Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3135
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dc.contributor.authorSrikanth, R-
dc.contributor.authorRaju, K. P-
dc.contributor.authorSingh, J-
dc.date.accessioned2008-08-14T10:10:04Z-
dc.date.available2008-08-14T10:10:04Z-
dc.date.issued1999-02-
dc.identifier.citationSolar Physics, Vol. 184, No. 2, pp. 267 - 280en
dc.identifier.issn0038 - 0938-
dc.identifier.urihttp://hdl.handle.net/2248/3135-
dc.description.abstractA time series of CaiiK filtergrams of the chromosphere was used to study the relationship between correlation lifetimes and autocorrelation length scales. The form of the lifetime-scale relation is inferred by comparing the distribution of the two parameters. A linear dependence of lifetime on cell area, with a least squares fit slope of 3.34x107km2hr-1, is deduced. The relation can be explained by assuming the network evolves by means of a diffusion process of the magnetic elements.en
dc.format.extent90761 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://dx.doi.org/10.1023/A:1005125326765en
dc.subjectThe Chromospheric Networken
dc.subjectK-Line Network Cellsen
dc.subjectSkewness and kurtosisen
dc.titleThe chromospheric network: Dependence of cell lifetime on length-scaleen
dc.typeArticleen
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