Math 2.0

Classical thermodynamics, heat transfer Thermal radiation Proposition

Lambert's cosine law

Builds on Thermal radiationBlack body

Statement

Let a small surface element of area dAdA emit or reflect radiation with a radiance LL. Assume that LL 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:

  1. The radiant intensity in a direction at angle θ\theta from the surface normal is I(θ)=L dAcos⁡θ=I(0)cos⁡θI(\theta) = L \, dA \cos\theta = I(0) \cos\theta.
  2. The total power leaving the element per unit area, its exitance, is M=πLM = \pi L.

Remarks

Proof: seen from a direction at angle θ\theta, the element has projected area dAcos⁡θdA \cos\theta, which gives clause 1. For clause 2, integrate over the hemisphere with dΩ=sin⁡θ dθ dϕd\Omega = \sin\theta \, d\theta \, d\phi: M=∫02π∫0π/2Lcos⁡θsin⁡θ dθ dϕ=2πL⋅12=πL.M = \int_0^{2\pi} \int_0^{\pi/2} L \cos\theta \sin\theta \, d\theta \, d\phi = 2\pi L \cdot \tfrac12 = \pi L. The factor is π\pi, not 2π2\pi, because of the cosine.

Example: a black body is such a surface, so its exitance is π\pi 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

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  1. Black body concept
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Where this leads

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Further reading

  1. Web https://en.wikipedia.org/wiki/Lambert%27s_cosine_law
About this page
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Kindstatement, proposition
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AboutThermal radiation
UsesThermal radiation, Black body
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Changed3 November 2026

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