18-months of UV irradiance observations from the Solar Mesosphere Explorer

Details 18-months of UV irradiance observations from the Solar Mesosphere Explorer 18-months of UV irradiance observations from the Solar Mesosphere Explorer

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984georl..11...54l&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 11, Jan. 1984, p. 54-56.

Physics

21

Irradiance, Solar Atmosphere, Stellar Spectrophotometry, Ultraviolet Spectra, Atmospheric Heating, Centimeter Waves, Lyman Alpha Radiation, Periodic Variations, Photochemical Reactions, Solar Mesosphere Explorer, Solar Rotation, Spectrum Analysis

Scientific paper

An instrument on the Solar Mesosphere Explorer has been making daily solar irradiance measurements in the 120-305 nm (UV) spectral interval since October 6, 1981. Calculations of the highest to lowest value of the irradiance within each solar rotation yield percent range values indicative of variations that are useful as input data for model calculations of stratosphere/mesosphere responses to short period solar variability, since solar radiation in the UV is largely responsible for the photochemical interactions and radiative heating of the stratosphere, mesosphere, and lower thermosphere.

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