X-class flares during solar cycle 24: pre-flare and post-flare conditions in active regions. PART II

  • Yu.A. Fursiak Crimean Astrophysical Observatory, Nauchny, 298409

Abstract

This paper analyzes dynamic processes and features of the magnetic configuration in active regions, there were two or more X-class solar flares recorded. It is concluded the role of high magnetic field gradients, features of group formation and instability of the magnetic configuration of the active region in the emergence and further development of high-power flare processes, the maximum energy flow from which at the Earth’s orbit in the wavelength range of 1–8 Å is not less than 10-1 erg/(cm2× s).

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