The dominant interplanetary phenomena causing intense magnetic storms are the interplanetary manifestations of fast coronal mass ejections (CMEs). Two interplanetary structures are important for the development of such class of storms, involving an intense and long duration Bs component of the IMF:
β¦ LIBER β¦
Interplanetary phenomena associated with very intense geomagnetic storms
β Scribed by W.D Gonzalez; B.T Tsurutani; R.P Lepping; R Schwenn
- Publisher
- Elsevier Science
- Year
- 2002
- Tongue
- English
- Weight
- 191 KB
- Volume
- 64
- Category
- Article
- ISSN
- 1364-6826
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