4:15 PM - 4:30 PM
*Takayuki MURANUSHI1, Eiji AKIYAMA2, Shu-ichiro INUTSUKA3, Hideko NOMURA4, Satoshi OKUZUMI4 (1.Kyoto University, 2.The National Astronomical Observatory of Japan, 3.Nagoya university, 4.Tokyo Institute of Technology)
Oral
Symbol P (Space and Planetary Sciences) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment
Thu. May 1, 2014 4:15 PM - 5:30 PM 503 (5F)
Convener:*Shuichi Matsukiyo(Department of Earth System Science and Technology, Kyushu University), Shu-ichiro Inutsuka(Department of Physics, Nagoya University), Chair:Shu-ichiro Inutsuka(Department of Physics, Nagoya University)
A plasma seen in a star's/planetary atmosphere, molecular clouds, and a laboratory is often not fully ionized and contains neutral gases and dusts. Studying the complex behaviors of such media contributes not only to understand the physics of a multi-layer coupling in space but also to plasma applications. Here, diverse plasma phenomena in such circumstances are discussed. This session is a part of 'plasma astrophysics joint session of the three academic societies'.
4:15 PM - 4:30 PM
*Takayuki MURANUSHI1, Eiji AKIYAMA2, Shu-ichiro INUTSUKA3, Hideko NOMURA4, Satoshi OKUZUMI4 (1.Kyoto University, 2.The National Astronomical Observatory of Japan, 3.Nagoya university, 4.Tokyo Institute of Technology)
4:30 PM - 4:45 PM
*Hotaka ITOU1, Takanobu AMANO1, Masahiro HOSHINO1 (1.Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo)
4:45 PM - 5:00 PM
*Hiroyasu TADOKORO1, Yuto KATOH2 (1.Tokyo University of Technology, 2.Department of Geophysics, Graduate School of Science, Tohoku University)
5:00 PM - 5:15 PM
*Yuki TANAKA1, Takeru SUZUKI1, Shu-ichiro INUTSUKA1 (1.Department of Physics, Nagoya University)
5:15 PM - 5:30 PM
*Tetsu MIENO1, Risa MASUDA2, Takashi MORIBAYASHI2, Yasuaki HAYASHI3 (1.Grad. School Sci. Technol, Shizuoka Univ., 2.Dept. Phys., Shizuoka Univ., 3.Grad. School Eng., Kyoto Inst. Technol.)
Please log in with your participant account.
» Participant Log In