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Solar flares observed by AVS-F instrument onboard CORONAS-F satellite during 2,5 year of it's operation

Published online by Cambridge University Press:  14 March 2005

Andrew Arkhangelsky
Affiliation:
Astrophysics Institute, Moscow State Engineering Physics Institute (State University) Kashirskoe shosse 31, Moscow, 115409 Russia email: [email protected]
I. V. Arkhangelskaja
Affiliation:
Astrophysics Institute, Moscow State Engineering Physics Institute (State University) Kashirskoe shosse 31, Moscow, 115409 Russia email: [email protected]
Yu. D. Kotov
Affiliation:
Astrophysics Institute, Moscow State Engineering Physics Institute (State University) Kashirskoe shosse 31, Moscow, 115409 Russia email: [email protected]
A.S Glyaneneko
Affiliation:
Astrophysics Institute, Moscow State Engineering Physics Institute (State University) Kashirskoe shosse 31, Moscow, 115409 Russia email: [email protected]
S. N. Kuznetsov
Affiliation:
Scobeltsyn Institute of Nuclear Physics, Moscow State University, 119899 Russia email:[email protected]
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Abstract

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AVS-F instrument (Amplitude-Time Spectrometry of the Sun) is the system of an electronics engineering for onboard data gathering from two detectors: scintillation (CsI (Tl)) detector SONG-D (SOlar Neutrons and Gamma quantums) of complex of detectors SKL (in low and high gamma-band) and from semiconducting detector (X-ray semiconducting spectrometer) XSS-1 (in X-ray band). The experiment is carried out on the satellite CORONAS-F launched on July 31 2001. During more than 2,5 year of apparatus operation more than 30 of solar flares were detected. Characteristics of observed solar flares are presented in this article.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Copyright
© 2004 International Astronomical Union