*Yasuhito Narita1, Andris Vaivads2, Alessandro Retino3, Yuri Khotyaintsev2, Jan Soucek4, Philippe Escoubet5, Francesco Valentini6, Christopher H. K. Chen7, Andrew Fazakerley8, Benoit Lavraud9,10, Federica Marcucci11, Rami Vainio12, Martin Gehler5, Arno Wielders5, Jens Romstedt5 (1.Space Research Institute, Austrian Academy of Sciences, Austria, 2.Swedish Institute of Space Physics Uppsala, Sweden, 3.Laboratoire de Physique des Plasmas, France, 4.Insittute of Atmospheric Physics, Czech Academy of Sciences, Czech Republic, 5.ESA/European Space Research and Technology Centre (ESTEC), The Netherlands, 6.Calabria University, Italy, 7.Imperial College London, UK, 8.Mullard Space Science Laboratory (MSSL), UK, 9.University of Toulouse, L'Institut de Recherche en Antrophsique et Planetologie, France, 10.Centre national de la recherche scientifique (CNRS), L'Institut de Recherche en Antrophsique et Planetologie (IRAP), France, 11.Instituto Nazionale di Astrofisica (INAF), Italy, 12.University of Turku, Finland)
Session information
[EJ] Poster
P (Space and Planetary Sciences) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment
[P-EM20] [EJ] Heliosphere and Interplanetary Space
Wed. May 24, 2017 5:15 PM - 6:30 PM Poster Hall (International Exhibition Hall HALL7)
This session aims to secure comprehensive insights into physical processes of plasmas and fields in the heliosphere. Presentations of the recent studies from any approaches (integrated observation/theoretical modeling/massive numerical simulation) are welcomed. Topics are not restricted to any specific issues: phenomenological studies on solar flares/CME/solar wind, and related fundamental physics problems such as shocks/waves/turbulence/particle transport and acceleration can be the main target, including heliospheric high-energy phenomena and their impact on the Earth's environment.
*Atsushi Ito1, J. J. Ramos2 (1.National Institute for Fusion Science, 2.Plasma Science and Fusion Center, MIT)
*Ya-Hui Yang1, Min-Shiu Hsieh2, Hsiu-Shan Yu3, P. F. Chen4 (1.Institute of Space Science, National Central University, Taiwan, 2.Geophysical Institute, University of Alaska Fairbanks, USA, 3.Center for Astrophysics and Space Sciences, University of California San Diego, USA, 4.School of Astronomy and Space Science, Nanjing University, China)
*Nobuhiko Nishimura1, Munetoshi Tokumaru1, Ken'ichi Fujiki1, Keishi Hayashi2,1, Kazuyuki Hakamada3 (1.Institute for Space Earth Environmental Research, Nagoya University, 2.National Space Science Center, Chinese Academy of Sciences, 3.Chubu University)
Saho Matsumoto1, *Hiroaki Misawa1, Fuminori Tsuchiya1, Satoshi Masuda2, Takahiro Obara1 (1.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 2. Institute for Space-Earth Environmental Research, Nagoya University)
Hisato Takatera1, *Tomoko Nakagawa1, Hideo Tsunakawa2 (1.Information and Communication Engineering, Tohoku Institute of Technology, 2.Department of Earth and Planetary Sciences, Tokyo Institute of Technology)
*Atsushi Yamazaki1, Go Murakami1, Kazuo Yoshioka2, Tomoki Kimura3, Fuminori Tsuchiya4, Masato Kagitani4, Takeshi Sakanoi4, Naoki Terada5, Yasumasa Kasaba5, Ichiro Yoshikawa6, Hisaki (SPRINT-A) Project team (1.Institute of Space and Astronautical Science / Japan Aerospace Exploration Agency, 2.Department of Earth & Planetary Science, Graduate School of Science, The University of Tokyo, 3.Nishina-Center for Accelerator Based Science, RIKEN, 4.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 5.Graduate School of Science, Tohoku University, 6.The University of Tokyo)