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dc.contributor.authorBailly-Grandvaux, M.
dc.contributor.authorFlorido, R.
dc.contributor.authorWalsh, C. A.
dc.contributor.authorBeg, F. N.
dc.contributor.authorMcGuffey, C.
dc.contributor.authorMancini, R. C.
dc.contributor.authorSuzuki-Vidal, F.
dc.contributor.authorVlachos, C.
dc.contributor.authorBradford, P.
dc.contributor.authorSantos, J. J.
dc.contributor.authorPérez Callejo, Gabriel 
dc.contributor.authorGigosos Pérez, Marco Antonio 
dc.date.accessioned2024-01-10T17:30:33Z
dc.date.available2024-01-10T17:30:33Z
dc.date.issued2022
dc.identifier.citationReview of Scientific Instruments, Noviembre 2022, vol. 93, n. 11, p. 113542es
dc.identifier.issn0034-6748es
dc.identifier.urihttps://uvadoc.uva.es/handle/10324/64396
dc.descriptionProducción Científicaes
dc.description.abstractMagnetization of inertial confinement implosions is a promising means of improving their performance, owing to the potential reduction of energy losses within the target and mitigation of hydrodynamic instabilities. In particular, cylindrical implosions are useful for studying the influence of a magnetic field thanks to their axial symmetry. Here we present experimental results from cylindrical implosions on the OMEGA-60 laser using a 40-beam, 14.5 kJ, 1.5 ns drive and an initial seed magnetic field of B0 = 24 T along the axis of the targets, compared with reference results without an imposed B-field. Implosions were characterized using time-resolved X-ray imaging from two orthogonal lines of sight. We found that the data agree well with magnetohydrodynamic simulations once radiation transport within the imploding plasma is considered. We show that for a correct interpretation of the data in this type of experiments, explicit radiation transport must be taken into account.es
dc.format.mimetypeapplication/pdfes
dc.language.isoenges
dc.publisherAmerican Institute of Physicses
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses
dc.titleX-ray imaging and radiation transport effects on cylindrical implosionses
dc.typeinfo:eu-repo/semantics/articlees
dc.identifier.doi10.1063/5.0099180es
dc.identifier.publicationissue11es
dc.identifier.publicationtitleReview of Scientific Instrumentses
dc.identifier.publicationvolume93es
dc.peerreviewedSIes
dc.description.projectThis work has been carried out within the framework of the EUROfusion Consortium, funded by the European Union via the Euratom Research and Training Programme (Grant Agreements No. 633053 and No. 101052200 — EUROfusion). Views and opinions ex pressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Commission. Neither the European Union nor the European Commission can be held responsible for them. The involved teams have operated within the framework of the Enabling Research Projects: AWP17- ENR-IFE-CEA-02 and AWP21-ENR-IFE.01.CEA.es
dc.description.projectThe work has also been supported by the Research Grant No. CEI2020- FEI02 from the Consejería de Economía, Industria, Comercio y Conocimiento del Gobierno de Canarias; and by Research Grant No. PID2019-108764RB-I00 from the Spanish Ministry of Science and Innovationes
dc.identifier.essn1089-7623es
dc.type.hasVersioninfo:eu-repo/semantics/acceptedVersiones


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