Unformatted text preview: • Amount of energy in an electromagnetic wave that passes perpendicularly through a unit surface area/ unit time Inverse square law • Rate at which solar flux decreases with increasing distance Blackbody : something that emits or absorbs electromagnetic radiation with 100% efficiency at all wavelengths Blackbody radiation: radiation emitted by a blackbody, characteristic wavelength distribution that depends on body’s absolute temp. Wien’s law: states that flux of radiation emitted by a blackbody reaches its peak value at a wavelength which depends inversely on body’s absolute temp. Photosphere: surface layer where sun emits most of its energy StefanBoltzmann law: states that the energy flux emitted by a blackbody is related to the fourth power of the body’s absolute temp....
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 Spring '11
 WilliamMcCoy
 Light, Photon Energy

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