Solar Cycle Phase Dependence of Supergranular Fractal Dimension

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5596

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DC Field	Value	Language
dc.contributor.author	Paniveni, U	-
dc.contributor.author	Krishan, V	-
dc.contributor.author	Singh, J	-
dc.contributor.author	Srikanth, R	-
dc.date.accessioned	2011-09-29T11:12:15Z	-
dc.date.available	2011-09-29T11:12:15Z	-
dc.date.issued	2011-06	-
dc.identifier.citation	Journal of Astrophysics & Astronomy , Vol. 32, No. 1-2, pp. 265-268	en
dc.identifier.uri	http://hdl.handle.net/2248/5596	-
dc.description.abstract	We study the complexity of supergranular cells using the intensity patterns obtained from the Kodaikanal Solar Observatory during the 23rd solar cycle. Our data consists of visually identified supergranular cells, from which a fractal dimension D for supergranulation is obtained according to the relation P ∝ A D/2, where A is the area and P is the perimeter of the supergranular cells. We find a difference in the fractal dimension between active and quiet region cells in the ascending phase, during the peak and in the descending phase which is conjectured to be due to the magnetic activity level.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://www.springerlink.com/content/9l77u4v640733670/	en
dc.rights	© Indian Academy of Sciences	en
dc.subject	Solar cycle – supergranulation – fractal dimension	en
dc.title	Solar Cycle Phase Dependence of Supergranular Fractal Dimension	en
dc.type	Article	en
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