書誌事項
- 公開日
- 1994-04
- 権利情報
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- http://onlinelibrary.wiley.com/termsAndConditions#vor
- DOI
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- 10.1029/93ja02867
- 公開者
- American Geophysical Union (AGU)
この論文をさがす
説明
<jats:p>After a brief review of magnetospheric and interplanetary phenomena for intervals with enhanced solar wind‐magnetosphere interaction, an attempt is made to define a geomagnetic storm as an interval of time when a sufficiently intense and long‐lasting interplanetary convection electric field leads, through a substantial energization in the magnetosphere‐ionosphere system, to an intensified ring current sufficiently strong to exceed some key threshold of the quantifying storm time <jats:italic>Dst</jats:italic> index. The associated storm/substorm relationship problem is also reviewed. Although the physics of this relationship does not seem to be fully understood at this time, basic and fairly well established mechanisms of this relationship are presented and discussed. Finally, toward the advancement of geomagnetic storm research, some recommendations are given concerning future improvements in monitoring existing geomagnetic indices as well as the solar wind near Earth.</jats:p>
収録刊行物
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- Journal of Geophysical Research: Space Physics
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Journal of Geophysical Research: Space Physics 99 (A4), 5771-5792, 1994-04
American Geophysical Union (AGU)
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詳細情報 詳細情報について
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- CRID
- 1363388844518895360
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- NII論文ID
- 80007591285
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- ISSN
- 01480227
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- データソース種別
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- Crossref
- CiNii Articles
- OpenAIRE
