Quasilinear analysis of loss-cone driven weakly relativistic electron cyclotron maser instability

Detalhes bibliográficos
Autor(a) principal: Ziebell, Luiz Fernando
Data de Publicação: 1995
Outros Autores: Yoon, Peter H.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/189486
Resumo: This paper presents a quasilinear analysis of the relativistic electron cyclotron maser instability. Two electron popUlations are assumed: a low-temperature background component and a more energetic loss-cone population. The dispersion relation is valid for any ratio of the energetic to cold populations, and includes thermal and relativistic effects. The quasilinear analysis is based upon·an efficient kinetic moment method, in which various moment equations are derived from the particle kinetic equation. A model time-dependent loss-cone electron distributidn function is assumed, which allows one to evaluate the instantaneous linear growth rate as well as the moment kinetic equations. These moment equations along with the wave kinetic equation form a fully self-consistent set of equations which governs the evolution of the particles as well as unstable waves.' This set of equations is solved with physical parameters typical of the earth's auroral zone plasma.
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spelling Ziebell, Luiz FernandoYoon, Peter H.2019-03-21T02:29:29Z19951070-664Xhttp://hdl.handle.net/10183/189486000262668This paper presents a quasilinear analysis of the relativistic electron cyclotron maser instability. Two electron popUlations are assumed: a low-temperature background component and a more energetic loss-cone population. The dispersion relation is valid for any ratio of the energetic to cold populations, and includes thermal and relativistic effects. The quasilinear analysis is based upon·an efficient kinetic moment method, in which various moment equations are derived from the particle kinetic equation. A model time-dependent loss-cone electron distributidn function is assumed, which allows one to evaluate the instantaneous linear growth rate as well as the moment kinetic equations. These moment equations along with the wave kinetic equation form a fully self-consistent set of equations which governs the evolution of the particles as well as unstable waves.' This set of equations is solved with physical parameters typical of the earth's auroral zone plasma.application/pdfengPhysics of plasmas. Woodbury. Vol. 2, n. 4 (Apr. 1995), p. 1285-1295PlasmasInstabilidades em plasmasInstabilidade de cone de perda : EletronsQuasilinear analysis of loss-cone driven weakly relativistic electron cyclotron maser instabilityEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSTEXT000262668.pdf.txt000262668.pdf.txtExtracted Texttext/plain46431http://www.lume.ufrgs.br/bitstream/10183/189486/2/000262668.pdf.txte05b36a551eb10f73dfa8c44a36de00cMD52ORIGINAL000262668.pdfTexto completo (Inglês)application/pdf956823http://www.lume.ufrgs.br/bitstream/10183/189486/1/000262668.pdf875cd702686c60640bb02caf97dff0b0MD5110183/1894862023-09-24 03:37:16.740506oai:www.lume.ufrgs.br:10183/189486Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-09-24T06:37:16Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Quasilinear analysis of loss-cone driven weakly relativistic electron cyclotron maser instability
title Quasilinear analysis of loss-cone driven weakly relativistic electron cyclotron maser instability
spellingShingle Quasilinear analysis of loss-cone driven weakly relativistic electron cyclotron maser instability
Ziebell, Luiz Fernando
Plasmas
Instabilidades em plasmas
Instabilidade de cone de perda : Eletrons
title_short Quasilinear analysis of loss-cone driven weakly relativistic electron cyclotron maser instability
title_full Quasilinear analysis of loss-cone driven weakly relativistic electron cyclotron maser instability
title_fullStr Quasilinear analysis of loss-cone driven weakly relativistic electron cyclotron maser instability
title_full_unstemmed Quasilinear analysis of loss-cone driven weakly relativistic electron cyclotron maser instability
title_sort Quasilinear analysis of loss-cone driven weakly relativistic electron cyclotron maser instability
author Ziebell, Luiz Fernando
author_facet Ziebell, Luiz Fernando
Yoon, Peter H.
author_role author
author2 Yoon, Peter H.
author2_role author
dc.contributor.author.fl_str_mv Ziebell, Luiz Fernando
Yoon, Peter H.
dc.subject.por.fl_str_mv Plasmas
Instabilidades em plasmas
Instabilidade de cone de perda : Eletrons
topic Plasmas
Instabilidades em plasmas
Instabilidade de cone de perda : Eletrons
description This paper presents a quasilinear analysis of the relativistic electron cyclotron maser instability. Two electron popUlations are assumed: a low-temperature background component and a more energetic loss-cone population. The dispersion relation is valid for any ratio of the energetic to cold populations, and includes thermal and relativistic effects. The quasilinear analysis is based upon·an efficient kinetic moment method, in which various moment equations are derived from the particle kinetic equation. A model time-dependent loss-cone electron distributidn function is assumed, which allows one to evaluate the instantaneous linear growth rate as well as the moment kinetic equations. These moment equations along with the wave kinetic equation form a fully self-consistent set of equations which governs the evolution of the particles as well as unstable waves.' This set of equations is solved with physical parameters typical of the earth's auroral zone plasma.
publishDate 1995
dc.date.issued.fl_str_mv 1995
dc.date.accessioned.fl_str_mv 2019-03-21T02:29:29Z
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dc.relation.ispartof.pt_BR.fl_str_mv Physics of plasmas. Woodbury. Vol. 2, n. 4 (Apr. 1995), p. 1285-1295
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