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Diagnostics of Coronal Magnetic Field in Terms of Radio Burst and Fine Structures

Published online by Cambridge University Press:  03 June 2005

M. Wang ,
C. Xu ,
R. X. Xie  and
Y. H. Yan
M. Wang
Affiliation:
National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China (email: wmynao@163.net) Present address: PO Box 650011, Kunming, Yunnan, China.
C. Xu
Affiliation:
National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China (email: wmynao@163.net)
R. X. Xie
Affiliation:
National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China (email: wmynao@163.net)
Y. H. Yan
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
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Abstract

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A complex solar radio burst was observed on 19 October 2001 with the spectrometers of NAOC (National Astronomical Observatory of China) and Nobeyama Radioheliograph (NoRH). Basing on the analysis of brightness temperature spectra of radio sources and various fine spectral structures, we get a diagnosis of magnetic field of radio active region.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: coronal mass ejections (CMEs)magnetic fieldsradio radiation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 137 - 138
Copyright
© 2005 International Astronomical Union