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Occurrence of Solar Radio Burst Fine Structures in 1–7.6 GHz Range Associated with CME Events

Published online by Cambridge University Press:  03 June 2005

Yihua Yan
Affiliation:
National Astronomical Obsevatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100012, China email: [email protected]
Yuying Liu
Affiliation:
National Astronomical Obsevatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100012, China email: [email protected]
Zhijun Chen
Affiliation:
National Astronomical Obsevatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100012, China email: [email protected]
Qijun Fu
Affiliation:
National Astronomical Obsevatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100012, China email: [email protected]
Chengming Tan
Affiliation:
National Astronomical Obsevatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100012, China email: [email protected]
Shujuan Wang
Affiliation:
National Astronomical Obsevatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100012, China email: [email protected]
Jian Zhang
Affiliation:
National Astronomical Obsevatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100012, China email: [email protected] Dept of Astronomy, Beijing University, Beijing, China
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Abstract

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The solar radio bursts and accompanying fine structures recorded by spectrometers at Huairou, Beijing during 1999-2003 are presented. The spectrometers are with high temporal (5-10 ms) and spectral (4-20 MHz) resolutions. We found 91 radio burst events that occurred within half hour of the onset of the CME events which cause solar energetic particle events. The associations of radio fine structures with CME events are discussed.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Copyright
© 2005 International Astronomical Union