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タイトル: Simulation study of near-Earth space disturbances: 1. magnetic storms
著者: Ebihara, Yusuke  kyouindb  KAKEN_id  orcid https://orcid.org/0000-0002-2293-1557 (unconfirmed)
著者名の別形: 海老原, 祐輔
キーワード: Magnetic storms
Computer simulation
Magnetosphere
Ionosphere
Inner magnetosphere
Ring current
発行日: 2019
出版者: Springer Nature
誌名: Progress in Earth and Planetary Science
巻: 6
論文番号: 16
抄録: A magnetic storm is the world-wide geomagnetic disturbance taking place in near-Earth space environment, lasting for a few days. Geomagnetic fields can be depressed by ~ 1% on the ground for large magnetic storms. The prime cause of the long-lasting, world-wide geomagnetic disturbance is the development of the ring current that surrounds the Earth. The ring current is an electric current carried by charged particles. Thus, the growth and decay of the ring current correspond to accumulation and loss of the ring current particles, respectively. The ring current is strong enough to modulate near-Earth space environment, and leads to many observable effects. In this sense, the ring current can be regarded as an important mediator in the near-Earth space environment. Here, the dynamics and structure of the ring current and its active role are briefly reviewed on the basis of numerical simulation results.
著作権等: © The Author(s). 2019. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
URI: http://hdl.handle.net/2433/236642
DOI(出版社版): 10.1186/s40645-019-0264-3
出現コレクション:学術雑誌掲載論文等

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