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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5420
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dc.contributor.authorKathiravan, C-
dc.contributor.authorRamesh, R-
dc.contributor.authorBarve, Indrajit V-
dc.contributor.authorRajalingam, M-
dc.date.accessioned2011-03-15T10:55:35Z-
dc.date.available2011-03-15T10:55:35Z-
dc.date.issued2011-04-01-
dc.identifier.citationThe Astrophysical Journal, Vol. 730, No. 2, 91en
dc.identifier.urihttp://hdl.handle.net/2248/5420-
dc.descriptionOpen Accessen
dc.description.abstractWe carried out radio observations of the solar corona at 170 MHz during the eclipse of 2008 August 1, from the Gauribidanur observatory located about 100 km north of Bangalore in India. The results indicate the presence of a discrete radio source of very small angular dimension (≈15'') in the corona from where the observed radiation originated.en
dc.language.isoenen
dc.publisherInstitute of Physics Publishingen
dc.relation.urihttp://iopscience.iop.org/0004-637X/730/2/91/en
dc.rights© Institute of Physics Publishingen
dc.subjectEclipsesen
dc.subjectSun: coronaen
dc.subjectSun: radio radiationen
dc.subjectTechniques: high angular resolutionen
dc.titleRadio Observations of the Solar Corona During an Eclipseen
dc.typeArticleen
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