Japan Geoscience Union Meeting 2014

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Poster

Symbol M (Multidisciplinary and Interdisciplinary) » M-GI General Geosciences, Information Geosciences & Simulations

[M-GI37_29PO1] Earth and planetary informatics with huge data management

Tue. Apr 29, 2014 6:15 PM - 7:30 PM Poster (3F)

Convener:*TOYODA Eizi(Numerical Prediction Division, Japan Meteorological Agency), Yasuhiro Murayama(National Institute of Information and Communications Technology), Junya Terazono Junya(The University of Aizu), Tomoaki Hori(Nagoya University Solar Terrestrial Environment Laboratory Geospace Research Center), Kazuo Ohtake(Japan Meteorological Agency), Mayumi Wakabayashi(Kiso-Jiban Consultants Co.,Ltd), Takeshi Horinouchi(Faculty of Environmental Earth Science, Hokkaido University), Susumu Nonogaki(Geological Survey of Japan, National Institute of Advanced Industrial Science and Technology)

6:15 PM - 7:30 PM

[MGI37-P02] Radio observation network of Tohoku University

*Manabu YAGI1, Takahiro OBARA1, Masato KAGITANI1, Mizuki YONEDA1, Atsushi KUMAMOTO1, Hiroaki MISAWA1, Fuminori TSUCHIYA1, Kazumasa IWAI2, Naoki TERADA1, Hiroyo OHYA3 (1.Tohoku Univ., 2.NAOJ, 3.Chiba Univ.)

Keywords:radio observation, database, upper atmosphere

Planetary Plasma and Atmospheric Research Center (PPARC) of the Tohoku University is now in progress to build a upper atmosphere, planetary, and space physics database under collaboration with the Inter-university Upper atmosphere Global Observation NETwork (IUGONET). The core data of the database are planetary and solar radio observation by Iitate Planetary Radio Telescope (IPRT) and Jupiter/galaxy decameter radio receiver working in Iitate observatory, that is one of the observatory of Tohoku University. Development of database of LF/VLF wave observation at Athabasca, Ny-Alesund, and Asia VLF Observation Network (AVON) are undergoing collaborated with Chiba University. In the presentation, we will introduce the observations of solar radio burst with high time resolution using the AMATERAS spectrometer of IPRT, as well as lightning and precipitation of high energy electrons into the atmosphere observed by LF/VLF wave.