Local Relaxation and Scale-Dependent Alignment in Compressible, Magnetized Turbulence
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Updated: Nov 2, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
James R Beattie1, Amitava Bhattacharjee2
1University of Toronto, Princeton University, Department of Astrophysical Sciences, Princeton, New Jersey 08540, USA; Canadian Institute for Theoretical Astrophysics, Toronto, M5S3H8, Ontario, Canada; and School of Natural Sciences, Institute for Advanced Study, 1 Einstein Drive, Princeton, New Jersey 08540, USA.
Abstract:
Patchy alignment pervades magnetohydrodynamic (MHD) turbulence, yet its role in the turbulent cascade remains unclear. Using net- and no-net-flux compressible simulations with up to 10,368^{3} grid cells, we uncover two distinct alignment laws. Our constant-flux model of departures from locally aligned states predicts the measured velocity-magnetic and velocity-vorticity angle scalings, λ^{1/8} and λ^{1/16}, over resolved inertial scales λ. These laws change the predicted shapes of turbulent eddies and raise the theoretical threshold for magnetic reconnection to control the flow of energy across scales.
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