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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/647
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dc.contributor.authorShelke, R. N-
dc.contributor.authorPande, M. C-
dc.date.accessioned2005-12-07T07:22:56Z-
dc.date.available2005-12-07T07:22:56Z-
dc.date.issued1985-03-
dc.identifier.citationBASI, Vol. 13, No. 1, pp 62-67en
dc.identifier.urihttp://hdl.handle.net/2248/647-
dc.description.abstractWe present an analysis which indicates that in several cases coronal holes exist in the vicinity of the active regions producing type II bursts. It is inferred that shock waves which produce type II bursts essentially travel along the coronal magnetic field.en
dc.format.extent497967 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectType II burstsen
dc.subjectCoronal holesen
dc.subjectThe Sunen
dc.titlePropagation of type II burst shock waves along the radial magnetic field in the solar coronaen
dc.typeArticleen
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