Identificador persistente para citar o vincular este elemento:
http://hdl.handle.net/10553/35732
Campo DC | Valor | idioma |
---|---|---|
dc.contributor.author | Clayson, T. | en_US |
dc.contributor.author | Suzuki-Vidal, F. | en_US |
dc.contributor.author | Lebedev, S. V. | en_US |
dc.contributor.author | Swadling, G.F. | en_US |
dc.contributor.author | Stehlé, C. | en_US |
dc.contributor.author | Burdiak, G. | en_US |
dc.contributor.author | Foster, J.M. | en_US |
dc.contributor.author | Skidmore, J. | en_US |
dc.contributor.author | Graham, P. | en_US |
dc.contributor.author | Gumbrell, E.T. | en_US |
dc.contributor.author | Patankar, S. | en_US |
dc.contributor.author | Spindloe, C. | en_US |
dc.contributor.author | Chaulagain, U. | en_US |
dc.contributor.author | Kozlova, M. | en_US |
dc.contributor.author | Larour, J. | en_US |
dc.contributor.author | Singh, R. L. | en_US |
dc.contributor.author | Rodriguez, R. | en_US |
dc.contributor.author | Gil, J. M. | en_US |
dc.contributor.author | Espinosa Vivas, Guadalupe | en_US |
dc.contributor.author | Velarde, P. | en_US |
dc.contributor.author | Danson, C. | en_US |
dc.contributor.other | Michaela, Kozlova | - |
dc.contributor.other | Gil de la Fe, Juan Miguel | - |
dc.contributor.other | Rodriguez, Rafael | - |
dc.contributor.other | Fyrth, Jim | - |
dc.contributor.other | Chaulagain, Uddhab | - |
dc.contributor.other | Swadling, George | - |
dc.date.accessioned | 2018-05-07T08:58:39Z | - |
dc.date.available | 2018-05-07T08:58:39Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 1574-1818 | en_US |
dc.identifier.uri | http://hdl.handle.net/10553/35732 | - |
dc.description.abstract | We 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.language | eng | en_US |
dc.relation.ispartof | High Energy Density Physics | en_US |
dc.source | High Energy Density Physics [ISSN 1574-1818], v. 23, p. 60-72 | en_US |
dc.subject | 22 Física | en_US |
dc.subject.other | Radiative shock | en_US |
dc.subject.other | Radiative precursor | en_US |
dc.subject.other | Counter propagating shocks | en_US |
dc.title | Counter-propagating radiative shock experiments on the Orion laser and the formation of radiative precursors | en_US |
dc.type | info:eu-repo/semantics/Article | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1016/j.hedp.2017.03.002 | |
dc.identifier.scopus | 85014848203 | |
dc.identifier.isi | 000404314500008 | - |
dcterms.isPartOf | High Energy Density Physics | |
dcterms.source | High Energy Density Physics[ISSN 1574-1818],v. 23, p. 60-72 | |
dc.contributor.authorscopusid | 57189619639 | |
dc.contributor.authorscopusid | 16239942100 | |
dc.contributor.authorscopusid | 57208873213 | |
dc.contributor.authorscopusid | 26421836300 | |
dc.contributor.authorscopusid | 7003944992 | |
dc.contributor.authorscopusid | 38360928400 | |
dc.contributor.authorscopusid | 57210545375 | |
dc.contributor.authorscopusid | 7403380971 | |
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dc.contributor.authorscopusid | 55285592600 | |
dc.contributor.authorscopusid | 6602358670 | |
dc.contributor.authorscopusid | 7006456591 | |
dc.identifier.eissn | 1878-0563 | - |
dc.description.lastpage | 72 | - |
dc.description.firstpage | 60 | - |
dc.relation.volume | 23 | - |
dc.investigacion | Ciencias | en_US |
dc.type2 | Artículo | en_US |
dc.identifier.wos | WOS:000404314500008 | - |
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dc.identifier.investigatorRID | G-5818-2014 | - |
dc.identifier.investigatorRID | R-2117-2018 | - |
dc.identifier.investigatorRID | L-1938-2017 | - |
dc.identifier.investigatorRID | No ID | - |
dc.identifier.investigatorRID | No ID | - |
dc.identifier.investigatorRID | No ID | - |
dc.contributor.wosstandard | WOS:Clayson, T | |
dc.contributor.wosstandard | WOS:Suzuki-Vidal, F | |
dc.contributor.wosstandard | WOS:Lebedev, SV | |
dc.contributor.wosstandard | WOS:Swadling, GF | |
dc.contributor.wosstandard | WOS:Stehle, C | |
dc.contributor.wosstandard | WOS:Burdiak, GC | |
dc.contributor.wosstandard | WOS:Foster, JM | |
dc.contributor.wosstandard | WOS:Skidmore, J | |
dc.contributor.wosstandard | WOS:Graham, P | |
dc.contributor.wosstandard | WOS:Gumbrell, E | |
dc.contributor.wosstandard | WOS:Patankar, S | |
dc.contributor.wosstandard | WOS:Spindloe, C | |
dc.contributor.wosstandard | WOS:Chaulagain, U | |
dc.contributor.wosstandard | WOS:Kozlova, M | |
dc.contributor.wosstandard | WOS:Larour, J | |
dc.contributor.wosstandard | WOS:Singh, RL | |
dc.contributor.wosstandard | WOS:Rodriguez, R | |
dc.contributor.wosstandard | WOS:Gil, JM | |
dc.contributor.wosstandard | WOS:Espinosa, G | |
dc.contributor.wosstandard | WOS:Velarde, P | |
dc.contributor.wosstandard | WOS:Danson, C | |
dc.date.coverdate | Junio 2017 | |
dc.identifier.ulpgc | Sí | es |
dc.description.sjr | 0,933 | |
dc.description.jcr | 1,696 | |
dc.description.sjrq | Q1 | |
dc.description.jcrq | Q3 | |
dc.description.scie | SCIE | |
item.grantfulltext | open | - |
item.fulltext | Con texto completo | - |
crisitem.author.dept | GIR IUNAT: Interacción Radiación-Materia | - |
crisitem.author.dept | IU de Estudios Ambientales y Recursos Naturales | - |
crisitem.author.dept | Departamento de Física | - |
crisitem.author.dept | GIR IUNAT: Interacción Radiación-Materia | - |
crisitem.author.dept | IU de Estudios Ambientales y Recursos Naturales | - |
crisitem.author.dept | Departamento de Física | - |
crisitem.author.dept | GIR IUNAT: Interacción Radiación-Materia | - |
crisitem.author.dept | IU de Estudios Ambientales y Recursos Naturales | - |
crisitem.author.dept | Departamento de Física | - |
crisitem.author.orcid | 0000-0002-8326-3169 | - |
crisitem.author.orcid | 0000-0001-9006-4128 | - |
crisitem.author.orcid | 0000-0002-2317-7277 | - |
crisitem.author.parentorg | IU de Estudios Ambientales y Recursos Naturales | - |
crisitem.author.parentorg | IU de Estudios Ambientales y Recursos Naturales | - |
crisitem.author.parentorg | IU de Estudios Ambientales y Recursos Naturales | - |
crisitem.author.fullName | Rodríguez Pérez, Rafael | - |
crisitem.author.fullName | Gil De La Fe, Juan Miguel | - |
crisitem.author.fullName | Espinosa Vivas, Guadalupe | - |
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