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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4061
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dc.contributor.authorRamesh, R-
dc.contributor.authorKathiravan, C-
dc.contributor.authorSundararajan, M. S-
dc.contributor.authorBarve, Indrajit V-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-12-15T14:21:03Z-
dc.date.available2008-12-15T14:21:03Z-
dc.date.issued2008-12-
dc.identifier.citationSolar Physics, Vol. 253, No. 1 - 2, pp. 319 - 327en
dc.identifier.issn0038-0938 (Print) 1573-093X (Online)-
dc.identifier.urihttp://hdl.handle.net/2248/4061-
dc.descriptionRestricted Access.en
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractAn interferometer antenna system to observe polarized radio emission from the solar corona at different frequencies in the range 30-110 MHz has been commissioned recently by the Indian Institute of Astrophysics at the Gauribidanur Radio Observatory (latitude 13°36'12''N and longitude 77°27'07''E), about 100 km north of Bangalore( http://www.iiap.res.in/centres_radio.htm ). This paper describes the antenna system, associated analog/digital receiver setup, calibration scheme, and preliminary results.en
dc.language.isoenen
dc.publisherSpringer Netherlandsen
dc.relation.urihttp://www.springerlink.com/content/p33772pj73h60332/en
dc.rights© Springeren
dc.subjectMagnetic Fieldsen
dc.subjectSolar Coronaen
dc.subjectRadio Observationsen
dc.subjectPolarizationen
dc.titleA low-frequency (30-110 MHz) Antenna system for observations of polarized radio emission from the solar coronaen
dc.typeArticleen
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