Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5540
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dc.contributor.authorRoopashree, M. B-
dc.contributor.authorVyas, A-
dc.contributor.authorPrasad, B. R-
dc.date.accessioned2011-08-02T17:02:43Z-
dc.date.available2011-08-02T17:02:43Z-
dc.date.issued2011-07-
dc.identifier.citationAdaptive Optics: Methods, Analysis and Applications, OSA Technical Digest, JMB3.en
dc.identifier.urihttp://hdl.handle.net/2248/5540-
dc.descriptionRestricted Accessen
dc.description.abstractAtmospheric phase screens are used for numerical evaluation of large telescope systems. In this paper, we optimized the grid size of the simulated phase screens in terms of the error in the structure function assuming a Kolmogorov turbulence model.en
dc.language.isoenen
dc.publisherOptical Society of Americaen
dc.relation.urihttp://www.opticsinfobase.org/abstract.cfm?URI=AO-2011-JMB3en
dc.rights© Optical Society of Americaen
dc.titleGrid size optimization for atmospheric turbulence phase screen simulationsen
dc.typeArticleen
Appears in Collections:IIAP Publications

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