Solar spectrum: Difference between revisions

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That part of the [[electromagnetic spectrum]] occupied by the wavelengths of [[solar radiation|solar  radiation]].<br/> The shape is well represented by the continuum [[emission]] from a [[blackbody]] with [[temperature]]  near 5700 K superimposed with [[Fraunhofer lines|Fraunhofer absorption lines]].
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== solar spectrum ==
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<div class="definition"><div class="short_definition">That part of the [[electromagnetic spectrum]] occupied by the wavelengths of [[solar radiation|solar  radiation]].</div><br/> <div class="paragraph">The shape is well represented by the continuum [[emission]] from a [[blackbody]] with [[temperature]]  near 5700 K superimposed with [[Fraunhofer lines|Fraunhofer absorption lines]].</div><br/> </div>
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Latest revision as of 06:21, 30 March 2024

That part of the electromagnetic spectrum occupied by the wavelengths of solar radiation.
The shape is well represented by the continuum emission from a blackbody with temperature near 5700 K superimposed with Fraunhofer absorption lines.

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