Eddy viscosity and laminarization of sheared flow in three dimensional reduced magnetohydrodynamic turbulence

被引:19
作者
Kim, EJ [1 ]
Hahm, TS
Diamond, PH
机构
[1] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA
[2] Princeton Univ, Princeton Plasma Phys Lab, Princeton, NJ 08543 USA
[3] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA
关键词
D O I
10.1063/1.1383284
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The effect of Alfven waves on turbulent momentum transport is studied in three-dimensional reduced magnetohydrodynamic turbulence. A strong external uniform magnetic field B-0 is assumed to be present orthogonal to both background shear flow and its inhomogeneity. Energy is injected into the fluid and/or magnetic field on small scales. It is shown analytically that eddy viscosity is reduced as 1/B-0(2) for a strong B-0, due to the cancellation of the Reynolds stress by Maxwell stress. The sign of eddy viscosity is found to depend on the detailed properties of forcings. Specifically, it is positive for fluid forcing but depends on the anisotropy of the forcing in the case of magnetic forcing. Furthermore, it is indicated that a magnetic field tends to laminarize a mean shear flow. The possible implication of these results for the dynamics of the zonal flows in tokamaks is discussed in view of the cancellation of stresses. (C) 2001 American Institute of Physics.
引用
收藏
页码:3576 / 3582
页数:7
相关论文
共 17 条
[1]   Instability, turbulence, and enhanced transport in accretion disks [J].
Balbus, SA ;
Hawley, JF .
REVIEWS OF MODERN PHYSICS, 1998, 70 (01) :1-53
[2]  
DIAMOND PH, 1998, PLASMA PHYSICS CONTR
[3]   WAVE VORTEX DYNAMICS IN DRIFT AND BETA-PLANE TURBULENCE [J].
DYACHENKO, AI ;
NAZARENKO, SV ;
ZAKHAROV, VE .
PHYSICS LETTERS A, 1992, 165 (04) :330-334
[4]  
GOLDREICH P, 1964, MON NOT R ASTRON SOC, V130, P126
[5]   SELF-CONSISTENT THEORY OF MEAN-FIELD ELECTRODYNAMICS [J].
GRUZINOV, AV ;
DIAMOND, PH .
PHYSICAL REVIEW LETTERS, 1994, 72 (11) :1651-1653
[6]   Shearing rate of time-dependent E x B flow [J].
Hahm, TS ;
Beer, MA ;
Lin, Z ;
Hammett, GW ;
Lee, WW ;
Tang, WM .
PHYSICS OF PLASMAS, 1999, 6 (03) :922-926
[7]   Turbulent transport and equilibrium profiles in two-dimensional magnetohydrodynamics with background shear [J].
Kim, E ;
Dubrulle, B .
PHYSICS OF PLASMAS, 2001, 8 (03) :813-824
[8]  
KIM E, UNPUB PHYSICA D
[9]   INERTIAL-RANGE SPECTRUM OF HYDROMAGNETIC TURBULENCE [J].
KRAICHNAN, RH .
PHYSICS OF FLUIDS, 1965, 8 (07) :1385-+
[10]   Angular momentum transport in magnetized stellar radiative zones. IV. Ferraro's theorem and the solar tachocline [J].
MacGregor, KB ;
Charbonneau, P .
ASTROPHYSICAL JOURNAL, 1999, 519 (02) :911-917