Residual Energy and Broken Symmetry in Reduced Magnetohydrodynamics

Residual Energy and Broken Symmetry in Reduced Magnetohydrodynamics

Alfvénic interactions that transfer energy from large to small spatial scales lie at the heart of magnetohydrodynamic turbulence. An important feature of the turbulence is the generation of negative residual energy—excess energy in magnetic fluctuations compared to velocity fluctuations. By contrast...

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Bibliographic Details
Main Authors: S. Dorfman, M. Abler, S. Boldyrev, C. H. K. Chen, S. Greess
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Magnetohydrodynamics
Interplanetary turbulence
Alfvén waves
Solar wind
Online Access:https://doi.org/10.3847/1538-4357/ad9012
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