fullseye

polarization_render — SPECULAR polarization op

使い方

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.

詳しい使い方ガイド

参考(サンプルデータ・文献)

実行できる例(この op を実際に呼ぶ検証済みサンプル)

型が繋がる次の op(polsweep を入力に取れる)

polarization_separate · polarization_dolp_map · polarization_stokes

同カテゴリ(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.