Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection

Autores
Firpo, M. C.; Ettoumi, W.; Lifschitz, Agustin Federico; Retinò, A.; Farengo, Ricardo; Ferrari, Hugo Emilio; Garcia Martinez, Pablo Luis
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Stochasticity is an ingredient that may allow the breaking of the frozen-in law in the reconnection process. It will first be argued that the non-ideal effects may be considered as an implicit way to introduce stochasticity. Yet there also exists an explicit stochasticity that does not require the invocation of non-ideal effects. This comes from the spatial (or Eulerian) chaos of magnetic field lines that can show up only in a truly three-dimensional description of magnetic reconnection since the two-dimensional models impose the integrability of the magnetic field lines. Some implications of this magnetic braiding, such as the increased particle finite-time Lyapunov exponents and increased acceleration of charged particles, are discussed in the frame of tokamak sawteeth that forms a laboratory prototype of spontaneous magnetic reconnection. A justification for an increased reconnection rate with chaotic vs. the integrable magnetic field lines is proposed. Moreover, in 3D, the Eulerian chaos of the magnetic field lines may coexist with the Eulerian chaos of velocity field lines, that is more commonly named the turbulence.
Fil: Firpo, M. C.. Centre National de la Recherche Scientifique; Francia
Fil: Ettoumi, W.. Centre National de la Recherche Scientifique; Francia. Universidad de Ginebra; Suiza
Fil: Lifschitz, Agustin Federico. Centre National de la Recherche Scientifique; Francia
Fil: Retinò, A.. Centre National de la Recherche Scientifique; Francia
Fil: Farengo, Ricardo. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; Argentina
Fil: Ferrari, Hugo Emilio. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; Argentina
Fil: Garcia Martinez, Pablo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Materia
Nuclear Fusion
Magnetic Confinement
Chaos and Stochasticity
Magnetic Reconnection
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/66490

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spelling Impact of the Eulerian chaos of magnetic field lines in magnetic reconnectionFirpo, M. C.Ettoumi, W.Lifschitz, Agustin FedericoRetinò, A.Farengo, RicardoFerrari, Hugo EmilioGarcia Martinez, Pablo LuisNuclear FusionMagnetic ConfinementChaos and StochasticityMagnetic Reconnectionhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Stochasticity is an ingredient that may allow the breaking of the frozen-in law in the reconnection process. It will first be argued that the non-ideal effects may be considered as an implicit way to introduce stochasticity. Yet there also exists an explicit stochasticity that does not require the invocation of non-ideal effects. This comes from the spatial (or Eulerian) chaos of magnetic field lines that can show up only in a truly three-dimensional description of magnetic reconnection since the two-dimensional models impose the integrability of the magnetic field lines. Some implications of this magnetic braiding, such as the increased particle finite-time Lyapunov exponents and increased acceleration of charged particles, are discussed in the frame of tokamak sawteeth that forms a laboratory prototype of spontaneous magnetic reconnection. A justification for an increased reconnection rate with chaotic vs. the integrable magnetic field lines is proposed. Moreover, in 3D, the Eulerian chaos of the magnetic field lines may coexist with the Eulerian chaos of velocity field lines, that is more commonly named the turbulence.Fil: Firpo, M. C.. Centre National de la Recherche Scientifique; FranciaFil: Ettoumi, W.. Centre National de la Recherche Scientifique; Francia. Universidad de Ginebra; SuizaFil: Lifschitz, Agustin Federico. Centre National de la Recherche Scientifique; FranciaFil: Retinò, A.. Centre National de la Recherche Scientifique; FranciaFil: Farengo, Ricardo. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; ArgentinaFil: Ferrari, Hugo Emilio. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; ArgentinaFil: Garcia Martinez, Pablo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaAmerican Institute of Physics2016-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/66490Firpo, M. C.; Ettoumi, W.; Lifschitz, Agustin Federico; Retinò, A.; Farengo, Ricardo; et al.; Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection; American Institute of Physics; Physics Of Plasmas; 23; 12; 12-2016; 122905-1/91070-664XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1063/1.4972544info:eu-repo/semantics/altIdentifier/url/https://aip.scitation.org/doi/10.1063/1.4972544info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:03:49Zoai:ri.conicet.gov.ar:11336/66490instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:03:49.643CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection
title Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection
spellingShingle Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection
Firpo, M. C.
Nuclear Fusion
Magnetic Confinement
Chaos and Stochasticity
Magnetic Reconnection
title_short Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection
title_full Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection
title_fullStr Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection
title_full_unstemmed Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection
title_sort Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection
dc.creator.none.fl_str_mv Firpo, M. C.
Ettoumi, W.
Lifschitz, Agustin Federico
Retinò, A.
Farengo, Ricardo
Ferrari, Hugo Emilio
Garcia Martinez, Pablo Luis
author Firpo, M. C.
author_facet Firpo, M. C.
Ettoumi, W.
Lifschitz, Agustin Federico
Retinò, A.
Farengo, Ricardo
Ferrari, Hugo Emilio
Garcia Martinez, Pablo Luis
author_role author
author2 Ettoumi, W.
Lifschitz, Agustin Federico
Retinò, A.
Farengo, Ricardo
Ferrari, Hugo Emilio
Garcia Martinez, Pablo Luis
author2_role author
author
author
author
author
author
dc.subject.none.fl_str_mv Nuclear Fusion
Magnetic Confinement
Chaos and Stochasticity
Magnetic Reconnection
topic Nuclear Fusion
Magnetic Confinement
Chaos and Stochasticity
Magnetic Reconnection
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Stochasticity is an ingredient that may allow the breaking of the frozen-in law in the reconnection process. It will first be argued that the non-ideal effects may be considered as an implicit way to introduce stochasticity. Yet there also exists an explicit stochasticity that does not require the invocation of non-ideal effects. This comes from the spatial (or Eulerian) chaos of magnetic field lines that can show up only in a truly three-dimensional description of magnetic reconnection since the two-dimensional models impose the integrability of the magnetic field lines. Some implications of this magnetic braiding, such as the increased particle finite-time Lyapunov exponents and increased acceleration of charged particles, are discussed in the frame of tokamak sawteeth that forms a laboratory prototype of spontaneous magnetic reconnection. A justification for an increased reconnection rate with chaotic vs. the integrable magnetic field lines is proposed. Moreover, in 3D, the Eulerian chaos of the magnetic field lines may coexist with the Eulerian chaos of velocity field lines, that is more commonly named the turbulence.
Fil: Firpo, M. C.. Centre National de la Recherche Scientifique; Francia
Fil: Ettoumi, W.. Centre National de la Recherche Scientifique; Francia. Universidad de Ginebra; Suiza
Fil: Lifschitz, Agustin Federico. Centre National de la Recherche Scientifique; Francia
Fil: Retinò, A.. Centre National de la Recherche Scientifique; Francia
Fil: Farengo, Ricardo. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; Argentina
Fil: Ferrari, Hugo Emilio. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Comisión Nacional de Energía Atómica. Gerencia del Área de Energía Nuclear. Instituto Balseiro; Argentina
Fil: Garcia Martinez, Pablo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
description Stochasticity is an ingredient that may allow the breaking of the frozen-in law in the reconnection process. It will first be argued that the non-ideal effects may be considered as an implicit way to introduce stochasticity. Yet there also exists an explicit stochasticity that does not require the invocation of non-ideal effects. This comes from the spatial (or Eulerian) chaos of magnetic field lines that can show up only in a truly three-dimensional description of magnetic reconnection since the two-dimensional models impose the integrability of the magnetic field lines. Some implications of this magnetic braiding, such as the increased particle finite-time Lyapunov exponents and increased acceleration of charged particles, are discussed in the frame of tokamak sawteeth that forms a laboratory prototype of spontaneous magnetic reconnection. A justification for an increased reconnection rate with chaotic vs. the integrable magnetic field lines is proposed. Moreover, in 3D, the Eulerian chaos of the magnetic field lines may coexist with the Eulerian chaos of velocity field lines, that is more commonly named the turbulence.
publishDate 2016
dc.date.none.fl_str_mv 2016-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/66490
Firpo, M. C.; Ettoumi, W.; Lifschitz, Agustin Federico; Retinò, A.; Farengo, Ricardo; et al.; Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection; American Institute of Physics; Physics Of Plasmas; 23; 12; 12-2016; 122905-1/9
1070-664X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/66490
identifier_str_mv Firpo, M. C.; Ettoumi, W.; Lifschitz, Agustin Federico; Retinò, A.; Farengo, Ricardo; et al.; Impact of the Eulerian chaos of magnetic field lines in magnetic reconnection; American Institute of Physics; Physics Of Plasmas; 23; 12; 12-2016; 122905-1/9
1070-664X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1063/1.4972544
info:eu-repo/semantics/altIdentifier/url/https://aip.scitation.org/doi/10.1063/1.4972544
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv American Institute of Physics
publisher.none.fl_str_mv American Institute of Physics
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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