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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/244
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dc.contributor.authorChakraborty, P-
dc.contributor.authorSankarasubramanian, K-
dc.contributor.authorMajumder, S-
dc.contributor.authorRajesh Nayak, K-
dc.contributor.authorSridharan, R-
dc.contributor.authorJana, A. D-
dc.contributor.authorRajalakshmi, G-
dc.contributor.authorSuresh, D-
dc.contributor.authorAsgekar, A-
dc.contributor.authorGeetha, K. P-
dc.contributor.authorRajesh, C. K-
dc.date.accessioned2005-01-18T02:58:02Z-
dc.date.available2005-01-18T02:58:02Z-
dc.date.issued1997-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 13, pp. 69-74en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/244-
dc.description.abstractWhite light images of the solar corona were taken on KODAK 2415 films using 3-inch (f/11.5) telescopes fitted with SLR cameras. Observations were made from 4 different sites spread over the totality belt by four different teams. Table 1 gives the observation sites, the teams and the positions of the palces in the totality belt.en
dc.format.extent1030876 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectTotal solar eclipseen
dc.subjectwhite light photographyen
dc.subjectcoronal structuresen
dc.titlePhotometry of Solar Corona to Study the Coronal Structuresen
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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