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

Beattie, James R. et al.
arXiv (OAI Expanded) · Papers
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astrophysics-of-galaxieschaotic-dynamicsfluid-dynamicsplasma-physics
Driven net- and no-net-flux MHD turbulence simulations up to $10,\!368^3$ 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
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