[EE] Poster
P (Space and Planetary Sciences) » P-PS Planetary Sciences
Tue. May 23, 2017 5:15 PM - 6:30 PM Poster Hall (International Exhibition Hall HALL7)
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 (Cassini, Juno, New Horizons, JUICE, 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.
*Hiroaki TOH1 (1.Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University)
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*Kunio M. Sayanagi1, Robert A. Dillman2, David H. Atkinson4, Sarag Saikia7, Amy A. Simon3, Thomas R. Spilker6, Michael H. Wong5, Drew J. Hope2 (1.Hampton University, 2.NASA Langley Research Center, 3.NASA Goddard Space Flight Center, 4.NASA Jet Propulsion Laboratory, 5.University of California, Bekerkeley, 6.Independent Consultant, 7.Purdue University)
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*Koichiro Terada1, Chihiro Tao2, Naoki Terada1, Yasumasa Kasaba1, Hajime Kita1, Aoi Nakamizo2, Akimasa Yoshikawa3, Shinichi Ohtani4, Fuminori Tsuchiya1, Masato Kagitani1, Takeshi Sakanoi1, Go Murakami5, Kazuo Yoshioka6, Tomoki Kimura7, Atsushi Yamazaki5, Ichiro Yoshikawa8 (1.Graduate School of Science, Tohoku University, 2.Applied Electromagnetic Research Institute, National Institute of Information and Communications Technology, 3.Department of Earth and Planetary Sciences, Faculty of Science, Kyushu University, / International Center for Space Weather Science and Education, Kyushu University, 4.The Johns Hopkins University Applied Physics Laboratory, 5.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 6.Department of Earth & Planetary Science, Graduate School of Science, The University of Toky, 7.Nishina-Center for Accelerator Based Science, RIKEN, 8.Graduate School of Frontier Sciences, The University of Tokyo)
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*Ryoichi Koga1, Fuminori Tsuchiya1, Masato Kagitani1, Takeshi Sakanoi1, Mizuki Yoneda2, Ichiro Yoshikawa3, Kazuo Yoshioka3, Go Murakami4, Atsushi Yamazaki4, Tomoki Kimura5 (1.Planetary Plasma and Atmospheric Research Center, Tohoku University, 2.Kiepenheuer Institute of Solarphysics, 3.University of Tokyo, 4.JAXA/ISAS, 5.RIKEN)
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*Masato Kagitani1, Mizuki Yoneda2, Fuminori Tsuchiya1, Kazuo Yoshioka3, Tomoki Kimura5, Go Murakami4, Atsushi Yamazaki4, Ichiro Yoshikawa3 (1.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 2.Kiepenheuer Institute for Solar Physics, 3.The University of Tokyo, 4.ISAS/JAXA, 5.RIKEN)
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Mika Shishido1, *Takeshi Sakanoi1, Masato Kagitani1, Fuminori Tsuchiya1, Ichiro Yoshikawa2, Atsushi Yamazaki3, Kazuo Yoshioka4, Go Murakami3, Tomoki Kimura5 (1.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 2.Graduate School of Frontier Sciences, The University of Tokyo, 3.Institute of Space and Astronautical Science, JAXA, 4.Graduate School of Science, The University of Tokyo, 5.Riken)
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*Arakawa Ryo1, Hiroaki Misawa1, Fuminori Tsuchiya1, Masato Kagitani1, Ichiro Yoshikawa2, Kazuo Yoshioka2, Fumiharu Suzuki2, Tomoki Kimura3, Go Murakami4, Atsushi Yamazaki4 (1.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 2.Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo, 3.Nishina-Center for Accelerator Based Science, RIKEN, 4.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
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*Sooman Han1, Hajime Kita2, Atsushi Yamazaki3, Go Murakami3, Fuminori Tsuchiya2, Masato Nakamura3 (1.Department of Earh and Planetary Science, Graduate School of Science, The University of Tokyo, 2.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 3.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
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*Jun Kimura1, Shunichi Kamata2 (1.Osaka University, 2.Hokkaido University)
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*Ryusuke Nishitani1, Atsushi Tani2, Sho Sasaki1, Jun Kimura1 (1.Department of Earth and Space Sciences, School of Science, Osaka University, 2.Graduate School Human Development and Environment, Kobe University)
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