reconnection

In this article, we employ EMHD model to investigate reconnection instability, especially tearing mode instability.

本文，正是采用这个模型，对磁场重联不稳定性，特别是撕裂模不稳定性进行了研究。

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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。

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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麽事情，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。

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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。

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MHD Numerical Simulations of Magnetic Reconnection in Solar Atmosphere

太阳大气中磁重联的MHD数值模拟

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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。

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This wizard helps you troubleshoot any conflicts and prepare the mailbox for reconnection.

此向导将帮助您解决任何冲突问题并准备好邮箱,以便进行重新连接.

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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

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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。

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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。

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Numerical study on the magnetic reconnection coupled with heat conduction

耦合热传导的磁重联的数值模拟

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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。

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This is designed to enable the reconnection of a client on a previous connection that has not yet fully cleaned up.

这种设计实际上实现了当之前的连接未完全消除时重新连接客户机。

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Cluster survey of cusp reconnection and its IMF dependence.

尖点重联的聚类调查及其IMF信赖.

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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。

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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。

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Numerical simulation for magnetic spontaneous reconnection in solar atmosphere(ⅰ)

太阳大气中自发重联的数值模拟（Ⅰ）

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The stage power excitation of stage reconnection gun must be synchronized with the position of projectile.

多级重接炮各级电源的激励需与发射体位置同步.

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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。

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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

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Direct Evidence of Magnetic Reconnection in Photospheric Layer on the Sun

太阳光球层磁重联的直接证据

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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

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The automatic reconnection is virtually seamless.

自动重新连接实际上是无缝的。

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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。

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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

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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

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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。

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