Generation of suprathermal electrons by collective processes in collisional plasma

Detalhes bibliográficos
Autor(a) principal: Ferrão, Sabrina Tigik
Data de Publicação: 2017
Outros Autores: Ziebell, Luiz Fernando, Yoon, Peter H.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/173037
Resumo: The ubiquity of high-energy tails in the charged particle velocity distribution functions (VDFs) observed in space plasmas suggests the existence of an underlying process responsible for taking a fraction of the charged particle population out of thermal equilibrium and redistributing it to suprathermal velocity and energy ranges. The present Letter focuses on a new and fundamental physical explanation for the origin of suprathermal electron velocity distribution function (EVDF) in a collisional plasma. This process involves a newly discovered electrostatic bremsstrahlung (EB) emission that is effective in a plasma in which binary collisions are present. The steady-state EVDF dictated by such a process corresponds to a Maxwellian core plus a quasi-inverse power-law tail, which is a feature commonly observed in many space plasma environments. In order to demonstrate this, the system of selfconsistent particle- and wave-kinetic equations are numerically solved with an initially Maxwellian EVDF and Langmuir wave spectral intensity, which is a state that does not reflect the presence of EB process, and hence not in force balance. The EB term subsequently drives the system to a new force-balanced steady state. After a long integration period it is demonstrated that the initial Langmuir fluctuation spectrum is modified, which in turn distorts the initial Maxwellian EVDF into a VDF that resembles the said core-suprathermal VDF. Such a mechanism may thus be operative at the coronal source region, which is characterized by high collisionality.
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spelling Ferrão, Sabrina TigikZiebell, Luiz FernandoYoon, Peter H.2018-02-28T02:27:57Z20170004-637Xhttp://hdl.handle.net/10183/173037001055818The ubiquity of high-energy tails in the charged particle velocity distribution functions (VDFs) observed in space plasmas suggests the existence of an underlying process responsible for taking a fraction of the charged particle population out of thermal equilibrium and redistributing it to suprathermal velocity and energy ranges. The present Letter focuses on a new and fundamental physical explanation for the origin of suprathermal electron velocity distribution function (EVDF) in a collisional plasma. This process involves a newly discovered electrostatic bremsstrahlung (EB) emission that is effective in a plasma in which binary collisions are present. The steady-state EVDF dictated by such a process corresponds to a Maxwellian core plus a quasi-inverse power-law tail, which is a feature commonly observed in many space plasma environments. In order to demonstrate this, the system of selfconsistent particle- and wave-kinetic equations are numerically solved with an initially Maxwellian EVDF and Langmuir wave spectral intensity, which is a state that does not reflect the presence of EB process, and hence not in force balance. The EB term subsequently drives the system to a new force-balanced steady state. After a long integration period it is demonstrated that the initial Langmuir fluctuation spectrum is modified, which in turn distorts the initial Maxwellian EVDF into a VDF that resembles the said core-suprathermal VDF. Such a mechanism may thus be operative at the coronal source region, which is characterized by high collisionality.application/pdfengThe astrophysical journal. Bristol. Vol. 849, no. 2 ( 2017), L30, 5 p.Vento solarProcessos de colisao em plasmasOndas de Langmuir em plasmasSolar windSun: coronaSun: particle emissionGeneration of suprathermal electrons by collective processes in collisional plasmaEstrangeiroinfo: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:UFRGSORIGINAL001055818.pdf001055818.pdfTexto completo (inglês)application/pdf296497http://www.lume.ufrgs.br/bitstream/10183/173037/1/001055818.pdf593dd258f62268c255cbc8f0d5ca50f0MD51TEXT001055818.pdf.txt001055818.pdf.txtExtracted Texttext/plain28367http://www.lume.ufrgs.br/bitstream/10183/173037/2/001055818.pdf.txt1d7bc86f44f511f5684859740a50a3c0MD52THUMBNAIL001055818.pdf.jpg001055818.pdf.jpgGenerated Thumbnailimage/jpeg2104http://www.lume.ufrgs.br/bitstream/10183/173037/3/001055818.pdf.jpg36d82e6860091741e5b7bfd12a27b7beMD5310183/1730372023-09-24 03:37:35.471835oai:www.lume.ufrgs.br:10183/173037Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-09-24T06:37:35Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Generation of suprathermal electrons by collective processes in collisional plasma
title Generation of suprathermal electrons by collective processes in collisional plasma
spellingShingle Generation of suprathermal electrons by collective processes in collisional plasma
Ferrão, Sabrina Tigik
Vento solar
Processos de colisao em plasmas
Ondas de Langmuir em plasmas
Solar wind
Sun: corona
Sun: particle emission
title_short Generation of suprathermal electrons by collective processes in collisional plasma
title_full Generation of suprathermal electrons by collective processes in collisional plasma
title_fullStr Generation of suprathermal electrons by collective processes in collisional plasma
title_full_unstemmed Generation of suprathermal electrons by collective processes in collisional plasma
title_sort Generation of suprathermal electrons by collective processes in collisional plasma
author Ferrão, Sabrina Tigik
author_facet Ferrão, Sabrina Tigik
Ziebell, Luiz Fernando
Yoon, Peter H.
author_role author
author2 Ziebell, Luiz Fernando
Yoon, Peter H.
author2_role author
author
dc.contributor.author.fl_str_mv Ferrão, Sabrina Tigik
Ziebell, Luiz Fernando
Yoon, Peter H.
dc.subject.por.fl_str_mv Vento solar
Processos de colisao em plasmas
Ondas de Langmuir em plasmas
topic Vento solar
Processos de colisao em plasmas
Ondas de Langmuir em plasmas
Solar wind
Sun: corona
Sun: particle emission
dc.subject.eng.fl_str_mv Solar wind
Sun: corona
Sun: particle emission
description The ubiquity of high-energy tails in the charged particle velocity distribution functions (VDFs) observed in space plasmas suggests the existence of an underlying process responsible for taking a fraction of the charged particle population out of thermal equilibrium and redistributing it to suprathermal velocity and energy ranges. The present Letter focuses on a new and fundamental physical explanation for the origin of suprathermal electron velocity distribution function (EVDF) in a collisional plasma. This process involves a newly discovered electrostatic bremsstrahlung (EB) emission that is effective in a plasma in which binary collisions are present. The steady-state EVDF dictated by such a process corresponds to a Maxwellian core plus a quasi-inverse power-law tail, which is a feature commonly observed in many space plasma environments. In order to demonstrate this, the system of selfconsistent particle- and wave-kinetic equations are numerically solved with an initially Maxwellian EVDF and Langmuir wave spectral intensity, which is a state that does not reflect the presence of EB process, and hence not in force balance. The EB term subsequently drives the system to a new force-balanced steady state. After a long integration period it is demonstrated that the initial Langmuir fluctuation spectrum is modified, which in turn distorts the initial Maxwellian EVDF into a VDF that resembles the said core-suprathermal VDF. Such a mechanism may thus be operative at the coronal source region, which is characterized by high collisionality.
publishDate 2017
dc.date.issued.fl_str_mv 2017
dc.date.accessioned.fl_str_mv 2018-02-28T02:27:57Z
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10183/173037
dc.identifier.issn.pt_BR.fl_str_mv 0004-637X
dc.identifier.nrb.pt_BR.fl_str_mv 001055818
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dc.relation.ispartof.pt_BR.fl_str_mv The astrophysical journal. Bristol. Vol. 849, no. 2 ( 2017), L30, 5 p.
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