大气风暴出现在几小时内，持续几天，而磁暴形成要几十年，持续几个世纪。
Whereas atmospheric storms arise in a matter of hours and last for days, magnetic tempests develop over decades and persist for centuries.
地球磁场是由地球外核的熔铁围绕固体内核旋转而产生的；当铁水激增，就会发生磁暴。
The Earth's magnetic field is generated as the molten iron of the Earth's outer core revolves around its solid inner core; when surges in the molten iron occur, magnetic tempests are created.
这种磁暴对磁法勘探产生严重的破坏。
Such storms cause considerable disruption in magnetic prospecting operation.
本文分析了磁暴期间南极长城站的电离层扰动特性。
In this paper, ionospheric disturbances during geomagnetic storms at the Great Wall station in Antarctic are studied.
航空预报员说，太磁暴的旋涡流将一直持续到下周。
Continued turbulence on the sun remains a concern for the next week, space forecasters say.
分析表明，南极极隙区与中低纬区磁暴形态差异很大。
This magnetic storm has different physical processes at the middle low latitudes and the southern polar cusp region.
本文研究了武昌上空与磁暴有关的电离层夜间分层事件。
In this paper, the stratification events of the ionosphere related to geomagnetic storm in the night-time over Wuchang are studied.
此外，此磁暴过程期间在中低纬区存在明显的波动过程。
Moreover, at the mid and low latitude areas there was an evident wavelike process.
英雄级的磁暴单位将会有黄色的闪电特效和新的开火特效。
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.
磁暴的充电粒子对航天员与在高空飞行器上的旅客的健康构成危害。
The storms' charged particles can be a hazard to the health of astronauts and passengers on high altitude flights.
磁暴线圈可以互相充能，充能的话增加射程与新的开火特效和音效。
Tesla Coils are able to charge each other. Increase Range when charged and new fire and sound fx.
磁暴步兵会自动给身边的线圈充能，你也可以手动命令他们去这么做。
Tesla Troopers will do this on their own to any nearby Coils, or you can manually order them to do so.
这表明利用IPS观测进行磁暴急始预报有很大的潜力和现实可能性。
This shows the potentiality of using IPS observations to predict the geomagnetic SSC.
可以，磁暴步兵仍旧能够给身边的磁暴线圈充能，提高磁暴线圈的功率。
Yes, Tesla Troopers will still be able to charge nearby Tesla Coils for a boost to their efficiency.
磁暴主相的形成同微粒流的速度关系密切，但同微粒流密度的关系不大。
The formation of the storm's main phase is closely related to the velocity of the corpuscular stream, while the relation with the density of stream, is poor.
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。
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.
磁暴还会对高层大气存在加热作用，改变其密度计组成，中断无线电通信与GPS装置。
Magnetic storms also heat the upper atmosphere, changing its density and composition and disrupting radio communications and GPS units.
但是，如果不发生大喷发，地球将不会受磁暴影响，也就不会产生明亮的极光。
But without a large prominence eruption, we will not have a magnetic storm here at Earth that drives the brilliant aurora.
太阳磁暴最严重的直接影响是北部航线飞机的高频声波通讯系统会发生中断。
The biggest immediate effect was the blackout of high-frequency voice-radio communications for planes flying far northern routes.
据初步估计，我们的计算与帕克尔等的理论结果相符，并可以解释磁暴主相。
With a suitable choice of the parameter of the solar wind and the capture probability, our result may explain fairly well the theoretical investigation of Parker and others.
虽然极光通常只出现在高纬度地区，但是在磁暴发生时，极光也能点亮稍低纬度地区的天空。
And while aurorae are normally visible only at high latitudes, they can light up the sky even at lower latitudes during a geomagnetic storm.
尽管他们呈现出如此的视觉效果，然而这些色彩斑斓的光线实际上是风暴地磁暴。
Despite their visual appeal, these brilliant light shows are actually storms - geomagnetic storms.
采用一个半经验模式利用垂测数据计算了磁暴效应引起的有效热层子午向中性风。
Baed on the ionosonde data, we used an empirical method to derive the neutral meridional wind during tile storm.
太阳上的磁暴威力足够强大，可以对人造卫星和地球上通信系统的各个方面产生影响。
Magnetic storms on the sun are powerful enough to have an effect on satellites and communication systems all the way here on Earth.
从电离层等离子体动力学方程出发，研究了磁暴期间中性风对中低纬度电离层的影响。
With the kinetic equation of ionospheric plasma, the paper studies the influences of neutral winds on the ionosphere at middle-low latitude.
从电离层等离子体动力学方程出发，研究了磁暴期间中性风对中低纬度电离层的影响。
With the kinetic equation of ionospheric plasma, the paper studies the influences of neutral winds on the ionosphere at middle-low latitude.
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