JpGU-AGU Joint Meeting 2020

講演情報

[E] ポスター発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM18] 太陽地球系結合過程の研究基盤形成

コンビーナ:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)

[PEM18-P14] Recent and future activities of ICSWSE and MAGDAS project

*阿部 修司1藤本 晶子2魚住 禎司1吉川 顕正1,3 (1.九州大学 国際宇宙天気科学・教育センター、2.九州工業大学、3.九州大学 大学院理学研究院地球惑星科学部門)

International Center for Space Weather Science and Education (ICSWSE), Kyushu University is the research institute for conducting research and education in space weather. We are operating world-wide magnetometer array named as "MAGDAS/CPMN (MAGnetic Data Acquisition System/Circum-pan Pacific Magnetometer Network)" (Principal Investigator: Dr. A. Yoshikawa) for these. It consists of over seventy fluxgate magnetometers, one induction magnetometer, and four FM-CW (Frequency Modulated Continuous Wave) radars. One of our recent research topics is Equatorial Electrojet (EEJ). To accelerate the understanding of EEJ structure, we are constructing dense instrument array across the magnetic equator at Peru and Malaysia in recent year. The latest magnetometer is installed at Penang, Malaysia last September. On last March, we maintained the latest FM-CW radar at Sicaya, Peru. We calculate EE-index (Uozumi et al, 2008; Fujimoto et al., 2016) for space weather nowcast/forecast using realtime magnetometer data along the magnetic equator, and publish it at each hour on the web. We provide our observational information and data including old project via our website, and via IUGONET (Inter-university Upper Atmosphere Observation NETwork) web service and data analysis software. We believe MAGDAS data will help any researchers for their research under proper rule.