Emissive power of blackbody is directly proportional to.....??
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The Stefan–Boltzmann law, also known as Stefan's law, states that the total energy radiated per unit surface area of a black body in unit time (known variously as the black-body irradiance, energy flux density, radiant flux, or the emissive power), j*, is directly proportional to the fourth power of the black body's ...
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itsaadil111:
then which is correct A) T^4 B) T^-4 C)lambda^4 D) lambda^-4??
option d is correct
thanks
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