Correlated flares in models of a magnetized "canopy"

Details Correlated flares in models of a magnetized "canopy" Correlated flares in models of a magnetized "canopy"

2007-09-13

arxiv.org/abs/0709.2053v1

PhysicaA387:167-176,2008

Astronomy and Astrophysics

Astrophysics

5 pages + 9 figures, Accepted to Physica A

Scientific paper

10.1016/j.physa.2007.09.003

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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