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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2708
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dc.contributor.authorSridharan, R-
dc.contributor.authorVenkatakrishnan, P-
dc.contributor.authorVerma, V. K-
dc.date.accessioned2008-07-16T06:26:50Z-
dc.date.available2008-07-16T06:26:50Z-
dc.date.issued2002-12-
dc.identifier.citationSolar Physics, Vol. 211, No. 1, pp. 395 - 410en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/2708-
dc.descriptionRestricted Accessen
dc.description.abstractA few methods of estimating Fried's parameter (r 0) from specklegrams of solar features are described. Some of these methods were used to estimate r 0 for the speckle data obtained from Kodaikanal Observatory (KO), Uttar Pradesh State Observatory (UPSO) and Udaipur Solar Observatory (USO). The average value of r 0 was found to be 3 cm at USO and UPSO during our observations. At KO, values of r 0 ranging from 6 to 10 cm were estimated.en
dc.format.extent122119 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/x18842k670141616/en
dc.subjectSpectral Ratio Methoden
dc.subjectObservatory Dataen
dc.subjectSpectrum Equalisationen
dc.subjectSpectral Ratioen
dc.subjectStellar Imagesen
dc.subjectSpeckle Imaging observations performed at KO, UPSO, and USOen
dc.titleEstimation of Fried's Parameter From Specklegrams of Solar Featuresen
dc.typeArticleen
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