Magnetohydrodynamic waves in the partially ionized solar plasma

Author:

Soler Roberto12ORCID

Affiliation:

1. Departament de Física, Universitat de les Illes Balears, Palma de Mallorca, Spain

2. Institut d’Aplicacions Computacionals de Codi Comunitari (IAC3), Universitat de les Illes Balears, Palma de Mallorca, Spain

Abstract

This paper provides a comprehensive review of recent theoretical investigations concerning magnetohydrodynamic (MHD) waves in partially ionized solar plasma. First, we examine the properties of linear MHD waves in a uniform partially ionized plasma and discuss the relevant effects arising from partial ionization. Subsequently, we delve into MHD wave studies in the more intricate settings of the lower solar atmosphere and solar prominences. These investigations involve topics such as MHD waves in magnetic flux tubes, wave excitation, linear and nonlinear mode coupling and wave heating. We outline new challenges that future research should tackle. This article is part of the theme issue ‘Partially ionized plasma of the solar atmosphere: recent advances and future pathways’.

Funder

Agencia Estatal de Investigación

Publisher

The Royal Society

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Partially ionized plasma of the solar atmosphere: recent advances and future pathways;Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences;2024-04-25

2. Analytical and numerical solution of sausage MHD wave oscillation in a thin magnetic flux tube;AIMS Mathematics;2024

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