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A review of the solar results from CORONAS-F satellite

Published online by Cambridge University Press:  14 March 2005

V.D. Kuznetsov ,
Yu.E Charikov ,
Yu.D. Kotov ,
S.N. Kuznetsov ,
E.P. Mazets ,
A.A. Nusinov ,
V.M. Pankov ,
I.I. Sobelman  and
J. Sylwester
V.D. Kuznetsov
Affiliation:
Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, 142190, Moscow Region, Troitsk, IZMIRAN, Russia, e-mail: [email protected]
Yu.E Charikov
Affiliation:
Ioffe Institute of Physics and Technology, Russian Academy of Sciences, 194021, St-Petersburg, Politechnicheskaya str. 26, Russia; e-mail: [email protected]; [email protected]
Yu.D. Kotov
Affiliation:
Moscow Physical Engineering Institute, 115409, Koshirskoe shosse 31, Moscow, Russia, e-mail: [email protected]
S.N. Kuznetsov
Affiliation:
Research Institute of Nuclear Physics, Moscow State University, 119899 Vorob'evi Gory, Moscow, Russia, e-mail: [email protected]
E.P. Mazets
Affiliation:
Ioffe Institute of Physics and Technology, Russian Academy of Sciences, 194021, St-Petersburg, Politechnicheskaya str. 26, Russia; e-mail: [email protected]; [email protected]
A.A. Nusinov
Affiliation:
Institute of Applied Geophysics, Russian Committee for Hydrometeorology, 129128, Moscow, Rostokinskaya str. 9, Russia, e-mail: [email protected]
V.M. Pankov
Affiliation:
Space Research Institute, Russian Academy of Sciences, 117997, Moscow, Profsoyznaya str. 84/32, e-mail: [email protected]
I.I. Sobelman
Affiliation:
Lebedev Physical Institute, 117997, Moscow, Leninsky prospekt 53, Russia, e-mail: [email protected]
J. Sylwester
Affiliation:
Space Research Centre, Polish Academy of Sciences, 51-622, Kopernika 11, Wroclaw, e-mail: [email protected]
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Abstract

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The solar results from CORONAS-F satellite have been reviewed. The observations with the DIFOS multi-channel photometer in a broad spectral range from 350 to 1500 nm have allowed to determine the dependence of the relative amplitudes of p-modes of the global solar oscillations on the wavelength. The EUV observations in SPIRIT experiment have enabled the study of various manifestations of solar activity and high-temperature events on the Sun. The data from the flare instruments-gamma spectrometer HELICON, flare spectrometer IRIS, amplitude-time spectrometer AVS-F, and X-ray spectrometer RPS-1 have been used to analyze the hard emission from solar flares and to carry out the diagnostics of the solar flare plasma. The Solar Cosmic Ray Complex has investigated the solar flare effects in the Earth's environment. The UV emission variations during solar flares in the vicinity of the 120-nm wavelengh have been recorded and the relative variation amplitude has been determined.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. 357 - 366
Copyright
© 2004 International Astronomical Union