DISSIPATION AND RECONNECTION IN BOUNDARY-DRIVEN REDUCED MAGNETOHYDRODYNAMICS

被引:31
|
作者
Wan, Minping [1 ,2 ]
Rappazzo, Antonio Franco [1 ,2 ,3 ]
Matthaeus, William H. [1 ,2 ]
Servidio, Sergio [4 ]
Oughton, Sean [5 ]
机构
[1] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA
[2] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA
[3] Adv Heliophys, Pasadena, CA 91106 USA
[4] Univ Calabria, Dipartimento Fis, I-87036 Cosenza, Italy
[5] Univ Waikato, Dept Math, Hamilton 3240, New Zealand
来源
ASTROPHYSICAL JOURNAL | 2014年 / 797卷 / 01期
基金
美国国家科学基金会;
关键词
magnetic reconnection; magnetohydrodynamics (MHD); Sun: corona; MAGNETIC RECONNECTION; MHD TURBULENCE; SOLAR-WIND; DYNAMICS; DISCONTINUITIES; RELEASE; FIELDS;
D O I
10.1088/0004-637X/797/1/63
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the statistics of coherent current sheets, the population of X-type critical points, and reconnection rates in a coronal loop geometry, via numerical simulations of reduced magnetohydrodynamic turbulence. Current sheets and sites of reconnection (magnetic X-points) are identified in two-dimensional planes of the three-dimensional simulation domain. The geometry of the identified current sheets-including area, length, and width-and the magnetic dissipation occurring in the current sheets are statistically characterized. We also examine the role of magnetic reconnection, by computing the reconnection rates at the identified X-points and investigating their association with current sheets.
引用
收藏
页数:10
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