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Detailed Reference Information |
Gopalswamy, N., Yashiro, S., Lara, A., Kaiser, M.L., Thompson, B.J., Gallagher, P.T. and Howard, R.A. (2003). Large solar energetic particle events of cycle 23: A global view. Geophysical Research Letters 30: doi: 10.1029/2002GL016435. issn: 0094-8276. |
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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. |
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Abstract |
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Keywords
Interplanetary Physics, Energetic particles, solar, Solar Physics, Astrophysics, and Astronomy, Coronal mass ejections, Solar Physics, Astrophysics, and Astronomy, Radio emissions, Solar Physics, Astrophysics, and Astronomy, Energetic particles |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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