【正文快照】： 磁场重联(magnetic reconnection)是指相互靠近的磁力线的反平行分量发生断裂和重新联结现象,伴有磁场能量的突然释放并转化为等离子体的动能和热能,是空间和天体等...
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驱动磁场重联 Driven magnetic reconnection
Magnetic reconnection is both regional phenomenon of astrophysics and very importantstudy subject in plasma physics of the solar system, also is general-existing basic physicalphenomenon in both space plasma and laboratory plasma.
磁场重联是天体等离子体物理中的一种局域现象，是太阳系等离子体物理学中的重要研究课题，也是空间等离子体和实验室等离子体中的普遍存在的基本物理现象。
参考来源 - 撕裂模不稳定性与边界扰动驱动磁场重联·2,447,543篇论文数据，部分数据来源于NoteExpress
磁场重联常常会被撕裂模不稳定性触发。
Magnetic reconnection is often triggered by the tearing mode instability.
采用二维全粒子模拟方法研究了无碰撞磁场重联。
The collisionless magnetic reconnection is studied using two dimensional full particle simulation.
应用二维三分量混合模拟方法数值研究了各向异性等离子体中的磁场重联过程。
The process of magnetic reconnection in an anisotropic plasma is studied based on two and half dimensional hybrid simulation.
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