<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-05-05T20:48:15Z</responseDate><request verb="GetRecord" identifier="oai:uvadoc.uva.es:10324/64399" metadataPrefix="qdc">https://uvadoc.uva.es/oai/request</request><GetRecord><record><header><identifier>oai:uvadoc.uva.es:10324/64399</identifier><datestamp>2024-01-10T20:01:16Z</datestamp><setSpec>com_10324_1159</setSpec><setSpec>com_10324_931</setSpec><setSpec>com_10324_894</setSpec><setSpec>col_10324_1310</setSpec></header><metadata><qdc:qualifieddc xmlns:qdc="http://dspace.org/qualifieddc/" xmlns:doc="http://www.lyncode.com/xoai" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:dc="http://purl.org/dc/elements/1.1/" xsi:schemaLocation="http://purl.org/dc/elements/1.1/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dc.xsd http://purl.org/dc/terms/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dcterms.xsd http://dspace.org/qualifieddc/ http://www.ukoln.ac.uk/metadata/dcmi/xmlschema/qualifieddc.xsd">
<dc:title>Demonstration of Geometric Effects and Resonant Scattering in the X-Ray Spectra of High-Energy-Density Plasmas</dc:title>
<dc:creator>Marley, E. V.</dc:creator>
<dc:creator>Liedahl, D. A.</dc:creator>
<dc:creator>Jarrott, L. C.</dc:creator>
<dc:creator>Kemp, G. E.</dc:creator>
<dc:creator>Heeter, R. F.</dc:creator>
<dc:creator>Emig, J. A.</dc:creator>
<dc:creator>Foord, M. E.</dc:creator>
<dc:creator>Schneider, M. B.</dc:creator>
<dc:creator>Rose, S. J.</dc:creator>
<dc:creator>Wark, J. S.</dc:creator>
<dc:creator>Pérez Callejo, Gabriel</dc:creator>
<dcterms:abstract>In a plasma of sufficient size and density, photons emitted within the system have a probability of being re-absorbed and re-emitted multiple times - a phenomenon known in astrophysics as resonant scattering. This effect alters the ratio of optically-thick to optically thin lines, depending on the plasma geometry and viewing angle, and has significant implications for the spectra observed in a number of astrophysical scenarios, but has not previously been studied in a controlled laboratory plasma. We demonstrate the effect in the x-ray spectra emitted by cylindrical plasmas generated by high power laser irradiation, and the results confirm the geometrical interpretation of resonant scattering.</dcterms:abstract>
<dcterms:dateAccepted>2024-01-10T17:36:54Z</dcterms:dateAccepted>
<dcterms:available>2024-01-10T17:36:54Z</dcterms:available>
<dcterms:created>2024-01-10T17:36:54Z</dcterms:created>
<dcterms:issued>2021</dcterms:issued>
<dc:type>info:eu-repo/semantics/article</dc:type>
<dc:identifier>Physical Review Letters, Febrero 2021, vol. 126, p. 085001</dc:identifier>
<dc:identifier>0031-9007</dc:identifier>
<dc:identifier>https://uvadoc.uva.es/handle/10324/64399</dc:identifier>
<dc:identifier>10.1103/PhysRevLett.126.085001</dc:identifier>
<dc:identifier>8</dc:identifier>
<dc:identifier>Physical Review Letters</dc:identifier>
<dc:identifier>126</dc:identifier>
<dc:identifier>1079-7114</dc:identifier>
<dc:language>eng</dc:language>
<dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
<dc:publisher>American Physical Society</dc:publisher>
</qdc:qualifieddc></metadata></record></GetRecord></OAI-PMH>