The Dependence of Chromospheric CA II K Network Cell Sizes on Solar Latitude

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3331

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DC Field	Value	Language
dc.contributor.author	Raju, K. P	-
dc.contributor.author	Srikanth, R	-
dc.contributor.author	Singh, J	-
dc.date.accessioned	2008-09-02T14:35:25Z	-
dc.date.available	2008-09-02T14:35:25Z	-
dc.date.issued	1998-06	-
dc.identifier.citation	Solar Physics, Vol. 180, No. 1/2, pp. 47 - 51	en
dc.identifier.issn	0038 - 0938	-
dc.identifier.uri	http://hdl.handle.net/2248/3331	-
dc.description	Restricted Access	en
dc.description.abstract	Calcium K line spectroheliograms obtained during the solar minimum phases at Kodaikanal between 1913–1974 have been used to study the network cell sizes. The autocorrelation is calculated for two-dimensional strips at 5° interval up to ±50° latitude. The average size of the network cells was found to have a dependence on solar latitude with a maximum variation of about 7%. The pattern shows an apparent north–south symmetry with two minima at about 20° N and S.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://dx.doi.org/10.1023/A:1005072907000	en
dc.subject	Chromospheric CA II K	en
dc.subject	Solar Latitude	en
dc.title	The Dependence of Chromospheric CA II K Network Cell Sizes on Solar Latitude	en
dc.type	Article	en
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