Basic properties of magnetohydrodynamic turbulence in the inertial range

被引:40
作者
Beresnyak, Andrey [1 ,2 ]
机构
[1] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[2] Ruhr Univ Bochum, D-44780 Bochum, Germany
关键词
MHD; turbulence; STRONG IMBALANCED TURBULENCE; NUMERICAL SIMULATIONS; SCALING LAWS; ALFVENIC TURBULENCE; ANISOTROPY; SPECTRUM; FIELD;
D O I
10.1111/j.1365-2966.2012.20859.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We revisit the issue of the spectral slope of magnetohydrodynamic (MHD) turbulence in the inertial range and argue that the numerics favour a GoldreichSridhar -5/3 slope rather than a -3/2 slope. We also perform precision measurements of the anisotropy of MHD turbulence and determine the anisotropy constant CA= 0.34 of Alfvenic turbulence. Together with the previously measured Kolmogorov constant CK= 4.2, or 3.3 for a purely Alfvenic case, it constitutes a full description of the MHD cascade in terms of spectral quantities, which is of high practical value for astrophysics.
引用
收藏
页码:3495 / 3502
页数:8
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