Correlated flares in models of a magnetized "canopy"

M. Baiesi; C. Maes; B. M. Shergelashvili

doi:10.1016/j.physa.2007.09.003

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arXiv · 0709.2053

Correlated flares in models of a magnetized "canopy"

M. Baiesi·C. Maes·B. M. Shergelashvili

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Abstract

A model of the Lu-Hamilton kind is applied to the study of critical behavior of the magnetized solar atmosphere. The main novelty is that its driving is done via sources undergoing a diffusion. This mimics the effect of a virtual turbulent substrate forcing the system. The system exhibits power-law statistics not only in the size of the flares, but also in the distribution of the waiting times.

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M. Baiesi, C. Maes, B. M. Shergelashvili. 2007-09-13. Correlated flares in models of a magnetized "canopy". https://doi.org/10.1016/j.physa.2007.09.003

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