Exploring the Ideal MHD Quasi-Modes of a Plasma Interface with a Thick Nonuniform Transition

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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Bibliographic Details
Main Author: Roberto Soler
Format: Article
Language:English
Published: MDPI AG 2022-11-01
Series:Physics
Subjects:
Sun: oscillations
Sun: atmosphere
waves
magnetohydrodynamics (MHD)
Online Access:https://www.mdpi.com/2624-8174/4/4/87

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