mirror of
https://github.com/zvx-echo6/central.git
synced 2026-08-26 09:21:36 +00:00
Adds a new SourceAdapter that publishes the current sub-satellite point
(lon, lat, alt) plus velocity + heading for every tracked NORAD ID every
60s on subject central.sat.position.<norad_id>. Complement to v0.11.1's
satpass_predict (observer-anchored pass alerts): sat_positions is the
GLOBAL counterpart, "where is sat X right now?" rather than "when does
sat X pass over observer Y?". Neither replaces the other.
data_class=telemetry surfaces these on /telemetry, not /events (60s ticks
across ~190 sats would drown discrete-event signal). Severity 1. Geo
centroid = sub-sat point so consumers can plot the satellite directly.
Refactors satpass_predict.py to import its pure SGP4 helpers from a new
sat_common.py module (matches the wfigs_common / swpc_common precedent).
Moved: EARTH_RADIUS_KM, gmst_rad, eci_to_ecef, subsatellite_point (4
symbols, ~25 lines of pure math). Observer-specific helpers stay in
satpass_predict.py. Existing satpass_predict tests pass unchanged.
CENTRAL_SAT stream max_bytes bumped from 1 GiB to 5 GiB to accommodate
the additional ~1.9 GiB/week of position events. STREAM_CATEGORY_DOMAINS
extended from ("tle", "pass") to ("tle", "pass", "position") so the
retention sweep covers position events.
Ships disabled (enabled=false) -- celestrak_tle must be enabled and have
polled at least once for sat_positions to have TLE data to propagate.
Co-Authored-By: Claude Opus 4.7 (1M context) <noreply@anthropic.com>
114 lines
4.3 KiB
Python
114 lines
4.3 KiB
Python
"""Tests for the shared satellite-math helpers extracted in v0.12.0.
|
|
|
|
These pin the public API surface (no leading underscores) and the numerical
|
|
behavior at known reference points. They duplicate some property tests from
|
|
test_satpass_predict.py by design -- those test the helpers via internal
|
|
re-exports (aliased imports), while these test the module's published
|
|
interface directly. If the public names ever drift or get renamed, these
|
|
fail first.
|
|
"""
|
|
|
|
from __future__ import annotations
|
|
|
|
import math
|
|
from datetime import datetime, timezone
|
|
|
|
import pytest
|
|
from sgp4.api import Satrec, jday
|
|
|
|
from central.adapters.sat_common import (
|
|
EARTH_RADIUS_KM,
|
|
eci_to_ecef,
|
|
gmst_rad,
|
|
subsatellite_point,
|
|
)
|
|
|
|
|
|
# Live TLE from the v0.11.0 stations fixture, ISS (NORAD 25544).
|
|
_ISS_L1 = "1 25544U 98067A 26159.80410962 .00007129 00000+0 13425-3 0 9999"
|
|
_ISS_L2 = "2 25544 51.6336 341.5878 0006923 148.5365 211.6039 15.49672912570453"
|
|
_REF = datetime(2026, 6, 9, 7, 0, 0, tzinfo=timezone.utc)
|
|
|
|
|
|
class TestEarthRadius:
|
|
def test_value_matches_wgs84_equatorial(self):
|
|
assert EARTH_RADIUS_KM == pytest.approx(6378.137, abs=1e-6)
|
|
|
|
|
|
class TestGmstRad:
|
|
def test_returns_value_in_canonical_range(self):
|
|
val = gmst_rad(2460835.0, 0.5) # arbitrary post-2000 JD
|
|
assert 0.0 <= val < 2.0 * math.pi
|
|
|
|
def test_monotonic_within_a_day(self):
|
|
"""GMST advances ~2π per sidereal day. Two samples 6h apart must
|
|
differ by roughly π/2 (modulo wraparound)."""
|
|
v0 = gmst_rad(2460835.0, 0.0)
|
|
v1 = gmst_rad(2460835.0, 0.25)
|
|
delta = (v1 - v0) % (2.0 * math.pi)
|
|
# 6h sidereal angle is slightly more than π/2 (sidereal day < solar day).
|
|
assert math.pi / 2.0 < delta < math.pi / 2.0 + 0.02
|
|
|
|
|
|
class TestEciToEcef:
|
|
def test_zero_rotation_is_identity(self):
|
|
result = eci_to_ecef((100.0, 200.0, 300.0), 0.0)
|
|
assert result == pytest.approx((100.0, 200.0, 300.0))
|
|
|
|
def test_rotation_preserves_magnitude(self):
|
|
"""Rotation about the z-axis preserves the vector norm."""
|
|
pos = (3000.0, 4000.0, 5000.0)
|
|
rot = eci_to_ecef(pos, math.pi / 3.0)
|
|
mag_in = math.sqrt(sum(c * c for c in pos))
|
|
mag_out = math.sqrt(sum(c * c for c in rot))
|
|
assert mag_out == pytest.approx(mag_in, rel=1e-12)
|
|
|
|
def test_z_component_unaffected(self):
|
|
"""Earth-rotation axis is z; z component never changes under GMST rotation."""
|
|
_, _, z = eci_to_ecef((1.0, 2.0, 42.0), 1.3)
|
|
assert z == 42.0
|
|
|
|
|
|
class TestSubsatellitePoint:
|
|
def test_north_pole_returns_pole(self):
|
|
lon, lat, alt = subsatellite_point((0.0, 0.0, 7000.0))
|
|
assert lat == pytest.approx(90.0)
|
|
assert alt == pytest.approx(7000.0 - EARTH_RADIUS_KM)
|
|
|
|
def test_equator_lon_zero(self):
|
|
lon, lat, alt = subsatellite_point((EARTH_RADIUS_KM + 400.0, 0.0, 0.0))
|
|
assert lon == pytest.approx(0.0)
|
|
assert lat == pytest.approx(0.0)
|
|
assert alt == pytest.approx(400.0, abs=1e-6)
|
|
|
|
def test_equator_lon_90_east(self):
|
|
lon, lat, alt = subsatellite_point((0.0, EARTH_RADIUS_KM + 400.0, 0.0))
|
|
assert lon == pytest.approx(90.0)
|
|
assert lat == pytest.approx(0.0)
|
|
|
|
def test_lon_normalised_into_180_range(self):
|
|
"""A satellite over the antimeridian (-y axis) reads as -90°, never +270°."""
|
|
lon, _, _ = subsatellite_point((0.0, -(EARTH_RADIUS_KM + 400.0), 0.0))
|
|
assert -180.0 <= lon <= 180.0
|
|
assert lon == pytest.approx(-90.0)
|
|
|
|
|
|
class TestIssRoundTripViaSgp4:
|
|
"""End-to-end: TLE -> SGP4 ECI -> ECEF -> sub-sat point. Pins the math
|
|
against a known orbital configuration. Drift from this would mean the
|
|
helpers regressed in a way that affects production output."""
|
|
|
|
def test_iss_sub_sat_point_at_pinned_ref_time(self):
|
|
sat = Satrec.twoline2rv(_ISS_L1, _ISS_L2)
|
|
jd, fr = jday(_REF.year, _REF.month, _REF.day,
|
|
_REF.hour, _REF.minute, _REF.second)
|
|
err, pos_eci, _ = sat.sgp4(jd, fr)
|
|
assert err == 0
|
|
pos_ecef = eci_to_ecef(pos_eci, gmst_rad(jd, fr))
|
|
lon, lat, alt = subsatellite_point(pos_ecef)
|
|
# ISS inclination 51.6° -- lat must lie within bounds
|
|
assert -52.0 <= lat <= 52.0
|
|
# lon in valid range
|
|
assert -180.0 <= lon <= 180.0
|
|
# ISS altitude ~400-420 km
|
|
assert 380.0 <= alt <= 460.0
|