Singular limits of anisotropic weak solutions to compressible magnetohydrodynamics
Nicolas Besse, Christophe Cheverry

TL;DR
This paper rigorously justifies the reduced magnetohydrodynamic (RMHD) model for strongly anisotropic plasmas by analyzing the asymptotic behavior of weak solutions to the compressible MHD equations, highlighting anisotropic incompressibility and convergence in both periodic and unbounded domains.
Contribution
It provides a rigorous mathematical proof of the convergence of anisotropic weak solutions to the RMHD equations in the context of strongly magnetized plasmas, including both periodic and unbounded domains.
Findings
Weak solutions converge to RMHD equations in the anisotropic limit.
Incompressibility is only in the perpendicular direction to the magnetic field.
The analysis employs tools from low Mach number limits and oscillatory group techniques.
Abstract
The aim is to justify rigorously the so-called reduced magnetohydrodynamic model (abbreviated as RMHD), which is widely used in fusion, space and astrophysical plasmas. Motivated by physics, the focus is on plasmas that are simultaneously strongly magnetized and anisotropic. We consider conducting fluids that can be described by viscous and resistive barotropic compressible magnetohydrodynamic equations. The purpose is to study the asymptotic behaviour of global weak solutions, which do exist, for strongly anisotropic plasmas such as the large aspect ratio framework. We prove that such anisotropic weak solutions converge to the weak solutions of the RMHD equations. Rigorous justification of this limit is performed both in a periodic domain and in the whole space. It turns out that the resulting system is incompressible only in the perpendicular direction to the external strong magnetic…
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Taxonomy
TopicsNavier-Stokes equation solutions · Nonlinear Waves and Solitons · Solar and Space Plasma Dynamics
