Difference between revisions of "Solar radiation"

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'''Solar radiation''' is a general term for the visible and near visible (ultraviolet and near-infrared) [[electromagnetic radiation]] that is emitted by the [[sun]].  
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'''Solar radiation''' is a general term for the [[electromagnetic radiation]] that is emitted by the [[sun]]. While the [[sun]] emits energy at a wide range of frequencies, peak radiance is within the visible range of the spectrum. 
  
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Solar radiation has a spectral, or wavelength, distribution that corresponds to different energy levels.  Short wavelength radiation has a higher energy than long-wavelength radiation.
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Solar radiation has a spectral, or wavelength, distribution that corresponds, roughly, to a black body curve.  Short wavelength radiation has a higher energy than long-wavelength radiation.
 
[[category:energy]]
 
[[category:energy]]

Revision as of 20:58, April 22, 2008

Solar radiation is a general term for the electromagnetic radiation that is emitted by the sun. While the sun emits energy at a wide range of frequencies, peak radiance is within the visible range of the spectrum.

Solar radiation has a spectral, or wavelength, distribution that corresponds, roughly, to a black body curve. Short wavelength radiation has a higher energy than long-wavelength radiation.