Magnetic field and dynamic pressure ULF fluctuations in coronal-mass-ejection-driven sheath regions
Compressed sheath regions form ahead of interplanetary coronal mass ejections (ICMEs) that are sufficiently faster than the preceding solar wind. The turbulent sheath regions are important drivers of magnetospheric activity, but due to their complex internal structure, relatively little is known...
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| Autori principali: | , , , , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Copernicus Publications
2013-09-01
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| Serie: | Annales Geophysicae |
| Accesso online: | https://www.ann-geophys.net/31/1559/2013/angeo-31-1559-2013.pdf |
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