Investigation of the daytime ionosphere of Venus on the basis of two-frequency radio-occultation data from Venera 9 and 10

Details Investigation of the daytime ionosphere of Venus on the basis of two-frequency radio-occultation data from Venera 9 and 10 Investigation of the daytime ionosphere of Venus on the basis of two-frequency radio-occultation data from Venera 9 and 10

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978rael...23q1840a&link_type=abstract

Radiotekhnika i Elektronika, vol. 23, Sept. 1978, p. 1840-1847. In Russian.

Physics

Daytime, Ionospheric Electron Density, Planetary Ionospheres, Radio Occultation, Venera Satellites, Venus Atmosphere, Angular Distribution, Solar Position, Vertical Distribution, Zenith

Scientific paper

Results are presented on the two-frequency radio occultation of the Venus daytime ionosphere carried out by means of Venera 9 and 10. Thirteen height profiles of electron density were obtained for solar zenith angles in the range 10-87 deg. Depending on solar zenith angle, the electron density, in the main maximum at heights of 140-150 km, varies from 500,000 to 140,000 per cu cm. A regular dependence of the upper boundary of the daytime ionosphere on solar zenith angle has been found.

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