Thermal structure of Venusian Atmosphere determined from results of measurements from Vega-2 landing module

Details Thermal structure of Venusian Atmosphere determined from results of measurements from Vega-2 landing module Thermal structure of Venusian Atmosphere determined from results of measurements from Vega-2 landing module

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988rpsct...5...14l&link_type=abstract

In its JPRS Report: Science and Technology. USSR: Space p 14-15 (SEE N88-20312 13-12) Transl. into ENGLISH from Kosmicheskiye Is

Physics

Atmospheric Temperature, Spaceborne Experiments, Vega Project, Venus Atmosphere, Atmospheric Pressure, Hydrostatics, Temperature Measurement, Vertical Distribution

Scientific paper

A description is given of the Meteo experiment which involved the measurement of the main thermodynamic characteristics of the Venus atmosphere using four temperature sensors and three pressure sensors on the Vega 2 lander. A table listing pressure and temperature values from about 430 separate measurements is presented. Data is also presented on the vertical thermal structure of the Venus atmosphere, the matching coefficient of hydrostatic and aerodynamic descent models, and the static stability profile.

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