Physics
Scientific paper
Sep 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978rael...23r1840a&link_type=abstract
(Radiotekhnika i Elektronika, vol. 23, Sept. 1978, p. 1840-1847.) Radio Engineering and Electronic Physics, vol. 23, Sept. 1978,
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.
Aleksandrov Iu. N.
Dubrovin V. M.
Kolosov M. A.
Petrov G. M.
Samovol V. A.
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