Evidence and relevance of spatially chaotic magnetic field lines in MCF devices
- Autores
- Firpo, Marie Christine; Lifschitz, Agustin Federico; Ettoumi, Wahb; Farengo, Ricardo; Ferrari, Hugo Emilio; Garcia Martinez, Pablo Luis
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Numerical evidence for the existence of spatially chaotic magnetic field lines about the collapse phase of tokamak sawteeth with incomplete reconnection is presented. This uses the results of
extensive test particle simulations in different sets of electromagnetic perturbations tested against experimental JET measurements. In tokamak sawteeth, that form a laboratory prototype of magnetic reconnection, the relative magnetic perturbation dB B may reach a few percents. This does not apply to tokamak operating regimes dominated by turbulence where dB B is usually not larger than 10^- 4 . However, this small magnetic perturbation being sustained by a large spectrum of modes is shown to be sufficient to ensure the existence of stochastic magnetic field lines. This has important consequences for magnetic confinement fusion where electrons are dominantly governed by the magnetic force. Indeed some overlap between magnetic resonances can locally induce chaotic magnetic field lines enabling the spatial redistribution of the electron population and of its thermal content. As they are the swiftest plasma particles, electrons feed back the most rapid perturbations of the magnetic field.
Fil: Firpo, Marie Christine. Centre National de la Recherche Scientifique; Francia
Fil: Lifschitz, Agustin Federico. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Centre National de la Recherche Scientifique; Francia
Fil: Ettoumi, Wahb. Centre National de la Recherche Scientifique; Francia. Universidad de Ginebra; Suiza
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. Centro Científico Tecnológico Conicet - Patagonia Norte; 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. Centro Científico Tecnológico Conicet - Patagonia Norte; Argentina - Materia
-
Magnetic confinement fusion
Chaotic magnetic field lines
Stochasticity
Magnetic turbulence - 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:11336/66254
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Evidence and relevance of spatially chaotic magnetic field lines in MCF devicesFirpo, Marie ChristineLifschitz, Agustin FedericoEttoumi, WahbFarengo, RicardoFerrari, Hugo EmilioGarcia Martinez, Pablo LuisMagnetic confinement fusionChaotic magnetic field linesStochasticityMagnetic turbulencehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Numerical evidence for the existence of spatially chaotic magnetic field lines about the collapse phase of tokamak sawteeth with incomplete reconnection is presented. This uses the results of<br />extensive test particle simulations in different sets of electromagnetic perturbations tested against experimental JET measurements. In tokamak sawteeth, that form a laboratory prototype of magnetic reconnection, the relative magnetic perturbation dB B may reach a few percents. This does not apply to tokamak operating regimes dominated by turbulence where dB B is usually not larger than 10^- 4 . However, this small magnetic perturbation being sustained by a large spectrum of modes is shown to be sufficient to ensure the existence of stochastic magnetic field lines. This has important consequences for magnetic confinement fusion where electrons are dominantly governed by the magnetic force. Indeed some overlap between magnetic resonances can locally induce chaotic magnetic field lines enabling the spatial redistribution of the electron population and of its thermal content. As they are the swiftest plasma particles, electrons feed back the most rapid perturbations of the magnetic field.Fil: Firpo, Marie Christine. Centre National de la Recherche Scientifique; FranciaFil: Lifschitz, Agustin Federico. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Centre National de la Recherche Scientifique; FranciaFil: Ettoumi, Wahb. Centre National de la Recherche Scientifique; Francia. Universidad de Ginebra; SuizaFil: 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. Centro Científico Tecnológico Conicet - Patagonia Norte; 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. Centro Científico Tecnológico Conicet - Patagonia Norte; ArgentinaIOP Publishing2017-03-31info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/66254Firpo, Marie Christine; Lifschitz, Agustin Federico; Ettoumi, Wahb; Farengo, Ricardo; Ferrari, Hugo Emilio; et al.; Evidence and relevance of spatially chaotic magnetic field lines in MCF devices; IOP Publishing; Plasma Physics And Controlled Fusion; 59; 3; 31-3-2017; 034005/1 - 034005/90741-3335CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1088/1361-6587/aa570dinfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/1361-6587/aa570dinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:23:38Zoai:ri.conicet.gov.ar:11336/66254instacron: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 11:23:39.012CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Evidence and relevance of spatially chaotic magnetic field lines in MCF devices |
title |
Evidence and relevance of spatially chaotic magnetic field lines in MCF devices |
spellingShingle |
Evidence and relevance of spatially chaotic magnetic field lines in MCF devices Firpo, Marie Christine Magnetic confinement fusion Chaotic magnetic field lines Stochasticity Magnetic turbulence |
title_short |
Evidence and relevance of spatially chaotic magnetic field lines in MCF devices |
title_full |
Evidence and relevance of spatially chaotic magnetic field lines in MCF devices |
title_fullStr |
Evidence and relevance of spatially chaotic magnetic field lines in MCF devices |
title_full_unstemmed |
Evidence and relevance of spatially chaotic magnetic field lines in MCF devices |
title_sort |
Evidence and relevance of spatially chaotic magnetic field lines in MCF devices |
dc.creator.none.fl_str_mv |
Firpo, Marie Christine Lifschitz, Agustin Federico Ettoumi, Wahb Farengo, Ricardo Ferrari, Hugo Emilio Garcia Martinez, Pablo Luis |
author |
Firpo, Marie Christine |
author_facet |
Firpo, Marie Christine Lifschitz, Agustin Federico Ettoumi, Wahb Farengo, Ricardo Ferrari, Hugo Emilio Garcia Martinez, Pablo Luis |
author_role |
author |
author2 |
Lifschitz, Agustin Federico Ettoumi, Wahb Farengo, Ricardo Ferrari, Hugo Emilio Garcia Martinez, Pablo Luis |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
Magnetic confinement fusion Chaotic magnetic field lines Stochasticity Magnetic turbulence |
topic |
Magnetic confinement fusion Chaotic magnetic field lines Stochasticity Magnetic turbulence |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Numerical evidence for the existence of spatially chaotic magnetic field lines about the collapse phase of tokamak sawteeth with incomplete reconnection is presented. This uses the results of<br />extensive test particle simulations in different sets of electromagnetic perturbations tested against experimental JET measurements. In tokamak sawteeth, that form a laboratory prototype of magnetic reconnection, the relative magnetic perturbation dB B may reach a few percents. This does not apply to tokamak operating regimes dominated by turbulence where dB B is usually not larger than 10^- 4 . However, this small magnetic perturbation being sustained by a large spectrum of modes is shown to be sufficient to ensure the existence of stochastic magnetic field lines. This has important consequences for magnetic confinement fusion where electrons are dominantly governed by the magnetic force. Indeed some overlap between magnetic resonances can locally induce chaotic magnetic field lines enabling the spatial redistribution of the electron population and of its thermal content. As they are the swiftest plasma particles, electrons feed back the most rapid perturbations of the magnetic field. Fil: Firpo, Marie Christine. Centre National de la Recherche Scientifique; Francia Fil: Lifschitz, Agustin Federico. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Centre National de la Recherche Scientifique; Francia Fil: Ettoumi, Wahb. Centre National de la Recherche Scientifique; Francia. Universidad de Ginebra; Suiza 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. Centro Científico Tecnológico Conicet - Patagonia Norte; 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. Centro Científico Tecnológico Conicet - Patagonia Norte; Argentina |
description |
Numerical evidence for the existence of spatially chaotic magnetic field lines about the collapse phase of tokamak sawteeth with incomplete reconnection is presented. This uses the results of<br />extensive test particle simulations in different sets of electromagnetic perturbations tested against experimental JET measurements. In tokamak sawteeth, that form a laboratory prototype of magnetic reconnection, the relative magnetic perturbation dB B may reach a few percents. This does not apply to tokamak operating regimes dominated by turbulence where dB B is usually not larger than 10^- 4 . However, this small magnetic perturbation being sustained by a large spectrum of modes is shown to be sufficient to ensure the existence of stochastic magnetic field lines. This has important consequences for magnetic confinement fusion where electrons are dominantly governed by the magnetic force. Indeed some overlap between magnetic resonances can locally induce chaotic magnetic field lines enabling the spatial redistribution of the electron population and of its thermal content. As they are the swiftest plasma particles, electrons feed back the most rapid perturbations of the magnetic field. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-03-31 |
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/11336/66254 Firpo, Marie Christine; Lifschitz, Agustin Federico; Ettoumi, Wahb; Farengo, Ricardo; Ferrari, Hugo Emilio; et al.; Evidence and relevance of spatially chaotic magnetic field lines in MCF devices; IOP Publishing; Plasma Physics And Controlled Fusion; 59; 3; 31-3-2017; 034005/1 - 034005/9 0741-3335 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/66254 |
identifier_str_mv |
Firpo, Marie Christine; Lifschitz, Agustin Federico; Ettoumi, Wahb; Farengo, Ricardo; Ferrari, Hugo Emilio; et al.; Evidence and relevance of spatially chaotic magnetic field lines in MCF devices; IOP Publishing; Plasma Physics And Controlled Fusion; 59; 3; 31-3-2017; 034005/1 - 034005/9 0741-3335 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1088/1361-6587/aa570d info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/1361-6587/aa570d |
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 |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
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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1846781767605813248 |
score |
12.982451 |