Changes

Solar radiation has a spectral, or wavelength, distribution that corresponds, roughly, to a black body curve of the sun's surface temperature.  A black body curve graphically  represents radiation coming from a "perfect" emitter across a range of wavelengths, based on temperature.  Short wavelength radiation has a higher energy than long-wavelength radiation.

Solar radiation has a spectral, or wavelength, distribution that corresponds, roughly, to a black body curve of the sun's surface temperature.  A black body curve graphically  represents radiation coming from a "perfect" emitter across a range of wavelengths, based on temperature.  Short wavelength radiation has a higher energy than long-wavelength radiation.

[[category:energy]]

[[category:energy]]