Please use this identifier to cite or link to this item: http://hdl.handle.net/10553/47990
DC FieldValueLanguage
dc.contributor.authorIvanov, V. V.en_US
dc.contributor.authorMancini, R. C.en_US
dc.contributor.authorPapp, D.en_US
dc.contributor.authorHakel, P.en_US
dc.contributor.authorDurmaz, T.en_US
dc.contributor.authorFlorido, R.en_US
dc.contributor.otherFlorido, Ricardo-
dc.contributor.otherHakel, Peter-
dc.date.accessioned2018-11-23T18:04:59Z-
dc.date.available2018-11-23T18:04:59Z-
dc.date.issued2014en_US
dc.identifier.issn1070-664Xen_US
dc.identifier.urihttp://hdl.handle.net/10553/47990-
dc.description.abstractWire-array two-component Z-pinch plasmas containing Al and other elements were studied experimentally and the observations interpreted with the help of theoretical modeling. Special attention was given to achieving reproducible implosions. Cascading implosions in star wire arrays mix components during the implosion phase and implosion dynamics were not affected by changes in concentration. A reduction in Al K-shell radiation and an increase in soft x-ray radiation emission were observed in Al-W plasma with 84% concentration of Al ions compared to only-Al plasma. Plasma with 84% of Al ions has radiative properties like those of W Z-pinches. The analysis of Al K-shell x-ray spectra with a collisional-radiative atomic kinetics model shows a drop of the electron temperature from 400 eV in pure Al plasma to below 300 eV in the Al-W mix. Al-Au Z-pinches present radiation features similar to Al-W plasma. This is indicative of a similar plasma cooling effect due to the presence of a high-Z element.en_US
dc.languageengen_US
dc.publisher1070-664X-
dc.relation.ispartofPhysics of Plasmasen_US
dc.sourcePhysics Of Plasmas [ISSN 1070-664X], v. 21 (8)en_US
dc.subject220410 Física de plasmasen_US
dc.subject.otherEmission spectroscopyen_US
dc.titleRadiative cooling of two-component wire-array Z-pinch plasmaen_US
dc.typeinfo:eu-repo/semantics/Articlees
dc.typeArticlees
dc.identifier.doi10.1063/1.4892180
dc.identifier.scopus84905718021-
dc.identifier.isi000342760600049-
dcterms.isPartOfPhysics Of Plasmas-
dcterms.sourcePhysics Of Plasmas[ISSN 1070-664X],v. 21 (8)-
dc.contributor.authorscopusid7404808725-
dc.contributor.authorscopusid35430576000-
dc.contributor.authorscopusid35115394700-
dc.contributor.authorscopusid6508381518-
dc.contributor.authorscopusid25626029200-
dc.contributor.authorscopusid6505795084-
dc.identifier.issue082704-
dc.relation.volume21-
dc.investigacionCienciasen_US
dc.type2Artículoen_US
dc.contributor.daisngid34944137
dc.contributor.daisngid4916-
dc.contributor.daisngid30268485
dc.contributor.daisngid27815-
dc.contributor.daisngid980399-
dc.contributor.daisngid722063-
dc.contributor.daisngid5001449-
dc.contributor.daisngid835287-
dc.identifier.investigatorRIDH-5513-2015-
dc.identifier.investigatorRIDNo ID-
dc.utils.revisionen_US
dc.contributor.wosstandardWOS:Ivanov, VV
dc.contributor.wosstandardWOS:Mancini, RC
dc.contributor.wosstandardWOS:Papp, D
dc.contributor.wosstandardWOS:Hakel, P
dc.contributor.wosstandardWOS:Durmaz, T
dc.contributor.wosstandardWOS:Florido, R
dc.date.coverdateEnero 2014
dc.identifier.ulpgces
dc.description.sjr1,126
dc.description.jcr2,142
dc.description.sjrqQ2
dc.description.jcrqQ2
dc.description.scieSCIE
item.grantfulltextopen-
item.fulltextCon texto completo-
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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