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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/66490
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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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1846781279539822592 |
score |
13.229304 |