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1)  Magnetic reconnection
磁场重联
1.
We observed whistler waves,electrostatic solitary waves(ESW),high frequency electrostatic modulated waves associated with magnetic reconnection with the data of Geotail.
利用GEOTAIL卫星探测得到的磁场、粒子和波的数据,通过观测伴随着磁场重联的哨声波、静电孤立波、高频静电调制波等波,统计分析了地球磁尾伴随重联过程的哨声波的频率、空间位置分布等特性。
2.
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
3.
Magnetic reconnection caused by the resistance tearing instability in a current sheet of solar corona with two-dimensional magnetostatic equilibrium in the spherical coordinate has been studied numerically.
本文在球坐标二维磁静力平衡基态下,数值研究了电阻撕裂模不稳定性引起日冕电流片中发生磁场重联的过程。
2)  Magnetic field reconnection
磁场重联
1.
The onset and nonlinear saturation of Weibel instability, the emergence of beams and magnetic field reconnection were discussed.
讨论了纯粹Weibel不稳定性的发生和非线性饱和过程 ,观察到电流束合并、磁场重联等引起的电子横向加热现象 。
3)  collisionless magnetic reconnection
无碰撞磁场重联
1.
A two-and-a-half dimensional electromagnetic particle-in-cell(PIC) simulation code is used to investigate electron behaviour in collisionless magnetic reconnection.
采用二维三分量的全粒子模拟方法研究了不同离子电子质量比(mi/me)下的无碰撞磁场重联中的电子特征。
2.
Collisionless magnetic reconnections with different initial temperature gradients across the current sheet are studied through two-dimensional Darwin Particle-in-cell simulations.
使用二维粒子模拟(PIC)的方法研究了在电流片两侧具有不同温度或密度情况下的无碰撞磁场重联过程。
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)  Nightside magnetopause
瞬时磁场重联
5)  Driven magnetic reconnection
驱动磁场重联
6)  vortex-induced magnetic reconnection
涡旋诱发磁场重联
补充资料:加特曼重氮盐偶联反应
分子式:
CAS号:

性质:重氮盐ArN2Cl在酸性溶液中用铜粉处理,放出氮气,发生偶联反应。当芳环上有吸电子基团时,偶联生成联苯型化合物Ar-Ar;当芳环上有给电子基团时,偶联生成偶氮化合物ArN=NAr。是合成这两类化合物常用的方法。   2ArN2Cl+2Cu→Ar-Ar(或ArN=NAr)+N2↑+CuCl2

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