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Investigating the Statistical Relationship between Coronal Mass Ejections and Solar Flares
Bulletin of the Russian Academy of Sciences: Physics Pub Date : 2021-04-29 , DOI: 10.3103/s1062873821030059 N. A. Barkhatov , V. G. Vorobjev , S. E. Revunov , E. A. Revunova
中文翻译:
研究日冕物质抛射与太阳耀斑之间的统计关系
更新日期:2021-04-29
Bulletin of the Russian Academy of Sciences: Physics Pub Date : 2021-04-29 , DOI: 10.3103/s1062873821030059 N. A. Barkhatov , V. G. Vorobjev , S. E. Revunov , E. A. Revunova
Abstract
An analysis is performed of the statistical relationship between coronal mass ejections and solar flares to establish the sequence of these events. Periods of delay in the occurrence of coronal mass ejections relative to the associated flare-like manifestations of solar activity are determined. It is found that situations in which flares occur several hours ahead of coronal ejections predominate.
中文翻译:
研究日冕物质抛射与太阳耀斑之间的统计关系
摘要
对日冕物质抛射与太阳耀斑之间的统计关系进行分析,以建立这些事件的顺序。确定相对于相关的太阳活动的耀斑状表现,冠状物质抛射发生的延迟时间。发现在冠状弹射之前几个小时发生耀斑的情况占主导。