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CORONAS-F observations of active phenomena on the sun |
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| Authors: | VN Oraevsky II Sobelman IA Zitnik VD Kuznetsov AI Stepanov GM Polishuk PN Kovilin AA Negoda VI Dranovsky YaS Yatskiv |
| Institution: | 1Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, 142190, Moscow Region, Troitsk, IZMIRAN, Russia 2Lebedev Physical Institute, 119991, Moscow, Leninsky prospekt 53, Russia 3Russian Aviation and Space Agency, 107996, Moscow, Shepkina str., 42, Russia 4Design Office “Yuzhnoye”, 49008, Dnepropetrovsk, Krivorozhskaya str., 3, Ukraine 5National Space Agency of Ukraine, 03022 Bozhenko str., 11, Kyiv, Ukraine 6Main Astronomical Observatory of the National Academy of Sciences of Ukraine,27 Akademika Zabolotnoho St., 03680 Kyiv, Ukraine |
| Abstract: | Complex observations in the framework of the CORONAS-F Mission aimed at the study of active phenomena inthe solar corona are described. The main features are given for the following experiments: (1) XUV-imaging spectroscopy with high temporal and spatial resolution, (2) X-ray spectroscopy, (3) X-ray and gamma-ray photometer/spectrometer, and (4) solar cosmic rays. Some new observational data on the structure and dynamics of flares and transient events are discussed along with their analysis. |
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