The Solar Flare of November 4, 2001, and Its Manifestations in Energetic Particles from Coronas-F Data |
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| Authors: | Kuznetsov S. N. Bogomolov A. V. Denisov Yu. I. Kordylewski Z. Kudela K. Kurt V. G. Lisin D. V. Myagkova I. N. Podorol'skii A. N. Podosenova T. B. Svertilov S. I. Sylwester J. Stepanov A. I. Yushkov B. Yu. |
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| Affiliation: | (1) Skobeltsyn Institute of Nuclear Physics, Moscow State University, Vorob'evy gory, Moscow, 119992, Russia;(2) Center for Space Research, Polish Academy of Sciences, Wroclaw, Poland;(3) Institute for Experimental Physics, Slovakian Academy of Sciences, Kosice, Slovakia;(4) Institute of Terrestrial Magnetism, Ionosphere, and Radio-Wave Propagation, Russian Academy of Sciences, Troitsk, 142092, Russia;(5) Faculty of Computational Mathematics and Cybernetics, Moscow State University, Vorob'evy gory, Moscow, 119992, Russia |
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| Abstract: | Based on X-ray, gamma-ray, and charged-particle measurements with several instruments onboard the Coronas-F satellite and on ACE and GOES experimental data presented on the Internet, we investigate the parameters of the solar flare of November 4, 2001, and the energetic-particle fluxes produced by it in circumterrestrial space. The increase in relativistic-electron fluxes for about 1.5 days points to a moving source (shock front). The structure of the energetic-particles fluxes in the second half of November 5, 2001, can be explained by the passage of the coronal mass ejection that was ejected on November 1, 2001, and that interacted with the shock wave from the flare of November 4, 2001. |
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