The magnetosphere as a complex system

被引:28
作者
Alejandro Valdivia, Juan [1 ]
Rogan, Jose [1 ]
Munoz, Victor [1 ]
Toledo, Benjamin A. [1 ]
Stepanova, Marina [2 ]
机构
[1] Univ Chile, Fac Ciencias, Dept Fis, Santiago, Chile
[2] Univ Santiago Chile, Fac Ciencias, Dept Fis, Santiago, Chile
基金
巴西圣保罗研究基金会;
关键词
Self-organizations; Space plasmas; Substorms; Multifractals; SELF-ORGANIZED CRITICALITY; MAGNETOTAIL CURRENT SHEET; EARTHS PLASMA SHEET; MULTIFRACTAL ANALYSIS; INTERMITTENT TURBULENCE; WAVELET LEADERS; COUPLED-MAP; MODEL; RECONNECTION; EVOLUTION;
D O I
10.1016/j.asr.2012.04.004
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The 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 approximate to 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 approximate to 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. (C) 2012 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:1934 / 1941
页数:8
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