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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2948
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dc.contributor.authorEbenezer, E-
dc.contributor.authorRamesh, R-
dc.contributor.authorSubramanian, K. R-
dc.contributor.authorSundararajan, M. S-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-07-31T04:51:10Z-
dc.date.available2008-07-31T04:51:10Z-
dc.date.issued2001-03-
dc.identifier.citationAstronomy and Astrophysics, Vol. 367, No. 3, pp. 1112 – 1116en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/2948-
dc.description.abstractA new digital spectrograph for obtaining a dynamic spectrum of radio burst emission from the Sun in the frequency range 30-80 MHz has been recently commissioned at the Gauribidanur Radio Observatory (Lat: 13degr 36\arcmin12\arcsec N and Long: 77degr 27\arcmin07\arcsec E), about 100 km north of Bangalore, India. This paper describes various aspects of the antenna system, frontend receiver and digital hardware of the spectrograph. Some of the initial results obtained with the instrument are also presented.en
dc.format.extent273067 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.relation.urihttp://www.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aa/abs/2001/09/aa10166/aa10166.htmlen
dc.subjectSun: Coronaen
dc.subjectRadio Radiationen
dc.subjectInstrumentation: Spectrographen
dc.titleA new digital spectrograph for observations of radio burst emission from the Sunen
dc.typeArticleen
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