Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4726
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dc.contributor.authorMonstein, C-
dc.contributor.authorRamesh, R-
dc.contributor.authorKathiravan, C-
dc.date.accessioned2009-08-06T10:39:10Z-
dc.date.available2009-08-06T10:39:10Z-
dc.date.issued2007-12-
dc.identifier.citationBulletin of the Astronomical Society of India, Vol. 35, No. 4, pp. 473 - 480en
dc.identifier.issn0304-9523-
dc.identifier.urihttp://hdl.handle.net/2248/4726-
dc.description.abstractDuring a campaign in December 2006, radio spectrum measure- ments over the frequency range 45-870 MHz were carried out at the Gauribida- nur observatory, located about 100 km north of Bangalore. The spectrometer used for the above purpose was subsequently configured for radio spectral ob- servations of the solar corona. This paper describes, (i) radio frequency inter- ference over some of the frequency bands `protected' for radio astronomy; and (ii) `first' solar radio burst observation and the above instrument.en
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://www.ncra.tifr.res.in/~basi/07December/Abstracts/354732007.htmen
dc.rights© Astronomical Society of Indiaen
dc.subjectSun: Coronaen
dc.subjectSolar Flaresen
dc.subjectRadio Observationsen
dc.subjectRadio Frequency Interference (RFI)en
dc.titleRadio spectrum measurements at the Gauribidanur observatoryen
dc.typeArticleen
Appears in Collections:BASI Publications
IIAP Publications

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