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Exact Relation with Two-point Correlation Functions and Phenomenological Approach for Compressible Magnetohydrodynamic Turbulence

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arxiv 1301.2470 v1 pith:YZGM4A75 submitted 2013-01-11 physics.flu-dyn astro-ph.SR

classification physics.flu-dynastro-ph.SR
keywords exactmagneticrelationcompressiblecorrelationenergyfieldfunctions
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Compressible isothermal magnetohydrodynamic turbulence is analyzed under the assumption of statistical homogeneity and in the asymptotic limit of large kinetic and magnetic Reynolds numbers. Following Kolmogorov we derive an exact relation for some two-point correlation functions which generalizes the expression recently found for hydrodynamics. We show that the magnetic field brings new source and flux terms into the dynamics which may act on the inertial range similarly as a source or a sink for the mean energy transfer rate. The introduction of a uniform magnetic field simplifies significantly the exact relation for which a simple phenomenology may be given. A prediction for axisymmetric energy spectra is eventually proposed.

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  1. Polarization geometry of magnetohydrodynamic turbulence

    astro-ph.SR 2026-07 conditional novelty 6.0 of 10

    MHD turbulence can be described by a polarization vector on a generalized Poincaré sphere whose rotation and diffusion map onto k^-1, k^-3/2, and k^-5/3 spectral regimes.

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