Please use this identifier to cite or link to this item: http://hdl.handle.net/10553/113552
DC FieldValueLanguage
dc.contributor.authorWalsh, Christopher-
dc.contributor.authorFlorido Hernández, Ricardo Jesús-
dc.contributor.authorBailly-Grandvaux, Mathieu-
dc.contributor.authorSuzuki-Vidal, F.-
dc.contributor.authorChittenden, J. P.-
dc.contributor.authorCrilly, A. J.-
dc.contributor.authorGigosos, M. A.-
dc.contributor.authorMancini, R. C.-
dc.contributor.authorPérez-Callejo, Gabriel-
dc.contributor.authorVlachos, Christos-
dc.contributor.authorMcGuffey, C.-
dc.contributor.authorBeg, Farhat-
dc.contributor.authorSantos, João Jorge-
dc.date.accessioned2022-01-26T10:17:11Z-
dc.date.available2022-01-26T10:17:11Z-
dc.date.issued2022-
dc.identifier.issn0741-3335-
dc.identifier.otherWoS-
dc.identifier.otherScopus-
dc.identifier.urihttp://hdl.handle.net/10553/113552-
dc.description.abstractThis paper uses extended-magnetohydrodynamics (MHD) simulations to explore an extreme magnetized plasma regime realizable by cylindrical implosions on the OMEGA laser facility. This regime is characterized by highly compressed magnetic fields (greater than 10 kT across the fuel), which contain a significant proportion of the implosion energy and induce large electrical currents in the plasma. Parameters governing the different magnetization processes such as Ohmic dissipation and suppression of instabilities by magnetic tension are presented, allowing for optimization of experiments to study specific phenomena. For instance, a dopant added to the target gas-fill can enhance magnetic flux compression while enabling spectroscopic diagnosis of the imploding core. In particular, the use of Ar K-shell spectroscopy is investigated by performing detailed non-LTE atomic kinetics and radiative transfer calculations on the MHD data. Direct measurement of the core electron density and temperature would be possible, allowing for both the impact of magnetization on the final temperature and thermal pressure to be obtained. By assuming the magnetic field is frozen into the plasma motion, which is shown to be a good approximation for highly magnetized implosions, spectroscopic diagnosis could be used to estimate which magnetization processes are ruling the implosion dynamics; for example, a relation is given for inferring whether thermally driven or current-driven transport is dominating.-
dc.languageeng-
dc.relationCinética atómica colisional-radiativa y dinámica molecular para la caracterización espectroscópica de plasmas de laboratorio de alta densidad de energía-
dc.relationCaracterización espectroscópica de plasmas de laboratorio de alta densidad de energía mediante cinética atómica colisional-radiativa y dinámica molecular-
dc.relation.ispartofPlasma Physics and Controlled Fusion-
dc.sourcePlasma Physics and Controlled Fusion [ISSN 0741-3335], v. 64 (2), (Febrero 2022)-
dc.subject22 Física-
dc.subject220410 Física de plasmas-
dc.subject.otherMagnetized HEDP-
dc.subject.otherICF-
dc.subject.otherMagnetized plasmas-
dc.subject.otherMagneto-inertial fusion-
dc.subject.otherMagnetohydrodynamics-
dc.subject.otherExtended-MHD-
dc.subject.otherMagnetic fields-
dc.titleExploring extreme magnetization phenomena in directly driven imploding cylindrical targets-
dc.typeinfo:eu-repo/semantics/Article-
dc.typeArticle-
dc.identifier.doi10.1088/1361-6587/ac3f25-
dc.identifier.scopus85123952040-
dc.identifier.isiWOS:000741709400001-
dc.contributor.orcid0000-0002-6639-3543-
dc.contributor.orcid0000-0001-7428-6273-
dc.contributor.orcid0000-0001-7529-4013-
dc.contributor.orcidNO DATA-
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dc.contributor.orcid0000-0003-3719-2352-
dc.contributor.orcid0000-0003-4834-1536-
dc.contributor.orcidNO DATA-
dc.contributor.orcid0000-0003-0391-8944-
dc.contributor.orcid0000-0002-4737-8559-
dc.contributor.authorscopusid57193901060-
dc.contributor.authorscopusid6505795084-
dc.contributor.authorscopusid56638674300-
dc.contributor.authorscopusid16239942100-
dc.contributor.authorscopusid57206430086-
dc.contributor.authorscopusid57205074381-
dc.contributor.authorscopusid6701840314-
dc.contributor.authorscopusid55845951200-
dc.contributor.authorscopusid57200540130-
dc.contributor.authorscopusid57215814301-
dc.contributor.authorscopusid26429702400-
dc.contributor.authorscopusid7004606385-
dc.contributor.authorscopusid57437744900-
dc.identifier.eissn1361-6587-
dc.identifier.issue2-
dc.relation.volume64-
dc.investigacionCiencias-
dc.type2Artículo-
dc.contributor.daisngid30015511-
dc.contributor.daisngid835287-
dc.contributor.daisngid41748302-
dc.contributor.daisngid36361012-
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dc.contributor.daisngid27881492-
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dc.contributor.daisngid13445431-
dc.contributor.daisngid30304994-
dc.contributor.daisngid37723133-
dc.description.numberofpages19-
dc.utils.revision-
dc.contributor.wosstandardWOS:Walsh, CA-
dc.contributor.wosstandardWOS:Florido, R-
dc.contributor.wosstandardWOS:Bailly-Grandvaux, M-
dc.contributor.wosstandardWOS:Suzuki-Vidal, F-
dc.contributor.wosstandardWOS:Chittenden, JP-
dc.contributor.wosstandardWOS:Crilly, AJ-
dc.contributor.wosstandardWOS:Gigosos, MA-
dc.contributor.wosstandardWOS:Mancini, RC-
dc.contributor.wosstandardWOS:Perez-Callejo, G-
dc.contributor.wosstandardWOS:Vlachos, C-
dc.contributor.wosstandardWOS:McGuffey, C-
dc.contributor.wosstandardWOS:Beg, FN-
dc.contributor.wosstandardWOS:Santos, JJ-
dc.date.coverdateFebrero 2022-
dc.identifier.ulpgc-
dc.contributor.buulpgcBU-BAS-
dc.description.sjr0,988-
dc.description.jcr2,2-
dc.description.sjrqQ1-
dc.description.jcrqQ3-
dc.description.scieSCIE-
dc.description.miaricds11,0
item.fulltextCon texto completo-
item.grantfulltextopen-
crisitem.project.principalinvestigatorFlorido Hernández, Ricardo Jesús-
crisitem.project.principalinvestigatorFlorido Hernández, Ricardo Jesús-
crisitem.author.deptGIR IUNAT: Interacción Radiación-Materia-
crisitem.author.deptIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.deptDepartamento de Física-
crisitem.author.orcid0000-0001-7428-6273-
crisitem.author.parentorgIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.fullNameFlorido Hernández, Ricardo Jesús-
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