Propagating torsional Alfv\'en waves in thermally active solar plasma
S.A. Belov, S. Vasheghani Farahani, N.E. Molevich

TL;DR
This study investigates how thermal misbalance affects the propagation of torsional and shear Alfvén waves in thermally active solar plasma, revealing differences in induced motions and the influence of plasma-beta.
Contribution
It provides an analytical description of nonlinear forces and the effects of thermal misbalance on Alfvén wave-induced motions in non-ideal, thermally active solar plasma.
Findings
Shear Alfvén waves induce greater phase shifts and amplitudes in longitudinal motions than torsional waves.
Thermal misbalance influences velocity perturbations more strongly in shear waves, especially at different plasma-beta values.
Density perturbations remain unaffected by thermal misbalance for harmonic Alfvén wave drivers.
Abstract
The aim of the present study is to shed light on the effects connected with thermal misbalance due to non-equal cooling and heating rates induced by density and temperature perturbations in solar active regions hosting either propagating torsional or shear Alfv\'en waves. A description for the nonlinear forces connected with Alfv\'en waves in non-ideal conditions is provided based on the second order thin flux tube approximation. This provides insight on the effects of Alfv\'en-induced motions on the boundary of thin magnetic structures in thermally active plasmas. The equations describing the process of generating longitudinal velocity perturbations together with density perturbations by nonlinear torsional Alfv\'en waves are obtained and solved analytically. It is shown that the phase shift (compared to the ideal case) and the amplitude of the induced longitudinal plasma motions…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Magnetic confinement fusion research
