M Sadegh Movahed et al J. Stat. Mech. (2006) P02003 doi:10.1088/1742-5468/2006/02/P02003
M Sadegh Movahed1,2,3, G R Jafari2,4, F Ghasemi2, Sohrab Rahvar1,2 and M Reza Rahimi Tabar1,5
Show affiliationsWe 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.
96.60.qd Sun spots, Solar cycles
05.40.-a Fluctuation phenomena, random processes, noise, and Brownian motion
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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