dc.creatorFirpo, Marie Christine
dc.creatorLifschitz, Agustin Federico
dc.creatorEttoumi, Wahb
dc.creatorFarengo, Ricardo
dc.creatorFerrari, Hugo Emilio
dc.creatorGarcia Martinez, Pablo Luis
dc.date.accessioned2018-12-11T17:36:02Z
dc.date.accessioned2022-10-15T04:46:17Z
dc.date.available2018-12-11T17:36:02Z
dc.date.available2022-10-15T04:46:17Z
dc.date.created2018-12-11T17:36:02Z
dc.date.issued2017-03-31
dc.identifierFirpo, 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.identifier0741-3335
dc.identifierhttp://hdl.handle.net/11336/66254
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4346458
dc.description.abstractNumerical 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.languageeng
dc.publisherIOP Publishing
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/https://dx.doi.org/10.1088/1361-6587/aa570d
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/1361-6587/aa570d
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectMagnetic confinement fusion
dc.subjectChaotic magnetic field lines
dc.subjectStochasticity
dc.subjectMagnetic turbulence
dc.titleEvidence and relevance of spatially chaotic magnetic field lines in MCF devices
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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