1.
Simulation of Atomic Coefficient and Radiation Losses of Impurity Using Non-coronal Model on HL-2A;
HL-2A杂质原子参数和非日冕辐射的模拟
2.
quiet coronal X-ray emissio
宁静日冕Ｘ射线辐射
3.
The Observational Evidence of Microwave Pulsations with Very Long Periods in the Corona
日冕微波辐射甚长周期脉动的观测证据
4.
Day Mian side go up, even Xie have made curious brilliance, radiate outward , arise especially big light beam, astronomer name is " Mian flow ".
日冕的边上，甚至泻出了奇异的光彩，向外辐射，出现特大的光束，天文学家称之为“冕流”。
5.
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。
6.
radiative inelastic scattering cross section
辐射非弹性散射截面
7.
non-Fraunhofer component
非夫琅和费部分-日冕光谱
8.
normal direct solar irradiance
法向直接日射辐照度
9.
THE MONITOR OF THE CME IN MARCH 1991 BY COSMIC RAYS
银河宇宙线对1991年3月日冕物质抛射的监测
10.
Solar Radio Type Ⅱ Burst in the Corona and Interplanetary Medium
日冕和行星际空间中的太阳射电Ⅱ型爆发
11.
Studies on the Prediction Method for Geomagnetic Disturbances Caused by Coronal Mass Ejections;
日冕物质抛射引起的地磁扰动预报方法研究
12.
Observations on Coronal Mass Ejections and Its Associated Solar Activities
日冕物质抛射及相关太阳活动的观测研究
13.
Stray light analysis of internally occulted mirror coronagraph
反射式内掩日冕仪的光学设计与杂散光分析
14.
The rate of delivery of solar radiation per unit of horizontal surface.
日射能量单位水平面上日辐射的量
15.
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.
16.
Applied Analysis on the Model of Global Solar Radiation and Hourly Solar Radiation;
日总辐射及逐时辐射模型的适用性分析
17.
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。
18.
the coronation day, robes, coach
加冕日、 袍、 马车等.