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http://hdl.handle.net/2248/1889
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DC Field | Value | Language |
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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 |
Appears in Collections: | BASI Publications |
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