Ray tracing methods for wave propagation in moving anisotropic media : application to magnetized plasmas

TL;DR

This paper develops a ray tracing method for wave propagation in moving anisotropic media, specifically magnetized plasmas, by transforming known dispersion relations to account for medium motion, aiding understanding in astrophysics and fusion devices.

Contribution

It introduces a novel approach using Lorentz transformations to derive ray tracing equations for moving anisotropic media, extending geometrical optics in plasma physics.

Findings

Derived effective dispersion relations for moving media

Applied method to magnetized plasma modes

Established foundation for higher-order polarization effects

Abstract

The propagation of a wave in a medium is generally affected when the medium is moving with respect to the observer. Because plasma equilibria often involve plasma flows, for instance in astrophysics or in magnetic confinement nuclear fusion devices, understanding the effect of motion on plasma waves is important. Meanwhile, the presence of a background magnetic field in a plasma makes it anisotropic. To address this problem, we derive here ray tracing equations for the trajectory of rays propagating in a moving anisotropic medium. The proposed approach is to use an effective dispersion relation for the moving medium as seen from the laboratory, obtained by performing a Lorentz transformation of the dispersion relation known for the medium at rest. This formalism is illustrated by considering the standard ordinary and extraordinary modes in a magnetized plasma at rest. Although we work here at lowest order in the geometrical optics approximation, this method is a first step towards higher order expansions, as required for instance to capture polarization effects.