Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7216
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dc.contributor.authorSreekanth Reddy, V-
dc.contributor.authorBanyal, R. K-
dc.contributor.authorSridharan, R-
dc.contributor.authorAishwarya, S-
dc.date.accessioned2020-11-19T13:09:29Z-
dc.date.available2020-11-19T13:09:29Z-
dc.date.issued2019-05-
dc.identifier.citationResearch in Astronomy and Astrophysics, Vol. 19, No. 5, 74en_US
dc.identifier.issn1674-4527-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7216-
dc.descriptionRestricted Access © IOP Publishing https://doi.org/10.1088/1674-4527/19/5/74en_US
dc.description.abstractWe report atmospheric turbulence parameters, namely atmospheric seeing, tilt-anisoplanatic angle (θ0) and coherence time (τ0), measured under various sky conditions, at Vainu Bappu Observatory in Kavalur. Bursts of short exposure images of selected stars were recorded with a high-speed, frame-transfer CCD mounted on the Cassegrain focus of a newly commissioned 1.3 m telescope. The estimated median seeing is ≈ 1.85′′ at wavelength of ∼ 600 nm, the image motion correlation between different pairs of stars is ∼ 44% for θ0 ≈ 36′′ and mean τ0 is ≈ 2.4 ms. This work was motivated by the design considerations and expected performance of an adaptive optics system that is currently being planned for the telescope.en_US
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.subjectAtmospheric effectsen_US
dc.subjectTurbulenceen_US
dc.subjectInstrumentation: adaptive opticsen_US
dc.subjectcatalogsen_US
dc.subjectMethods: observationalen_US
dc.titleMeasurements of atmospheric turbulence parameters at Vainu Bappu Observatory using short-exposure CCD imagesen_US
dc.typeArticleen_US
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