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非稳态多重X线重联的类型与特征
引用本文:金曙平 宋锦文. 非稳态多重X线重联的类型与特征[J]. 地球物理学报, 1996, 39(6): 739-746
作者姓名:金曙平 宋锦文
作者单位:1. 中国科学技术大学,合肥 230026;2. 第三世界科学院地球科学与天文学高级研究中心,合肥 230026
摘    要:为了进一步认识间歇性多重X线重联的特征,本文分析计算结果,发现入流自边界进入后向两侧发散,沿着x轴(z=0)和出流边界(z=2),压强P和磁场B的分布形态表明这种非稳态重联属快模式扩张型.数值结果还表明,进入扩散区的入流马赫数M与磁雷诺数Rm之间基本满足关系式M≈1.5R-1/2─1.75R-1/2,而且等离子体的加速与压强P(P

关 键 词:非稳态多重x线重联  快模式扩张  重联率  切向速度  
收稿时间:1995-07-16

THE CHARACTERISTICS AND TYPE OF THE UNSTEADY STATE MAGNETIC RECONNECTION
JIN SHU-PING, SONG JIN-WEN. THE CHARACTERISTICS AND TYPE OF THE UNSTEADY STATE MAGNETIC RECONNECTION[J]. Chinese Journal of Geophysics, 1996, 39(6): 739-746
Authors:JIN SHU-PING   SONG JIN-WEN
Affiliation:1. Departmenr of Earth and Space Science, University of Science and Technology of China, Hefei 230026, China;2. Advanced Ccntre for Eorsh Science and Astronomy, University of Science and Technology of China, Third World Academy of Science, Hefei 230026, China
Abstract:The intermittent multiple X-line reconnection is numerically analyzed in this paper. A fast-mode expansion is expected in the light of the divergent plasma flow and the features of the profiles for magnetic field strength B and pressure P along the lines z=0 and z=2. It can be seen from numerical results that the inflow Mach Number Mi reached at the diffusion region scales with magnetic Reynolds number Rm as Rm-1/2 and the plasma is accelerated by the pressure gradient force. These characteristics are close to the features of Sweet-Parker reconnection with a long current sheet. The tangential velocity component Vz at the inflow boundary (x=1).is defined as V 0. The comparison of numerical results shows that a low uniform resistivity (corresponding to high Magnetic Reynolds nuinber) play a key role in the formation of the unsteady multiple X-line reconnection, but the different setting of tangential velocity Vz at x =1 is not so important.
Keywords:Unsteady state magnetic reconnection   Fast-mode expansion   Reconnection rate   Tangential velocity.
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