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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3061
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dc.contributor.authorRamesh, R-
dc.contributor.authorKathiravan, C-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-08-12T08:46:24Z-
dc.date.available2008-08-12T08:46:24Z-
dc.date.issued2001-02-
dc.identifier.citationAstrophysical Journal, Vol. 548, No. 2, pp. L229 - L231en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/3061-
dc.description.abstractWe report two-dimensional, low-frequency radio observations of the angular broadening of the Crab Nebula (Taurus A) due to a coronal mass ejection (CME), at a distance of ~41 Rsolar from the Sun. The estimated electron density in the CME is about 50 times greater than that of the ambient corona at that location. The calculated mass agrees approximately with that reported earlier for similar events at large distances from the Sun.en
dc.format.extent272196 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Astronomical Societyen
dc.relation.urihttp://www.journals.uchicago.edu/doi/abs/10.1086/319098en
dc.subjectScatteringen
dc.subjectSun: Solar-terrestrial Relationsen
dc.subjectSun: Activityen
dc.subjectSun: Coronaen
dc.subjectSun: Radio Radiationen
dc.titleLow-Frequency Radio Observations of the Angular Broadening of the Crab Nebula Due to a Coronal Mass Ejectionen
dc.typeArticleen
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