Mathematical estimates for the attractor dimension in MHD turbulence
Alban Poth\'erat, Thierry Alboussi\`ere

TL;DR
This paper derives rigorous mathematical estimates for the attractor dimension and dissipative scales in magnetohydrodynamic turbulence, considering the effects of strong magnetic fields on flow complexity and structure.
Contribution
It introduces a new method to estimate the attractor dimension in MHD turbulence with periodic boundary conditions and magnetic fields, extending previous hydrodynamic turbulence results.
Findings
Upper bounds for attractor dimension in MHD turbulence derived.
Analysis of flow anisotropy and dissipative scales under magnetic influence.
Comparison of mathematical estimates with heuristic predictions.
Abstract
The aim of the present work is to derive rigorous estimates for turbulent MHD flow quantities such as the size and anisotropy of the dissipative scales, as well as the transition between 2D and 3D state. To this end, we calculate an upper bound for the attractor dimension of the motion equations, which indicates the number of modes present in the fully developed flow. This method has already been used successfully to derive such estimates for 2D and 3D hydrodynamic turbulence as a function of the norm of the dissipation, as in \cite{doering95}. We tackle here the problem of a flow periodic in the 3 spatial directions (spatial period ), to which a permanent magnetic field is applied. In addition, the detailed study of the dissipation operator provides more indications about the structure of the flow. In section 2, we review the tools of the dynamical system…
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Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Navier-Stokes equation solutions · Advanced Thermodynamics and Statistical Mechanics
