Dynamics of fast and slow magnetoacoustic waves in plasma slabs with thermal misbalance

Abstract

Non-uniformity of the solar atmosphere along with the presence of non-adiabatic processes such as radiation cooling and unspecified heating can significantly affect the dynamics and properties of magnetoacoustic (MA) waves. To address the co-influence of these factors on the dispersion properties of MA waves, we considered a single magnetic slab composed of the thermally active plasma. Using the perturbation theory, we obtained a differential equation that determines the dynamics of the two-dimensional perturbations. Applying the assumption of strong magnetic structuring, we derived the dispersion relations for the sausage and kink MA modes. The numerical solution of the dispersion relations for the coronal conditions was performed to investigate the interplay between the non-uniformity and the thermal misbalance. For the heating scenario considered, it was obtained that the phase speed of both the sausage and kink slow MA waves is highly affected by the thermal misbalance in the long wavelength limit. The obtained characteristic timescales of the slow waves dissipation coincide with the periods of waves observed in the corona. Simultaneously, the phase speed of the fast waves is not affected by the thermal misbalance. The geometry of the magnetic structure still remains the main dispersion mechanism for the fast waves. Our estimation reveals that dissipation of the fast waves is weaker than dissipation of the slow waves in the coronal conditions. The obtained results are of importance for using the magnetoacoustic waves not only as a tool for estimating plasma parameters, but also as a tool for estimating the non-adiabatic processes.

References in corpus (11)

• CHIANTI -- an atomic database for emission lines -- Paper XVI: Version 10, further extensions
• Kink oscillations of coronal loops
• Slow-Mode Magnetoacoustic Waves in Coronal Loops
• MHD Waves in open coronal structures
• Frequency-dependent damping in propagating slow magneto-acoustic waves
• Magnetohydrodynamic Fast Sausage Waves in the Solar Corona
• The solar corona as an active medium for magnetoacoustic waves
• The effect of magnetic field on the damping of slow waves in the solar corona
• Dispersion of Slow Magnetoacoustic Waves in the Active Region Fan Loops Introduced by Thermal Misbalance
• Mixed properties of slow magnetoacoustic and entropy waves in a plasma with heating/cooling misbalance
• Effect of Thermal Conductivity, Compressive Viscosity and Radiative Cooling on the Phase Shift of Propagating Slow Waves with and without Heating-Cooling Imbalance

Cited by in corpus (3)

• Exact solution to the problem of slow oscillations in coronal loops and its diagnostic applications
• Impact of thermal misbalance on acoustic-gravity waves in the solar atmosphere
• The effect of thermal misbalance on magnetohydrodynamic modes in coronal magnetic cylinders