A smooth double power law, not a single power law, best fits the photospheric flux distribution over the full solar cycle; its large-scale slope varies with activity while the small-scale slope is stable.
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Solar Cycle Variation of the Distribution of Photospheric Magnetic Flux Features
A smooth double power law, not a single power law, best fits the photospheric flux distribution over the full solar cycle; its large-scale slope varies with activity while the small-scale slope is stable.