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Microwave Fine Structures in the Initial Phase of Solar Flares and CMEs

Published online by Cambridge University Press:  03 June 2005

C.M Tan ,
Y.H. Yan ,
Q.J. Fu ,
Y.Y. Liu ,
H.R. Ji  and
Z.J. Chen
C.M Tan
Affiliation:
National Astronomical Observatories Chinese Academy of Sciences, Beijing 100012, China email: Tanchm@bao.ac.cn
Y.H. Yan
Affiliation:
National Astronomical Observatories Chinese Academy of Sciences, Beijing 100012, China email: Tanchm@bao.ac.cn
Q.J. Fu
Affiliation:
National Astronomical Observatories Chinese Academy of Sciences, Beijing 100012, China email: Tanchm@bao.ac.cn
Y.Y. Liu
Affiliation:
National Astronomical Observatories Chinese Academy of Sciences, Beijing 100012, China email: Tanchm@bao.ac.cn
H.R. Ji
Affiliation:
National Astronomical Observatories Chinese Academy of Sciences, Beijing 100012, China email: Tanchm@bao.ac.cn
Z.J. Chen
Affiliation:
National Astronomical Observatories Chinese Academy of Sciences, Beijing 100012, China email: Tanchm@bao.ac.cn
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Abstract

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Solar radio fine structures (FSs) may be as an important diagnostics stool to draw the evolution map of the flare loop in the initial phase of solar flares. Also, it may be an important signature of the initial phase of CMEs. Here we analyzed a series of solar radio bursts with drift pulsation structures (DPS) and FSs during the former part of the 23rd solar activity cycle. Found they were associated with CMEs, and got some important statistic conclusions.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: coronal mass ejections (CMEs)flaresradio radiation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 131 - 132
Copyright
© 2005 International Astronomical Union