dc.creatorValdivia Hepp, Juan
dc.creatorRogan Castillo, José
dc.creatorMuñoz, Victor
dc.creatorToledo Cabrera, Benjamín
dc.creatorStepanova, Marina
dc.date.accessioned2018-12-20T14:06:19Z
dc.date.available2018-12-20T14:06:19Z
dc.date.created2018-12-20T14:06:19Z
dc.date.issued2013
dc.identifierAdvances in Space Research, Volumen 51, Issue 10, 2018, Pages 1934-1941
dc.identifier02731177
dc.identifier10.1016/j.asr.2012.04.004
dc.identifierhttp://repositorio.uchile.cl/handle/2250/153903
dc.description.abstractThe magnetosphere is a multi-scale spatio-temporal complex dynamical system. In this context, we have analyzed the multifractal behavior of the AL index, as a proxy for an energy dissipation rate, using discrete wavelet leaders. This technique allows the calculation of the spectrum for both positive and negative values of q, giving a robust peak at h≈0.5. The same technique is applied to the dissipation rate of a simple 1D model of intermittent magnetic field annihilation, showing a clear multifractal behavior, but with a peak at h≈0.2. Even though this intuitive 1D model, because of its simplicity, is not expected to reproduce all the complex dynamics that occur in the Earth's magnetotail, it suggests that the existence of a multifractal dissipation dynamics is necessary to the establishment of the self-organized state, as shown in a 2D simulation of intermittent plasma dynamics.© 2012 COSPAR. Published by Elsevier Ltd. All rights reserved.
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
dc.sourceAdvances in Space Research
dc.subjectMultifractals
dc.subjectSelf-organizations
dc.subjectSpace plasmas
dc.subjectSubstorms
dc.titleThe magnetosphere as a complex system
dc.typeArtículos de revistas


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