Properties of magnetic reconnection in MHD turbulence

被引：1
|
作者：
Servidio, S. [1 ,2 ]
Shay, M. A. [1 ,2 ]
Matthaeus, W. H. [1 ,2 ]
Dmitruk, P. [3 ]
Cassak, P. A. [4 ]
Wan, M. [1 ,2 ]
机构：
[1] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA
[2] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA
[3] Univ Buenos Aires, Fac Ciencias Exactas & Nat, Dept Fis, RA-1428 Buenos Aires, DF, Argentina
[4] West Virginia Univ, Dept Phys, Morgantown, WV 26506 USA
来源：
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE | 2010年 / 1216卷
关键词：
Magnetic reconnection; Magnetohydrodynamic; plasma turbulence; FIELDS;
D O I：
10.1063/1.3395835
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Numerical simulations of two-dimensional Magnetohydrodynamic (2D MHD) turbulence reveal the presence of a huge number of sites where magnetic reconnection locally occurs. The properties of this ensemble of reconnection events, that are spontaneously generated by turbulence, have been studied. The associated reconnection rates, computed as the electric field at the neutral points, are broadly distributed and the statistics of these events are presented. This new description of reconnection is relevant for space and laboratory plasmas, where generally turbulence is present.
引用
收藏
页码：198 / +
页数：2
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