Weakly imbalanced strong turbulence
Abstract
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.
- Publication:
-
Advances in Plasma Astrophysics
- Pub Date:
- June 2011
- DOI:
- Bibcode:
- 2011IAUS..274...72B
- Keywords:
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- MHD;
- turbulence;
- ISM: kinematics and dynamics