Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1979
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dc.contributor.authorSingh, J-
dc.contributor.authorBappu, M. K. V-
dc.date.accessioned2007-11-24T11:22:12Z-
dc.date.available2007-11-24T11:22:12Z-
dc.date.issued1981-05-
dc.identifier.citationSolar Physics, Vol. 71, May, pp. 161-168en
dc.identifier.urihttp://hdl.handle.net/2248/1979-
dc.description.abstractCalcium network diameters are shown to be smaller by 5% at solar maximum than at minimum. The average cell size at minimum is 22,115 + or - 99 km. The average size at solar maximum is 20,920 + or - 112 km, though individual maxima perform differently from each other depending probably on the dispersed remnant magnetic fields. The change in size of the network is interpreted in terms of changes in the size of the supergranular convective cell.en
dc.format.extent640921 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://adsabs.harvard.edu/abs/1981SoPh...71..161S-
dc.subjectCalciumen
dc.subjectChromosphereen
dc.subjectMetal Ionsen
dc.subjectSolar atmosphereen
dc.subjectSolar Cyclesen
dc.subjectM.K.V. Bappuen
dc.titleA dependence on solar cycle of the size of the Ca/+/ networken
dc.typeArticleen
Appears in Collections:M.K. Vainu Bappu ( 1960 - 1982 )

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