Influence of tearing instability on magnetohydrodynamic turbulence

被引:25
作者
Walker, Justin [1 ]
Boldyrev, Stanislav [1 ,2 ]
Loureiro, Nuno F. [3 ]
机构
[1] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA
[2] Space Sci Inst, Boulder, CO 80301 USA
[3] MIT, Plasma Sci & Fus Ctr, 77 Massachusetts Ave, Cambridge, MA 02139 USA
关键词
MAGNETIC RECONNECTION; ALFVENIC TURBULENCE; SHEET PINCH; SOLAR-WIND; SHEAR; FIELD; SIMULATIONS; ANISOTROPY; SPECTRUM; PLASMA;
D O I
10.1103/PhysRevE.98.033209
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
It was proposed recently by Loureiro and Boldyrev [Phys. Rev. Lett. 118, 245101 (2017)] and Mallet et al. [Mon. Not. R. Aston. Soc. 468, 4/162 (2017)] that strongly anisotropic current sheets formed in the inertial range of magnetohydrodynamic turbulence become affected by the tearing instability at scales smaller than a critical scale lambda(c), and larger than the dissipation scale of turbulence. If true, this process can modify the nature of energy cascade at smaller scales, leading to a new, tearing-mediated regime of magnetohydrodynamic (MHD) turbulence. In this work, we present a numerical study of strongly anisotropic, two-dimensional turbulent eddies, and we demonstrate that the tearing instability can indeed compete with their nonlinear evolution. The results, therefore, provide direct numerical support for the picture that a new regime of MHD turbulence can exist below lambda(c).
引用
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页数:6
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