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 |
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dc.format.mimetype |
application/pdf |
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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 |