9:00 AM - 9:15 AM
*Tada-nori GOTO1 (1.Graduate School of Engineering, Kyoto University)
Oral
Symbol M (Multidisciplinary and Interdisciplinary) » M-IS Intersection
Thu. May 1, 2014 9:00 AM - 10:45 AM 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:Ikuko Fujii(Kakioka Magnetic Observatory, Japan Meteorological Agency), Shigeru Fujita(Meteorological College, Japan Meteorological Agency)
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.
9:00 AM - 9:15 AM
*Tada-nori GOTO1 (1.Graduate School of Engineering, Kyoto University)
9:15 AM - 9:30 AM
*Arata ENDO1, Shigeru FUJITA2, Ikuko FUJII3 (1.Japan Meteorological Agency, 2.Meteorological College, 3.Magnetic Observatory)
9:30 AM - 9:45 AM
*Naoto IMAMURA1, Adam SCHULTZ2, Tada-nori GOTO1, Junichi TAKEKAWA1, Hitoshi MIKADA1 (1.Graduate School of Engineering, Kyoto University, 2.Oregon State University)
9:45 AM - 10:00 AM
*Ikuko FUJII1 (1.Kakioka Magnetic Observatory, JMA)
10:00 AM - 10:15 AM
*Yasuo OGAWA1 (1.Volcanic Fluid Research Center, Tokyo Institute of Technology)
10:15 AM - 10:30 AM
*Akimasa YOSHIKAWA1 (1.International Center for Space Science and Education, Kyushu University)
10:30 AM - 10:45 AM
*Kodai IWASHITA1, Hiroaki TOH2 (1.Graduate School of Science, Kyoto University, 2.Data Analysis Center for Geomagnetism and Space Magnetism,)