Скачать или смотреть Part 10 "Stefan Boltzmann law" and "Wien displacement law"?

For an ideal absorber/emitter or black body, the Stefan–Boltzmann law states that the total energy radiated per unit surface area per unit time (also known as the radiant exitance) is directly proportional to the fourth power of the black body's temperature, T

Wien's law or Wien's displacement law, named after Wilhelm Wien, was derived in the year 1893 which states that black body radiation has different peaks of temperature at wavelengths that are inversely proportional to temperatures.

Topics to be covered:
Stefan Boltzmann law
Numerical of Stefan Boltzmann law
Wien Displacement Law

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