dc.contributor.author |
Singh, J |
|
dc.contributor.author |
Nagabhushana, B. S |
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dc.contributor.author |
Babu, G. S. D |
|
dc.contributor.author |
Uddin, Wahab |
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dc.date.accessioned |
2008-07-11T10:12:12Z |
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dc.date.available |
2008-07-11T10:12:12Z |
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dc.date.issued |
1994-08 |
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dc.identifier.citation |
Solar Physics, Vol. 153, No. 1-2, pp. 157 - 167 |
en |
dc.identifier.issn |
0038-0938 |
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dc.identifier.uri |
http://hdl.handle.net/2248/2635 |
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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. |
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dc.format.extent |
927860 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Springer |
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dc.relation.uri |
http://adsabs.harvard.edu/abs/1994SoPh..153..157S |
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dc.relation.uri |
http://www.springerlink.com/content/r3862811364w8173/ |
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dc.subject |
Antarctic Regions |
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dc.subject |
Calcium |
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dc.subject |
Chromosphere |
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dc.subject |
K Lines |
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dc.subject |
Solar Activity |
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dc.subject |
Solar Granulation |
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dc.subject |
Solar Magnetic Field |
en |
dc.subject |
Cameras |
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dc.subject |
Data Correlation |
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dc.subject |
Filtergrams |
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dc.subject |
Frequency Distribution |
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dc.subject |
H Alpha Line |
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dc.subject |
Heliostats |
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dc.subject |
Telescopes |
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dc.title |
Study of calcium-K network evolution from Antarctica |
en |
dc.type |
Article |
en |