太阳风层

计算表明，K-H不稳定性确实能在太阳风-磁层耦合中起重要作用。

The calculations show that the Kelvin-Helmholtz instability can indeed play an important role in the coupling processes between the solar wind and the magnetosphere .

太阳风和磁层能量耦合系数的计算研究

The Statistic Study of the Energy Coupling Coefficient Between Solar Wind and the Magnetosphere

磁暴期间太阳风-磁层-电离层间的耦合过程

The solar wind-magnetosphere-ionosphere coupling during magnetic storm

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。

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

而重联磁力管起源于磁层的部分则仍然位于磁层顶内侧，并为太阳风进入磁层提供了路径。

The magnetosphere part of the flux tube is still inside the magnetosphere after reconnection and applies the path for the solar wind entry into dayside magnetosphere .

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。

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 .

太阳风与磁层相互作用不仅会导致地磁扰动，还会导致磁层辐射带电子环境的变化。

The interaction between the solar wind and the magnetosphere not only will lead to the disturbance in the geomagnetic field but also will lead to the variation in the electron environment .

本文用行星际和地面磁场以及电离层资料，讨论了三次磁暴期间高、中纬电离层电场对太阳风和磁层内变化的响应。

The indices of IMF , ground magnetic field and observations of ionospheric E-field are used to study the response of E-field in high and middle latitude ionosphere to variation of the solar wind and the magnetosphere .

从太阳风-磁层能量耦合的普遍表达式出发，用34天连续的太阳风观测资料对电磁耦合机制进行了数值检验。

Based on the general formula of the energy transfer rate from the solar wind into the magnetosphere , the coupling mechanism of MHD flow is examined by using solar wind data for a period , of 34 days .

极区电离层通过对流电场、粒子沉降和场向电流与磁层紧密耦合在一起，在太阳风-磁层-电离层以及热层耦合过程中起着重要作用。

Polar ionosphere is especially structured and coupled with magnetosphere via convection electric field , particle precipitation and field-aligned current . It plays an important role in the coupling processes among the solar wind , magnetosphere , ionosphere and thermosphere .

太阳风-磁层-电离层组成了地球空间的一个复杂的耦合体系，基于不同行星际条件或地磁条件下，等离子体层和电离层间物质输运机制仍未弄明。

A complex coupling system is formed by the solar wind , magnetosphere and ionosphere in geospace . And an important process in geospace that is still not fully understood is the plasma transport between the plasmasphere and the ionosphere during different interplanetary disturbance and geomagnetic condition .

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

携带着行星际磁场的太阳风被地球磁层所减速产生了弓激波以及磁鞘区。

The solar wind , carrying the plasma and IMF , is slowed down by the magnetosphere , produce the bow shock region and the magnetosheath .

通量管为太阳风等离子体向磁层输运和磁层粒子向行星际空间逃逸提供了通道。

The flux ropes offered channels for the transport of the solar wind plasma into the magnetosphere and the escape of the magnetospheric plasma into the interplanetary space .

太阳在地球附近的电磁场已经偏向南方，在地球抵御太阳风的磁场防卫层上打开了一道口子。

The sun 's magnetic field near Earth has tipped south , opening a crack in Earth 's magnetic defenses against the solar wind .