Thermal structure in the Venus middle cloud layer

Details Thermal structure in the Venus middle cloud layer Thermal structure in the Venus middle cloud layer

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12...36l&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, Jan. 1986, p. 36-40) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, Jan.-Feb.

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Atmospheric Temperature, Balloon Sounding, Vega Project, Venus Clouds, Air Masses, Atmospheric Stratification, Temperature Measurement, Temperature Profiles

Scientific paper

Thermal structure measurements obtained by the two Vega balloons show the Venus atmosphere in the middle cloud layer to be near-adiabatic, on the whole; but discrete air masses are present that differ slightly from one another in potential temperature and entropy. The Vega 1 temperatures are 6.5 K warmer than measured by Vega 2 at given pressures. Measurements taken by the Vega 2 lander on descent through these levels agree with the Vega 2 balloon data.

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