Characteristics of the dayside ionosphere of Venus in years of low and high solar activity

Details Characteristics of the dayside ionosphere of Venus in years of low and high solar activity Characteristics of the dayside ionosphere of Venus in years of low and high solar activity

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kosis..25..285g&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 25, Mar.-Apr. 1987, p. 285-291. In Russian.

Astronomy and Astrophysics

Astronomy

1

Daytime, Planetary Ionospheres, Solar Activity Effects, Solar Planetary Interactions, Spaceborne Astronomy, Venus Atmosphere, Pioneer Venus Spacecraft, Solar Cycles, Venera Satellites

Scientific paper

Venera 15 and 16 two-frequency radio-occultation measurements carried out in 1983-1984 were used to determine the characteristics of the dayside atmosphere of Venus for intermediate states of solar activity. A comparison of these data with Venera 9 and 10 and Pioneer-Venus data revealed a series of ionospheric characteristics connected with the phase of the solar cycle.

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