Simulation study of near-Earth space disturbances : 1. magnetic storms
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DOI[10.1186/s40645-019-0264-3]to the data of the same series
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- Material Type
- 記事
- Author/Editor
- Yusuke Ebihara
- Publication, Distribution, etc.
- Publication Date
- 2019-02-13
- Publication Date (W3CDTF)
- 2019-02-13
- Periodical title
- Progress in earth and planetary science
- No. or year of volume/issue
- 6(16)
- Volume
- 6(16)
- ISSN (Periodical Title)
- 2197-4284
- ISSN-L (Periodical Title)
- 2197-4284
- Text Language Code
- eng
- DOI
- 10.1186/s40645-019-0264-3
- Persistent ID (NDL)
- info:ndljp/pid/11249504
- Collection
- Collection (Materials For Handicapped People:1)
- Collection (particular)
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- Acquisition Basis
- オンライン資料収集制度
- Date Accepted (W3CDTF)
- 2019-03-05T23:10:26+09:00
- Date Captured (W3CDTF)
- 2019-03-05
- Format (IMT)
- application/pdf
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/11249488
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- Summary, etc.
- 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.
- DOI
- 10.1186/s40645-019-0264-3
- Access Restrictions
- インターネット公開
- Rights (production)
- © 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.
- Related Material (URI)
- References
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Ngwira, A. Pulkkinen, M.M. Kuznetsova and A. Glocer”International Geomagnetic Reference Field : the 12th generation
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 学術機関リポジトリデータベース雑誌記事索引データベースCrossrefCiNii Articles科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース
- Bibliographic ID (NDL)
- 11249504
- NAID
- 120006576447