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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3936
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dc.contributor.authorPaniveni, U.-
dc.contributor.authorKrishan, Vinod-
dc.contributor.authorSingh, Jagdev-
dc.contributor.authorSrikanth, R.-
dc.date.accessioned2010-07-22T08:48:37Z-
dc.date.available2010-07-22T08:48:37Z-
dc.date.issued2009-11-27-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2009, Vol.402, p424en
dc.identifier.issn1365-2966 (Online)-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2289/3936-
dc.descriptionRestricted Access.en
dc.description.abstractWe 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.en
dc.language.isoenen
dc.publisherWiley Interscience for the RASen
dc.relation.urihttp://adsabs.harvard.edu/abs/2010MNRAS.402..424Pen
dc.relation.urihttp://dx.doi.org/10.1111/j.1365-2966.2009.15889.xen
dc.rights2009 Wiley Interscience for the RASen
dc.subjectmethods: data analysisen
dc.subjectstatistical techniquesen
dc.subjectimage processingen
dc.subjectSun: activityen
dc.subjectSun granulation photosphereen
dc.titleActivity dependence of solar supergranular fractal dimensionen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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