Nonlocal Phenomenology for anisotropic MHD turbulence

TL;DR

This paper proposes a non-local cascade model for anisotropic MHD turbulence, accounting for scale interactions and resonance conditions, leading to a specific anisotropic energy spectrum and discussing its relation to existing theories and simulations.

Contribution

It introduces a novel non-local cascade model for anisotropic MHD turbulence that incorporates resonance conditions and scale interactions, providing new insights into the energy spectrum.

Findings

Energy spectrum follows $E(k_\|,k_ot) \\sim \\epsilon^{2/3}k_\|^{-1}k_ot^{-5/3}$.

Energy cascades along lines $k_\| \\sim C + k_ot^{2/3} \\epsilon^{1/3}/B_0$.

Model suggests non-universal behavior with different forcing conditions.

Abstract

A non-local cascade model for anisotropic MHD turbulence in the presence of a guiding magnetic field is proposed. The model takes into account that (a) energy cascades in an anisotropic manner and as a result a different estimate for the cascade rate in the direction parallel and perpendicular to the guiding field is made. (b) the interactions that result in the cascade are between different scales. Eddies with wave numbers $k_\|$ and $k_\perp$ interact with eddies with wave numbers $q_\|,q_\perp$ such that a resonance condition between the wave numbers $q_\|,q_\perp$ and $k_\|,k_\perp$ holds. As a consequence energy from the eddy with wave numbers $k_\|$ and $k_\perp$ cascades due to interactions with eddies located in the resonant manifold whose wavenumbers are determined by: $q_\|\simeq \epsilon^{{1}/{3}}k_\perp^{2/3}/B$, $q_\perp=k_\perp$ and energy will cascade along the lines $k_\|\sim C+k_\perp^{2/3} \epsilon^{1/3}/B_0$. For a uniform energy injection rate in the parallel direction the resulting energy spectrum is $E(k_\|,k_\perp)\simeq \epsilon^{2/3}k_\|^{-1}k_\perp^{-5/3}$. For a general forcing however the model suggests a non-universal behavior. The connections with previous models, numerical simulations and weak turbulence theory are discussed.