Micro-fluctuations of fried's parameter (ro)

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