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Exercise · Q14

Q.Define the absorptive power and the emissive power of a surface at a given temperature and wavelength. State Kirchhoff's law of radiation connecting them, and use it to explain why a good absorber of radiation (such as a black, lamp-soot-coated surface) is also necessarily a good emitter.

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The absorptive power (absorptivity) aa of a surface is the fraction of the total radiant energy incident on it that the surface actually absorbs, with 0≤a≤10 \le a \le 1; a perfectly black surface has a=1a = 1, absorbing all incident radiation. The emissive power (emissivity) ee of a surface is a measure of how efficiently it radiates thermal energy, expressed relative to an ideal black body at the same temperature, with 0≤e≤10 \le e \le 1; a perfectly black surface has e=1e = 1, the maximum possible emissive power.

Kirchhoff's law of radiation states that, for any surface in thermal equilibrium, the ratio e/ae/a (its emissive power divided by its absorptive power) is the same fixed value for every surface at a given wavelength and temperature, equal to the emissive power of a perfectly black body at that same wavelength and temperature. Since this ratio is the same universal value for every surface, a surface cannot have a large aa together with a small ee, or vice versa: if aa is close to 11 (a good absorber), ee must also be close to 11 (a good …

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