| 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 |