Nightside ionosphere of Venus

Details Nightside ionosphere of Venus Nightside ionosphere of Venus

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979p%26ss...27.1403k&link_type=abstract

Planetary and Space Science, vol. 27, Dec. 1979, p. 1403-1408.

Computer Science

2

Ionospheric Composition, Nightglow, Planetary Ionospheres, Venus Atmosphere, Helium Ions, Ionospheric Electron Density, Sulfur, U.S.S.R. Space Program, Venera Satellites, Venus, Nightside, Ionosphere, Venera 9, Venera 10, Airglow, Layers, Formation, Radiation, Meteorites, Ionization, Electron Flux, Ions, Energy, Helium, Flux, Nitric Oxide, Mixing, Sulfur, Altitudes, Observations, Density, Analysis, Photoionization, Models, Review, Comparisons

Scientific paper

Veneral 9, 10 measurements of the nightside ionospheric profile and the night airglow were used for investigating ionosphere formation processes. The upper ionospheric layer may be formed by He I 584 A radiation; the lower layer by meteorite ionization. Upper limits on the electron energy flux, 4 x 10 to the 8 eV/sq cm s, the helium ion flux 10 to the 7th/sq cm s, the nitric oxide mixing ratio, 1.5 x 10 to the -4, and the atomic sulfur mixing ratio, 10 to the -6, are deduced for ionospheric altitudes.

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