magnetic reconnection

Numerical study on the magnetic reconnection coupled with heat conduction

耦合热传导的磁重联的数值模拟

Magnetic reconnection plays a very important role in solar flares, corona mass ejections ( CME), and other solar activities.

在太阳耀斑、日冕物质抛射（CME）和其他太阳活动现象中，磁重联一直都扮演着至关重要的作用。

For the certain discontinuities with specific initial configuration, the magnetosheath magnetic reconnection, as an important consequence of such evolution, has been confirmed by simulation and observation.

对于某些具有特定结构的间断面，磁鞘磁场重联是这一演化过程的必然结果，并且已经被计算机数值模拟和空间卫星观测所证实。

Magnetic reconnection, as a fundamental process, has been used to explain many natural phenomena of the sudden release of energy in space physics and magnetic confinement fusion.

磁场重联作为一个基本过程，被用来解释自然界中的能量的突然释放现象，例如在空间物理和磁约束聚变中。

Direct Evidence of Magnetic Reconnection in Photospheric Layer on the Sun

太阳光球层磁重联的直接证据

Tearing mode instability research have great significance for understanding the activities of magnetic reconnection in solar flares.

撕裂模不稳定性的研究对理解耀斑等爆发活动中的重联有重要意义。

MHD Numerical Simulations of Magnetic Reconnection in Solar Atmosphere

太阳大气中磁重联的MHD数值模拟

Magnetic reconnection, strong electric currents in sheared low lying magnetic loops and coronal cavity in solar multipolar magnetic fields

太阳多极活动区中的磁重联、剪切低磁弧内的强电流和冕穴结构

Magnetic reconnection in the earth's distant magnetotail ( I) streaming tearing instability

地球远磁尾中的磁场重联（Ⅰ）流动撕裂模不稳定性

The instability of the tearing mode exists widespread in the space and laboratory plasmas while the magnetic reconnection plays an important role on the tearing mode evolution.

在实验室和空间等离子体中，撕裂模的不稳定性是普遍存在的，而磁场重联在撕裂模的演化中扮演了十分重要的角色。

A simulation study of magnetic reconnection in a multiple current sheet system

K-H不稳定性在多电流片系统磁场重联中的效应

Tearing mode instability is the unsteady magnetic reconnection, which is one of the most dangerous instabilities in tokamak discharge and can cause disruption.

撕裂模不稳定性是非稳念的磁场重联，它是托卡马克装置中最危险的不稳定性之一，会引起等离子体约束的大破裂。

Magnetic reconnection is one important subject of space physics and laboratory plasma physics. It is a very difficult issue and hot topic also.

磁场重联是空间物理和实验室等离子体物理中重要的研究课题，也是研究热点和难点。

The tearing mode instability and magnetic reconnection process in an anisotropic plasma ( P ⊥≠ P ∥, T ⊥≠ T ∥) are numerically studied by a two dimensional three component time dependant compressible MHD simulation.

应用二维三分量时变可压缩磁流体动力学模拟方法，数值研究了各向异性等离子体（P⊥≠P‖，T⊥≠T‖）中的撕裂模不稳定性和磁场重联过程。

In the case with S →∞(η→ 0), the streaming tearing mode retrogrades to the streaming sausage mode in which no magnetic reconnection occurs.

在S→∞的情况下，流动撕裂模将退化为流动颈缩模，磁场重联不再发生。

Using this method, we design a2D 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。

Numerical simulation of spontaneous magnetic reconnection in solar atmosphere(ⅱ) 2.5d results with gravity and heat conduction

太阳大气中自发磁重联的数值模拟（Ⅱ）重力、热传导下二维三分量的计算结果

Numerical studies of tearing mode instability and magnetic reconnection in anisotropic plasma

各向异性等离子体中撕裂模不稳定性和磁场重联的数值研究

Observation by spacecrafts is one important method to study magnetic reconnection.

卫星观测是研究磁场重联的重要手段之一。