日冕的变化反映的是太阳内部的变化。
Changes we see in the corona reflect changes deep inside the sun.
我们想要寻找日冕中的热波。
图像显示太阳最外层的大气上只有日冕。
The images show only the Sun’s corona, the outermost layer of the atmosphere.
这被称为日冕物质抛射。
日冕物质抛射在过去已经影响过发电站的运作。
Coronal mass ejections have affected power stations in the past.
在这些之外还有太阳风——由日冕而来的气体流。
Beyond that is the solar wind, an outflow of gas from the corona.
太阳大气则由光球层、色球层、过渡区和日冕组成。
The solar atmosphere above that consists of the photosphere, chromosphere, a transition region and the corona.
大量等离子体脱离太阳，这种现象被称作日冕物质喷发。
When significant amounts of plasma escape the Sun, the event is called a coronal mass ejection.
日冕将成为一个世纪以来这座形象建筑最引人注目的改变。
The corona will be the most dramatic alteration in the profile of the building in a century.
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。
Both flares and coronal mass ejections can create space weather if aimed at Earth.
“日冕的温度高达两百万度，但是我们不知其原因，”她说。
"The [Sun's] corona has a temperature of 2 million degrees but we don't know why it is so hot," she said.
日冕显的比太阳的其他部分暗淡，但那是有原因的。
The holes appear darker than other parts of the sun, but there's a reason for that.
最顶层的是超热日冕，由日冕环和电离气体流组成。
At the top is the super-hot corona, which is made of structures such as loops and streams of ionized gas.
这样的复合显示出内部日冕和外部日冕结构上的关联。
The composite brings out the correlation of structures in the inner and outer corona.
2月1日，日本的日之出太阳观测卫星拍摄了太阳的两个日冕。
Japan's Hinode sun-watching satellite photographed the sun's two coronal holes on Feb. 1.
日全食期间能看见的只有太阳上部相对模糊的大气，被称为日冕。
All that's visible during totality is the sun's relatively faint upper atmosphere, called the corona.
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。
These distortions create features ranging from sunspots to spectacular eruptions known as flares and coronal mass ejections.
图上太阳的最外层的区域称为日冕，在日全食时，照耀得如同月亮周围的光环。
The sun's outermost region, called the corona, shines like a halo around the moon during a total solar eclipse.
最后，恒星大气的最外层部分是日冕，这是一个由于外层对流导致的超热区域。
Finally, the outermost part of a star's atmosphere is the corona, which if super-hot might be linked with convection in the outer layers.
最后是日冕物质抛射，或是CME，一阵雨携带带电粒子云可在几天内到达地球大气。
Finally comes a coronal mass ejection, or CME, a slower moving cloud of charged particles that can take several days to reach Earth's atmosphere.
太阳海啸"也是能量释放的结果，天文学家目前认为它是日冕物质抛射产生的巨大冲击波。
The tsunami, a circular shockwave, is caused by a huge explosion, known as a coronal mass ejection.
天文学家们对日全食特别感兴趣，因为它是可以从地球表面看到的太阳日冕唯一的一次机会。
Total solar eclipses are of special interest to astronomers because it is the only time the sun's corona can be seen from the Earth's surface.
周日太阳表面出现了喷发现象——成吨的日冕抛射物质(等离子体流)被抛到太空中。
The sun's surface erupted early Sunday, blasting - tons of plasma (ionized atoms) into space.
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。
Most coronal mass ejections are more bulbous and wide: this one is quite narrow and contained.
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。
Sunspots are dark patches marking magnetically active regions that often host solar flares and violent belches called coronal mass ejections.
“如果类地行星很常见，那么第一代配备日冕仪的太空望远镜就能捕获光谱并识别生命迹象，”她说。
"If Earths are common, then the first generation of space telescopes with coronagraphs would get a spectrum and ID signs of life, " she said.
它能在太阳上形成一个亮点称为耀斑，也经常伴随着等离子云的释放，称为日冕物质抛射(CME)。
This can create a brightening on the sun called a flare, and is also often accompanied by the release of a cloud of plasma called a coronal mass ejection (CME).
他说，日冕层的大部分热量，很明显地仍是通过日冕层中应力磁场的强烈作用而释放出来的。
Most of the heat in the corona, said Klimchuk, is apparently still released by the snapping of stressed magnetic fields in the corona.
戏剧化的前景是岛上著名的巨大的单体石像莫埃，与微亮的日冕及黑暗的白天天空共同出现在海边的景色中。
In the foreground of the dramatic scene, the island's famous large, monolithic statues (Moai) share a beachside view of the shimmering solar corona and the darkened daytime sky.
“我认为有必要指出，我们还没有解决日冕是如何被加热的，但是我们离答案又近了一步”，巴特德巴日尔说。
"I think it's important to point out that we have not solved coronal heating, but we have provided a piece of the puzzle," he says.
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