Waves in weakly ionised solar plasmas
A. Alharbi, I. Ballai, V. Fedun, G. Verth

TL;DR
This paper investigates wave propagation in weakly ionised solar plasmas, revealing how collisional and magnetic effects influence wave characteristics in different solar atmospheric regions.
Contribution
It provides a detailed analysis of wave behavior in weakly ionised solar plasmas, highlighting the transition from three-fluid to two-fluid models across the chromosphere and photosphere.
Findings
Neutral sound waves propagate without damping in the photosphere.
Ion and electron acoustic modes are affected by collisional damping.
Wave propagation varies significantly between the photosphere and chromosphere.
Abstract
Here we study the nature and characteristics of waves propagating in partially ionised plasmas in the weakly ionised limit, typical for the lower part of the solar atmosphere. The framework in which the properties of waves are discussed depends on the relative magnitude of collisions between particles, but also on the relative magnitude of the collisional frequencies compared to the gyro-frequency of charged particles. Our investigation shows that the weakly ionised solar atmospheric plasma can divided into two regions and this division occurs, roughly, at the base of the chromosphere. In the solar photosphere the plasma is non-magnetised and the dynamics can described within the three-fluid framework where acoustic waves associated to each species can propagate. Due to the very high concentration of neutrals, the neutral sound waves propagates with no damping, while for the other two…
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