NASA NTRS · 19900018846
Solar UV variability
Abstract
Measurements from the Solar Backscatter Ultraviolet (SBUV) provide solar UV flux in the 160 to 400 nm wavelength range, backed up by independent measurement in the 115 to 305 nm range from the Solar Mesosphere Explorer (SME). The full disc UV flux from spatially resolved measurements of solar activity was modeled, which provides a better understanding of why the UV variations have their observed temporal and wavelength dependencies. Long term, intermediate term, and short term variations are briefly examined.
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Donnelly, Richard F.. 1989-09-01. Solar UV variability. https://ntrs.nasa.gov/citations/19900018846
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