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日冕

na.【天】 corona
网络solar corona; aureole; solar crown

日冕

英-汉网络释义

日冕

corona

为什么日冕（corona）那么热？日冕是太阳最外层的大气，其温度介于摄氏50万至600万度之间。

solar corona

托福词汇_百度文库 ... solar system 太阳系 solar corona 日冕 solar eclipse 日食 ...

aureole

gre词汇精选（最新词汇） - 豆丁网 ... augmentation 增加 aureole 日冕，光轮 auricular 耳的 ...

solar crown

航海及海运专业词汇英语翻译(S) ... solar corona 日华 solar crown 日冕 solar day 太阳日 ...

coronal

《太阳攻击》讲的是太阳皮肤（skin）日冕(coronal)有一天发生剥落飞向地球，即将引起大灾难的故事。这创意大约来源于《圣 …

The Corona

... 日冕 (The Corona) 日冕是太阳内部释出的气流所形成的,环绕在色球层的外围。 ... 一般日冕的外观随著太阳黑子活动的周期 …

sun's corona

SAT巴朗3500词汇 E-21CN教育 ... 夸张 exaggeration;overstatement. 日冕 sun's corona;halo. 哄骗，勾引 coax;wheedle. ...

CME

现在，你们中的一些人正从你们的太阳刚通过日冕（CME）所发出的能量冲击中慢慢恢复。我们的管道在上个周末花了很长时 …

例句：

For astronomers, today was a chance for a prolonged view of the sun 's corona , a spectacular blaze of plasma extending far into space .

为天文学家，今天是一个机会，长期鉴于太阳的日冕，壮观的大火血浆远远送入太空。

The top image shows the beginning of the coronal mass ejection , while the lower image shows the solar matter leaving the Sun 's corona .

上图显示的是日冕物质抛射的开始，而下图显示的是太阳物质脱离日冕的景象。

Much of visible light reaching us from the solar corona also seems to be due to scattering by electrons .

从日冕中射来的相当大一部分可见光看来也是由电子散射产生的。

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，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。

"The [Sun's] corona has a temperature of 2 million degrees but we don't know why it is so hot , " she said.

“日冕的温度高达两百万度，但是我们不知其原因，”她说。

When significant amounts of plasma escape the Sun , the event is called a coronal mass ejection .

大量等离子体脱离太阳，这种现象被称作日冕物质喷发。

All that's visible during totality is the sun's relatively faint upper atmosphere , called the corona .

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。

Total solar eclipse , the darkness outside the sun is the light silver-white, like the hat in the sun like a deduction, so called the corona .

日全食时，黑暗的太阳外围是银白色的光芒，像帽子似地扣在太阳上，因此称为日冕。

Solar eclipses allow scientists to see the gases surrounding the sun , or its corona .

科学家们能够在日食发生时观测到围绕在太阳周围的气体，也称日冕。

Explanation : During a total solar eclipse , the Sun's extensive outer atmosphere , or corona, is an inspirational sight .

说明：在日全蚀的时候，我们可以观察太阳的大气层形状，或称为日冕，日冕是一种太阳的光辉。

Aurora on May 29 were likely triggered by the interaction of the magnetosphere with a coronal mass ejection erupting from the Sun on May 24.

5月29日的极光可能是由 5月4日太阳日冕物质抛射影响磁层而触发。

The Solar Probe Cup will scoop up bits of the sun's corona and solar wind to continuously measure its speed , temperature and density .

太阳探测杯（TheSolarProbeCup ）会收集一些日冕和太阳风去持续地测量速度、温度和密度等数据。

One other interesting aspect of the relation of coronal holes to the solar wind follows from the appearance of coronal holes at the poles .

日冕洞与太阳风的关系的另一个有趣的方面是日冕洞在两极的形状。

Once at the solar corona , where the sun 's magnetic field is strong , the axions would convert back into photons .

一旦到达太阳磁场强烈的日冕处，这些轴子又会转变为光子。

The images show only the Sun 's corona, the outermost layer of the atmosphere .

图像显示太阳最外层的大气上只有日冕。

At each solar maximum , the corona sloughs off the magnetic fingerprint of the previous cycle by pushing it to the poles .

在每次太阳极大期，日冕通过把气体推向两极而使前一活动周期的磁性特征消退掉。

In the sudden darkness , the magnificent corona of the Sun became visible around the Moon .

在那短暂的黑暗期间，月亮的周围可以清楚的看到壮丽的日冕。

NASA planned to send a spacecraft to the Sun , aiming to solve two great mysteries of astrophysics - the corona and solar wind .

美国航空航天局计划派遣一艘宇宙飞船飞往太阳，试图解开日冕和太阳风两大太阳谜团。

Acoustic waves are a primary candidate for supplying the energy necessary to heat the solar chromosphere and corona .

声波是供给太阳色球和日冕加热所需能量的主要候选能源。

Nonetheless, NASA solar scientists agree that its speed and characteristics suggest that it was indeed a non-typical coronal mass ejection .

不过，NASA 研究太阳的科学家认为以这次日冕爆发的速度和特征，表明它是一个非典型的日冕物质喷发。

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