<?xml version='1.0' encoding='UTF-8'?>
<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>2026-03-09T17:46:31Z</responseDate>
  <request verb="GetRecord" metadataPrefix="oai_dc" identifier="oai:kitami-it.repo.nii.ac.jp:00006906">https://kitami-it.repo.nii.ac.jp/oai</request>
  <GetRecord>
    <record>
      <header>
        <identifier>oai:kitami-it.repo.nii.ac.jp:00006906</identifier>
        <datestamp>2026-02-24T04:47:38Z</datestamp>
        <setSpec>1:87</setSpec>
      </header>
      <metadata>
        <oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns="http://www.w3.org/2001/XMLSchema" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
          <dc:title>Influence of oxygen flow ratio on the oxidation of Ti target and the formation process of TiO_2 films by reactive sputtering</dc:title>
          <dc:creator>Takamura, K.</dc:creator>
          <dc:creator>Abe, Y.</dc:creator>
          <dc:creator>Sasaki, K.</dc:creator>
          <dc:description>Ti and TiO_2 films were deposited by RF reactive sputtering using a mixed gas of Ar and O_2. TiO_2 films were found to be formed at oxygen flow ratios above 7%. At the critical O_2 flow ratio, the amount of supplied Ti atoms was found to agree with that of O_2 molecules. Above the critical O_2 flow ratio, the amount of supplied O_2 molecules exceeded the gettering effect of the sputtering Ti atoms and oxygen density in the plasma began to increase. As a result, the surface of the Ti target was oxidized and TiO_2 films were formed. The thickness of the oxide film formed on the Ti target increased with increasing oxygen flow ratio and a maximum thickness of 5-6 nm was obtained at oxygen flow ratios of 40-100%.</dc:description>
          <dc:description>application/pdf</dc:description>
          <dc:description>journal article</dc:description>
          <dc:publisher>Elsevier</dc:publisher>
          <dc:date>2004-06</dc:date>
          <dc:format>application/pdf</dc:format>
          <dc:identifier>Vacuum</dc:identifier>
          <dc:identifier>3-4</dc:identifier>
          <dc:identifier>74</dc:identifier>
          <dc:identifier>397</dc:identifier>
          <dc:identifier>401</dc:identifier>
          <dc:identifier>https://kitami-it.repo.nii.ac.jp/record/6906/files/4655.pdf</dc:identifier>
          <dc:identifier>https://kitami-it.repo.nii.ac.jp/records/6906</dc:identifier>
          <dc:language>eng</dc:language>
          <dc:relation>http://doi.org/10.1016/j.vacuum.2004.01.006</dc:relation>
          <dc:rights>http://www.sciencedirect.com/science/journal/0042207X</dc:rights>
          <dc:rights>Elsevier Ltd., K. Takamura, Y. Abe and K. Sasaki, Vacuum, 74(3-4), 2004, 397-401.</dc:rights>
          <dc:rights>open access</dc:rights>
        </oai_dc:dc>
      </metadata>
    </record>
  </GetRecord>
</OAI-PMH>
