磁层

用能量色散X荧光法测定磁盘磁层厚度

The thickness measurements of magnetic layer on aluminum disc packs by energy dispersive X-ray fluorescence analysis

脉冲星表面磁层中电子运动的曲率辐射

Curvature radiation of motion electron in magnetic layer of pulsar surface

行星际磁场By分量对地球磁层顶场向电流调制

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

低能X射线在磁带磁层中的散射和吸收校正

Scattering and absorbed correction of low energy X-ray in magnetic tape and magnetosphere

类Crab脉冲星的三维磁层外隙模型

A Three-dimensional Outer - magnetospheric Gap Model for Crab-like Pulsars

在喜欢的方式，对地球磁层是被扭曲的X行星的影响，在极端。

In like manner , the Earth 's magnetosphere is being twisted by the influence of Planet X , in the extreme .

磁层顶边界层剪切流引起的MHD波模转化

Wave transformation induced by shear flow in the magnetopause boundary layer

利用AE指数重构磁层相空间&对存在问题的讨论

Phase space reconstruction of magnetosphere from AE index ── discussion of the problems existed

AE指数表现出的磁层的浑沌行为

Chaotic behaviour of magnetosphere revealed by AE index

行星际激波与地球磁层作用的全球MHD数值模拟

Global MHD Simulation of Interaction between Interplanetary Shocks and Magnetosphere

不考虑磁层顶磁重联的全球三维MHD模型

No magnetic reconnection at the magnetopause : A new 3-D MHD simulation model

对于典型的磁层等离子体参数，ωc的极大值约为0.3秒~（-1）。

For the typical parameters of the magnetospheric plasma , the maximum of ω c is about 0.3 sec-1 . We discuss also the relations between magneto-acoustic-gravity waves and geomagnetic micropulsations .

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 .

脉冲星B的X射线辐射能够被看到可能是因为脉冲星A的星风阻断了脉冲星B的磁层，为脉冲星B的星风提供了动力并加热中子星的表面。

Pulsar B 's X-ray emission might be visible because pulsar A 's wind intercepts the magnetosphere of pulsar B , powering pulsar B 's wind and heating up the neutron star 's surface .

磁层顶边界区剪切流MHD不稳定性的数值模拟研究III.大振幅MHD波

Simulation study of the MHD instabilities caused by the sheared flow at the boundarylayer of the magnetosphere

APS（AdvancedPhotoSystem）技术是感光胶卷反面涂有磁层以记录成像信息的新技术。

APS ( Advanced Photo System ) is a new technology of the sensitive film on which magnetic materials are besmeared over its reverse side to record and / or read imaging information .

本文介绍同位素源X射线荧光在磁带磁层厚度测定中，散射和吸收校正的两种方法&双道计数法和斜率校正法。

This paper describes two methods for the scattering and absorbed correction in a radioisotope source excited X-ray fluorescence analysis technique , that is two channel counting method and slope correction method .

低纬磁层边界区的可压缩性Kelvin-Helmholtz不稳定波

Compressional Kelvin-Helmholtz unstable waves in low latitude magnetospheric boundary regions

关于磁层边界区Kelvin-Helmholtz不稳定性的研究

On the Kelvin-Helmholtz instability in the magnetospheric boundary layer region

采用了Monte-Carlo方法，讨论了反铁磁层中不同非磁性掺杂浓度下，铁磁/反铁磁双层膜中交换偏置的温度特性。

Based on Monte Carlo method , the characteristic of exchange bias is discussed in diluted antiferromagnets in FM / AFM bilayers by changing the dilute concentration .

我国北极黄河站全天空极光观测显示了北极极区电离层对磁层顶磁重联有很好的响应，并且发现极光增亮的区域与行星际磁场（IMF）时钟角有很强的依赖关系。

The optical aurora measurements showed that the observational ionospheric region was good response to the magnetopause reconnections . The regions of the aurora brightening were much dependent on the IMF clock angle .

太阳风正负动压脉冲激发磁层ULF波的数值模拟

Numerical simulation of magnetospheric ULF waves excited by positive and negative impulses of solar wind dynamic pressure

在磁层昼侧，若IMF有南向分量，也就是和北向的地球磁场方向相反，则磁力线重连的效率最高。

Reconnection is most efficient when the IMF has a component that is directed southward & that is , opposite to the northward direction of the earth 's magnetic field at the dayside of the magnetosphere .

Shueetal.[1997]模型中提出了一个数学函数：其中（r，θ）是磁层顶的空间参数，用来表示磁层顶的位置。

Shue et al . [ 1997 ] model proposed a new function form : where ( r ,θ) is the spatial parameters of the magnetopause , to represent the place of the magnetopause .

用STARE-TRIAD联合观测对磁层-电离层不完全耦合的实例研究

A Case Study for Imperfect Magnetosphere-Ionosphere Coupling by STARE-TRIAD Joint Observations

通过改变NiO层的厚度、溅射气体Ar分压以及溅射气体与反应气体的比例Ar／O2，研究了反铁磁层厚度以及溅射条件对交换耦合场的影响。

The changes of the exchange fields with the thickness of NiO layers , the partial pressure of Ar and the ratio of Ar / O 2 were observed . The mechanisms of these changes were discussed .

任意多个磁层的层状结构中MSFVW和MSBVW的通用色散方程

The universal dispersion equations of msfvw and msbvw in arbitrary multilayer magnetic structure

地磁活动指数Kp增高时上行离子进入磁层的概率增大，因而上行离子起动力学作用的地球空间范围增大。

If K p is higher the probability of the up flowing ions to entry the magnetosphere will be bigger and region where the up flowing ions are dominant will be bigger .

本文解出了三维磁层顶的Chapman-Ferraro模型。

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

本文用STARE-TRIAD联合观测的一个实例研究磁层-电离层不完全耦合现象。

A case from STARE-TRIAD simultaneous observations is used to investigate the Magnetosphere-Ionosphere imperfect coupling .