Exploring the Ideal MHD Quasi-Modes of a Plasma Interface with a Thick Nonuniform Transition
Nonuniform plasma across an imposed magnetic field, such as those present in the solar atmosphere, can support collective Alfvénic oscillations with a characteristic damping time. The damped transverse oscillations of coronal loops are an example of this process. In ideal magnetohydrodynamics (MHD),...
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| Format: | Article |
| Language: | English |
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MDPI AG
2022-11-01
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| Series: | Physics |
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| Online Access: | https://www.mdpi.com/2624-8174/4/4/87 |