No CrossRef data available.
Article contents
Weakly imbalanced strong turbulence
Published online by Cambridge University Press: 08 June 2011
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 6 , Symposium S274: Advances in Plasma Astrophysics , September 2010 , pp. 72 - 75
- Copyright
- Copyright © International Astronomical Union 2011
References
Boldyrev, S. 2005, ApJ, 626, L37; Boldyrev, S. 2006, Phys. Rev. Lett., 96, 115002CrossRefGoogle Scholar