A review of the solar results from CORONAS-F satellite

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...

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Published inProceedings of the International Astronomical Union Vol. 2004; no. IAUS223; pp. 357 - 366
Main Authors Kuznetsov, V.D., Charikov, Yu.E, Kotov, Yu.D., Kuznetsov, S.N., Mazets, E.P., Nusinov, A.A., Pankov, V.M., Sobelman, I.I., Sylwester, J.
Format Journal Article
LanguageEnglish
Published Cambridge, UK Cambridge University Press 01.06.2004
Subjects
Chemical elements
Contributed Papers
Corona
Cosmic rays
Experiments
Gamma rays
Plasma
Radiation
Solar physics
Spectrum analysis
Sun
Temperature
X-rays
Russia
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Summary: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
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921304006131