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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
Affiliation:
National Astronomical Observatories of China, Beijing 100012, China email: [email protected]
Y. Yan
Affiliation:
National Astronomical Observatories of China, Beijing 100012, China email: [email protected]
Q. Fu
Affiliation:
National Astronomical Observatories of China, Beijing 100012, China email: [email protected]
Y. Liu
Affiliation:
National Astronomical Observatories of China, Beijing 100012, China email: [email protected]
Z. Chen
Affiliation:
National Astronomical Observatories of China, Beijing 100012, China email: [email protected]
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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

Type
Contributed Papers
Copyright
© 2005 International Astronomical Union