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Multi-Wavelength Radio Features Associated with Large CMEs on Oct. 26–28, 2003

Published online by Cambridge University Press:  03 June 2005

S. J. Wang ,
Y. Yan ,
Q. Fu ,
Y. Liu  and
Z. Chen
S. J. Wang
Affiliation:
National Astronomical Observatories of China, Beijing 100012, China email: wsj@bao.ac.cn
Y. Yan
Affiliation:
National Astronomical Observatories of China, Beijing 100012, China email: wsj@bao.ac.cn
Q. Fu
Affiliation:
National Astronomical Observatories of China, Beijing 100012, China email: wsj@bao.ac.cn
Y. Liu
Affiliation:
National Astronomical Observatories of China, Beijing 100012, China email: wsj@bao.ac.cn
Z. Chen
Affiliation:
National Astronomical Observatories of China, Beijing 100012, China email: wsj@bao.ac.cn
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Abstract

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We study in focus to the multi-wavelength radio spectra associated with quite strong CME events observed in the time interval of October 26–28, 2003. Using multi-wavelength observations recorded by WIND/WAVES experiment, Learmouth Spectrograph (Australian), PHOENIX-2 (Switzerland), Hiraiso (Japan), DAM/Nançay (France), Izmiran (Russia) and Huairou/NAOC (China), an analyzing of radio bursts was performed for the those events over a large coronal region across the microwave, the decimetric wavelength, the metric wavelength and even to much longer wavelength. The composite spectra indicate there were many complicated structures of radio bursts, including type II bursts, type IV bursts, type III bursts, drifting pulsation structures (DPS) and many radio fine structures (FS).To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: coronal mass ejections (CMEs)radio radiation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 139 - 140
Copyright
© 2005 International Astronomical Union