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¦
The solar causes of major geomagnetic storms
β Scribed by S. Bravo; A. L. Rivera
- Publisher
- Copernicus Group
- Year
- 1994
- Tongue
- English
- Weight
- 61 KB
- Volume
- 12
- Category
- Article
- ISSN
- 0992-7689
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