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Magnetoacoustic Waves and the Kelvin–Helmholtz Instability in a Steady Asymmetric Slab: I: The Effects of Varying Density Ratios
Recent observations have shown that bulk flow motions in structured solar plasmas, most evidently in coronal mass ejections (CMEs), may lead to the formation of Kelvin–Helmholtz instabilities (KHIs). Analytical models are thus essential in understanding both how the flows affect the propagation of m...
| Autores principales: | , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Springer Netherlands
2018
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6438655/ https://www.ncbi.nlm.nih.gov/pubmed/30996491 http://dx.doi.org/10.1007/s11207-018-1305-6 |