Computer Science
Scientific paper
Sep 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kosis..28..765s&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 28, Sept.-Oct. 1990, p. 765-775. In Russian.
Computer Science
Ionospheric Electron Density, Planetary Ionospheres, Radio Occultation, Satellite Observation, Venus Atmosphere, Atmospheric Models, Solar Activity, Thermosphere, Ultraviolet Radiation, Venera Satellites
Scientific paper
The behavior of vertical distributions of electron density in the Venus ionosphere as observed in radio-occultation experiments carried out with Venera satellites is interpreted using a planetary thermosphere model based on Pioneer-Venus data. Model and experimental distributions are compared for different zenith angles and solar activity indices, and it is shown that the observed variations of vertical profiles in the photoequilibrium region of the dayside Venusian ionosphere can be explained by variations of UV radiation and thermospheric parameters in the course of a solar cycle.
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