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Study of Filament Eruption and its Relationship to a CME on 2003 August 25

Published online by Cambridge University Press:  03 June 2005

H. D. Chen ,
Y. C. Jiang ,
Q. Y. Li  and
S. Q. Zhao
H. D. Chen
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: hdchen@ynao.ac.cn
Y. C. Jiang
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: hdchen@ynao.ac.cn
Q. Y. Li
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: hdchen@ynao.ac.cn
S. Q. Zhao
Affiliation:
National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China email: hdchen@ynao.ac.cn
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Abstract

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By means of multiwavelength data, we study the eruptions of two filaments and the relationship between the first filament eruption and a subsequent CME. The main results are: (1) The disturbances of the two filaments showed different features, indicating that their eruptive mechanisms were possibly different. (2) A subsequent CME was well correlated with the first eruption in both time and space.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: activitycoronal mass ejections (CMEs)filamentsflares
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 209 - 210
Copyright
© 2005 International Astronomical Union