日本地球惑星科学連合2023年大会

講演情報

[E] オンラインポスター発表

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-EM15] 太陽地球系結合過程の研究基盤形成

2023年5月26日(金) 15:30 〜 17:00 オンラインポスターZoom会場 (4) (オンラインポスター)

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)

現地ポスター発表開催日時 (2023/5/26 17:15-18:45)

15:30 〜 17:00

[PEM15-P15] Recent activities of i-SPES and MAGDAS project

*阿部 修司1藤本 晶子2池田 昭大4魚住 禎司1吉川 顕正1,3 (1.九州大学 国際宇宙惑星環境研究センター、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、4.鹿児島工業高等専門学校)

International research center for Space and Planetary Environmental Science(I-SPES), Kyushu University is the research institute for conducting research and education in in solar terrestrial physics. "MAGDAS/CPMN (MAGnetic Data Acquisition System/Circum-pan Pacific Magnetometer Network)" (Principal Investigator: Dr. A. Yoshikawa) is world-wide observation array, which consists of over seventy fluxgate magnetometers, one induction magnetometer, and four FM-CW (Frequency Modulated Continuous Wave) radars. One of our research topics is Equatorial Electrojet (EEJ). To observe the temporal and long-term variation of EEJ, we installed many magnetometers around the magnetic equator, and calculate EE-index (Uozumi et al, 2008; Fujimoto et al., 2016) for space weather nowcast/forecast using realtime data along the magnetic equator. These results are published on our web, and updated at each hour. Furthermore, we are planning to extend our observation network to the region east of Java, Indonesia. By constructing an observation network extends to the longitude region, we expect to investigate the spatial and temporal evolution of space weather phenomena in detail and to understand their physical mechanisms. From the viewpoint of internal electromagnetics, the objective is to improve the observation accuracy by covering a wider area with higher density, and to detect local variation of internal electromagnetic phenomena early. This research will be conducted as international joint research between Japan, Indonesia, and Egypt.
To provide our observational information and data including old project is also important matter for us. We are one of the members of IUGONET (Inter-university Upper Atmosphere Observation NETwork), and users can access our information via IUGONET metadata database and data analysis software. In addition, we plan to work with the Kyushu University Library to obtain a DOI to make our data more widely available to the public. In this paper, we will introduce our current activities on observation, science, and informatics fields.