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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4079
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dc.contributor.authorKrishan, V-
dc.date.accessioned2008-12-16T14:33:21Z-
dc.date.available2008-12-16T14:33:21Z-
dc.date.issued1978-08-
dc.identifier.citationAstrophysics and Space Science, Vol. 57, No. 1, pp. 191 - 194en
dc.identifier.issn0004-640X (Print) 1572-946X (Online)-
dc.identifier.urihttp://hdl.handle.net/2248/4079-
dc.descriptionOpen Access-
dc.description.abstractThe nonlinear theory of electromagnetic modes in the radio frequency range, excited from a system consisting of two contra-streaming electron beams, supports the experimental observation that out of w~(n + ½)w/subce,w = 3/2w/subce is the most prominent mode.en
dc.language.isoenen
dc.publisherD.Reidel Publishing Co.,en
dc.relation.urihttp://adsabs.harvard.edu/abs/1978Ap%26SS..57..191Ken
dc.relation.urihttp://dx.doi.org/10.1007/BF00639055en
dc.rightsD.Reidel Publishing Co.,-
dc.subjectEarth Magnetosphereen
dc.subjectElectron Beamsen
dc.subjectNonlinear Systemsen
dc.subjectPlasma-Electromagnetic Interactionen
dc.subjectPlasma-Particle Interactionsen
dc.subjectPropagation Modesen
dc.subjectAmplitudesen
dc.subjectAuroral Zonesen
dc.subjectCyclotron Frequencyen
dc.subjectElectron Energyen
dc.titleNonlinear analysis of two contra-streaming electron beams - plasma systemen
dc.typeArticleen
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