegmentResult]
+ public let loads: FluidLoads
+ public let iterations: Int
+ public let maximumNormalizedCirculationResidual: Double
+}
+
+/// Nonlinear discrete horseshoe lifting line for multiple unswept lifting surfaces.
+/// Uses supplied section polars and nonuniform incident flow, with fixed straight
+/// wakes and a finite vortex core. No free-wake rollup, compressibility or separated
+/// 3-D flow prediction. Nonlinear polar input does not establish post-stall accuracy.
+/// Setup O(N²); solve O(iterations*N²), N≤256. Geometry is aerodynamic, not assembly state.
+public struct NonlinearLiftingLine: Sendable {
+ public let segments: [WingSegment]
+ public let wakeDirection: SIMD3
+ public let wakeLengthMetres: Double
+ public let vortexCoreRadiusMetres: Double
+ public let relaxation: Double
+ public let tolerance: Double
+ public let maximumIterations: Int
+ private let influence: [[SIMD3]]
+ public init(segments: [WingSegment], wakeDirection: SIMD3 = SIMD3(-1,0,0),
+ wakeLengthMetres: Double, vortexCoreRadiusMetres: Double,
+ relaxation: Double = 0.1, tolerance: Double = 1e-8, maximumIterations: Int = 1000) throws {
+ let directionLength = fluidNorm(wakeDirection)
+ guard !segments.isEmpty, segments.count <= 256, fluidFinite(wakeDirection), directionLength.isFinite, directionLength > 0,
+ wakeLengthMetres.isFinite, wakeLengthMetres > 0, vortexCoreRadiusMetres.isFinite, vortexCoreRadiusMetres > 0,
+ relaxation.isFinite, relaxation > 0, relaxation <= 0.5,
+ tolerance.isFinite, tolerance > 0, tolerance <= 1e-3,
+ (1...10000).contains(maximumIterations) else { throw FluidError.invalidParameter }
+ let direction = wakeDirection/directionLength
+ let minimumWidth = segments.map { $0.areaSquareMetres/$0.chordMetres }.min()!
+ guard minimumWidth.isFinite, minimumWidth > 0, vortexCoreRadiusMetres <= minimumWidth*0.02,
+ segments.allSatisfy({ abs(($0.axes.span*direction).sum()) < 1e-10
+ && -($0.axes.forward*direction).sum() >= cos(0.35) }) else { throw FluidError.invalidGeometry }
+ // Duplicate control points are ambiguous even with core regularization.
+ for i in segments.indices {
+ for j in 0.. 2*vortexCoreRadiusMetres else {
+ throw FluidError.invalidGeometry
+ }
+ }
+ }
+ self.segments = segments; self.wakeDirection = direction; self.wakeLengthMetres = wakeLengthMetres
+ self.vortexCoreRadiusMetres = vortexCoreRadiusMetres; self.relaxation = relaxation
+ self.tolerance = tolerance; self.maximumIterations = maximumIterations
+ self.influence = try segments.map { target in
+ try segments.map { source in
+ try Self.horseshoe(at: target.positionMetres,segment: source,direction: direction,
+ length: wakeLengthMetres,core: vortexCoreRadiusMetres)
+ }
+ }
+ }
+ /// Unit-circulation finite straight segment, regularized Biot–Savart kernel.
+ private static func vortex(at p: SIMD3, from a: SIMD3, to b: SIMD3, core: Double) throws -> SIMD3 {
+ let r1 = p-a, r2 = p-b, line = b-a
+ let l1 = fluidNorm(r1), l2 = fluidNorm(r2), lineLength = fluidNorm(line)
+ guard l1.isFinite, l2.isFinite, lineLength.isFinite, lineLength > 0,
+ l1 > core, l2 > core else { throw FluidError.invalidGeometry }
+ let cross = fluidCross(r1,r2)
+ let denominator = (cross*cross).sum()+core*core*lineLength*lineLength
+ let velocity = cross*((line*(r1/l1-r2/l2)).sum()/(4*Double.pi*denominator))
+ guard fluidFinite(velocity) else { throw FluidError.nonFiniteResult }
+ return velocity
+ }
+ private static func horseshoe(at p: SIMD3, segment: WingSegment, direction: SIMD3,
+ length: Double, core: Double) throws -> SIMD3 {
+ let halfSpan = segment.axes.span*(0.5*segment.areaSquareMetres/segment.chordMetres)
+ let a = segment.positionMetres-halfSpan, b = segment.positionMetres+halfSpan
+ return try vortex(at: p,from: a+direction*length,to: a,core: core)
+ + vortex(at: p,from: a,to: b,core: core)
+ + vortex(at: p,from: b,to: b+direction*length,core: core)
+ }
+ /// Physical induced medium velocity for external bodies/tails. This includes
+ /// bound and trailing vortices; callers must avoid the finite-core/end-point region.
+ public func inducedAirVelocity(at positionMetres: SIMD3, circulation: [Double]) throws -> SIMD3 {
+ guard fluidFinite(positionMetres), circulation.count == segments.count,
+ circulation.allSatisfy(\.isFinite) else { throw FluidError.invalidParameter }
+ var velocity = SIMD3.zero
+ for i in segments.indices {
+ velocity += try Self.horseshoe(at: positionMetres,segment: segments[i],direction: wakeDirection,
+ length: wakeLengthMetres,core: vortexCoreRadiusMetres)*circulation[i]
+ }
+ guard fluidFinite(velocity) else { throw FluidError.nonFiniteResult }
+ return velocity
+ }
+ public func evaluate(momentReferencePointMetres: SIMD3 = .zero,
+ flowAtSegment: (WingSegment) throws -> FluidFlow) throws -> NonlinearLiftingLineResult {
+ let incident = try segments.map(flowAtSegment)
+ for (segment,flow) in zip(segments,incident) {
+ guard let mach = flow.machNumber else { throw FluidError.missingFlowProperty }
+ let speed = flow.speedMetresPerSecond
+ guard speed >= 1, mach <= 0.3, flow.densityKilogramsPerCubicMetre > 0,
+ abs((flow.relativeVelocityMetresPerSecond*segment.axes.span).sum())/speed <= 0.1,
+ -(flow.relativeVelocityMetresPerSecond*wakeDirection).sum()/speed >= cos(0.35) else {
+ throw FluidError.outsideCoverage
+ }
+ }
+ var gamma = [Double](repeating: 0,count: segments.count)
+ for iteration in 1...maximumIterations {
+ var results: [WingSegmentResult] = [], velocities: [SIMD3] = [], targets: [Double] = []
+ var residual = 0.0
+ for i in segments.indices {
+ let induced = zip(influence[i],gamma).reduce(SIMD3.zero) { $0+$1.0*$1.1 }
+ let local = try incident[i].replacingRelativeVelocity(incident[i].relativeVelocityMetresPerSecond-induced)
+ guard let mach = local.machNumber, mach <= 0.3 else { throw FluidError.outsideCoverage }
+ let result = try segments[i].evaluate(bodyFlow: local)
+ guard let alpha = result.sectionFlow.angleOfAttackRadians, abs(alpha) <= 0.35,
+ let coefficients = result.coefficients, coefficients.drag >= 0,
+ abs(coefficients.lift) <= 2 else { throw FluidError.outsideCoverage }
+ let target = 0.5*result.sectionFlow.speedMetresPerSecond*segments[i].chordMetres*coefficients.lift
+ let scale = 0.5*incident[i].speedMetresPerSecond*segments[i].chordMetres
+ let error = abs(target-gamma[i])/scale
+ guard target.isFinite, error.isFinite else { throw FluidError.nonFiniteResult }
+ residual = max(residual,error); targets.append(target); results.append(result); velocities.append(induced)
+ }
+ if residual <= tolerance {
+ var loads = try FluidLoads(forceNewtons: .zero,momentNewtonMetres: .zero,referencePointMetres: momentReferencePointMetres)
+ for result in results { loads = try loads.adding(result.loads) }
+ return NonlinearLiftingLineResult(circulationSquareMetresPerSecond: gamma,
+ inducedAirVelocityMetresPerSecond: velocities,segments: results,loads: loads,
+ iterations: iteration,maximumNormalizedCirculationResidual: residual)
+ }
+ for i in gamma.indices { gamma[i] += relaxation*(targets[i]-gamma[i]) }
+ }
+ throw FluidError.nonConvergence
+ }
+}
diff --git a/Sources/Aerodynamics/ParachuteAerodynamics.swift b/Sources/Aerodynamics/ParachuteAerodynamics.swift
new file mode 100644
index 0000000..c17691a
--- /dev/null
+++ b/Sources/Aerodynamics/ParachuteAerodynamics.swift
@@ -0,0 +1,27 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+/// Current-canopy steady drag. No opening loads, tether transmission or deployment.
+public struct ParachuteAerodynamics: Sendable {
+ public let drag: DragAreaForces
+ public init(drag: DragAreaForces) { self.drag = drag }
+ public func evaluate(flow: FluidFlow, momentReferencePointMetres: SIMD3 = .zero) throws -> FluidLoads {
+ try drag.evaluate(flow: flow, momentReferencePointMetres: momentReferencePointMetres)
+ }
+}
diff --git a/Sources/Aerodynamics/SurfaceHeating.swift b/Sources/Aerodynamics/SurfaceHeating.swift
new file mode 100644
index 0000000..e437d69
--- /dev/null
+++ b/Sources/Aerodynamics/SurfaceHeating.swift
@@ -0,0 +1,121 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// Local boundary-layer-edge flow, not freestream flow across an intervening shock.
+/// Distance follows the surface streamline from the thermal/aerodynamic leading edge.
+public struct SurfaceHeatingQuery: Sendable {
+ public let edgeFlow: FluidFlow
+ public let distanceFromLeadingEdgeMetres: Double
+ public let surfacePositionMetres: SIMD3
+ public let wall: AerothermalWallState
+ public let transport: ThermalTransportProperties
+ public init(edgeFlow: FluidFlow, distanceFromLeadingEdgeMetres: Double,
+ surfacePositionMetres: SIMD3, wall: AerothermalWallState,
+ transport: ThermalTransportProperties) throws {
+ guard distanceFromLeadingEdgeMetres.isFinite, distanceFromLeadingEdgeMetres > 0 else {
+ throw FluidError.invalidGeometry
+ }
+ guard fluidFinite(surfacePositionMetres) else { throw FluidError.invalidGeometry }
+ self.edgeFlow = edgeFlow; self.distanceFromLeadingEdgeMetres = distanceFromLeadingEdgeMetres
+ self.surfacePositionMetres = surfacePositionMetres; self.wall = wall; self.transport = transport
+ }
+}
+
+/// Signed convection: positive into the wall, negative cooling into the gas.
+/// Unlike incoming-only SurfaceHeatFlux, this retains convective cooling.
+public struct SurfaceConvectionResult: Sendable {
+ public let wattsPerSquareMetre: Double
+ public let surfacePositionMetres: SIMD3
+ public let heatTransferCoefficientWattsPerSquareMetreKelvin: Double
+ public let localNusseltNumber: Double
+ public let localReynoldsNumber: Double
+ public let prandtlNumber: Double
+ public init(wattsPerSquareMetre: Double, surfacePositionMetres: SIMD3,
+ heatTransferCoefficientWattsPerSquareMetreKelvin: Double,
+ localNusseltNumber: Double, localReynoldsNumber: Double, prandtlNumber: Double) throws {
+ guard wattsPerSquareMetre.isFinite, fluidFinite(surfacePositionMetres),
+ [heatTransferCoefficientWattsPerSquareMetreKelvin,localNusseltNumber,localReynoldsNumber,prandtlNumber]
+ .allSatisfy({ $0.isFinite && $0 > 0 }) else { throw FluidError.nonFiniteResult }
+ self.wattsPerSquareMetre = wattsPerSquareMetre; self.surfacePositionMetres = surfacePositionMetres
+ self.heatTransferCoefficientWattsPerSquareMetreKelvin = heatTransferCoefficientWattsPerSquareMetreKelvin
+ self.localNusseltNumber = localNusseltNumber; self.localReynoldsNumber = localReynoldsNumber
+ self.prandtlNumber = prandtlNumber
+ }
+}
+
+/// Replaceable local surface convection, separate from blunt-body stagnation heating.
+public protocol SurfaceConvectiveHeatingModel: Sendable {
+ func evaluate(_ query: SurfaceHeatingQuery) throws -> SurfaceConvectionResult
+}
+
+/// Isothermal flat plate, attached laminar parallel flow with zero pressure gradient.
+/// Nu_x = 0.332 sqrt(Re_x) Pr^(1/3). O(1) per point; no surface mesh or thermal state.
+/// Conservative implementation limits: Mach ≤ 0.3, 1000 ≤ Re_x ≤ 500000,
+/// 0.6 ≤ Pr ≤ 15, Kn_x ≤ 0.01 and 0.8 ≤ Tw/Te ≤ 1.25.
+/// The caller must establish the plate/flow assumptions; these bounds do not detect transition.
+public struct LaminarFlatPlateHeating: SurfaceConvectiveHeatingModel {
+ public init() {}
+ public var source: String {
+ "https://archive.nptel.ac.in/content/storage2/courses/112104159/module2/Lec8.pdf"
+ }
+ public func evaluate(_ query: SurfaceHeatingQuery) throws -> SurfaceConvectionResult {
+ try flatPlateConvection(query,coefficient: 0.332,reynoldsExponent: 0.5,reynoldsRange: 1000...500000)
+ }
+}
+
+
+/// Fully turbulent isothermal flat plate from its leading edge, not a transition
+/// model. Nu_x=0.0296 Re_x^0.8 Pr^(1/3). Same low-Mach/Kn/temperature restrictions
+/// as the laminar model, but 500000 ≤ Re_x ≤ 10000000 and 0.6 ≤ Pr ≤ 15.
+public struct TurbulentFlatPlateHeating: SurfaceConvectiveHeatingModel {
+ public init() {}
+ public var source: String { "https://archive.nptel.ac.in/content/storage2/courses/112104159/module2/Lec12.pdf" }
+ public func evaluate(_ query: SurfaceHeatingQuery) throws -> SurfaceConvectionResult {
+ try flatPlateConvection(query,coefficient: 0.0296,reynoldsExponent: 0.8,reynoldsRange: 500000...10000000)
+ }
+}
+
+private func flatPlateConvection(_ query: SurfaceHeatingQuery, coefficient: Double,
+ reynoldsExponent: Double, reynoldsRange: ClosedRange) throws -> SurfaceConvectionResult {
+ let flow = query.edgeFlow, properties = query.transport, x = query.distanceFromLeadingEdgeMetres
+ guard let temperature = flow.temperatureKelvin, let mach = flow.machNumber,
+ let kn = try flow.knudsenNumber(referenceLengthMetres: x) else {
+ throw FluidError.missingFlowProperty
+ }
+ let wallTemperature = query.wall.temperatureKelvin
+ let filmTemperature = 0.5*temperature+0.5*wallTemperature
+ guard abs(properties.temperatureKelvin-filmTemperature) <= 1e-8*filmTemperature else {
+ throw FluidError.unsupportedQuery
+ }
+ // Transport properties are at film conditions, independently of edge-flow density/viscosity.
+ let re = properties.densityKilogramsPerCubicMetre*flow.speedMetresPerSecond*x/properties.dynamicViscosityPascalSeconds
+ let pr = properties.prandtlNumber
+ guard re.isFinite else { throw FluidError.nonFiniteResult }
+ guard mach <= 0.3, reynoldsRange.contains(re), (0.6...15).contains(pr),
+ kn <= 0.01, (0.8...1.25).contains(wallTemperature/temperature) else {
+ throw FluidError.outsideCoverage
+ }
+ let nu = coefficient*pow(re,reynoldsExponent)*pow(pr,1.0/3.0)
+ let h = nu*properties.thermalConductivityWattsPerMetreKelvin/x
+ return try SurfaceConvectionResult(wattsPerSquareMetre: h*(temperature-wallTemperature),
+ surfacePositionMetres: query.surfacePositionMetres,
+ heatTransferCoefficientWattsPerSquareMetreKelvin: h,
+ localNusseltNumber: nu, localReynoldsNumber: re, prandtlNumber: pr)
+}
diff --git a/Sources/Aerodynamics/SurfacePressure.swift b/Sources/Aerodynamics/SurfacePressure.swift
new file mode 100644
index 0000000..86f9a8d
--- /dev/null
+++ b/Sources/Aerodynamics/SurfacePressure.swift
@@ -0,0 +1,59 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+/// Idealized calorically perfect gas, windward modified-Newtonian pressure only.
+/// Cp = CpMax max(0, normal·velocityDirection)². No shear, base suction, heating,
+/// shock interaction or real-gas chemistry. Gas gamma is supplied, not Earth-specific.
+public struct ModifiedNewtonianPressure: SurfacePressureCoefficientModel {
+ public let specificHeatRatio: Double
+ public let machRange: ClosedRange
+ public let maximumKnudsenNumber: Double
+ public init(specificHeatRatio: Double, machRange: ClosedRange = 5...25,
+ maximumKnudsenNumber: Double = 0.01) throws {
+ guard specificHeatRatio.isFinite, specificHeatRatio > 1, specificHeatRatio <= 2,
+ machRange.lowerBound.isFinite, machRange.upperBound.isFinite,
+ machRange.lowerBound >= 5, machRange.upperBound <= 50,
+ maximumKnudsenNumber.isFinite, maximumKnudsenNumber > 0,
+ maximumKnudsenNumber <= 0.01 else { throw FluidError.invalidParameter }
+ self.specificHeatRatio = specificHeatRatio; self.machRange = machRange
+ self.maximumKnudsenNumber = maximumKnudsenNumber
+ }
+ /// Normal shock followed by isentropic deceleration to stagnation.
+ public func stagnationPressureCoefficient(machNumber m: Double) throws -> Double {
+ guard m.isFinite, machRange.contains(m) else { throw FluidError.outsideCoverage }
+ let g = specificHeatRatio, m2 = m*m
+ let pressureRatio = (2*g*m2-(g-1))/(g+1)
+ let downstreamMachSquared = ((g-1)*m2+2)/(2*g*m2-(g-1))
+ let stagnationRatio = pressureRatio*exp((g/(g-1))*log1p((g-1)*downstreamMachSquared/2))
+ let result = (stagnationRatio-1)/(0.5*g*m2)
+ guard result.isFinite, result > 0 else { throw FluidError.nonFiniteResult }
+ return result
+ }
+ public func pressureCoefficient(panel: FluidSurfacePanel, flow: FluidFlow,
+ referenceLengthMetres: Double) throws -> Double {
+ // Validate length even at rest, but rest needs no Mach/rarefaction inference.
+ let kn = try flow.knudsenNumber(referenceLengthMetres: referenceLengthMetres)
+ if flow.speedMetresPerSecond == 0 { return 0 }
+ guard let mach = flow.machNumber, let kn else { throw FluidError.missingFlowProperty }
+ guard kn <= maximumKnudsenNumber else { throw FluidError.outsideCoverage }
+ let maximum = try stagnationPressureCoefficient(machNumber: mach)
+ let incidence = max(0, min(1, (panel.outwardNormal*flow.relativeVelocityMetresPerSecond).sum()/flow.speedMetresPerSecond))
+ return panel.exposedToFlow ? maximum*incidence*incidence : 0
+ }
+}
diff --git a/Sources/Aerodynamics/SuttonGravesMixtures.swift b/Sources/Aerodynamics/SuttonGravesMixtures.swift
new file mode 100644
index 0000000..a035a8f
--- /dev/null
+++ b/Sources/Aerodynamics/SuttonGravesMixtures.swift
@@ -0,0 +1,104 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// Molecular weights and Mγ transport products from NASA TR R-376, table I.
+public enum SuttonGravesBaseGas: String, Sendable, CaseIterable {
+ case nitrogen, oxygen, hydrogen, helium, neon, argon, carbonDioxide, ammonia, methane
+ public var molecularWeight: Double {
+ switch self {
+ case .nitrogen: 28.014; case .oxygen: 32; case .hydrogen: 2.016
+ case .helium: 4.003; case .neon: 20.183; case .argon: 39.948
+ case .carbonDioxide: 44.011; case .ammonia: 17.031; case .methane: 16.043
+ }
+ }
+ var molecularWeightTransportProduct: Double {
+ switch self {
+ case .nitrogen: 1.024; case .oxygen: 1.321; case .hydrogen: 0.137
+ case .helium: 0.434; case .neon: 1.504; case .argon: 1.612
+ case .carbonDioxide: 1.285; case .ammonia: 0.784; case .methane: 0.537
+ }
+ }
+}
+
+/// Equation 42 mixture K, distinct from the coefficient of sqrt(ρ/R) V³.
+/// Uses wall Prandtl number 0.69 and the report's rounded table-I products.
+public struct SuttonGravesMixtureParameters: Sendable {
+ public let gasIdentifier: String
+ public let massFractions: [SuttonGravesBaseGas: Double]
+ /// Source units kg/(s m^1.5 atm^0.5). Evaluators convert supplied Pa to atm.
+ public let enthalpyCoefficient: Double
+ public let source = "https://ntrs.nasa.gov/citations/19720003329"
+ public let version = "NASA TR R-376, equation 42 and table I"
+ public init(gasIdentifier: String, massFractions: [SuttonGravesBaseGas: Double]) throws {
+ guard !gasIdentifier.trimmingCharacters(in: .whitespacesAndNewlines).isEmpty,
+ !massFractions.isEmpty, massFractions.values.allSatisfy({ $0.isFinite && $0 >= 0 }),
+ abs(massFractions.values.reduce(0,+)-1) <= 1e-10 else { throw FluidError.invalidParameter }
+ self.gasIdentifier = gasIdentifier; self.massFractions = massFractions
+ let sum = SuttonGravesBaseGas.allCases.reduce(0.0) {
+ $0 + (massFractions[$1] ?? 0)/$1.molecularWeightTransportProduct
+ }
+ enthalpyCoefficient = 0.1106/sqrt(sum)
+ }
+ public init(gasIdentifier: String, moleFractions: [SuttonGravesBaseGas: Double]) throws {
+ guard !moleFractions.isEmpty, moleFractions.values.allSatisfy({ $0.isFinite && $0 >= 0 }),
+ abs(moleFractions.values.reduce(0,+)-1) <= 1e-10 else { throw FluidError.invalidParameter }
+ let mass = moleFractions.reduce(0.0) { $0+$1.value*$1.key.molecularWeight }
+ try self.init(gasIdentifier: gasIdentifier, massFractions: moleFractions.reduce(into: [:]) {
+ $0[$1.key] = $1.value*$1.key.molecularWeight/mass
+ })
+ }
+ /// Idealized 96.5% CO₂ / 3.5% N₂ by mole, ignoring trace constituents.
+ /// Composition source: NASA Venus fact sheet; this is a derived mixture, not
+ /// a fitted or flight-validated Venus coefficient.
+ public static var venusCarbonDioxideNitrogen: Self {
+ try! Self(gasIdentifier: "venus-co2-n2-96.5-3.5-mole",
+ moleFractions: [.carbonDioxide: 0.965, .nitrogen: 0.035])
+ }
+}
+
+/// Cold-wall enthalpy-form mixture approximation q=K sqrt(pStag[atm]/R) hEdge.
+/// Requires caller-supplied shock-layer pressure/enthalpy; wall enthalpy is neglected.
+public struct SuttonGravesMixtureHeating: ConvectiveHeatingModel {
+ public let parameters: SuttonGravesMixtureParameters
+ public let coverage: StagnationHeatingCoverage
+ public init(parameters: SuttonGravesMixtureParameters, coverage: StagnationHeatingCoverage) {
+ self.parameters = parameters; self.coverage = coverage
+ }
+ public func heatFlux(for query: StagnationHeatingQuery) throws -> SurfaceHeatFlux {
+ guard query.gasIdentifier == parameters.gasIdentifier, query.wall == nil else { throw FluidError.unsupportedQuery }
+ guard coverage.noseRadiusMetres.contains(query.noseRadiusMetres) else { throw FluidError.outsideCoverage }
+ if query.flow.speedMetresPerSecond == 0 {
+ return try SurfaceHeatFlux(wattsPerSquareMetre: 0, surfacePositionMetres: query.surfacePositionMetres)
+ }
+ guard let state = query.gasState, let mach = query.flow.machNumber,
+ let kn = try query.flow.knudsenNumber(referenceLengthMetres: query.noseRadiusMetres) else {
+ throw FluidError.missingFlowProperty
+ }
+ guard coverage.speedMetresPerSecond.contains(query.flow.speedMetresPerSecond),
+ coverage.densityKilogramsPerCubicMetre.contains(query.flow.densityKilogramsPerCubicMetre),
+ coverage.machNumber.contains(mach), kn <= coverage.maximumKnudsenNumber,
+ (101.325...10_132_500).contains(state.pressurePascals),
+ (2.3e6...116.2e6).contains(state.edgeSpecificEnthalpyJoulesPerKilogram) else { throw FluidError.outsideCoverage }
+ let flux = parameters.enthalpyCoefficient*sqrt((state.pressurePascals/101325)/query.noseRadiusMetres)
+ * state.edgeSpecificEnthalpyJoulesPerKilogram
+ guard flux.isFinite else { throw FluidError.nonFiniteResult }
+ return try SurfaceHeatFlux(wattsPerSquareMetre: flux, surfacePositionMetres: query.surfacePositionMetres)
+ }
+}
diff --git a/Sources/Aerodynamics/TabulatedRarefiedTraction.swift b/Sources/Aerodynamics/TabulatedRarefiedTraction.swift
new file mode 100644
index 0000000..d5a13bd
--- /dev/null
+++ b/Sources/Aerodynamics/TabulatedRarefiedTraction.swift
@@ -0,0 +1,64 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// Supplied continuum/slip/transitional/free-molecular pressure and shear data.
+/// Axes in order: log10(Kn), outward-normal incidence cosine, speed/sqrt(RT), Tw/T.
+/// Pressure is gauge pressure/(rho RT). Shear magnitude/(rho RT) opposes tangential
+/// body-relative velocity. Values must come from a consistent gas/surface dataset;
+/// the table does not extrapolate either asymptotic evaluator into transitional flow.
+public struct TabulatedRarefiedTraction: SurfaceTractionModel {
+ public let gas: FreeMolecularGas
+ public let wallTemperatureKelvin: Double
+ public let pressure: FluidScalarTable
+ public let shear: FluidScalarTable
+ public init(gas: FreeMolecularGas, wallTemperatureKelvin: Double,
+ pressure: FluidScalarTable, shear: FluidScalarTable) throws {
+ guard wallTemperatureKelvin.isFinite, wallTemperatureKelvin > 0,
+ pressure.axes == shear.axes, pressure.valueUnits == "1", shear.valueUnits == "1",
+ pressure.axes.map(\.name) == ["log10Kn","incidenceCosine","speedRatio","wallTemperatureRatio"],
+ pressure.axes.allSatisfy({ $0.units == "1" }),
+ pressure.axes[1].coordinates.first! >= -1, pressure.axes[1].coordinates.last! <= 1,
+ pressure.axes[2].coordinates.first! >= 0, pressure.axes[3].coordinates.first! > 0,
+ shear.values.allSatisfy({ $0 >= 0 }) else { throw FluidError.malformedData }
+ self.gas = gas; self.wallTemperatureKelvin = wallTemperatureKelvin
+ self.pressure = pressure; self.shear = shear
+ }
+ public func traction(panel: FluidSurfacePanel, flow: FluidFlow,
+ referenceLengthMetres: Double) throws -> SurfaceTraction {
+ guard let temperature = flow.temperatureKelvin,
+ let kn = try flow.knudsenNumber(referenceLengthMetres: referenceLengthMetres) else {
+ throw FluidError.missingFlowProperty
+ }
+ let rt = gas.specificGasConstantJoulesPerKilogramKelvin*temperature
+ guard rt.isFinite, rt > 0 else { throw FluidError.nonFiniteResult }
+ let speed = flow.speedMetresPerSecond
+ let cosine = speed == 0 ? 0 : max(-1,min(1,(flow.relativeVelocityMetresPerSecond*panel.outwardNormal).sum()/speed))
+ let coordinates = [log10(kn),cosine,speed/sqrt(rt),wallTemperatureKelvin/temperature]
+ let p = try pressure.value(at: coordinates), tau = try shear.value(at: coordinates)
+ if !panel.exposedToFlow { return try SurfaceTraction(gaugePressurePascals: 0,shearPascals: .zero) }
+ let tangent = fluidCross(panel.outwardNormal,fluidCross(flow.relativeVelocityMetresPerSecond,panel.outwardNormal))
+ let tangentSpeed = fluidNorm(tangent)
+ // A normal/rest query has no defined shear direction. Nonzero table shear is inconsistent.
+ guard tangentSpeed > 1e-12*max(1,speed) || tau == 0 else { throw FluidError.invalidCoefficients }
+ let scale = flow.densityKilogramsPerCubicMetre*rt
+ return try SurfaceTraction(gaugePressurePascals: p*scale,
+ shearPascals: tangentSpeed > 0 ? -tangent/tangentSpeed*(tau*scale) : .zero)
+ }
+}
diff --git a/Sources/Aerodynamics/ThinAirfoil.swift b/Sources/Aerodynamics/ThinAirfoil.swift
index 95aa7d9..2708f63 100644
--- a/Sources/Aerodynamics/ThinAirfoil.swift
+++ b/Sources/Aerodynamics/ThinAirfoil.swift
@@ -19,6 +19,7 @@
import Foundation
public struct ThinSymetricAirfoil : Airfoil {
+ public init() {}
public func liftCoefficient(at alpha: Double, for reynoldsNumber: Double) -> Double {
return 2 * .pi * alpha
}
@@ -54,7 +55,7 @@ public struct ThinCamberedAirfoil : Airfoil {
return 0
}
public func coefficients(at alpha: Double, for reynoldsNumber: Double) -> AirfoilCoefficients {
- return AirfoilCoefficients(lift: 2 * .pi * alpha, drag: 0, moment: 0)
+ return AirfoilCoefficients(lift: cl0 + 2 * .pi * alpha, drag: 0, moment: 0)
}
}
diff --git a/Sources/Aerodynamics/WingAerodynamics.swift b/Sources/Aerodynamics/WingAerodynamics.swift
new file mode 100644
index 0000000..9f21a15
--- /dev/null
+++ b/Sources/Aerodynamics/WingAerodynamics.swift
@@ -0,0 +1,184 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import FluidDynamics
+import Foundation
+
+/// Orthonormal section axes expressed in body axes. Forward points toward the
+/// leading edge, span points section-right, down = forward × span.
+public struct WingSectionAxes: Sendable {
+ public let forward: SIMD3
+ public let span: SIMD3
+ public var down: SIMD3 { fluidCross(forward,span) }
+ public init(forward: SIMD3 = SIMD3(1,0,0), span: SIMD3 = SIMD3(0,1,0)) throws {
+ guard fluidFinite(forward), fluidFinite(span), fluidNorm(forward) > 0, fluidNorm(span) > 0,
+ fluidNorm(forward).isFinite, fluidNorm(span).isFinite else { throw FluidError.invalidGeometry }
+ let x = forward/fluidNorm(forward), y = span/fluidNorm(span)
+ guard abs((x*y).sum()) < 1e-12 else { throw FluidError.invalidGeometry }
+ self.forward = x
+ let orthogonal = y-x*(x*y).sum()
+ self.span = orthogonal/fluidNorm(orthogonal)
+ }
+ /// Positive geometric incidence raises the leading edge in X-forward/Z-down axes.
+ public init(incidenceRadians: Double) throws {
+ guard incidenceRadians.isFinite else { throw FluidError.invalidGeometry }
+ try self.init(forward: SIMD3(cos(incidenceRadians),0,-sin(incidenceRadians)))
+ }
+ public func sectionVector(fromBody vector: SIMD3) -> SIMD3 {
+ SIMD3((vector*forward).sum(),(vector*span).sum(),(vector*down).sum())
+ }
+ public func bodyVector(fromSection vector: SIMD3) -> SIMD3 {
+ forward*vector.x+span*vector.y+down*vector.z
+ }
+}
+
+/// Inputs to a section coefficient model; section flow excludes spanwise velocity.
+/// Deflection is caller-supplied geometry/state, with sign defined by the provider.
+public struct WingSectionQuery: Sendable {
+ public let flow: FluidFlow
+ public let chordMetres: Double
+ public let controlDeflectionRadians: Double
+ public var angleOfAttackRadians: Double? { flow.angleOfAttackRadians }
+ public var machNumber: Double? { flow.machNumber }
+ public func reynoldsNumber() throws -> Double? { try flow.reynoldsNumber(referenceLengthMetres: chordMetres) }
+ public init(flow: FluidFlow, chordMetres: Double, controlDeflectionRadians: Double = 0) throws {
+ guard chordMetres.isFinite, chordMetres > 0, controlDeflectionRadians.isFinite else { throw FluidError.invalidParameter }
+ self.flow = flow; self.chordMetres = chordMetres; self.controlDeflectionRadians = controlDeflectionRadians
+ }
+}
+public protocol WingSectionCoefficientModel: Sendable {
+ /// CL/CD and CM about the segment's supplied moment-reference position.
+ /// Positive lift is section-up; positive moment rotates about section +span.
+ func coefficients(for query: WingSectionQuery) throws -> AirfoilCoefficients
+}
+
+/// Uses a checked polar. Control deflection requires a separate calibrated provider;
+/// it is never silently converted into an incidence change or ignored.
+public struct AirfoilWingSectionModel: WingSectionCoefficientModel {
+ public let airfoil: any AirfoilCoefficientModel
+ public init(airfoil: any AirfoilCoefficientModel) { self.airfoil = airfoil }
+ public func coefficients(for query: WingSectionQuery) throws -> AirfoilCoefficients {
+ guard query.controlDeflectionRadians == 0 else { throw FluidError.unsupportedQuery }
+ guard let angle = query.angleOfAttackRadians, let mach = query.machNumber,
+ let re = try query.reynoldsNumber() else { throw FluidError.missingFlowProperty }
+ return try airfoil.coefficients(angleOfAttackRadians: angle,reynoldsNumber: re,machNumber: mach)
+ }
+}
+
+/// One aerodynamic strip, not a vehicle-system component. Coefficient CM and
+/// physical strip position must refer to the same moment reference (e.g. quarter chord).
+public struct WingSegment: Sendable {
+ public let positionMetres: SIMD3
+ public let axes: WingSectionAxes
+ public let chordMetres: Double
+ public let areaSquareMetres: Double
+ public let controlDeflectionRadians: Double
+ public let model: any WingSectionCoefficientModel
+ public init(positionMetres: SIMD3, axes: WingSectionAxes, chordMetres: Double,
+ areaSquareMetres: Double, controlDeflectionRadians: Double = 0,
+ model: any WingSectionCoefficientModel) throws {
+ guard fluidFinite(positionMetres), chordMetres.isFinite, chordMetres > 0,
+ areaSquareMetres.isFinite, areaSquareMetres > 0, controlDeflectionRadians.isFinite else {
+ throw FluidError.invalidGeometry
+ }
+ self.positionMetres = positionMetres; self.axes = axes; self.chordMetres = chordMetres
+ self.areaSquareMetres = areaSquareMetres; self.controlDeflectionRadians = controlDeflectionRadians; self.model = model
+ }
+ public func evaluate(bodyFlow: FluidFlow) throws -> WingSegmentResult {
+ let v = axes.sectionVector(fromBody: bodyFlow.relativeVelocityMetresPerSecond)
+ let flow = try FluidFlow(relativeVelocityMetresPerSecond: SIMD3(v.x,0,v.z),
+ densityKilogramsPerCubicMetre: bodyFlow.densityKilogramsPerCubicMetre,
+ pressurePascals: bodyFlow.pressurePascals,temperatureKelvin: bodyFlow.temperatureKelvin,
+ speedOfSoundMetresPerSecond: bodyFlow.speedOfSoundMetresPerSecond,
+ dynamicViscosityPascalSeconds: bodyFlow.dynamicViscosityPascalSeconds,meanFreePathMetres: bodyFlow.meanFreePathMetres)
+ // Zero chord-plane flow or zero density contributes no aerodynamic load;
+ // do not query a coefficient model at undefined incidence or Reynolds zero.
+ guard flow.dynamicPressurePascals > 0 else {
+ return WingSegmentResult(sectionFlow: flow,coefficients: nil,
+ loads: try FluidLoads(forceNewtons: .zero,momentNewtonMetres: .zero,referencePointMetres: positionMetres))
+ }
+ let query = try WingSectionQuery(flow: flow,chordMetres: chordMetres,controlDeflectionRadians: controlDeflectionRadians)
+ let c = try model.coefficients(for: query)
+ guard c.isFinite else { throw FluidError.invalidCoefficients }
+ let direction = flow.relativeVelocityMetresPerSecond/flow.speedMetresPerSecond
+ let liftDirection = fluidCross(SIMD3(0,1,0),direction)
+ let scale = flow.dynamicPressurePascals*areaSquareMetres
+ guard scale.isFinite else { throw FluidError.nonFiniteResult }
+ let force = axes.bodyVector(fromSection: (liftDirection*c.lift-direction*c.drag)*scale)
+ let moment = axes.span*(scale*c.moment*chordMetres)
+ return WingSegmentResult(sectionFlow: flow,coefficients: c,
+ loads: try FluidLoads(forceNewtons: force,momentNewtonMetres: moment,referencePointMetres: positionMetres))
+ }
+}
+public struct WingSegmentResult: Sendable {
+ public let sectionFlow: FluidFlow
+ /// nil for inactive strips (zero chord-plane dynamic pressure).
+ public let coefficients: AirfoilCoefficients?
+ public let loads: FluidLoads
+}
+public struct SegmentedWingResult: Sendable {
+ public let segments: [WingSegmentResult]
+ public let loads: FluidLoads
+}
+
+/// Independent-strip evaluator. No induced drag, downwash, wake or finite-wing
+/// correction is inferred. Supply corrected local flow or a suitable section model.
+public struct SegmentedWing: Sendable {
+ public let segments: [WingSegment]
+ public init(segments: [WingSegment]) throws {
+ guard !segments.isEmpty else { throw FluidError.invalidGeometry }
+ self.segments = segments
+ }
+ /// Uniform rectangular geometry centred on its supplied section-moment-reference line.
+ /// Positions are body axes; incidence rotates each section, not the spanwise positions.
+ public static func rectangular(spanMetres: Double, chordMetres: Double, segmentCount: Int = 8,
+ centreMetres: SIMD3 = .zero, incidenceRadians: Double = 0,
+ model: any WingSectionCoefficientModel) throws -> Self {
+ guard spanMetres.isFinite, spanMetres > 0, chordMetres.isFinite, chordMetres > 0,
+ segmentCount > 0, segmentCount <= 65536, fluidFinite(centreMetres) else { throw FluidError.invalidGeometry }
+ let width = spanMetres/Double(segmentCount), axes = try WingSectionAxes(incidenceRadians: incidenceRadians)
+ return try Self(segments: (0.. = .zero,
+ flowAtSegment: (WingSegment) throws -> FluidFlow) throws -> SegmentedWingResult {
+ var total = try FluidLoads(forceNewtons: .zero,momentNewtonMetres: .zero,referencePointMetres: momentReferencePointMetres)
+ var results = [WingSegmentResult]()
+ for segment in segments {
+ let result = try segment.evaluate(bodyFlow: flowAtSegment(segment))
+ total = try total.adding(result.loads); results.append(result)
+ }
+ return SegmentedWingResult(segments: results,loads: total)
+ }
+ /// Uniform or rigidly rotating medium convenience. Flow's linear velocity is measured at the stated
+ /// velocity reference point; both rates use the same reference frame and body axes.
+ public func evaluate(flow: FluidFlow, angularVelocityRadiansPerSecond: SIMD3 = .zero,
+ mediumAngularVelocityRadiansPerSecond: SIMD3 = .zero,
+ velocityReferencePointMetres: SIMD3 = .zero,
+ momentReferencePointMetres: SIMD3 = .zero) throws -> SegmentedWingResult {
+ guard fluidFinite(angularVelocityRadiansPerSecond), fluidFinite(velocityReferencePointMetres) else { throw FluidError.invalidFlow }
+ return try evaluate(momentReferencePointMetres: momentReferencePointMetres) {
+ try flow.atLocalPoint(offsetMetres: $0.positionMetres-velocityReferencePointMetres,
+ angularVelocityRadiansPerSecond: angularVelocityRadiansPerSecond,
+ mediumAngularVelocityRadiansPerSecond: mediumAngularVelocityRadiansPerSecond)
+ }
+ }
+}
diff --git a/Sources/Atmospheres/Atmosphere.swift b/Sources/Atmospheres/Atmosphere.swift
new file mode 100644
index 0000000..5f2ce71
--- /dev/null
+++ b/Sources/Atmospheres/Atmosphere.swift
@@ -0,0 +1,54 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2023 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Foundation
+
+/// Legacy scalar queries: altitude in metres, results in SI units.
+public protocol Atmosphere {
+ func pressure(at altitude: Double) -> Double
+ func temperature(at altitude: Double) -> Double
+ func density(at altitude: Double) -> Double
+ func speedOfSound(at altitude: Double) -> Double
+ func dynamicViscosity(at altitude: Double) -> Double
+}
+
+public extension Atmosphere {
+ func kinematicViscosity(at altitude: Double) -> Double {
+ return dynamicViscosity(at: altitude)/density(at: altitude)
+ }
+}
+
+/// Compatibility facade for ISA. All values use SI (K, Pa, kg/m³, m/s, Pa s).
+/// Out-of-coverage and nonfinite altitudes return NaN; use ISAAtmosphere for checked queries.
+public struct EarthAtmosphere: Atmosphere {
+ public init() {}
+ private func sample(_ altitude: Double) -> AtmosphericProperties? {
+ try? ISAAtmosphere().properties(at: altitude)
+ }
+ public func pressure(at altitude: Double) -> Double { sample(altitude)?.pressurePascals ?? .nan }
+ public func temperature(at altitude: Double) -> Double { sample(altitude)?.temperatureKelvin ?? .nan }
+ public func density(at altitude: Double) -> Double { sample(altitude)?.densityKilogramsPerCubicMetre ?? .nan }
+ public func speedOfSound(at altitude: Double) -> Double { sample(altitude)?.speedOfSoundMetresPerSecond ?? .nan }
+ public func dynamicViscosity(at altitude: Double) -> Double { sample(altitude)?.dynamicViscosityPascalSeconds ?? .nan }
+}
+
+extension Atmosphere {
+ func reynoldsNumber(at altitude: Double, forLength length: Double, atVelocity velocity: Double) -> Double {
+ // Re = density * velocity * length / viscosity
+ return self.density(at: altitude) * velocity * length / self.dynamicViscosity(at: altitude)
+ }
+}
diff --git a/Sources/Atmospheres/AtmosphereCatalogue.swift b/Sources/Atmospheres/AtmosphereCatalogue.swift
new file mode 100644
index 0000000..c15daa2
--- /dev/null
+++ b/Sources/Atmospheres/AtmosphereCatalogue.swift
@@ -0,0 +1,95 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Foundation
+
+/// Body centres use NAIF IDs; system barycentres deliberately have no profile.
+public enum AtmosphericBody: Int32, CaseIterable, Sendable {
+ case venus = 299, earth = 399, mars = 499, jupiter = 599, saturn = 699
+ case uranus = 799, neptune = 899, titan = 606, triton = 801, io = 501, callisto = 504
+}
+public enum AtmosphericRegime: Sendable { case continuum, tenuous, exosphere }
+
+/// Fixed nominal profiles, not forecasts or mission-grade entry models.
+public struct BodyAtmosphere: AtmosphericProfile {
+ public let body: AtmosphericBody
+ public let regime: AtmosphericRegime
+ private let profile: any AtmosphericProfile
+ public var altitudeRangeMetres: ClosedRange { profile.altitudeRangeMetres }
+ public var altitudeDatum: String { profile.altitudeDatum }
+ public var source: String { profile.source }
+ public var assumptions: String { profile.assumptions }
+ private init(body: AtmosphericBody, regime: AtmosphericRegime = .continuum, profile: any AtmosphericProfile) {
+ self.body = body; self.regime = regime; self.profile = profile
+ }
+ public func properties(at altitudeMetres: Double) throws -> AtmosphericProperties {
+ try profile.properties(at: altitudeMetres)
+ }
+ public static func model(for body: AtmosphericBody) -> BodyAtmosphere {
+ if body == .earth { return BodyAtmosphere(body: body, profile: ISAAtmosphere()) }
+ let r = 8314.46261815324 // Universal gas constant divided by molar mass in g/mol.
+ let fact = "https://nssdc.gsfc.nasa.gov/planetary/factsheet/"
+ var pressure: Double, temperature: Double, molecularMass: Double, gravity: Double
+ var gamma: Double? = 1.4, top = 100_000.0, regime = AtmosphericRegime.continuum
+ var source: String
+ var levels: [HydrostaticAtmosphere.TemperatureLevel]
+ var datum = "Metres above nominal mean surface"
+ var assumptions = "Nominal isothermal ideal gas, constant gravity and composition; no weather, winds, seasons or escape. Coverage is a chosen simulation bound, not a measured atmospheric edge. Viscosity unavailable."
+ switch body {
+ case .venus: (pressure,temperature,molecularMass,gravity) = (9.2e6,737,43.45,8.87); gamma = 1.3; source = fact+"venusfact.html"
+ case .mars: (pressure,temperature,molecularMass,gravity) = (636,214,43.49,3.73); gamma = 1.3; source = fact+"marsfact.html"
+ case .titan: (pressure,temperature,molecularMass,gravity) = (1.5e5,94,28.0,1.352); source = "https://www.nasa.gov/wp-content/uploads/2015/04/niac_sunspiral_superballbot_phaseii_finalreport_tagged.pdf"
+ case .triton: (pressure,temperature,molecularMass,gravity) = (1.4,38,28.0,0.779); regime = .tenuous; source = "https://ntrs.nasa.gov/citations/19950012719"
+ case .io: (pressure,temperature,molecularMass,gravity) = (1e-4,150,64.066,1.796); gamma = nil; regime = .tenuous; top = 50_000; source = "https://doi.org/10.1006/icar.1996.0186"
+ assumptions += " Io SO2 pressure is order-of-magnitude only; 150 K is a chosen nominal gas temperature. Volcanism and eclipse collapse omitted; continuum transport unavailable."
+ case .callisto: (pressure,temperature,molecularMass,gravity) = (7.5e-7,150,44.01,1.236); gamma = nil; regime = .exosphere; source = "https://doi.org/10.1126/science.283.5403.820"
+ assumptions += " Historical CO2 component only; pressure is an equivalent number-density measure. Exponential density is a proxy, not a collisional hydrostatic atmosphere; no sound or continuum transport."
+ case .jupiter: (pressure,temperature,molecularMass,gravity) = (1e5,165,2.22,24.79); source = fact+"jupiterfact.html"
+ case .saturn: (pressure,temperature,molecularMass,gravity) = (1e5,134,2.07,10.44); source = fact+"saturnfact.html"
+ case .uranus: (pressure,temperature,molecularMass,gravity) = (1e5,76,2.64,8.87); source = fact+"uranusfact.html"
+ case .neptune: (pressure,temperature,molecularMass,gravity) = (1e5,72,2.60,11.15); source = fact+"neptunefact.html"
+ case .earth: preconditionFailure("Handled above")
+ }
+ let gasConstant = r/molecularMass
+ if [.jupiter,.saturn,.uranus,.neptune].contains(body) {
+ // Dry ideal diatomic adiabat below 1 bar, limited to 100 bar.
+ let lapse = -gravity*(1.4-1)/1.4/gasConstant
+ let deepTemperature = temperature*pow(100,(1.4-1)/1.4)
+ let bottom = (deepTemperature-temperature)/lapse
+ let upperTemperature: Double
+ switch body { case .jupiter: upperTemperature = 112; case .saturn: upperTemperature = 84
+ case .uranus: upperTemperature = 53; default: upperTemperature = 55 }
+ // Linear temperature layer calibrated to the published 0.1-bar temperature.
+ let upperHeight = gasConstant/gravity*(temperature-upperTemperature)
+ / log(temperature/upperTemperature)*log(10)
+ levels = [(bottom,deepTemperature),(0,temperature),(upperHeight,upperTemperature),
+ (upperHeight+5*gasConstant*upperTemperature/gravity,upperTemperature)]
+ .map { .init(altitudeMetres: $0.0, temperatureKelvin: $0.1) }
+ datum = "Metres above the 1-bar level; negative altitudes descend into the clouds, no solid surface"
+ assumptions = "Ideal gas with constant gravity/composition; dry gamma=1.4 adiabat from 1 to 100 bar, linear temperature fit from 1 to 0.1 bar, then isothermal. No cloud microphysics, winds, condensation or deep interior equation of state. Coverage is a simulation bound. Viscosity unavailable."
+ } else {
+ levels = [(0.0,temperature),(top,temperature)].map { .init(altitudeMetres: $0.0, temperatureKelvin: $0.1) }
+ }
+ return BodyAtmosphere(body: body, regime: regime, profile: try! HydrostaticAtmosphere(levels: levels,
+ referencePressurePascals: pressure, specificGasConstant: gasConstant,
+ gravityMetresPerSecondSquared: gravity, heatCapacityRatio: gamma,
+ altitudeDatum: datum, source: source, assumptions: assumptions))
+ }
+ public static func model(naifBodyCode: Int32) -> BodyAtmosphere? {
+ AtmosphericBody(rawValue: naifBodyCode).map { model(for: $0) }
+ }
+}
diff --git a/Sources/Atmospheres/Atmospheres.docc/Atmospheres.md b/Sources/Atmospheres/Atmospheres.docc/Atmospheres.md
new file mode 100644
index 0000000..0cd4a39
--- /dev/null
+++ b/Sources/Atmospheres/Atmospheres.docc/Atmospheres.md
@@ -0,0 +1,17 @@
+# ``Atmospheres``
+
+Bounded SI atmospheric profiles for planets and moons.
+
+Evaluate Earth ISA, nominal body atmospheres or custom hydrostatic profiles with
+explicit altitude datums, coverage and physical assumptions.
+
+## Topics
+
+### Using atmospheric models
+-
+- ``AtmosphericProfile``
+- ``AtmosphericProperties``
+- ``ISAAtmosphere``
+- ``HydrostaticAtmosphere``
+- ``BodyAtmosphere``
+- ``EarthAtmosphere``
diff --git a/Sources/Atmospheres/Atmospheres.docc/Guide.md b/Sources/Atmospheres/Atmospheres.docc/Guide.md
new file mode 100644
index 0000000..ec30cad
--- /dev/null
+++ b/Sources/Atmospheres/Atmospheres.docc/Guide.md
@@ -0,0 +1,55 @@
+# Atmospheres
+
+Swift target with no external dependencies. Import `Atmospheres` via
+swift-celmek's `Atmospheres` or `Physics` product.
+
+```swift
+import Atmospheres
+let earth = ISAAtmosphere()
+let seaLevel = try earth.properties(at: 0) // Pa, K, kg/m³, m/s, Pa s
+let jupiter = BodyAtmosphere.model(for: .jupiter)
+let belowClouds = try jupiter.properties(at: -50_000) // below the 1-bar datum
+```
+
+Earth uses dry-air ISA/US Standard Atmosphere 1976 lower layers, through 84.852 km
+geopotential height, converting geometric input altitude internally. All profiles
+throw outside their explicit coverage; coverage is not an atmospheric edge or a
+promise of vacuum above it. Custom `HydrostaticAtmosphere` profiles accept increasing
+temperature levels and a reference pressure at one of those levels.
+
+Built-ins cover Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Titan, Triton,
+Io and Callisto. Non-Earth solid-body profiles are **nominal isothermal approximations**;
+they reproduce a reference state, not a measured vertical temperature profile.
+Gas giants fit the published 1-bar and 0.1-bar temperatures with a hydrostatic
+linear-temperature layer, a dry adiabat below 1 bar (limited to 100 bar), and an
+isothermal upper extension. Neither cloud microphysics nor deep interiors are modeled.
+
+Io is highly variable; its pressure is an order-of-magnitude nominal value, with a
+chosen 150 K gas temperature. Callisto represents the historically observed CO2
+component as an exponential exosphere proxy. Its pressure is equivalent kinetic
+pressure; continuum sound speed and viscosity are absent. Non-Earth viscosity is
+unavailable rather than guessed. These fixed profiles omit latitude, seasons, solar
+activity, winds, plumes and atmospheric escape. Additional moons can be represented
+with custom profiles; no poorly constrained defaults are silently supplied.
+
+Every model exposes its source URL, assumptions, altitude datum and coverage.
+Reference data: [NASA planetary factsheets](https://nssdc.gsfc.nasa.gov/planetary/factsheet/),
+[US Standard Atmosphere 1976](https://ntrs.nasa.gov/citations/19770009539),
+[Titan nominal reference](https://www.nasa.gov/wp-content/uploads/2015/04/niac_sunspiral_superballbot_phaseii_finalreport_tagged.pdf),
+[Triton reference](https://ntrs.nasa.gov/citations/19950012719),
+[Io review](https://doi.org/10.1006/icar.1996.0186),
+[Callisto CO2 observation](https://doi.org/10.1126/science.283.5403.820).
+
+For CelMek, `BodyIdentifier.earth.atmosphericModel` returns the built-in profile.
+`SphericalBodyAtmosphere` adapts a profile to `AtmosphericDrag`. Supply a compatible
+body-centred inertial frame, the radius of the profile's datum (1 bar for giants),
+and optionally angular velocity in those axes. It computes density and co-rotation;
+it neither transforms frames nor obtains ephemerides. Exosphere density should be
+paired with a suitable rarefied-gas force model rather than assumed continuum drag.
+
+Migration: `EarthAtmosphere` remains accessible through `import Aerodynamics`.
+Its formerly incorrect scalar results now use SI: Kelvin rather than Celsius,
+pressure in Pa, density in kg/m³ and viscosity in Pa s (about 1.789e-5 at sea level).
+Legacy scalar queries return NaN outside coverage; prefer the throwing profile API.
+
+Run `swift test --filter ProfileTests` from the repository root.
diff --git a/Sources/Atmospheres/AtmosphericProfile.swift b/Sources/Atmospheres/AtmosphericProfile.swift
new file mode 100644
index 0000000..29190be
--- /dev/null
+++ b/Sources/Atmospheres/AtmosphericProfile.swift
@@ -0,0 +1,151 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Foundation
+
+public enum AtmosphericModelError: Error, Equatable {
+ case invalidParameters, altitudeOutsideCoverage, nonFiniteResult
+}
+
+/// SI properties. Optional transport quantities are absent where no continuum model is supplied.
+public struct AtmosphericProperties: Sendable {
+ public let pressurePascals: Double
+ public let temperatureKelvin: Double
+ public let densityKilogramsPerCubicMetre: Double
+ public let speedOfSoundMetresPerSecond: Double?
+ public let dynamicViscosityPascalSeconds: Double?
+}
+
+/// Altitude is measured in metres above the explicitly described datum.
+public protocol AtmosphericProfile: Sendable {
+ var altitudeRangeMetres: ClosedRange { get }
+ var altitudeDatum: String { get }
+ var source: String { get }
+ var assumptions: String { get }
+ func properties(at altitudeMetres: Double) throws -> AtmosphericProperties
+}
+
+/// Piecewise linear temperature with constant gravity and molecular composition.
+/// Pressure is integrated analytically from hydrostatic balance; density uses the ideal gas law.
+public struct HydrostaticAtmosphere: AtmosphericProfile {
+ public struct TemperatureLevel: Sendable {
+ public let altitudeMetres: Double
+ public let temperatureKelvin: Double
+ public init(altitudeMetres: Double, temperatureKelvin: Double) {
+ self.altitudeMetres = altitudeMetres; self.temperatureKelvin = temperatureKelvin
+ }
+ }
+ public let altitudeRangeMetres: ClosedRange
+ public let altitudeDatum: String
+ public let source: String
+ public let assumptions: String
+ public let specificGasConstant: Double
+ public let gravityMetresPerSecondSquared: Double
+ public let heatCapacityRatio: Double?
+ private let levels: [TemperatureLevel]
+ private let logPressures: [Double]
+
+ public init(levels: [TemperatureLevel], referenceAltitudeMetres: Double = 0,
+ referencePressurePascals: Double, specificGasConstant: Double,
+ gravityMetresPerSecondSquared: Double, heatCapacityRatio: Double? = nil,
+ altitudeDatum: String, source: String, assumptions: String) throws {
+ guard levels.count >= 2,
+ levels.allSatisfy({ $0.altitudeMetres.isFinite && $0.temperatureKelvin.isFinite && $0.temperatureKelvin > 0 }),
+ zip(levels, levels.dropFirst()).allSatisfy({ $0.altitudeMetres < $1.altitudeMetres }),
+ [referencePressurePascals, specificGasConstant, gravityMetresPerSecondSquared].allSatisfy({ $0.isFinite && $0 > 0 }),
+ heatCapacityRatio.map({ $0.isFinite && $0 > 1 }) ?? true,
+ !altitudeDatum.isEmpty, !source.isEmpty,
+ let referenceIndex = levels.firstIndex(where: { $0.altitudeMetres == referenceAltitudeMetres }) else {
+ throw AtmosphericModelError.invalidParameters
+ }
+ self.levels = levels; self.specificGasConstant = specificGasConstant
+ self.gravityMetresPerSecondSquared = gravityMetresPerSecondSquared
+ self.heatCapacityRatio = heatCapacityRatio; self.altitudeDatum = altitudeDatum
+ self.source = source; self.assumptions = assumptions
+ altitudeRangeMetres = levels.first!.altitudeMetres...levels.last!.altitudeMetres
+ var integrals = [0.0]
+ for i in 1.. Double {
+ let difference = temperature-baseTemperature
+ if abs(difference) < 1e-10 * baseTemperature {
+ return -gravityOverR * height/baseTemperature
+ }
+ return -gravityOverR * height/difference * log1p(difference/baseTemperature)
+ }
+
+ public func properties(at altitudeMetres: Double) throws -> AtmosphericProperties {
+ guard altitudeMetres.isFinite, altitudeRangeMetres.contains(altitudeMetres) else {
+ throw AtmosphericModelError.altitudeOutsideCoverage
+ }
+ let i = min(levels.lastIndex(where: { $0.altitudeMetres <= altitudeMetres })!, levels.count-2)
+ let lower = levels[i], upper = levels[i+1]
+ let height = altitudeMetres-lower.altitudeMetres
+ let temperature = lower.temperatureKelvin + (upper.temperatureKelvin-lower.temperatureKelvin)
+ * height/(upper.altitudeMetres-lower.altitudeMetres)
+ let pressure = exp(logPressures[i] + Self.logPressureRatio(height: height,
+ baseTemperature: lower.temperatureKelvin, temperature: temperature,
+ gravityOverR: gravityMetresPerSecondSquared/specificGasConstant))
+ let density = pressure/specificGasConstant/temperature
+ let sound = heatCapacityRatio.map { sqrt($0*specificGasConstant*temperature) }
+ guard pressure.isFinite, pressure > 0, density.isFinite, density > 0,
+ sound.map(\.isFinite) ?? true else { throw AtmosphericModelError.nonFiniteResult }
+ return AtmosphericProperties(pressurePascals: pressure, temperatureKelvin: temperature,
+ densityKilogramsPerCubicMetre: density, speedOfSoundMetresPerSecond: sound,
+ dynamicViscosityPascalSeconds: nil)
+ }
+}
+
+/// ISA dry-air layers through 84.852 km geopotential altitude (about 86 km geometric).
+public struct ISAAtmosphere: AtmosphericProfile {
+ public let altitudeDatum = "Geometric altitude above mean sea level; internally converted to geopotential height"
+ public let source = "https://ntrs.nasa.gov/citations/19770009539"
+ public let assumptions = "ISA/US Standard Atmosphere lower layers; dry ideal air, no weather or thermosphere"
+ public let altitudeRangeMetres = -500.0...(6_356_766 * 84_852 / (6_356_766 - 84_852))
+ private static let profile = try! HydrostaticAtmosphere(
+ levels: [(-1000.0,294.65),(0,288.15),(11000,216.65),(20000,216.65),
+ (32000,228.65),(47000,270.65),(51000,270.65),(71000,214.65),(84852,186.946)]
+ .map { .init(altitudeMetres: $0.0, temperatureKelvin: $0.1) },
+ referencePressurePascals: 101325, specificGasConstant: 287.05287,
+ gravityMetresPerSecondSquared: 9.80665, heatCapacityRatio: 1.4,
+ altitudeDatum: "Geopotential height", source: "US Standard Atmosphere 1976", assumptions: "Dry air")
+ public init() {}
+ public func properties(at altitudeMetres: Double) throws -> AtmosphericProperties {
+ guard altitudeMetres.isFinite, altitudeRangeMetres.contains(altitudeMetres) else {
+ throw AtmosphericModelError.altitudeOutsideCoverage
+ }
+ let h = 6_356_766*altitudeMetres/(6_356_766+altitudeMetres)
+ let result = try Self.profile.properties(at: min(84852, h))
+ let t = result.temperatureKelvin
+ // Sutherland's law for dry air, Pa s.
+ let viscosity = 1.458e-6 * pow(t,1.5)/(t+110.4)
+ return AtmosphericProperties(pressurePascals: result.pressurePascals,
+ temperatureKelvin: t, densityKilogramsPerCubicMetre: result.densityKilogramsPerCubicMetre,
+ speedOfSoundMetresPerSecond: result.speedOfSoundMetresPerSecond,
+ dynamicViscosityPascalSeconds: viscosity)
+ }
+}
diff --git a/Sources/CelMek/AccuracyLevel.swift b/Sources/CelMek/AccuracyLevel.swift
new file mode 100644
index 0000000..b5a83c5
--- /dev/null
+++ b/Sources/CelMek/AccuracyLevel.swift
@@ -0,0 +1,43 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+
+/// A tolerance hint: models may use a higher accuracy than requested.
+/// Shared caller intent, not a universal physical error bound or runtime guarantee.
+/// Each algorithm must document its settings, supported intervals and measured error.
+public enum AccuracyLevel: String, CaseIterable, Hashable, Sendable {
+ /// Prioritize computational cost, allowing the model's largest supported approximation.
+ case low
+ /// A model-specific compromise between computational cost and approximation error.
+ case balanced
+ /// Prefer smaller approximation error while permitting documented simplifications.
+ case high
+ /// Complete evaluation of the implemented model, including any intrinsic truncation.
+ /// Does not imply exact physics, full original published theory, or the newest data.
+ case full
+}
+
+/// Opt-in contract reporting requested hints and effective evaluation modes. Algorithm-specific
+/// controls (such as derivative intervals and TDB models) remain explicit and independent.
+public protocol AccuracyAwareEphemerisProvider: EphemerisProvider {
+ /// Requested tolerance hint.
+ var accuracy: AccuracyLevel { get }
+ /// Actual model mode; may be more accurate than the hint.
+ var effectiveAccuracy: AccuracyLevel { get }
+ /// Implemented evaluation modes, not a restriction on accepted hints.
+ var availableAccuracyLevels: Set { get }
+}
diff --git a/Sources/CelMek/AdaptiveWaypointTimingSearch.swift b/Sources/CelMek/AdaptiveWaypointTimingSearch.swift
new file mode 100644
index 0000000..05534b4
--- /dev/null
+++ b/Sources/CelMek/AdaptiveWaypointTimingSearch.swift
@@ -0,0 +1,138 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Math
+
+public struct WaypointTimingRefinementOptions: Equatable, Sendable {
+ public let initialSpacingSeconds, minimumSpacingSeconds: Double
+ public let maximumRounds, maximumCandidateEvaluations, maximumGeneratedCandidates: Int
+ public init(initialSpacingSeconds: Double, minimumSpacingSeconds: Double,
+ maximumRounds: Int = 8, maximumCandidateEvaluations: Int = 1000,
+ maximumGeneratedCandidates: Int = 100_000) throws {
+ guard initialSpacingSeconds.isFinite, minimumSpacingSeconds.isFinite,
+ minimumSpacingSeconds > 0, initialSpacingSeconds >= minimumSpacingSeconds else {
+ throw WaypointTimingSearchError.invalidCandidateSpacing
+ }
+ guard (1...32).contains(maximumRounds), (1...10_000).contains(maximumCandidateEvaluations),
+ (1...100_000).contains(maximumGeneratedCandidates) else { throw WaypointTimingSearchError.invalidBudget }
+ self.initialSpacingSeconds = initialSpacingSeconds; self.minimumSpacingSeconds = minimumSpacingSeconds
+ self.maximumRounds = maximumRounds; self.maximumCandidateEvaluations = maximumCandidateEvaluations
+ self.maximumGeneratedCandidates = maximumGeneratedCandidates
+ }
+}
+public enum WaypointTimingRefinementStatus: Equatable, Sendable {
+ case feasible, resolutionLimitReached, evaluationLimitReached
+ case refinementLimitReached, candidateGenerationLimitReached
+}
+public struct WaypointTimingRefinementRound {
+ public let spacingSeconds: Double
+ public let generatedCandidates: Int
+ public let evaluatedCandidates: Int
+ public let status: WaypointTimingSearchStatus
+}
+public struct WaypointTimingRefinementResult {
+ public let status: WaypointTimingRefinementStatus
+ public let evaluatedCandidates: Int
+ public let rounds: [WaypointTimingRefinementRound]
+ public let route: WaypointBrachistochroneRoute?
+ public let propagation: WaypointRoutePropagationResult?
+ public let failedAttempts: [WaypointTimingAttempt]
+}
+
+extension WaypointRouteTimingPlanner {
+ /// Refine the grid only after its candidates fail. Halving spacing retains
+ /// phase boundaries and avoids replaying previously rejected combinations.
+ /// This searches for feasibility, not a minimum-time or continuous optimum.
+ public static func adaptiveSearch(departureEpoch: Epoch, frame: Frame, origin: BodyIdentifier,
+ waypoints: [BrachistochroneWaypoint], legAccelerationsMetresPerSecondSquared: [Double],
+ arrivalWindows: [ClosedRange], refinementOptions: WaypointTimingRefinementOptions,
+ initialMass: SpacecraftMassProperties, backgroundDynamics: SpacecraftDynamics,
+ legEngineLimits: [WaypointRouteEngineLimits], timedEnginePhases: [WaypointRouteEnginePhase] = [],
+ obstacles: [SphericalExclusionRegion] = [],
+ numericalOptions: NumericalPropagationOptions = try! NumericalPropagationOptions(),
+ endpointPositionToleranceMetres: Double = 0.01,
+ endpointVelocityToleranceMetresPerSecond: Double = 1e-5,
+ movingTarget: MovingWaypointRouteTarget? = nil,
+ movingWaypoints: [Int: MovingWaypointPassage] = [:],
+ movingObstacles: [MovingSphericalExclusionRegion] = [],
+ physicalConstraints: WaypointRoutePhysicalConstraints = .unconstrained) throws -> WaypointTimingRefinementResult {
+ guard (2...10_001).contains(waypoints.count), arrivalWindows.count == waypoints.count-1 else {
+ throw WaypointTimingSearchError.invalidCandidates
+ }
+ _ = try validateTimingConfiguration(departureEpoch: departureEpoch, frame: frame, origin: origin,
+ waypoints: waypoints, legAccelerationsMetresPerSecondSquared: legAccelerationsMetresPerSecondSquared,
+ backgroundDynamics: backgroundDynamics, legEngineLimits: legEngineLimits,
+ timedEnginePhases: timedEnginePhases, obstacles: obstacles,
+ endpointPositionToleranceMetres: endpointPositionToleranceMetres,
+ endpointVelocityToleranceMetresPerSecond: endpointVelocityToleranceMetresPerSecond, movingTarget: movingTarget, movingWaypoints: movingWaypoints, movingObstacles: movingObstacles, physicalConstraints: physicalConstraints)
+ var windows = try intersectPassageCoverage(arrivalWindows, movingWaypoints: movingWaypoints)
+ for index in windows.indices {
+ if let constraint = waypoints[index+1].arrivalWindow {
+ let lower = max(windows[index].lowerBound, constraint.lowerBound)
+ let upper = min(windows[index].upperBound, constraint.upperBound)
+ guard lower <= upper else { throw WaypointTimingSearchError.invalidCandidates }
+ windows[index] = lower...upper
+ }
+ }
+ if let movingTarget {
+ let last = windows.count-1
+ let lower = max(windows[last].lowerBound, movingTarget.coverage.lowerBound)
+ let upper = min(windows[last].upperBound, movingTarget.coverage.upperBound)
+ guard lower <= upper else { throw WaypointTimingSearchError.invalidCandidates }
+ windows[last] = lower...upper
+ }
+ var spacing = refinementOptions.initialSpacingSeconds
+ var failures: [WaypointTimingAttempt] = [], rounds: [WaypointTimingRefinementRound] = []
+ var evaluated = 0, excluded = Set<[Epoch]>()
+ func finish(_ status: WaypointTimingRefinementStatus,
+ _ success: WaypointTimingSearchResult? = nil) -> WaypointTimingRefinementResult {
+ WaypointTimingRefinementResult(status: status, evaluatedCandidates: evaluated, rounds: rounds,
+ route: success?.route, propagation: success?.propagation, failedAttempts: failures)
+ }
+ for _ in 0.. { Set(AccuracyLevel.allCases) }
+ public let coefficientSelection: VSOP87CoefficientSelection
+ private let provider: VSOP87StateProvider
+ public init(body: vsop87_body, coverage: ClosedRange, tdbModel: any TDBTimeModel, accuracy: AccuracyLevel = .full) throws {
+ self.accuracy = accuracy
+ guard coverage.lowerBound >= tdbModel.coverage.lowerBound,
+ coverage.upperBound <= tdbModel.coverage.upperBound else { throw EphemerisError.outsideCoverage }
+ let id: BodyIdentifier
+ switch body.body_id {
+ case .vsop87_sun: id = .sun
+ case .vsop87_mercury: id = .mercury
+ case .vsop87_venus: id = .venus
+ case .vsop87_earth: id = .earth
+ case .vsop87_mars: id = .marsBarycentre
+ case .vsop87_jupiter: id = .jupiterBarycentre
+ case .vsop87_saturn: id = .saturnBarycentre
+ case .vsop87_uranus: id = .uranusBarycentre
+ case .vsop87_neptune: id = .neptuneBarycentre
+ }
+ let selection = try VSOP87CoefficientSelection(body: body,coverage: coverage,tdbModel: tdbModel,accuracy: accuracy)
+ coefficientSelection = selection
+ effectiveAccuracy = selection.retainedTermCount == selection.originalTermCount ? .full : accuracy
+ provider = VSOP87StateProvider(body: selection.selectedBody,tdbModel: tdbModel)
+ metadata = try EphemerisMetadata(body: id,origin: .solarSystemBarycentre,frame: body.frame,
+ coverage: coverage,coverageBasis: .callerSelected,modelTimeScale: .tdb,
+ velocityMethod: .analytic,accelerationMethod: .unavailable,
+ provenance: PhysicalDataProvenance(source: "VSOP87E \(effectiveAccuracy) evaluation, \(selection.retainedTermCount)/\(selection.originalTermCount) terms; \(tdbModel.provenance)",
+ version: "VSOP87",reference: "https://ftp.imcce.fr/pub/ephem/planets/vsop87/"),accuracy: accuracy,effectiveAccuracy: effectiveAccuracy)
+ }
+ public func state(at epoch: Epoch) throws -> CartesianState {
+ guard metadata.coverage.contains(epoch) else { throw EphemerisError.outsideCoverage }
+ return try provider.state(at: epoch)
+ }
+}
+
+/// Native identities for the legacy lunar and Pluto approximations. Retain this
+/// object and register its transforms to query these states in other frames.
+public struct AnalyticEphemerisFrames {
+ public let moonEclipticOfDate: Frame
+ public let plutoEclipticJ2000: Frame
+ internal init(moon: Frame, pluto: Frame) { moonEclipticOfDate = moon; plutoEclipticJ2000 = pluto }
+}
+
+extension FrameTree {
+ /// Earth and Sun states must already be expressed in this tree's ICRF frame.
+ public func makeAnalyticEphemerisFrames(earth: any StateProvider, sun: any StateProvider,
+ accelerationPolicy: OriginAccelerationPolicy = .requireProvided,
+ derivativeStep: Duration = try! Duration(seconds: 60)) throws -> AnalyticEphemerisFrames {
+ guard earth.frame === CelestialFrames.icrf, sun.frame === CelestialFrames.icrf else {
+ throw EphemerisError.frameMismatch
+ }
+ let dated = try MeanEclipticOfDateProvider(step: derivativeStep)
+ let geo = try makeGeocentricFrames(earth: earth,accelerationPolicy: accelerationPolicy)
+ let lunar = try makeFrame(parent: geo.eme2000,name: "Meeus Moon mean ecliptic/equinox of date",provider: dated)
+ let ecliptic = Quaternion(angle: -84381.448 * .pi/(180*3600),axis: SIMD3(1,0,0)) * CelestialFrames.icrfToEME2000
+ let orientation = try FixedAxisOrientationProvider(referenceFrame: CelestialFrames.icrf,axis: SIMD3(1,0,0),
+ rate: 0,initialRotation: ecliptic)
+ let heliocentric = try makeBodyFixedFrame(name: "Goffin heliocentric ecliptic J2000",centre: sun,
+ orientation: orientation,accelerationPolicy: accelerationPolicy)
+ return AnalyticEphemerisFrames(moon: lunar,pluto: heliocentric)
+ }
+}
+
+/// Adapters for the existing truncated lunar and Pluto spherical series. TT is the
+/// legacy ephemeris-time argument. Position coverage is caller selected; query
+/// coverage is shortened by ±2*velocityStep for the five-point Cartesian derivative.
+public struct SphericalAnalyticEphemeris: AccuracyAwareEphemerisProvider {
+ public enum Model: Sendable { case meeusMoon, goffinPluto }
+ public let metadata: EphemerisMetadata
+ public let accuracy: AccuracyLevel
+ public let effectiveAccuracy: AccuracyLevel = .full
+ public var availableAccuracyLevels: Set { [.full] }
+ public let model: Model
+ public let positionCoverage: ClosedRange
+ public let velocityStep: Duration
+ public init(model: Model, frames: AnalyticEphemerisFrames, positionCoverage: ClosedRange,
+ velocityStep: Duration, accuracy: AccuracyLevel = .full) throws {
+ self.accuracy = accuracy
+ guard velocityStep > .zero else { throw EphemerisError.invalidDerivativeMethod }
+ let margin = try velocityStep.adding(velocityStep)
+ let lower = try positionCoverage.lowerBound.advanced(by: margin)
+ let upper = try positionCoverage.upperBound.advanced(by: margin.negated())
+ guard lower <= upper else { throw EphemerisError.outsideCoverage }
+ self.model = model; self.positionCoverage = positionCoverage; self.velocityStep = velocityStep
+ let moon = model == .meeusMoon
+ metadata = try EphemerisMetadata(body: moon ? .moon : .plutoBarycentre,origin: moon ? .earth : .sun,
+ frame: moon ? frames.moonEclipticOfDate : frames.plutoEclipticJ2000,coverage: lower...upper,
+ coverageBasis: .callerSelected,modelTimeScale: .tt,
+ velocityMethod: .finiteDifference(step: velocityStep),accelerationMethod: .unavailable,
+ provenance: PhysicalDataProvenance(source: moon ? "Meeus chapter 47 truncated lunar series, including constant light-time longitude term; legacy elp2000_82b" : "Meeus/Goffin Pluto spherical series; legacy goffin2000",
+ version: "built-in legacy coefficients; TT adapter"),accuracy: accuracy,effectiveAccuracy: effectiveAccuracy)
+ }
+ private func position(at epoch: Epoch) throws -> SIMD3 {
+ guard positionCoverage.contains(epoch) else { throw EphemerisError.outsideCoverage }
+ let t = try centuriesTT(epoch)
+ let spherical = model == .meeusMoon ? meeusMoonPosition(centuries: t) : goffinPosition(centuries: t)
+ let distance = spherical.z * (model == .meeusMoon ? 1 : CartesianUnits.metresPerAstronomicalUnit)
+ return SIMD3(distance*cos(spherical.y)*cos(spherical.x),distance*cos(spherical.y)*sin(spherical.x),distance*sin(spherical.y))
+ }
+ public func state(at epoch: Epoch) throws -> CartesianState {
+ guard metadata.coverage.contains(epoch) else { throw EphemerisError.outsideCoverage }
+ let h = velocityStep.seconds
+ let p = try position(at: epoch)
+ let samples = try [-2.0,-1,1,2].map { try position(at: epoch.advanced(by: Duration(seconds: $0*h))) }
+ let velocity = (samples[0]-8*samples[1]+8*samples[2]-samples[3])/(12*h)
+ return try CartesianState(epoch: epoch,frame: frame,position: p,velocity: velocity)
+ }
+}
+
+internal func centuriesTT(_ epoch: Epoch) throws -> Double {
+ let date = try epoch.julianDate(in: .tt)
+ return (Double(date.wholeDay-2451545)+date.fractionalDay)/36525
+}
+
+/// IAU 1976 precession and IAU 1980 mean obliquity, compatible with the legacy series.
+/// Native Swift; rotation convention follows ERFA pmat76. No nutation is applied.
+internal struct MeanEclipticOfDateProvider: TransformProvider {
+ let step: Duration
+ init(step: Duration) throws {
+ guard step > .zero else { throw EphemerisError.invalidDerivativeMethod }
+ self.step = step
+ }
+ func rotation(at epoch: Epoch) throws -> Quaternion {
+ let t = try centuriesTT(epoch), arcsecond = Double.pi/(180*3600)
+ let zeta = (2306.2181*t+0.30188*t*t+0.017998*t*t*t)*arcsecond
+ let z = (2306.2181*t+1.09468*t*t+0.018203*t*t*t)*arcsecond
+ let theta = (2004.3109*t-0.42665*t*t-0.041833*t*t*t)*arcsecond
+ let eps = (84381.448-46.815*t-0.00059*t*t+0.001813*t*t*t)*arcsecond
+ return Quaternion(angle: -eps,axis: SIMD3(1,0,0)) * Quaternion(angle: z,axis: SIMD3(0,0,1))
+ * Quaternion(angle: -theta,axis: SIMD3(0,1,0)) * Quaternion(angle: zeta,axis: SIMD3(0,0,1))
+ }
+ func transform(at epoch: Epoch) throws -> FrameTransform {
+ let q = try rotation(at: epoch), r = q.matrix, h = step.seconds
+ let samples = try [-2.0,-1,1,2].map { try rotation(at: epoch.advanced(by: Duration(seconds: $0*h))).matrix }
+ var d = [Double](), dd = [Double]()
+ for i in 0..<3 { for j in 0..<3 {
+ d.append((samples[0][i,j]-8*samples[1][i,j]+8*samples[2][i,j]-samples[3][i,j])/(12*h))
+ dd.append((-samples[3][i,j]+16*samples[2][i,j]-30*r[i,j]+16*samples[1][i,j]-samples[0][i,j])/(12*h*h))
+ }}
+ func axial(_ v: [Double]) -> SIMD3 {
+ func e(_ i: Int,_ j: Int) -> Double { (0..<3).reduce(0) { $0+v[3*i+$1]*r[j,$1] } }
+ return SIMD3((e(2,1)-e(1,2))/2,(e(0,2)-e(2,0))/2,(e(1,0)-e(0,1))/2)
+ }
+ return try FrameTransform(epoch: epoch,rotation: q,angularVelocity: axial(d),angularAcceleration: axial(dd))
+ }
+}
diff --git a/Sources/CelMek/ApparentPlaceOfAStar.swift b/Sources/CelMek/ApparentPlaceOfAStar.swift
new file mode 100644
index 0000000..64e68e2
--- /dev/null
+++ b/Sources/CelMek/ApparentPlaceOfAStar.swift
@@ -0,0 +1,20 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2023 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+
+import Foundation
+// Meeus, chapter 23
diff --git a/Sources/CelMek/AtmosphericRefraction.swift b/Sources/CelMek/AtmosphericRefraction.swift
new file mode 100644
index 0000000..40d9af2
--- /dev/null
+++ b/Sources/CelMek/AtmosphericRefraction.swift
@@ -0,0 +1,20 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2023 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+
+import Foundation
+// Meeus, chapter 16
diff --git a/Sources/CelMek/Attitude.swift b/Sources/CelMek/Attitude.swift
new file mode 100644
index 0000000..3665b5f
--- /dev/null
+++ b/Sources/CelMek/Attitude.swift
@@ -0,0 +1,210 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Foundation
+import Math
+
+public enum AttitudeError: Error, Equatable {
+ case invalidRotation, invalidVector, nonInertialReference, frameMismatch, epochMismatch
+ case undefinedDirection, undefinedRoll, invalidConfiguration, angularAccelerationUnavailable
+ case invalidInertia, numericalRangeExceeded
+}
+func attitudeCross(_ a: SIMD3, _ b: SIMD3) -> SIMD3 {
+ SIMD3(a.y*b.z-a.z*b.y,a.z*b.x-a.x*b.z,a.x*b.y-a.y*b.x)
+}
+func attitudeFinite(_ vector: SIMD3) -> Bool { [vector.x,vector.y,vector.z].allSatisfy(\.isFinite) }
+func attitudeUnit(_ vector: SIMD3) throws -> SIMD3 {
+ guard attitudeFinite(vector) else { throw AttitudeError.invalidVector }
+ let scale = max(abs(vector.x),abs(vector.y),abs(vector.z))
+ guard scale > 0 else { throw AttitudeError.undefinedDirection }
+ let scaled = vector/scale
+ return scaled/routeNorm(scaled)
+}
+func attitudeQuaternion(_ quaternion: Quaternion) throws -> Quaternion {
+ let scale = max(abs(quaternion.x),abs(quaternion.y),abs(quaternion.z),abs(quaternion.w))
+ guard [quaternion.x,quaternion.y,quaternion.z,quaternion.w].allSatisfy(\.isFinite), scale > 0 else { throw AttitudeError.invalidRotation }
+ let scaled = quaternion/scale
+ return scaled/sqrt(Quaternion.dot(lhs: scaled,rhs: scaled))
+}
+/// Hamilton quaternion maps body vectors into inertial reference axes.
+/// Angular velocity/acceleration are physical rates relative to that reference,
+/// expressed in body axes (rad/s and rad/s²), not coordinate-map rates.
+public struct AttitudeState {
+ public let epoch: Epoch
+ public let referenceFrame: Frame
+ public let bodyFrame: Frame
+ public let bodyToReference: Quaternion
+ public let angularVelocityBodyRadiansPerSecond: SIMD3
+ public let angularAccelerationBodyRadiansPerSecondSquared: SIMD3?
+ public init(epoch: Epoch, referenceFrame: Frame, bodyFrame: Frame, bodyToReference: Quaternion,
+ angularVelocityBodyRadiansPerSecond: SIMD3 = .zero,
+ angularAccelerationBodyRadiansPerSecondSquared: SIMD3? = nil) throws {
+ guard referenceFrame.pseudoInertial else { throw AttitudeError.nonInertialReference }
+ guard referenceFrame !== bodyFrame else { throw AttitudeError.frameMismatch }
+ guard attitudeFinite(angularVelocityBodyRadiansPerSecond), angularAccelerationBodyRadiansPerSecondSquared.map(attitudeFinite) ?? true else { throw AttitudeError.invalidVector }
+ self.epoch = epoch; self.referenceFrame = referenceFrame; self.bodyFrame = bodyFrame
+ self.bodyToReference = try attitudeQuaternion(bodyToReference)
+ self.angularVelocityBodyRadiansPerSecond = angularVelocityBodyRadiansPerSecond
+ self.angularAccelerationBodyRadiansPerSecondSquared = angularAccelerationBodyRadiansPerSecondSquared
+ }
+ public func referenceVector(fromBody vector: SIMD3) throws -> SIMD3 {
+ guard attitudeFinite(vector) else { throw AttitudeError.invalidVector }
+ let result = bodyToReference.matrix*vector
+ guard attitudeFinite(result) else { throw AttitudeError.numericalRangeExceeded }
+ return result
+ }
+ public func bodyVector(fromReference vector: SIMD3) throws -> SIMD3 {
+ guard attitudeFinite(vector) else { throw AttitudeError.invalidVector }
+ let result = bodyToReference.conj.matrix*vector
+ guard attitudeFinite(result) else { throw AttitudeError.numericalRangeExceeded }
+ return result
+ }
+ public func orientation() throws -> BodyOrientation {
+ guard let alpha = angularAccelerationBodyRadiansPerSecondSquared else { throw AttitudeError.angularAccelerationUnavailable }
+ return try BodyOrientation(referenceFrame: referenceFrame,epoch: epoch,rotation: bodyToReference.conj,
+ angularVelocity: -angularVelocityBodyRadiansPerSecond,angularAcceleration: -alpha)
+ }
+}
+public protocol AttitudeProvider {
+ var referenceFrame: Frame { get }
+ var bodyFrame: Frame { get }
+ func attitude(at epoch: Epoch) throws -> AttitudeState
+}
+extension AttitudeProvider {
+ public func checkedAttitude(at epoch: Epoch) throws -> AttitudeState {
+ let state = try attitude(at: epoch)
+ guard state.epoch == epoch else { throw AttitudeError.epochMismatch }
+ guard state.referenceFrame === referenceFrame, state.bodyFrame === bodyFrame else { throw AttitudeError.frameMismatch }
+ return state
+ }
+}
+public struct AttitudeOrientationProvider: OrientationProvider {
+ public let attitudeProvider: any AttitudeProvider
+ public var referenceFrame: Frame { attitudeProvider.referenceFrame }
+ public init(_ provider: any AttitudeProvider) { attitudeProvider = provider }
+ public func orientation(at epoch: Epoch) throws -> BodyOrientation { try attitudeProvider.checkedAttitude(at: epoch).orientation() }
+}
+/// Adapts existing planetary/local-orbital orientation providers without changing
+/// their reference-to-body coordinate-map convention.
+public struct OrientationAttitudeProvider: AttitudeProvider {
+ public let orientationProvider: any OrientationProvider
+ public let bodyFrame: Frame
+ public var referenceFrame: Frame { orientationProvider.referenceFrame }
+ public init(orientation: any OrientationProvider, bodyFrame: Frame) { orientationProvider = orientation; self.bodyFrame = bodyFrame }
+ public func attitude(at epoch: Epoch) throws -> AttitudeState {
+ let orientation = try orientationProvider.orientation(at: epoch)
+ guard orientation.epoch == epoch else { throw AttitudeError.epochMismatch }
+ guard orientation.referenceFrame === referenceFrame else { throw AttitudeError.frameMismatch }
+ return try AttitudeState(epoch: epoch,referenceFrame: referenceFrame,bodyFrame: bodyFrame,bodyToReference: orientation.rotation.conj,
+ angularVelocityBodyRadiansPerSecond: -orientation.angularVelocity,
+ angularAccelerationBodyRadiansPerSecondSquared: -orientation.angularAcceleration)
+ }
+}
+public struct InertialHoldAttitudeProvider: AttitudeProvider {
+ public let referenceFrame: Frame
+ public let bodyFrame: Frame
+ public let bodyToReference: Quaternion
+ public init(referenceFrame: Frame, bodyFrame: Frame, bodyToReference: Quaternion = .identity) throws {
+ let seed = try AttitudeState(epoch: .j2000,referenceFrame: referenceFrame,bodyFrame: bodyFrame,bodyToReference: bodyToReference)
+ self.referenceFrame = referenceFrame; self.bodyFrame = bodyFrame; self.bodyToReference = seed.bodyToReference
+ }
+ public func attitude(at epoch: Epoch) throws -> AttitudeState {
+ try AttitudeState(epoch: epoch,referenceFrame: referenceFrame,bodyFrame: bodyFrame,bodyToReference: bodyToReference,
+ angularAccelerationBodyRadiansPerSecondSquared: .zero)
+ }
+}
+/// Prescribed constant physical spin in body axes; no torque model is inferred.
+public struct UniformSpinAttitudeProvider: AttitudeProvider {
+ public let initialState: AttitudeState
+ public var referenceFrame: Frame { initialState.referenceFrame }
+ public var bodyFrame: Frame { initialState.bodyFrame }
+ public init(initialState: AttitudeState) { self.initialState = initialState }
+ public func attitude(at epoch: Epoch) throws -> AttitudeState {
+ let omega = initialState.angularVelocityBodyRadiansPerSecond, speed = routeNorm(omega)
+ let angle = speed * (try epoch.duration(since: initialState.epoch).seconds)
+ guard angle.isFinite else { throw AttitudeError.numericalRangeExceeded }
+ let rotation = speed == 0 ? Quaternion.identity : Quaternion(angle: angle.truncatingRemainder(dividingBy: 2 * .pi),axis: omega)
+ return try AttitudeState(epoch: epoch,referenceFrame: referenceFrame,bodyFrame: bodyFrame,
+ bodyToReference: initialState.bodyToReference*rotation,angularVelocityBodyRadiansPerSecond: omega,
+ angularAccelerationBodyRadiansPerSecondSquared: .zero)
+ }
+}
+public enum AttitudeTrackingDirection { case target, velocity, nadir }
+/// Body X follows the selected direction, Z follows the projected explicit roll
+/// reference, Y = Z × X. Zero direction or parallel roll axes fail explicitly.
+/// Five-point angular derivatives require provider coverage at epoch ±2*step.
+public struct TrackingAttitudeProvider: AttitudeProvider {
+ public let referenceFrame: Frame
+ public let bodyFrame: Frame
+ public let derivativeStep: Duration
+ public let direction: AttitudeTrackingDirection
+ public let rollReference: SIMD3
+ private let spacecraft: any StateProvider
+ private let target: (any StateProvider)?
+ public init(spacecraft: any StateProvider, bodyFrame: Frame, direction: AttitudeTrackingDirection,
+ target: (any StateProvider)? = nil, rollReference: SIMD3, derivativeStep: Duration) throws {
+ guard spacecraft.frame.pseudoInertial else { throw AttitudeError.nonInertialReference }
+ guard target == nil || target!.frame === spacecraft.frame, bodyFrame !== spacecraft.frame else { throw AttitudeError.frameMismatch }
+ guard derivativeStep.seconds.isFinite, derivativeStep > .zero,
+ (derivativeStep.seconds*derivativeStep.seconds).isFinite, derivativeStep.seconds*derivativeStep.seconds > 0 else { throw AttitudeError.invalidConfiguration }
+ if case .target = direction, target == nil { throw AttitudeError.invalidConfiguration }
+ referenceFrame = spacecraft.frame; self.bodyFrame = bodyFrame; self.direction = direction
+ self.spacecraft = spacecraft; self.target = target; self.derivativeStep = derivativeStep
+ self.rollReference = try attitudeUnit(rollReference)
+ }
+ private func matrix(at epoch: Epoch) throws -> [Double] {
+ func checked(_ provider: any StateProvider) throws -> CartesianState {
+ let state = try provider.state(at: epoch)
+ guard state.epoch == epoch else { throw AttitudeError.epochMismatch }
+ guard state.frame === referenceFrame else { throw AttitudeError.frameMismatch }
+ return state
+ }
+ let state = try checked(spacecraft), centre = try target.map(checked)
+ let look: SIMD3
+ switch direction {
+ case .target, .nadir: look = (centre?.position ?? .zero)-state.position
+ case .velocity: look = state.velocity-(centre?.velocity ?? .zero)
+ }
+ let x = try attitudeUnit(look), projected = rollReference-x*(rollReference*x).sum()
+ guard routeNorm(projected) > 1e-12 else { throw AttitudeError.undefinedRoll }
+ let z = try attitudeUnit(projected), y = attitudeCross(z,x)
+ return [x.x,x.y,x.z,y.x,y.y,y.z,z.x,z.y,z.z]
+ }
+ public func attitude(at epoch: Epoch) throws -> AttitudeState {
+ let h = derivativeStep.seconds, r = try matrix(at: epoch)
+ let samples = try [-2.0,-1,1,2].map { try matrix(at: epoch.advanced(by: Duration(seconds: $0*h))) }
+ let d = (0..<9).map { (samples[0][$0]-8*samples[1][$0]+8*samples[2][$0]-samples[3][$0])/(12*h) }
+ let dd = (0..<9).map { (-samples[3][$0]+16*samples[2][$0]-30*r[$0]+16*samples[1][$0]-samples[0][$0])/(12*h*h) }
+ func axial(_ derivative: [Double]) -> SIMD3 {
+ func entry(_ i: Int, _ j: Int) -> Double { (0..<3).reduce(0) { $0+derivative[3*i+$1]*r[3*j+$1] } }
+ return SIMD3((entry(2,1)-entry(1,2))/2,(entry(0,2)-entry(2,0))/2,(entry(1,0)-entry(0,1))/2)
+ }
+ return try AttitudeState(epoch: epoch,referenceFrame: referenceFrame,bodyFrame: bodyFrame,
+ bodyToReference: Matrix3x3(elements: r).quaternion.conj,
+ angularVelocityBodyRadiansPerSecond: -axial(d),angularAccelerationBodyRadiansPerSecondSquared: -axial(dd))
+ }
+}
+extension FrameTree {
+ /// Registers the provider's exact body-frame identity with its inertial parent.
+ /// As with other frame providers, do not capture the owning tree strongly.
+ public func registerSpacecraftFrame(spacecraft: any StateProvider, attitude: any AttitudeProvider,
+ accelerationPolicy: OriginAccelerationPolicy = .requireProvided) throws {
+ guard attitude.bodyFrame.parent === attitude.referenceFrame, spacecraft.frame === attitude.referenceFrame else { throw AttitudeError.frameMismatch }
+ try registerFrame(attitude.bodyFrame,provider: BodyFixedTransformProvider(centre: spacecraft,
+ orientation: AttitudeOrientationProvider(attitude),accelerationPolicy: accelerationPolicy))
+ }
+}
diff --git a/Sources/CelMek/BiEllipticTransfer.swift b/Sources/CelMek/BiEllipticTransfer.swift
new file mode 100644
index 0000000..91465fe
--- /dev/null
+++ b/Sources/CelMek/BiEllipticTransfer.swift
@@ -0,0 +1,125 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Foundation
+import Math
+
+public enum BiEllipticTransferError: Error, Equatable {
+ case invalidIntermediateRadius, numericalRangeExceeded, invalidComparison
+}
+
+/// Three-impulse transfer between circular orbits via a caller-selected apoapsis.
+/// An optional plane change is combined with the impulse at that apoapsis.
+public struct BiEllipticTransfer {
+ public let departureRadiusMetres, arrivalRadiusMetres, intermediateRadiusMetres: Double
+ public let gravitationalParameter: GravitationalParameter
+ public let firstSemiMajorAxisMetres, secondSemiMajorAxisMetres: Double
+ public let firstLegDuration, secondLegDuration, duration: Duration
+ public let departureDeltaVelocityMetresPerSecond, arrivalDeltaVelocityMetresPerSecond: Double
+ /// Signed coplanar speed difference; the combined middle impulse may be larger.
+ public let intermediateSpeedChangeMetresPerSecond: Double
+ public let intermediateImpulse: PlaneChangeImpulse
+ public let intermediateDeltaVelocityMetresPerSecond: Double
+ public let totalDeltaVelocityMetresPerSecond: Double
+ private let departureCircularSpeed, arrivalCircularSpeed: Double
+
+ public init(departureRadiusMetres: Double, arrivalRadiusMetres: Double, intermediateRadiusMetres: Double,
+ gravitationalParameter: GravitationalParameter, planeChangeRadians: Double = 0) throws {
+ guard intermediateRadiusMetres.isFinite, intermediateRadiusMetres > max(departureRadiusMetres, arrivalRadiusMetres) else {
+ throw BiEllipticTransferError.invalidIntermediateRadius
+ }
+ let first = try HohmannTransfer(departureRadiusMetres: departureRadiusMetres,
+ arrivalRadiusMetres: intermediateRadiusMetres, gravitationalParameter: gravitationalParameter)
+ let second = try HohmannTransfer(departureRadiusMetres: intermediateRadiusMetres,
+ arrivalRadiusMetres: arrivalRadiusMetres, gravitationalParameter: gravitationalParameter)
+ let x = departureRadiusMetres/intermediateRadiusMetres, y = arrivalRadiusMetres/intermediateRadiusMetres
+ let apoCircular = first.arrivalCircularSpeedMetresPerSecond
+ let before = apoCircular*sqrt(2*x/(1+x)), after = apoCircular*sqrt(2*y/(1+y))
+ let speedChange = apoCircular*(2*((arrivalRadiusMetres-departureRadiusMetres)/intermediateRadiusMetres) /
+ ((1+x)*(1+y)))/(sqrt(2*x/(1+x))+sqrt(2*y/(1+y)))
+ let impulse = try PlaneChangeImpulse(beforeSpeedMetresPerSecond: before,
+ afterSpeedMetresPerSecond: after, angleRadians: planeChangeRadians)
+ // Keep the rationalized coplanar difference for nearly equal endpoint radii.
+ let middleCost = planeChangeRadians == 0 ? abs(speedChange) : impulse.deltaVelocityMetresPerSecond
+ let total = abs(first.departureDeltaVelocityMetresPerSecond)+middleCost+abs(second.arrivalDeltaVelocityMetresPerSecond)
+ guard [before, after, speedChange, total].allSatisfy(\.isFinite), before > 0, after > 0 else {
+ throw BiEllipticTransferError.numericalRangeExceeded
+ }
+ self.departureRadiusMetres = departureRadiusMetres; self.arrivalRadiusMetres = arrivalRadiusMetres
+ self.intermediateRadiusMetres = intermediateRadiusMetres; self.gravitationalParameter = gravitationalParameter
+ firstSemiMajorAxisMetres = first.semiMajorAxisMetres; secondSemiMajorAxisMetres = second.semiMajorAxisMetres
+ firstLegDuration = first.duration; secondLegDuration = second.duration
+ duration = try first.duration.adding(second.duration)
+ departureDeltaVelocityMetresPerSecond = first.departureDeltaVelocityMetresPerSecond
+ arrivalDeltaVelocityMetresPerSecond = second.arrivalDeltaVelocityMetresPerSecond
+ intermediateSpeedChangeMetresPerSecond = speedChange; intermediateImpulse = impulse
+ totalDeltaVelocityMetresPerSecond = total; intermediateDeltaVelocityMetresPerSecond = middleCost
+ departureCircularSpeed = first.departureCircularSpeedMetresPerSecond
+ arrivalCircularSpeed = second.arrivalCircularSpeedMetresPerSecond
+ }
+
+ public func plan(departureEpoch: Epoch, frame: Frame, centralBody: BodyIdentifier,
+ radialDirection: SIMD3, progradeDirection: SIMD3, planeChangeSense: PlaneChangeSense = .positive,
+ propagationOptions: TwoBodyPropagationOptions = try! TwoBodyPropagationOptions()) throws -> BiEllipticTransferPlan {
+ guard frame.pseudoInertial else { throw PropagationError.nonInertialFrame }
+ let radial = try biUnit(radialDirection), supplied = try biUnit(progradeDirection)
+ let dot = (radial*supplied).sum()
+ guard abs(dot) <= 1e-12 else { throw HohmannTransferError.invalidDirections }
+ let tangent = try biUnit(supplied-radial*dot)
+ let intermediateEpoch = try departureEpoch.advanced(by: firstLegDuration)
+ let arrivalEpoch = try intermediateEpoch.advanced(by: secondLegDuration)
+ guard intermediateEpoch > departureEpoch, arrivalEpoch > intermediateEpoch else {
+ throw BiEllipticTransferError.numericalRangeExceeded
+ }
+ let initial = try CartesianState(epoch: departureEpoch, frame: frame,
+ position: radial*departureRadiusMetres, velocity: tangent*departureCircularSpeed)
+ let base = try TwoBodyPropagator(initialState: initial, centralBody: centralBody,
+ gravitationalParameter: gravitationalParameter, options: propagationOptions)
+ let departure = try ImpulsiveManeuver(epoch: departureEpoch, frame: frame,
+ deltaVelocityMetresPerSecond: tangent*departureDeltaVelocityMetresPerSecond)
+ let middle: ImpulsiveManeuver
+ if intermediateImpulse.angleRadians == 0 {
+ middle = try ImpulsiveManeuver(epoch: intermediateEpoch, frame: frame,
+ deltaVelocityMetresPerSecond: -tangent*intermediateSpeedChangeMetresPerSecond)
+ } else {
+ middle = try intermediateImpulse.maneuver(epoch: intermediateEpoch, frame: frame,
+ radialDirection: -radial, progradeDirection: -tangent, sense: planeChangeSense)
+ }
+ let finalTangent = Quaternion(angle: planeChangeSense == .positive ?
+ intermediateImpulse.angleRadians : -intermediateImpulse.angleRadians, axis: -radial).matrix*tangent
+ let arrival = try ImpulsiveManeuver(epoch: arrivalEpoch, frame: frame,
+ deltaVelocityMetresPerSecond: finalTangent*arrivalDeltaVelocityMetresPerSecond)
+ let trajectory = try ManeuveredTwoBodyPropagator(base: base, maneuvers: [departure,middle,arrival])
+ let expected = try CartesianState(epoch: arrivalEpoch, frame: frame,
+ position: radial*arrivalRadiusMetres, velocity: finalTangent*arrivalCircularSpeed)
+ return BiEllipticTransferPlan(transfer: self, intermediateEpoch: intermediateEpoch, arrivalEpoch: arrivalEpoch,
+ departureBurn: departure, intermediateBurn: middle, arrivalBurn: arrival,
+ expectedArrivalState: expected, trajectory: trajectory)
+ }
+}
+public struct BiEllipticTransferPlan {
+ public let transfer: BiEllipticTransfer
+ public let intermediateEpoch, arrivalEpoch: Epoch
+ public let departureBurn, intermediateBurn, arrivalBurn: ImpulsiveManeuver
+ public let expectedArrivalState: CartesianState
+ public let trajectory: ManeuveredTwoBodyPropagator
+}
+private func biUnit(_ v: SIMD3) throws -> SIMD3 {
+ let n = hypot(hypot(v.x,v.y),v.z)
+ guard n.isFinite, n > 0 else { throw HohmannTransferError.invalidDirections }
+ return v/n
+}
diff --git a/Sources/CelMek/Igrf.swift b/Sources/CelMek/BodiesInStraightLines.swift
similarity index 92%
rename from Sources/CelMek/Igrf.swift
rename to Sources/CelMek/BodiesInStraightLines.swift
index 06c3dd7..91776ae 100644
--- a/Sources/CelMek/Igrf.swift
+++ b/Sources/CelMek/BodiesInStraightLines.swift
@@ -1,7 +1,7 @@
//
// SPDX-License-Identifier: Apache-2.0
//
-// Copyright 2020 Mattias Holm
+// Copyright 2023 Mattias Holm
//
// Licensed under the Apache License, Version 2.0 (the "License");
// you may not use this file except in compliance with the License.
@@ -16,5 +16,6 @@
// limitations under the License.
//
-
import Foundation
+// Meeus, chapter 19
+
diff --git a/Sources/CelMek/BodyAtmosphere.swift b/Sources/CelMek/BodyAtmosphere.swift
new file mode 100644
index 0000000..b6d7298
--- /dev/null
+++ b/Sources/CelMek/BodyAtmosphere.swift
@@ -0,0 +1,65 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Foundation
+import Math
+import Atmospheres
+
+public extension BodyIdentifier {
+ /// Nominal built-in atmosphere for a body centre; nil means no supplied model.
+ var atmosphericModel: BodyAtmosphere? {
+ guard case .naif(let code) = self else { return nil }
+ return BodyAtmosphere.model(naifBodyCode: code)
+ }
+}
+
+/// Spherical altitude adapter for drag. Caller supplies the radius of the profile's
+/// datum and angular velocity in the state's inertial axes. Atmospheric co-rotation
+/// is included as Ω×r; no additional meteorological winds are inferred.
+/// Origin must be the body's centre; no implicit ephemeris or orientation transform.
+public struct SphericalBodyAtmosphere: AtmosphereProvider {
+ public let bodyIdentifier: BodyIdentifier
+ public let profile: any AtmosphericProfile
+ public let referenceRadiusMetres: Double
+ public let angularVelocityRadiansPerSecond: SIMD3
+ public let frame: Frame
+ public init(bodyIdentifier: BodyIdentifier, profile: any AtmosphericProfile,
+ referenceRadiusMetres: Double, frame: Frame,
+ angularVelocityRadiansPerSecond: SIMD3 = .zero) throws {
+ try bodyIdentifier.validate()
+ guard referenceRadiusMetres.isFinite, referenceRadiusMetres > 0,
+ [angularVelocityRadiansPerSecond.x, angularVelocityRadiansPerSecond.y,
+ angularVelocityRadiansPerSecond.z].allSatisfy(\.isFinite) else {
+ throw EnvironmentalForceError.invalidParameter
+ }
+ if let identified = profile as? BodyAtmosphere,
+ bodyIdentifier != .naif(identified.body.rawValue) { throw BodyModelError.bodyMismatch }
+ guard frame.pseudoInertial else { throw SpacecraftDynamicsError.nonInertialFrame }
+ self.bodyIdentifier = bodyIdentifier; self.profile = profile; self.referenceRadiusMetres = referenceRadiusMetres
+ self.frame = frame; self.angularVelocityRadiansPerSecond = angularVelocityRadiansPerSecond
+ }
+ public func sample(for state: SpacecraftState, in context: ForceEvaluationContext) throws -> AtmosphereSample {
+ guard context.origin == bodyIdentifier else { throw EnvironmentalForceError.originMismatch }
+ guard state.frame === frame, context.frame === frame else { throw SpacecraftDynamicsError.frameMismatch }
+ let p = state.cartesian.position, w = angularVelocityRadiansPerSecond
+ let altitude = hypot(hypot(p.x,p.y),p.z)-referenceRadiusMetres
+ let properties = try profile.properties(at: altitude)
+ return try AtmosphereSample(epoch: state.epoch, frame: frame, origin: bodyIdentifier,
+ densityKilogramsPerCubicMetre: properties.densityKilogramsPerCubicMetre,
+ velocityMetresPerSecond: SIMD3(w.y*p.z-w.z*p.y, w.z*p.x-w.x*p.z, w.x*p.y-w.y*p.x))
+ }
+}
diff --git a/Sources/CelMek/BodyFixedFrame.swift b/Sources/CelMek/BodyFixedFrame.swift
new file mode 100644
index 0000000..bad1c91
--- /dev/null
+++ b/Sources/CelMek/BodyFixedFrame.swift
@@ -0,0 +1,145 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Math
+
+public enum BodyFixedFrameError: Error, Equatable {
+ case frameMismatch, accelerationUnavailable, invalidDifferenceStep
+}
+
+/// Orientation from reference coordinates into body-fixed axes, without an
+/// origin translation. Angular derivatives are expressed in body-fixed axes.
+public struct BodyOrientation {
+ public let referenceFrame: Frame
+ public let epoch: Epoch
+ public let rotation: Quaternion
+ public let angularVelocity: SIMD3
+ public let angularAcceleration: SIMD3
+
+ public init(referenceFrame: Frame, epoch: Epoch, rotation: Quaternion,
+ angularVelocity: SIMD3 = .zero,
+ angularAcceleration: SIMD3 = .zero) throws {
+ let validated = try FrameTransform(epoch: epoch, rotation: rotation,
+ angularVelocity: angularVelocity, angularAcceleration: angularAcceleration)
+ self.referenceFrame = referenceFrame
+ self.epoch = epoch
+ self.rotation = validated.rotation
+ self.angularVelocity = angularVelocity
+ self.angularAcceleration = angularAcceleration
+ }
+}
+
+public protocol OrientationProvider {
+ var referenceFrame: Frame { get }
+ func orientation(at epoch: Epoch) throws -> BodyOrientation
+}
+
+/// Prescribed fixed-axis spin; no planetary orientation model is implied.
+/// Axis, rate, and initial rotation follow UniformRotationProvider conventions.
+public struct FixedAxisOrientationProvider: OrientationProvider {
+ public let referenceFrame: Frame
+ private let spin: UniformRotationProvider
+ public init(referenceFrame: Frame, referenceEpoch: Epoch = .j2000,
+ axis: SIMD3, rate: Double, initialRotation: Quaternion = .identity) throws {
+ self.referenceFrame = referenceFrame
+ spin = try UniformRotationProvider(referenceEpoch: referenceEpoch, axis: axis,
+ rate: rate, initialRotation: initialRotation)
+ }
+ public func orientation(at epoch: Epoch) throws -> BodyOrientation {
+ let transform = try spin.transform(at: epoch)
+ return try BodyOrientation(referenceFrame: referenceFrame, epoch: epoch,
+ rotation: transform.rotation, angularVelocity: transform.angularVelocity,
+ angularAcceleration: transform.angularAcceleration)
+ }
+}
+
+/// Handling of missing acceleration at the body's centre. A supplied value
+/// always takes precedence; approximation is never selected implicitly.
+public enum OriginAccelerationPolicy {
+ case requireProvided
+ /// Explicitly treat origin acceleration as zero, suitable for prescribed
+ /// constant-velocity motion but approximate for orbiting bodies.
+ case assumeZero
+ /// Central difference of provider velocity over elapsed atomic seconds.
+ /// Both neighbouring samples must be available in the same frame.
+ case estimate(step: CelMek.Duration)
+}
+
+/// Parent-to-body-fixed mapping: p_body = R * (p_parent - centre).
+/// The centre and orientation must use the exact same reference frame identity.
+public struct BodyFixedTransformProvider: TransformProvider {
+ public let referenceFrame: Frame
+ private let centre: any StateProvider
+ private let orientationProvider: any OrientationProvider
+ private let accelerationPolicy: OriginAccelerationPolicy
+
+ public init(centre: any StateProvider, orientation: any OrientationProvider,
+ accelerationPolicy: OriginAccelerationPolicy = .requireProvided) throws {
+ guard centre.frame === orientation.referenceFrame else { throw BodyFixedFrameError.frameMismatch }
+ if case .estimate(let step) = accelerationPolicy {
+ guard step > .zero, step.seconds.isFinite else { throw BodyFixedFrameError.invalidDifferenceStep }
+ }
+ referenceFrame = centre.frame
+ self.centre = centre
+ orientationProvider = orientation
+ self.accelerationPolicy = accelerationPolicy
+ }
+
+ private func centreState(at epoch: Epoch) throws -> CartesianState {
+ let state = try centre.state(at: epoch)
+ guard state.epoch == epoch else { throw FrameTransformError.epochMismatch }
+ guard state.frame === referenceFrame else { throw BodyFixedFrameError.frameMismatch }
+ return state
+ }
+
+ public func transform(at epoch: Epoch) throws -> FrameTransform {
+ let state = try centreState(at: epoch)
+ let orientation = try orientationProvider.orientation(at: epoch)
+ guard orientation.epoch == epoch else { throw FrameTransformError.epochMismatch }
+ guard orientation.referenceFrame === referenceFrame else { throw BodyFixedFrameError.frameMismatch }
+ let acceleration: SIMD3
+ if let supplied = state.acceleration { acceleration = supplied }
+ else {
+ switch accelerationPolicy {
+ case .requireProvided: throw BodyFixedFrameError.accelerationUnavailable
+ case .assumeZero: acceleration = .zero
+ case .estimate(let step):
+ let before = try epoch.advanced(by: step.negated())
+ let after = try epoch.advanced(by: step)
+ let beforeState = try centreState(at: before)
+ let afterState = try centreState(at: after)
+ acceleration = (afterState.velocity - beforeState.velocity) / (2 * step.seconds)
+ }
+ }
+ let centring = try FrameTransform(epoch: epoch, translation: -state.position,
+ velocity: -state.velocity, acceleration: -acceleration)
+ let axes = try FrameTransform(epoch: epoch, rotation: orientation.rotation,
+ angularVelocity: orientation.angularVelocity, angularAcceleration: orientation.angularAcceleration)
+ return try centring.followed(by: axes)
+ }
+}
+
+extension FrameTree {
+ /// Adds a body-fixed child to the providers' common reference frame.
+ public func makeBodyFixedFrame(name: String, centre: any StateProvider,
+ orientation: any OrientationProvider,
+ accelerationPolicy: OriginAccelerationPolicy = .requireProvided) throws -> Frame {
+ let provider = try BodyFixedTransformProvider(centre: centre, orientation: orientation,
+ accelerationPolicy: accelerationPolicy)
+ return try makeFrame(parent: provider.referenceFrame, name: name, provider: provider)
+ }
+}
diff --git a/Sources/CelMek/BodyMagneticField.swift b/Sources/CelMek/BodyMagneticField.swift
new file mode 100644
index 0000000..32d30cf
--- /dev/null
+++ b/Sources/CelMek/BodyMagneticField.swift
@@ -0,0 +1,92 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Math
+import MagneticFields
+
+public extension BodyIdentifier {
+ /// Preset intrinsic field. Missing means no supplied model, never a zero total field.
+ var magneticModel: BodyMagneticField? {
+ guard case .naif(let code) = self else { return nil }
+ return BodyMagneticField.model(naifBodyCode: code)
+ }
+}
+
+public struct BodyMagneticSample {
+ public let epoch: Epoch
+ /// Body-fixed components in the provider's documented axes, in tesla.
+ public let vectorTesla: SIMD3
+ public init(epoch: Epoch, vectorTesla: SIMD3) throws {
+ let validated = try MagneticFluxDensity(vectorTesla: vectorTesla)
+ self.epoch = epoch; self.vectorTesla = validated.vectorTesla
+ }
+}
+
+/// Body identity and epoch contract independent of the concrete field evaluator.
+public protocol BodyMagneticProvider {
+ var bodyIdentifier: BodyIdentifier { get }
+ var metadata: MagneticFieldMetadata { get }
+ func magneticField(at epoch: Epoch, displacementMetres: SIMD3) throws -> BodyMagneticSample
+}
+
+/// Labels a pluggable field model. Calendar conversion is injected explicitly:
+/// future WMM/IGRF models require calendar decimal years, not Julian-year offsets.
+public struct ModelBodyMagneticField: BodyMagneticProvider {
+ public let bodyIdentifier: BodyIdentifier
+ public let model: any MagneticFieldModel
+ public var metadata: MagneticFieldMetadata { model.metadata }
+ private let decimalYear: (Epoch) throws -> Double
+ public init(bodyIdentifier: BodyIdentifier, model: any MagneticFieldModel,
+ decimalYear: @escaping (Epoch) throws -> Double) throws {
+ try bodyIdentifier.validate()
+ if let identified = model as? BodyMagneticField,
+ bodyIdentifier != .naif(identified.body.rawValue) { throw BodyModelError.bodyMismatch }
+ self.bodyIdentifier = bodyIdentifier; self.model = model; self.decimalYear = decimalYear
+ }
+ public func magneticField(at epoch: Epoch, displacementMetres: SIMD3) throws -> BodyMagneticSample {
+ let query = try MagneticFieldQuery(positionMetres: displacementMetres,decimalYear: decimalYear(epoch))
+ let field = try model.checkedField(at: query)
+ return try BodyMagneticSample(epoch: epoch, vectorTesla: field.vectorTesla)
+ }
+}
+
+/// Rotates body-centred positions into model axes and B back to reference axes.
+/// Caller must ensure the orientation axes agree with the magnetic model metadata.
+/// Magnetic fields transform as vectors; no angular-velocity or origin-velocity terms.
+public struct OrientedBodyMagneticField: MagneticFieldProvider {
+ public let provider: any BodyMagneticProvider
+ public let orientation: any BodyOrientationProvider
+ public init(provider: any BodyMagneticProvider, orientation: any BodyOrientationProvider) throws {
+ guard provider.bodyIdentifier == orientation.bodyIdentifier else { throw BodyModelError.bodyMismatch }
+ self.provider = provider; self.orientation = orientation
+ }
+ /// Spacecraft state positions must be relative to this provider's body centre.
+ public func field(at state: SpacecraftState) throws -> MagneticFieldSample {
+ try magneticField(at: state.epoch,displacementMetres: state.cartesian.position,in: state.frame)
+ }
+ public func magneticField(at epoch: Epoch, displacementMetres: SIMD3,
+ in frame: Frame) throws -> MagneticFieldSample {
+ guard frame === orientation.referenceFrame else { throw BodyFixedFrameError.frameMismatch }
+ let axes = try orientation.orientation(at: epoch)
+ guard axes.epoch == epoch else { throw FrameTransformError.epochMismatch }
+ guard axes.referenceFrame === frame else { throw BodyFixedFrameError.frameMismatch }
+ let field = try provider.magneticField(at: epoch,displacementMetres: axes.rotation.matrix*displacementMetres)
+ guard field.epoch == epoch else { throw FrameTransformError.epochMismatch }
+ let validated = try MagneticFluxDensity(vectorTesla: axes.rotation.conj.matrix*field.vectorTesla)
+ return try MagneticFieldSample(epoch: epoch,frame: frame,origin: provider.bodyIdentifier,fieldTeslas: validated.vectorTesla)
+ }
+}
diff --git a/Sources/CelMek/BodyModels.swift b/Sources/CelMek/BodyModels.swift
new file mode 100644
index 0000000..9def194
--- /dev/null
+++ b/Sources/CelMek/BodyModels.swift
@@ -0,0 +1,174 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Foundation
+import Math
+
+public enum BodyModelError: Error, Equatable {
+ case bodyMismatch, invalidDirection, invalidPosition, singularGravity, nonFiniteResult
+}
+
+/// Orientation with an explicit body identity, independent of geometric and gravity models.
+public protocol BodyOrientationProvider: OrientationProvider {
+ var bodyIdentifier: BodyIdentifier { get }
+ var provenance: PhysicalDataProvenance { get }
+}
+
+/// Labels an existing attitude provider without changing its frames or rotations.
+public struct IdentifiedBodyOrientationProvider: BodyOrientationProvider {
+ public let bodyIdentifier: BodyIdentifier
+ public let provenance: PhysicalDataProvenance
+ public var referenceFrame: Frame { provider.referenceFrame }
+ private let provider: any OrientationProvider
+ public init(bodyIdentifier: BodyIdentifier, provider: any OrientationProvider,
+ provenance: PhysicalDataProvenance) throws {
+ try bodyIdentifier.validate()
+ self.bodyIdentifier = bodyIdentifier; self.provider = provider; self.provenance = provenance
+ }
+ public func orientation(at epoch: Epoch) throws -> BodyOrientation {
+ let result = try provider.orientation(at: epoch)
+ guard result.epoch == epoch else { throw FrameTransformError.epochMismatch }
+ guard result.referenceFrame === referenceFrame else { throw BodyFixedFrameError.frameMismatch }
+ return result
+ }
+}
+
+/// Surface point and outward unit normal in the shape's stated body-fixed axes.
+public struct BodySurfacePoint: Sendable {
+ public let positionMetres: SIMD3
+ public let outwardNormal: SIMD3
+ public init(positionMetres: SIMD3, outwardNormal: SIMD3) throws {
+ guard [positionMetres.x,positionMetres.y,positionMetres.z].allSatisfy(\.isFinite) else {
+ throw BodyModelError.nonFiniteResult
+ }
+ self.positionMetres = positionMetres
+ self.outwardNormal = try bodyModelUnit(outwardNormal)
+ }
+}
+
+/// Geometry relative to the body's centre. This initial query describes a surface
+/// reachable along a radial direction; it does not promise arbitrary mesh intersections.
+public protocol BodyShapeProvider {
+ var bodyIdentifier: BodyIdentifier { get }
+ var axesDescription: String { get }
+ var provenance: PhysicalDataProvenance { get }
+ func surface(inDirection direction: SIMD3) throws -> BodySurfacePoint
+}
+
+/// Positive reference ellipsoid, including a sphere when all three radii match.
+/// Radii and axes come from supplied shape data, independently of body metadata.
+public struct EllipsoidBodyShape: BodyShapeProvider {
+ public let bodyIdentifier: BodyIdentifier
+ public let referenceRadii: BodyReferenceRadii
+ public var axesDescription: String { referenceRadii.axesDescription }
+ public var provenance: PhysicalDataProvenance { referenceRadii.provenance }
+ public init(bodyIdentifier: BodyIdentifier, referenceRadii: BodyReferenceRadii) throws {
+ try bodyIdentifier.validate()
+ self.bodyIdentifier = bodyIdentifier; self.referenceRadii = referenceRadii
+ }
+ public func surface(inDirection direction: SIMD3) throws -> BodySurfacePoint {
+ let u = try bodyModelUnit(direction), radii = referenceRadii.metres
+ // Scale by the smallest radius, so intermediate ratios cannot overflow.
+ let scale = min(radii.x,radii.y,radii.z), inverse = SIMD3(scale/radii.x,scale/radii.y,scale/radii.z)
+ let weighted = u*inverse
+ let denominator = sqrt((weighted*weighted).sum())
+ guard denominator > 0 else { throw BodyModelError.nonFiniteResult }
+ let point = u*(scale/denominator)
+ // Gradient of sum((x_i/a_i)^2): direction is proportional to u_i/a_i^2.
+ return try BodySurfacePoint(positionMetres: point,outwardNormal: u*inverse*inverse)
+ }
+}
+
+/// Local gravity field. Units use the model's explicit coordinate-time convention;
+/// conversion to atomic-time dynamics is a responsibility of the consuming dynamics model.
+public struct BodyGravitySample: Sendable {
+ public let epoch: Epoch
+ public let acceleration: SIMD3
+ /// Gravitational potential in m²/s² with zero at infinity for point-mass gravity.
+ public let potential: Double
+ public let convention: GravitationalParameterConvention
+ public init(epoch: Epoch, acceleration: SIMD3, potential: Double,
+ convention: GravitationalParameterConvention) throws {
+ guard [acceleration.x,acceleration.y,acceleration.z,potential].allSatisfy(\.isFinite) else {
+ throw BodyModelError.nonFiniteResult
+ }
+ self.epoch = epoch; self.acceleration = acceleration; self.potential = potential; self.convention = convention
+ }
+}
+
+/// Field evaluated at a body-centred displacement in the model's described axes.
+/// Providers neither fetch ephemerides nor transform world coordinates implicitly.
+public protocol BodyGravityProvider {
+ var bodyIdentifier: BodyIdentifier { get }
+ var axesDescription: String { get }
+ var provenance: PhysicalDataProvenance { get }
+ var convention: GravitationalParameterConvention { get }
+ func gravity(at epoch: Epoch, displacementMetres: SIMD3) throws -> BodyGravitySample
+}
+
+/// Prescribed Newtonian point-mass field: acceleration = −μ r/|r|³, potential = −μ/|r|.
+/// No surface, collision, nonspherical field or relativistic correction is implied.
+public struct PointMassBodyGravity: BodyGravityProvider {
+ public let bodyIdentifier: BodyIdentifier
+ public let parameter: GravitationalParameter
+ public let axesDescription = "Any orthonormal body-centred Cartesian axes (spherically symmetric field)"
+ public var provenance: PhysicalDataProvenance { parameter.provenance }
+ public var convention: GravitationalParameterConvention { parameter.convention }
+ public init(bodyIdentifier: BodyIdentifier, parameter: GravitationalParameter) throws {
+ try bodyIdentifier.validate()
+ self.bodyIdentifier = bodyIdentifier; self.parameter = parameter
+ }
+ public func gravity(at epoch: Epoch, displacementMetres r: SIMD3) throws -> BodyGravitySample {
+ guard [r.x,r.y,r.z].allSatisfy(\.isFinite) else { throw BodyModelError.invalidPosition }
+ let scale = max(abs(r.x),abs(r.y),abs(r.z))
+ guard scale > 0 else { throw BodyModelError.singularGravity }
+ let scaled = r/scale, length = sqrt((scaled*scaled).sum())
+ let inverseRadius = (1/scale)/length
+ let potential = -parameter.cubicMetresPerSecondSquared*inverseRadius
+ let magnitude = potential*inverseRadius
+ return try BodyGravitySample(epoch: epoch,acceleration: (scaled/length)*magnitude,
+ potential: potential,convention: convention)
+ }
+}
+
+/// Optional independent models selected for one body, including magnetic fields. Missing models stay absent;
+/// GM/radii in metadata never silently create gravity or shape providers.
+/// Identity validation does not certify consistency of model versions or axis descriptions.
+public struct CelestialBodyModels {
+ public let body: CelestialBody
+ public let ephemeris: (any EphemerisProvider)?
+ public let orientation: (any BodyOrientationProvider)?
+ public let shape: (any BodyShapeProvider)?
+ public let gravity: (any BodyGravityProvider)?
+ public let magneticField: (any BodyMagneticProvider)?
+ public init(body: CelestialBody, ephemeris: (any EphemerisProvider)? = nil,
+ orientation: (any BodyOrientationProvider)? = nil,
+ shape: (any BodyShapeProvider)? = nil, gravity: (any BodyGravityProvider)? = nil,
+ magneticField: (any BodyMagneticProvider)? = nil) throws {
+ let ids = [ephemeris?.metadata.body,orientation?.bodyIdentifier,shape?.bodyIdentifier,gravity?.bodyIdentifier,magneticField?.bodyIdentifier]
+ guard ids.compactMap({ $0 }).allSatisfy({ $0 == body.identifier }) else { throw BodyModelError.bodyMismatch }
+ self.body = body; self.ephemeris = ephemeris; self.orientation = orientation; self.shape = shape; self.gravity = gravity
+ self.magneticField = magneticField
+ }
+}
+
+private func bodyModelUnit(_ vector: SIMD3) throws -> SIMD3 {
+ let scale = max(abs(vector.x),abs(vector.y),abs(vector.z))
+ guard [vector.x,vector.y,vector.z].allSatisfy(\.isFinite), scale > 0 else { throw BodyModelError.invalidDirection }
+ let scaled = vector/scale
+ return scaled/sqrt((scaled*scaled).sum())
+}
diff --git a/Sources/CelMek/CalendarDateTime.swift b/Sources/CelMek/CalendarDateTime.swift
new file mode 100644
index 0000000..d9e5af3
--- /dev/null
+++ b/Sources/CelMek/CalendarDateTime.swift
@@ -0,0 +1,127 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Foundation
+
+public enum CalendarConversionError: Error, Equatable, Sendable {
+ case invalidDate, invalidClock, outsideCalendarRange, leapSecondTableRequired
+}
+
+/// Proleptic Gregorian day with astronomical year numbering (year 0 = 1 BCE).
+/// Supported years: −1,000,000...1,000,000. No historical Julian/Gregorian cutover.
+public struct GregorianDay: Hashable, Sendable {
+ public let year: Int
+ public let month: Int
+ public let day: Int
+ public init(year: Int, month: Int, day: Int) throws {
+ guard (-1_000_000...1_000_000).contains(year) else { throw CalendarConversionError.outsideCalendarRange }
+ guard (1...12).contains(month) else { throw CalendarConversionError.invalidDate }
+ let leap = year % 4 == 0 && (year % 100 != 0 || year % 400 == 0)
+ let lengths = [31,leap ? 29 : 28,31,30,31,30,31,31,30,31,30,31]
+ guard (1...lengths[month-1]).contains(day) else { throw CalendarConversionError.invalidDate }
+ self.year = year; self.month = month; self.day = day
+ }
+ /// Integer MJD at midnight, independent of the time scale of a clock reading.
+ public var modifiedJulianDay: Int64 {
+ // March-based 400-year era decomposition described by Howard Hinnant:
+ // https://howardhinnant.github.io/date_algorithms.html
+ let y = Int64(year) - (month <= 2 ? 1 : 0)
+ let era = (y >= 0 ? y : y-399)/400
+ let within = y-era*400
+ let doy = (153*Int64(month > 2 ? month-3 : month+9)+2)/5+Int64(day)-1
+ return era*146097 + within*365 + within/4 - within/100 + doy - 719468 + 40587
+ }
+ public init(modifiedJulianDay: Int64) throws {
+ let first = try GregorianDay(year: -1_000_000,month: 1,day: 1).modifiedJulianDay
+ let last = try GregorianDay(year: 1_000_000,month: 12,day: 31).modifiedJulianDay
+ guard (first...last).contains(modifiedJulianDay) else { throw CalendarConversionError.outsideCalendarRange }
+ let z = modifiedJulianDay-40587+719468
+ let era = (z >= 0 ? z : z-146096)/146097
+ let doe = z-era*146097
+ let yoe = (doe-doe/1460+doe/36524-doe/146096)/365
+ let doy = doe-(365*yoe+yoe/4-yoe/100)
+ let mp = (5*doy+2)/153
+ let d = doy-(153*mp+2)/5+1
+ let m = mp+(mp < 10 ? 3 : -9)
+ let y = yoe+era*400+(m <= 2 ? 1 : 0)
+ try self.init(year: Int(y),month: Int(m),day: Int(d))
+ }
+}
+
+/// Scale of a Gregorian clock reading. UTC requires a leap-second table;
+/// continuous Julian dates continue to use TimeScale (TAI/TT/TDB).
+public enum CalendarTimeScale: Hashable, Sendable { case tai, tt, tdb, utc }
+
+public struct CalendarDateTime: Hashable, Sendable {
+ public let date: GregorianDay
+ public let hour: Int
+ public let minute: Int
+ public let second: Duration
+ public let scale: CalendarTimeScale
+ public init(date: GregorianDay, hour: Int, minute: Int, second: Duration, scale: CalendarTimeScale) throws {
+ guard (0..<24).contains(hour), (0..<60).contains(minute), second >= .zero,
+ second.wholeSeconds < 61 else { throw CalendarConversionError.invalidClock }
+ if second.wholeSeconds == 60 {
+ guard scale == .utc, hour == 23, minute == 59 else { throw CalendarConversionError.invalidClock }
+ }
+ self.date = date; self.hour = hour; self.minute = minute; self.second = second; self.scale = scale
+ }
+ public func epoch(using table: LeapSecondTable? = nil, tdbModel: (any TDBTimeModel)? = nil) throws -> Epoch {
+ let seconds = try Duration(wholeSeconds: Int64(hour*3600+minute*60)).adding(second)
+ if scale == .utc {
+ guard let table else { throw CalendarConversionError.leapSecondTableRequired }
+ return try Epoch(utc: UTCDate(modifiedJulianDay: date.modifiedJulianDay, secondOfDay: seconds), using: table)
+ }
+ let continuous: TimeScale = scale == .tai ? .tai : (scale == .tt ? .tt : .tdb)
+ let jd = try JulianDateComponents(wholeDay: date.modifiedJulianDay+2400000,
+ fractionalDay: 0.5+seconds.seconds/86400,scale: continuous)
+ return try Epoch(julianDate: jd, using: tdbModel)
+ }
+}
+
+extension Epoch {
+ public init(calendar: CalendarDateTime, using table: LeapSecondTable? = nil, tdbModel: (any TDBTimeModel)? = nil) throws {
+ self = try calendar.epoch(using: table, tdbModel: tdbModel)
+ }
+ public func calendar(in scale: CalendarTimeScale, using table: LeapSecondTable? = nil, tdbModel: (any TDBTimeModel)? = nil) throws -> CalendarDateTime {
+ let mjd: Int64
+ let seconds: Duration
+ if scale == .utc {
+ guard let table else { throw CalendarConversionError.leapSecondTableRequired }
+ let date = try utc(using: table)
+ mjd = date.modifiedJulianDay; seconds = date.secondOfDay
+ } else {
+ let continuous: TimeScale = scale == .tai ? .tai : (scale == .tt ? .tt : .tdb)
+ let jd = try julianDate(in: continuous, using: tdbModel)
+ // JD turns at noon; Gregorian clock days turn at midnight.
+ let shifted = try JulianDateComponents(wholeDay: jd.wholeDay-2400001,
+ fractionalDay: jd.fractionalDay+0.5,scale: continuous)
+ mjd = shifted.wholeDay
+ let raw = try Duration(seconds: shifted.fractionalDay*86400)
+ // Avoid a rounded clock label of 24:00 for a date already chosen below midnight.
+ seconds = raw.wholeSeconds < 86400 ? raw : try Duration(wholeSeconds: 86399,fractionalSecond: Double(1).nextDown)
+ }
+ let day = try GregorianDay(modifiedJulianDay: mjd)
+ if seconds.wholeSeconds == 86400 {
+ return try CalendarDateTime(date: day,hour: 23,minute: 59,
+ second: Duration(wholeSeconds: 60,fractionalSecond: seconds.fractionalSecond),scale: scale)
+ }
+ return try CalendarDateTime(date: day,hour: Int(seconds.wholeSeconds/3600),
+ minute: Int(seconds.wholeSeconds%3600/60),
+ second: Duration(wholeSeconds: seconds.wholeSeconds%60,fractionalSecond: seconds.fractionalSecond),scale: scale)
+ }
+}
diff --git a/Sources/CelMek/CartesianState.swift b/Sources/CelMek/CartesianState.swift
new file mode 100644
index 0000000..7764bea
--- /dev/null
+++ b/Sources/CelMek/CartesianState.swift
@@ -0,0 +1,96 @@
+//
+// SPDX-License-Identifier: Apache-2.0
+//
+// Copyright 2026 Mattias Holm
+//
+// Licensed under the Apache License, Version 2.0 (the "License");
+// you may not use this file except in compliance with the License.
+// You may obtain a copy of the License at
+//
+// http://www.apache.org/licenses/LICENSE-2.0
+//
+// Unless required by applicable law or agreed to in writing, software
+// distributed under the License is distributed on an "AS IS" BASIS,
+// WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+// See the License for the specific language governing permissions and
+// limitations under the License.
+//
+import Math
+
+/// Input conventions for normalizing Cartesian coordinates to SI units.
+public enum CartesianUnits: Sendable {
+ /// Position m, velocity m/s, acceleration m/s².
+ case metresAndSeconds
+ /// Position km, velocity km/s, acceleration km/s².
+ case kilometresAndSeconds
+ /// Position AU, velocity AU/day, acceleration AU/day².
+ case astronomicalUnitsAndDays
+
+ public static let metresPerAstronomicalUnit = 149_597_870_700.0
+ public static let secondsPerDay = 86_400.0
+
+ fileprivate var scales: (position: Double, velocity: Double, acceleration: Double) {
+ switch self {
+ case .metresAndSeconds: return (1, 1, 1)
+ case .kilometresAndSeconds: return (1000, 1000, 1000)
+ case .astronomicalUnitsAndDays:
+ let au = Self.metresPerAstronomicalUnit
+ let day = Self.secondsPerDay
+ return (au, au / day, au / (day * day))
+ }
+ }
+}
+
+public enum CartesianStateError: Error, Equatable, Sendable {
+ case nonFinitePosition
+ case nonFiniteVelocity
+ case nonFiniteAcceleration
+}
+
+/// Position and its time derivatives at an epoch, expressed in one reference frame.
+/// Stored units are always metres, metres/second, and metres/second².
+/// A nil acceleration means unavailable, not zero. Frame identity is object identity.
+public struct CartesianState: Equatable, Sendable {
+ public let epoch: Epoch
+ public let frame: Frame
+ public let position: SIMD3
+ public let velocity: SIMD3
+ public let acceleration: SIMD3?
+
+ /// Normalizes the supplied Cartesian input units and rejects nonfinite values,
+ /// including overflow during conversion. Spherical coordinates must first be
+ /// converted to Cartesian coordinates in the intended frame.
+ public init(epoch: Epoch, frame: Frame, position: SIMD3, velocity: SIMD3,
+ acceleration: SIMD3? = nil, units: CartesianUnits = .metresAndSeconds) throws {
+ let scales = units.scales
+ let position = position * scales.position
+ let velocity = velocity * scales.velocity
+ let acceleration = acceleration.map { $0 * scales.acceleration }
+ guard position.isFiniteVector else { throw CartesianStateError.nonFinitePosition }
+ guard velocity.isFiniteVector else { throw CartesianStateError.nonFiniteVelocity }
+ guard acceleration?.isFiniteVector != false else { throw CartesianStateError.nonFiniteAcceleration }
+ self.epoch = epoch
+ self.frame = frame
+ self.position = position
+ self.velocity = velocity
+ self.acceleration = acceleration
+ }
+
+ public static func == (lhs: CartesianState, rhs: CartesianState) -> Bool {
+ lhs.epoch == rhs.epoch && lhs.frame === rhs.frame && lhs.position == rhs.position
+ && lhs.velocity == rhs.velocity && lhs.acceleration == rhs.acceleration
+ }
+}
+
+/// A common query surface for prescribed ephemerides and future propagators.
+/// A result must carry the requested epoch and this provider's native frame.
+public protocol StateProvider {
+ var frame: Frame { get }
+ func state(at epoch: Epoch) throws -> CartesianState
+}
+
+/// Named astronomical frame identities that can be adopted as FrameTree roots.
+
+private extension SIMD3 where Scalar == Double {
+ var isFiniteVector: Bool { x.isFinite && y.isFinite && z.isFinite }
+}
diff --git a/Sources/CelMek/CelMek.docc/ACCURACY.md b/Sources/CelMek/CelMek.docc/ACCURACY.md
new file mode 100644
index 0000000..c761998
--- /dev/null
+++ b/Sources/CelMek/CelMek.docc/ACCURACY.md
@@ -0,0 +1,167 @@
+# Accuracy hints
+
+`AccuracyLevel` expresses the approximation an end user tolerates. It is a hint:
+a model may evaluate at higher accuracy than requested, including full evaluation.
+A lower hint does not require degraded results or promise a particular runtime.
+
+| Hint | Intent |
+| --- | --- |
+| `low` | Allow the model's largest supported approximation to reduce cost |
+| `balanced` | Permit a model-specific compromise between cost and approximation error |
+| `high` | Prefer smaller approximation error while allowing documented simplifications |
+| `full` | Evaluate the complete implemented model |
+
+Levels are not universal physical error bounds. Full evaluation can still mean a
+truncated theory, old coefficients, or approximate physics. Each algorithm must
+document its selection rule and limitations. Independent physical accuracy and
+runtime characterization remain separate from coefficient truncation bounds.
+
+`AccuracyAwareEphemerisProvider.accuracy` is the requested hint;
+`effectiveAccuracy` reports the evaluation mode used. `availableAccuracyLevels`
+lists the implemented evaluation modes, not the accepted hints. Every hint is
+accepted by the analytic adapters. Ephemeris metadata records both requested and
+effective levels; nil means unspecified. Composed providers leave those fields
+unspecified rather than inventing a single accuracy level for their inputs.
+
+## VSOP87 subsets
+
+`VSOP87Ephemeris` supports all four evaluation modes. It prepares its coefficient
+subset once during construction and reuses it for position and analytic velocity.
+The original coefficient tables remain intact. Full evaluation retains every term
+and remains the default.
+
+For a term A cos(B+Ct) tⁿ, selection bounds its individual positional contribution
+by |A| max(|t|)ⁿ over the caller's coverage. Here t is TDB Julian millennia from
+J2000. Coverage endpoints use the selected TDB model. The adapter adds a small
+margin to max(|t|), preserves the original order of retained terms, and retains
+terms at or above these cutoffs:
+
+| Hint | Individual contribution cutoff, AU |
+| --- | --- |
+| `low` | 1e-6 |
+| `balanced` | 1e-8 |
+| `high` | 1e-10 |
+| `full` | No terms removed |
+
+These are initial algorithm-specific settings, not certified position tolerances.
+They depend on coverage: larger intervals retain higher polynomial-order terms.
+`coefficientSelection` exposes original/retained term counts, the cutoff, and a
+conservative per-axis `positionErrorBoundMetres`. The bound sums omitted maximum
+amplitudes relative to the complete implemented series; cancellation generally
+makes observed error smaller. Ordinary floating evaluation error remains separate.
+It does not bound error against observations or a modern DE solution.
+
+If selection removes no terms, effective accuracy is full even for a lower hint.
+Velocity analytically differentiates exactly the selected terms and uses the same
+TDB-to-atomic rate conversion as full evaluation. The position bound is not a
+velocity error bound: small, fast oscillating terms can have larger derivatives.
+ cover all nine bodies at
+4,567 epochs from 1950 to 2050 (eight-day spacing plus the endpoint), using the
+same Fairhead TDB model in every mode. These are sampled maxima relative to full
+VSOP87E and local release-build timings, not independent physical error bounds.
+
+| Mode | Worst sampled position difference, km | Worst sampled velocity difference, m/s | Query speedup across bodies |
+| --- | ---: | ---: | ---: |
+| low | 2.9e+03 (Saturn system) | 2.69 | 3.07–10.03× |
+| balanced | 55.8 (Mars system) | 0.114 | 1.29–6.88× |
+| high | 0.513 (Mercury) | 0.000905 | 1.03–2.86× |
+
+The complete report includes per-body RMS errors, retained counts, query timings,
+preparation costs and conservative coefficient bounds. Run the characterization
+executable to measure your actual workload and machine. The eight-day sampling
+can miss short-period extrema; velocity accuracy deserves its own assessment.
+
+```swift
+let tdb = try FairheadTDBModel()
+let model = try VSOP87Ephemeris(
+ body: earth, coverage: coverage, tdbModel: tdb, accuracy: .balanced)
+let effective = model.effectiveAccuracy
+let retained = model.coefficientSelection.retainedTermCount
+let positionBound = model.coefficientSelection.positionErrorBoundMetres
+```
+
+## Other models and independent settings
+
+The shorter Meeus lunar and Goffin Pluto adapters accept every hint and currently
+use full evaluation. Their requested hint remains visible while effective accuracy
+is full. No artificial reduction or unsupported-level error occurs.
+
+TDB conversion, frame differentiation, coefficient reduction, body orientation,
+force selection and integrator tolerances are independent sources of error.
+Accuracy hints do not change explicit TDB models, derivative intervals, coverage,
+or missing-body handling. Legacy low-level functions keep complete-series behavior.
+Selecting full lunar evaluation still evaluates the existing truncated Meeus series,
+not the full ELP theory.
+
+Tests verify that lower hints can return full results, full VSOP87 output remains
+unchanged, retained term counts increase with tighter hints, sampled position
+errors respect the coefficient bound, and selected analytic velocities match
+independently differenced positions. Reduced-versus-full checks measure truncation
+within one theory, not independent physical validation.
+
+## Numerical spacecraft integration
+
+`NumericalPropagationOptions.preset(for:)` maps shared hints to version 1
+Dormand–Prince 5(4) local-error settings:
+
+| Hint | Absolute position, m | Absolute velocity, m/s | Absolute propellant, kg | Relative tolerance |
+| --- | ---: | ---: | ---: | ---: |
+| `low` | 10 | 1e-2 | 1e-4 | 1e-5 |
+| `balanced` | 1e-1 | 1e-4 | 1e-6 | 1e-7 |
+| `high` | 1e-3 | 1e-6 | 1e-9 | 1e-9 |
+| `full` | 1e-5 | 1e-8 | 1e-11 | 1e-11 |
+
+Every preset uses initial/minimum/maximum steps of 10 / 1e-6 / 300 seconds,
+100,000 maximum attempts and 700,001 maximum derivative evaluations. These work
+controls remain explicit and do not vary with the hint. The existing default
+`NumericalPropagationOptions()` equals the `high` preset, preserving its behavior.
+
+```swift
+let provider = try NumericalSpacecraftPropagator(
+ initialState: seed, dynamics: dynamics, accuracy: .balanced)
+let requested = provider.accuracy
+let preset = provider.effectiveAccuracy
+let actualSettings = provider.options
+```
+
+`accuracy` reports requested intent; `effectiveAccuracy` reports the selected
+preset, not measured trajectory error. All levels evaluate every supplied force
+model with the same numerical method. `full` selects the tightest preset; it does
+not imply exact integration, new force models, complete physics or unlimited work.
+Low hints may obtain much better results than their tolerances, particularly for
+unforced or polynomial motion; there is no artificial degradation.
+
+For direct control, construct validated options and pass them through either
+initializer. Explicit options are authoritative even when a hint is present:
+
+```swift
+let settings = try NumericalPropagationOptions(
+ absolutePositionToleranceMetres: 1e-4,
+ absoluteVelocityToleranceMetresPerSecond: 1e-7,
+ relativeTolerance: 1e-11,
+ maximumStepSeconds: 60)
+let custom = try NumericalSpacecraftPropagator(
+ initialState: seed, dynamics: dynamics, accuracy: .low, options: settings)
+// custom.accuracy == .low; custom.options == settings.
+// custom.effectiveAccuracy == nil: explicit settings are not classified as a preset.
+```
+
+The direct-options initializer reports nil for both hint fields. Nil means
+unspecified, not full. To adjust a preset's work controls, obtain it with
+`preset(for:)` and copy its tolerance fields into the explicit options initializer
+with the desired step limits; the options are immutable.
+
+Presets are initial numerical policies, not universal physical or final-position
+bounds. Acceptance scales each component by absolute tolerance plus relative
+tolerance times its state magnitude. Coordinate origin, trip duration, model
+smoothness and supplied forces all matter. Tightening tolerances can increase
+cost or fail at work/step/precision limits; there is no automatic downgrade to a
+looser preset. See for the error norm,
+propellant handling and numerical limits.
+
+Tests verify every preset's values tighten in order, unchanged defaults/work
+controls, requested/effective reporting and identical results for explicit
+settings regardless of a lower hint. An analytic exponential-velocity problem
+shows smaller error and greater evaluation cost for full versus low. This is a
+representative convergence check, not a benchmark or an error envelope covering
+all spacecraft scenarios; use propagation diagnostics for the actual workload.
diff --git a/Sources/CelMek/CelMek.docc/ATTITUDE_DYNAMICS.md b/Sources/CelMek/CelMek.docc/ATTITUDE_DYNAMICS.md
new file mode 100644
index 0000000..900f5b5
--- /dev/null
+++ b/Sources/CelMek/CelMek.docc/ATTITUDE_DYNAMICS.md
@@ -0,0 +1,158 @@
+# Attitude and rotational dynamics
+
+All rotations are right handed. Quantities use SI units and elapsed atomic
+seconds. Providers and propagators are immutable queries: a prediction restarts
+from its seed and does not consume fuel or advance hidden simulation time.
+
+## State and conventions
+
+`AttitudeState` contains an explicit epoch, inertial reference-frame identity,
+body-frame identity, a normalized Hamilton `bodyToReference` quaternion, physical
+angular velocity in body axes (rad/s), and optional physical angular acceleration
+in body axes (rad/s²). Body vectors transform as `reference = q.matrix * body`.
+Quaternions q and −q represent the same rotation. Input normalization handles
+large finite scales; a zero/non-finite quaternion is rejected.
+
+`AttitudeProvider.checkedAttitude` verifies exact frame identities and epoch.
+`AttitudeOrientationProvider` adapts the physical state to the frame system:
+its reference-to-body rotation is q conjugate, and its coordinate-map angular
+velocity and acceleration are the negatives of the physical body rates.
+The adapter requires angular acceleration, so missing derivatives never silently
+become zero. `OrientationAttitudeProvider` performs the reverse conversion and
+supports existing planetary and local-orbital orientation providers.
+
+`FrameTree.registerSpacecraftFrame` registers the provider's exact body-frame
+identity. Construct that frame with the inertial reference as its parent, then
+supply the spacecraft centre-state provider and attitude provider. The existing
+origin-acceleration policy still applies. As with other frame providers, a provider
+must not capture its owning tree strongly. Forces rotate as free vectors; centre
+translation and frame-rate terms are used for point-state transforms, not thrust.
+
+## Prescribed attitudes
+
+`InertialHoldAttitudeProvider` keeps a fixed body-to-reference orientation and
+supplies zero angular rates. `UniformSpinAttitudeProvider` prescribes constant
+physical spin in body axes with analytic quaternion evolution.
+
+`TrackingAttitudeProvider` supports target pointing, velocity tracking (relative
+to an optional moving target), and nadir pointing toward a supplied centre or the
+reference origin. Body X follows that direction; body Z follows the projected
+explicit roll-reference vector, and Y = Z × X. Coincident targets, zero velocity
+and parallel roll references fail instead of selecting arbitrary axes. Inputs
+must share a physical origin as well as exact reference axes.
+
+Five-point derivatives of the rotation matrix supply angular velocity and
+acceleration. Provider coverage at epoch ±2*derivativeStep is required. The step
+must resolve the motion; it is an explicit numerical setting, not an accuracy
+certificate. Existing `LocalOrbitalOrientationProvider` laws and mounting rotations
+can also be adapted through `OrientationAttitudeProvider`.
+
+Prescribed attitude is a kinematic command. It does not certify that available
+hardware can realize the angular rates or torques.
+
+## Inertia, torques and control
+
+`RigidBodyInertia` represents a constant centre-of-mass tensor in body axes
+(kg m²), including off-diagonal entries. Its parameters are tensor entries, not
+unsigned products of inertia. Scaled Cholesky validation requires positive
+definiteness; second-moment positive-semidefiniteness enforces the physical
+principal-moment triangle inequalities with a small floating-point allowance.
+Planar mass distributions are allowed; singular rotational inertia is rejected.
+The same factorization solves torque-to-angular-acceleration systems without
+forming an inverse. Angular momentum and kinetic energy are exposed for checks.
+
+`TorqueModel` evaluates a pure `TorqueContribution` about the centre of mass in
+body axes (N m). `RotationalEvaluationContext` carries the tensor, body identity,
+and inertial force context/physical origin. Torque output epochs and identities
+are checked. Translation is optional for standalone rotation and mandatory for
+models that need position or environmental fields.
+
+`RigidBodyDynamics` uses Euler's equation
+`I ωdot = τ − ω × (I ω)` and quaternion kinematics `qdot = 0.5 q * (ω, 0)`.
+The tensor remains constant, and internal wheel momentum is not inferred.
+`ConstantBodyTorque` is an explicit external torque input. `AttitudePDController`
+uses a shortest-rotation quaternion error and body-relative rate error, with a
+norm limit on commanded torque. The exact 180° tie is deterministic and invariant
+under quaternion sign. It is an ideal external torque controller; hardware
+allocation, sensor delays, wheel saturation/desaturation and power demand belong
+to additional models.
+
+`GravityGradientTorque` supplies the leading-order point-mass torque
+`3 μ/r³ * rHatBody × (I rHatBody)` using a checked moving centre. It assumes the
+spacecraft's extent is small relative to its distance from the source. It adds
+torque only; add a translational gravity model separately.
+
+`MagnetorquerTorque` evaluates a bounded commanded body dipole (A m²) against an
+explicit `MagneticFieldProvider` (tesla): `τBody = dipoleBody × fieldBody`.
+The sample's epoch, frame and physical origin are checked. A constant command also
+represents a residual dipole. `UniformMagneticField` is a simple prescribed field,
+not an inferred Earth magnetic model. Field gradients, hysteresis, electronics
+and electrical power are separate concerns.
+
+The equations follow [MIT rigid-body dynamics notes](https://ocw.mit.edu/courses/8-09-classical-mechanics-iii-fall-2014/6fe39e8d5ce4ce746ca256dfea665eda_MIT8_09F14_Chapter_2.pdf),
+[NASA gravity-gradient analysis](https://ntrs.nasa.gov/api/citations/19690028658/downloads/19690028658.pdf),
+and [NASA magnetic-torque specifications](https://ntrs.nasa.gov/api/citations/19690020961/downloads/19690020961.pdf).
+Implementations are native Swift and use no NASA implementation source.
+
+## Rotation and coupled propagation
+
+`RigidBodyAttitudePropagator` integrates rotation alone with an optional prescribed
+`SpacecraftStateProvider` for environmental torque inputs. It reports the attitude,
+angular acceleration, energy, reference-frame angular momentum and numerical work.
+`AttitudePropagationOptions` supplies angle/rate tolerances, step bounds, sampled
+rotation-per-step limits and work budgets. Accuracy presets change local tolerances;
+explicit settings remain authoritative.
+
+The native Dormand–Prince 5(4) method compares embedded physical quaternion angles
+with q/−q equivalence, angular velocities and quaternion norm drift. Stage vector
+transforms use a unit quaternion while quaternion derivatives retain the raw RK
+state. Accepted states normalize the quaternion without a sign reset. A sampled
+angular-speed step limiter avoids advancing too far through rapid rotation. These
+are local numerical controls, not a guarantee of global physical accuracy.
+
+`CoupledSpacecraftState` combines translation, mass and attitude at the same epoch
+and reference frame. `SpacecraftWrenchModel` returns force in reference axes, torque
+in body axes and reservoir mass rate from one physical model. `BodyMountedThruster`
+rotates the spacecraft force direction with the actual attitude, contributes
+`leverArmBody × forceBody`, and consumes propellant using an explicit effective
+exhaust velocity. The direction is force on the spacecraft, not exhaust direction.
+
+`CoupledSpacecraftDynamics` composes translational forces, torque models and
+wrenches. `CoupledSpacecraftPropagator` evolves position, velocity, propellant,
+quaternion and angular velocity at the same RK stages. This lets an off-centre
+engine rotate its own inertial thrust direction during a burn. Separate attitude
+and translation provider views support frames, sampling and event queries.
+
+For prescribed attitude, `BodyMountedThruster.forceModel(attitude:)` integrates
+translation and fuel through the existing force API, including its dry-boundary
+interface. The adapter does not integrate lever-arm torque. Use the coupled wrench
+for that; do not add both representations of the same engine to coupled dynamics.
+
+The current rigid-body approximation holds inertia and centre of mass fixed even
+when the propellant reservoir changes. Changing mass geometry, internal reaction
+wheels, moving appendages and outflow angular-momentum models are not silently
+inferred. Propagation expects continuous models; split and reseed with the carried
+state at command discontinuities. Coupled fuel exhaustion fails explicitly; no
+automatic engine cutoff or torque schedule is inferred. Forward/backward immutable
+replay supports predictions and consistency checks, not physical fuel recovery.
+
+## Demonstration and validation
+
+Run the off-centre Earth-orbit engine example:
+
+```sh
+swift run --disable-sandbox AttitudeDynamicsDemo
+```
+
+It prints SI position, inertial force direction, physical body rate, quaternion and
+mass samples. The initial body +X engine force points along inertial +Y; its lever
+arm drives negative body-Z rotation and changes the force direction. Its coupled
+provider views also register a fully kinematic spacecraft frame.
+
+Swift Testing checks quaternion signs and frame derivatives, target/nadir/velocity
+tracking, full and scaled inertia solves, invalid tensors, an analytic torque-free
+symmetric top, asymmetric-body energy and inertial momentum conservation, constant
+principal-axis torque, bounded control, magnetic/gravity-gradient signs, prescribed
+and coupled thrust, independent Simpson integrals of the off-centre engine's
+translation, tighter-tolerance convergence, backward replay, contracts, dry firing
+and work-budget exhaustion.
diff --git a/Sources/CelMek/CelMek.docc/Algorithms.md b/Sources/CelMek/CelMek.docc/Algorithms.md
new file mode 100644
index 0000000..4ced2b0
--- /dev/null
+++ b/Sources/CelMek/CelMek.docc/Algorithms.md
@@ -0,0 +1,18 @@
+# Astronomical algorithms and references
+
+The original CelMek library contains VSOP87 planetary series, ELP2000-82b lunar
+series and a Goffin Pluto implementation.
+
+The public provider contracts, native frames, time scales, SI conversion and
+coverage are described in . Approximation policies and measured
+error are described in and .
+
+## Original bibliography
+
+The retired Antora documentation cited the following works. Its BibTeX entries
+are preserved in `Documentation/bibliography.bib` in the repository.
+
+- Jean Meeus, *Astronomical Algorithms*, second edition, Willmann-Bell, 1998,
+ ISBN 0-943396-61-1.
+- E. Goffin, J. Meeus and C. Steyaert, *An accurate representation of the motion
+ of Pluto*, Astronomy and Astrophysics 155(2), 323–325, 1986.
diff --git a/Sources/CelMek/CelMek.docc/Attribution.md b/Sources/CelMek/CelMek.docc/Attribution.md
new file mode 100644
index 0000000..bd2872b
--- /dev/null
+++ b/Sources/CelMek/CelMek.docc/Attribution.md
@@ -0,0 +1,17 @@
+# Licensing and attribution
+
+CelMek is copyright Mattias Holm and distributed under Apache License 2.0.
+
+The repository's `LICENSE` is the authoritative package license. Third-party data
+and reference algorithms carry their own provenance and attribution in the relevant
+sources and fixture notes. ERFA-derived numerical routines and coefficient tables
+are isolated in the internal `ERFASwift` module under their BSD terms. The full
+copyright, license, and SOFA heritage notice is colocated at
+`Sources/ERFASwift/LICENSE.txt`, with a documentation copy at
+`Documentation/licenses/ERFA.txt`. CelMek depends on this module for Earth
+orientation and the full Fairhead TDB model; their public APIs remain in CelMek.
+
+Aerodynamics uses Yams, and the documentation build uses the Swift-DocC plugin.
+WMM2025 coefficients are distributed by NOAA; IGRF-14 coefficients are attributed
+to IAGA in the MagneticFields guide. Optional JPL/SPICE datasets are supplied
+separately and documented in