Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5593
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dc.contributor.authorPaniveni, U-
dc.contributor.authorKrishan, V-
dc.contributor.authorSingh, J-
dc.contributor.authorSrikanth, R-
dc.date.accessioned2011-09-28T10:59:55Z-
dc.date.available2011-09-28T10:59:55Z-
dc.date.issued2011-08-
dc.identifier.citationProceedings of the International Astronomical Union Symposium, Vol. 271, pp. 391-392en
dc.identifier.urihttp://hdl.handle.net/2248/5593-
dc.descriptionOpen Accessen
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 consists of visually identified supergranular cells, from which a fractal dimension D is obtained according to the relation P ∝ AD/2 where A is the area and P is the perimeter of the cells. We find a difference in the fractal dimension between the active and the quiet region cells which is conjectured to be due to the magnetic activity level.en
dc.language.isoenen
dc.publisherCambridge University Pressen
dc.relation.urihttp://dx.doi.org/10.1017/S1743921311017947en
dc.rights© Cambridge University Pressen
dc.subjectSun: granulation - turbulenceen
dc.titleSupergranulation and its Activity Dependenceen
dc.typeArticleen
Appears in Collections:IIAP Publications

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