Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1889
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dc.contributor.authorRaju, K. P-
dc.contributor.authorSrikanth, R-
dc.contributor.authorSingh, J-
dc.date.accessioned2007-10-16T10:05:42Z-
dc.date.available2007-10-16T10:05:42Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 1, pp. 65 - 68en
dc.identifier.urihttp://hdl.handle.net/2248/1889-
dc.description.abstractSupergranulation is the surface manifestation of large scale solar convection. Since there is a strong correspondence between supergranulation pattern and Ca K chromospheric network, lifetimes and sizes may be obtained from the temporal and spatial autocorrelation functions (ACF), calculated from Ca K filtergrams of the Sun. We have developed a program to study the lifetimes and spatial scales of supergranulation through an extenasive digital analysis. The temporal ACF was calculataed from a 106 hour time-sequence of the data obtained from Antarctica. The lifetimes of quiet cells were found to be about 24-34 hours while that of active cells were about 58-61 hours. The temporal autocorrelation function sometimes showed an oscillataory pattern which may be due to long-term intensity variations or length scale changes associataed with the network. The cell sizes were obtained from Ca K spectroheliograms belonging to the solar minimum phases of 1913-1974 from Kodaikanal Solar Observatory. The average cell size was found to show a curious dependence on solar latitude.en
dc.format.extent240120 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSunen
dc.subjectSolar Coronaen
dc.subjectSupergranulationen
dc.titleLifetimes and sizes of supergranular cellsen
dc.typeArticleen
Appears in Collections:BASI Publications

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