magnetopause

Wave transformation induced by shear flow in the magnetopause boundary layer

磁层顶边界层剪切流引起的MHD波模转化

Vortex-induced reconnection and single X line reconnection at the earth 's magnetopause

磁层顶的涡旋诱发重联和单X线重联

The influence of the magnetopause on magnetic field within the magnetosphere

磁层顶对磁层磁场的影响

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

The magnetopause exerts a tremendous influence on magnetic field within the magnetosphere .

太阳风与地磁场相互作用形成的磁层顶对磁层内磁场有重要影响。

They may play an important role in the interaction of the magnetosheath plasma with the magnetopause .

它们在磁鞘等离子体和磁层顶的相互作用过程中可能起很重要的作用。

The analysis shows that this method may be used to identify several types of the discontinuities which may occur at the magnetopause .

分析表明，这种方法可以用来识别磁层顶上可能出现的若干种间断。

Maximum of the magnetopause current intensity was used to identify the magnetopause at these locations in this paper .

本文采用磁层顶电流密度极大值来判断磁层顶的位置。

These results provide some basis for further study of three-dimensional magnetopause structure and the forecasting of magnetopause shape for space weather .

这些结果可以为我们进一步开展三维磁层顶结构研究和磁层顶位形的空间天气预报提供一定的基础。

A study of orientation and motion of flux transfer events observed at the high-latitude dayside magnetopause

高纬向阳侧磁层顶通量传输事件的特性研究&通量管轴线方位及运动分析

Chapman-Ferraro model is solved for a three dimentional magnetopause .

本文解出了三维磁层顶的Chapman-Ferraro模型。

The spacecraft observations of the position of magnetopause

磁层顶位置的卫星观测

Influence of interplanetary magnetic field b_y on the field-aligned current in the magnetopause

行星际磁场By分量对地球磁层顶场向电流调制

Magnetic field chiefly affect the shape of the magnetopause , dynamic pressure chiefly affect the size of the magnetopause .

磁场主要影响磁层顶形状，动压主要影响磁层顶尺度。

A Simplified Model of the Magnetopause and the Lower-hybrid-drift Instability

磁层顶的简化模型和低杂漂移不稳定性

A further study of multiple flux rope events at the magnetopause observed by TC-1 on 18 March 2004

2004年3月18日高纬磁层顶多重通量管事件分析

There are few models for the high-latitude magnetopause because of the limit of the satellite observations data .

受卫星观测数据的限制，高纬磁层顶位形模型比较少。

Multiple flux rope events at the high-latitude magnetopause : cluster / rapid observations on January 26 , 2001

2001年1月26日高纬磁层顶通量管事件的观测研究

The dayside magnetopause boundary layer is the key region for the solar wind-magnetosphere coupling and interaction .

日侧磁层顶边界层是太阳风-磁层耦合和相互作用的重要区域。

Observations of the average values of the size , shape and orientation of the dayside magnetopause agree quite well with the theoretical prediction .

该椭球面的平均大小、形状和方位的观测值与理论预计值是非常一致的。

These discontinuities , carried by the solar wind , will go across the bow shock and then interact with the magnetopause .

这些间断面会在太阳风的驱动下穿越弓激波并与地球磁层顶发生相互作用。

The location and intensity of the CF-current on the magnetopause are almost same as the results from the model of the ideal discontinuous surface .

实际磁层顶电流片的位置和强度与我们假设的理想磁层顶间断面计算结果基本吻合。

Under the quiet solar wind condition , the dayside magnetopause is at about 10R_E from the center of the Earth .

向日面磁层顶在平静太阳风条件下，处于10RE（RE为地球半径）左右。

Stabilities of Rotational Discontinuity for Magnetopause

磁层顶旋转间断的稳定性

In this paper , by using a three-layer model and the observations from Satellite ISEE , the stabilities of rotational discontinuity for magnetopause are discussed .

本文应用三层模式和ISEE卫星观测资料，讨论了磁层顶旋转间断的稳定性。

By using a two-dimensional compressible MHD model , the local reconnection processes at the dayside magnetopause region are simulated based on the theory of vortex-induced reconnection .

本文用二维可压缩MHD模型，模拟研究了向阳面磁顶区的涡旋诱发重联过程。

When solar wind conditions are changing , the shape of the magnetopause in the meridian plane changes larger than the shape of the magnetopause in the equatorial plane .

太阳风条件变化，子午面磁层顶形状的变化大于赤道面磁层顶形状的变化。

The case analysis gives observational evidence and more details how the reconnection process at dayside low latitude magnetopause causes solar wind transport or entry into magnetosphere . 3 .

对这个事件的分析为向阳面磁层顶低纬区域的磁场重联如何引起太阳风进入磁层提供了更多的观测证据和物理细节。

All flux ropes moved along the surface of the magnetopause in a similar direction indicating that these flux ropes were coming from the dawnside low latitude .

所有通量管都沿磁层顶表面运动，速度方向大体相同，都来自晨侧下方。

A transition layer is observed existing inside the magnetopause at the latitude of about 40o and magnetic local time ( MLT ) of 13:20 during the southward IMF .

在这个事件中，卫星在纬度40o、磁地方时13：20的位置观测到一个位于磁层顶内侧的过渡层。