Quasilinear analysis of loss-cone driven weakly relativistic electron cyclotron maser instability
Autor(a) principal: | |
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Data de Publicação: | 1995 |
Outros Autores: | |
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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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 |
dc.type.driver.fl_str_mv |
Estrangeiro info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10183/189486 |
dc.identifier.issn.pt_BR.fl_str_mv |
1070-664X |
dc.identifier.nrb.pt_BR.fl_str_mv |
000262668 |
identifier_str_mv |
1070-664X 000262668 |
url |
http://hdl.handle.net/10183/189486 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
Physics of plasmas. Woodbury. Vol. 2, n. 4 (Apr. 1995), p. 1285-1295 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
reponame:Repositório Institucional da UFRGS instname:Universidade Federal do Rio Grande do Sul (UFRGS) instacron:UFRGS |
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institution |
UFRGS |
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Repositório Institucional da UFRGS |
collection |
Repositório Institucional da UFRGS |
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