Wave turbulence in magnetohydrodynamics
Sebastien Galtier

TL;DR
This paper reviews recent advances in understanding wave turbulence in magnetized plasmas, focusing on theoretical frameworks, key results, and applications to space and laboratory plasmas over the past two decades.
Contribution
It provides a comprehensive overview of wave turbulence in MHD, Hall MHD, and electron MHD, highlighting recent progress and discussing potential issues in interpretation.
Findings
Key results on wave turbulence in space plasmas
Analysis of anisotropic turbulence in magnetized media
Discussion of theoretical and experimental challenges
Abstract
This chapter reviews the recent progress made mainly during the last two decades on wave turbulence in magnetized plasmas (MHD, Hall MHD and electron MHD) in the incompressible and compressible cases. The emphasis is made on homogeneous and anisotropic turbulence which usually provides the best theoretical framework to investigate space and laboratory plasmas. The interplanetary medium and the solar atmosphere are presented as two examples of media where anisotropic wave turbulence is relevant. The most important results of wave turbulence are reported and discussed in the context of space and simulated magnetized plasmas. Important issues and possible spurious interpretations are eventually discussed.
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Magnetic confinement fusion research
