Thin structure of temporal profiles of solar flares January 15, 17 and 20, 2005 by data of AVS-F apparatus onboard CORONAS-F satellite |
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Authors: | I.V. Arkhangelskaja Yu.D. KotovA.I. Arkhangelsky A.S. Glyanenko |
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Affiliation: | Astrophysics Institute of Moscow Engineering Physics Institute (State University), Kashirskoe shosse, 31, 115409 Moscow, Russia |
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Abstract: | The count rate temporal profiles and energy spectra of the solar flares January 15, 17, 20 2005 in hard X-ray and gamma energy bands by data of AVS-F apparatus onboard CORONAS-F satellite are discussed. The energy spectra of these solar flares contain positron line and neutron capture line. Solar flares of January 17 and 20 spectra also contain some nuclear lines. Thin structure with characteristic timescales of 33–92 s is presented on flares temporal profiles in energy bands corresponding to the observed spectral features, which are confirmed by periodogram analysis (confidence level is 99%). |
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Keywords: | Solar flares CORONAS-F Solar activity Gamma energy bands Hard X-rays |
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