Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989maph...29....1d&link_type=abstract
In International Council of Scientific Unions, Middle Atmosphere Program. Handbook for MAP, volume 29. Part 1: Extended Abstract
Physics
3
Radiation Distribution, Solar Activity, Solar Flux, Solar Radiation, Temporal Distribution, Ultraviolet Radiation, Solar Backscatter Uv Spectrometer, Solar Cycles, Solar Mesosphere Explorer, Solar X-Rays, Spatial Resolution
Scientific paper
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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