English

Scaling laws and diffuse locality of balanced and imbalanced MHD turbulence

Astrophysics of Galaxies 2015-05-18 v2 Solar and Stellar Astrophysics Fluid Dynamics

Abstract

The search of ways to generalize the theory of strong MHD turbulence for the case of non-zero cross-helicity (or energy imbalance) has attracted considerable interest recently. In our earlier publications we performed three-dimensional numerical simulations and showed that some of existing models are inconsistent with numerics. In this paper we focused our attention on low-imbalance limit and performed new high-resolution simulations. The results strongly suggest that in the limit of small imbalances we smoothly transition to a standard Goldreich-Sridhar (1995) balanced model. We also claim that Perez-Boldyrev (2009) model that predicts the same nonlinear timescale for both components due to so-called "dynamic alignment" strongly contradicts numerical evidence.

Keywords

Cite

@article{arxiv.1002.2428,
  title  = {Scaling laws and diffuse locality of balanced and imbalanced MHD turbulence},
  author = {A. Beresnyak and A. Lazarian},
  journal= {arXiv preprint arXiv:1002.2428},
  year   = {2015}
}

Comments

4 pages, 4 figures