Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4343
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dc.contributor.authorKrishan, V-
dc.date.accessioned2009-02-05T11:49:21Z-
dc.date.available2009-02-05T11:49:21Z-
dc.date.issued1980-02-
dc.identifier.citationPlasma Physics, Vol. 22, No. 2, pp. 163 - 173en
dc.identifier.issn0022-3778-
dc.identifier.urihttp://hdl.handle.net/2248/4343-
dc.descriptionRestricted Access-
dc.description.abstractA possible mechanism for the direct generation of electromagnetic modes of frequencies near the electron plasma frequency, is suggested. The spatial variation of the interplanetary magnetic field seems to play an essential role for the excitation of the type III radio bursts. The values of the frequency drift rate and the characteristic rise time of the bursts compare well with the observations.en
dc.language.isoenen
dc.publisherInstitute of Physicsen
dc.relation.urihttp://www.iop.org/EJ/abstract/0032-1028/22/2/005/en
dc.subjectElectron Plasmaen
dc.subjectPlasma Frequenciesen
dc.subjectPlasma-Electromagnetic Interactionen
dc.subjectPlasma-Particle Interactionsen
dc.subjectSolar Winden
dc.subjectBessel Functionsen
dc.subjectElectron Beamsen
dc.subjectInterplanetary Magnetic Fieldsen
dc.subjectPlasma Oscillationsen
dc.subjectSpatial Dependenciesen
dc.subjectType 3 Burstsen
dc.titleDirect generation of electromagnetic radiation from a beam-plasma systemen
dc.typeArticleen
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