Development of a model for the formation of the nighttime ionosphere of Venus for a period of low solar activity

Details Development of a model for the formation of the nighttime ionosphere of Venus for a period of low solar activity Development of a model for the formation of the nighttime ionosphere of Venus for a period of low solar activity

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kosis..28..282s&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 28, Mar.-Apr. 1990, p. 282-292. In Russian.

Physics

Ionospheric Electron Density, Planetary Ionospheres, Two Dimensional Models, Venus Atmosphere, Radio Occultation, Solar Activity, Venera Satellites

Scientific paper

A two-dimensional model for the formation of the nighttime ionosphere of Venus is verified for the case of low solar activity using radio-occultation data from Venera 9 and 10 as well as from Venera 15 and 16. The model takes into account two probable sources of ionosphere formation: ionization by superthermal electrons and horizontal transport of ions from the daytime sector.

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