Micro-fluctuations of fried's parameter (ro)

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4990

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DC Field	Value	Language
dc.contributor.author	Saha, S. K	-
dc.contributor.author	Yeswanth, L	-
dc.date.accessioned	2010-01-16T15:11:35Z	-
dc.date.available	2010-01-16T15:11:35Z	-
dc.date.issued	2004	-
dc.identifier.citation	Asian Journal of Physics, Vol. 13, No. 3 - 4, pp. 227 - 232	en
dc.identifier.issn	0971-3063	-
dc.identifier.uri	http://hdl.handle.net/2248/4990	-
dc.description.abstract	The atmospheric coherence is a highly variable parameter depending upon the high velocity wind. The size of the atmospheric coherence length widely known as, Fried's parameter, ro, has been computed during night at the Cassegrain focus of the 2.34 meter Vainu Bappu Telescope (VBT), Vainu Bappu Observatory (VBO), Kavalur, India, using the speckle interferometric technique. The variation of ro value at a different interval during the night is also computed. Measurements of ro at a step of ~100 milliseconds (msec) have been carried out.	en
dc.language.iso	en	en
dc.publisher	Anita Publications	en
dc.rights	© Anita Publications	en
dc.subject	Micro-fluctuations	en
dc.subject	Frieds Parameter	en
dc.subject	Speckle Interferometric Technique	en
dc.title	Micro-fluctuations of fried's parameter (ro)	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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