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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2885
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dc.contributor.authorChinnappan, V-
dc.contributor.authorSaxena, A. K-
dc.contributor.authorSreenivasan, A-
dc.date.accessioned2008-07-25T06:34:47Z-
dc.date.available2008-07-25T06:34:47Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 815 - 817en
dc.identifier.urihttp://hdl.handle.net/2248/2885-
dc.description.abstractAtmospheric turbulence distorts the incoming wavefront from the star light, thus severely limiting the resolution of the groundbased optical telescopes (Fried 1966). Adaptive optics is being implemented in all big telescopes to remove the distortion created by the atmosphere. In this paper, we are dealing with the selection and testing of three types of high-speed imaging systems, a crucial component for wavefront sensing.en
dc.format.extent116068 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectAtmospheric Turbulenceen
dc.subjectCCDen
dc.titlePerformance evaluation of high-speed camera system for adaptive opticsen
dc.typeArticleen
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