2021年10月28日地面增强事件中重离子组成的纵向依赖性

C. M. S. Cohen, G. M. Mason, E. R. Christian, A. C. Cummings, G. A. de Nolfo, M. I. Desai, J. Giacalone, M. E. Hill, A. W. Labrador, R. A. Leske, D. J. McComas, R. L. McNutt Jr, D. G. Mitchell, J. G. Mitchell, G. D. Muro, J. S. Rankin, N. A. Schwadron, M. M. Shen, M. E. Wiedenbeck, Z. G. Xu, G. C. Ho and R. F. Wimmer-Schweingrüber
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摘要

2021年10月28日的太阳高能粒子(SEP)事件是一次罕见的地面增强(GLE)事件,地面上的中子监测仪探测到了SEP与地球大气相互作用产生的二次粒子。许多论文研究了该事件的太阳特征、中子监测观测以及SEP质子和电子的特征。在这里,我们描述了重离子的特征,特别是O和Fe,由多个航天器观测到。帕克太阳探测器、超前日地关系天文台和高级成分探测器分布在太阳经度近60°和日心距离0.4 au的位置。尽管它们是分离的,但所有三个航天器都测量了事件积分的O和Fe光谱,很好地用幂律表示,幂律指数几乎相同,约为- 1.7,这比大多数大型SEP事件和许多GLE事件要困难得多。此外,由这些光谱确定的Fe/O丰度比也发现在经度60°和日心距离0.4 au范围内具有空间不变性。这种近乎一致的现象是非常不寻常的,在之前的多航天器中只发现过一次类似的现象。观察到的Fe/O比率为0.39,高于大型SEP事件的典型比率,但对于GLE事件来说并不罕见。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Longitudinal Dependence of Heavy Ion Composition in the 2021 October 28 Ground Level Enhancement Event
The 2021 October 28 solar energetic particle (SEP) event was a rare ground level enhancement (GLE) event, where secondary particles from the interactions of SEPs with the Earth’s atmosphere were detected by neutron monitors on the ground. A number of papers have examined the solar signatures, neutron monitor observations, and the characteristics of the SEP protons and electrons for this event. Here we describe the heavy ion signatures, specifically O and Fe, observed by multiple spacecraft. Parker Solar Probe, Solar Terrestrial Relations Observatory-Ahead, and Advanced Composition Explorer were distributed over nearly 60° in solar longitude and 0.4 au in heliocentric distance. Despite their separations, all three spacecraft measured event-integrated O and Fe spectra, well represented by power laws, with nearly the same power-law index of approximately −1.7, which is significantly harder than most large SEP events and many GLE events. Moreover, the Fe/O abundance ratio determined from these spectra was also found to be spatially invariant over the 60° in longitude and 0.4 au in heliocentric distance. Such near uniformity is highly unusual, and only one similar occurrence was found in a previous multispacecraft. The observed Fe/O ratio of 0.39 is higher than typical for large SEP events but not unusual for GLE events.
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