Session Details
[P-PS01]Outer Solar System Exploration Today, and Tomorrow
Fri. Jun 4, 2021 5:15 PM - 6:30 PM JST
Fri. Jun 4, 2021 8:15 AM - 9:30 AM UTC
Fri. Jun 4, 2021 8:15 AM - 9:30 AM UTC
Ch.02_1
convener:Jun Kimura(Osaka University), M. Kunio Sayanagi(Hampton University), Fuminori Tsuchiya(Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University), Cindy Young(NASA Langley Research Center)
The giant planets provide many keys to understanding planetary processes. They play an important role in shaping our solar system, and the physical and chemical processes they harbor also provide a unique opportunity to study the phenomena relevant for studying Earth and other planets, including exoplanetary systems. In this session, we discuss a wide range of topics encompassing the giant planets and their moons, including their origins, interiors, atmospheres, compositions, surface features, and electromagnetic fields. To advocate for current and future outer planets exploration (Juno, New Horizons, JUICE, Europa Clipper, Dragonfly and beyond), we also call for discussions on future missions to explore giant planet systems, including how to develop better international cooperation. Discussion in this latter category will include progress in developing a solar sail mission concept for observing the Jupiter system and its Trojan asteroids.[PPS01-P01]Estimation of apparent areas of Earth-orbiting UV telescope required to detect water plumes on icy moons
*Ryoichi Koga1, Fuminori Tsuchiya2, Go Murakami3, Shotaro Sakai2 (1.Nagoya University, 2.Tohoku University, 3.ISAS/JAXA)
[PPS01-P02]Quantitative analysis of hot electron density variation during transient brightening in the Io plasma torus observed by Hisaki/EXCEED
*Kento Furukawa1, Fuminori Tsuchiya1, Kazuo Yoshioka2, Reina Hikida3, Tomoki Kimura1, Masato Kagitani1, Go Murakami3, Atsushi Yamazaki3, Hajime Kita4, Ichiro Yoshikawa2 (1.Tohoku University, 2.the University of Tokyo, 3.JAXA, 4.Tohoku Institute of Technology)
[PPS01-P03]Expected source regions of Jupiter’s hectometric radio components viewed from their polarization characteristics
*Hiroaki Misawa1, Fuminori Tsuchiya1, Atsushi Kumamoto2, Yoshiya Kasahara3, Yoshizumi Miyoshi4, Masahiro Kitahara4, Satoko Nakamura4 (1.PPARC, Graduate School of Science, Tohoku University, 2.Department of Geophysics, Graduate School of Science, Tohoku University, 3.ARC-SAT, Kanazawa University, 4.ISEE, Nagoya University)
[PPS01-P04]New magnetic field and current sheet models of the night-side Jovian magnetosphere and their long-term variations
*Naoya Momoki1, Hiroaki TOH2 (1.Division of Earth and Planetary Sciences, Graduate School of Science, Kyoto University, 2.Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University)
[PPS01-P05]Exploring the roof of Jovian atmosphere by large and small groundbased telescopes in visible and infrared light
*Yasumasa Kasaba1, Takeshi Sakanoi1, Masato Kagitani1, Hajime Kita2 (1.Planetary Plasma and Atmospheric Research Center, Tohoku University, 2.Tohoku Institute of Technology)
[PPS01-P06]Jupiter Icy Moons Explorer JUICE: Science perspectives from planetary formation and geochemistry of the JUICE Japan team
*Yasuhito Sekine1, Yoshifumi Saito2, Kazushi Asamura2, Keigo Enya2, YASUKO KASAI4, Yasumasa Kasaba3, Junichi Haruyama2, Ayako Matsuoka5 (1.Earth-Life Science Insitute, Tokyo Institute of Technology, 2.ISAS, JAXA, 3.Tohoku University, 4.NICT, 5.Kyoto University)
[PPS01-P07]Numerical simulation of the passive subsurface radar for Jupiter's icy moons
*Tomoki Kimura1, Rikuto Yasuda1, Fuminori Tsuchiya1, Atsushi Kumamoto1, Hiroaki Misawa1, Yasumasa Kasaba1 (1.Tohoku U.)
[PPS01-P08]Numerical radar simulation for the explorations of the ionosphere and plume at Jupiter's icy moons
*Rikuto Yasuda1, Tomoki Kimura1, Hiroaki Misawa1, Fuminori Tsuchiya1, Atsushi Kumamoto1, Yasumasa Kasaba1 (1.TOHOKU UNIVERSITY)
<img src="https://confit-sfs.atlas.jp/customer/jpgu2021/web/OSPA.png"><br/>
[PPS01-P09]Performance, Operation and their Feasibilities for Jupiter and Icy Moons: High Frequency Receiver of Radio & Plasma Wave Investigation (RPWI) aboard JUICE during the Flight Model Test campaign
*Yasumasa Kasaba1, Hiroaki Misawa1, Fuminori Tsuchiya1, Tomoki Kimura1, Hajime Kita2, Atsushi Kumamoto1, Yuto Katoh1, Yoshizumi Miyoshi3, Yoshiya Kasahara4, Satoshi Yagitani4, Hirotsugu Kojima5, Baptiste Cecconi6 (1.Tohoku University, 2.Tohoku Institute of Technology, 3.Nagoya University, 4.Kanazawa University, 5.Kyoto University, 6.Obs. de Paris)