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        <identifier>oai:kanazawa-u.repo.nii.ac.jp:00010714</identifier>
        <datestamp>2024-06-20T06:08:04Z</datestamp>
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          <dc:title>Spatial variation in coda Q around the Nobi fault zone, central Japan: Relation to S-wave velocity and seismicity</dc:title>
          <jpcoar:creator>
            <jpcoar:creatorName>平松, 良浩</jpcoar:creatorName>
          </jpcoar:creator>
          <jpcoar:creator>
            <jpcoar:creatorName>Tsuji, Sugane</jpcoar:creatorName>
          </jpcoar:creator>
          <jpcoar:creator>
            <jpcoar:nameIdentifier nameIdentifierURI="https://kaken.nii.ac.jp/ja/search/?qm=80283092" nameIdentifierScheme="e-Rad">80283092</jpcoar:nameIdentifier>
            <jpcoar:creatorName>Hiramatsu, Yoshihiro</jpcoar:creatorName>
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          <datacite:description descriptionType="Abstract">We investigate the spatial variation in coda Q around the Nobi fault zone in a high strain rate zone to assess the relation between coda Q, shear wave velocity, and seismicity. Waveform data were obtained from dense seismic observations. Low coda Q that follows the Niigata-Kobe Tectonic Zone in the high strain rate zone is distinct at the lowest frequency band of 1 to 2∈Hz. However, at higher frequencies, such a spatial pattern in coda Q is unclear. A good positive correlation was found between coda Q at the 1- to 2-Hz frequency band and the S-wave velocity perturbation at 25-km depth, which suggests that the coda Q reflects the ductile deformation below the brittle-ductile transition zone. Furthermore, coda Q at the 1- to 2-Hz frequency band correlates negatively with seismicity at 10- to 15-km depth, which implies that there is a high stressing rate in the low coda Q area. These facts, together with results of previous studies, imply that a high deformation rate below the brittle-ductile transition zone produces the high strain rate observed by the Global Positioning System (GPS) on the surface in this region.</datacite:description>
          <dc:publisher>Springer</dc:publisher>
          <datacite:date dateType="Issued">2014-12-01</datacite:date>
          <datacite:date>2017-10-03</datacite:date>
          <dc:language>eng</dc:language>
          <dc:type rdf:resource="http://purl.org/coar/resource_type/c_6501">journal article</dc:type>
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          <jpcoar:identifier identifierType="DOI">https://doi.org/10.24517/00010701</jpcoar:identifier>
          <jpcoar:identifier identifierType="HDL">http://hdl.handle.net/2297/40599</jpcoar:identifier>
          <jpcoar:identifier identifierType="URI">https://kanazawa-u.repo.nii.ac.jp/records/10714</jpcoar:identifier>
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            <jpcoar:relatedIdentifier identifierType="DOI">10.1186/1880-5981-66-97</jpcoar:relatedIdentifier>
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          <jpcoar:sourceIdentifier identifierType="NCID">AA11211921</jpcoar:sourceIdentifier>
          <jpcoar:sourceIdentifier identifierType="ISSN">1343-8832</jpcoar:sourceIdentifier>
          <jpcoar:sourceTitle>Earth, Planets and Space</jpcoar:sourceTitle>
          <jpcoar:volume>66</jpcoar:volume>
          <jpcoar:issue>1</jpcoar:issue>
          <jpcoar:pageStart>97</jpcoar:pageStart>
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            <jpcoar:URI label="SC-PR-HIRAMATSU-Y-97.pdf">https://kanazawa-u.repo.nii.ac.jp/record/10714/files/SC-PR-HIRAMATSU-Y-97.pdf</jpcoar:URI>
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            <datacite:date dateType="Available">2017-10-03</datacite:date>
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