The vertical gradient of the atmospheric temperature of Venus studied on the basis of radio occultation data

Details The vertical gradient of the atmospheric temperature of Venus studied on the basis of radio occultation data The vertical gradient of the atmospheric temperature of Venus studied on the basis of radio occultation data

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980kosis..18..783m&link_type=abstract

Kosmicheskie Issledovaniia, vol. 18, Sept.-Oct. 1980, p. 783-786. In Russian.

Computer Science

Atmospheric Temperature, Radio Occultation, Temperature Gradients, Venera Satellites, Venus Atmosphere, Daytime, Height, Night, Venera 10 Satellite, Venera 9 Satellite, Vertical Distribution

Scientific paper

The vertical gradient of the temperature of the Venus atmosphere on the
night and day sides of the planet was obtained from Venera-9 and
Venera-10 radio occultation data. Results on the height dependence of
the vertical temperature gradient for 40-75 km are compared with data on
fluctuations of radio waves and winds in the planetary atmosphere.

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