Strong Imbalanced Turbulence

Details Strong Imbalanced Turbulence Strong Imbalanced Turbulence

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..444....3b&link_type=abstract

5th international conference of numerical modeling of space plasma flows (astronum 2010). Proceedings of a 5th international con

Astronomy and Astrophysics

Astronomy

Scientific paper

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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