High-resolution spectroscopy of Venus: Detection of OCS, upper limit to H2S, and latitudinal variations of CO and HF in the upper cloud layer-Reference-Cited by-同舟云学术

High-resolution spectroscopy of Venus: Detection of OCS, upper limit to H2S, and latitudinal variations of CO and HF in the upper cloud layer

Published:2008-10 Issue:2 Volume:197 Page:377-385
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Krasnopolsky Vladimir A.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference46 articles.

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3. The deep atmosphere of Venus revealed by high-resolution nightside spectra;Bezard;Nature,1990

4. Airborne observations of the gas composition of Venus above the cloud tops: Measurements of H2O, HF, and the D/H and 18O/16O isotopic ratios;Bjoraker;Bull. Am. Astron. Soc.,1992

5. Traces of HCl and HF in the atmosphere of Venus;Connes;Astrophys. J.,1967

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