Estimation of Fried's Parameter From Specklegrams of Solar Features

dc.contributor.author	Sridharan, R
dc.contributor.author	Venkatakrishnan, P
dc.contributor.author	Verma, V. K
dc.date.accessioned	2008-07-16T06:26:50Z
dc.date.available	2008-07-16T06:26:50Z
dc.date.issued	2002-12
dc.identifier.citation	Solar Physics, Vol. 211, No. 1, pp. 395 - 410	en
dc.identifier.issn	0038-0938
dc.identifier.uri	http://hdl.handle.net/2248/2708
dc.description	Restricted Access	en
dc.description.abstract	A 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.extent	122119 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/x18842k670141616/	en
dc.subject	Spectral Ratio Method	en
dc.subject	Observatory Data	en
dc.subject	Spectrum Equalisation	en
dc.subject	Spectral Ratio	en
dc.subject	Stellar Images	en
dc.subject	Speckle Imaging observations performed at KO, UPSO, and USO	en
dc.title	Estimation of Fried's Parameter From Specklegrams of Solar Features	en
dc.type	Article	en