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      Three-Dimensional Structures of Thermal Tides Simulated by a Venus GCM : 3-D STRUCTURES OF VENUSIAN THERMAL TIDES

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          Models of the structure of the atmosphere of Venus from the surface to 100 kilometers altitude

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            Meridional Circulation and the Maintenance of the Venus Atmospheric Rotation

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              Structure and meteorology of the middle atmosphere of Venus: Infrared remote sensing from the Pioneer Orbiter

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                Author and article information

                Journal
                Journal of Geophysical Research: Planets
                J. Geophys. Res. Planets
                Wiley
                21699097
                February 2018
                February 2018
                February 05 2018
                : 123
                : 2
                : 335-352
                Affiliations
                [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
                Article
                10.1002/2017JE005449
                ea5dcca0-1235-46f1-bf97-e04d4231d839
                © 2018

                http://doi.wiley.com/10.1002/tdm_license_1.1

                http://onlinelibrary.wiley.com/termsAndConditions#vor

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