Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4134
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dc.contributor.authorKrishan, V-
dc.date.accessioned2008-12-19T10:35:53Z-
dc.date.available2008-12-19T10:35:53Z-
dc.date.issued1982-01-
dc.identifier.citationPlasma Physics, Vol. 24, No. 1, pp. 31 - 36en
dc.identifier.issn1876-5343-
dc.identifier.urihttp://hdl.handle.net/2248/4134-
dc.descriptionRestricted Access-
dc.description.abstractThe excitation of electromagnetic radiation near the harmonics of electron plasma frequency from a helical electron beam travelling parallel to a helical magnetic field through a stationary inhomogeneous plasma is studied. The motivation behind this study is to explain the observed characteristics of the type III solar radio bursts and thus to predict the nature of the plasma system responsible for the generation of these radio bursts.en
dc.language.isoenen
dc.publisherInstitute of Physicsen
dc.relation.urihttp://dx.doi.org/10.1088/0032-1028/24/1/003en
dc.subjectElectron Beamsen
dc.subjectMagnetic Field Configurationsen
dc.subjectNonuniform Plasmasen
dc.subjectPlasma Frequenciesen
dc.subjectType 3 Burstsen
dc.subjectElectromagnetic Radiationen
dc.subjectMagnetic Dispersionen
dc.subjectPhotosphereen
dc.subjectSolar Magnetic Fielden
dc.titleRadio emission from a helical electron beam-plasma system in a twisted magnetic fielden
dc.typeArticleen
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