Computer Science
Scientific paper
Jul 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sers.conf.....d&link_type=abstract
Proceedings of the Workshop on the Solar Electromagnetic Radiation Study for Solar Cycle 22, held in Boulder, CO, 3-7 Jun. 1991.
Computer Science
2
Atmospheric Composition, Atmospheric Temperature, Climate Change, Conferences, Electromagnetic Radiation, Environment Effects, Irradiance, Radiation Effects, Solar Cycles, Solar Flux, Solar Radiation, Solar Terrestrial Interactions, Spectral Emission, Sunlight, Atmospheric Heating, Climate, D Region, E Region, Extreme Ultraviolet Radiation, Gas Density, Infrared Radiation, Ozone, Solar Energy, Solar Spectra, Solar X-Rays, Stratosphere, Thermosphere, Ultraviolet Spectra
Scientific paper
The Solar Electromagnetic Radiation Study for Solar Cycle 22 (SOLERS22) is an international program for collaborative research of long-term changes in the solar total and spectral irradiance. SOLERS22 is project 1.2 of STEP Working Group 1, The Sun as a Source of Energy and Disturbance. Temporal variations (0.1 percent) in the total solar irradiance (S) are important because of their possible effects on climate. Changes in the solar ultraviolet (UV) flux (10 percent) modulate the ozone density and temperature in the stratosphere and mesosphere. Large-percentage fluctuations (100 percent) in the solar extreme-ultraviolet flux induce sizable changes in the ionosphere and thermosphere. Huge enhancements (X10, X100) in solar soft x-ray flux cause enhancements in ionization and heating in the ionospheric D and E regions. It is, therefore, important to know what these solar electromagnetic fluxes are, as a function of time, to determine the main solar energy inputs to the terrestrial atmosphere. The Workshop had 5 major topics (Parts): Total Solar Irradiance and Near-UV, Visible and Infrared Spectral Irradiance; Solar Activity and Proxy Measurements; Solar UV Spectral Irradiance; Solar EUV Spectral Irradiance; Solar X-Ray Spectral Irradiance.
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