Japan Geoscience Union Meeting 2019

Presentation information

[J] Poster

A (Atmospheric and Hydrospheric Sciences ) » A-OS Ocean Sciences & Ocean Environment

[A-OS19] Dynamics of oceanic and atmospheric waves, vortices, and circulations

Mon. May 27, 2019 5:15 PM - 6:30 PM Poster Hall (International Exhibition Hall8, Makuhari Messe)

convener:Yuki Tanaka(Graduate School of Science, The University of Tokyo), Ryo Furue(APL/JAMSTEC), Yukiharu Hisaki(University of the Ryukyus), Norihiko Sugimoto(Keio University, Department of Physics)

[AOS19-P02] Data assimilation of the Venus atmosphere assuming radio occultation measurement by small satellites

*Mirai Abe1, Norihiko Sugimoto1, Yukako Kikuchi2, Asako Hosono3, Hiroki Ando4, Masahiro Takagi4, Itziar Garate Lopez5, Sebastien Lebonnois6, Chi Ao7 (1.Keio University, 2.Yokohama Futaba High School, 3.Toshimagaoka Women High School, 4.Kyoto Sangyo University, 5.Euskal Herriko Unibertsitatea, 6.Sorbonne Universite, 7.Jet Propulsion Laboratory)

Keywords:Data assimilation, Venus, Radio occultation

At the altitude of approximately 60-70 km in the Venus atmosphere, there is an interesting phenomenon called “cold collar” where the temperature of the polar region is higher than that of the surroundings (latitude of about 60-80 degrees). The Japanese Venus Atmospheric GCM For the Earth Simulator (AFES-Venus) succeeded for the first time in the reproduction of cold collar1. However, the temperature difference between the pole and the surroundings is small compared with that observed. Recently, using the Local Ensemble Transform Kalman Filter (LETKF), we have succeeded in developing the Venus AFES LETKF Data Assimilation System (VALEDAS)2. In this study, we investigated the reproducibility of cold collar by the data assimilation of French Venus Atmospheric GCM(LMD/VGCM) in which cold collar is realistically reproduced3. We prepared idealized observation data assuming radio occultation measurement by small satellites. We will report the reproducibility of cold collar by changing the conditions such as observation point, observation number, and time interval. Figure shows three vertical profiles of temperature observations at 85 degrees North every Earth hour (obtained by temperature field from 30-90 degrees North at the altitude of about 66 km). Therefore, such kind of future mission would be promising.

[1] The puzzling Venusian polar atmospheric structure reproduced by a general circulation model,
Hiroki Ando, Norihiko Sugimoto, Masahiro Takagi, Hiroki Kashimura, Takeshi Imamura, and Yoshihisa Matsuda, Nature Communications, Vol. 7, (2016), 10398, 8pp.
[2] Development of an ensemble Kalman filter data assimilation system for the Venusian atmosphere,
Norihiko Sugimoto, Akira Yamazaki, Toru Kouyama, Hiroki Kashimura, Takeshi Enomoto, and Masahiro Takagi, Scientific Reports, Vol. 7, (2017), 9321, 9pp
[3] Latitudinal variation of clouds’ structure responsible for Venus’ cold collar,
Itziar Garate-Lopez, Sébastien Lebonnois, Icarus, Vol. 314, (2018), p1-11.