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NEW SUNS IN THE COSMOS. III. MULTIFRACTAL SIGNATURE ANALYSIS

  • Authors: D. B. de Freitas, M. M. F. Nepomuceno, P. R. V. de Moraes Junior, C. E. F. Lopes, M. L. Das Chagas, J. P. Bravo, A. D. Costa, B. L. Canto Martins, J. R. De Medeiros, and I. C. Leão

2016 The Astrophysical Journal 831 87.

  • Provider: AAS Journals

Caption: Figure 1.

Multifractal fluctuation function Fq(n) obtained from MFDMA for the active (left panels) and quiet (right panels) Sun. Each curve corresponds to different fixed values of ﹩q=-5,\ldots ,5﹩ from top to bottom, while top bold, middle bold, and the bottom bold lines correspond to ﹩q=5,q=0﹩, and ﹩q=-5﹩, respectively. Black lines are shuffled data and red lines are original data (top). Comparison of the multifractal scaling exponent ﹩\tau (q)﹩ of the original (red), shuffled (green), and surrogate (blue) time series (left-bottom). Multifractal spectrum ﹩f(\alpha )﹩ of the the original (red), shuffled (green). and surrogate (blue) time series. The solid curves represent the best fourth-order fit (right-bottom).

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