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:
✦ LIBER ✦
Roles of interplanetary and geomagnetic parameters in ‘intense’ and ‘very intense’ magnetic storms generation and their geoeffectiveness
✍ Scribed by Adebesin, B.
- Book ID
- 120889490
- Publisher
- Akadmiai Kiad
- Year
- 2008
- Tongue
- English
- Weight
- 777 KB
- Volume
- 43
- Category
- Article
- ISSN
- 1217-8977
No coin nor oath required. For personal study only.
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