Estimating slow intensity fluctuations from short data stretches - The case of pulsar scintillation

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2635

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DC Field	Value	Language
dc.contributor.author	Deshpande, A.A.	-
dc.contributor.author	Nityananda, R.	-
dc.date.accessioned	2007-06-08T09:26:41Z	-
dc.date.available	2007-06-08T09:26:41Z	-
dc.date.issued	1990	-
dc.identifier.citation	URSI/IAU Symposium on Radio Astronomical Seeing, Beijing, People's Republic of China, May 15-19, 1989, Proceedings. Beijing/Oxford, International Academic Publishers/Pergamon Press, 1990, p262-265	en
dc.identifier.uri	http://hdl.handle.net/2289/2635	-
dc.description	Restricted Access.	en
dc.format.extent	147586 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Pergamon Press	en
dc.rights	1990 Pergamon Press	en
dc.title	Estimating slow intensity fluctuations from short data stretches - The case of pulsar scintillation	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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