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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3071
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dc.contributor.authorSankarasubramanian, K-
dc.contributor.authorSrinivasulu, G-
dc.contributor.authorAnanth, A. V-
dc.contributor.authorVenkatakrishnan, P-
dc.date.accessioned2008-08-12T08:55:30Z-
dc.date.available2008-08-12T08:55:30Z-
dc.date.issued2000-12-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 21, No. 3 – 4, pp. 241 - 244en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3071-
dc.description.abstractA Stokes Polarimeter has been developed using a masked CCD arrangement for the measurement of the vector magnetic field of sunspots. Charge shifting within the CCD is used to record near simul taneous orthogonal polarisation. The testing of the Stokes Polarimeter and the behavior of the integrated system combined with the Kodaikanal tower tunnel telescope will be discussed.en
dc.format.extent75486 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000JApA...21..241Sen
dc.subjectSolar Polarimetryen
dc.subjectCharge Shiftingen
dc.subjectvector magnetic fielden
dc.titleStokes Polarimetry at the Kodiakanal Tower Tunnel Telescopeen
dc.typeArticleen
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