FA-55082 / Astronomical coordinate conventions / Member archive
Stokes linear basis: Stokes intensity normalization imports a half-sum convention from another adapter · case 02
The adapter reports an incorrect intensity while other fields remain valid.
Case contract
Two real linear-feed correlations XX,YY and real/imaginary XY define stipulated Stokes I=XX+YY,Q=XX-YY,U=2re,V=-2im. Reversing feed labels negates Q and V, leaves I and U unchanged. Output rotated fields model only that feed swap. Output fields are defined by: intensity = d['xx']+d['yy']; linear_q = d['xx']-d['yy']; linear_u = 2*d['re']; circular_v = -2*d['im']; swapped_q = d['yy']-d['xx']; swapped_v = 2*d['im']
Why this case matters
Catalog, detector, sky-coordinate, and spectroscopy adapters must preserve the association between numeric coordinates and their declared reference conventions.
One recorded failure
Sample boundary fixtureThis sample comes from the broken implementation of a controlled reproducer.
| Boundary fixture | Actual | Expected | Outcome |
|---|---|---|---|
| astronomical fixture 0 | {"circular_v": -8, "intensity": 6.0, "linear_q": 6, "linear_u": 4, "swapped_q": -6, "swapped_v": 8} | {"circular_v": -8, "intensity": 12, "linear_q": 6, "linear_u": 4, "swapped_q": -6, "swapped_v": 8} | Failed |
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