Reconstruction of the H2O profile from the results of modeling the heat flux in the lower atmosphere of Venus

Details Reconstruction of the H2O profile from the results of modeling the heat flux in the lower atmosphere of Venus Reconstruction of the H2O profile from the results of modeling the heat flux in the lower atmosphere of Venus

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8330343m&link_type=abstract

"Reconstruction of the H2O profile from the results of modeling the heat flux in the lower atmosphere of Venus Transl. into ENG

Computer Science

Atmospheric Composition, Venus Atmosphere, Vertical Distribution, Water Vapor, Carbon Dioxide, Optical Measurement, Spectrophotometers

Scientific paper

The H2O profile in the Venus lower atmosphere is reconstructed by the effective radiation flux data. It is shown that the H2O vapor abundance is concentrated mainly in the 20 to 48 km layer and depends on measurement time and location. The magnitudes of H2O optically determined are much less than those obtained by probing, especially below 20 km.

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