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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1483
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dc.contributor.authorKariyappa, R-
dc.contributor.authorJayarajan, A. P-
dc.contributor.authorRaheem, K. C. A-
dc.contributor.authorSivaraman, K. R-
dc.date.accessioned2007-04-17T07:18:33Z-
dc.date.available2007-04-17T07:18:33Z-
dc.date.issued1993-06-
dc.identifier.citationBASI, Vol. 21, No.2, pp. 139-142en
dc.identifier.urihttp://hdl.handle.net/2248/1483-
dc.description.abstractWe have described the double-pass spectrograph built at the Indian Institute of Astrophysics. Measurements of the scattered light within the spectrograph using the photoelectric scans of the NaI D-lines show that this is a good near-scatter-free system. This instrument is used to monitor the disk integrated CaII K line profile of the Sun on a regular basisen
dc.format.extent8101296 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectDouble -passen
dc.subjectCa II K-line profilesen
dc.titleA double-pass spectrograph for solar researchen
dc.typeArticleen
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