Three-Dimensional Structures of Thermal Tides Simulated by a Venus GCM-Reference-Cited by-同舟云学术

Three-Dimensional Structures of Thermal Tides Simulated by a Venus GCM

Published:2018-02 Issue:2 Volume:123 Page:335-352
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Takagi Masahiro¹^ORCID,Sugimoto Norihiko²^ORCID,Ando Hiroki¹,Matsuda Yoshihisa³

Affiliation:

1. Department of Astrophysics and Atmospheric Science, Faculty of Science; Kyoto Sangyo University; Kyoto Japan

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

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

Funder

JSPS KAKENHI

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/10.1002/2017JE005449/fullpdf

Reference71 articles.

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2. The puzzling Venusian polar atmospheric structure reproduced by a general circulation model;Ando;Nature Communications,2016

3. Venus mesosphere and thermosphere: III. Three-dimensional general circulation with coupled dynamics and composition;Bougher;Icarus,1988

4. Dynamics of the Venus upper atmosphere: Outstanding problems and new constraints expected from Venus Express;Bougher;Planetary and Space Science,2006

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