Classical thermodynamics, heat transfer Thermal radiation Proposition
Lambert's cosine law
Builds on Thermal radiationBlack body
Statement
Let a small surface element of area emit or reflect radiation with a radiance . Assume that is the same in all directions of the hemisphere above the element. Here radiance is the power per unit area projected normal to the direction and per unit solid angle. Then:
- The radiant intensity in a direction at angle from the surface normal is .
- The total power leaving the element per unit area, its exitance, is .
Remarks
Proof: seen from a direction at angle , the element has projected area , which gives clause 1. For clause 2, integrate over the hemisphere with : The factor is , not , because of the cosine.
Example: a black body is such a surface, so its exitance is times its radiance, which turns Planck's radiance into the Stefan–Boltzmann exitance. Matte paper and fresh snow are nearly such surfaces, while a mirror or a glossy surface is not, and for them the cosine law fails.
Going deeper
For a student
Surfaces that obey the law are called Lambertian, or ideal diffuse. The law is the assumption behind view factors and radiosity methods, both in heat transfer and in computer graphics.
Reading path
To understand this page from the ground up, read these 3 pages in order. The foundations come first.
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- Black body concept
- Thermal radiation concept
- Lambert's cosine law statement
Where this leads
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Further reading
About this page
| Tag | XTXT8YSP5N |
|---|---|
| URI | m2://XTXT8YSP5N |
| Kind | statement, proposition |
| Writing | W0 stub |
| MSC | 80A21, 78A40 |
| Status | This copy of the site has no build data. Run m2 status XTXT8YSP5N. |
| About | Thermal radiation |
| Uses | Thermal radiation, Black body |
| Same as | |
| Changed | 3 November 2026 |
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