Venusian Cloud Distribution Simulated by a General Circulation Model
Author:
Affiliation:
1. Faculty of Science Kyoto Sangyo University Kyoto Japan
2. Research and Education Center for Natural Sciences, Department of Physics Keio University Kanagawa Japan
3. Department of Astronomy and Earth Science Tokyo Gakugei University Tokyo Japan
Funder
Japan Society for the Promotion of Science London
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JE006208
Reference80 articles.
1. Vertical structure of the axi-asymmetric temperature disturbance in the Venusian polar atmosphere: Comparison between radio occultation measurements and GCM results
2. Thermal structure of the Venusian atmosphere from the sub-cloud region to the mesosphere as observed by radio occultation
3. Vertical Wavenumber Spectra of Gravity Waves in the Venus Atmosphere Obtained from Venus Express Radio Occultation Data: Evidence for Saturation
4. The puzzling Venusian polar atmospheric structure reproduced by a general circulation model
5. Local Time Dependence of the Thermal Structure in the Venusian Equatorial Upper Atmosphere: Comparison of Akatsuki Radio Occultation Measurements and GCM Results
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