magnetosphere
A sixth region in the magnetosphere?
磁层的第六区域？
Now, it is storms in the magnetosphere that are recorded.
现在，磁力计中所记录下的都与暴风雨有关。
The earth's magnetosphere is at once protective and dangerous.
地球的磁层既具有保护的功能，却又极其危险。
A continuous stream of charged particles, called the solar wind, impinges on the earth's magnetosphere.
称作太阳风的连续带电子流撞击在地球的磁层上。
The transfer of magnetic energy from the solar wind radically alters the shape of the magnetosphere.
从太阳风传来的磁场能量，彻底改变了磁层形状。
The magnetosphere is a bubble of magnetism that surrounds earth and protects us from solar wind.
磁气圈是一个包裹着地球的磁性泡泡，保护着我们免受太阳风的吹袭。
But in the magnetosphere, weather results from the interaction between the earth's magnetic field and the solar wind.
但在磁层里，太空天气却是由地球磁场和太阳风的交互作用所造成。
CMEs can interact with the Earth's magnetosphere, causing problems for satellites, communications, and power grids.
日冕物质抛射与地球磁层相互作用导致卫星发生故障，通信无法进行，电网瘫痪等问题。
Sensors recorded a torrent of solar wind particles streaming into the magnetosphere, says Raeder.
两个磁场的对齐让他们链接起来把地球的磁场在两极处撕开两个洞。
Barabash points out that a planet's magnetosphere will always be far larger than the planet itself or its atmosphere.
巴拉瓦什指出，一个行星的磁层总是远大于行星本身或它的大气层。
SPG studies the interaction of theSun on the Earth's magnetosphere and ionosphere.
由新的地球空间物理实验室（GPL）资助并参与其许多活动中。
Photo Gallery: Sun An aurora glows from the Earth's magnetosphere, as seen from the International Space Station.
意译：太阳图片画廊。极光指示灯从地球的磁层，从国际空间站。
This animation shows a conceptual sketch of Mercury's magnetosphere at the time of the MESSENGER flyby.
这个动画是信使号探测船探测水星磁层时的模拟图。
An aurora glows from the Earth's magnetosphere, as seen from the International Space Station.
太阳图片画廊。极光指示灯从地球的磁层，从国际空间站。
Its rapid rotation, acting on electric currents in the core, generates a strong magnetic field and large magnetosphere.
它自转很快，由地核的电子流推动，产生强大的磁场和磁气圈。
British "team from Rutherford-Appleton plans to build an artificial magnetosphere in the laboratory.
以下经验：-5年以上相关行业开发经验，构建和商业网站；
A continuous stream of charged particles, called the solar wind, impinges on the earth's magnetosphere .
称作太阳风的连续带电子流撞击在地球的磁层上。
We use a three dimensional pulsar magnetosphere model to study the geometry of outer-magnetospheric gaps.
利用三维脉冲星磁层模型研究了磁层外隙的几何结构。
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。
The Earth is protected from much of this radiation because it has an internal magnetic field that generates a protective magnetosphere.
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。
Studies of Jovian magnetosphere via local measurements of charged particle fluxes and by remote sensing of auroral emissions.
研究木星磁层,测量与遥感带电粒子的数量。
In the afternoon, convective winds push the cloak out toward the edge of the magnetosphere, where it's peeled off by solar winds.
到了下午，对流风将“斗篷”推至磁层边缘，在那里“斗篷”逐渐被太阳风吞噬。
The three ST5 satellites, each no bigger than an average TV set, will help scientists to study magnetic fields in Earth's magnetosphere.
三个空间技术5号卫星(每个尺寸都不大于一台普通的电视机)将帮助科学家研究地球磁气圈的磁场。
In other words, how can the wind overcome the barrier of the geomagnetic field and drive the motions of the plasma inside the magnetosphere?
换言之，即太阳风是如何克服地球磁场的阻碍，进而驱动磁层里的电浆运动?
Thus, this research could not say much about the effects of interplanetary charged particles, which cannot penetrate Earth's magnetosphere.
因此，对游走于行星之间，但是无法穿透地球磁层的带电粒子所产生的效应，这项研究所透露的讯息不多。
Scientists have found two large leaks in Earth's magnetosphere, the region around our planet that shields us from severe solar storms.
科学家在地磁层中发现了两个很大的漏洞，地磁层环绕着我们的星球并且保护我们不会被太阳风暴袭击。
Yet the actual long-term survival of active organisms, spores or complex organic molecules beyond Earth's magnetosphere has never been tested.
活性有机体、孢子或复杂的有机分子，在地球磁层之外能否长期幸存，则从未实地验证过。
This tangling of the field lines allows large amounts of plasma and magnetic energy to be transferred from the solar wind to the magnetosphere.
两者的磁力线互相纠缠，促使大量的电浆和磁场能量从太阳风转移到地球磁层里。
These studies revealed that Jupiter's magnetosphere is lopsided, with an unexpected abundance of ions and electrons escaping from one flank.
上述研究发现，木星的磁层是偏斜的，而且有大量的离子和电子由一侧逃逸。
Other instruments will examine the interaction of Titan's atmosphere with charged particles from Saturn's magnetosphere.
其他仪器则会检视土卫六大气与土星磁层带电粒子的交互作用。
Earth's magnetosphere is more than a million miles in the tail, which trails off in the downwind direction from the sun.
地球磁层的尾部长度超过100万英里，并且自太阳的顺风方向渐渐消失。
In this paper, it is supposed that the wavy magnetodisc structure of the Jovian magnetosphere may be caused by large-scale bending waves in the Jovian plasma sheet.
本文提出,术星磁盘的波状结构可能是由木星等离子体片中存在的大尺度弯曲波引起的。
They move under the influence of the dynamo currents in the Earth's core,as well as electric currents flowing in the ionosphere,the radiation belts and the Earth's magnetosphere.
它们在地核内发电机流以及流动在电离层、辐射带和地球磁气圈内电流的影响下产生移动。
Caption:: The Jovian magnetosphere, including the Io flux tube, plasma torus, Jovian aurorae, the sodium cloud, and sulfur torus is shown in this illustration.
木星的磁层是全太阳系最大的物体。若我们肉眼可以看到木星的磁层，它足足有满月的五倍般大小。在木星附近，它的卫星活在这个庞大的磁层内，如木卫一艾奥就形成了等离子圆环，而且也跟木星通电。
The distribution characteristic of auroral electrojet in AZS, is helpful for the studies of F layer and magnetosphere coupling in polar region and aurora dynamics.
了解了极光电集流在南极中山站的分布特征,有利于极区电离层和磁层耦合及极光动力学的研究。
In principle, there are two topologically disconnected outer gaps in the magnetosphere of a pulsar.Both incoming and outgoing particle flows are allowed.
在脉冲星的磁层中，原则上有两个拓扑分离的外隙，允许同时进入和流出粒子。
The abrupt movement of the field lines heats and accelerates the ions and electrons in the plasma sheet, injecting them into the inner part of the magnetosphere.
这种磁力线的突然变化，会加热并加速电浆片里的离子和电子，将它们抛向磁层内层；
The region in space that contains the Earth's magnetic field, known as the magnetosphere, protects us from the charged particles that come streaming from the sun.
含有通常叫做磁层的地球磁场的空间区域，它能使我们免受从太阳上流下的带电粒子流的冲击。
The pitch angle scattering of particles is studied in the magnetosphere for three cases:the strong scattering,the weak scattering and the regular scattering.
研究了地球磁层中粒子投掷角扩散过程,分析了强扩散、弱扩散和一般扩散等特性.计算结果表明,在强扩散过程中,粒子填满整个损失锤区域;
Physics of Solar System Plasmas provides a comprehensive introduction to the plasma physics and magnetohydrodynamics that are needed to study the solar wind and magnetosphere.
太阳系等离子的物理学提供综合的被需要研究太阳风和磁性层的等离子物理和磁流体力学的介绍。
Under these circumstances, reconnection takes place along a wide equatorial belt, opening up nearly the entire outer boundary of the magnetosphere to the solar wind.
在这种情况下，磁力线重连会在赤道面上宽广的带状区域内发生，几乎把整个磁层外围边界都打开，放太阳风进来。
They move under the influence of the dynamo currents in the Earth's core, as well as electric currents flowing in the ionosphere, the radiation belts and the Earth's magnetosphere.
它们在地核内发电机流以及流动在电离层、辐射带和地球磁气圈内电流的影响下产生移动。
A synthetical study by using the results from the GEOS-2 electron gun experiment S329 and the relaxation sounding experiment S301 is made to discuss the convection pattern in the magnetosphere.
本文对GEOS-2卫星S329电子枪实验和S301冷等离子体电子浓度实验所得对流图象进行了综合分析比较.
The wide-ranging auroral activity was triggered as a large solar flare - an energetic cloud of particles blasted outward from the Sun a few days earlier - collided with planet Earth's magnetosphere.
这大范围的极光活动是由一个巨大的太阳耀斑引起的，几天前就有高能粒子云从太阳表面爆发出来，之后与地球的磁场发生碰撞。
For other orientations of the IMF, reconnection still happens, but it may be more localized in the higher latitudes, where the released energy mainly flows around the magnetosphere rather than into it.
假如IMF指向别的方向，磁力线重连仍能发生，但会比较局限在高纬度，释放出的能量则主要流经磁层外围，而非流入磁层内部。
Implying the up-wind scheme and adaptive grids, we have established a 3-D simulation model of the magnetosphere based on the ideal MHD equations, and successfully achieved quasi-steady states.
我们基于理想磁流体力学方程,采用迎风格式差分和可变格点大小的数据结构,建立了一个三维磁层MHD模型,并实现了准稳态运行。
Once the transfer of energy from the solar wind abates, the flow of plasma into the inner magnetosphere slows, and ions are lost from the ring current more rapidly than new ones arrive.
一旦从太阳风传来的能量趋缓，进入磁层内部的电浆流就变慢，这时在环电流中，离子的流失远比补充进来的快。
Waves are in fact observed along the magnetopause.But they do not seem capable of driving the large-scale circulation of the magnetosphere or the great disturbances that often occur there.
事实上，研究人员的确曾经观测到地球磁层顶上的波动，只是以它们的强度，似乎不足以驱动磁层里的大规模循环运动，或造成经常性的剧烈扰动。
Each encounter will also reshape Cassini's orbit, enabling the craft to get close-up views of Saturn's other satellites and its rings, as well as sample different parts of its magnetosphere.
每接近一次，便会改变卡西尼号的轨道，使太空船能够就近观测土星的其他卫星和土星环，同时对土星磁层不同的部份进行采样。
They move under the influence of the dynamo currents in the Earth 's core , as well as electric currents flowing in the ionosphere, the radiation belts and the Earth 's magnetosphere.
它们在地核内发电机流以及流动在电离层、辐射带和地球磁气圈内电流的影响下产生移动。