<didl:DIDL xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:didl="urn:mpeg:mpeg21:2002:02-DIDL-NS" xsi:schemaLocation="urn:mpeg:mpeg21:2002:02-DIDL-NS 
			 http://standards.iso.org/ittf/PubliclyAvailableStandards/MPEG-21_schema_files/did/didmodel.xsd"><didl:Item><didl:Descriptior><didl:Statement mimeType="application/xml; charset=utf-8"><dii:Identifier xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="urn:mpeg:mpeg21:2002:01-DII-NS
		 	http://standards.iso.org/ittf/PubliclyAvailableStandards/MPEG-21_schema_files/dii/dii.xsd" xmlns:dii="urn:mpeg:mpeg21:2002:01-DII-NS">http://eprints.utas.edu.au/382/</dii:Identifier></didl:Statement></didl:Descriptior><didl:Descriptior><didl:Statement mimeType="application/xml; charset=utf-8"><oai_dc:dc 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" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/">
        <dc:title>Magmatic origin of low-Ca olivine in subduction-related magmas: Co-existence of contrasting magmas</dc:title>
        <dc:creator>Kamenetsky, VS</dc:creator>
        <dc:creator>Elburg, MA</dc:creator>
        <dc:creator>Arculus, RJ</dc:creator>
        <dc:creator>Thomas, R</dc:creator>
        <dc:subject>260100 Geology</dc:subject>
        <dc:description>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.</dc:description>
        <dc:date>2006-10</dc:date>
        <dc:type>Article</dc:type>
        <dc:type>PeerReviewed</dc:type>
        <dc:format>application/pdf</dc:format>
        <dc:identifier>http://eprints.utas.edu.au/382/1/CG-lowCa-olivine.pdf</dc:identifier>
        <dc:relation>http://dx.doi.org/10.1016/j.chemgeo.2006.03.010</dc:relation>
        <dc:identifier>Kamenetsky, VS and Elburg, MA and Arculus, RJ and Thomas, R (2006) Magmatic origin of low-Ca olivine in subduction-related magmas: Co-existence of contrasting magmas. Chemical Geology, 233 (3-4). pp. 346-357.</dc:identifier>
        <dc:relation>http://eprints.utas.edu.au/382/</dc:relation></oai_dc:dc></didl:Statement></didl:Descriptior><didl:Component><didl:Descriptior><didl:Statement mimeType="application/xml; charset=utf-8"><dii:Identifier xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="urn:mpeg:mpeg21:2002:01-DII-NS
		 	    http://standards.iso.org/ittf/PubliclyAvailableStandards/MPEG-21_schema_files/dii/dii.xsd" xmlns:dii="urn:mpeg:mpeg21:2002:01-DII-NS">http://eprints.utas.edu.au/382/1/</dii:Identifier></didl:Statement></didl:Descriptior><didl:Resource ref="http://eprints.utas.edu.au/382/1/CG-lowCa-olivine.pdf"></didl:Resource></didl:Component></didl:Item></didl:DIDL>