太阳高能粒子事件强度与相关双CME事件关系的两个事例

陈旻昊; 陈玉林; 乐贵明; 陆阳平; 李仲怡; 尹志强

doi:10.11728/cjss2016.03.267

太阳高能粒子事件强度与相关双CME事件关系的两个事例

doi: 10.11728/cjss2016.03.267

1.
南京信息工程大学数学与统计学院南京 210044
2.
中国气象局空间天气重点实验室北京 100081
3.
中国气象局国家空间天气监测预警中心北京 100081
4.
中国科学院国家天文台北京 100012

详细信息

作者简介:
陈旻昊,E-mail:fireflycmh@foxmail.com

中图分类号: P353
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- 被引次数: 0
出版历程
- 收稿日期: 2015-03-25
- 修回日期: 2015-07-09
- 刊出日期: 2016-05-15

Dependence of the Intensity of Solar Energetic Particle Event on the Twin-CME:Two Cases Study

1.
School of Mathematics and Statistics, Nanjing University of Information Science and Technology, Nanjing 210044
2.
Key laboratory of Space Weather, China Meteorological Administration, Beijing 100081
3.
National Center for Space Weather, China Meteorological Administration, Beijing 100081
4.
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012

摘要

摘要: 太阳高能粒子事件常伴随太阳耀斑和日冕物质抛射事件(Coronal Mass Ejections,CME)出现,由于太阳高能粒子事件的关键因素是双CME的相互作用,利用SOHO卫星观测的高能粒子强度、耀斑强度以及CME的相对高度与时间,通过高度与时间拟合得到的速度,分析了2001年4月15日和2005年1月20日的太阳高能粒子事件强度与相关双CME事件的关系,发现这两个太阳高能粒子事件中E ≥ 10MeV质子的强度与双CME事件无关.因此在这两次太阳高能粒子事件早期,E ≥ 10MeV质子的强度只与相关太阳耀斑和CME有关.
- 太阳高能粒子事件 /
- 双CME事件 /
- 粒子加速
Abstract: Solar energetic particle events often associate with solar flare and Coronal Mass Ejection (CME).Because the interaction of twin-CME is the key factor of solar energetic particle events,by using the SOHO satellite observations of energetic particle strength,flare intensity and relative height and time of CMEs,and through the speed of height fitting,the relationship between the intensity of Solar Energetic Particle events (SEP) and the associated twin-CME is investigated.The two SEP occurred on 15 April 2001 and 20 January 2005 respectively.The results show that the intensities of the two SEP have no relationship with the associated twin-CME.The protons of E ≥ 10 MeV are only associated with the concurrent solar flare and CME.
- Solar energetic particle event /
- Twin-CMEs /
- Particle acceleration

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参考文献(7)

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