Turbulent magnetic pressure instability in stratified turbulence

被引:0
作者
Kemel, K. [1 ]
Brandenburg, A. [1 ]
Kleeorin, N.
Rogachevskii, I.
机构
[1] AlbaNova Univ Ctr, NORDITA, SE-10691 Stockholm, Sweden
来源
ADVANCES IN PLASMA ASTROPHYSICS | 2011年 / 274期
关键词
turbulence; MHD; sunspots; FLUX;
D O I
10.1017/S1743921311007538
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A reduction of total mean turbulent pressure due to the presence of magnetic fields was previously shown to be a measurable effect in direct numerical simulations. However, in the studied parameter regime the formation of large-scale structures, as anticipated from earlier mean-field simulations, was not found. An analysis of the relevant mean-field parameter dependency and the parameter domain of interest is conducted in order to clarify this apparent discrepancy.
引用
收藏
页码:473 / 475
页数:3
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