Influence of Venus topography on the zonal wind and UV albedo at cloud top level: The role of stationary gravity waves
Author:
Affiliation:
1. LATMOS/INSU/CNRS, UVSQ; Guyancourt France
2. Space Research Institute; RAS; Moscow Russia
3. Max Planck Institute for Solar System Research; Göttingen Germany
4. Laboratoire de Météorologie Dynamique; UMR 8539, IPSL, UPMC, CNRS; Paris France
Funder
CNES
CNRS
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1002/2015JE004958/fullpdf
Reference41 articles.
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2. Vega-1 and Vega-2 entry probes: An investigation of local UV absorption (220-400 nm) in the atmosphere of Venus (SO2, aerosols, cloud structure);Bertaux;J. Geophys. Res.,1996
3. The 1.10- and 1.18-µm nightside windows of Venus observed by SPICAV-IR aboard Venus Express;Bézard;Icarus,2011
4. Implications of the VEGA balloon results for Venus atmospheric dynamics;Blamont;Science,1986
5. Observations photographiques de la planète Vénus;Boyer;Ann. Astrophys.,1961
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