磁层液和塑料，作为模拟的地球磁层显示。
Magnetospheres are fluid and plastic, as the simulation of Earth's magnetosphere shows.
土星磁层的性质似乎是在中坚饽地球和木星的。
Saturn's magnetosphere appears to be intermediate in nature to those of Earth and Jupiter.
本文在理论上探讨了地球磁层中哨声导管的物理特征。
The physical characteristics of whistler ducts in Earth's magnetosphere is inquired theoretically.
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.
本文讨论有力场的脉冲星磁层结构。用极角展开的方法。
In this paper, the magnetospheric structure of pulsar is discussed for the forced magnetic field.
在相同的参数下，振荡周期与铁磁-非磁层的对数有关。
The oscillation period and the oscillation amplitude relate to CO concentration, heating power PF and so on.
地球因为有一个由内部磁场产生的保护磁层而免受大部分辐射的影响。
The Earth is protected from much of this radiation because it has an internal magnetic field that generates a protective magnetosphere.
因此磁暴的地面观测是了解磁层的最基本、最有效的手段。
Therefore ground-based observations of the magnetic storm is the most basic understanding of the magnetosphere, the most effective means.
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.
由于磁层内部的磁场很强，其位形基本满足无作用力磁场近似。
Owing to the strong magnetic field in the magnetosphere, the magnetic field configuration essentially satisfies the approximation of the force-free field.
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。
The magnetopause exerts a tremendous influence on magnetic field within the magnetosphere.
练习效应则是由于交换耦合系统中反铁磁层的热激活反转所引起的。
The training effect is a result of thermally activation reversal of the antiferromagnetic layer through the exchange coupling.
因此，太阳风向磁层的传输是磁层物理研究的一个非常重要的问题。
So solar wind transport into magnetosphere is one of the most important problems in magnetosphere research.
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。
The analysis shows that this method may be used to identify several types of the discontinuities which may occur at the magnetopause.
计算了剪切流场中阿尔文波的传播过程，以及磁层中阿尔文波的耗散。
The propagation process of the Alfven wave in a shear velocity field is calculated, and the dissipation of Alfven waves in the magnetosphere is given.
涵盖的区域包括地球高层大气、电离层、磁层、行星际空间直至太阳。
The field that space environment contain is high - layer atmosphere, ionosphere, magnetic layer, interplanetary space and even sun.
这些结果，对于了解火星感应磁层形成的物理机制有着重要科学意义。
These results are significant to study the physical mechanism of the solar wind interaction with Mars.
结果表明，增加铁磁层和导电层的厚度都会增强多层膜的应力阻抗效应。
The results show that the stress-impedance effect increases with the increase of the thickness of the ferromagnetic layer and metal layer.
研究了中间绝缘层厚度、界面状况及反铁磁层钉扎对隧穿磁电阻的影响。
The effects of barrier thickness, interface and anti-ferromagnetic pinning on the TMR values of the MTJs have been studied.
当行星际磁场有大的南向分量时，磁层的位形可由基本闭式转变为开式。
The magnetospheric configuration is converted from the nearly closed one into an open one, when the IMF has a large southward component.
上述物理过程可能对解释磁鞘至磁层的能量及动量异常输运现象有所帮助。
The physical processes described above may be useful in understanding the anomalous transport phenomena of energy and momentum from the magnetosheath to the magnetosphere.
本文利用EISCAT雷达资料讨论磁层-电离层耦合的高纬电离层效应。
The data observed by EISCAT are used to study the effect of the magnetosphere-ionosphere coupling on the high latitude ionosphere.
结果表明，冬季中山站电离层内的电离生成主要取决于从磁层沉降的粒子。
The results show that the major source of electron and ion production at Zhongshan Station is almost completely dependent on particles precipitated from the magnetosphere.
地球空间包括高层大气、电离层和磁层，是人类空间活动的最主要的区域。
The geospace, which includes the upper atmosphere, ionosphere and magnetosphere, is the most important region of human space activities.
结果表明，铁磁层和中间导电层厚度的增加都会增强多层膜的应力阻抗效应。
The results show that the stress-impedance effect increases with the increase of the thickness of the ferromagnetic layer and the metal layer.
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.
为了提取地壳异常场，必须从观测资料中消除主磁场、磁层场，感应场和电离层场。
In order to get the crustal anomaly field, the main field, magnetospheric, ionospheric and induction fields from the Magsat data must be subtracted.
为了提取地壳异常场，必须从观测资料中消除主磁场、磁层场，感应场和电离层场。
In order to get the crustal anomaly field, the main field, magnetospheric, ionospheric and induction fields from the Magsat data must be subtracted.
应用推荐