After analyzing the records of "er"(solar ear jade)in Chinese annals,and textual researching the meanings of "er" and the origin of modern terms "solar prominences" and "parhelion",this paper concludes that the records of so-called celestial phenomena "er" are atmospheric optical phenomena—parhelion,and the modern terms "solar prominences" are borrowed from ancient terms.
现代术语"日珥"是对古代术语的转义借用,历史典籍中的"珥"记载皆非太阳日珥。
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
Computing the Coronal Temperature by Using the Filter Ratio Method;
用Filter Ratio方法计算太阳日冕温度
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。
intermediate corona
中介日冕-中等太阳活动时的日冕
THE GREEN CORONAL LINE ABOVE ACTIVE REGION AT SOLAR LIMB ON 5 AUG. OF 1989
1989年8月5日太阳边缘活动区之上的绿日冕线
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
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
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
One other interesting aspect of the relation of coronal holes to the solar wind follows from the appearance of coronal holes at the poles.
日冕洞与太阳风的关系的另一个有趣的方面是日冕洞在两极的形状。
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。
The luminous, irregular envelope of highly ionized gas outside the chromosphere of the sun.
日冕太阳色球层外的高电离气体所形成的发光的、不规则的环
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。
The necessary exposure time for corona at different solar radius is estimated as well.
文章还估计了拍摄不同太阳半径上日冕所需的曝光时间.
The Heat-Engine Effect of the Material Exchange in Solar Super Atmosphere--The Model of the Chromosphere-Corona Transition Region
太阳高层大气物质交换的热机效应——色球-日冕过渡区模型
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。
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。
The excess energy goes into creating and accelerating a high-speed solar wind that emanates primarily from the regions of the holes.
多余的能量用来产生并加速高速的太阳风，而太阳风主要发端于日冕洞区域。
Solar radio burst on metric wavelengths, which is associated with solar flare, is a phenomenon in the corona above solar active regions.
太阳米波射电爆发是活动区上空日冕中的现象,与太阳耀斑有密切关系。