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Kelvin-Helmholtz instability in solar spicules
Magneto hydrodynamic waves, propagating along spicules, may become unstable and the expected instability is of Kelvin-Helmholtz type. Such instability can trigger the onset of wave turbulence leading to an effective plasma heating and particle acceleration. In present study, two-dimensional magneto...
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| 1. autor: | |
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| Format: | Artigo |
| Język: | Inglês |
| Wydane: |
Isfahan University of Technology
2016-12-01
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| Seria: | Iranian Journal of Physics Research |
| Hasła przedmiotowe: | |
| Dostęp online: | http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-782&slc_lang=en&sid=1 |
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