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    <responseDate>2026-10-12T08:58:12Z</responseDate>
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    <identifier>10.57760/sciencedb.04609</identifier>
    <datestamp>2022-12-05T17:30:56Z</datestamp>
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<oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" 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:date>2022-12-05</dc:date>
  <dc:title>Measurement of tungsten impurity spectra with a two-crystal X-ray crystal spectrometer on EAST</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.04609</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>Spectral measurement of tungsten (W) impurity is essential to study impurity transport. Therefore, an X-ray crystal spectrometer (XCS) on EAST was used to measure the line spectra from highly ionized W ions. On EAST, both poloidal XCS and tangential XCS have been developed to measure the plasma temperature as well as the rotation velocity. Recently, He-like and H-like argon spectra have also been obtained using a two-crystal setup. W lines are identified in this study. Through a careful analysis, the W lines of 3.9336, 3.9321, and 3.664 &amp;Aring; are found to be diffracted by He-like or H-like crystals. The lines are confirmed with the NIST database. We also calculated the ion temperature with Doppler broadening of these lines. The ion temperature from the W lines is entirely consistent with that from Ar line spectra. The measurement of these W line spectra could be used to study W impurity transport in future work.</dc:description>
  <dc:subject>tungsten spectra; X-ray spectrometer; two-crystal</dc:subject>
  <dc:creator>Hongming Zhang</dc:creator>
  <dc:creator>Liang He</dc:creator>
  <dc:creator>Bo Lyu</dc:creator>
  <dc:creator>Jun Chen</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:relation>http://www.doi.org/10.1088/2058-6272/ab84ee</dc:relation>
  <dc:publisher>Science Data Bank</dc:publisher>
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