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  Extreme value theory for singular measures

Lucarini, V., Faranda, D., Turchetti, G., & Vaienti, S. (2012). Extreme value theory for singular measures. CHAOS, 22(2): 023135. doi:10.1063/1.4718935.

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 Creators:
Lucarini, Valerio1, Author           
Faranda, Davide2, Author           
Turchetti, Giorgio3, Author
Vaienti, Sandro3, Author
Affiliations:
1A 1 - Climate Variability and Predictability, Research Area A: Climate Dynamics and Variability, The CliSAP Cluster of Excellence, External Organizations, ou_1863478              
2External Organizations, ou_persistent22              
3external, ou_persistent22              

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Free keywords: BOWEN-RUELLE MEASURES; STRANGE ATTRACTORS; GENERALIZED DIMENSIONS; DYNAMICAL-SYSTEMS; TIME STATISTICS; METRIC ENTROPY; SEISMIC RISK; EVENTS; PRECIPITATION; EXPONENTS
 Abstract: In this paper, we perform an analytical and numerical study of the extreme values of specific observables of dynamical systems possessing an invariant singular measure. Such observables are expressed as functions of the distance of the orbit of initial conditions with respect to a given point of the attractor. Using the block maxima approach, we show that the extremes are distributed according to the generalised extreme value distribution, where the parameters can be written as functions of the information dimension of the attractor. The numerical analysis is performed on a few low dimensional maps. For the Cantor ternary set and the Sierpinskij triangle, which can be constructed as iterated function systems, the inferred parameters show a very good agreement with the theoretical values. For strange attractors like those corresponding to the Lozi and Henon maps, a slower convergence to the generalised extreme value distribution is observed. Nevertheless, the results are in good statistical agreement with the theoretical estimates. It is apparent that the analysis of extremes allows for capturing fundamental information of the geometrical structure of the attractor of the underlying dynamical system, the basic reason being that the chosen observables act as magnifying glass in the neighborhood of the point from which the distance is computed. (C) 2012 American Institute of Physics. [http://dx.doi.org/10.1063/1.4718935]

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Language(s): eng - English
 Dates: 2012-06
 Publication Status: Published online
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: ISI: 000305833900035
DOI: 10.1063/1.4718935
 Degree: -

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Title: CHAOS
Source Genre: Journal
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Pages: - Volume / Issue: 22 (2) Sequence Number: 023135 Start / End Page: - Identifier: ISSN: 1054-1500