Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3327
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dc.contributor.authorRamesh, R-
dc.contributor.authorSundararajan, M. S-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-09-02T11:06:49Z-
dc.date.available2008-09-02T11:06:49Z-
dc.date.issued2006-02-
dc.identifier.citationExperimental Astronomy, Vol. 21, No. 1, pp. 31 - 40en
dc.identifier.issn0922-6435-
dc.identifier.urihttp://hdl.handle.net/2248/3327-
dc.descriptionRestricted Accessen
dc.description.abstractA low frequency (40 150 MHz) radioheliograph for observations of the solar corona is in operation for the last few years at the Gauribidanur radio observatory, about 100 km north of Bangalore. The array has 32 antenna groups and a 1-bit digital correlator system consisting of 1024 channels is used as the back-end receiver. This paper describes the latter and results of the associated system tests.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/y3j262p53512241n/en
dc.subjectAperture Synthesisen
dc.subjectDigital Correlatoren
dc.subjectInterferometryen
dc.subjectRadio Telescopesen
dc.titleThe 1024 channel digital correlator receiver of the Gauribidanur radioheliographen
dc.typeArticleen
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