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Voyager 2 observation of the multifractal spectrum in the heliosphere and the heliosheath

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Fig. 2. The singularity multifractal spectrumorigin to the point on the f (α) versus the sin-gularity strength α with some general properties: (1) the maximumvalue of f (α) is D0; (2) f (D1) = D1; and (3) the line joining the f (α) curve, where α = D1, is tangent tothe curve, as taken from Ott (1993).
Fig. 3. The singularity spectrummeasured by Voyager 2 in the relatively near heliosphere (within planetary orbits) at f (α) as a function of a singularity strength α
Fig. 4. The singularity spectrummeasured by Voyager 2 in the distant heliosphere (beyond the planetary orbits) at(e) f (α) as a function of a singularity strength α
Fig. 5. The singularity spectrummeasured by Voyager 2 in the very deep heliosphere (before) at f (α) as a function of a singularity strength α
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