Weakly imbalanced strong turbulence

Andrey Beresnyak
2010 Proceedings of the International Astronomical Union  
AbstractThe 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.
doi:10.1017/s1743921311006594 fatcat:xnhv5pgp6jcqhf65n4jtnms6ji