Descripción
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Radiativeshockwavesplayapivotalroleinthetransportenergyintothestellarmedium.This facthasledtomanyeffortstoscaletheastrophysicalphenomenatoaccessiblelaboratory conditions andtheirstudyhasbeenhighlightedasanarearequiringfurtherexperimental investigations.Lowdensitymaterialwithhighatomicmassissuitabletoachieveradiative regime,and,therefore,lowdensityxenongasiscommonlyusedforthemediuminwhichthe radiativeshockssuchasradiativeblastwavespropagate.Inthiswork,bymeansofcollisional- radiativesteady-statecalculations,acharacterizationandananalysisofmicroscopicmagni- tudesoflaboratoryblastwaveslaunchedinxenonclustersaremade.Thus,forexample,the averageionization,thechargestatedistribution,thecoolingtimeorphotonmeanfreepaths arestudied.Furthermore,foraparticularexperiment,theeffectsoftheself-absorptionand self-emissioninthespecificintensityemittedbytheshockfrontandthatisgoingthroughthe radiativeprecursorareinvestigated.Finally,forthatexperiment,sincetheelectrontempera- tureisnotmeasuredexperimentally,anestimationofthismagnitudeismadebothforthe shockshellandtheradiativeprecursor. | |
Internacional
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Si |
JCR del ISI
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Si |
Título de la revista
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JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER |
ISSN
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0022-4073 |
Factor de impacto JCR
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3,193 |
Información de impacto
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Volumen
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125 |
DOI
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10.1016/j.jqsrt.2013.03.019 |
Número de revista
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Desde la página
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69 |
Hasta la página
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83 |
Mes
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SIN MES |
Ranking
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0 |