Identificador persistente para citar o vincular este elemento: http://hdl.handle.net/10553/35732
Campo DC Valoridioma
dc.contributor.authorClayson, T.en_US
dc.contributor.authorSuzuki-Vidal, F.en_US
dc.contributor.authorLebedev, S. V.en_US
dc.contributor.authorSwadling, G.F.en_US
dc.contributor.authorStehlé, C.en_US
dc.contributor.authorBurdiak, G.en_US
dc.contributor.authorFoster, J.M.en_US
dc.contributor.authorSkidmore, J.en_US
dc.contributor.authorGraham, P.en_US
dc.contributor.authorGumbrell, E.T.en_US
dc.contributor.authorPatankar, S.en_US
dc.contributor.authorSpindloe, C.en_US
dc.contributor.authorChaulagain, U.en_US
dc.contributor.authorKozlova, M.en_US
dc.contributor.authorLarour, J.en_US
dc.contributor.authorSingh, R. L.en_US
dc.contributor.authorRodriguez, R.en_US
dc.contributor.authorGil, J. M.en_US
dc.contributor.authorEspinosa Vivas, Guadalupeen_US
dc.contributor.authorVelarde, P.en_US
dc.contributor.authorDanson, C.en_US
dc.contributor.otherMichaela, Kozlova-
dc.contributor.otherGil de la Fe, Juan Miguel-
dc.contributor.otherRodriguez, Rafael-
dc.contributor.otherFyrth, Jim-
dc.contributor.otherChaulagain, Uddhab-
dc.contributor.otherSwadling, George-
dc.date.accessioned2018-05-07T08:58:39Z-
dc.date.available2018-05-07T08:58:39Z-
dc.date.issued2017en_US
dc.identifier.issn1574-1818en_US
dc.identifier.urihttp://hdl.handle.net/10553/35732-
dc.description.abstractWe present results from new experiments to study the dynamics of radiative shocks, reverse shocks and radiative precursors. Laser ablation of a solid piston by the Orion high-power laser at AWE Aldermaston UK was used to drive radiative shocks into a gas cell initially pressurised between 0.1 and 1.0 bar with different noble gases. Shocks propagated at 80 +/- 10 km/s and experienced strong radiative cooling resulting in post-shock compressions of x25 +/- 2. A combination of X-ray backlighting, optical self-emission streak imaging and interferometry (multi-frame and streak imaging) were used to simultaneously study both the shock front and the radiative precursor. These experiments present a new configuration to produce counter-propagating radiative shocks, allowing for the study of reverse shocks and providing a unique platform for numerical validation. In addition, the radiative shocks were able to expand freely into a large gas volume without being confined by the walls of the gas cell. This allows for 3-D effects of the shocks to be studied which, in principle, could lead to a more direct comparison to astrophysical phenomena. By maintaining a constant mass density between different gas fills the shocks evolved with similar hydrodynamics but the radiative precursor was found to extend significantly further in higher atomic number gases (similar to 4 times further in xenon than neon). Finally, 1-D and 2-D radiative-hydrodynamic simulations are presented showing good agreement with the experimental data.en_US
dc.languageengen_US
dc.relation.ispartofHigh Energy Density Physicsen_US
dc.sourceHigh Energy Density Physics [ISSN 1574-1818], v. 23, p. 60-72en_US
dc.subject22 Físicaen_US
dc.subject.otherRadiative shocken_US
dc.subject.otherRadiative precursoren_US
dc.subject.otherCounter propagating shocksen_US
dc.titleCounter-propagating radiative shock experiments on the Orion laser and the formation of radiative precursorsen_US
dc.typeinfo:eu-repo/semantics/Articleen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.hedp.2017.03.002
dc.identifier.scopus85014848203
dc.identifier.isi000404314500008-
dcterms.isPartOfHigh Energy Density Physics
dcterms.sourceHigh Energy Density Physics[ISSN 1574-1818],v. 23, p. 60-72
dc.contributor.authorscopusid57189619639
dc.contributor.authorscopusid16239942100
dc.contributor.authorscopusid57208873213
dc.contributor.authorscopusid26421836300
dc.contributor.authorscopusid7003944992
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dc.contributor.authorscopusid7403380971
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dc.contributor.authorscopusid55613236067
dc.contributor.authorscopusid6603297950
dc.contributor.authorscopusid55751301600
dc.contributor.authorscopusid8854991300
dc.contributor.authorscopusid55607357900
dc.contributor.authorscopusid8849976300
dc.contributor.authorscopusid6603890490
dc.contributor.authorscopusid56517259400
dc.contributor.authorscopusid56314921800
dc.contributor.authorscopusid55566759900
dc.contributor.authorscopusid55285592600
dc.contributor.authorscopusid6602358670
dc.contributor.authorscopusid7006456591
dc.identifier.eissn1878-0563-
dc.description.lastpage72-
dc.description.firstpage60-
dc.relation.volume23-
dc.investigacionCienciasen_US
dc.type2Artículoen_US
dc.identifier.wosWOS:000404314500008-
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dc.identifier.investigatorRIDG-5818-2014-
dc.identifier.investigatorRIDR-2117-2018-
dc.identifier.investigatorRIDL-1938-2017-
dc.identifier.investigatorRIDNo ID-
dc.identifier.investigatorRIDNo ID-
dc.identifier.investigatorRIDNo ID-
dc.contributor.wosstandardWOS:Clayson, T
dc.contributor.wosstandardWOS:Suzuki-Vidal, F
dc.contributor.wosstandardWOS:Lebedev, SV
dc.contributor.wosstandardWOS:Swadling, GF
dc.contributor.wosstandardWOS:Stehle, C
dc.contributor.wosstandardWOS:Burdiak, GC
dc.contributor.wosstandardWOS:Foster, JM
dc.contributor.wosstandardWOS:Skidmore, J
dc.contributor.wosstandardWOS:Graham, P
dc.contributor.wosstandardWOS:Gumbrell, E
dc.contributor.wosstandardWOS:Patankar, S
dc.contributor.wosstandardWOS:Spindloe, C
dc.contributor.wosstandardWOS:Chaulagain, U
dc.contributor.wosstandardWOS:Kozlova, M
dc.contributor.wosstandardWOS:Larour, J
dc.contributor.wosstandardWOS:Singh, RL
dc.contributor.wosstandardWOS:Rodriguez, R
dc.contributor.wosstandardWOS:Gil, JM
dc.contributor.wosstandardWOS:Espinosa, G
dc.contributor.wosstandardWOS:Velarde, P
dc.contributor.wosstandardWOS:Danson, C
dc.date.coverdateJunio 2017
dc.identifier.ulpgces
dc.description.sjr0,933
dc.description.jcr1,696
dc.description.sjrqQ1
dc.description.jcrqQ3
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.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.orcid0000-0002-8326-3169-
crisitem.author.orcid0000-0001-9006-4128-
crisitem.author.orcid0000-0002-2317-7277-
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.fullNameRodríguez Pérez, Rafael-
crisitem.author.fullNameGil De La Fe, Juan Miguel-
crisitem.author.fullNameEspinosa Vivas, Guadalupe-
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