solar corona

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。

On the Transport of Magnetic Energy and Complexity to the Solar Corona

磁能和磁复杂性向日冕的传输

A Theorem on the Steady Magnetohydrodynamic Flows in the Solar Corona

关于日冕中稳恒态磁流体力学流动的一个定理

There are two approaches in the research of the effect of Alfven waves in solar corona and solar wind .

具体研究阿尔芬波如何在日冕与太阳风中起作用，主要从两方面入手。

Polarimetry of the Solar Corona at the 1997 March 9 Eclipse

1997年3月9日的日冕偏振CCD观测

An Interpretation of Rapid Frequency Drift and Polarization Sense Reversals by Radio Wave Propagation in the Solar Corona

太阳射电快速频漂和偏振逆转波的传播解释

Two-dimensional magnetohydrodynamic equilibria in the solar corona ( ii )

二维磁流体动力学平衡日冕（Ⅱ）

The exploration of bidirectional electron beams originating in the solar corona with pairs of type ⅲ radio bursts

由对偶的Ⅲ型射电爆发观测探讨日冕双向电子束的起源问题

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。

Despite thin clouds , it captures the shimmering solar corona just before the end of the eclipse total phase .

尽管薄云片片，图片仍然捕捉到了日全食接近尾声时的日冕。

Once at the solar corona , where the sun 's magnetic field is strong , the axions would convert back into photons .

一旦到达太阳磁场强烈的日冕处，这些轴子又会转变为光子。

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。

A theorem and an important relation on the steady magnetohydrodynamic flows flowing along the magnetic field lines in the solar corona or other astrophysical circumstances are reported ;

本文报告了在日冕或其他天体物理环境中，沿磁力线流动的稳恒态磁流体力学流动的一个定理和一个重要关系。

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。

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。

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。

A lovely solar corona and bright inner planets Mercury and Venus emerged during the total eclipse phase , while the flickering view screens of eclipse watchers'digital cameras dotted the landscape .

影像中，除了可见到美丽的日冕以及水星和金星这两颗内行星之外，日食观赏者的数位相机闪烁之视景窗妆点著地面的原野。

Ion-cyclotron-resonance heating mechanism of the hely ions in lower solar polar corona

太阳极区低日冕重离子的回旋波加热机制

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。

Acoustic waves are a primary candidate for supplying the energy necessary to heat the solar chromosphere and corona .

声波是供给太阳色球和日冕加热所需能量的主要候选能源。

Magnetic reconnection plays a very important role in solar flares , corona mass ejections ( CME ), and other solar activities .

在太阳耀斑、日冕物质抛射（CME）和其他太阳活动现象中，磁重联一直都扮演着至关重要的作用。

The gas pressure eventually overcomes the force of solar gravity and the corona inevitably expands into space as the solar wind .

这里的气体压强最终会超过太阳的引力作用，使日冕终于只好以太阳风的形式向空间膨胀。

Electrostatic instability excited by solar flare electron beams in solar corona

太阳耀斑电子束在日冕区产生的静电不稳定性

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。

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。