Role and Nature of Intermittency and Self-Organized Criticality in Solar Phenomena

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4425 Critical Phenomena, 4440 Fractals And Multifractals, 4475 Scaling: Spatial And Temporal (1872, 3270, 4277), 4480 Self-Organized Criticality, 7524 Magnetic Fields

Scientific paper

In Solar Physics, last decades demonstrated a considerable progress in understanding of both macro-scale processes (e.g., magneto-hydro-dynamic modeling of the heliosphere, magnetic field modeling in coronal structures, etc.), on the one hand, and micro-scale phenomena (e.g., turbulence of the solar plasma), on the other hand. Further progress seems to be associated with our realization of how various micro-scale processes are involved and manifested in the macro-scale behavior of the entire Sun. A similar problem unavoidably arises in studies of any other non-linear dynamical dissipative system in Nature. Such systems that can be placed in between a chaos and a completely determined structure. The goal of this talk is to show how the conceptions of intermittency, multifractality, percolation, and self-organized criticality are closely intertwined, and how they are currently elaborated in Solar Physics and help in understanding of unpredictable behavior of our closest star.

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