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<dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:invenio="http://invenio-software.org/elements/1.0" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"><dc:identifier>doi:10.1063/1.4949216</dc:identifier><dc:language>eng</dc:language><dc:creator>Fernández-García, A.</dc:creator><dc:creator>Sutter, F.</dc:creator><dc:creator>Heimsath, A.</dc:creator><dc:creator>Montecchi, M.</dc:creator><dc:creator>Sallaberry, F.</dc:creator><dc:creator>Peña Lapuente, Adrián</dc:creator><dc:creator>Delord, C.</dc:creator><dc:creator>Martínez-Arcos, L.</dc:creator><dc:creator>Reche-Navarro, T.</dc:creator><dc:creator>Schmid, T.</dc:creator><dc:creator>Heras Vila, Carlos David</dc:creator><dc:title>Simplified analysis of solar-weighted specular reflectance for mirrors with high specularity</dc:title><dc:identifier>ART-2016-96286</dc:identifier><dc:description>The most relevant parameter to properly characterize solar mirrors is the solar-weighted near-specular reflectance. As this parameter cannot be directly measured with off-the-shelf instruments, a simplified procedure to be applied for highly specular solar mirrors is proposed in this paper. The approach, based on two criteria, was experimentally employed to check a wide variety of solar reflector materials. Only those mirrors with known high specularity passed the criteria, indicating that the proposed method is suitable.</dc:description><dc:date>2016</dc:date><dc:source>http://zaguan.unizar.es/record/56801</dc:source><dc:doi>10.1063/1.4949216</dc:doi><dc:identifier>http://zaguan.unizar.es/record/56801</dc:identifier><dc:identifier>oai:zaguan.unizar.es:56801</dc:identifier><dc:identifier.citation>AIP conference proceedings 1734 (2016), 130006 [8 pp.]</dc:identifier.citation><dc:rights>by</dc:rights><dc:rights>http://creativecommons.org/licenses/by/3.0/es/</dc:rights><dc:rights>info:eu-repo/semantics/openAccess</dc:rights></dc:dc>

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