Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4731
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dc.contributor.authorNagaraju, K-
dc.contributor.authorSankarasubramanian, K-
dc.contributor.authorRangarajan, K. E-
dc.contributor.authorRamesh, K. B-
dc.contributor.authorSingh, J-
dc.contributor.authorDevendran, P-
dc.contributor.authorHariharan-
dc.date.accessioned2009-08-07T10:18:26Z-
dc.date.available2009-08-07T10:18:26Z-
dc.date.issued2008-09-
dc.identifier.citationBulletin of the Astronomical Society of India, Vol. 36, No. 2 & 3, pp. 99 – 110en
dc.identifier.issn0304-9523-
dc.identifier.urihttp://hdl.handle.net/2248/4731-
dc.description.abstractCalibration and characterization of a dual-beam polarimeter installed at Kodaikanal Tower Telescope (KTT) for spectropolarimetric observations are presented in this paper. It was found that a slit width of 48 μ is optimum for the spectrograph setup at KTT and corresponding spectral resolution is 32.47 m\AA. It was demonstrated that the precision in polarization measurement can be achieved better than 0.1 % by increasing the exposure time. However, the polarimetric calibration accuracy is limited to 0.35% for Stokes Q and U parameters and 0.2% for Stokes V parameter, mainly due to the uncertainty in the retardance of the calibration retarder. A comparison of the magnetic field measurement between the Solar Optical Telescope (SOT) onboard Hinode and KTT for an active region was made and a good match was found after spatial smearing of Hinode/SOT measurements by 5.12''.en
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://www.ncra.tifr.res.in/~basi/08JunSep/BASI_ABS/36992008.htmen
dc.rights© Astronomical Society of Indiaen
dc.subjectInstrumentation: Polarimeteren
dc.titleOn the performance of a dual-beam polarimeter at Kodaikanal tower telescopeen
dc.typeArticleen
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