def test_GeocentricSolarEcliptic_raises_error_nonscalar_obstime():
with pytest.raises(ValueError) as excinfo:
gcrs = GCRS(ra="02h31m49.09s", dec="+89d15m50.8s", distance=200 * u.km)
gcrs.transform_to(
GeocentricSolarEcliptic(obstime=Time(["J3200", "J2000"])))
assert ("To perform this transformation the "
"obstime Attribute must be a scalar." in str(excinfo.value))
def test_GeocentricSolarEcliptic_against_data():
gcrs = GCRS(ra="02h31m49.09s", dec="+89d15m50.8s", distance=200 * u.km)
gse = gcrs.transform_to(GeocentricSolarEcliptic(obstime=J2000))
lon = 233.11691362602866
lat = 48.64606410986667
assert_quantity_allclose(gse.lat.value, lat, atol=1e-7)
assert_quantity_allclose(gse.lon.value, lon, atol=1e-7)
def validate_GCRF_to_ITRF(r_vec, v_vec):
# Compute for the norm of position and velocity vectors
r_norm, v_norm = [norm(vec) for vec in [r_vec, v_vec]]
R = Earth_poliastro.R.to(u.m).value
# Correction factor to normalize position and velocity vectors
k_r = R / r_norm if r_norm != 0 else 1.00
k_v = 1 / v_norm if v_norm != 0 else 1.00
# Make a position vector who's norm is equal to the body's radius. Make a
# unitary velocity vector. Units are in [m] and [m / s].
rx, ry, rz = [float(k_r * r_i) for r_i in r_vec]
vx, vy, vz = [float(k_v * v_i) for v_i in v_vec]
# orekit: build r_vec and v_vec wrt inertial body frame
xyz_orekit = Vector3D(rx, ry, rz)
uvw_orekit = Vector3D(vx, vy, vz)
coords_GCRF_orekit = TimeStampedPVCoordinates(J2000_OREKIT, xyz_orekit,
uvw_orekit)
# orekit: build conversion between GCRF and ITRF
GCRF_TO_ITRF_OREKIT = GCRF_FRAME_OREKIT.getTransformTo(
ITRF_FRAME_OREKIT,
J2000_OREKIT,
)
# orekit: convert from GCRF to ITRF using previous built conversion
coords_ITRF_orekit = (GCRF_TO_ITRF_OREKIT.transformPVCoordinates(
coords_GCRF_orekit).getPosition().toArray())
coords_ITRF_orekit = np.asarray(coords_ITRF_orekit) * u.m
# poliastro: build r_vec and v_vec wrt GCRF
xyz_poliastro = CartesianRepresentation(rx * u.m, ry * u.m, rz * u.m)
coords_GCRS_poliastro = GCRS_poliastro(xyz_poliastro)
# poliastro: convert from inertial to fixed frame at given epoch
coords_ITRS_poliastro = (coords_GCRS_poliastro.transform_to(
ITRS_poliastro(
obstime=J2000_POLIASTRO)).represent_as(CartesianRepresentation).xyz
)
# Check position conversion
assert_quantity_allclose(
coords_ITRS_poliastro,
coords_ITRF_orekit,
atol=1e-3 * u.m,
rtol=1e-2,
)
def test_round_trip_from_GeocentricSolarEcliptic_gives_same_results():
gcrs = GCRS(ra="02h31m49.09s", dec="+89d15m50.8s", distance=200 * u.km)
gse = gcrs.transform_to(GeocentricSolarEcliptic(obstime=Time("J2000")))
gcrs_back = gse.transform_to(GCRS(obstime=Time("J2000")))
assert_quantity_allclose(gcrs_back.dec.value, gcrs.dec.value, atol=1e-7)
assert_quantity_allclose(gcrs_back.ra.value, gcrs.ra.value, atol=1e-7)
