1.
Coronal structure and brightness profile of the total solar eclipse on August 1,2008
2008年8月1日日全食的日冕结构和亮度分布
2.
Looking at small details we find that the corona has a delicate structure.
仔细研究细节后，我们发现日冕有精细结构。
3.
the coronation day, robes, coach
加冕日、 袍、 马车等.
4.
We show that both the preevent corona and the driving mechanism are important in the formation and evolution of CMEs.
结果表明,初态日冕和驱动机制对日冕物质抛射的形成及演化都有重要影响.
5.
intermediate corona
中介日冕-中等太阳活动时的日冕
6.
Structures and Spectra from Slim Disk and Slim Disk/Two-temperature Corona;
细盘与细盘/双温冕的结构和出射谱研究
7.
These results may interpret the formation of plasmoid type CME.
这些结果可用于解释等离子体团型日冕物质抛射的形成。
8.
Fraunhofer component
日冕光谱夫琅和费部分
9.
quiet coronal X-ray emissio
宁静日冕Ｘ射线辐射
10.
In this paper the author expound mainly the current status in the research of solar quiet corona, coronal holes and heating mechanism of corona.
主要论述宁静日冕和冕洞，以及日冕加热问题的研究现状。
11.
coronograph and similar instruments, for observing the sun's corona
日冕仪和用于观察太阳日冕的类似仪器
12.
POLARIZATION OBSERVATION OF THE SOLAR CORONA AT THE SOLAR ECLIPSE OF 1968 SEPTEMBER 22.
1968年9月22日日食的日冕偏振观测
13.
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。
14.
On the other hand, all the material in the transversal sheet comes from the corona and produces a high-temperature coronal loop.
横向电流片的物质则全部来自日冕,从而形成高温日冕环。
15.
Polarization Observation of White Light Corona during the Total Solar Eclipse on 2006 March 29
2006年3月29日日全食白光日冕偏振测量(英文)
16.
non-Fraunhofer component
非夫琅和费部分-日冕光谱
17.
The corona gains and loses energy continuously.
日冕总是不断地获得能量和损失能量。
18.
The continuum of the corona is essentially radially polarized.
日冕连续区基本上是经向偏振。