- #71
Philip Koeck
- 781
- 218
I completely agree with that, but I can't see how to apply that to emission from a black body. The surface of a black body gives off radiation from its surface. No energy is flowing through the surface as far as I can see.vanhees71 said:What's observed is the energy density or in this case the energy-current density (Poynting vector). Given the Poynting vector ##\vec{S}## the energy flowing through an arbitrarily oriented surface per unit time (power) is given by
$$P(t)=\int_A \mathrm{d}^2 \vec{f} \cdot \vec{S}(t,\vec{x}).$$
I'd really like to focus the discussion on thermal emission. So no scattering or reflection.
Unfortunately the Wiki shared by Sophie seems to jump between these topics and many sources only discuss scattering, as pointed out by Sophie.
What it is clear, I think is the following:
A black body is a Lambertian emitter and it always looks flat no matter what shape it is.
For example a sphere looks like a disk. (See several statements in the Wiki and other sources.)
This means (to me) that the current per solid angle and projected surface area is independent of θ.
The above means that the current per solid angle and actual surface area is proportional to cos(θ).
I believe the above statement is Lambert's law for emission, but I might be wrong.
Based on the above statement I argued in post 63 that Lambert's law is not due to the projection being smaller than the actual surface by a factor cos(θ), but that it has to come from the properties of the "elementary emitters", whatever they might be.
I'd really like to know what people think of this argument
An afterthought:
If I don't assume that the "elementary sources" sit on the surface, but rather in a small volume just below the surface, then I would get the cos-dependence even for isotropic emission (on average) from the individual sources.
Maybe that's a better model.
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