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    <eprintid>382</eprintid>
    <rev_number>6</rev_number>
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    <dir>disk0/00/00/03/82</dir>
    <datestamp>2006-09-14</datestamp>
    <lastmod>2008-07-18 09:42:57</lastmod>
    <status_changed>2008-07-16 15:45:29</status_changed>
    <type>article</type>
    <metadata_visibility>show</metadata_visibility>
    <contact_email>Dima.Kamenetsky@utas.edu.au</contact_email>
    <creators>
      <item>
        <name>
          <family>Kamenetsky</family>
          <given>VS</given>
        </name>
        <id></id>
      </item>
      <item>
        <name>
          <family>Elburg</family>
          <given>MA</given>
        </name>
        <id></id>
      </item>
      <item>
        <name>
          <family>Arculus</family>
          <given>RJ</given>
        </name>
        <id></id>
      </item>
      <item>
        <name>
          <family>Thomas</family>
          <given>R</given>
        </name>
        <id></id>
      </item>
    </creators>
    <title>Magmatic origin of low-Ca olivine in subduction-related magmas: Co-existence of contrasting magmas</title>
    <ispublished>pub</ispublished>
    <subjects>
      <item>260100</item>
    </subjects>
    <full_text_status>restricted</full_text_status>
    <monograph_type>NULL</monograph_type>
    <keywords>Island-arc magmas; Picrites; Olivine; Clinoenstatite; Magmatic inclusions; Xenocrysts; Mantle</keywords>
    <suggestions>(15/4 SvA) fixed initials, added DOI and URL; restricted access as is an Elsevier journal and pub version cannot be used.</suggestions>
    <abstract>Unravelling the origin of different components contributing to subduction-related magmas is a prerequisite to understanding the sources and processes involved in their origins. Mafic, high-Ca subduction-related magmas from geographically-diverse areas (Indonesia, Solomon Islands, Kamchatka, Valu Fa Ridge) contain two populations of olivine crystals, of which only the high-Ca population (CaO = 0.3-0.5 wt.%) crystallized from the melt that dominantly contributed to the whole rock composition. Forsterite-rich (Fo90-94), low-Ca (CaO &lt; 0.15 wt.%), high-Ni (NiO &gt; 0.3 wt.%) olivine crystals, which constitute 16-37 vol.% of total olivine population, are generally interpreted as mantle or lithospheric xenocrysts. However, in these samples, the olivine shape and chemical zoning, the composition of included minerals (orthopyroxene, clinoenstatite and Cr-spinel) and presence of melt inclusions, are indications that these crystals are phenocrysts from a mafic magma with high silica and low calcium contents. The coexistence of contrasting magmas (mafic high-Ca silica-poor versus low-Ca silica-rich) within a number of arc systems and their mixing may not be a rare event, and should be taken into account when developing models of arc petrogenesis.</abstract>
    <date>2006-10</date>
    <date_type>published</date_type>
    <publication>Chemical Geology</publication>
    <volume>233</volume>
    <number>3-4</number>
    <pagerange>346-357</pagerange>
    <id_number>10.1016/j.chemgeo.2006.03.010</id_number>
    <institution>University of Tasmania</institution>
    <thesis_type>UNSPECIFIED</thesis_type>
    <refereed>TRUE</refereed>
    <official_url>http://dx.doi.org/10.1016/j.chemgeo.2006.03.010</official_url>
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