1.
A discussion on the transport of magnetic energy and complexity to the corona is given in this paper.
本文讨论了从太阳光球向日冕传输磁能和磁复杂性的过程。
2.
the coronation day, robes, coach
加冕日、 袍、 马车等.
3.
intermediate corona
中介日冕-中等太阳活动时的日冕
4.
Characteristics of the Propagation and Evolution of Interplanetary Coronal Mass Ejections in the Heliosphere;
行星际日冕物质抛射在行星际空间的传播和演化规律
5.
Fraunhofer component
日冕光谱夫琅和费部分
6.
quiet coronal X-ray emissio
宁静日冕Ｘ射线辐射
7.
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。
8.
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
9.
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
10.
Traditional English May Day rites and celebrations include Morris dancing, crowning a May Queen, celebrating Green Man day and dancing around a Maypole.
传统的英国五一节习俗和庆祝活动包括莫理斯舞、五月女王加冕、庆“绿人日”、月花柱舞。
11.
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。
12.
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)
13.
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
14.
Scripting for Transfer failed. Check log files.
编写传输脚本失败，请检查日志文件。
15.
non-Fraunhofer component
非夫琅和费部分-日冕光谱
16.
The corona gains and loses energy continuously.
日冕总是不断地获得能量和损失能量。
17.
The continuum of the corona is essentially radially polarized.
日冕连续区基本上是经向偏振。
18.
Computing the Coronal Temperature by Using the Filter Ratio Method;
用Filter Ratio方法计算太阳日冕温度