Solar wind drivers of geomagnetic storms during more than four solar cycles
Using a classification of the near-Earth solar wind into three basic flow types: (1) High-speed streams associated with coronal holes at the Sun; (2) Slow, interstream solar wind; and (3) Transient flows originating with coronal mass ejections (CMEs) at the Sun, including interplanetary CMEs and the...
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| Principais autores: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
EDP Sciences
2012-05-01
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| coleção: | Journal of Space Weather and Space Climate |
| Assuntos: | |
| Acesso em linha: | http://dx.doi.org/10.1051/swsc/2012001 |
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