The lower atmosphere of Venus after VEGA 1 and 2 missions

Details The lower atmosphere of Venus after VEGA 1 and 2 missions The lower atmosphere of Venus after VEGA 1 and 2 missions

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988em%26p...43...45p&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 43, Oct. 1988, p. 45-60.

Physics

1

Atmospheric Composition, Atmospheric Density, Atmospheric Pressure, Lower Atmosphere, Venus Atmosphere, Atmospheric Physics, Atmospheric Temperature, Temperature Distribution, Temperature Inversions, Vega Project

Scientific paper

The authors have computed the physical parameters for the Venus
atmosphere between 0 - 64 km altitude by using Vega measurements. The
proposed model can be used in order to study the structure of Venus
atmosphere and its chemical composition between 60 - 64 km, where an
inversion in temperature profiles has been measured by Vega.

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