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Large solar flares of October-November, 2003-development in Soft X-ray, Hard X-ray and gamma-ray emissions

Published online by Cambridge University Press:  14 March 2005

Sergey N. Kuznetsov ,
V. G. Kurt ,
I. N. Myagkova ,
B. Yu. Yushkov  and
K. Kudela
Sergey N. Kuznetsov
Affiliation:
Skobeltsyn Institute of Nuclear Physics, Moscow State University, Russia email: kuznets@srd.sinp.msu.ru
V. G. Kurt
Affiliation:
Skobeltsyn Institute of Nuclear Physics, Moscow State University, Russia email: kuznets@srd.sinp.msu.ru
I. N. Myagkova
Affiliation:
Skobeltsyn Institute of Nuclear Physics, Moscow State University, Russia email: kuznets@srd.sinp.msu.ru
B. Yu. Yushkov
Affiliation:
Skobeltsyn Institute of Nuclear Physics, Moscow State University, Russia email: kuznets@srd.sinp.msu.ru
K. Kudela
Affiliation:
Institute of Experimental Physics, Slovak Academia of Science, Slovakia email: kkudela@upjs.kosice.sk.ru
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Abstract

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The description of two major flares detected by SONG spectrometer on board the CORONAS-F mission during famous period of solar activity in October- November 2003 and their comparison with soft X-ray measured by GOES-12 is given.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. 467 - 468
Copyright
© 2004 International Astronomical Union