Phase and gain adjustment of the Ooty radio telescope

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/5205

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DC Field	Value	Language
dc.contributor.author	Sarma, N.V.G.	-
dc.contributor.author	Joshi, M.N.	-
dc.contributor.author	Ananthakrishnan, S.	-
dc.date.accessioned	2012-08-06T09:43:48Z	-
dc.date.available	2012-08-06T09:43:48Z	-
dc.date.issued	1975	-
dc.identifier.citation	Journal of the Institution of Electronics and Telecommunications Engineering, 1975, Vol.21, p107	en
dc.identifier.uri	http://hdl.handle.net/2289/5205	-
dc.description	Restricted Access.	en
dc.description.abstract	The methods used for gain and phase adjustment of the 22 sections of the 530 m long cylindrical radio telescope at Ootacamund which operates at 326.5 MHz are described. Periodic adjustments are made by observing strong radio sources. A monitoring system using the modulated reflection technique has been installed for rapid measurements.	en
dc.language.iso	en	en
dc.publisher	The Institution of Electronics and Telecommunication Engineers	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1975JIETE..21..107S	en
dc.rights	1975 IETE	en
dc.title	Phase and gain adjustment of the Ooty radio telescope	en
dc.type	Article	en
Appears in Collections:	Research Papers (SCM)

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