Computer Science
Scientific paper
Jul 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kosis..24..620g&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 24, July-Aug. 1986, p. 620-630. In Russian.
Computer Science
Atmospheric Models, Ionospheric Electron Density, Night Sky, Planetary Ionospheres, Radio Occultation, Venus Atmosphere, Magnetohydrodynamic Flow, Plasma Density, Solar Activity, Temperature Distribution, Vertical Distribution
Scientific paper
A three-component (O+, O2+, and NO+) model for the formation of the Venus nightside ionosphere with two ionization maxima is developed on the basis of radio-occultation data (Mariner-10, Pioneer-Venus, and Venera 9, 10, 15, and 16) obtained during periods of low solar activity. The source of primary ions was assumed to be the O(+) plasma flux flowing from the dayside to the nightside, and diffusing downward. Vertical temperature distributions of the neutral and ionized components in the ionopshere are determined.
Gavrik Anatoly L.
Osmolovskii I. K.
Samoznaev L. P.
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