Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3070
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dc.contributor.authorRamesh, R-
dc.date.accessioned2008-08-12T08:55:01Z-
dc.date.available2008-08-12T08:55:01Z-
dc.date.issued2000-12-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 21, No. 3 – 4, pp. 237 - 240en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3070-
dc.description.abstractWe present observations of the 'quiet' Sun close to the recent solar minimum (Cycle 22), with the Gauribidanur radioheliograph. Our main conclusion is that coronal streamers also influence the observed radio brightness temperature.en
dc.format.extent333230 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000JApA...21..237Ren
dc.subjectSunen
dc.subjectCoronaen
dc.subjectRadio Observationsen
dc.subjectStreamersen
dc.subjectScatteringen
dc.titleLow Frequency Radio Emission from the 'Quiet Sun'en
dc.typeArticleen
Appears in Collections:IIAP Publications

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