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A CME and Related Phenomena on 2003 October 26

Published online by Cambridge University Press:  03 June 2005

Zongjun Ning ,
C. Fang ,
M. D. Ding ,
C.-T. Yeh ,
H. Li ,
Y. N Xu ,
Y. Zhang  and
C. M. Tan
Zongjun Ning
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: ningzongjun@hotmail.com
C. Fang
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: ningzongjun@hotmail.com
M. D. Ding
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: ningzongjun@hotmail.com
C.-T. Yeh
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: ningzongjun@hotmail.com
H. Li
Affiliation:
Purple Mountain Observatory, Nanjing 210008, China
Y. N Xu
Affiliation:
Purple Mountain Observatory, Nanjing 210008, China
Y. Zhang
Affiliation:
Chinese National Observatory, Beijing 100021, China
C. M. Tan
Affiliation:
Chinese National Observatory, Beijing 100021, China
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Abstract

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We present the observational results of the solar bursts on the band of 1-80 GHz (NORH) associated with both a CME and a flare on Oct. 26 2003. This event shows two parts of radio bursts in the time profile. The first part is associated with an X1.2 flare. However, the following part seams related to both the flare and the CME, as the radio emission is enhanced while the ${\rm H}\alpha$ is decreasing. Thus, these two parts of radio bursts may originate from different physical processes, i.e., flare and CME shock. A primary study is performed on the difference between this two parts.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: flaresCMEsradio radiation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 123 - 124
Copyright
© 2005 International Astronomical Union