Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2635
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dc.contributor.authorSingh, J-
dc.contributor.authorNagabhushana, B. S-
dc.contributor.authorBabu, G. S. D-
dc.contributor.authorUddin, Wahab-
dc.date.accessioned2008-07-11T10:12:12Z-
dc.date.available2008-07-11T10:12:12Z-
dc.date.issued1994-08-
dc.identifier.citationSolar Physics, Vol. 153, No. 1-2, pp. 157 - 167en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/2635-
dc.description.abstractTo study the evolution of large convective cells known as supergranules, a solar telescope was set up at Maitri, Indian permanent station in Antarctica region, during the local summer months (December 1989 through March 1990). A continuous sequence of calcium K-line filtergrams for 106 hours spaced at intervals of about 10 min was obtained. The analysis of the data indicates that the most probable lifetime of the calcium-K network is about 22 hours. The lifetime depends upon the size of the cell and is larger for bigger cells. The data also show that cells (of a given size) associated with remnant magnetic field regions live longer than those in the field-free region. This may mean that the magnetic field plays an important role in the confinement of these structures.en
dc.format.extent927860 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://adsabs.harvard.edu/abs/1994SoPh..153..157Sen
dc.relation.urihttp://www.springerlink.com/content/r3862811364w8173/en
dc.subjectAntarctic Regionsen
dc.subjectCalciumen
dc.subjectChromosphereen
dc.subjectK Linesen
dc.subjectSolar Activityen
dc.subjectSolar Granulationen
dc.subjectSolar Magnetic Fielden
dc.subjectCamerasen
dc.subjectData Correlationen
dc.subjectFiltergramsen
dc.subjectFrequency Distributionen
dc.subjectH Alpha Lineen
dc.subjectHeliostatsen
dc.subjectTelescopesen
dc.titleStudy of calcium-K network evolution from Antarcticaen
dc.typeArticleen
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