11:00 AM - 11:15 AM
*Kunihiro KEIKA1, Yusuke EBIHARA2, Ryuho KATAOKA3 (1.Solar-Terrestrial Environment Laboratory, Nagoya University, 2.Research Institute for Sustainable Humanosphere, Kyoto University, 3.National Institute of Polar Research)
Oral
Symbol M (Multidisciplinary and Interdisciplinary) » M-IS Intersection
Thu. May 1, 2014 11:00 AM - 12:45 PM 313 (3F)
Convener:*Shigeru Fujita(Meteorological College, Japan Meteorological Agency), Ryuho Kataoka(National Institute of Polar Research), Ikuko Fujii(Kakioka Magnetic Observatory, Japan Meteorological Agency), Shinichi Watari(National Institute of Information and Communications Technology), Chair:Shinichi Watari(National Institute of Information and Communications Technology), Ryuho Kataoka(National Institute of Polar Research)
The extremely large geomagnetically induced current (GIC) which possibly causes serious disasters to our society has not been supposed to occur in low-latitude countries like Japan. This groundless assumption has prevented active researches about the GICs in Japan. It is noted that the disaster possibly caused by the extremely large GIC will be catastrophic to our society. Therefore, we had the first scientific session about this issue in the last JpGU assembly. It was the epoch-making event that the space scientists including solar physicists and the solid-Earth geophysicists discussed the common issue together. As outputs of this session, we recognized the following problems to be settled for the GIC research in Japan, 1) estimations of intensity of the extremely large space weather event and the occurrence frequency, 2) propagation of extremely large solar wind disturbances from Sun to Earth and its impact to the geospace, 3) modeling of the GIC with a realistic ground conductivity distribution. Research papers about these problems will be published in the special issue of Earth, Planets and Space.In the session this year, we will discuss the recent progresses about the GIC research stimulated by the last GIC session as well as the new topics including the magnetotelluric sounding based on a source field with finite spatial structure in the magnetosphere/ionosphere, recent modeling researches, and the new observation plans. We welcome related scientific and technical researches.
11:00 AM - 11:15 AM
*Kunihiro KEIKA1, Yusuke EBIHARA2, Ryuho KATAOKA3 (1.Solar-Terrestrial Environment Laboratory, Nagoya University, 2.Research Institute for Sustainable Humanosphere, Kyoto University, 3.National Institute of Polar Research)
11:15 AM - 11:30 AM
*Tohru ARAKI1, Atsuki SHINBORI2 (1.Polar Research Institute of China, 2.RISH, Kyoto University)
11:30 AM - 11:45 AM
*Takashi KIKUCHI1, Shinichi WATARI2, Kumiko HASHIMOTO3, Yusuke EBIHARA4 (1.Solar-Terrestrial Environment Laboratory, 2.National Institute of Information and Communications Technology, 3.Kibi International University, 4.Research Institute for Sustainable Humanosphere)
11:45 AM - 12:00 PM
*Hiroyuki MAEHARA1, Takuya SHIBAYAMA2, Yuta NOTSU2, Shota NOTSU2, Satoshi HONDA3, Daisaku NOGAMI2, Kazunari SHIBATA2 (1.University of Tokyo, 2.Kyoto University, 3.University of Hyogo)
12:00 PM - 12:15 PM
*Masao NAKAMURA1, Asato YONEDA1, Ken TSUBOUCHI2 (1.Osaka Prefecture University, 2.Tokyo Institute of Technology)
12:15 PM - 12:30 PM
*Yasuhiro MINAMOTO1, Shigeru FUJITA2, Junpei OOGI1, Masahiro HARA1 (1.Kakioka Magnetic Observatory, Japan Meteorological Agency, 2.Meteorological College, Japan Meteorological Agency)
12:30 PM - 12:45 PM
*Shinichi WATARI1 (1.National Institute of Informaton and Communications Technology)