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Study of calcium-K network evolution from Antarctica

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dc.contributor.author Singh, J
dc.contributor.author Nagabhushana, B. S
dc.contributor.author Babu, G. S. D
dc.contributor.author Uddin, Wahab
dc.date.accessioned 2008-07-11T10:12:12Z
dc.date.available 2008-07-11T10:12:12Z
dc.date.issued 1994-08
dc.identifier.citation Solar Physics, Vol. 153, No. 1-2, pp. 157 - 167 en
dc.identifier.issn 0038-0938
dc.identifier.uri http://hdl.handle.net/2248/2635
dc.description.abstract To study the evolution of large convective cells known as supergranules, a solar telescope was set up at Maitri, Indian permanent station in Antarctica region, during the local summer months (December 1989 through March 1990). A continuous sequence of calcium K-line filtergrams for 106 hours spaced at intervals of about 10 min was obtained. The analysis of the data indicates that the most probable lifetime of the calcium-K network is about 22 hours. The lifetime depends upon the size of the cell and is larger for bigger cells. The data also show that cells (of a given size) associated with remnant magnetic field regions live longer than those in the field-free region. This may mean that the magnetic field plays an important role in the confinement of these structures. en
dc.format.extent 927860 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Springer en
dc.relation.uri http://adsabs.harvard.edu/abs/1994SoPh..153..157S en
dc.relation.uri http://www.springerlink.com/content/r3862811364w8173/ en
dc.subject Antarctic Regions en
dc.subject Calcium en
dc.subject Chromosphere en
dc.subject K Lines en
dc.subject Solar Activity en
dc.subject Solar Granulation en
dc.subject Solar Magnetic Field en
dc.subject Cameras en
dc.subject Data Correlation en
dc.subject Filtergrams en
dc.subject Frequency Distribution en
dc.subject H Alpha Line en
dc.subject Heliostats en
dc.subject Telescopes en
dc.title Study of calcium-K network evolution from Antarctica en
dc.type Article en


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