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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1003
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dc.contributor.authorAnanda Rao, B. G-
dc.contributor.authorAshok, N. M-
dc.contributor.authorChandrasekhar, T-
dc.contributor.authorDesai, J. N-
dc.contributor.authorNanda Kumar, M. S-
dc.date.accessioned2006-06-13T11:54:59Z-
dc.date.available2006-06-13T11:54:59Z-
dc.date.issued1997-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 13, pp. 113en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/1003-
dc.description.abstractWe have obtained Fabry-Perot Interferograms of the solar corona during the 1995 total solar eclipse, in two emission lines, Fe X line at 6374Å and Fe XIV line at s303 Å. We have also obtained a Fabry-perot-gram of the corona in the high temperature Ca XV Å line at 569 4 nm. The Co. XV FP-gram showed two concentrated blobs of emission from the equatorial regions of the Sun.-
dc.format.extent864297 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Institute of Astrophysicsen
dc.titleSpectroscopic studies of the solar corona during total solar eclipse of October 24, 1995en
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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