magnetopause

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。

For these reasons, magnetopause waves are not considered the primary means by which the solar wind affects the magnetosphere.

基于上述理由，一般并不认为磁层顶上的波动是太阳风影响磁层的主要机制。

When the pressure increases, as occurred during the Bastille Day storm, the dayside magnetopause is pushed closer to the earth, sometimes by as much as 26,000 kilometers.

在地球昼侧，磁层顶通常在距地球中心64000公里附近，但磁层顶的位置会随太阳风的压力而改变，当太阳风压力变大，譬如在巴士底日太空风暴的期间，昼侧的磁层顶就被推向地球，有时可推近26000公里之多。

According to this hypothesis, the solar wind could transfer energy and momentum to the plasma surrounding the earth only by wave motions along the magnetopause.

根据这项假说，太阳风只能靠磁层顶上的波动，来传递能量与动量给地球四周的电浆。

In this process, the field lines of the IMF become temporarily interconnected with the geomagnetic field lines on the dayside of the magnetopause [see illustration on page 89].

在磁力线重连过程中，昼侧的磁层顶的IMF磁力线，暂时与地球磁场的磁力线相连（见本篇pdf111页上图）。

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

Simultaneous Geotail and Wind observations of reconnection at the subsolar and tail flank magnetopause

在日下和尾侧面磁层顶重联同时发生的地尾和风观测

Keywords energetic particle;ULF wave;adiabatic invariants;radiation belt;cusp region;magnetopause;

能量粒子;超低频波;寝渐不变量;辐射带;极尖区;磁层顶;

the inner magnetosphere and the dayside magnetopause, with each cake-size craft recording the basic characteristics of the plasmas and magnetic fields.

第一个大卫星群可能用来监测磁层内层及昼侧的磁层顶，每个蛋糕般大小的小卫星都将记录各别区域内，电浆与磁场的基本数据。

“Important discoveries were made, but scientists didn’t detect any dynamic features, other than some Kelvin-Helmholtz waves along its outer boundary, the magnetopause.

“重要的发现了，但是科学家并没有发现任何动态特征以外，有些开尔文一亥姆霍兹波沿线的外边界，磁层顶。

Magnetopause boundary layer

磁层顶边界层

Magnetopause compression

磁层顶压缩

Magnetopause current

磁层顶电流

magnetopause

n. 磁顶, 磁(大气层)顶层