Obliquely propagating electromagnetic waves in magnetized kappa plasmas

Detalhes bibliográficos
Autor(a) principal: Gaelzer, Rudi
Data de Publicação: 2016
Outros Autores: Ziebell, Luiz Fernando
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/189586
Resumo: Velocity distribution functions (VDFs) that exhibit a power-law dependence on the high-energy tail have been the subject of intense research by the plasma physics community. Such functions, known as kappa or superthermal distributions, have been found to provide a better fitting to the VDFs measured by spacecraft in the solar wind. One of the problems that is being addressed on this new light is the temperature anisotropy of solar wind protons and electrons. In the literature, the general treatment for waves excited by (bi-)Maxwellian plasmas is well-established. However, for kappa distributions, the wave characteristics have been studied mostly for the limiting cases of purely parallel or perpendicular propagation, relative to the ambient magnetic field. Contributions to the general case of obliquely propagating electromagnetic waves have been scarcely reported so far. The absence of a general treatment prevents a complete analysis of the wave-particle interaction in kappa plasmas, since some instabilities can operate simultaneously both in the parallel and oblique directions. In a recent work, Gaelzer and Ziebell [J. Geophys. Res. 119, 9334 (2014)] obtained expressions for the dielectric tensor and dispersion relations for the low-frequency, quasi-perpendicular dispersive Alfv en waves resulting from a kappa VDF. In the present work, the formalism is generalized for the general case of electrostatic and/or electromagnetic waves propagating in a kappa plasma in any frequency range and for arbitrary angles. An isotropic distribution is considered, but the methods used here can be easily applied to more general anisotropic distributions such as the bi-kappa or product-bi-kappa. VC 2016 AIP Publishing LLC.
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spelling Gaelzer, RudiZiebell, Luiz Fernando2019-03-27T04:06:15Z20161070-664Xhttp://hdl.handle.net/10183/189586000995850Velocity distribution functions (VDFs) that exhibit a power-law dependence on the high-energy tail have been the subject of intense research by the plasma physics community. Such functions, known as kappa or superthermal distributions, have been found to provide a better fitting to the VDFs measured by spacecraft in the solar wind. One of the problems that is being addressed on this new light is the temperature anisotropy of solar wind protons and electrons. In the literature, the general treatment for waves excited by (bi-)Maxwellian plasmas is well-established. However, for kappa distributions, the wave characteristics have been studied mostly for the limiting cases of purely parallel or perpendicular propagation, relative to the ambient magnetic field. Contributions to the general case of obliquely propagating electromagnetic waves have been scarcely reported so far. The absence of a general treatment prevents a complete analysis of the wave-particle interaction in kappa plasmas, since some instabilities can operate simultaneously both in the parallel and oblique directions. In a recent work, Gaelzer and Ziebell [J. Geophys. Res. 119, 9334 (2014)] obtained expressions for the dielectric tensor and dispersion relations for the low-frequency, quasi-perpendicular dispersive Alfv en waves resulting from a kappa VDF. In the present work, the formalism is generalized for the general case of electrostatic and/or electromagnetic waves propagating in a kappa plasma in any frequency range and for arbitrary angles. An isotropic distribution is considered, but the methods used here can be easily applied to more general anisotropic distributions such as the bi-kappa or product-bi-kappa. VC 2016 AIP Publishing LLC.application/pdfengPhysics of plasmas. Melville. Vol. 23, no. 2 (Feb. 2016), 022110, 18 p.Relações de dispersãoPropagação de ondas eletromagnéticasVento solarObliquely propagating electromagnetic waves in magnetized kappa plasmasEstrangeiroinfo: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:UFRGSTEXT000995850.pdf.txt000995850.pdf.txtExtracted Texttext/plain85724http://www.lume.ufrgs.br/bitstream/10183/189586/2/000995850.pdf.txt545c9f67f5c3e53118d43d40b9e75413MD52ORIGINAL000995850.pdfTexto completo (inglês)application/pdf1652157http://www.lume.ufrgs.br/bitstream/10183/189586/1/000995850.pdfe59f1606d8f52c58d0c5548aa900f149MD5110183/1895862023-09-23 03:35:08.72396oai:www.lume.ufrgs.br:10183/189586Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-09-23T06:35:08Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Obliquely propagating electromagnetic waves in magnetized kappa plasmas
title Obliquely propagating electromagnetic waves in magnetized kappa plasmas
spellingShingle Obliquely propagating electromagnetic waves in magnetized kappa plasmas
Gaelzer, Rudi
Relações de dispersão
Propagação de ondas eletromagnéticas
Vento solar
title_short Obliquely propagating electromagnetic waves in magnetized kappa plasmas
title_full Obliquely propagating electromagnetic waves in magnetized kappa plasmas
title_fullStr Obliquely propagating electromagnetic waves in magnetized kappa plasmas
title_full_unstemmed Obliquely propagating electromagnetic waves in magnetized kappa plasmas
title_sort Obliquely propagating electromagnetic waves in magnetized kappa plasmas
author Gaelzer, Rudi
author_facet Gaelzer, Rudi
Ziebell, Luiz Fernando
author_role author
author2 Ziebell, Luiz Fernando
author2_role author
dc.contributor.author.fl_str_mv Gaelzer, Rudi
Ziebell, Luiz Fernando
dc.subject.por.fl_str_mv Relações de dispersão
Propagação de ondas eletromagnéticas
Vento solar
topic Relações de dispersão
Propagação de ondas eletromagnéticas
Vento solar
description Velocity distribution functions (VDFs) that exhibit a power-law dependence on the high-energy tail have been the subject of intense research by the plasma physics community. Such functions, known as kappa or superthermal distributions, have been found to provide a better fitting to the VDFs measured by spacecraft in the solar wind. One of the problems that is being addressed on this new light is the temperature anisotropy of solar wind protons and electrons. In the literature, the general treatment for waves excited by (bi-)Maxwellian plasmas is well-established. However, for kappa distributions, the wave characteristics have been studied mostly for the limiting cases of purely parallel or perpendicular propagation, relative to the ambient magnetic field. Contributions to the general case of obliquely propagating electromagnetic waves have been scarcely reported so far. The absence of a general treatment prevents a complete analysis of the wave-particle interaction in kappa plasmas, since some instabilities can operate simultaneously both in the parallel and oblique directions. In a recent work, Gaelzer and Ziebell [J. Geophys. Res. 119, 9334 (2014)] obtained expressions for the dielectric tensor and dispersion relations for the low-frequency, quasi-perpendicular dispersive Alfv en waves resulting from a kappa VDF. In the present work, the formalism is generalized for the general case of electrostatic and/or electromagnetic waves propagating in a kappa plasma in any frequency range and for arbitrary angles. An isotropic distribution is considered, but the methods used here can be easily applied to more general anisotropic distributions such as the bi-kappa or product-bi-kappa. VC 2016 AIP Publishing LLC.
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dc.date.issued.fl_str_mv 2016
dc.date.accessioned.fl_str_mv 2019-03-27T04:06:15Z
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dc.relation.ispartof.pt_BR.fl_str_mv Physics of plasmas. Melville. Vol. 23, no. 2 (Feb. 2016), 022110, 18 p.
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