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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3132
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dc.contributor.authorRamesh, R-
dc.contributor.authorSubramanian, K. R-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-08-14T09:46:05Z-
dc.date.available2008-08-14T09:46:05Z-
dc.date.issued1999-03-
dc.identifier.citationSolar Physics, Vol. 185, No. 1, pp. 77 - 85en
dc.identifier.urihttp://hdl.handle.net/2248/3132-
dc.description.abstractWe report here on high angular resolution observations of solar noise storm sources at a frequency of 75MHz. The data for the study were obtained at the Gauribidanur Radio Observatory (long.: 77 deg26'12''E, lat.: 13 deg36'12''N) about 100km north of Bangalore, India, during the solar eclipse of 24October 1995. Our main conclusion is that there are structures of angular size <=2.5arcmin in the outer solar corona.en
dc.format.extent128908 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://www.springerlink.com/content/k76784k767q13967/en
dc.subjectEclipse Observationsen
dc.subjectOuter Solar Coronaen
dc.titleEclipse Observations of Compact Sources in the Outer Solar Coronaen
dc.typeArticleen
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