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MULTI-TEMPERATURE STRUCTURE OF THE SOLAR CORONA OBSERVED BY YOHKOH AND SOHO

机译:Yohkoh和Soho观察到太阳能电晕的多温度

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The relationship between higher-temperature (T > 2 MK) coronal loops seen with Yohkoh SXT and lower-temperature (~ 1 MK) loops seen with SOHO EIT is discussed. Hot and cool loops are not co-spatial, and their observed lifetime is much longer then the estimated cooling timescales. This suggests that each loop has its own destined heating rate, and that there are high heating-rate loops and low heating-rate (dormant) loops.
机译:讨论了用Yohkoh SXT看到的高温(T> 2 MK)冠状环之间的关系,并用SOHO EIT看到的较低温度(〜1 mk)环。热凉爽的环路不合适,并且其观察到的寿命长得多于估计的冷却时间尺寸。这表明每个环路都有其目的地加热速率,并且有很高的加热速率环和低热速率(休眠)环。

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