Plasma equilibrium equations in coordinates connected with magnetic surfaces. Exact equilibrium solutions
Alexei F. Cheviakov

TL;DR
This paper introduces a method to represent static MHD equilibrium equations in specialized coordinates, enabling the construction of exact 3D plasma equilibrium solutions in various geometries without relying on symmetries.
Contribution
It proposes a new coordinate-based approach to derive exact 3D plasma equilibrium solutions, expanding the possibilities for modeling complex plasma configurations.
Findings
Generated families of non-trivial 3D plasma equilibrium solutions
Applicable to both isotropic and anisotropic plasmas
Solutions include static and dynamic equilibria in diverse geometries
Abstract
A representation of the static MHD equilibrium system in coordinates connected with magnetic surfaces is suggested. It is used for producing families of non-trivial 3D exact solutions of isotropic and anisotropic plasma equilibria in different geometries, with and without dynamics, and often without geometrical symmetries. The ways of finding coordinates in which exact equilibria can be constructed are discussed; examples and their applications as physical models are presented.
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Taxonomy
TopicsGas Dynamics and Kinetic Theory · Solar and Space Plasma Dynamics · Atomic and Molecular Physics
