Current sheets from Ulysses observation
Current sheet is a significant source of solar wind MHD turbulence intermittency. It has long been recognized that these structures can arise from non-linear interactions of MHD turbulence. Alternatively, they may also be relic structures in the solar wind that have a solar origin, e.g., magnetic...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2011-02-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/29/237/2011/angeo-29-237-2011.pdf |