Turbulent magnetic Prandtl number and magnetic diffusivity quenching from simulations

被引:95
作者
Yousef, TA
Brandenburg, A
Rüdiger, G
机构
[1] Norwegian Univ Sci & Technol, Dept Energy & Proc Engn, N-7491 Trondheim, Norway
[2] NORDITA, DK-2100 Copenhagen O, Denmark
[3] Astrophys Inst Potsdam, D-14482 Potsdam, Germany
关键词
magnetohydrodynamics (MHD); turbulence;
D O I
10.1051/0004-6361:20031371
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Forced turbulence simulations are used to determine the turbulent kinematic viscosity, v(t), from the decay rate of a large scale velocity field. Likewise, the turbulent magnetic diffusivity, eta(t), is determined from the decay of a large scale magnetic field. In the kinematic regime, when the field is weak, the turbulent magnetic Prandtl number, v(t)/eta(t), is about unity. When the field is nonhelical, eta(t) is quenched when magnetic and kinetic energies become comparable. For helical fields the quenching is stronger and can be described by a dynamical quenching formula.
引用
收藏
页码:321 / 327
页数:7
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