Spectral peculiarities of high energy X-ray radiation, gamma radiation, and Submillimeter radio emission in the impulsive phase of a solar flare

• Published in: Bulletin of the Russian Academy of Sciences. Physics 2011-06, Vol.75 (6), p.747-750
• Main Authors: Makhmutov, V. S., Kurt, V. G., Yushkov, B. Yu, Grechnev, V. V., Kaufmann, P., Raulin, J. -P., Bazilevskaya, G. A., Stozhkov, Yu. I.
• Format: Article
• Language: English
• Subjects: Coronas; Emission analysis; Energy spectra; Fluxes; Frequency spectrum; Gamma rays; GOES satellites; Ground-based observation; Hadrons; Heavy Ions; Jupiter; Nuclear Physics; Onboard; Physics; Physics and Astronomy; Proceeding of the 31st Russian Conference on Cosmic Rays; Radio; Radio emission; Satellites
• ISSN: 1062-8738; 1934-9432
• DOI: 10.3103/S106287381106030X

We analyze experimental data on the temporal behavior of fluxes and energy spectra of hard solar X-ray and gamma radiation in the energy range of 0.015 to 300 MeV, obtained onboard the CORONAS-F satellite during a solar flare on August 25, 2001. These data are compared with measurements of the radio emission fluxes over the wide frequency range of 1–405 GHz. For our analysis, we use data obtained onboard the YOHKOH, TRACE and GOES satellites, along with ground-based observations of this solar event using the Solar Submillimeter Telescope (SST; Argentina). For the first time, we find nearly simultaneous changes in the energy spectra of gamma radiation over the range 10–150 MeV and the frequency spectrum of radio emission at the beginning and during a impulsive phase of this event (whose duration did not exceed three minutes).