• The magnetosphere was discovered in 1957.

    1957年,人们发现了磁气圈的存在。

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  • Charged particles carry currents, which cause significant modifications in the Earth's magnetosphere.

    带电粒子形成一股电流,对地球的磁气圈具有着很大的影响。

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  • The movie almost gets this one right-earth's magnetosphere does protect us from blasts of subatomic particles from the sun.

    影片在这点上倒是说对了,地球的磁气圈确实保护我们免受太阳风中亚原子颗粒的直击。

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  • 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。

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  • Lyons and Kim used the radar measurements to study the strength of the interaction between the solar wind and the Earth's magnetosphere.

    里昂和金使用雷达量测来研究太阳风和地球的磁气圈之间相互作用的强度。

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  • 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。

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  • The magnetopause exerts a tremendous influence on magnetic field within the magnetosphere.

    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。

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  • 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。

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  • The physical characteristics of whistler ducts in Earth's magnetosphere is inquired theoretically.

    本文在理论上探讨了地球磁层中哨声导管的物理特征。

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  • So solar wind transport into magnetosphere is one of the most important problems in magnetosphere research.

    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。

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  • Is there a relationship between recent quakes or signs of stress on the Earth plates and the twisting of the magnetosphere?

    最近的地震,地球板块所受的压力与磁气圈的扭曲有关联吗?

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  • The compass will be no help in this matter for perhaps months as the Earth's magnetosphere will take some time to re-establish.

    在这种情况下指南针将在大约几个月之内没有一点用处,因为地球的磁气圈需要时间来重建。

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  • The data observed by EISCAT are used to study the effect of the magnetosphere-ionosphere coupling on the high latitude ionosphere.

    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。

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  • The geospace, which includes the upper atmosphere, ionosphere and magnetosphere, is the most important region of human space activities.

    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。

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  • The rate at which the solar wind transfers energy to the magnetosphere can vary widely, but what determines the rate of energy transfer is unclear.

    太阳风将能量转化至磁气圈的速率变化很大。但是目前为止,我们仍不清楚到底是什么在决定着这种传送速率。

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  • The magnetosheath and foreshock are the key regions which somewhat modify and then transmit the solar wind variations to the Earth's magnetosphere.

    磁鞘区和地球弓激波前兆区是影响和改变太阳风波动特性,将太阳风能量传输到地球磁层的关键区域。

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  • Alternatively Icarus could use an extremely large magnetic sail to help decelerate, once within reach of the target star's solar wind or magnetosphere.

    或者伊卡洛斯飞船可以在到达目标恒星系统时,使用一张超大的磁力网,借助当地的太阳风或磁场来辅助减速。

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  • 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.

    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。

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  • Unlike the symmetrical pattern of the iron filings and magnet, the magnetosphere is pushed in on the side facing the Sun and stretched out in the Earth's wake.

    与铁屑和磁棒对称整齐的磁场模式不同,地球磁层面向太阳的一面被向内推,在相反的方向上延伸出磁场的轨迹。

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  • When the charged electrical particles approach the Earth, they carve out a highly magnetized region —the magnetosphere —which surrounds and protects the Earth.

    当这些带电粒子接近地球时,便形成一个很强的磁场区--磁气圈--包围着地球并对地球起一定的保护作用。

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  • Owing to the strong magnetic field in the magnetosphere, the magnetic field configuration essentially satisfies the approximation of the force-free field.

    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。

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  • The interaction of the solar particles with our planet's magnetic field has the potential to create geomagnetic storms, or disturbances in Earth's magnetosphere.

    太阳粒子同地球磁场的这种交互作用极有可能引起磁暴或者扰乱地球的磁场。

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  • An aurora is a bright glow that occurs in the night sky when energetic particles, mostly electrons, enter the Earth's upper atmosphere from the magnetosphere.

    极光出现于夜空中,是高能粒子,主要是电子,从地球的磁层进入高层大气时而产生的明亮光芒。

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  • Once it reaches Jupiter, Juno will orbit the planet's pole taking measurements that will provide insight into Jupiter's origin, structure, atmosphere and magnetosphere.

    当它抵达木星后,朱诺探测器将环绕其极点进行观测,了解木星的起源、结构、大气层和磁力圈。

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  • Since both KAWs and SKAWs have the magnetic-filed-aligned electric field, these waves are applied to the acceleration and heating of plasmas in magnetosphere widely.

    KAW和SKAW均携带平行于背景磁场的电场,因此被广泛应用于带电粒子的加速和加热。

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  • The physical processes described above may be useful in understanding the anomalous transport phenomena of energy and momentum from the magnetosheath to the magnetosphere.

    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。

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  • 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.

    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。

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  • 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.

    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。

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