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Source Regions of Major Solar Energetic Particle Events

机译:主要太阳能粒子事件的源区

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We examine the source regions of the largest prompt solar energetic particle (SEP) events (J_(proton)[>10 MeV] >100 pr/cm~2/s/sr) occurring between 1992 and 2002.We find that the 25 such events originated in a broad spectrum of solar regions,ranging from large complex active regions with delta sunspot groups (e.g.,30 October 1992) to a very weak active region in which the major feature was a large filament that erupted to produce the SEP event (12 September 2000).Most source regions are less than two rotation old.In terms of recent work to identify two types of large SEP events on the basis of composition,spectra,and charge state,we find that large complex active regions can give rise to both types,whereas simple and magnetically weak regions are preferentially linked to one type.
机译:我们检查1992年至2002年之间发生的最大提示太阳能粒子(SEP)事件(J_(质子)[> 10 mev]> 100 Pr / cm〜2 / sr)。我们发现25个事件起源于广泛的太阳能区域,从大型复杂活跃区域,三角洲太阳黑子群(例如,1992年10月30日)到一个非常薄弱的​​活性区域,其中主要特征是产生生产SEP事件的大灯丝( 2000年9月12日)。大多数源地区旧的次旋转。最近的工作条款在组成,光谱和充电状态的基础上识别两种类型的大型SEP事件,我们发现大型复杂的活跃区域可以产生两种类型,而简单且磁弱的区域优先链接到一种类型。

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