Magnetohydrodynamic waves in the partially ionized solar plasma

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’.

Partially ionized plasma of the solar atmosphere: recent advances and future pathways

“…As these waves are ubiquitous in the partially ionized solar atmosphere, understanding the influence of partial ionization on MHD waves is a key topic of this issue. To lead this area, the review article by Soler [ 4 ] provides a comprehensive overview of the current understanding of the field. Ballester et al [ 5 ] studied the coupling of nonlinear Alfvén waves to thermodynamics in partially ionized plasma finding a complex interplay of damping mechanisms for the waves.…”