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Nonlinear fluctuation analysis for a set of 41 magnetic clouds measured by the Advanced Composition Explorer (ACE) spacecraft

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Figure

Table 1. Solar wind data studied (from Huttunen et al., 2005).
Table 2. We calculate the persistence in the IMF components usingfour different methods: β exponent of power spectrum, α exponentof DFA, Hurst of R/S analysis, and Hausdorff Ha exponent of semi-variogram, respectively
Figure 1. In (a), a histogram is construct from a frequency table of ⟨β(j)⟩ values, plotted in Fig
Figure 2. Insymbols corresponds to the sheath, MCs, and post-MC regions, re-spectively
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