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      <rec-number>1</rec-number>
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      <ref-type name="Journal Article">17</ref-type>
      <work-type>ACL : Articles dans des revues avec comité de lecture répertoriées par l'AERES</work-type>
      <contributors>
        <authors>
          <author>
            <style face="normal" font="default" size="100%">Rivera, M.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Martin, H.</style>
          </author>
          <author>
            <style face="bold" font="default" size="100%">Le Pennec, Jean-Luc</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Thouret, J. C.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Gourgaud, A.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Gerbe, M. C.</style>
          </author>
        </authors>
      </contributors>
      <titles>
        <title>Petro-geochemical constraints on the source and evolution of magmas at El Misti volcano (Peru)</title>
        <secondary-title>Lithos</secondary-title>
      </titles>
      <pages>240-259</pages>
      <keywords>
        <keyword>El Misti</keyword>
        <keyword>Central Andes</keyword>
        <keyword>Arc magmatism</keyword>
        <keyword>Magmatic evolution</keyword>
        <keyword>Geochemistry</keyword>
        <keyword>Assimilation-fractional crystallisation</keyword>
        <keyword>PEROU</keyword>
        <keyword>ANDES</keyword>
        <keyword>EL MISTI VOLCAN</keyword>
      </keywords>
      <dates>
        <year>2017</year>
      </dates>
      <call-num>fdi:010068904</call-num>
      <language>ENG</language>
      <periodical>
        <full-title>Lithos</full-title>
      </periodical>
      <isbn>0024-4937</isbn>
      <accession-num>ISI:000392680400016</accession-num>
      <electronic-resource-num>10.1016/j.lithos.2016.11.009</electronic-resource-num>
      <urls>
        <related-urls>
          <url>https://www.documentation.ird.fr/hor/fdi:010068904</url>
        </related-urls>
        <pdf-urls>
          <url>https://www.documentation.ird.fr/intranet/publi/2017/02/010068904.pdf</url>
        </pdf-urls>
      </urls>
      <volume>268</volume>
      <remote-database-provider>Horizon (IRD)</remote-database-provider>
      <abstract>El Misti volcano, a large and hazardous edifice of the Andean Central Volcanic Zone (CVZ) of southern Peru, consists of four main growth stages. Misti 1 (&gt;112 ka) is an old stratovolcano partly concealed by two younger stratocones (Misti 2, 112-40 ka; Misti 3, 38-11 ka), capped in turn by a recent summit cone (Misti 4, &lt;11 ka). In order to gain insights into magma composition controls on eruptive behaviour through time at El Misti, we have conducted a petrological and geochemical study of selected rock samples from the main growth stages of the volcano. Whole rock compositions range from andesite to rhyolite and belong to a medium to high-K calk alkaline magmatic suite. El Misti samples are characterised by high large-ion lithophile elements, but low concentrations of high field strength elements, and heavy rare earth elements, consistent with a subduction zone setting. The Sr-87/Sr-86 (0.70715-0.70882) and Nd-143/Nd-144 (0.511983-0.512277) isotope ratios suggest that magma composition is significantly affected by contamination and/or assimilation processes during their evolution, likely due to the presence of thick (65-70 km) continental crust beneath the CVZ in southern Peru. Geochemical evidence indicates that magmatic evolution is mostly controlled by Assimilation-Fractional Crystallisation (AFC) mechanisms. Modelling reveals a mass-assimilated/mass-fractionated ratio (p) &lt;= 2.2, which suggests an assimilated crust fraction below 14 wt.% on average. Our isotopic data clearly identify the Proterozoic "Charcani gneiss" basement as the main contaminant. Both contamination and assimilation processes peaked at similar to 30 wt.%, during the Misti 3 stage when rhyolites were generated. We ascribe the general depletion in HREE and Y and elevated La/Yb and Sr/Y ratios in El Misti samples to the enrichment of the mantle wedge source of the parental magmas by a felsic melt of adakitic composition and hydrous fluids. Our work highlights that El Misti's magmatic system has remained relatively homogeneous since at least 0.12 Ma, with a marked influence of the contaminating crust in the Late Pleistocene Misti 3 stage, which resulted in highly explosive eruptions. Andesitic-dacitic compositions are dominant in the Holocene and historical Misti 4 stage, and are expected for future volcanic events at El Misti.</abstract>
      <custom6>066 ; 064</custom6>
      <custom1>UR163</custom1>
      <custom7>Pérou</custom7>
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