Three-dimensional MHD simulation study of the structure at the leading part of a reconnection jet

被引:15
|
作者
TanDokoro, R [1 ]
Fujimoto, M [1 ]
机构
[1] Tokyo Inst Technol, Dept Earth & Planetary Sci, Meguro Ku, Tokyo 1528551, Japan
关键词
D O I
10.1029/2005GL024467
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We have performed three-dimensional MHD simulations of magnetic reconnection to investigate the structure of a reconnection jet. Our simulation results show that the leading edge of a reconnection jet deforms to put on a significantly complicated structure. In a randomly perturbed environment, smaller scale structure develops rapidly and finally the front of the reconnection jet becomes turbulent. In contrast when the initial perturbation is composed of a single sinusoidal mode, coherent magnetic bubbles are generated. The magnetic bubbles elongate significantly when the wavelength is small giving onset to a secondary instability that may subsequently lead to turbulence. We interpret the deformation of the jet front to be due to excitation of the Rayleigh-Taylor/ballooning-like instability and emphasize the significance of the three-dimensionality in considering the dynamics of a reconnection jet.
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页码:1 / 4
页数:4
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