A Statistical Fractal-Diffusive Avalanche Model of a Slowly-Driven Self-Organized Criticality System

Abstract

We develop a statistical analytical model that predicts the occurrence frequency distributions and parameter correlations of avalanches in nonlinear dissipative systems in the state of a slowly-driven self-organized criticality (SOC) system. This model, called the fractal-diffusive SOC model, is based on the following four assumptions: (i) The avalanche size L grows as a diffusive random walk with time T, following L T1/2; (ii) The instantaneous energy dissipation rate f(t) occupies a fractal volume with dimension DS, which predicts the relationships F = f(t=T) LDS TDS/2, P LS TS/2 for the peak energy dissipation rate, and E F T T1+DS/2 for the total dissipated energy; (iii) The mean fractal dimension of avalanches in Euclidean space S=1,2,3 is DS ≈ (1+S)/2; and (iv) The occurrence frequency distributions N(x) x-αx based on spatially uniform probabilities in a SOC system are given by N(L) L-S, which predicts powerlaw distributions for all parameters, with the slopes αT=(1+S)/2, αF=1+(S-1)/DS, αP=2-1/S, and αE=1+(S-1)/(DS+2). We test the predicted fractal dimensions, occurrence frequency distributions, and correlations with numerical simulations of cellular automaton models in three dimensions S=1,2,3 and find satisfactory agreement within ≈ 10%. One profound prediction of this universal SOC model is that the energy distribution has a powerlaw slope in the range of αE=1.40-1.67, and the peak energy distribution has a slope of αP=1.67 (for any fractal dimension DS=1,...,3 in Euclidean space S=3), and thus predicts that the bulk energy is always contained in the largest events, which rules out significant nanoflare heating in the case of solar flares.

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