Correlated flares in models of a magnetized "canopy"

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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.
5 pages + 9 figures, Accepted to Physica A

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Astrophysics, Statistical Mechanics, Plasma Physics

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http://salesiana.dossiersoluciones.com/handle/123456789/186739

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0709.2053
 http://arxiv.org/abs/0709.2053
 PhysicaA387:167-176,2008
 doi:10.1016/j.physa.2007.09.003

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arXiv