| solar spectrum |
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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| solar spectrum |
The intensity variation of sunlight across its spectral range.
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| solar spectrum |
Radiation originating from the sun, including ultraviolet, visible, and near-infrared radiation. Approximately 99% of solar energy lies between wavelengths of 0.3 to 3.5 micrometers.
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