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CME Interaction and the Intensity of Solar Energetic Particle Events.

Authors :
Gopalswamy, N.
Yashiro, S.
Krucker, S.
Howard, R. A.
Source :
Proceedings of the International Astronomical Union; 10/15/2004, Vol. 2004 Issue IAUS226, p367-373, 7p
Publication Year :
2004

Abstract

Large Solar Energetic Particles (SEPs) are closely associated with coronal mass ejections (CMEs). The significant correlation observed between SEP intensity and CME speed has been considered as the evidence for such a close connection. The recent finding that SEP events with preceding wide CMEs are likely to have higher intensities compared to those without was attributed to the interaction of the CME-driven shocks with the preceding CMEs or with their aftermath. It is also possible that the intensity of SEPs may also be affected by the properties of the solar source region. In this study, we found that the active region area has no relation with the SEP intensity and CME speed, thus supporting the importance of CME interaction. However, there is a significant correlation between flare size and the active region area, which probably reflects the spatial scale of the flare phenomenon as compared to that of the CME-driven shock.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html [ABSTRACT FROM PUBLISHER]

Details

Language :
English
ISSN :
17439213
Volume :
2004
Issue :
IAUS226
Database :
Complementary Index
Journal :
Proceedings of the International Astronomical Union
Publication Type :
Academic Journal
Accession number :
57121106
Full Text :
https://doi.org/10.1017/S1743921305000876