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Stefan-Boltzmann's law of radiation -- Stefan-Boltzmannsches Strahlungsgesetz

According of Stefan-Boltzmann's law, the energy emitted by a black body per unit area and unit time is proportional to the power "four" of the absolute temperature of the body.

Nach dem Stefan-Boltzmann-Gesetz ist die Energie, die von einem schwarzen Körper per Flächeneinheit und Zeiteinheit emittiert wird, proportional zur Leistung "vier" der absoluten Temperatur des Körpers.

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Uploaded on March 28, 2012
Taken on January 21, 2011