書誌事項
- 公開日
- 2000
- 権利情報
-
- https://www.elsevier.com/tdm/userlicense/1.0/
- https://www.elsevier.com/legal/tdmrep-license
- DOI
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- 10.1016/s0273-1177(99)01087-x
- 公開者
- Elsevier BV
この論文をさがす
説明
Abstract Comparative studies of solar flares and substorms are useful in obtaining comprehensive understanding of magnetic reconnection processes, since flare studies give us better information on macroscopic processes such as global changes of magnetic field configuration while substorm studies give us more detailed knowledge on microscopic processes. Recent spacecraft observations both for magnetospheric substorms and solar flares have dramatically enriched our understanding for physical processes occurring during these interesting phenomena. We first summarize keys of these new observations from the magnetotail studies, and try to compare them with those from the solar flare studies on a common physical basis.
収録刊行物
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- Advances in Space Research
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Advances in Space Research 26 (3), 573-583, 2000
Elsevier BV
