Dynamical Effect on Static Stability of the Venus Atmosphere Simulated Using a General Circulation Model: A Comparison With Radio Occultation Measurements-Reference-Cited by-同舟云学术

Dynamical Effect on Static Stability of the Venus Atmosphere Simulated Using a General Circulation Model: A Comparison With Radio Occultation Measurements

Published:2022-03 Issue:3 Volume:127 Page:
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:JGR Planets

Author:

Ando Hiroki¹^ORCID,Takaya Koutarou¹,Takagi Masahiro¹^ORCID,Sugimoto Norihiko²^ORCID,Imamura Takeshi³^ORCID,Sagawa Hideo¹^ORCID,Tellmann Silvia⁴,Pätzold Martin⁴,Matsuda Yoshihisa⁵,Häusler Bernd⁶^ORCID,Limaye Sanjay⁷,Choudhary Raj Kumar⁸^ORCID,Antonita Maria⁹

Affiliation:

1. Faculty of Science Kyoto Sangyo University Kyoto Japan

2. Department of Physics Research and Education Center for Natural Sciences Keio University Yokohama Japan

3. Graduate School of Frontier Sciences The University of Tokyo Kashiwa Japan

4. Abteilung Planetenforschung Rheinisches Institut für Umweltforschung Universität zu Köln Koln Germany

5. Department of Astronomy and Earth Science Tokyo Gakugei University Koganei Japan

6. Institut für Raumfahrttechnik und Weltraumnutzung Universität der Bundeswehr München Neubiberg Germany

7. University of Wisconsin Madison WI USA

8. Space Physics Laboratory Vikram Sarabhai Space Center Trivandrum India

9. Indian Space Research Organization Bangalore India

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/10.1029/2021JE006957

Reference33 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. The puzzling Venusian polar atmospheric structure reproduced by a general circulation model

4. 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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2. Formation and Quasi‐Periodic Variation of Equatorial Jet Caused by Planetary‐Scale Waves in the Venusian Lower Cloud Layer;Journal of Geophysical Research: Planets;2023-11

3. Cold Collar Reproduced by a Venus GCM With the Akatsuki Horizontal Wind Assimilation;Journal of Geophysical Research: Planets;2023-04