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Lifetimes and sizes of supergranular cells

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dc.contributor.author Raju, K. P
dc.contributor.author Srikanth, R
dc.contributor.author Singh, J
dc.date.accessioned 2007-10-16T10:05:42Z
dc.date.available 2007-10-16T10:05:42Z
dc.date.issued 1999
dc.identifier.citation BASI, Vol. 27, No. 1, pp. 65 - 68 en
dc.identifier.uri http://hdl.handle.net/2248/1889
dc.description.abstract Supergranulation 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.extent 240120 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.subject Sun en
dc.subject Solar Corona en
dc.subject Supergranulation en
dc.title Lifetimes and sizes of supergranular cells en
dc.type Article en


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