polarization opimage2d × image2d → polsweepimport fullseye as fs; fs.ledger.polarization_render(diffuse, specular, angles_deg=(0.0, 45.0, 90.0, 135.0), azimuth_deg=0.0) (実装を直接呼ぶなら import specularity; specularity.polarization_render(diffuse, specular, angles_deg=(0.0, 45.0, 90.0, 135.0), azimuth_deg=0.0)、台帳から引くなら opsspecular.get("polarization_render"))Forward model of a polariser sweep: turn a known split into the frames a polarisation camera would record. → (N, H, W).
I(t) = 0.5 * diffuse + specular * cos^2(t - azimuth). The diffuse term is
treated as completely unpolarised, so it contributes half its radiance at
every analyser angle; the specular term is treated as completely linearly
polarised at azimuth_deg, so it follows Malus’s law. Those are the two
assumptions :func:polarization_separate inverts, and rendering with them
is how the inversion gets a ground truth to be exact against.
Physically the assumptions hold near Brewster’s angle for a dielectric and fail at normal incidence; the module docstring says where. This operator does not model the incidence angle at all — it takes the two radiance maps you specify and produces the sweep they imply.
Raises ValueError: diffuse / specular are not 2-D arrays of the
same shape, or are complex / masked / non-finite / string-typed; either has
a negative value (a negative radiance is not a scene); angles_deg has
fewer than 3 entries or does not determine the three unknowns.
py -3.11 examples/poc_polarization_specular.pypy -3.11 examples/specular_photometric.pypolsweep を入力に取れる)polarization_separate · polarization_dolp_map · polarization_stokes
polarization)polarization_separate · polarization_dolp_map · polarization_stokes
Provenance: specularity.py — SPECULAR operator registry. この per-op ノートは tools/opdocs.py md が自動生成(手編集しない)。
© 2026 Kazufumi Furuse — Fullseye operator documentation. Licensed under Apache-2.0.