Guided Waves Along a Density Interface in Partially Ionised Solar Plasmas
S. Alshammari, Istvan Ballai, Gary Verth, Viktor Fedun, Lyudmila Kozak

TL;DR
This paper studies how waves behave along density interfaces in partially ionised solar plasmas, focusing on how ionisation and pressure affect wave propagation and damping.
Contribution
The study introduces a new analysis of guided wave properties in partially ionised solar plasmas using a single-fluid approximation and ambipolar diffusion.
Findings
Guided waves along density interfaces show minimal changes in propagation speed but significant damping rate variations.
Waves can only propagate when the plasma-β exceeds 1.2, indicating pressure-driven dynamics in moderate magnetic fields.
Damping increases with higher neutral particle content but decreases with higher plasma-β values.
Abstract
This study investigates the properties of waves that propagate along a density interface in partially ionised plasmas, separating two regions of different properties, including ionisation degree. Our analysis covers frequencies that are much smaller than the collisional frequency of particles, so we are using a single-fluid approximation, where the partial ionisation aspect of the plasma appears through the ambipolar diffusion in the generalised Ohm’s law. The derived dispersion relation is solved numerically. Our results show that guided waves along a density interface undergo very little change in their propagation speed (frequency); however, their damping rate shows variation with the ionisation degree and plasma-\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy}…
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Taxonomy
TopicsIonosphere and magnetosphere dynamics · Dust and Plasma Wave Phenomena · Solar and Space Plasma Dynamics
