Radiation Intensity Thermodynamics

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A black body is a diffuse emitter that radiates energy according to the Stefan-Boltzmann law, expressed as σT^4. The intensity of radiation is influenced by the angle between the emitting surface and the observer, leading to a cosine dependence, which is a characteristic of Lambertian sources. This relationship arises because the effective area for radiation decreases as the angle increases, which is reflected in the formula for radiation intensity. The solid angle plays a crucial role in determining the distribution of intensity across the hemisphere. Understanding these principles clarifies the relationship between radiation intensity and angular dependence.
Chacabucogod
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So I understand that a black body is a diffuse emitter, and that it radiates energy at a rate of σT^4.
I also understand the correspondence between a solid angle and the superficial area of a sphere.

<br /> dS=r^2sin(θ)dθd\phi=\frac{ds}{r^2}=d\omega=\frac{dAcos(\alpha)}{r^2}<br />

What I don't understand is how they get to the formulation for intensity of radiation.

Why is the intensity of radiation proportional to the cos of the angle between the two areas? Isn't the intensity the same for every part of the half sphere since it's a black body? Why is it proportional to the solid angle? The area is proportional to the solid angle right?

The formula for Radiation Intensity is:

<br /> I_e(θ,\phi)=\frac{\frac{dQ}{dt}}{dA*cos(θ)sin(θ)dθd\phi}<br />
 
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Alright! Thank you! Now I know.
 

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