CORONAS-F observations of active phenomena on the Sun

1Oraevsky, VN, 2Sobelman, II, 2Zhitnik, IA, 1Kuznetsov, VD, 1Stepanov, AI, 3Polishuk, GM, 3Kovilin, PN, 4Negoda, AA, 5Dranovsky, VI, 6Yatskiv, Ya.S
1Pushkov Institute of Terrestrial Magnetism, Ionosphere and Propagation of Radio Waves of the Russian AS, Troitsk, Russia
2P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moskow, Russia
3Roskosmos State Corporation, Moscow, Russia
4State Space Agency of Ukraine, Kyiv, Ukraine
5Yangel Yuzhnoye State Design Office, Dnipropetrovsk, Ukraine
6Main Astronomical Observatory of the National Academy of Sciences of Ukraine, Kyiv, Ukraine
Kosm. nauka tehnol. 2003, 9 ;(2-3):003-009
Publication Language: Ukrainian
Complex observations in the framework of the CORONAS-F Mission aimed at the study of active phenomena in the solar corona are described. The main features are given for the following experiments: XUV-imaging spectroscopy with high temporal and spatial resolution, X-ray spectroscopy, X-ray and gamma-ray photometer/spectrometer, and solar cosmic rays. Some new observational data on the structure and dynamics of flares and transient events are discussed along with their analysis.
Keywords: solar corona, solar flares, «CORONAS-F»
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