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Measurments of Solar EUV fluxes on board the “CORONAS” satellites: equipment and main results

Published online by Cambridge University Press:  14 March 2005

T. V. Kazachevskaya ,
A. A. Nusinov ,
V. V. Katyushina  and
D. A. Gonyukh
T. V. Kazachevskaya
Affiliation:
Institute of Applied Geophysics, Russian Hydrometeorological Service, Moscow email:[email protected]
A. A. Nusinov
Affiliation:
Institute of Applied Geophysics, Russian Hydrometeorological Service, Moscow email:[email protected]
V. V. Katyushina
Affiliation:
Institute of Applied Geophysics, Russian Hydrometeorological Service, Moscow email:[email protected]
D. A. Gonyukh
Affiliation:
Special design bureau, Russian Hydrometeorological Service, Obninsk email:[email protected]
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The CORONAS project is aimed at observation of the Sun in the wide wave-range. The CORONAS-I satellite has been launched to an orbit on 2 March 1994, the CORONAS-F satellite has been launched on 31 July 2001 (see for example Kazachevskaya et al., 1998; Oraevsky et al., 2002). Solar Ultraviolet Radiometer — SUVR provides measurements in the wavelength region $\lambda < 130$ nm and also in the line $L_{\alpha}(\lambda = 121.6)$nm. (Kazachevskaya et al., 1998).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. 633 - 634
Copyright
© 2004 International Astronomical Union