Energetics of Kinetic Reconnection in a Three-Dimensional Null-Point Cluster

被引:29
|
作者
Olshevsky, V. [1 ,2 ]
Lapenta, G. [1 ]
Markidis, S. [3 ]
机构
[1] Katholieke Univ Leuven, Dept Math, Ctr Math Plasma Astrophys CmPA, Celestijnenlaan 200B, B-3001 Louvain, Belgium
[2] Main Astron Observ NAS, Akad Zabolotnoho 27, UA-03680 Kiev, Ukraine
[3] KTH Royal Inst Technol, High Performance Comp & Visualizat HPCViz, SE-10044 Stockholm, Sweden
关键词
KINEMATIC RECONNECTION; SOLAR CORONA; FIELD; ACCELERATION; SIMULATIONS; PLASMA;
D O I
10.1103/PhysRevLett.111.045002
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We perform three-dimensional particle-in-cell simulations of magnetic reconnection with multiple magnetic null points. Magnetic field energy conversion into kinetic energy is about five times higher than in traditional Harris sheet configuration. More than 85% of initial magnetic field energy is transferred to particle energy during 25 reversed ion cyclofrequencies. Magnetic reconnection in the cluster of null points evolves in three phases. During the first phase, ion beams are excited, then give part of their energy back to the magnetic field in the second phase. In the third phase, magnetic reconnection occurs in many small patches around the current channels formed along the stripes of a low magnetic field. Magnetic reconnection in null points essentially presents three-dimensional features, with no two-dimensional symmetries or current sheets.
引用
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页数:4
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