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- 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。
- 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。
- 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
- Wang, S., Zhang, B. and Zheng, H. N. , 1993, Numerical simulation of propagation of disturbance in solar corona (III) Effects of solar wind, Chinese J. Space Sci., 13 , 81. 王水，张兵，郑惠南;1993，日冕扰动传播的数值模拟（III）太阳风的影响，空间科学学报，13;81.
- Zheng, H. 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.
- 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。
- In this composite view, SOHO's uninterrupted view of the solar corona above the solar photosphere (center) and corona far beyond the Sun's disk, are shown in orange hues. 在这张合成图像中，SOHO拍摄到了日冕的连续影像，上面太阳光球（中心）和太阳圆盘周围的日冕都显示在桔黄色的图像中。
- Magnetic reconnection caused by the resistance tearing instability in a current sheet of solar corona with two-dimensional magnetostatic equilibrium in the spherical coordinate has been studied numerically. 本文在球坐标二维磁静力平衡基态下，数值研究了电阻撕裂模不稳定性引起日冕电流片中发生磁场重联的过程。
- Based on a combination of analytical and numerical methods,two-dimensional magneto-hydrodynamic equilibria in the non-uniform gravitational field for the solar corona are discussed. 基于解析和数值相结合的方法,进一步讨论了非均匀引力场中日冕的二维磁流体动力学平衡。
- From the significance of the observation and research of the solar corona, the necessity of setting up the observation of the solar corona at the Yunnan Observatory is explained in this present article. 本文从日冕观测和研究的意义出发,说明云南天文台建立日冕观测的必要性。
- In this paper, the dynamical response under the basic state with two-dimensional magne-tohydrodynamic equilibrium in the solar corona caused by the radial ejection of cold mass at the solar surface of the open magnetic field is studied numerically. 本文数值研究了二维磁流体动力学平衡基态下开场区日面冷物质径向喷射所引起的日冕动力学响应。
- Analysis and calculations show that the energy densities of different structure in the solar corona can be measured quantitatively and directly by the method,and the results are more accurate than the filter ratio method. 分析和计算表明,使用“物理参数”法能直接定量测定太阳日冕不同结构物的热能密度。 而且,“物理参数”法比传统的“滤光片比”法精确。
- radio wave scattering of the solar corona 日冕的电波散射
- THE PLASMA WAKE FIELD BY SOLAR HIGHENERGY ELECTRONS IN SOLAR CORONA 日冕背景下的等离子体尾场效应
- Solar energy is a new kind of source of energy. 太阳能是一种新型能源。
- We can use solar energy to do many things today. 如今，我们可以利用太阳能做很多事情。
- They accurately predicted solar eclipses. 他们精确地预告了日蚀。
- The solar system was formed 4.5 billion years ago. 太阳系是四十五亿年前形成的。
- He gave a lecture on the use of solar energy. 他就太阳能的利用作了一场讲演。
- A mechanical model of the solar system. 太阳系仪太阳系的机械模型
