Nighttime Venusian atmosphere from dual-frequency radio occultation measurement results with the Venera 9 and Venera 10 satellites

Physics

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Ionospheric Electron Density, Night Sky, Radio Occultation, Venus Atmosphere, Midlatitude Atmosphere, Planetary Ionospheres, Venera Satellites, Vertical Distribution

Scientific paper

Electron concentration profiles of the nighttime ionosphere of Venus, characterizing the state of the ionosphere in equatorial and mid-latitude regions of the planet, were obtained from dual-frequency radio occultation data. In one group of measurements, the profiles had two pronounced peaks. The higher-altitude peak was located at about 134-114 km, with electron concentration in the range 3,000-8,800 per cu cm. The lower peak was shifted 17-14 km with respect to the higher one and had a concentration attaining 2,000 electrons per cu cm. A second group featured only one peak. The data reveal high variability of nighttime parameters of the Venusian ionosphere.

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