• These are called coronal mass ejections.

    这被称为日冕物质抛射。

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  • Coronal mass ejections have affected power stations in the past.

    日冕物质抛射在过去已经影响过发电站的运作。

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  • You may be seeing a pattern with the solar flares and coronal mass ejections.

    你也许会看到在太阳耀斑和日冕抛射中体现的一种模式。

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  • Both flares and coronal mass ejections can create space weather if aimed at Earth.

    太阳耀斑和日冕物质抛射都能产生对地球有影响的空间天气。

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  • Most coronal mass ejections are more bulbous and wide: this one is quite narrow and contained.

    绝大多数日冕物质抛射看起来是球根形的、宽的;而这次日冕则是很窄的并且包裹住的。

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  • Very large coronal mass ejections are thought to happen every 500 years or so (the most recent was in 1859).

    大规模的日冕物质抛射被认为每隔500年或约500年发生一次(最近一次发生于1859年)。

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  • This means that slight perturbations of the star might cause enormous ejections of matter from its surface.

    其意思也就是即使轻微的干扰,恒星都可能引起剧烈的表面物质抛射。

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  • These distortions create features ranging from sunspots to spectacular eruptions known as flares and coronal mass ejections.

    这种变形造就了太阳黑子以及耀斑和日冕物质抛射等壮观的景象。

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  • One telescope aboard SOHO can provide three or four days' warning of major solar events by spotting coronal mass ejections.

    通过观测日冕物质的喷发,SOHO上的一台望远镜能提前三到四天预报太阳的重大活动。

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  • One telescope aboard SOHO can provide three or four days ' warning of major solar events by spotting coronal mass ejections .

    通过观测日冕物质的喷发,SOHO上的一台望远镜能提前三到四天预报太阳的重大活动。

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  • He says the Coronal Mass Ejections are extremely large magnetic clouds that are expelled from the sun at extremely high speeds.

    他说,日冕物质抛射是指太阳以极高速度释放出来的非常大的磁云。

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  • The website contains imagery collected by two NASA spacecraft that together create "stereo" 3-d images of the sun's coronal mass ejections.

    这个网站包含了由两台美国国家航空航天局的航天器收集到的图像。这两台航天器一起制作太阳日冕物质喷发的“立体”3维图像。

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  • Sunspots are dark patches marking magnetically active regions that often host solar flares and violent belches called coronal mass ejections.

    黑子是太阳表面比较暗的区域,也叫活动区。那里经常发生耀斑和日冕物质抛射等剧烈的喷发现象。

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  • So enjoy the current rash of solar flares and beautiful coronal mass ejections; it might be some time before we see a solar cycle like this again.

    所以好好的享受这些美妙的太阳耀斑和日冕带来的太阳风吧,可能要经过相当长一段时间我们才能再次观赏到他们了。

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  • More recently, however, our sun has become increasingly active and exhibiting a greater abundance of sunspots, flares, and coronal mass ejections.

    但是最近,我们的太阳变得活跃起来,其表面出现了大量的黑子,耀斑以及日冕物质抛射。

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  • Extreme events - including massive ejections of material from the sun's corona - have been known to disrupt power lines and trigger widespread blackouts on earth.

    人们知道,极端情况——包括太阳日冕的大量物质喷发——会破坏地球的供电线路,从而引发大面积停电。

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  • What's more, a decrease in sunspots doesn't necessarilymean a drop in other solar features such as prominences, which can produce aurora-triggering coronal mass ejections.

    而且,太阳黑子减少并不一定意味着太阳的其它特征的减少,比如日珥——它能产生引起极光的日冕物质抛射。

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  • Giant eruptions from the sun called Coronal mass Ejections cause "space weather storms" which, if large enough, could lead to massive disruption of electric grids on Earth.

    太阳表面物质的大喷发,即所谓的日冕物质抛射,导致“空间气象的风暴”,如果喷发的能量足够大,可能引起地球上电网系统的大规模破坏。

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  • The solar ejections that cause auroras can also create geomagnetic storms that can affect spacewalking astronauts, Earth-orbiting satellites, and even communications and power systems on the ground.

    引起极光的太阳能量抛射还能引起地磁风暴,能够影响宇航员的太空行走,绕地卫星甚至是地面上的通信和电力系统。

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  • The solar ejections that cause auroras can also create geomagnetic storms that can affect spacewalking astronauts, Earth-orbiting satellites, and even communications and power systems on the ground.

    引起极光的太阳能量抛射还能引起地磁风暴,能够影响宇航员的太空行走,绕地卫星甚至是地面上的通信和电力系统。

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