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Fig. 1.

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Distributions of the magnetic field increments ΔB/B. The increments are computed at different timescales, τ, for each panel, as indicated at the top. The different colours represent different heliocentric distances. The shaded area represents the statistical error estimated as the square root of the number of points in a given bin. The error is not visible in most cases because it is small and comparable with the width of the plot lines.

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