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Analytic characterization of sub-Alfv\'enic turbulence energetics

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arxiv 2209.14143 v5 pith:3DDPBJS2 submitted 2022-09-28 physics.flu-dyn astro-ph.IMphysics.plasm-phphysics.space-ph

classification physics.flu-dynastro-ph.IMphysics.plasm-phphysics.space-ph
keywords energyturbulencemagneticenergeticskineticcompressibleenicfluctuating
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Magnetohydrodynamic (MHD) turbulence is a cross-field process relevant to many systems. A prerequisite for understanding these systems is to constrain the role of MHD turbulence, and in particular the energy exchange between kinetic and magnetic forms. The energetics of strongly magnetized and compressible turbulence has so far resisted attempts to understand them. Numerical simulations reveal that kinetic energy can be orders of magnitude larger than fluctuating magnetic energy. We solve this lack-of-balance puzzle by calculating the energetics of compressible and sub-Alfv\'enic turbulence based on the dynamics of coherent cylindrical fluid parcels. Using the MHD Lagrangian, we prove analytically that the bulk of the magnetic energy transferred to kinetic is the energy stored in the coupling between the ordered and fluctuating magnetic field. The analytical relations are in striking agreement with numerical data, up to second order terms.

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  1. Revealing hidden correlations from complex spatial distributions: Adjacent Correlation Analysis

    physics.comp-ph 2025-06 conditional novelty 6.0 of 10

    A new method, adjacent correlation analysis, extracts local correlations between two measured quantities from spatial gradients and visualizes them as vector fields in phase space.

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