The Venus ionosphere according to spacecraft radio occultation data

Details The Venus ionosphere according to spacecraft radio occultation data The Venus ionosphere according to spacecraft radio occultation data

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985stoc.iafcq....s&link_type=abstract

IAF, International Astronautical Congress, 36th, Stockholm, Sweden, Oct. 7-12, 1985. 6 p.

Astronomy and Astrophysics

Astronomy

Ionospheric Electron Density, Planetary Ionospheres, Radio Occultation, Spaceborne Astronomy, Venus Atmosphere, Diurnal Variations, Temperature Distribution, Venera Satellites, Vertical Distribution

Scientific paper

A quantitative description of the structure of the Venusian ionosphere is given on the basis of radio occultation data obtained by the satellites Venera 15 and 16 during the period 1983-1984. Height profiles of electron density in the dayside and nightside ionospheres were derived from the radio occultation data, and the results were compared with calculated profiles. The appearance of a spike in the neutral particle temperature profile for the altitude range 112-140 km is explained within the framework of current theory. The electron density height profiles are reproduced in graphic form.

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