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Turbulent mass transfer caused by vortex induced reconnection in collisionless magnetospheric plasmas
Magnetic reconnection is believed to be the main driver to transport solar wind into the Earth’s magnetosphere when the magnetopause features a large magnetic shear. However, even when the magnetic shear is too small for spontaneous reconnection, the Kelvin–Helmholtz instability driven by a super-Al...
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| Veröffentlicht in: | Nat Commun |
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| Hauptverfasser: | , , , , , |
| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
Nature Publishing Group UK
2017
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| Schlagworte: | |
| Online Zugang: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5693928/ https://ncbi.nlm.nih.gov/pubmed/29150662 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/s41467-017-01579-0 |
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