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EUV and X-Ray Solar Flares Observed on-board the “Coronas-F” Satellite

Published online by Cambridge University Press:  14 March 2005

A. A. Nusinov ,
T. V. Kazachevskaya  and
V. V. Katyushina
A. A. Nusinov
Affiliation:
Institute of Applied Geophysics, Russian Hydrometeorological Service, Moscow email: geophys@hydromet.ru
T. V. Kazachevskaya
Affiliation:
Institute of Applied Geophysics, Russian Hydrometeorological Service, Moscow email: geophys@hydromet.ru
V. V. Katyushina
Affiliation:
Institute of Applied Geophysics, Russian Hydrometeorological Service, Moscow email: geophys@hydromet.ru
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The CORONAS-F satellite has been launched on 31 July 2001 (Oraevsky et al. 2002). To conduct measurements of the intensity of solar radiation in the EUV spectral region near the hydrogen line $L_{\alpha}(\lambda = 121.6$ nm) the spectrophotometer VUSS was installed onboard CORONAS-F. A vacuum photodiode was used as EUV detector in VUSS with the $CuJ$ cathode and $MgF_2$ entrance window.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. 475 - 476
Copyright
© 2004 International Astronomical Union