magnetic reconnection

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。

The theories of magnetic reconnection have been developed for many years .

自从磁重联理论提出以来，已经得到很多学者的不断完善。

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

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。

Magnetic reconnection process play an important role in solar flares .

磁重联在太阳耀斑过程中扮演着重要角色。

A numerical simulation study on the mechanism of electron acceleration in magnetic reconnection

磁场重联中的电子加速机制的数值模拟研究

Physical analysis and numerical simulation on the mechanism of electron acceleration in magnetic reconnection

磁场重联中电子加速问题的物理分析和数值研究

The characteristics and type of the unsteady state magnetic reconnection

非稳态多重X线重联的类型与特征

Numerical study on the magnetic reconnection coupled with heat conduction

耦合热传导的磁重联的数值模拟

Effects of pressure anisotropy of space plasma on magnetic reconnection

空间等离子体压力各向异性对磁场重联的影响

Three dimensional nonlinear coupling of tearing modes and fast magnetic reconnection

三维非线性撕裂模耦合和快速磁场重联

Transient magnetic reconnection processes at the high latitude boundary layer

磁层顶高纬边界层的瞬时重联过程

A numerical study of magnetic reconnection driven by an emerging of magnetic flux

磁通量浮现驱动磁场重联的数值研究

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

Two-dimensional particle simulation study of magnetic reconnection

磁场重联的二维粒子模拟研究

Magnetic Reconnection of Triple Force - Free Current Sheets in the Corona

日冕三重无力场电流片的磁场重联

Observation and Statistic Analysis of the Whistler Waves Associated with Magnetic Reconnection

伴随磁场重联哨声波的观测与统计分析

The results may be applied to understand the dynamic process of magnetic reconnection in laboratory and space plasma .

这些结果可应用于理解实验室等离子体和空间等离子体中的磁场重联的动力学过程。

Direct Evidence of Magnetic Reconnection in Photospheric Layer on the Sun

太阳光球层磁重联的直接证据

No magnetic reconnection at the magnetopause : A new 3-D MHD simulation model

不考虑磁层顶磁重联的全球三维MHD模型

Numerical simulation of the magnetic reconnection in solar flares

太阳耀斑磁重联的数值模拟

The magnetic reconnection is arguably the most important plasma transport and energy conversion process in space physical plasma .

在空间物理中，磁场重联是最重要的等离子体和能量转换的过程。

Therefore , in this thesis , we apply MHD models numerically for magnetic reconnection studies .

本论文从磁流体动力学（MHD）模型出发，采用数值模拟的方法对磁场重联问题展开讨论。

MHD Numerical Simulations of Magnetic Reconnection in Solar Atmosphere

太阳大气中磁重联的MHD数值模拟

Collisionless Magnetic Reconnection in Presence of a Guide Field

存在初始引导场情况下的无碰撞磁场重联

Magnetic reconnection plays a crucial role in almost all rapid macroscale plasma precess .

几乎在所有的快速，宏观的等离子体物理过程中，磁场重联都扮演着关键性的角色。

D magnetic reconnection in solar flares is numerically simulated .

数值模拟了太阳耀斑中二维磁重联过程。

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。

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

The Modified SHASTA Code by Refined Self-adaptive Mesh and the Numerical Experiment of the Magnetic Reconnection

经自适应网格改造后的SHASTA程序和磁重联数值实验