Weakly imbalanced strong turbulence

Details Weakly imbalanced strong turbulence Weakly imbalanced strong turbulence

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..274...72b&link_type=abstract

Advances in Plasma Astrophysics, Proceedings of the International Astronomical Union, IAU Symposium, Volume 274, p. 72-75

Astronomy and Astrophysics

Astrophysics

Mhd, Turbulence, Ism: Kinematics And Dynamics

Scientific paper

The theory of strong MHD turbulence with cross-helicity 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 this limit both w+=v+b and w-=v-b are cascaded strongly. The model for imbalance based on so-called ``dynamic alignment'' strongly contradicts numerical evidence.

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