Magnetic field disturbances in the sheath region of a super-sonic interplanetary magnetic cloud
It is well-known that interplanetary magnetic clouds can cause strong geomagnetic storms due to the high magnetic field magnitude in their interior, especially if there is a large negative <I>B<sub>z</sub></I> component present. In addition, the magnetic disturbances aroun...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2008-10-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/26/3153/2008/angeo-26-3153-2008.pdf |