polarization op• 資料種類:polsweep → image2d
• 呼叫:import specularity; specularity.polarization_dolp_map(images, angles_deg=(0.0, 45.0, 90.0, 135.0), max_violation_frac=0.0)(或 opsspecular.get("polarization_dolp_map"))
逐像素的線偏振度。→ [0, 1] 的 (H, W)。
> 以下的詳細說明為原文 —— 摘要與標題已翻譯。
`sqrt(S1^2 + S2^2) / S0`, from the same sinusoid fit as
:func:polarization_separate. It answers the question that decides whether
a polariser is worth mounting at all: 1 means the light at that pixel is
fully linearly polarised and a crossed analyser extinguishes it completely,
0 means the polariser will only cost you a stop of exposure.
Being a ratio, it is invariant to exposure: scaling every frame by 1e-4,
1e4 or 1e8 moves it by at most 3.9e-16 (measured), which is what makes it
comparable across a production line where the lamps age. Not *bit*-
identical — the least-squares fit rounds differently at a different scale —
and the difference between "invariant" and "bit-identical" is the kind of
claim this library measures rather than asserts.
Pixels with zero total radiance have no degree of polarisation (every ratio
would be 0/0) and are returned as 0.0 rather than as NaN; that is a
convention, and it is stated here because a NaN spreading into a
thresholding routine is exactly the silent failure this library refuses.
Raises `ValueError: as :func:polarization_separate`.
• 範例資料目錄(下載 URL / 授權) —— 2-D 用 skimage.data(BSD/公有領域)加合成圖,3-D 給出真實資料源(Stanford/PDS 等)的下載 URL。
• 運算子來歷與參考文獻 —— 該運算子族所依據的研究/方法出處。
• 演算法的正典(作者・年份)與用途見上面的族使用指南。
• poc_polarization_specular — py -3.11 examples/poc_polarization_specular.py
• specular_photometric — py -3.11 examples/specular_photometric.py
image2d 作為輸入)polarization)polarization_render · polarization_separate · polarization_stokes
*Provenance: specularity.py — SPECULAR 運算子登記表。本條目由 tools/opdocs.py md 自動產生(請勿手動編輯)。*
© 2026 Kazufumi Furuse — Fullseye operator documentation. Licensed under Apache-2.0.