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dc.contributor.authorYoon, Peter H.pt_BR
dc.contributor.authorZiebell, Luiz Fernandopt_BR
dc.date.accessioned2014-09-23T02:12:34Zpt_BR
dc.date.issued1995pt_BR
dc.identifier.issn1063-651Xpt_BR
dc.identifier.urihttp://hdl.handle.net/10183/103645pt_BR
dc.description.abstractA quasilinear analysis of the relativistic electron cyclotron maser instability is presented. A background plasma is assumed to support the wave motion, while the instability is driven by a tenuous population of energetic electrons possessing a loss-cone feature. The analysis makes use of an efBcient moment method. In this approach, evolution equations for the moments of particle distribution function are derived from the particle kinetic equation. Then, a self-similar model of the loss-cone electron distribution function is imposed. Simultaneously, the wave kinetic equation is solved. The resulting fully self-consistent set of equations that governs the evolution of the particles and unstable waves is solved numerically under physical parameters that represent typical solar microwave burst sources.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofPhysical Review. E, Statistical physics, plasmas, fluids and related interdisciplinary topics. New York. Vol. 51, no. 5, part b (May 1995), p. 4908-4916pt_BR
dc.rightsOpen Accessen
dc.subjectPlasmaspt_BR
dc.subjectOndas : Oscilacoespt_BR
dc.subjectInstabilidades em plasmaspt_BR
dc.subjectMaserspt_BR
dc.titleQuasilinear evolution of cyclotron maser instabilitypt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000140535pt_BR
dc.type.originEstrangeiropt_BR


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