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

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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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