Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5580
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dc.contributor.authorSaxena, A. K-
dc.contributor.authorLancelot, J. P-
dc.contributor.authorSamson, J. P-
dc.date.accessioned2011-09-26T10:59:41Z-
dc.date.available2011-09-26T10:59:41Z-
dc.date.issued1993-12-
dc.identifier.citationProceedings of SPIE; Vol. 2003, pp. 88-97en
dc.identifier.urihttp://hdl.handle.net/2248/5580-
dc.descriptionRestricted Accessen
dc.description.abstractIndia is planning to build a large Optical/Infrared Telescope of 4 to 5 M in size. This telescope will adopt most of the features of the New Technology Telescope including active and adoptive optics corrections for achieving improved image quality. Keeping this in view a prototype active optics system for a 27 inch thin mirror is being developed at Indian Institute of Astrophysics. A new digital polarization shearing interferometer will be used for wavefront sensing. The paper describes in detail the procedure for wavefront sensing and the approach for the active correction.en
dc.language.isoenen
dc.publisherSPIE-The International Society for Optical Engineeringen
dc.relation.ispartofseriesProceedings of SPIE; Vol. 2003-
dc.relation.urihttp://dx.doi.org/10.1117/12.165442en
dc.rights© SPIE-The International Society for Optical Engineeringen
dc.titleDevelopment of an active-optics system for 27-inch thin mirroren
dc.typeArticleen
Appears in Collections:IIAP Publications

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