dichromatic_render — SPECULAR reflectance op

• Data kinds: normalmap → rgbimage

• Call: import fullseye as fs; fs.ledger.dichromatic_render(normals, albedo_rgb=(0.8, 0.55, 0.35), light=(0.3, 0.2, 1.0), illuminant_rgb=(1.0, 1.0, 1.0), view=(0.0, 0.0, 1.0), specular=0.25, model='blinn_phong', shininess=32.0, roughness=0.3, f0=0.04, ambient=0.0) (to call the implementation directly, import specularity; specularity.dichromatic_render(normals, albedo_rgb=(0.8, 0.55, 0.35), light=(0.3, 0.2, 1.0), illuminant_rgb=(1.0, 1.0, 1.0), view=(0.0, 0.0, 1.0), specular=0.25, model='blinn_phong', shininess=32.0, roughness=0.3, f0=0.04, ambient=0.0); from the registry, opsspecular.get("dichromatic_render"))

Usage

Forward dichromatic model: render a known highlight so a separation can be checked against it. → (H, W, 3).

I = albedo_rgb * max(n.l, 0) + specular * lobe(n) * illuminant_unit, the body term coming straight from photometric.render_lambertian (called, not re-implemented, so the two modules cannot drift apart in convention) and the interface term carrying the illuminant colour, which is what makes the image obey the dichromatic model exactly.

*albedo_rgb* may be a single (3,) colour — the single-material case that specular_diffuse_split handles without help — or an (H, W, 3) map, which is the textured case that needs body_rgb passed to the split.

*model* selects the lobe: "blinn_phong" (*shininess*) or "microfacet" (*roughness*, *f0*). Both are available on purpose: the separation operators must be blind to the lobe shape, and swapping the model is how that is tested rather than asserted.

This is a shading model, not light transport. No interreflection, no cast shadow, no subsurface term, no occlusion between pixels — the same

boundary visiondesign draws. Its purpose is a synthetic image whose decomposition is known exactly.

Raises ValueError: geometry problems as in brdf_blinn_phong; *albedo_rgb* is neither (3,) nor (H, W, 3); *specular* or *ambient* is negative, non-finite, a string or a bool; *model* is not in BRDF_MODELS.

Detailed usage guide

• specular_photometric family guide

References (sample data, literature)

• Sample-data catalog (download URLs / licences) — 2-D uses skimage.data (BSD/public domain) plus synthetic images; 3-D lists download URLs for real data sources (Stanford, PDS, …).

• Operator provenance and references — the sources of the research/methods this op family came from.

• The canonical algorithm (author, year) and its uses are named in the family usage guide above.

Runnable examples (verified samples that actually call this op)

• specular_photometric — py -3.11 examples/specular_photometric.py

Ops the type connects to (they accept rgbimage as input)

specular_diffuse_split · specular_coefficient_map · specular_free_transform · illuminant_from_dichromatic_planes

Same category (reflectance)

brdf_blinn_phong · brdf_microfacet


*Provenance: specularity.py — SPECULAR operator registry. This per-op note is generated by tools/opdocs.py md (do not hand-edit).*

© 2026 Kazufumi Furuse — Fullseye operator documentation. Licensed under Apache-2.0.