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A solar flare scenario based on multi-wavelength observations

Published online by Cambridge University Press:  14 March 2005

W. Q. Gan ,
Y. P. Li ,
H. Li ,
X. F. Yu  and
Q. S. Du
W. Q. Gan
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: wqgan@pmo.ac.cn
Y. P. Li
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: wqgan@pmo.ac.cn
H. Li
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: wqgan@pmo.ac.cn
X. F. Yu
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: wqgan@pmo.ac.cn
Q. S. Du
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: wqgan@pmo.ac.cn
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The 1N/M7.6 flare of 24 October 2003 at S19E72 were well observed by RHESSI, TRACE, NORH, and the Spectrograph at the Purple Mountain Observatory. After analyzing all the data collected, we established a scenario of the flare and compared it with the standard cartoon of solar flares (e.g., Dennis 1988).To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 623 - 624
Copyright
© 2004 International Astronomical Union