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Multifractal detrended fluctuation analysis of sunspot time series

M Sadegh Movahed1,2,3, G R Jafari2,4, F Ghasemi2, Sohrab Rahvar1,2 and M Reza Rahimi Tabar1,5

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We use multifractal detrended fluctuation analysis (MF-DFA), to study sunspot number fluctuations. The result of the MF-DFA shows that there are three crossover timescales in the fluctuation function. We discuss how the existence of the crossover timescales is related to a sinusoidal trend. Using Fourier detrended fluctuation analysis, the sinusoidal trend is eliminated. The Hurst exponent of the time series without the sinusoidal trend is 0.12 ± 0.01. Also we find that these fluctuations have multifractal nature. Comparing the MF-DFA results for the remaining data set to those for shuffled and surrogate series, we conclude that its multifractal nature is almost entirely due to long range correlations.


Keywords

new applications of statistical mechanics

PACS

96.60.qd Sun spots, Solar cycles

05.40.-a Fluctuation phenomena, random processes, noise, and Brownian motion

05.45.Df Fractals

96.60.Hv Electric and magnetic fields

Subjects

Statistical physics and nonlinear systems

Astrophysics and astroparticles

Dates

Issue 02 (February 2006)

Received 6 December 2005, accepted for publication 20 January 2006

Published 9 February 2006


An Erratum for this article has been published in J. Stat. Mech. (2011) E09001


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