dc.contributor.author |
Singh, J |
|
dc.contributor.author |
Muneer, S |
|
dc.contributor.author |
Bagare, S. P |
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dc.contributor.author |
Rangarajan, K. E |
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dc.contributor.author |
Ramesh, K. B |
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dc.contributor.author |
Varghese, B. A |
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dc.contributor.author |
Samson, J. P. A |
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dc.contributor.author |
Devendran, P |
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dc.contributor.author |
Hariharan, G |
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dc.date.accessioned |
2008-05-27T08:15:10Z |
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dc.date.available |
2008-05-27T08:15:10Z |
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dc.date.issued |
2003 |
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dc.identifier.citation |
BASI, Vol. 31, No. 2, pp. 111 - 115 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2350 |
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dc.description.abstract |
In this report we describe a digitizer developed in the laboratories of the Indian Institutes of Astrophysics (IIA) to digitize the large amount of solar synoptic data obtained since 1904 at Kodaikanal. We show a sample spectrum, an Hα Spectroheliogram, and a Ca+K spectroheliogram digitized using this equipment. The digitized data will be used to study the temporal variations in photospheric and chromospheric rotation rates, the solar differential rotation, the evolution of sunspots & Hα filaments, and in the evaluation of Ca+K plage and network indices. The digitized data will be made available to the scientific community as a part of IIA's astronomical data archive. |
en |
dc.format.extent |
153634 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.relation.uri |
http://adsabs.harvard.edu/abs/2003BASI...31..111S |
en |
dc.subject |
Digitization |
en |
dc.subject |
Spectroheliogram |
en |
dc.subject |
Solar synoptic data |
en |
dc.title |
Digitization of Kodaikanal Data |
en |
dc.type |
Article |
en |