Brightness of a solar image, observed from a satellite in the visible spectral range

Details Brightness of a solar image, observed from a satellite in the visible spectral range Brightness of a solar image, observed from a satellite in the visible spectral range

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986fizao..22..431p&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Fizika Atmosfery i Okeana (ISSN 0002-3515), vol. 22, April 1986, p. 431-433. In Russian.

Astronomy and Astrophysics

Astronomy

Brightness, Satellite Observation, Solar Radiation, Spaceborne Astronomy, Aerosols, Atmospheric Models, Ozone, Stratosphere, Visible Spectrum

Scientific paper

It has been found that solar images observed in the visible range from satellites experience changes in shape and brightness as the line of sight sinks; the lower part of the image is found to have a lesser brightness. This phenomenon is assessed quantitatively on the basis of various aerosol and atmospheric models. It is noted that the results obtained can be used to interpret satellite photographs of the sun as well as to analyze data from occultation-sounding experiments designed to investigate the vertical structure of the atmosphere.

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