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Statistical analyses of Microwave type III bursts and CMEs

Published online by Cambridge University Press:  01 November 2006

Y. Ma ,
D. Y. Wang  and
Y. H. Yan
Y. Ma
Affiliation:
National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences Kunming, 650011, P.R. China email: mayuanf@yahoo.com.cn Present address: P.O.Box 110, Kunming, 650011, China
D. Y. Wang
Affiliation:
Purple Mountain Observatories, Chinese Academy of Sciences, 210008 Nanjing, P.R. China
Y. H. Yan
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, 100012 Beijing China
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Abstract

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The Statistics analyses of the microwave type III bursts, coronal mass ejections (CMEs), H$\alpha$flares and relevant events observed with 5200–7600 MHz spectrograph at the Chinese National Astronomical Observatory during the 23rd solar cycle are carried out in this article. Some significant results are obtained from the relevant events. The radiation mechanism of that is also discussed from the observation characteristics.

Keywords

Microwave type III burstsH$\alpha$ flaresCMEs
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S233: Solar Activity and its Magnetic Origin , March 2006 , pp. 187 - 188
Copyright
© 2006 International Astronomical Union