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Solar UV variabilityMeasurements 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.
Document ID
19900018846
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Donnelly, Richard F.
(National Oceanic and Atmospheric Administration Boulder, CO, United States)
Date Acquired
September 6, 2013
Publication Date
September 1, 1989
Publication Information
Publication: International Council of Scientific Unions, Middle Atmosphere Program. Handbook for MAP, volume 29. Part 1: Extended Abstracts, International Symposium on Solar Activity Forcing of the Middle Atmosphere. Part 2: MASH Workshop, Williamsburg, 1986
Subject Category
Solar Physics
Accession Number
90N28162
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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