Correlated flares in models of a magnetized "canopy"

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dc.creatorBaiesi, M.
dc.creatorMaes, C.
dc.creatorShergelashvili, B. M.
dc.date2007-09-13
dc.date.accessioned2026-07-07T10:57:24Z
dc.date.available2026-07-07T10:57:24Z
dc.descriptionA 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.
dc.description5 pages + 9 figures, Accepted to Physica A
dc.identifierhttps://arxiv.org/abs/0709.2053
dc.identifierhttp://arxiv.org/abs/0709.2053
dc.identifierPhysicaA387:167-176,2008
dc.identifierdoi:10.1016/j.physa.2007.09.003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186739
dc.subjectAstrophysics
dc.subjectStatistical Mechanics
dc.subjectPlasma Physics
dc.titleCorrelated flares in models of a magnetized "canopy"
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