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Activity dependence of solar supergranular fractal dimension

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Wiley Interscience for the RAS

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We study the complexity of supergranular cells using the intensity patterns obtained at the Kodaikanal Solar Observatory during the solar maximum. Our data consist of visually identified supergranular cells, from which a fractal dimension D for supergranulation is obtained according to the relation P∝AD/2 , where A is the area and P the perimeter of the supergranular cells. We find a fractal dimension of about 1.12 for active region cells and about 1.25 for quiet region cells, a difference that could be attributed to the inhibiting effect of the magnetic field.

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Monthly Notices of the Royal Astronomical Society, 2009, Vol.402, p424

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2009 Wiley Interscience for the RAS