Determining field correlations produced by stars from the study of special changes in double slit experiment

dc.contributor.author	Kandpal, H. C.
dc.contributor.author	Mehta, D. S.
dc.contributor.author	Gopal, E. S. R.
dc.contributor.author	Vaishya, J. S.
dc.contributor.author	Sanwal, B. B.
dc.contributor.author	Singh, M.
dc.contributor.author	Sagar, R.
dc.date.accessioned	2009-08-07T07:01:57Z
dc.date.available	2009-08-07T07:01:57Z
dc.date.issued	2001
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/233
dc.description.abstract	Experiments are performed to determine the coherence properties of wave fields, produced by the broadband stellar sources on the earth surface, from the study of spectral changes produced on interference in the Young’s double slit experiment. The spectral degree of coherence obtained experimentally in this study for four bright stars in the wavelength range from 325 nm to 660 nm is in close agreement with the value that is expected theoretically from the known angular diameter of the stars. It is shown that the spectral degree of coherence obtained experimentally by this spectral interferometric technique could be used to determine the angular diameter of stars	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass280-209
dc.subject	Stars	en_US
dc.title	Determining field correlations produced by stars from the study of special changes in double slit experiment	en_US
dc.type	Article	en_US