The extreme-ultraviolet spectrum (300-630 Å) of an erupting prominence observed from Skylab
The extreme-ultraviolet spectrum (300-630 Å) of an erupting prominence observed from Skylab
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DOI：
10.1086/164566
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发表时间：
1986-09
期刊：
影响因子：
--
通讯作者：
K. Widing;U. Feldman;A. Bhatia
中科院分区：
文献类型：
--
作者：
K. Widing;U. Feldman;A. Bhatia
Skylab 300-630 A 拍摄的 1974 年 1 月 17 日喷发喷雾事件的图像表明，在最初 22 分钟内，输入拱门的能量一直保持不变，并伴有向上运动和加热。根据获得的光谱，可以得出拱门几乎伸直的腿的最亮部分的热特性。给出了在 100,000 至 1,000,000 K 温度之间形成的约 90 条发射线的波长、标识和强度。获得的发射测量图与在安静太阳下观察到的那些图相似。
The Skylab 300-630 A images of the January 17, 1974 eruptive spray event imply that the energy input to the arch was maintained during the first 22 min, accompanied by upward motion and heating. From the spectrum obtained, thermal properties are derived for the brightest portion of the nearly straightened leg of the arch. Wavelengths, identifications and intensities are presented for about 90 emission lines formed at temperatures between 100,000 and 1,000,000 K. The emission measure plot obtained is similar to those plots observed for the quiet sun.