Radiation laws: Difference between revisions
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#The four physical laws or equations that are most commonly used to explain the [[emission]] of [[radiation]]: 1) [[Kirchhoff's law]]; 2) [[Planck's radiation law|Planck's law]]; 3) [[Stefan–Boltzmann law]]; and 4) [[Wien's displacement law]].<br/> Of these, 1) and 2) are fundamental. The remaining two can be derived from 2).<br/> | |||
#All of the more inclusive assemblage of empirical and theoretical laws describing all manifestations of radiative phenomena, for example, [[Bouguer–Lambert law]], [[Lambert's law]], [[Stefan–Boltzmann law|Stefan– Boltzmann law]], etc. | |||
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Latest revision as of 04:48, 27 March 2024
- The four physical laws or equations that are most commonly used to explain the emission of radiation: 1) Kirchhoff's law; 2) Planck's law; 3) Stefan–Boltzmann law; and 4) Wien's displacement law.
Of these, 1) and 2) are fundamental. The remaining two can be derived from 2). - All of the more inclusive assemblage of empirical and theoretical laws describing all manifestations of radiative phenomena, for example, Bouguer–Lambert law, Lambert's law, Stefan– Boltzmann law, etc.
