lensrender optable → tableimport fullseye as fs; fs.ledger.trace_sensor_rays(system, pixel_xy_mm=None, pupil_xy_mm=None, wavelength_um=None, defocus_mm=0.0, fresnel=False, focus_mm=None) -> 'dict' (実装を直接呼ぶなら import lensrender; lensrender.trace_sensor_rays(system, pixel_xy_mm=None, pupil_xy_mm=None, wavelength_um=None, defocus_mm=0.0, fresnel=False, focus_mm=None) -> 'dict'、台帳から引くなら opsoptics.get("trace_sensor_rays"))Trace rays from sensor points through exit-pupil points backwards to object space -> dict.
pixel_xy_mm (M, 2) are points (x, y) in the image plane (lens-frame axes, the image is inverted); pupil_xy_mm (K, 2)
are points in the exit-pupil plane (default: 16 hexapolar samples of :func:exit_pupil_samples). All M x K
pairs are traced through every surface from the last to the first (Snell’s law at wavelength_um with the
dispersion of each medium, conics and aspheres, mirrors, the semi-diameters as apertures, total internal
reflection); the sensor plane is the system’s image plane (or the paraxial image of an object at focus_mm) moved by
defocus_mm along the light. The table has origin / direction (M, K, 3): where the ray leaves the first surface and
its unit direction into the scene (NaN where lost), transmission (M, K) - 1 for a ray that gets out, or with
fresnel=True the product of the unpolarised Fresnel transmittances of the refracting surfaces (no coating, no
absorption), 0 for a lost ray - vignetted (M, K) (any loss: a semi-diameter, a miss, TIR), tir, geometry_mm2
(cos^2(theta) / d^2 of the pupil sample seen from the sensor point, the weight of the irradiance integral), z_sensor_mm,
z_pupil_mm and wavelength_um. Reversibility is exact: a forward ray from raytrace.ray_bundle traced back from its
image point through its exit-pupil point returns to its entrance point (tested to 1e-9 mm and 1e-12 in direction).
optics の全 op は入力を検証してから計算する(黙って通さない):
_mm / _um / _deg / _mrad。mm と µm の取り違えは crash ではなく「もっともらしく間違った答え」なので、名前で防ぐ。大きさから単位を推測する処理は一切しない。ValueError — float('50') は成功してしまうため、未パースの設定値が長さとして通り抜ける(実測: thin_lens('50', '200') がもっともらしい 66.667 mm を返していた)。bool も True == 1 の暗黙昇格として拒否。ValueError(実数枠のみ。虚部の無言切り捨て・マスク剥がしを拒否)。NaN/Inf は全入力で ValueError。depth_of_field の過焦点距離以遠の far_mm = inf(それが過焦点距離の定義)と gaussian_beam のウエストでの wavefront_radius_mm = inf(平面波面の曲率半径)。どちらも有限の相棒(far_is_infinite / curvature_per_mm)を併せて返す。それ以外の無言 NaN/Inf は内部で検出して ValueError —「float64 が溢れた」と「答えが無限大」は別の主張なので、後者の顔で前者を返さない。optics.MAX_GRID(4096)、供給された場/PSF/開口は optics.MAX_FIELD_ELEMENTS(2^24)、ABCD 素子列は optics.MAX_SYSTEM_ELEMENTS(1024)、Zernike は MAX_ZERNIKE_TERMS(512)/ MAX_ZERNIKE_ORDER(40)/ MAX_ZERNIKE_BASIS(2^25)。小さな引数から巨大な内部確保が起きる経路(実測: n_max=40 × 4096² で 108 GB)を fail-closed で塞ぐ。| 物理的に不可能な状態も拒否: 偏光度 > 1 の Stokes ベクトル、負の透過率、負の強度、n- | m | が奇数などの不正な Zernike 添字。 |
py -3.11 examples/poc_photograph_through_prescription.pytable を入力に取れる)abcd_matrix · wavefront_stats · sfr_from_edge · paraxial_trace · seidel_coefficients · spot_stats · tolerance_analysis · wavefront_from_opd
lensrender)lens_scene · exit_pupil_samples · scene_radiance · render_scene_through_lens · bokeh_shape · render_ghost_overlay · render_compare_prescriptions
Provenance: lensrender.py — OPTICS 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.