Large solar energetic particle events of cycle 23: A global view

被引:93
作者
Gopalswamy, N
Yashiro, S
Lara, A
Kaiser, ML
Thompson, BJ
Gallagher, PT
Howard, RA
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Catholic Univ Amer, Dept Phys, Inst Astrophys & Computat Sci, Washington, DC 20064 USA
[3] Univ Nacl Autonoma Mexico, Inst Geofis, Mexico City 04510, DF, Mexico
[4] L3 Com Anal Corp, Greenbelt, MD USA
[5] USN, Res Lab, Solar Phys Branch, Div Space Sci, Washington, DC 20375 USA
关键词
D O I
10.1029/2002GL016435
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
[1] We report on a study of all the large solar energetic particle (SEP) events that occurred during the minimum to maximum interval of solar cycle 23. The main results are: 1. The occurrence rate of the SEP events, long-wavelength type II bursts and the fast and wide frontside western hemispheric CMEs is quite similar, consistent with the scenario that CME-driven shocks accelerate both protons and electrons; major flares have a much higher rate. 2. The SEP intensity is better correlated with the CME speed than with the X-ray flare class. 3. CMEs associated with high-intensity SEPs are about 4 times more likely to be preceded by wide CMEs from the same solar source region, suggesting the importance of the preconditioning of the eruption region. We use a specific event to demonstrate that preceding eruption from a nearby source can significantly affect the properties of SEPs and type II radio bursts.
引用
收藏
页码:SEP3 / 1
页数:4
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