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    <journal-meta>
      <journal-title-group><journal-title>SET Proceedings</journal-title></journal-title-group>
      <issn pub-type="epub">2978-4387</issn>
      <publisher><publisher-name>Caravel Press</publisher-name></publisher>
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.65582/set.2010.131</article-id>
      <article-id pub-id-type="publisher-id">2010.131</article-id>
      <title-group><article-title>Numerical simulation of a high temperature solar thermal receiver</article-title></title-group>
    <contrib-group>
      <contrib contrib-type="author">
        <name><surname>Wu</surname><given-names>Xiaocui</given-names></name>
        <xref ref-type="aff" rid="aff1"/>
      </contrib>
      <contrib contrib-type="author">
        <name><surname>Huang</surname><given-names>Hulin</given-names></name>
        <xref ref-type="aff" rid="aff1"/>
        <email>hlhuang@nuaa.edu.cn</email>
      </contrib>
      <aff id="aff1">Academy of Frontier Science, Nanjing University of Aeronautics and Astronautics, Nanjing, 210016, P.R.China</aff>
    </contrib-group>
      <pub-date publication-format="electronic" date-type="pub"><day>24</day><month>08</month><year>2010</year></pub-date>
      <volume>9</volume>
      <isbn publication-format="electronic">978-1-995850-04-7</isbn>
      <fpage>1</fpage>
      <lpage>9</lpage>
      <self-uri xlink:href="https://caravelpress.com/proceedings/set/papers/2010.131"/>
      <history>
        <date date-type="received"><string-date>24 August 2010</string-date></date>
      </history>
      <permissions>
        <copyright-statement>© 2010 Copyright WSSET</copyright-statement>
        <copyright-year>2010</copyright-year>
      </permissions>
      <abstract><p>The solar high temperature receiver is a key component of solar energy application for a high temperature thermal or a thermochemical process, which absorbs concentrated sunlight and transfers its energy to a working medium (gas, liquid or solid particles). In various attractive high-performance solar receivers, the Directly Irradiated Annular Pressurized Receiver (DIAPR) is a volumetric (directly irradiated), windowed cavity receiver which has some advantageous characteristics, such as supplying hot gas at a pressure of 10-30 bar and exit temperature of up to 1300°C and the aperture flux of up to 10 MW/m². This paper simulated numerically using the Fluent software the hydrogen flow field, temperature field and transfer efficiency of solar energy to the modified DIAPR, whose absorber was made of a layer high-temperature ceramic bubbles. The results show that the exit temperature of gas is up to 1500K and the solar energy transfer efficiency is up to 0.86.</p></abstract>
      <kwd-group kwd-group-type="author">
        <kwd>Directly Irradiated Annular Pressurized Receiver DIAPR numerical simulation solar thermal receiver</kwd>
      </kwd-group>
      <conference>
        <conf-date>24 to 27 August 2010</conf-date>
        <conf-name>9th International Conference on Sustainable Energy Technologies</conf-name>
        <conf-acronym>SET2010</conf-acronym>
        <conf-num>9</conf-num>
        <conf-loc>Shanghai, China</conf-loc>
      </conference>
    </article-meta>
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