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A Reconsideration of the Classification of Two Types of CMEs

Published online by Cambridge University Press:  03 June 2005

A.Q. Chen ,
C.T. Yeh ,
J.X. Cheng  and
P.F. Chen
A.Q. Chen
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: jdye@nju.edu.cn
C.T. Yeh
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: jdye@nju.edu.cn
J.X. Cheng
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: jdye@nju.edu.cn
P.F. Chen
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: jdye@nju.edu.cn
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Abstract

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Conventionally coronal mass ejections (CMEs) are categorized into flare-associated and filament-associated types. Since there are also many CMEs of the overlapping type, we classify CMEs into three types in order to compare their characteristics. It is found that the three types of CMEs have quite similar distributions of apparent speeds, with small difference in the average speeds.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: coronal mass ejections (CMEs)filamentflares
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 110 - 111
Copyright
© 2005 International Astronomical Union