During geomagnetic storms, some fraction of the solar wind energy is coupled via reconnection at the dayside magnetopause, a process that requires a southward interplanetary magnetic field
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The total energy transfer from the solar wind to the magnetosphere is governed by the reconnection rate at the magnetosphere edges as the Z‐component of interplanetary magnetic field (IMF
- Award ID(s):
- 2148653
- NSF-PAR ID:
- 10490449
- Publisher / Repository:
- AGU
- Date Published:
- Journal Name:
- Space Weather
- Volume:
- 21
- Issue:
- 10
- ISSN:
- 1542-7390
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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