Difference between revisions of "Dictionary:Stefan-Boltzmann’s law"

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(shte&#x2019; fan b&#x014D;ltz&#x2019; monz) The amount of energy radiated by a blackbody per unit time per unit area is proportional to the fourth power of the temperature in kelvin.
 
(shte&#x2019; fan b&#x014D;ltz&#x2019; monz) The amount of energy radiated by a blackbody per unit time per unit area is proportional to the fourth power of the temperature in kelvin.
 
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Revision as of 16:36, 18 October 2017

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(shte’ fan bōltz’ monz) The amount of energy radiated by a blackbody per unit time per unit area is proportional to the fourth power of the temperature in kelvin.