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What can we learn from the intensity-time profiles of large gradual solar energetic particle events?

机译:我们可以从大型渐进的太阳高能粒子事件的强度-时间剖面中学到什么?

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摘要

Large gradual solar energetic particle events (LGSEPEs, 0pfu in the >10MeV channel as measured by GOES) are closely associated with coronal mass ejections (CMEs). The intensity-time profile of a LGSEPE reveals important information on the moving directions of a CME or an interplanetary CME (ICME). This paper analyzes the moving directions of ICMEs, using the intensity-time profiles of 3 typical solar energetic particle events, and the statistical results are presented.
机译:大型渐进式太阳高能粒子事件(LGSEPEs,GOES测得> 10MeV通道中的0pfu)与日冕物质抛射(CME)密切相关。 LGSEPE的强度-时间剖面揭示了有关CME或行星际CME(ICME)运动方向的重要信息。本文利用3个典型的太阳高能粒子事件的强度-时间剖面分析了ICMEs的运动方向,并给出了统计结果。

著录项

  • 来源
  • 会议地点 Beijing(CN)
  • 作者单位

    National Center for Space Weather China Meteorological Administration 100081 Institute of High Energy Physics Chines Academy of Sciences 100049 Department of Astronomy Nanjing University Nanjing China 210039;

    Department of Astronomy Nanjing University Nanjing China 210039;

    University of Chinese Academy of Sciences Beijing 100049 China;

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  • 原文格式 PDF
  • 正文语种
  • 中图分类
  • 关键词

    CME; LGSEPEs; geomagnetic storm;

    机译:芝商所LGSEPE;地磁风暴;

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