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日珥

na.【天】prominence; solar prominence
网络prominences; solar prominences; arcs of Lowitz

日珥

英-汉网络释义

日珥

prominence

加速世界第二季_百度百科 ... 黑暗星云（ Nega Nebulas）日珥（ Prominence）长城（ Green Wall） ...

solar prominence

日珥（英文：Solar prominence）是太阳表面喷出的炽热的气流，是在太阳的色球层上产生的一种非常强烈的太阳活动，是太阳 …

prominences

图中粉红色的结构就是日珥 (Prominences)。图中水蓝色的结构就是日冕(Corona)。

solar prominences

天体物理学词汇[ASTROPHYSICS] ... solar wind 太阳风 solar prominences 日珥 disk 太阳的可视圆面 ...

arcs of Lowitz

大气科学辞典/ 外语沙龙/... ... arcs of contact of halo 晕耳 arcs of Lowitz 日珥；罗氏弧 arctic air 北极空气；北极气团 ...

lowitz arc

航海及海运专业词汇英语翻译(J-L29) ... lowest 最下的 lowitz arc 日珥 lowmedium frequency radio range 低中频无线电导航信标 ...

Lowitz arcs

气象学专业词汇英语翻译L-24... ... 下对流层 lower troposphere 日珥；罗氏弧 Lowitz arcs 恒向线 loxodrome ...

lateral tangent arcs

气象学专业词汇英语翻译L-7-SCIdict学术词典... ... 侧向折射 lateral refraction 日珥 lateral tangent arcs 侧风 lateral wind ...

例句：

Nasa says the image is a classic example of a solar prominence (also known as a filament when viewed against the solar disk ).

美国宇航局称上面的图片是日珥（在太阳圆面观看时又称一暗条）的一个典型例子。

A solar prominence is a cloud of solar gas held just above the surface by the Sun 's magnetic field .

日珥是被太阳磁场束缚太阳表面之上的气体云。

Although very hot , prominences typically appear dark when viewed against the Sun , since they are slightly cooler than the surface .

虽然很热，日珥典型表现是在太阳的衬托下显得较暗，因为它们比太阳表面稍冷一些。

A tongue like cloud of flaming gas rising from the sun 's surface , visible as part of the corona during a total solar eclipse .

日珥从太阳表面升起的舌头状的燃烧气体的云，在日全蚀时成为。

The next day , the same prominence looked slightly different .

另一天，同一个日珥看起来会略有不同。

Known as a solar filament, the loop is a cloud of relatively cool gas held aloft by magnetic forces.

作为太阳的 “耳环 ”，日珥是一种被磁力托起的冷气团。

A tonguelike cloud of flaming gas rising from the sun's surface , visible as part of the corona during a total solar eclipse.

日珥从太阳表面升起的舌头状的燃烧气体的云，在日全蚀时成为日冕的一部分可看到

The prominence plasma flows along a tangled and twisted structure of magnetic fields generated by the sun 's internal dynamo.

日珥等离子体沿着一个由于太阳的内部活动产生的复杂弯曲磁场结构流动。

Prominences are clouds of relatively cool and dense plasma escaping from the Sun's hot and thin corona .

日珥是相对地较冷和较高密度的电离气体，并从较热和较薄的日冕之中喷射出来。温度高达六万度。

Sunspots , the Solar Cycle , and solar prominences are all caused by the Sun 's changing magnetic field .

黑子，太阳活动周期，以及日珥都是由太阳不断变化的磁场造成的。

A total solar eclipse , showing solar flares and prominences past the limb of the Sun, which is blocked by the Moon, and the solar corona .

日食发生在太阳黑子周期的高峰期，经过处理的图像不仅显示了日冕，而且显示了色球层和日珥。

The energy mechanism that creates a solar prominence is still a topic of research .

产生日珥的能量机制仍然是一个有待研究的课题。

However , scientists are still researching how and why prominences are formed .

然而，科学家依然在研究日珥形成的方式和原因。

Prominences occur in a variety of forms .

日珥以各种形状出现。

China has the earliest record of a solar prominence in the world .

中国有世界上最早的日珥记录。

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