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SO2 in the middle atmosphere of Venus: IR measurements from Venera 15 and comparison to UVTwo sets of measurements of SO2 bands in the Venus spectra are presented and compared: IR spectra obtained on the USSR Venera 15 orbiter and UV spectra from the American Pioneer Venus orbiter and sounding rockets. The 40-mbar level was chosen as a reference level for comparison. The UV data are referred to this level. There are three SO2 bands in the infrared spectrum: at 519, 1150, and 1360 cm(exp -1). The levels of their formation in the atmosphere may differ significantly, by more than 10 km.
Document ID
19930005209
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Zasova, L. V. (Academy of Sciences (USSR) Moscow, Ussr)
Moroz, V. I. (Academy of Sciences (USSR) Moscow, Ussr)
Esposito, L. W. (Colorado Univ. Boulder., United States)
Na, C. Y. (Colorado Univ. Boulder., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: Lunar and Planetary Inst., Papers Presented to the International Colloquium on Venus
Subject Category
Lunar And Planetary Exploration
Accession Number
93N14397
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19930005100Collected WorksPapers presented to the International Colloquium on Venus19930005100Collected WorksPapers presented to the International Colloquium on Venus
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