Exact solution to the problem of slow oscillations in coronal loops and its diagnostic applications
Magnetoacoustic oscillations are nowadays routinely observed in various regions of the solar corona. This allows them to be used as means of diagnosing plasma parameters and processes occurring in it. Plasma diagnostics, in turn, requires a sufficiently reliable MHD model to describe the wave evolut...
| Hlavní autoři: | , , , |
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| Médium: | Článek |
| Jazyk: | English |
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Frontiers Media S.A.
2023-05-01
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| Edice: | Frontiers in Astronomy and Space Sciences |
| Témata: | |
| On-line přístup: | https://www.frontiersin.org/articles/10.3389/fspas.2023.1167781/full |