<?xml version="1.0"?>
<oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" 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">
  <dc:title>Petro-geochemical constraints on the source and evolution of magmas at El Misti volcano (Peru)</dc:title>
  <dc:creator>Rivera, M.</dc:creator>
  <dc:creator>Martin, H.</dc:creator>
  <dc:creator>/Le Pennec, Jean-Luc</dc:creator>
  <dc:creator>Thouret, J. C.</dc:creator>
  <dc:creator>Gourgaud, A.</dc:creator>
  <dc:creator>Gerbe, M. C.</dc:creator>
  <dc:subject>El Misti</dc:subject>
  <dc:subject>Central Andes</dc:subject>
  <dc:subject>Arc magmatism</dc:subject>
  <dc:subject>Magmatic evolution</dc:subject>
  <dc:subject>Geochemistry</dc:subject>
  <dc:subject>Assimilation-fractional crystallisation</dc:subject>
  <dc:description>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.</dc:description>
  <dc:date>2017</dc:date>
  <dc:type>text</dc:type>
  <dc:identifier>https://www.documentation.ird.fr/hor/fdi:010068904</dc:identifier>
  <dc:identifier>fdi:010068904</dc:identifier>
  <dc:identifier>Rivera M., Martin H., Le Pennec Jean-Luc, Thouret J. C., Gourgaud A., Gerbe M. C.. Petro-geochemical constraints on the source and evolution of magmas at El Misti volcano (Peru). 2017, 268,  240-259</dc:identifier>
  <dc:language>EN</dc:language>
  <dc:coverage>PEROU</dc:coverage>
  <dc:coverage>ANDES</dc:coverage>
  <dc:coverage>EL MISTI VOLCAN</dc:coverage>
</oai_dc:dc>
