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Statistical studies of duration of low-power solar flares

机译:低功率太阳耀斑持续时间的统计研究

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This paper is a sequel to papers dealing with time parameters of solar flares in the Hα line. Using data from the international flare patrol for 1972–2010, we have determined the mean duration of flares of different importance and classes of area. We have established that 94.6 % of flares last more than 60 min. The duration of 90 % of flares with min is 2.1–3.3 hrs. In rare cases, flares can last about 12 hrs. The duration of powerful solar flares does not exceed 8.3 hrs.We have found that the duration of solar flares depends on features of their development. Flares with one brilliant point in the flare region have the shortest duration; two-ribbon flares and flares exhibiting several intensity maxima have the longest duration. We have confirmed that the duration of flares increases with increasing classes of area and brightness.
机译:本文是处理Hα线中太阳耀斑的时间参数的论文的续篇。利用国际照明巡逻队1972-2010年的数据,我们确定了不同重要性和区域类别的平均耀斑持续时间。我们确定94.6%的耀斑持续超过60分钟。 90%的耀斑持续时间为2.1-3.3小时。在极少数情况下,耀斑可能会持续约12小时。太阳耀斑的持续时间不超过8.3小时,我们发现太阳耀斑的持续时间取决于它们的发展特征。耀斑区域中具有亮点的耀斑持续时间最短;两个功能区的耀斑和表现出最大强度的耀斑的持续时间最长。我们已经证实,耀斑的持续时间随着面积和亮度类别的增加而增加。

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