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The investigation of the spectra of solar events observed in October-November 2003.

Published online by Cambridge University Press:  14 March 2005

Irene V. Arkhangelskyaja ,
A.I. Arkhangelsky ,
Yu. D. Kotov  and
S. N. Kuznetsov
Irene V. Arkhangelskyaja
Affiliation:
Astrophysics Institute, Moscow State Engineering Physics Institute (State University) Kashirskoe shosse 31, Moscow, 115409 Russia email: irene.belousova@usa.net
A.I. Arkhangelsky
Affiliation:
Astrophysics Institute, Moscow State Engineering Physics Institute (State University) Kashirskoe shosse 31, Moscow, 115409 Russia email: irene.belousova@usa.net
Yu. D. Kotov
Affiliation:
Astrophysics Institute, Moscow State Engineering Physics Institute (State University) Kashirskoe shosse 31, Moscow, 115409 Russia email: irene.belousova@usa.net
S. N. Kuznetsov
Affiliation:
Scobeltsyn Institute of Nuclear Physics, Moscow State University, 119899 Russia
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Abstract

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More than 30 active regions were observed on the Sun during October-November 2003 by SOHO. Approximately half of such regions induced hard X-ray and $\gamma$-ray emission and some solar flares with class M and X were detected during this time by GOES, RHESSI and other experiments. 5 solar flares were detected by AVS-F instrument onboard CORONAS-F satellite. Nuclear $\gamma$-emission lines were detected during some flares observed in this period, in particular, during all flares on October 29 2003.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. 439 - 440
Copyright
© 2004 International Astronomical Union