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Number of items: 4.

Ando, Hiroki, Imamura, Takeshi, Tellmann, Silvia, Patzold, Martin, Hausler, Bernd, Sugimoto, Norihiko ORCID: 0000-0002-5135-7179, Takagi, Masahiro, Sagawa, Hideo, Limaye, Sanjay, Matsuda, Yoshihisa, Choudhary, Raj Kumar and Antonita, Maria (2020). Thermal structure of the Venusian atmosphere from the sub-cloud region to the mesosphere as observed by radio occultation. Sci Rep, 10 (1). LONDON: NATURE PUBLISHING GROUP. ISSN 2045-2322

Ando, Hiroki, Takagi, Masahiro ORCID: 0000-0002-4629-6279, Fukuhara, Tetsuya, Imamura, Takeshi, Sugimoto, Norihiko ORCID: 0000-0002-5135-7179, Sagawa, Hideo, Noguchi, Katsuyuki, Tellmann, Silvia, Paetzold, Martin, Haeusler, Bernd, Murata, Yasuhiro, Takeuchi, Hiroshi ORCID: 0000-0001-5863-4653, Yamazaki, Atsushi, Toda, Tomoaki, Tomiki, Atsushi, Choudhary, Rajkumar, Kumar, Kishore, Ramkumar, Geetha and Antonita, Maria (2018). Local Time Dependence of the Thermal Structure in the Venusian Equatorial Upper Atmosphere: Comparison of Akatsuki Radio Occultation Measurements and GCM Results. J. Geophys. Res.-Planets, 123 (9). S. 2270 - 2281. WASHINGTON: AMER GEOPHYSICAL UNION. ISSN 2169-9100

Ando, Hiroki ORCID: 0000-0001-5088-6186, Takaya, Koutarou, Takagi, Masahiro ORCID: 0000-0002-4629-6279, Sugimoto, Norihiko ORCID: 0000-0002-5135-7179, Imamura, Takeshi, Sagawa, Hideo, Tellmann, Silvia, Paetzold, Martin, Matsuda, Yoshihisa, Haeusler, Bernd, Limaye, Sanjay, Choudhary, Raj Kumar and Antonita, Maria (2022). Dynamical Effect on Static Stability of the Venus Atmosphere Simulated Using a General Circulation Model: A Comparison With Radio Occultation Measurements. J. Geophys. Res.-Planets, 127 (3). WASHINGTON: AMER GEOPHYSICAL UNION. ISSN 2169-9100

Takami, Kosuke, Nakagawa, Hiromu, Sagawa, Hideo, Krause, Pia, Murata, Isao, Kasaba, Yasumasa ORCID: 0000-0002-8160-3553, Kuroda, Takeshi ORCID: 0000-0003-4789-4737, Aoki, Shohei ORCID: 0000-0001-6727-125X, Kouyama, Toru, Kostiuk, Theodor, Livengood, Timothy A. and Gilli, Gabriella ORCID: 0000-0002-2253-5802 (2020). Evaluation of a method to retrieve temperature and wind velocity profiles of the Venusian nightside mesosphere from mid-infrared CO2 absorption line observed by heterodyne spectroscopy. Earth Planets Space, 72 (1). NEW YORK: SPRINGER. ISSN 1880-5981

This list was generated on Fri Apr 19 23:42:05 2024 CEST.