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

preprint2011arXivOpen access

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 LL grows as a diffusive random walk with time TT, following L∝T1/2L \propto T^{1/2}; (ii) The instantaneous energy dissipation rate f(t)f(t) occupies a fractal volume with dimension DSD_S, which predicts the relationships F=f(t=T)∝LDS∝TDS/2F = f(t=T) \propto L^{D_S} \propto T^{D_S/2}, P∝LS∝TS/2P \propto L^{S} \propto T^{S/2} for the peak energy dissipation rate, and E∝FT∝T1+DS/2E \propto F T \propto T^{1+D_S/2} for the total dissipated energy; (iii) The mean fractal dimension of avalanches in Euclidean space S=1,2,3S=1,2,3 is DS≈(1+S)/2D_S \approx (1+S)/2; and (iv) The occurrence frequency distributions N(x)∝x−αxN(x) \propto x^{-α_x} based on spatially uniform probabilities in a SOC system are given by N(L)∝L−SN(L) \propto L^{-S}, which predicts powerlaw distributions for all parameters, with the slopes αT=(1+S)/2α_T=(1+S)/2, αF=1+(S−1)/DSα_F=1+(S-1)/D_S, αP=2−1/Sα_P=2-1/S, and αE=1+(S−1)/(DS+2)α_E=1+(S-1)/(D_S+2). We test the predicted fractal dimensions, occurrence frequency distributions, and correlations with numerical simulations of cellular automaton models in three dimensions S=1,2,3S=1,2,3 and find satisfactory agreement within ≈10\approx 10%. One profound prediction of this universal SOC model is that the energy distribution has a powerlaw slope in the range of αE=1.40−1.67α_E=1.40-1.67, and the peak energy distribution has a slope of αP=1.67α_P=1.67 (for any fractal dimension DS=1,...,3D_S=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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