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1·All observed results support the previous magnetic reconnection model.

这些观测结果支持日浪的磁重联模型。

2·Magnetic reconnection is often triggered by the tearing mode instability.

磁场重联常常会被撕裂模不稳定性触发。

3·The collisionless magnetic reconnection is studied using two dimensional full particle simulation.

采用二维全粒子模拟方法研究了无碰撞磁场重联。

4·The process of magnetic reconnection in an anisotropic plasma is studied based on two and half dimensional hybrid 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。

5·Magnetic reconnection as an important mechanism to trigger the solar flares is closely related to these electromagnetic radiation phenomena in the course of flares.

磁场重联作为一种重要的耀斑触发机制，和耀斑过程中的这些电磁辐射现象有着密切关系。

6·Using this method, we design a 2D particle simulation code, and numerically study two common physical phenomena in space physics:beam instability and magnetic reconnection.

设计了一个二维三分量的粒子模拟程序，并用它计算了空间物理中两种常见的物理现象：束流不稳定性和磁场重联。

7·The process of magnetic reconnection in the collisionless plasma and distributions of particles in different positions are studied based on two-dimensional particle simulation.

利用二维全粒子模拟方法研究了无碰撞等离子体中的磁场重联过程，得到了不同区域的离子和电子速度分布。

8·Following what exactly happens during a reconnection event requires, first off, a general understanding of how invisible magnetic loops can trap hot gas in the solar atmosphere.

想了解磁力线重连事件中究竟发生了些什么事情，必须先对看不见的磁力环圈如何捕捉太阳大气里的热气有一些基本认识。

9·Reconnection is most efficient when the IMF has a component that is directed southward-that is, opposite to the northward direction of the earth's magnetic field at the dayside of the magnetosphere.

在磁层昼侧，若imf有南向分量，也就是和北向的地球磁场方向相反，则磁力线重连的效率最高。

10·With this new model, spontaneous fast reconnection in a neutral current sheet, which provides an effective mechanism for rapid magnetic energy release, is carefully studied.

基于此模式，我们详细研究了中性电流片中的自发快速重联过程，它提供了一种有效的磁能快速释放机制。