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Paper: Strong Imbalanced Turbulence
Volume: 444, 5th International Conference of Numerical Modeling of Space Plasma Flows (ASTRONUM 2010)
Page: 3
Authors: Beresnyak, A.
Abstract: The theory of strong MHD turbulence with cross-helicity (or energy imbalance) has been a subject of many recent studies. In this paper we focused our attention on low-imbalance limit and performed high-resolution 3D simulations. The results suggest that in the limit of small imbalances both w+= v + b and w = v – b components are cascaded strongly, as expected, while the model for imbalance based on so-called “dynamic alignment” strongly contradicts numerical evidence.
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