ESTIMATION OF THE MAIN PARAMETERS OF THE CORONAL BRIGHT POINTS WITHIN THE MODEL OF INTERACTION OF INDUCED CURRENT SYSTEMS

Within the proposed phenomenological model of the formation of coronal bright points (CBPs), as the results of the interaction of current systems in the solar corona, numerical estimates of the main parameters of the CBPs are carried out. The considered model is fundamentally different from the standard concept of magnetic reconnection. The source of coronal current systems (CCS) are small-scale magnetic structures, that emerge from under the photosphere through the transition layer into a corona with ionized plasma. In particular, the model of CCS, in the first approximation, gives rather good agreement with the observed parameters and characteristics of CBPs, such as size, energy release, lifetime, spectrum and level of generated radio emission. The possibility of local heating of coronal plasma, generation of X-ray and radio radiation in the region of interaction of the CCS due to the development of plasma and MHD instabilities is shown.

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