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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2522
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dc.contributor.authorSridharan, R-
dc.contributor.authorRaja Bayanna, A-
dc.contributor.authorSrivastava, N-
dc.contributor.authorKumar, B-
dc.contributor.authorRavindra, B-
dc.contributor.authorGupta, S. K-
dc.contributor.authorJain, N-
dc.contributor.authorAmbastha, A-
dc.contributor.authorVenkatakrishnan, P-
dc.date.accessioned2008-06-27T09:31:53Z-
dc.date.available2008-06-27T09:31:53Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 455 - 456en
dc.identifier.urihttp://hdl.handle.net/2248/2522-
dc.description.abstractAdaptive Optics (AO) systems improve the resolution of ground based telescopes and allow for long exposure images. Their performance depends on the seeing conditions at the time of observations. In this paper, we evaluate the performance of an AO system under various seeing conditions through simulations. Then we present the wave-front sensing and correction schemes that would be used in the first phase of the AO system to be developed at the Udaipur Solar Observatory.en
dc.format.extent67032 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..455Sen
dc.subjectHigh resolution imagingen
dc.subjectAdaptive opticsen
dc.titlePerformance Evaluation of Adaptive Optics Systemsen
dc.typeArticleen
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