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Strong Imbalanced Turbulence
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We consider stationary, forced, imbalanced, or cross-helical MHD Alfvenic turbulence where the waves traveling in one direction have higher amplitudes than the opposite waves. This paper is dedicated to so-called strong turbulence, which cannot be treated perturbatively. Our main result is that the anisotropy of the weak waves is stronger than the anisotropy of a strong waves. We propose that critical balance, which was originally conceived as a causality argument, has to be amended by what we call a propagation argument. This revised formulation of critical balance is able to handle the imbalanced case and reduces to old formulation in the balanced case. We also provide phenomenological model of energy cascading and discuss possibility of self-similar solutions in a realistic setup of driven turbulence.
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Cited by 1 Pith paper
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Intermittent, Reflection-Driven, Strong Imbalanced MHD Turbulence
A new phenomenological model predicts structure-function, spectrum, and parallel-length scalings for intermittent, reflection-driven imbalanced MHD turbulence, matching Parker Solar Probe data.
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