Identificador persistente para citar o vincular este elemento: http://hdl.handle.net/10553/47292
Campo DC Valoridioma
dc.contributor.authorFlorido, R.en_US
dc.contributor.authorNagayama, Taisuke N.en_US
dc.contributor.authorMancini, Roberto C.en_US
dc.contributor.authorTommasini, Riccardoen_US
dc.contributor.authorDelettrez, Jacques A.en_US
dc.contributor.authorRegan, Sean P.en_US
dc.contributor.authorSmalyuk, Vladimir A.en_US
dc.contributor.authorRodriguez, R.en_US
dc.contributor.authorGil, J. M.en_US
dc.contributor.otherTommasini, Riccardo-
dc.contributor.otherFlorido, Ricardo-
dc.contributor.otherRodriguez, Rafael-
dc.contributor.otherGil de la Fe, Juan Miguel-
dc.date.accessioned2018-11-23T12:22:56Z-
dc.date.available2018-11-23T12:22:56Z-
dc.date.issued2008en_US
dc.identifier.issn0034-6748en_US
dc.identifier.urihttp://hdl.handle.net/10553/47292-
dc.description.abstractWe discuss the observation and data analysis of argon K-shell line spectra from argon-doped deuterium-filled OMEGA direct-drive implosion cores based on data recorded with two streaked crystal spectrometers. The targets were 870μm in diameter, 27μm wall thickness plastic shells filled with 20atm of deuterium gas, and a tracer amount of argon for diagnostic purposes. The argon K-shell line spectrum is primarily emitted at the collapse of the implosion and its analysis provides a spectroscopic diagnostic of the core implosion conditions. The observed spectra includes the Heα, Lyα, Heβ, Heγ, Lyβ, and Lyγ line emissions and their associated He- and Li-like satellites thus covering a broad photon energy range from 3100to4200eV with a spectral resolution power of approximately 500. The data analysis relies on detailed atomic and spectral models that take into account nonequilibrium collisional-radiative atomic kinetics, Stark-broadened line shapes, and radiation transport calculations.en_US
dc.languageengen_US
dc.publisherAmerican Institute of Physics (AIP)en_US
dc.relation.ispartofReview of Scientific Instrumentsen_US
dc.sourceReview Of Scientific Instruments [ISSN 0034-6748], v. 79 (10)en_US
dc.subject220410 Física de plasmasen_US
dc.subject.otherShell Spectroscopy
dc.subject.otherCore Conditions
dc.subject.otherProfiles
dc.subject.otherOpacity
dc.subject.otherPlasmas
dc.titleAnalysis of time-resolved argon line spectra from OMEGA direct-drive implosionsen_US
dc.typeinfo:eu-repo/semantics/conferenceObjecten_US
dc.typeConferenceObjecten_US
dc.relation.conference17th Topical Conference on High-Temperature Plasma Diagnosticsen_US
dc.identifier.doi10.1063/1.2965779en_US
dc.identifier.scopus55349105450-
dc.identifier.isi000260573500068-
dcterms.isPartOfReview Of Scientific Instruments-
dcterms.sourceReview Of Scientific Instruments[ISSN 0034-6748],v. 79 (10)-
dc.contributor.authorscopusid6505795084-
dc.contributor.authorscopusid25633968700-
dc.contributor.authorscopusid35430576000-
dc.contributor.authorscopusid56931713500-
dc.contributor.authorscopusid7004421154-
dc.contributor.authorscopusid7006162272-
dc.contributor.authorscopusid7004013363-
dc.contributor.authorscopusid56314921800-
dc.contributor.authorscopusid7201625504-
dc.identifier.issue10E310-
dc.relation.volume79en_US
dc.investigacionCienciasen_US
dc.type2Actas de congresosen_US
dc.identifier.wosWOS:000260573500068-
dc.contributor.daisngid835287-
dc.contributor.daisngid32708-
dc.contributor.daisngid5309876-
dc.contributor.daisngid27815-
dc.contributor.daisngid30268485-
dc.contributor.daisngid118270-
dc.contributor.daisngid75402-
dc.contributor.daisngid51124-
dc.contributor.daisngid100553-
dc.contributor.daisngid799688-
dc.contributor.daisngid292327-
dc.description.notasContributed paper, published as part of the Proceedings of the 17th Topical Conference on High-Temperature Plasma Diagnostics, Albuquerque, New Mexico, May 2008.en_US
dc.identifier.investigatorRIDA-8214-2009-
dc.identifier.investigatorRIDH-5513-2015-
dc.identifier.investigatorRIDL-1938-2017-
dc.identifier.investigatorRIDR-2117-2018-
dc.contributor.wosstandardWOS:Florido, R-
dc.contributor.wosstandardWOS:Nagayama, T-
dc.contributor.wosstandardWOS:Mancini, RC-
dc.contributor.wosstandardWOS:Tommasini, R-
dc.contributor.wosstandardWOS:Delettrez, JA-
dc.contributor.wosstandardWOS:Regan, SP-
dc.contributor.wosstandardWOS:Smalyuk, VA-
dc.contributor.wosstandardWOS:Rodriguez, R-
dc.contributor.wosstandardWOS:Gil, JM-
dc.date.coverdateNoviembre 2008en_US
dc.identifier.ulpgces
dc.contributor.buulpgcBU-BASen_US
dc.description.jcr1,738
dc.description.jcrqQ2
dc.description.scieSCIE
item.fulltextCon texto completo-
item.grantfulltextopen-
crisitem.author.deptGIR IUNAT: Interacción Radiación-Materia-
crisitem.author.deptIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.deptDepartamento de Física-
crisitem.author.deptGIR IUNAT: Interacción Radiación-Materia-
crisitem.author.deptIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.deptDepartamento de Física-
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.orcid0000-0002-8326-3169-
crisitem.author.orcid0000-0001-9006-4128-
crisitem.author.parentorgIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.parentorgIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.parentorgIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.fullNameFlorido Hernández, Ricardo Jesús-
crisitem.author.fullNameRodríguez Pérez, Rafael-
crisitem.author.fullNameGil De La Fe, Juan Miguel-
Colección:Actas de congresos
miniatura
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