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Factors Affecting The Intensity of Solar Energetic Particle Events

机译:影响太阳能粒子事件强度的因素

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This paper updates the influence of environmental and source factors of shocks driven by coronal mass ejections (CMEs) that are likely to influence the solar energetic particle (SEP) events. The intensity variation due to CME interaction reported in [1] is confirmed by expanding the investigation to all the large SEP events of solar cycle 23. The large SEP events are separated into two groups, one associated with CMEs running into other CMEs, and the other with CMEs running into the ambient solar wind. SEP events with CME interaction generally have a higher intensity. New possibilities such as the influence of coronal holes on the SEP intensity are also discussed. For example, the presence of a large coronal hole between a well-connected eruption and the solar disk center may render the shock poorly connected because of the interaction between the CME and the coronal hole. This point is illustrated using the 2004 December 3 SEP event delayed by about 12 hours from the onset of the associated CME. There is no other event at the Sun that can be associated with the SEP onset. This event is consistent with the possibility that the coronal hole interaction influences the connectivity of the CMEs that produce SEPs, and hence the intensity of the SEP event.
机译:本文更新了可能影响太阳能粒子(SEP)事件的冠状大规模喷射(CMES)驱动的冲击的环境和源极因素的影响。通过在[1]中报告的CME交互引起的强度变化通过扩展对太阳循环23的所有大型SEP事件的调查来确认。大的SEP事件分为两组,与CME一起运行到其他CME中,以及其他与CMES跑进环境太阳风。具有CME交互的SEP事件通常具有更高的强度。还讨论了新的可能性,例如冠状孔对SEP强度的影响。例如,由于CME和冠状孔之间的相互作用,在连接良好连接的喷发和太阳能盘中心之间的大冠孔的存在可能使震动不良。使用2004年12月3日第3个SEP事件从相关联的CME的开始延迟约12小时来说明这一点。太阳中没有其他事件可以与SEP发作相关联。此事件与冠状孔交互影响产生产生SEPS的CME的连接的可能性一致,因此SEP事件的强度。

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