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1·He tracks streamers from the solar corona, the sun's outer atmosphere seen during eclipses.

他目前在追踪观测日冕(即日食时我们看到的太阳的外层大气)中发射出的粒子流。

2·The final speed of the solar wind depends mainly on the maximum temperature in the solar corona.

太阳风的最终速度主要取决于日冕中的最高温度。

3·The harmonic number of the spike emission is confirmed by the comparison of the diagnosis with the typical parameters in solar corona.

最后从诊断结果和太阳日冕典型参数的比较以确定尖峰辐射的谐波数。

4·N. , Zhang, B. and Wang, S. , 1995, A mechanism for the formation of plasmoid-type CME in the solar corona, ACTA Astron. Sinica, 36 , 341.

郑惠南，张兵，王水， 1995，等离子体团型日冕物质抛射的形成机制，天文学报， 36 ， 341。

5·The Moon's silhouette surrounded by a glistening solar corona hangs above the Jiayuguan Fort along the western edge of the Great Wall of China.

影像中，月亮的暗影和太阳闪耀的日冕，高悬在中国长城西端的嘉峪关上空。

6·Clearly drawn is not only a total solar eclipse, but the solar corona and the diamond ring effect visible when sunlight flows only between mountains on the Moon.

很明显画中并不仅仅是日全食，其中还能看到日冕以及当日光刚从月球山峰之间露出时出现的钻石环效应。

7·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.

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。

8·During Sunday's total solar eclipse, the moon covered the sun over Easter Island, so that only the faint, white ring of the sun's upper atmosphere, or corona, was visible.

周日发生在复活节岛上的日全食，月亮将太阳覆盖了起来，只有太阳上层大气所形成的一圈微弱的白色圆环或称日冕处于可见状态。

9·The sun's outermost region, called the corona, shines like a halo around the moon during a total solar eclipse.

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。

10·NASA’s goals are to figure out why the sun’s corona is several hundred times hotter than the surface and why it produces an accelerating solar wind.

NASA的目标是能够清楚描述出为什么日冕的温度要高于太阳表面温度上百倍，为什么其会产生加速太阳风。

日冕

1·He tracks streamers from the solar corona, the sun's outer atmosphere seen during eclipses.

他目前在追踪观测日冕(即日食时我们看到的太阳的外层大气)中发射出的粒子流。

2·The final speed of the solar wind depends mainly on the maximum temperature in the solar corona.

太阳风的最终速度主要取决于日冕中的最高温度。