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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2794
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dc.contributor.authorKapoor, R. C-
dc.contributor.authorShukre, C. S-
dc.date.accessioned2008-07-22T07:44:03Z-
dc.date.available2008-07-22T07:44:03Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 695 - 696en
dc.identifier.urihttp://hdl.handle.net/2248/2794-
dc.description.abstractBy attributing the often seen longitude offsets between the core and conal component centres of pulsar radio pulses to different emission altitudes, we present a new method for investigating these altitudes. OUf method can explain these offsets and also sheds light on them.en
dc.format.extent33677 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectRadio Pulsar Emission Altitudesen
dc.subjectMagnetic Field Lineen
dc.titleRadio pulsar emission altitudesen
dc.typeArticleen
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