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

Physics

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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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