Magnetohydrodynamic waves in the partially ionized solar plasma

被引:5
|
作者
Soler, Roberto [1 ,2 ]
机构
[1] Univ Illes Balears, Dept Fis, Palma De Mallorca, Spain
[2] Univ Illes Balears, Inst Aplicac Computac Codi Comunitari IAC3, Palma De Mallorca, Spain
关键词
magnetohydrodynamic waves; solar atmosphere; partially ionized plasma; MAGNETIC TUBE WAVES; SLOW MAGNETOACOUSTIC WAVES; STELLAR CONVECTION ZONES; TORSIONAL ALFVEN WAVES; ION-NEUTRAL COLLISIONS; MHD WAVES; ENERGY FLUX; GENERATION; CHROMOSPHERE; PROMINENCE;
D O I
10.1098/rsta.2023.0223
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
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'.
引用
收藏
页数:39
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