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Thermal structure of the Venusian atmosphere from the sub-cloud region to the mesosphere as observed by radio occultation.
Ando, Hiroki; Imamura, Takeshi; Tellmann, Silvia; Pätzold, Martin; Häusler, Bernd; Sugimoto, Norihiko; Takagi, Masahiro; Sagawa, Hideo; Limaye, Sanjay; Matsuda, Yoshihisa; Choudhary, Raj Kumar; Antonita, Maria.
Affiliation
  • Ando H; Faculty of Science, Kyoto Sangyo University, Kyoto, Japan. hando@cc.kyoto-su.ac.jp.
  • Imamura T; Department of Complexity Science and Engineering, The University of Tokyo, Chiba, Japan.
  • Tellmann S; Abteilung Planetenforschung, Rheinisches Institut für Umweltforschung, Universität zu Köln, Köln, Germany.
  • Pätzold M; Abteilung Planetenforschung, Rheinisches Institut für Umweltforschung, Universität zu Köln, Köln, Germany.
  • Häusler B; Institut für Raumfahrttechnik und Weltraumnutzung, Universität der Bundeswehr München, Neubiberg, Germany.
  • Sugimoto N; Research and Education Center for Natural Sciences, Department of Physics, Keio University, Kanagawa, Japan.
  • Takagi M; Faculty of Science, Kyoto Sangyo University, Kyoto, Japan.
  • Sagawa H; Faculty of Science, Kyoto Sangyo University, Kyoto, Japan.
  • Limaye S; University of Wisconsin, Wisconsin, USA.
  • Matsuda Y; Department of Astronomy and Earth Sciences, Tokyo Gakugei University, Tokyo, Japan.
  • Choudhary RK; Vikram Sarabhai Space Center, Space Physics Laboratory, Thiruvananthapuram, India.
  • Antonita M; Indian Space Research Organization, Bengaluru, India.
Sci Rep ; 10(1): 3448, 2020 Feb 26.
Article in En | MEDLINE | ID: mdl-32103048
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Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Sci Rep Year: 2020 Document type: Article Affiliation country: Japan Country of publication: United kingdom
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Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Sci Rep Year: 2020 Document type: Article Affiliation country: Japan Country of publication: United kingdom