Local relaxation and scale-dependent alignment in compressible, magnetized turbulence

arXiv:2504.15538 · physics.plasm-ph, astro-ph.GA, nlin.CD, physics.flu-dyn · Submitted 2025-04-22 · Read on arXiv

physics.plasm-ph, astro-ph.GA, nlin.CD, physics.flu-dyn

Submitted: 2025-04-22

Updated: 2026-09-12

Comments: 6 pages including acknowledgments, 3 main figures; 14 pages total, including Supplemental Material with 2 figures. Accepted in PRL

License: http://creativecommons.org/licenses/by/4.0/

The gist: Driven net- and no-net-flux MHD turbulence simulations up to 10,!368 cubed reveal sign-mixed velocity--magnetic, velocity--vorticity, and magnetic--current aligned patches below the energy

Terminology

Abstract

Driven net- and no-net-flux MHD turbulence simulations up to 10,!368 cubed reveal sign-mixed velocity--magnetic, velocity--vorticity, and magnetic--current aligned patches below the energy equipartition scale. The first two angles scale as λ 1/8 and λ 1/16, while the third angle varies weakly with scale. We develop and test a constant-flux transport model for departures from relaxed states, which predicts both exponents. These findings affect eddy anisotropy, reconnection-mediated turbulence onset, large-scale dynamos, and the nature of magnetized turbulence.

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