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dc.contributor.author
Firpo, Marie Christine  
dc.contributor.author
Lifschitz, Agustin Federico  
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Ettoumi, Wahb  
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Farengo, Ricardo  
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Ferrari, Hugo Emilio  
dc.contributor.author
Garcia Martinez, Pablo Luis  
dc.date.available
2018-12-11T17:36:02Z  
dc.date.issued
2017-03-31  
dc.identifier.citation
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  
dc.identifier.issn
0741-3335  
dc.identifier.uri
http://hdl.handle.net/11336/66254  
dc.description.abstract
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.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
IOP Publishing  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Magnetic Confinement Fusion  
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Chaotic Magnetic Field Lines  
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Stochasticity  
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Magnetic Turbulence  
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Astronomía  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
Evidence and relevance of spatially chaotic magnetic field lines in MCF devices  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2018-10-29T15:10:36Z  
dc.journal.volume
59  
dc.journal.number
3  
dc.journal.pagination
034005/1 - 034005/9  
dc.journal.pais
Reino Unido  
dc.journal.ciudad
Londres  
dc.description.fil
Fil: Firpo, Marie Christine. Centre National de la Recherche Scientifique; Francia  
dc.description.fil
Fil: Lifschitz, Agustin Federico. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Centre National de la Recherche Scientifique; Francia  
dc.description.fil
Fil: Ettoumi, Wahb. Centre National de la Recherche Scientifique; Francia. Universidad de Ginebra; Suiza  
dc.description.fil
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  
dc.description.fil
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  
dc.description.fil
Fil: Garcia Martinez, Pablo Luis. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Patagonia Norte; Argentina  
dc.journal.title
Plasma Physics And Controlled Fusion  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/https://dx.doi.org/10.1088/1361-6587/aa570d  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/1361-6587/aa570d