磁层亚暴

磁层亚暴膨胀相的近地触发模型

A near-Earth triggering model for the magnetospheric substorm expansion phase

本文根据两个理想的磁流体力学模型研究了磁层亚暴恢复期间等离子体片边界层区的Kelvin-Helmholtz不稳定性。

The Kelvin-Helmholtz instability in boundary layer regions of the plasma sheet during magnetospheric substorm recovery is studied based on two idealized MHD models .

所以本文认为极光X射线总强度可以作为新的磁层亚暴卫星实时监测指数。

We suggest that the auroral X-ray intensity ( AI ) be a candidate of a new real-time index obtained from satellite observations for monitoring magnetosphere sub-storms .

太阳风湍流和磁层亚暴的一种机制

Mechanism of magnetospheric substorm and the turbulence of solar wind

磁层亚暴时环电流的局部加速机制

The mechanism of acceleration of ring current during a substorm of magnetosphere

磁层亚暴的磁重联-电流中断-电离层、磁层耦合全球模型

The global magnetic reconnection-current disruption-ionosphere-magnetosphere coupling model for substorms

磁层亚暴期间高纬地区三维电流体系

Three-dimensional current system at high-latitude during substorm

所谓卫星表面充电环境是指使卫星表面充电的环境，它主要指磁层亚暴时的等离子体环境。

Said the satellite surface charging environment means the environment of the satellite surface charged . It mainly means the plasma environment when the magnetic substorm occurred .

研究磁层亚暴、磁暴和磁层粒子暴的触发机制及磁层空间暴对太阳活动和行星际扰动的响应过程；

The second is to investigate the trigger mechanisms of magnetic storm , magnetospheric substorm , and magnetospheric particle storm , as well as the responses of magnetospheric space storm to the solar activities and interplanetary disturbance .

磁场重联可以在短时间年内将磁能转化为等离子体的动能和热能，并改变磁场的拓扑结构，被认为与许多爆发性现象有关，比如太阳耀斑和磁层亚暴等。

Magnetic reconnection can transfer magnetic energy into plasma thermal and kinetic energy in short time period , and changes the topology of magnetic field , thus it is suggested as related many explosive phenomena , such as solar flare , magnetosphere substorm .

磁层动力学最为重要的研究任务就是对磁层亚暴的理解。

The effect of such high flux upflowing ions on the composition and the dynamic process of the magnetosphere is still unclear .