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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5192
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dc.contributor.authorSankarasubramanian, K-
dc.contributor.authorHasan, S. S-
dc.contributor.authorRangarajan, K. E-
dc.date.accessioned2010-07-15T12:28:46Z-
dc.date.available2010-07-15T12:28:46Z-
dc.date.issued2010-
dc.identifier.citationHasan, S. S and Rutten, R. T., eds., Magnetic coupling between the interior and atmosphere of the Sun, Proceedings of the conference "Centenary commemoration of the discovery of the Evershed effect" Dec, 2 - 5, 2008, Indian Institute of Astrophysics, Bangalore, India, pp. 156 – 165en
dc.identifier.isbn978-3-642-02858-8-
dc.identifier.urihttp://hdl.handle.net/2248/5192-
dc.descriptionThe original publication is available at springerlink.comen
dc.descriptionRestricted Access-
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractIndia’s National Large Solar Telescope (NLST) will provide opportunities to observe the Sun with high spatial, spectral, and polarimetric resolution. The large aperture also enables high-cadence spectropolarimetry with moderate spatial resolution. A multi-slit spectropolarimeter is planned as one of the back-end instruments for this powerful telescope, primarily to measure vector magnetic fields in both active and quiet regions. An integral-field unit added with the multi-slit spectropolarimeter will enable fast-cadence observation. Here we discuss the scientific requirements for such an instrument, along with advantages and limitations of the concept and preliminary design details.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.ispartofseriesAstrophysics and Space Science Proceedings;-
dc.relation.urihttp://dx.doi.org/10.1007/978-3-642-02859-5_12en
dc.rights© Springeren
dc.titleSpectropolarimetry with the NLSTen
dc.typeArticleen
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