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[P-PS08]Science of Venus in the post-VEx/Akatsuki era

2026年5月29日(金) 17:15 〜 19:00
ポスター会場 幕張メッセ国際展示場 7・8ホール_3
コンビーナ:佐藤 毅彦(宇宙航空研究開発機構・宇宙科学研究本部)、McGouldrick Kevin(University of Colorado Boulder)、Kleinboehl Armin(NASA Jet Propulsion Laboratory)、Tellmann Silvia(University of Cologne)、原田 裕己(名古屋大学宇宙地球環境研究所)、Lee Yeon Joo(Institute for Basic Science)
On 18 September 2025, the Akatsuki team transmitted the "termination of telecommunication" command to the spacecraft, thereby officially ending the operation of Akatsuki which has been and still is in the Venus' orbit since December 2015. ESA's Venus Express (in orbit from April 2006 till December 2014) and Akatsuki together had greatly advanced our knowledge about the Venusian atmosphere, with the focus of VEx being primarily chemistry and Akatsuki's focus being almost exclusively dynamics. The planetary science community in the world gained a strong momentum to further investigate Earth's twin sister: Two of the upcoming three Venus missions, NASA's VERITAS and ESA's EnVision, are more focused on the geology, interior and evolution of the solid body with the synthetic aperture radar and other tools. Another NASA mission DAVINCI will sense both the atmosphere and the surface by a descent probe. Other recent developments include the approval of the Venus Orbiter Mission (VOM) by the Indian government; the upgrade of Chinese VOICE mission to a Venus sample return mission, and announcement of the first private sector Venus mission, Venus Life Finder.<br/>This momentum is driven by the analytical studies based on all previous Venus missions, numerical simulations (recently with data assimilation), ground-based observations, as well as laboratory experiments. This session will therefore cover all aspects of Venus science, derived observationally or theoretically, from its interior over the surface and atmosphere to the surrounding plasma environment and including possible implications for exoplanets. Contributions at all levels, from early-career researchers to experts, are all welcome.

[PPS08-P02]Ground-based spectral observation of Venus UV absorption by Pirka Telescope

*濱本 昂1、高橋 幸弘1、高木 聖子1、田口 真2、今井 正尭3 (1.北海道大学大学院理学院、2.立教大学、3.東京大学)

[PPS08-P03]Ground-based observations using IRTF/iSHEL for monitoring trace gases near the cloud tops of Venus

*佐藤 隆雄1、佐川 英夫2、青木 翔平3 (1.北海道情報大学、2.京都産業大学、3.東京大学)

[PPS08-P04]超高分散近赤外線分光装置GARNETを用いた金星下層大気微量成分観測の実現性評価

*高森 碧1、佐川 英夫1,2、猿楽 祐樹2、大坪 翔悟2、竹内 智美2 (1.京都産業大学、2.京都産業大学 神山宇宙科学研究所)

[PPS08-P05]Concept study for Korea’s future Venus exploration to understand the three-dimensional structures of the variable atmosphere

*Yeon Joo Lee1、Zizung Yoon2,1、Hyeonjun Kim 3、Sujin Choi 4、Jinsung Lee 5、Gwanghyeok Ju 6、Youngho Eun 6、Jaewook Jaewook 3、Jaehueng Park 7、Hyochoong Bang 5、Jae-Hung Han 5、Taeho Kim 8、Young-Joo Song 9、Hyeonju Kang1,6、Taekhyun Kim2,1、Dongho You1,5、Changmin Lee2,1、Chanhee Jong2,1、Nicolas Streel1、Jaeboem Kim 10、Hyeonwoo Kang 10、Kyungin Kang 10 (1.Planetary Atmospheres Group (PAG), Institute for Basic Science (IBS), Daejeon, S. Korea、2.Korea Aerospace University, Goyang, S. Korea 、3.Korea Aerospace Research Institute (KARI), Daejeon, S. Korea、4.Korea University of Technology and Education, Cheonan, S. Korea、5.Korea Advanced Institute of Science and Technology (KAIST), Daejeon, S. Korea、6.Yonsei Univ., Seoul, S. Korea、7.Korea Astronomy and Space Science Institute (KASI), Daejeon, S. Korea、8.Electronics and Telecommunications Research Institute (ETRI), Daejeon, S. Korea、9.Kyung Hee Univ., S. Korea、10.Korea AeroSpace Administration (KASA), Sacheon, S. Korea)

[PPS08-P07]Radiative Transfer Analysis of Gigantic Discontinuity in Venus Cloud Layer and Its Lifecycle

*佐藤 毅彦1、佐藤 隆雄2、今村 剛3、黒田 剛史4 (1.宇宙航空研究開発機構・宇宙科学研究所、2.北海道情報大学、3.東京大学、4.東北大学)

[PPS08-P08]Poleward Heat Transport by a 5-Day Rossby Wave at the Venus Cloud Top

*今井 正尭1,2、神山 徹3、堀之内 武4、田口 真5 (1.東京大学、2.現所属: 工学院大学、3.産業技術総合研究所、4.北海道大学、5.立教大学)

[PPS08-P09]Variability of Venusian Polar Tropopause Studied by Radio Occultation and Venus SCALE-GM

*杉浦 美優1、樫村 博基2、今村 剛1、安藤 紘基3、Bernd Häusler4、Martin Pätzold5、Silvia Tellmann5 (1. 東京大学大学院 新領域創成科学研究科 複雑理工学専攻、2.神戸大学 大学院理学研究科 惑星学専攻、3.京都産業大学 理学部 宇宙物理・気象学科、4.Institut für Raumfahrttechnik, Universität der Bundeswehr München, Neubiberg, Germany、5.Rheinisches Institut für Umweltforschung, Planetenforschung, Cologne, Germany)

[PPS08-P10]Three-Dimensional Empirical Orthogonal Function (3D-EOF) Analysis of Venusian Atmosphere Dynamics

*Tong Ding1、Takeshi Imamura1、Norihiko Sugimoto2 (1.Graduate School of Frontier Sciences, The University of Tokyo、2.Department of Physics, Keio University)

[PPS08-P11]Long Term Variability of Super-Rotation Reproduced by Akatsuki Horizontal Wind Assimilation★Invited Papers

*藤澤 由貴子1、杉本 憲彦1、小守 信正1、村上 真也2、安藤 紘基3、高木 征弘3、今村 剛4、堀之内 武5、はしもと じょーじ6、石渡 正樹5、榎本 剛7、三好 建正8、樫村 博基6、林 祥介6 (1.慶應義塾大学、2.宇宙航空研究開発機構、3.京都産業大学、4.東京大学、5.北海道大学、6.神戸大学、7.京都大学、8.理化学研究所計算科学研究センター)

[PPS08-P12]Sensitivity Tests of the Venusian Atmospheric Model Parameters Toward Akatsuki Data Assimilation

*岩中 達郎1、杉本 憲彦2、三好 建正1、Liang Jianyu3 (1.理化学研究所 計算科学研究センター、2.慶應義塾大学 法学部 物理学教室、3.Centre for Climate Research Singapore)