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Observations of systematic temporal evolution in elemental composition during gradual solar energetic particle events

机译:逐渐的太阳高能粒子事件期间元素组成的系统时间演化的观察

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摘要

The WIND/EPACT experiment offers a approximately 100 fold increase in collecting power over instruments flown in previous solar cycles, thus allowing unprecedented detailed studies of temporal evolution in gradual solar energetic particle (SEP) events. We present hourly WIND/EPACT observations at approximately 2-10 MeVuc from the 20 April 1998 and 26 August 1998 SEP events. These observations show striking patterns in elemental composition which evolve in a systematic fashion throughout the events' several-day durations. These data, combined with theoretical modeling in a companion Letter, suggest that a dynamic Alfven wave field, generated primarily by streaming energetic protons, is responsible for the complex behavior which is observed.
机译:WIND / EPACT实验的收集功率比以前的太阳周期飞行的仪器提高了约100倍,因此可以对渐进式太阳高能粒子(SEP)事件的时间演化进行前所未有的详细研究。从1998年4月20日和1998年8月26日的SEP事件开始,我们大约每小时以2-10 MeV / nuc的速度进行WIND / EPACT观测。这些观察结果显示了元素组成的惊人模式,这些模式在事件的几天持续时间内以系统的方式演变。这些数据,再加上伴随的Letter中的理论模型,表明主要由流动的高能质子产生的动态Alfven波场负责观察到的复杂行为。

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