Supergranulation and its Activity Dependence

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5706

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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	2012-02-24T14:43:19Z	-
dc.date.available	2012-02-24T14:43:19Z	-
dc.date.issued	2011-08	-
dc.identifier.citation	Astrophysical Dynamics: From Stars to Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Vol. 271, pp. 391-392	en
dc.identifier.uri	http://hdl.handle.net/2248/5706	-
dc.description	Open Access	en
dc.description.abstract	We 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.iso	en	en
dc.publisher	Cambridge University Press	en
dc.relation.ispartofseries	International Astronomical Union Symposium; No. 271	-
dc.relation.uri	http://dx.doi.org/10.1017/S1743921311017947	en
dc.rights	© International Astronomical Union	en
dc.subject	Sun: granulation —-turbulence	en
dc.title	Supergranulation and its Activity Dependence	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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