<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>0718-7106</journal-id>
<journal-title><![CDATA[Andean geology]]></journal-title>
<abbrev-journal-title><![CDATA[AndGeo]]></abbrev-journal-title>
<issn>0718-7106</issn>
<publisher>
<publisher-name><![CDATA[Servicio Nacional de Geología y Minería (SERNAGEOMIN)]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0718-71062012000100008</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Volcanic stratigraphy and evidence of magma mixing in the Quaternary Payún Matrú volcano, andean backarc in western Argentina]]></article-title>
<article-title xml:lang="es"><![CDATA[Estratigrafía volcánica y evidencia de mezcla de magmas en el volcán Payún Matrú del Cuaternario, en el retroarco andino de Argentina occidental]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Hernando]]></surname>
<given-names><![CDATA[Irene R]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Llambías]]></surname>
<given-names><![CDATA[Eduardo J]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[González]]></surname>
<given-names><![CDATA[Pablo D]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Sato]]></surname>
<given-names><![CDATA[Kei]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Centro de Investigaciones Geológicas  ]]></institution>
<addr-line><![CDATA[La Plata ]]></addr-line>
<country>Argentina</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Universidade de São Paulo Instituto de Geociências Centro de Pesquisas Geocronológicas]]></institution>
<addr-line><![CDATA[São Paulo ]]></addr-line>
<country>Brasil</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>01</month>
<year>2012</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>01</month>
<year>2012</year>
</pub-date>
<volume>39</volume>
<numero>1</numero>
<fpage>158</fpage>
<lpage>179</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.cl/scielo.php?script=sci_arttext&amp;pid=S0718-71062012000100008&amp;lng=en&amp;nrm=iso&amp;tlng=en"></self-uri><self-uri xlink:href="http://www.scielo.cl/scielo.php?script=sci_abstract&amp;pid=S0718-71062012000100008&amp;lng=en&amp;nrm=iso&amp;tlng=en"></self-uri><self-uri xlink:href="http://www.scielo.cl/scielo.php?script=sci_pdf&amp;pid=S0718-71062012000100008&amp;lng=en&amp;nrm=iso&amp;tlng=en"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[The Payún Matrú Volcanic Field is located in the Payenia Basaltic Province of the recent back-arc of western Argentina (35°S-38°S). This province is younger than 5 Ma, and most of its volcanic activity took place since 2 Ma. The Payún Matrú Volcanic Field contains two composite volcanoes, Payún Matrú and Payún Liso, and two basaltic fields in an E-W oriented zone, located east and west of the Payún Matrú volcano. Payún Matrú is the largest volcano of this volcanic field, and consists of a shield-shaped edifice with a circular summit caldera of 8 km in diameter. The composition of both composite volcanoes is alkaline and predominantly trachytic, having also minor intermediate lavas. The basaltic fields consist of basalts and trachybasalts, with clinopyroxene and abundant olivine as phenocrysts and also in the groundmass. Textures indicating mixing and mingling processes, such as dusty plagioclases along with clear ones, biotite replaced by anhydrous minerals and two groundmasses with a fluid-fluid relationship, are common in the early pre-caldera stage of Payún Matrú and some post-caldera lavas. The latest post-caldera lavas are trachytic, with clean sanidine phenocrysts without disequilibrium textures. A remarkable characteristic of the Payún Matrú Volcanic Field is the fact that the Payún Matrú caldera is surrounded by basaltic fields at its base, while no basalts were erupted in the caldera region. We propose that the absence of basaltic lavas in the Payún Matrú volcano is due to the presence of a magmatic chamber below it, and that the mafic magmas rising from deeper levels were unable to erupt without interaction with more evolved melts. Intermediate hybrid magmas produced as a consequence of magma mixing and mingling between basaltic and trachytic magmas, are present in the early and mid-history of Payún Matrú volcano. We present here new information about the Quaternary Payún Matrú Volcanic Field derived from field work, petrography, and major element geochemistry and 87Sr/86Sr isotopic ratios. For the first time a detailed map of the Payún Matrú Volcanic Field and its volcanic stratigraphy, primarily based on field observations, are presented.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[El Campo Volcánico Payún Matrú está localizado en la Provincia Basáltica Payenia, en el retroarco reciente al oeste de Argentina (35°S-38°S). Esta provincia es más joven que 5 Ma, y la mayor parte de su actividad volcánica tuvo lugar desde hace 2 Ma. El Campo Volcánico Payún Matrú contiene dos volcanes compuestos, el Payún Matrú y el Payún Liso, así como dos campos basálticos en una franja E-W, ubicados al este y oeste del Payún Matrú. El Payún Matrú es el volcán más grande de este campo volcánico, y consiste en un edificio en forma de escudo con una caldera circular en su cúspide de 8 km de diámetro. La composición de ambos volcanes compuestos es alcalina y predominantemente traquítica, con menor participación de lavas intermedias. Los campos basálticos consisten en basaltos y traquibasaltos, con clinopiroxeno y abundante olivina como fenocristales, presentes también en la pasta. En la etapa pre-caldera del Payún Matrú y en algunas lavas post-caldera son comunes las texturas que indican procesos de mezcla de magmas, 'mixing' y 'mingling', como plagioclasas cribadas en panal de abejas junto con otras limpias, biotitas reemplazadas por minerales anhidros y la presencia de dos pastas con una relación fluido-fluido. Las lavas post-caldera tardías son traquíticas, con fenocristales limpios de sanidina y sin texturas de desequilibrio. Una característica destacable del Campo Volcánico Payún Matrú es el hecho de que la caldera está rodeada por campos basálticos en su base, mientras que no se han producido erupciones de basaltos en la zona de la caldera. Proponemos que la ausencia de lavas basálticas en el volcán Payún Matrú se debe a la presencia de una cámara magmática por debajo del mismo, y a que los magmas máficos que ascienden desde niveles más profundos fueron incapaces de extruirse sin interactuar antes con fundidos más evolucionados. Magmas intermedios híbridos, producidos a consecuencia de la mezcla entre magmas basálticos y traquíticos, están presentes en la historia temprana y media del volcán Payún Matrú. Presentamos aquí nueva información sobre el Campo Volcánico Payún Matrú de edad Cuaternaria, basada en trabajos de campo, petrografía, geoquímica de elementos mayoritarios y relaciones isotópicas de 87Sr/86Sr. Por primera vez se presenta un mapa detallado del Campo Volcánico Payún Matrú y su estratigrafía, basado fundamentalmente en observaciones de campo.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Payún Matrú caldera]]></kwd>
<kwd lng="en"><![CDATA[Alkaline basalts]]></kwd>
<kwd lng="en"><![CDATA[Magma mixing]]></kwd>
<kwd lng="en"><![CDATA[Back-arc magmatism]]></kwd>
<kwd lng="es"><![CDATA[Caldera del Payún Matrú]]></kwd>
<kwd lng="es"><![CDATA[Basaltos alcalinos]]></kwd>
<kwd lng="es"><![CDATA[Mezcla de magmas]]></kwd>
<kwd lng="es"><![CDATA[Magmatismo de retroarco]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[  	    <p align="justify"><font size="2" face="Verdana"><i>Andean Geology 39 (1): 158&#45;179. January, 2012    <br>   formerly Revista Geol&oacute;gica de Chile    <br>   <a href="http://www.andeangeology.cl/index.php/revista1" target="_blank">www.andeangeology.cl</a></i></font></p> 	    <p align="justify">&nbsp;</p>     <p align="justify"><font size="4" face="Verdana"><b>Volcanic stratigraphy and evidence of magma mixing in the Quaternary Pay&uacute;n Matr&uacute; volcano, andean backarc in western Argentina</b></font></p>     <p align="justify"><font size="3" face="Verdana"><b>Estratigraf&iacute;a volc&aacute;nica y evidencia de mezcla de magmas en el volc&aacute;n Pay&uacute;n Matr&uacute; del Cuaternario, en el retroarco andino de Argentina occidental</b></font></p>     <p align="justify">&nbsp;</p>     <p align="justify"><font size="2" face="Verdana"><b>Irene R. Hernando<sup>1</sup>, Eduardo J. Llamb&iacute;as<sup>1</sup>, Pablo D. Gonz&aacute;lez<sup>1</sup>, Kei Sato<sup>2</sup></b></font></p>  	    <p align="justify"><font size="2" face="Verdana"><i><sup>1</sup>&nbsp;Centro de Investigaciones Geol&oacute;gicas (CONICET&#45;UNLP), 1 No. 644, B1900TAC, La Plata, Argentina.</i> <a href="mailto:ihernando@cig.museo.unlp.edu.ar"><i>ihernando@cig.museo.unlp.edu.ar</i></a><i>;</i> <a href="mailto:llambias@cig.museo.unlp.edu.ar"><i>llambias@cig.museo.unlp.edu.ar</i></a><i>;</i> <a href="mailto:gonzapab@cig.museo.unlp.edu.ar"><i>gonzapab@cig.museo.unlp.edu.ar    ]]></body>
<body><![CDATA[<br> 	</i></a><i><sup>2</sup>&nbsp;Centro de Pesquisas Geocronol&oacute;gicas (CPGeo), Instituto de Geoci&ecirc;ncias, Universidade de S&atilde;o Paulo (IG&#45;USP), Rua do Lago 562, Cidade Universit&aacute;ria, CEP 05508&#45;080, S&atilde;o Paulo, Brasil.</i> <a href="mailto:keisato@usp.br"><i>keisato@usp.br</i></a></font></p>      <p align="justify"><hr size="1">     <p align="justify"><font size="2" face="Verdana"><b>ABSTRACT.</b> The Pay&uacute;n Matr&uacute; Volcanic Field is located in the Payenia Basaltic Province of the recent back&#45;arc of western Argentina (35&deg;S&#45;38&deg;S). This province is younger than 5 Ma, and most of its volcanic activity took place since 2 Ma. The Pay&uacute;n Matr&uacute; Volcanic Field contains two composite volcanoes, Pay&uacute;n Matr&uacute; and Pay&uacute;n Liso, and two basaltic fields in an E&#45;W oriented zone, located east and west of the Pay&uacute;n Matr&uacute; volcano. Pay&uacute;n Matr&uacute; is the largest volcano of this volcanic field, and consists of a shield&#45;shaped edifice with a circular summit caldera of 8 km in diameter. The composition of both composite volcanoes is alkaline and predominantly trachytic, having also minor intermediate lavas. The basaltic fields consist of basalts and trachybasalts, with clinopyroxene and abundant olivine as phenocrysts and also in the groundmass. Textures indicating mixing and mingling processes, such as dusty plagioclases along with clear ones, biotite replaced by anhydrous minerals and two groundmasses with a fluid&#45;fluid relationship, are common in the early pre&#45;caldera stage of Pay&uacute;n Matr&uacute; and some post&#45;caldera lavas. The latest post&#45;caldera lavas are trachytic, with clean sanidine phenocrysts without disequilibrium textures. A remarkable characteristic of the Pay&uacute;n Matr&uacute; Volcanic Field is the fact that the Pay&uacute;n Matr&uacute; caldera is surrounded by basaltic fields at its base, while no basalts were erupted in the caldera region. We propose that the absence of basaltic lavas in the Pay&uacute;n Matr&uacute; volcano is due to the presence of a magmatic chamber below it, and that the mafic magmas rising from deeper levels were unable to erupt without interaction with more evolved melts. Intermediate hybrid magmas produced as a consequence of magma mixing and mingling between basaltic and trachytic magmas, are present in the early and mid&#45;history of Pay&uacute;n Matr&uacute; volcano. We present here new information about the Quaternary Pay&uacute;n Matr&uacute; Volcanic Field derived from field work, petrography, and major element geochemistry and <sup>87</sup>Sr/<sup>86</sup>Sr isotopic ratios. For the first time a detailed map of the Pay&uacute;n Matr&uacute; Volcanic Field and its volcanic stratigraphy, primarily based on field observations, are presented.</font></p>     <p align="justify"><font size="2" face="Verdana"><i>Keywords: Pay&uacute;n Matr&uacute; caldera, Alkaline basalts, Magma mixing, Back&#45;arc magmatism.</i></font></p>     <p align="justify"><hr size="1">     <p align="justify"><font size="2" face="Verdana"><b>RESUMEN. </b> El Campo Volc&aacute;nico Pay&uacute;n Matr&uacute; est&aacute; localizado en la Provincia Bas&aacute;ltica Payenia, en el retroarco reciente al oeste de Argentina (35&deg;S&#45;38&deg;S). Esta provincia es m&aacute;s joven que 5 Ma, y la mayor parte de su actividad volc&aacute;nica tuvo lugar desde hace 2 Ma. El Campo Volc&aacute;nico Pay&uacute;n Matr&uacute; contiene dos volcanes compuestos, el Pay&uacute;n Matr&uacute; y el Pay&uacute;n Liso, as&iacute; como dos campos bas&aacute;lticos en una franja E&#45;W, ubicados al este y oeste del Pay&uacute;n Matr&uacute;. El Pay&uacute;n Matr&uacute; es el volc&aacute;n m&aacute;s grande de este campo volc&aacute;nico, y consiste en un edificio en forma de escudo con una caldera circular en su c&uacute;spide de 8 km de di&aacute;metro. La composici&oacute;n de ambos volcanes compuestos es alcalina y predominantemente traqu&iacute;tica, con menor participaci&oacute;n de lavas intermedias. Los campos bas&aacute;lticos consisten en basaltos y traquibasaltos, con clinopiroxeno y abundante olivina como fenocristales, presentes tambi&eacute;n en la pasta. En la etapa pre&#45;caldera del Pay&uacute;n Matr&uacute; y en algunas lavas post&#45;caldera son comunes las texturas que indican procesos de mezcla de magmas, 'mixing' y 'mingling', como plagioclasas cribadas en panal de abejas junto con otras limpias, biotitas reemplazadas por minerales anhidros y la presencia de dos pastas con una relaci&oacute;n fluido&#45;fluido. Las lavas post&#45;caldera tard&iacute;as son traqu&iacute;ticas, con fenocristales limpios de sanidina y sin texturas de desequilibrio. Una caracter&iacute;stica destacable del Campo Volc&aacute;nico Pay&uacute;n Matr&uacute; es el hecho de que la caldera est&aacute; rodeada por campos bas&aacute;lticos en su base, mientras que no se han producido erupciones de basaltos en la zona de la caldera. Proponemos que la ausencia de lavas bas&aacute;lticas en el volc&aacute;n Pay&uacute;n Matr&uacute; se debe a la presencia de una c&aacute;mara magm&aacute;tica por debajo del mismo, y a que los magmas m&aacute;ficos que ascienden desde niveles m&aacute;s profundos fueron incapaces de extruirse sin interactuar antes con fundidos m&aacute;s evolucionados. Magmas intermedios h&iacute;bridos, producidos a consecuencia de la mezcla entre magmas bas&aacute;lticos y traqu&iacute;ticos, est&aacute;n presentes en la historia temprana y media del volc&aacute;n Pay&uacute;n Matr&uacute;. Presentamos aqu&iacute; nueva informaci&oacute;n sobre el Campo Volc&aacute;nico Pay&uacute;n Matr&uacute; de edad Cuaternaria, basada en trabajos de campo, petrograf&iacute;a, geoqu&iacute;mica de elementos mayoritarios y relaciones isot&oacute;picas de <sup>87</sup>Sr/<sup>86</sup>Sr. Por primera vez se presenta un mapa detallado del Campo Volc&aacute;nico Pay&uacute;n Matr&uacute; y su estratigraf&iacute;a, basado fundamentalmente en observaciones de campo.</font></p>  	    <p align="justify"><font size="2" face="Verdana"><i>Palabras clave: Caldera del Pay&uacute;n Matr&uacute;, Basaltos alcalinos, Mezcla de magmas, Magmatismo de retroarco.</i></font></p> 	    <p align="justify"><hr size="1"> 	    <p align="justify"><font size="3" face="Verdana"><b>1. &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Introduction and Regional Setting</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">Although the volcanic arc in the South American Andes is a major feature, the volcanic activity in the back&#45;arc is not so well developed. In the Quaternary Andean back&#45;arc in western Argentina, between 35&deg;S and 38&deg;S, an intense volcanism was developed, mostly of alkaline basalts, in the Payenia Basaltic Province (Polanski, 1954), or simply 'Payenia', also named Andino&#45;Cuyana Basaltic Province (Berm&uacute;dez and Delpino, 1989). Payenia is younger than 5 Ma, with an increase in the volcanic activity since 2 Ma, and it is the largest basaltic province of this age in the back&#45;arc of South America, covering an area of 15,900 km<sup>2</sup> (Berm&uacute;dez <i>et al.,</i> 1993; Folguera <i>et al.,</i> 2009; Llamb&iacute;as <i>et al,</i> 2010). This province is divided into two basaltic fields: the Llancanelo Volcanic Field in the north, with an area of 10,700 km<sup>2</sup>, and the Pay&uacute;n Matr&uacute; Volcanic Field in the south, which covers an area of 5,200 km<sup>2</sup> (Berm&uacute;dez and Delpino, 1989; Berm&uacute;dez <i>et</i> al., 1993) (<a href="#img01">Fig. 1</a>).</font></p>  	    ]]></body>
<body><![CDATA[<p align="center"><font size="2" face="Verdana"><a name="img01"></a>    <br> 	</font></p>  	<table width="60%" border="0" align="center">       <tr>         <td align="center"><font size="2" face="Verdana"><img src="/fbpe/img/andgeol/v39n1/fig08-01.jpg" width="609" height="425"></font></td>       </tr>       <tr>         <td align="center"><font size="2" face="Verdana">FIG. 1. Location of the Pay&uacute;n Matr&uacute; Volcanic Field and the Llancanelo Volcanic Field (LLVF) in the recent Andean back&#45;arc.</font></td>       </tr>     </table> 	    
<p align="justify"><font size="2" face="Verdana">Payenia contains around 800 monogenic basaltic cones, along with a few polygenic volcanoes such as Chachahu&eacute;n (upper Miocene), Nevado (Pliocene), Auca Mahuida (Pleistocene) and Pay&uacute;n Matr&uacute; (upper Pleistocene&#45;Holocene) (Inbar and Risso, 2001a; Llamb&iacute;as <i>et al.</i>, 2010). The volcanism in Payenia had two distinct episodes differentiated in age, composition and tectonic affinity (Kay <i>et al.,</i> 2006a). The first episode occurred during the late Miocene&#45;Pliocene and it is represented by Chachahu&eacute;n, Plateado and Nevado volcanoes, which have arc&#45;signatures (Kay <i>et al.,</i> 2004; Kay <i>et al.</i> 2006a). The second episode occurred in late Pliocene&#45;Quaternary times with an intraplate affinity and widespread basaltic volcanism in the Llancanelo Volcanic Field and the Pay&uacute;n Matr&uacute; Volcanic Field. In this episode, the Pay&uacute;n Matr&uacute;, Pay&uacute;n Liso and Auca Mahuida volcanoes were originated (Kay <i>et al.,</i> 2006a). In the late early Miocene to late Miocene, between 19 and 5 Ma, a period of flat&#45;slab subduction and a compressive regime, are inferred to have peaked in the late Miocene, between 8 and 5 Ma (Kay <i>et</i> al., 2006a; Galland <i>et al,</i> 2007). Evidence for this flat&#45;slab subduction period, among others, is the presence of Chachahu&eacute;n volcano, located as far as 500 km from the trench and exhibiting arc chemical signature <i>(e.g.,</i> high ratios of La/Ta and Ba/Ta, and low Ta/Hf, and Sr, Nd, Pb isotopic ratios) (Kay <i>et</i> <i>al.,</i> 2006b).</font></p>  	    <p align="justify"><font size="2" face="Verdana">A NW&#45;SE linear structural feature named Cortaderas lineament, located south of Tromen and Auca Mahuida volcanoes, divides the back&#45;arc in two volcanic regions (<a href="#img01">Fig. 1</a>): <b>1.</b> North of the lineament the back&#45;arc volcanism from Miocene to Holocene is widespread, and compressional deformation during late Miocene was important, and <b>2.</b> South of the lineament the back&#45;arc volcanism is nearly absent and the Miocene deformation is not significant (Ramos, 1978; Kay <i>et al.,</i> 2006a; Ramos and Kay, 2006; Ramos and Folguera, 2010). The Cortaderas lineament is assumed to be the southern limit of the Miocene flat slab (Kay <i>et al.,</i> 2006a). Llamb&iacute;as <i>et al.</i> (2010) proposed the Tromen&#45;Domuyo volcanic belt with the same NW orientation as the Cortaderas lineament, and with its southern limit coinciding with the Cortaderas lineament. This volcanic belt is 40 km wide and contains three Pleistocene volcanoes (Tilhue, Tromen and Domuyo) and the Palao mon&#45;zogranite of the same age (Llamb&iacute;as <i>et al.,</i> 2010). Auca Mahuida may belong to this volcanic belt, but further studies are needed to affirm or discard the idea (<a href="#img01">Fig. 1</a>).</font></p>  	    <p align="justify"><font size="2" face="Verdana">The widespread basaltic volcanism in Payenia is thought to be the result of the end of the Miocene flat&#45;slab subduction period and the start of a normal subduction zone, since 5 Ma until present times, which allowed an already hydrated mantle to melt (Kay <i>et</i> al., 2004; Kay <i>et al.,</i> 2006a). In this period, there was also a shift to an extensional regime in the back&#45;arc (Kay <i>et al.,</i> 2006a; Folguera <i>et al,</i> 2009; Berm&uacute;dez <i>et al.,</i> 1993). The Payenia basaltic lavas have mainly an intraplate signature, with no depletion in the HFSE typical of arc magmas (Kay <i>et al</i>., 2004; Kay, 2002), and it has been modeled as a result of 2&#45;8% of partial melting of an enriched mantle source (Kay, 2002). The volume of the Pliocene to Holocene magmatism in this region is difficult to explain based solely on a mantle 'wet spot' in a steep subduction zone, and it was postulated that the mantle has remained hot since Jurassic times, leading to the melting of the mantle by small perturbations (Kay <i>et al.,</i> 2006a).</font></p>  	    <p align="justify"><font size="2" face="Verdana">Previous studies of the Payenia Basaltic Province have been focused on the widespread basaltic volcanism, but little has been said about Pay&uacute;n Matr&uacute; volcano, in a more local scale. An important feature of the Pay&uacute;n Matr&uacute; Volcanic Field is the abundant basaltic volcanism surrounding the Pay&uacute;n Matr&uacute; caldera and the lack of basaltic lavas inside the caldera. The absence of basaltic lavas in the Pay&uacute;n Matr&uacute; volcano may be explained by the entrapment of the mafic magmas rising from deeper levels with the trachytic magmas located in the Pay&uacute;n Matr&uacute; magma chamber.</font></p>  	    <p align="justify"><font size="2" face="Verdana">The aim of this work is to present a detailed geological map, the volcanic stratigraphy and evolution of the Pay&uacute;n Matr&uacute; Volcanic Field, and to show evidence of magma mixing as is suggested by satellite images, and supported by petrography and geochemical and isotopic analysis of the different volcanic products of Pay&uacute;n Matr&uacute;.</font></p>  	    <p align="justify"><font size="3" face="Verdana"><b>2.&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Geology of the Pay&uacute;n Matr&uacute; Volcanic Field</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">Pay&uacute;n Matr&uacute; volcano (3,680 m) located in the center of the Pay&uacute;n Matr&uacute; Volcanic Field, stands 2,000 m above the surrounding plain and has a diameter of 15 km. It presents a summit caldera, which is defined in its northern and southeastern rim by a conspicuous scarp that reaches 450 m in height (<a href="#img02">Fig. 2</a>). The remaining caldera rim is defined by numerous domes and pumiceous cones distributed along the annular fractures of the caldera. The caldera was formed by collapse of a previously built volcanic edifice as a consequence of the only volumetrically important explosive eruption, which deposited ignimbrites radially from the caldera, leading to the caldera collapse. East and west of the Pay&uacute;n Matr&uacute; caldera, there are two basaltic fields with more than 200 scoria cones distributed in a wide E&#45;W oriented zone (<a href="#img03">Figs. 3a, b</a>). These basaltic centers were contemporaneous with the evolution of Pay&uacute;n Matr&uacute; volcano, and the eruptions of the older basalts were also contemporaneous with the Pay&uacute;n Liso volcano (Llamb&iacute;as, 1966; Germa <i>et al.,</i> 2010).</font></p> 	    <p align="center"><font size="2" face="Verdana"><a name="img02"></a>    ]]></body>
<body><![CDATA[<br> 	</font></p> 	<table width="60%" border="0" align="center">       <tr>         <td align="center"><font size="2" face="Verdana"><img src="/fbpe/img/andgeol/v39n1/fig08-02.jpg" width="652" height="271"></font></td>       </tr>       <tr>         <td align="center"><font size="2" face="Verdana">FIG. 2. Interior of the Pay&uacute;n Matr&uacute; showing the eastern inner caldera wall and the two largest post-caldera and intra-cardera.</font></td>       </tr>     </table> 	    
<p align="justify"><font size="2" face="Verdana">Pay&uacute;n Liso (3,715 m) is a typical cone&#45;shaped stratovolcano of Pleistocene age (Germa <i>et al.,</i> 2010) located southwest of Pay&uacute;n Matr&uacute;. The growth of this volcano occurred previously to the formation of Pay&uacute;n Matr&uacute; caldera (<a href="#img03">Fig. 3b</a>).</font></p> 	    <p align="center"><font size="2" face="Verdana"><a name="img03"></a>    <br> 	</font></p> 	<table width="60%" border="0" align="center">       <tr>         <td align="center"><font size="2" face="Verdana"><img src="/fbpe/img/andgeol/v39n1/fig08-03.jpg" width="655" height="572"></font></td>       </tr>       <tr>         <td><font size="2" face="Verdana">FIG. 3. <b>a.</b> LANDSAT 7 image of the Pay&uacute;n Matr&uacute; Volcanic Field, showing the Pay&uacute;n Matr&uacute; caldera, the eastern and western basaltic fields and the Pay&uacute;n Liso stratovolcano. The rectangle marks the limit of the map shown on figure 4; <b>b.</b> View from the west of the Pay&uacute;n Matr&uacute; and Pay&uacute;n Liso volcanoes showing their different morphologies, along with the western basaltic field. See the person for scale inside the circle.</font></td>       </tr>     </table> 	    
<p align="justify"><font size="2" face="Verdana">The stratigraphy of the Pay&uacute;n Matr&uacute; Volcanic Field was first outlined by Llamb&iacute;as (1966), who postulated a lower Quaternary stage, comprising three volcanic units, and an upper Quaternary stage with four units. The three lower Quaternary units are: <b>1.</b> La Nariz Andesites and Trachyandesites; <b>2.</b> Morados Grandes Basalts; <b>3.</b> El Portezuelo Tuff, further divided in two subunits according to the degree of welding. This unit was later named El Portezuelo Formation (Gonz&aacute;lez D&iacute;az, 1972), and it represents the only important explosive eruption. The four upper Quaternary units are: <b>1.</b> El Mollar Basalts; <b>2.</b> La Calle Trachytes; <b>3.</b> La Explanada Hyalotrachytes, further divided in lavas and pyro&#45;clastic deposits; and finally <b>4.</b> Media Luna Basalts, divided in a lower flow and an upper flow. The age of the Portezuelo Ignimbrite was first proposed to be upper Pleistocene&#45;Holocene (Llamb&iacute;as, 1966; Gonz&aacute;lez Diaz, 1970), and later constrained to upper Pleistocene by <sup>40</sup>Ar/<sup>39</sup>Ar datings of pre&#45; and post&#45;caldera lavas (Germa <i>et al.,</i> 2010).</font></p>  	    <p align="justify"><font size="2" face="Verdana">The Llamb&iacute;as (1966) stratigraphic scheme is updated in the present work. We suggest not to use the stratigraphic names given by Llamb&iacute;as (1966) but the new ones proposed in the present work.</font></p>  	    <p align="justify"><font size="3" face="Verdana"><b>3.&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Materials and methods</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">Detailed field work was carried out in order to perform the geologic mapping at 1:50.000 scale, on the basis of Llamb&iacute;as (1966), and using LANDSAT 7 satellite images from the NASA website and aerial photographs. The storage of geologic information and mapping was made in GIS software. Over 200 samples were collected for petrography and 30 representative samples of different volcanic units were selected for geochemical analysis of major elements, and 9 samples were selected for <sup>87</sup>Sr/<sup>86</sup>Sr isotopic ratio.</font></p>  	    <p align="justify"><font size="2" face="Verdana">The whole rock geochemical analyses were performed at Activation Laboratories LTD, Ontario, Canada, by lithium metaborate/tetraborate fusion ICP (major and minor oxides).</font></p>  	    <p align="justify"><font size="2" face="Verdana">One out of two selected ignimbrites belongs to fiamme fragments (sample PMB 4), representing directly the juvenile composition (sample PM 14), and the other represents the bulk rock composition, which has a low content of lithic fragments (&lt;2%).</font></p>  	    ]]></body>
<body><![CDATA[<p align="justify"><font size="2" face="Verdana">The whole rock samples preparation (crushing, milling) was performed at the Centro de Investigaciones Geol&oacute;gicas (Universidad Nacional de La Plata). Powdered whole rock samples for Strontium isotope analysis were treated at clean Rb&#45;Sr Laboratory of the same institution with HNO<sub>3</sub>&#45;HF, and natural Sr separated through resin columns following the technique described by Varela <i>et al.</i> (2000).</font></p>  	    <p align="justify"><font size="2" face="Verdana">XRF determinations for Rb and Sr contents as well as mass spectrometry were performed at Centro de Pesquisas Geocronologicas (CPGeo), Universidad de S&atilde;o Paulo, Brazil. The mass spectrometry was performed in the 'Thermal Ionization Mass Spectrometer' (TIMS) model MAT262&#45;multicollector&#45;Finnigan Mat. The normalization value is <sup>87</sup>Sr/<sup>86</sup>Sr=0.1194 and analytical error is quoted as 2&#963;. Other analytical conditions were NBS 987 standard value to <sup>87</sup>Sr/<sup>86</sup>Sr ra&#45;tio=0.710250&plusmn;0.000008 (mean value), and the spike utilized to Isotopic Dilution (if Sr is low concentration) was spike <sup>84</sup>Sr.</font></p>  	    <p align="justify"><font size="3" face="Verdana"><b>4. &nbsp;&nbsp;&nbsp;&nbsp;Results</b></font></p>  	    <p align="justify"><font size="2" face="Verdana"><b>4.1. &nbsp;&nbsp;&nbsp;Volcanic stratigraphy</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">Volcanic units were defined based on their occurrence either in polygenic volcanoes or in monogenic cones, their morphology, eruptive style and composition of magmas. In this way, basalts belonging to the eastern and western basaltic fields are separated from Pay&uacute;n Matr&uacute; and Pay&uacute;n Liso volcanoes. As the Portezuelo Ignimbrite is the only deposit of its kind in the Pay&uacute;n Matr&uacute; Volcanic Field, and marks an important event in the evolution of Pay&uacute;n Matr&uacute;, it is defined as a single unit. It also serves as a reference horizon due to its widespread areal distribution. An important discrimination criterion for both the composite volcanoes and the basaltic fields is the stratigraphic position of the different units with respect to the Portezuelo Ignimbrite. All volcanic units are grouped in a pre&#45;, syn&#45;, and a post&#45;caldera stage. The basaltic fields were divided into three units, named Pre&#45;caldera Basalts, Post&#45;caldera Basalts I and Post&#45;caldera Basalts II. The Pay&uacute;n Matr&uacute; volcano was divided into four units: Pre&#45;caldera Trachytes, Portezuelo Ignimbrite, Post&#45;caldera Trachyandesites, and finally Post&#45;caldera Trachytes. The Post&#45;caldera Trachytes unit was further divided into three litho&#45;facies, according to their different morphologies and effusive or explosive eruption styles. These three lithofacies were named Blocky Trachytes, Pumice cones and Vitreous Trachytes. The Pay&uacute;n Liso volcano was grouped in a single unit since it is not the object of the present study. The correspondence between the stratigraphy by Llamb&iacute;as (1966) and the new stratigraphy proposed in this work is shown in <a href="#img04">figure 4</a>. The Post&#45;caldera Trachyandesites unit corresponds to some, but not all, of the lava flows present in the caldera region previously grouped in the El Mollar Basalts unit (Llamb&iacute;as, 1966). The Post&#45;caldera Basalts I unit corresponds to lava flows of El Mollar Basalts which were not included in Post&#45;caldera Trachyandesites unit, and also to the lower flows of Media Luna Basalts.</font></p> 	    <p align="center"><font size="2" face="Verdana"><a name="img04"></a>    <br> 	</font></p> 	<table width="45%" border="0" align="center">       <tr>         <td align="center"><font size="2" face="Verdana"><img src="/fbpe/img/andgeol/v39n1/fig08-04.jpg" width="530" height="308"></font></td>       </tr>       <tr>         <td><font size="2" face="Verdana">FIG. 4. Diagram showing the correspondence between the Llamb&iacute;as (1966) stratigraphy and the one proposed in this work.</font></td>       </tr>     </table> 	    
<p align="justify"><font size="2" face="Verdana">The geological map of the Pay&uacute;n Matr&uacute; Volcanic Field is presented in <a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>, and a general stratigraphic scheme in <a href="#img06">figure 6</a>.</font></p> 	    
<p align="center"><font size="2" face="Verdana"><a name="img06"></a>    <br> 	</font></p> 	<table width="45%" border="0" align="center">       <tr>         <td align="center"><font size="2" face="Verdana"><img src="/fbpe/img/andgeol/v39n1/fig08-06.jpg" width="326" height="306"></font></td>       </tr>       <tr>         <td><font size="2" face="Verdana">FIG 6. Stratigraphic scheme for the Pay&uacute;n Matr&uacute; Volcanic Field that shows the contemporaneous volcanic activity of the basaltic fields and Pay&uacute;n Matr&uacute;. <sup>40</sup>Ar/<sup>39</sup>Ar ages from Germa <i>et al.</i> (2010).</font></td>       </tr>     </table> 	    
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<body><![CDATA[<p align="justify"><font size="2" face="Verdana"><b><i>4.1.1. Pay&uacute;n Matr&uacute;</i></b></font></p>  	    <p align="justify"><font size="2" face="Verdana"><b>4.1.1.1. Pre&#45;caldera stage</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">The Pre&#45;caldera Trachytes is the oldest unit of Pay&uacute;n Matr&uacute; volcano. It is composed mostly by lava flows and domes of trachytic compositions, with fewer trachybasalts and basaltic trachyandesites. Scarce radial dykes and volcaniclastic rocks of the same compositions are also present. This unit has outcrops in the exposed caldera wall and in the NE to SE outer slopes of the caldera (<a href="#img02">Figs. 2</a> and <a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">5</a>). The highest altitude of the caldera scarp is in its NE zone ('La Nariz'), with 450 m of exposed caldera wall (<a href="#img02">Fig. 2</a>). Trachytic lava outcrops are partially to almost completely covered by ignimbrites on the southern zone of Pay&uacute;n Matr&uacute;. This unit was considered to be Pleistocene by Llamb&iacute;as (1966), and was recently dated in 168&plusmn;4 ka by <sup>40</sup>Ar/<sup>39</sup>Ar in groundmass of trachytic lava (Germa <i>et al.,</i> 2010).</font></p>  	    
<p align="justify"><font size="2" face="Verdana"><b>4.1.1.2. Syn&#45;caldera stage</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">This stage is represented by the trachytic Portezuelo Ignimbrite, which is dispersed radially from the caldera up to a distance of about 40 km. There are no exposures of this unit inside the caldera due to the important and voluminous post&#45;caldera volcanism. The intra&#45;caldera ignimbrite, if present, is completely covered. The outcrops extend mostly north and south of the caldera rim, but they are partially covered by post&#45;caldera basaltic flows and scoria cones in the eastern basaltic field, and almost completely covered in the western basaltic field (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Figs. 5</a> and <a href="#img03">3b</a>). The ignimbrite is mostly massive, generally with a medium grade of welding except in some lower parts of its profile where it is highly welded. Its thickness varies widely, from less than 0.5 m to more than 20 m. Due to the discontinuity of the outcrops, the highly variable thickness, the fact that the base of the ignimbrite is not always exposed and the lack of subsurface information about the presence or absence of an intra&#45;caldera ignimbrite, its volume is hard to determine precisely but it is estimated to be around 30 km<sup>3</sup> (dense rock equivalent) (Llamb&iacute;as <i>et al.,</i> 2010). The widespread outcrops of the Portezuelo Ignimbrite in the region between Pay&uacute;n Liso and Pay&uacute;n Matr&uacute; volcanoes are eroded by the strong winds typical of this region, forming yardangs oriented NW&#45;SE, the main wind direction (Llamb&iacute;as, 1966; Inbar and Risso, 2001b). The <sup>40</sup>Ar/<sup>39</sup>Ar datings of pre&#45; and post&#45;caldera lavas constrain the age of this unit to upper Pleistocene, between 168 ka and 82 ka (Germa <i>et al.,</i> 2010).</font></p>  	    
<p align="justify"><font size="2" face="Verdana"><b>4.1.1.3. Post&#45;caldera stage</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">It is represented by two different units in terms of composition and morphology:</font></p>  	    <p align="justify"><font size="2" face="Verdana">&nbsp;&nbsp;&nbsp;&nbsp;<b>a. Post&#45;caldera Trachyandesites:</b> These are the first lavas erupted after the caldera collapse. They are basaltic trachyandesitic to trachyandesitic lava flows, representing a marked shift towards less evolved products with respect to the Portezuelo Ignimbrite. These lavas were erupted through the annular fractures of the caldera and flowed over the S and NW slopes of Pay&uacute;n Matr&uacute;, and also inside its caldera (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>). The lavas erupted in the southern caldera slope resemble pahoehoe flows, showing smooth surfaces, tumuli and ropy texture, while the only intra&#45;caldera lava flow has a blocky and hummocky surface with poorly developed lev&eacute;es, resembling <i>aa</i> lava morphology (<a href="#img02">Fig. 2</a>). Their lengths vary from those typical for blocky lavas (a few km) to those typical for <i>aa</i> basaltic lavas in the Pay&uacute;n Matr&uacute; Volcanic Field (up to 18 km in length). The intra&#45;caldera lava flow was dated in 82&plusmn;2 ka by <sup>40</sup>Ar/<sup>39</sup>Ar dating in groundmass (Germa <i>et al.,</i> 2010).</font></p>  	    
<p align="justify"><font size="2" face="Verdana">After the eruptions of these intermediate lavas of the Post&#45;caldera Trachyandesites unit, there was again an abrupt change in the composition of the emitted products, shifting to a more homogeneous trachytic composition. This latest stage of the post&#45;caldera stage is grouped in a single unit, Post&#45;caldera Trachytes, and further subdivided into three distinct lithofacies named above. The complexity of the stratigraphic relationship between these three lithofacies, along with the homogeneity of their compositions, was the reason for grouping them in a single unit. As an example, in the NW and SW rim of the caldera the Blocky Trachytes lavas are covered by Vitreous Trachytes lavas and Pumice cones deposits (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>), but the Blocky Trachytes intra&#45;caldera lava flow is younger than Pumice cones deposits. The pumice cones lithofacies are restrained between Blocky Trachytes and Vitreous Trachytes lavas, and the time span of the Vitreous Trachytes overlaps that of the Blocky Trachytes unit. The description of these three lithofacies is as follows:</font></p>  	    
<p align="justify"><font size="2" face="Verdana"><b>&nbsp;&nbsp;&nbsp;&nbsp;b.&nbsp;Blocky trachytes:</b> This lithofacies comprises the lava flows with a characteristic blocky morphology erupted through the caldera annular fissures and in the NW and SE flanks of Pay&uacute;n Matr&uacute;. They are up to 9 km in length and 250 m in thickness, a common range for this type of lava flows (<a href="#img02">Figs. 2</a> and <a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">5</a>). They possess strongly developed morphologic features of blocky lavas like lobes, lev&eacute;es and pressure ridges. Three <sup>40</sup>Ar/<sup>39</sup>Ar ages of these lavas range from 26&plusmn;2 ka (NW caldera slope flow) to 7&plusmn;1 ka (intra&#45;caldera flow) (Germa <i>et al.,</i> 2010). Some other flows which were erupted in the southern and northwestern rim of the caldera, partially covered by the <i>Pumice cones</i> and <i>Vitreous Trachytes</i> lithofacies, may be older.</font></p>  	    
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<body><![CDATA[<p align="justify"><font size="2" face="Verdana"><b>&nbsp;&nbsp;&nbsp;&nbsp;c.&nbsp;Pumiceous cones:</b> These cones are mound&#45;shaped deposits with circular to elongated bases, with a diameter/length of up to 1,300 m (<a href="#img07">Fig. 7a</a>), and which were erupted along the southeastern to the northern rim of the caldera (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>). These deposits are almost entirely composed of light gray to reddish trachytic pumice fragments, including minor contents of black glassy bombs with polygonal shapes, also of trachyte. The pumiceous cones constitute pyroclastic deposits with a very low to high degree of welding and a very poor selection, comprising glassy bombs of up to 1 m of diameter along with pumice clasts from milimetric to tens of centimeters in size. The deposits are clast supported and lack fine matrix, showing a diffuse coarse stratification. The pumice cones are closely related to the vitreous trachytes, in the sense that the vitreous black bombs are of the same composition and texture as the vitreous trachytes lithofacies, and that a few flows have a pumice layer on its base or flow from a pumice cone. On the NW inner rim of the caldera, sanidine from pumice fragments were dated in 37&plusmn;2 ka (Germa <i>et al</i>., 2010).</font></p>     
<p align="center"><a name="img07"></a> <table width="60%" border="0" align="center">       <tr>         <td width="47%" align="center" valign="bottom"><font size="2" face="Verdana"><img src="/fbpe/img/andgeol/v39n1/fig08-07.jpg" width="312" height="431"></font></td>         <td width="6%" valign="bottom">&nbsp;</td>         <td valign="bottom"><font size="2" face="Verdana">FIG. 7. <b>a.</b> Two pumiceous cones in the western caldera rim. See the person inside the circles for scale; <b>b.</b> View of a lava of the <i>Vitreous Trachyte</i> lithofacies in the northern caldera rim.</font></td>       </tr>     </table> 	    
<p align="justify"><font size="2" face="Verdana"><b>&nbsp;&nbsp;&nbsp;&nbsp;d.&nbsp;Vitreous trachytes:</b> This lithofacies is represented by a number of small domes and coul&eacute;es, with fewer but longer lava flows (<a href="#img07">Fig. 7b</a>). They are mostly distributed along the southern and western rim of the caldera, with few representatives in the western lower flank of Pay&uacute;n Matr&uacute; (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>). The domes are circular in plain view, ranging from 150 m to 1,000 m in diameter, and the lava flows are shorter than that of the Blocky Trachytes lithofacies, reaching 3.5 km in length. Pressure ridges are conspicuous and are more closely spaced than in the blocky lavas of Blocky Trachytes lithofacies (<a href="#img07">Fig. 7b</a>). There are no ages available for this lithofacies.</font></p>  	    
<p align="justify"><font size="2" face="Verdana"><b><i>4.1.2. Pay&uacute;n Liso</i></b></font></p>  	    <p align="justify"><font size="2" face="Verdana">Pay&uacute;n Liso stratovolcano (<a href="#img03">Figs. 3 a, 3b</a> and <a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">5</a>) belongs to the pre&#45;caldera stage. It is contemporaneous or slightly older than the early eruptions of Pay&uacute;n Matr&uacute;, as indicated by the partial cover of its northern slope by the Portezuelo ignimbrite and also by four <sup>40</sup>Ar/<sup>39</sup>Ar dates in groundmass of lavas, ranging between 261&plusmn;4 ka and 285&plusmn;5 ka (Germa <i>et</i> al., 2010). The Pay&uacute;n Liso volcano mostly comprises lavas with minor pyroclastic rocks. The lavas are trachytic to trachyandesitic, similar to that of the pre&#45;caldera stage of Pay&uacute;n Matr&uacute;. On its N and NE flank, the Portezuelo Ignimbrite reaches an altitude of nearly 300 m above the base of Pay&uacute;n Liso volcano. Pay&uacute;n Liso has a volume estimated in 40 km<sup>3</sup> (Germa <i>et al.,</i> 2010), and its morphology is different from that of Pay&uacute;n Matr&uacute;, with a clearly defined central vent and steeper slopes, as for a typical stratovolcano.</font></p>  	    
<p align="justify"><font size="2" face="Verdana"><b><i>4.1.3. Basaltic fields</i></b></font></p>  	    <p align="justify"><font size="2" face="Verdana">The numerous basaltic eruptions in the eastern and western basaltic fields were contemporaneous with the Pay&uacute;n Matr&uacute; volcano, as proposed by Llamb&iacute;as (1966), and later corroborated by <sup>40</sup>Ar/<sup>39</sup>Ar ages in pre&#45; to post&#45;caldera basaltic lavas, which range from 233&plusmn;11 ka to &lt;7 ka (Germa <i>et al,</i> 2010).</font></p>  	    <p align="justify"><font size="2" face="Verdana">These basaltic fields are separated by the Pay&uacute;n Matr&uacute; caldera, with almost no eruptions south and north of the caldera region. The lavas are alkaline basalts and trachybasalts, with a tendency of the younger Post&#45;caldera Basalts II unit to be tra&#45;chybasalts and the older Pre&#45;caldera Basalts unit to be basalts, with the Post&#45;caldera Basalts I in between the two, suggesting a continuous trend. The two post&#45;caldera basaltic units are separated on the basis of their stratigraphic position (Postcaldera Basalts II cover the lavas of Post&#45;caldera basalts I), on their degree of preservation and on the sedimentary and/or vegetal cover of the lavas and scoria cones. The surface morphology of the younger Post&#45;caldera basalts II flows is aa in all cases, with rugged surfaces and a principal central lava channel surrounded by wide 'lev&eacute;es'. The flows reach lengths up to 21 km. The scoria cones associated with these flows have frequently abundant bombs in an <i>in situ</i> position, with aerodynamical or irregular shapes. Morphological studies in scoria cones belonging to this unit indicate that they are Holocene (Inbar and Risso, 2001a), as does an <sup>40</sup>Ar/<sup>39</sup>Ar date in basalt groundmass of &lt;7 ka (Germa <i>et al.,</i> 2010). Older basalts of Post&#45;caldera Basalts I and Pre&#45;caldera Basalts units are mostly compound flows with pahoehoe morphology, showing smooth surfaces and the development of tumuli and lava tubes in a few cases. In the eastern region of the eastern basaltic field, there is a pahoehoe lava flow named 'Pampas Onduladas' (only its proximal area is visible in <a href="#img03">Fig. 3 a</a>, outside the inset, near the NE corner of the image), which has a total length of 181 km and is considered the longest Quaternary lava flow on Earth (Pasquar&egrave; <i>et al.,</i> 2008). In both western and eastern basaltic fields there are pre&#45; and post&#45;caldera basalts, but there is a marked contrast in their relative abundances to either side of the caldera region. In the eastern field the outcrops of pre&#45;caldera basalts are widespread, especially north of the Carbonilla Fault, were no basalts were erupted in the post&#45;caldera stage (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>). The younger basalts of Post&#45;caldera Basalts II unit are mostly distributed on the western side of Pay&uacute;n Matr&uacute; caldera, in 'Los Volcanes' region, where the basaltic flows are still not covered by vegetation and a blanket of lapillitic scoria covers older flows (<a href="#img03">Figs. 3b</a> and <a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">5</a>). Very few outcrops of basaltic scoria cones and lava flows of the pre&#45;caldera stage are still visible in this region (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>).</font></p>  	    
<p align="justify"><font size="2" face="Verdana"><b>4.2.&nbsp;&nbsp;&nbsp;Structural controls on volcanism</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">Fractures clearly control the location of the eruptions of both the basaltic lava fields and the more silicic rocks of Pay&uacute;n Matr&uacute;. In first place, there are fisural eruptions with E&#45;W and NW&#45;SE orientations in the basaltic fields and distributed over a relatively wide area (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>). In second place, there are more local annular structures related to the caldera collapse and located in the caldera region. The eruption of basaltic lavas occurred along linear fissures, as seen in La Carbonilla Fault (<a href="#img03">Figs. 3a</a> and <a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">5</a>) with fissure ridges and a scoria cone aligned in E&#45;W direction (<a href="#img08">Fig. 8</a>). Outside the zone of La Carbonilla Fault, vent alignments are not so obvious but seem to follow the same orientation (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>). In the western basaltic field, vent alignments marked by few scoria cones and fissure ridges in NW directions are common and noticeable, with minor E&#45;W vent alignments (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>). Not only are the basaltic vents aligned in NW directions, but also there is one marked alignment of pumice cones and lava flows of Vitreous Trachytes lithofacies on the western slope of the caldera with the same orientation (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>). This alignment has the same orientation as the scoria cones near them, and it shows that the younger units of Pay&uacute;n Matr&uacute; are not only controlled by the annular fractures of the caldera collapse but they are also controlled, at least in this region, by the same type of fractures that control the basaltic volcanism.</font></p> 	    
]]></body>
<body><![CDATA[<p align="center"><font size="2" face="Verdana"><a name="img08"></a>    <br> 	</font></p> 	<table width="55%" border="0" align="center">       <tr>         <td align="center"><font size="2" face="Verdana"><img src="/fbpe/img/andgeol/v39n1/fig08-08.jpg" width="542" height="234"></font></td>       </tr>       <tr>         <td><font size="2" face="Verdana">FIG. 8. Photo of a basaltic fissure eruption along La Carbonilla fault in the eastern basaltic field, showing the main scoria cone and small fissure ridges aligned in a E&#45;W orientation. See the person inside the circle for scale.</font></td>       </tr>     </table> 	    
<p align="justify"><font size="2" face="Verdana">The caldera structure is clearly visible along the north to the southeast rim, where there is a scarp of less than 10 m (northern rim) to 450 m (eastern rim) (<a href="#img02">Figs. 2</a> and <a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">5</a>). No post&#45;caldera eruptions along this zone of the caldera rim were emitted. The remaining rim of the caldera is not so clearly defined; it is indicated by a wide annular zone where numerous post&#45;caldera eruptions took place. The distribution of the trachytic vents of lava flows, 'coul&eacute;es', domes and pumiceous cones shows that there are annular fractures and that the caldera rim is wider in this zone. A few lava flows erupted relatively far from the caldera rim, on its southeast and northwest slopes (<a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">Fig. 5</a>).</font></p>  	    
<p align="justify"><font size="2" face="Verdana"><b>4.3.&nbsp;&nbsp;&nbsp;Petrography</b></font></p>  	    <p align="justify"><font size="2" face="Verdana"><b><i>4.3.1. Pre&#45;caldera stage</i></b></font></p>  	    <p align="justify"><font size="2" face="Verdana">&nbsp;&nbsp;&nbsp;&nbsp;<b>a. Pre&#45;caldera trachytes unit:</b> The petrography of this unit is not simple and uniform. They present in most cases a variety of disequilibrium textures and, in a few cases, inclusions of more mafic magmas. The rocks are all porphyritic with plagioclase that predominates over sanidine. Clinopyroxene is always present and predominates over olivine, biotite and amphibole in this order of abundance. Biotite and amphibole are not always present and apatite is a common accessory phase. Sanidine phenocrysts (12&#45;20%) are clean and euhedral, up to 4 mm in size. Plagioclase crystals (8&#45;20%) have textures that vary widely, even in the same sample. Commonly, there are euhedral and clean crystals along with more anhedral crystals which show either dusty o coarse sieved zones (<a href="#img09">Fig. 9a</a>). Clinopyroxene (up to 3%) is subhedral to euhedral, and up to 2 mm in size. It is sometimes rounded, and the occurrence of rounded and non&#45;rounded phenocrysts in the same sample is common. Olivine phenocrysts (1&#45;3%) are subhedral up to 1 mm in size, generally less than 0.5 mm. They are rounded and present a slight alteration to iddingsite. Biotite (up to 2%) is subhedral, up to 1 mm in size and it shows a reaction rim with anhydrous minerals that in some cases replaces the whole crystal (<a href="#img09">Fig. 9b</a>). The amphibole (2%) is generally anhedral, up to 1 mm in size and it displays a medium brown to a darker reddish brown pleocroism. It always exhibits an opaque rim (<a href="#img09">Fig. 9c</a>). Blobs of a different magma without quench textures and showing a fluid&#45;fluid relationship with the host magma are present in a few trachytic and trachyandesitic samples (<a href="#img09">Fig. 9d</a>). These same samples also have phenocrysts with disequilibrium textures, like sieved and un&#45;sieved plagioclase phenocrysts and biotite with reaction rims.</font></p> 	    <p align="center"><font size="2" face="Verdana"><a name="img09"></a>    <br> 	</font></p> 	<table width="55%" border="0" align="center">       <tr>         <td align="center"><font size="2" face="Verdana"><img src="/fbpe/img/andgeol/v39n1/fig08-09.jpg" width="493" height="251"></font></td>       </tr>       <tr>         <td><font size="2" face="Verdana">FIG. 9. Microphotographs of Pre&#45;caldera Trachytes (a&#45;d) and the Portezuelo Ignimbrite (e&#45;f). <b>a.</b> Two plagioclase phenocrysts in a trachyte lava with different textures: one clean, euhedral and showing slightly rounded corners, and the other rounded with a coarse sieve texture; <b>b.</b> Biotite phenocrysts partially replaced by an anhydrous mineral association; <b>c.</b> Glomerocryst of am&#45;phibole with an opaque rim; <b>d.</b> Two different groundmasses showing a fluid&#45;fluid relationship, indicating magma mingling processes; <b>e.</b> Sieved plagioclase crystals in the Portezuelo Ignimbrite with a high grade of welding, along with a few olivine crystals; <b>f.</b> Biotite, clinopyroxene and sanidine crystals in the same ignimbrite. Biotite is euhedral and shows no replacement textures.</font></td>       </tr>     </table> 	    
<p align="justify"><font size="2" face="Verdana"><b><i>4.3.2. Syn&#45;caldera stage</i></b></font></p>  	    <p align="justify"><font size="2" face="Verdana">&nbsp;&nbsp;&nbsp;&nbsp;<b>a. Portezuelo Ignimbrite unit:</b> The ignimbrite is ash&#45;rich, with abundant crystals of sanidine and plagioclase, with minor contents of olivine, clino&#45;pyroxene, biotite and opaque minerals, and apatite as an accessory mineral. The feldspars (up to 25%) are seriate up to 2 mm in size. They are generally clean except for minor amounts of subhedral and anhedral sieved crystals, with a sieved texture that is slightly coarser than dusty zones (<a href="#img09">Fig. 9e</a>). Fragmented crystals and glomerocrysts are common. Olivine and clinopyroxene have similar low abundances, 1 to 2%. They are euhedral to subhedral and fresh, less than 1 mm in size. Biotite (1%) shows no signs of reaction with the melt (<a href="#img09">Fig. 9f</a>). Pummice fragments range in degree of compaction from those with globular shapes and highly vesicular to fiamme with lenticular shapes (<a href="#img09">Figs. 9e and 9f</a>). Their sizes can vary widely, from millimeter to 1 meter long in fiamme present in the lower part of the north scarp of the caldera rim profile. Basaltic to trachytic lithic fragments are generally scarce, up to a few tens of centimeters in size.</font></p>  	    ]]></body>
<body><![CDATA[<p align="justify"><font size="2" face="Verdana"><b><i>4.3.3. Post&#45;caldera stage</i></b></font></p>  	    <p align="justify"><font size="2" face="Verdana">&nbsp;&nbsp;&nbsp;&nbsp;<b>a. Post&#45;caldera trachyandesites unit:</b> This unit is by far the most variable among the post&#45;caldera rocks, both in composition and in mineralogical textures. All lava flows possess disequilibrium textures, especially in plagioclase phenocrysts. They are porphyritic, with plagioclase as the most abundant phase, plus olivine and clinopyroxene. Apatite is also a common accessory mineral. The groundmass is intergranular and more rarely pilotaxitic. Plagioclase phenocrysts are abundant (15&#45;22%) and seriated, up to 4 mm in size. Dusty zones in euhedral plagioclase phenocrysts are widespread and they are distributed in several ways, most commonly in the core of the crystal with clear overgrowths, or in a rim leaving a clear core. Euhedral and clear crystals are also common, and sieved and clear crystals may occur side by side in the same sample (<a href="#img10">Fig. 10a</a>). Coarse sieved textures with groundmass inclusions of up to a few tens of micrometers or, more rarely, a few hundred micrometers in size occur in some euhedral plagioclases, distributed in cores or rims, and can be present along dusty zones in the same crystals (<a href="#img10">Fig. 10b</a>). Olivine (up to 5%) is subhedral, seriated up to 1 mm in size, and it presents, in some cases, rounded corners and an incipient alteration to iddingsite. Clinopyroxene (up to 5%) is subhedral, with rounded and non&#45;rounded corners present in the same sample, up to 1.5 mm in size. The intra&#45;caldera lava flow possesses evidence of mingling involving two melts of different compositions, with few pockets of trachytic magma immersed in less evolved basaltic trachyandesitic lava, which constitutes the vast majority of the flow. Although these two melts have the same mineralogical association, they have different textures in groundmass and plagioclase phenocrysts (<a href="#img10">Figs. 10a, c, d</a>). Plagioclases in the trachytic pockets are basically of two types: the most common one is subhedral with rounded corners and a marked zonation in the outer margin, and the other shares the same characteristics but it also has a coarse sieved texture. The plagioclase phenocrysts in the basaltic trachyandesitic portion are mainly euhedral, with clean and dusty or coarse sieved crystals coexisting in the same sample, and with minor anhedral, coarse sieved and dusty plagioclases (<a href="#img10">Figs. 10a, b</a>).</font></p>  	    <p align="center"><font size="2" face="Verdana"><a name="img10"></a>    <br> 	</font></p>  	<table width="55%" border="0" align="center">       <tr>         <td align="center"><font size="2" face="Verdana"><img src="/fbpe/img/andgeol/v39n1/fig08-10.jpg" width="491" height="248"></font></td>       </tr>       <tr>         <td><font size="2" face="Verdana">FIG. 10. Microphotographs of the intra&#45;caldera lava flow of the Post&#45;caldera Trachyandesites unit (a&#45;d), and lavas from the Blocky Trachytes lithofacies (e) and Vitreous Trachytes lithofacies (f) of the Post&#45;caldera Trachytes unit. <b>a.</b> Clean and euhedral plagioclase phenocryst, along with a euhedral and dusty crystal with a clear rim; <b>b.</b> Plagioclase phenocrysts showing a clear core with a dusty rim that also shows a coarse sieved texture with groundmass inclusions; <b>c.</b> Clean and euhedral plagioclase phenocrysts in a pilotaxitic groundmass. This sample belongs to the trachytic pockets immersed in the basaltic trachyan&#45;desitic intra&#45;caldera lava flow; <b>d.</b> Two melts of different composition and texture in the same lava flow, indicating mingling; <b>e.</b> Clean and euhedral sanidine phenocryst in a pilotaxitic groundmass, intra&#45;caldera trachytic lava flow; <b>f.</b> Vitrophyre with euhedral sanidine and clinopyroxene phenocrysts. Note a few glass inclusions in the sanidine crystal, which are controlled by cleavage directions.</font></td>       </tr>     </table> 	    
<p align="justify"><font size="2" face="Verdana">&nbsp;&nbsp;&nbsp;&nbsp;<b>b. Post&#45;caldera trachytes unit:</b> Although this unit shares many petrographic characteristics among its three lithofacies, they have also differences and they will be described separately:</font></p>  	    <p align="justify"><font size="2" face="Verdana"><i>Blocky Trachytes lithofacies:</i> These are light gray trachyte lavas, mainly composed of sanidine phenocrysts (8&#45;15%), clinopyroxene (2&#45;3%) and minor contents of biotite (1%), which is not always present. Olivine is scarce, and apatite occurs as an accessory mineral. Groundmass is holocrystalline, with pilotaxitic and/or trachytic texture. sanidine phenocrysts are seriate, up to 5 mm long, mainly clean and euhedral without signs of reaction with the melt (<a href="#img10">Fig. 10e</a>). The clinopyroxene is abundant, subhedral to euhedral and shows a narrow opaque rim. Biotite is of 1 mm in size and it is almost completely replaced by opaque minerals. Glomeroporphyritic texture with sanidine plus mafic minerals is common.</font></p>  	    <p align="justify"><font size="2" face="Verdana"><i>Vitreous Trachytes lithofacies:</i> They are composed of black porphyritic vitrophyres. They have abundant sanidine phenocrysts as the <i>T bq</i> litho&#45;facies, with clinopyroxene (2&#45;4%), lesser amounts of olivine (1&#45;2%), opaque minerals and in a few cases biotite (&lt;1%). Apatite is an accessory mineral. Glass is partially recrystallized in discontinuous bands of variable thickness, from millimeters to tens of centimeters. Sanidine phenocrysts are seriate up to 4 mm in size. They are always clean with euhedral shapes, some of them showing glass inclusions controlled by the cleavage directions and without rounding of the corners (<a href="#img10">Fig. 10f</a>). Sanidine micro&#45;lites with 'swallow tail' morphologies are frequent. Clinopyroxene is also seriate, ranging between 0.1 and 1.2 mm in size, euhedral and showing no signs of disequilibrium with the melt, such as rounded corners or mantles. Olivine is less abundant, 1 mm in size approximately and commonly with rounded corners and an incipient alteration to iddingsite. Biotite is scarce and not always present, seriated up to 1 mm long and sometimes replaced by opaque minerals. Glomeroporphyritic texture, with sanidine&plusmn;clinopyroxene and opaque minerals is common.</font></p>  	    <p align="justify"><font size="2" face="Verdana"><i>Pumice cones lithofacies:</i> The pumice fragments are light gray to reddish and porphyritic. The type and abundances of phenocrysts are identical to those of the <i>Tv</i> lithofacies described above. They differ from the <i>T v</i> lithofacies only in the degree of vesiculation and fragmentation of the lava, a result of the more explosive eruptions that formed these pyroclastic deposits.</font></p>  	    <p align="justify"><font size="2" face="Verdana"><b><i>4.3.4. Basalts from Pre&#45; and Post&#45;caldera units</i></b></font></p>  	    <p align="justify"><font size="2" face="Verdana">The three basaltic units are porphyritic or micro&#45;porphyritic, mainly composed of plagioclase and olivine, and generally with minor clinopyroxene and opaque minerals. There are exceptions to this general rule, with some basalts without plagioclase phenocrysts and some others without clinopyroxene; olivine is always present, both in the groundmass and as phenocrysts. These differences in the content of phenocrysts are not correlated with the chemical evolution of the basaltic units (discussed later), although there is a tendency in the younger Postcaldera Basalts II to have slightly higher phenocrysts content. The groundmass is intergranular with the same mineralogy, except that the amount of clino&#45;pyroxene is markedly lower and olivine is by far the most abundant mafic microlite, frequently showing skeletal morphologies. Plagioclase phenocrysts are mostly euhedral and clean, seriate up to 2.5 mm in length, present in low abundances, up to 5%. A few have skeletal morphologies in their outer rim, and some have sieved cores with a clear and zoned rim. Olivine phenocrysts (up to 5%) are fresh and seriated up to 2 mm in size and frequently showing skeletal morphologies. Clinopyroxene is euhedral, up to 3% and 1 mm in size, and in some cases it can have markedly rounded corners.</font></p>  	    ]]></body>
<body><![CDATA[<p align="justify"><font size="2" face="Verdana"><a href="#t1">Table 1</a> illustrates the principal petrographic characteristics of the volcanic units described above.</font></p>  	    <p align="center"><font size="2" face="Verdana"><a name="t1"></a>    <br> 	    <img src="/fbpe/img/andgeol/v39n1/tb08-01.jpg" width="651" height="509"></font></p>  	    
<p align="justify"><font size="2" face="Verdana"><b>4.4. &nbsp;&nbsp;&nbsp;Whole rock major elements geochemistry</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">Pay&uacute;n Matr&uacute; Volcanic Field rocks belong to the alkaline series, ranging from basalts to trachytes (Hernando <i>et al.,</i> 2011). The lavas of the basaltic fields have basaltic to trachybasaltic compositions (46.5&#45;49.1% SiO<sub>2</sub> on an anhydrous basis) and the rocks of Pay&uacute;n Matr&uacute; and Pay&uacute;n Liso volcanoes have basaltic trachyandesitic to trachytic compositions (51.8&#45;68.2% SiO<sub>2</sub>). They define a linear trend in the TAS classification diagram, with a small gap of 2.7% SiO<sub>2</sub> separating both groups of rocks (<a href="#img11">Fig. 11</a>). The younger basalts of Postcaldera Basalts II unit are all trachybasalts, while Post&#45;caldera Basalts I and Pre&#45;caldera Basalts units are both basalts and trachybasalts. The older unit of Pay&uacute;n Matr&uacute;, Pre&#45;caldera Trachytes, has a wide range in composition compared to the younger trachytes of Post&#45;caldera Trachytes unit, although it is mainly composed of trachytes. The most silicic pre&#45;caldera lavas are porphyritic with clean sanidine phenocrysts, while in the other pre&#45;caldera lavas plagioclase predominates over sanidine, and sieved phenocrysts are common. In both cases, the clinopyroxene and olivine is also present. The Portezuelo Ignimbrite is also trachytic (64.6&#45;65.2% SiO<sub>2</sub>), but with the eruption of the first post&#45;caldera lavas, represented by the Post&#45;caldera Trachyandesites unit, there is a marked shift to intermediate compositions (52.7&#45;60% SiO<sub>2</sub>). The post&#45;caldera trachyandesitic intra&#45;caldera lava flow possesses two different compositions (samples PM 13 with 60.08 SiO<sub>2</sub>%, and PM 34 with 54.43 SiO<sub>2</sub>%, see <a href="/fbpe/img/andgeol/v39n1/t08-02.html" target="_blank">Table 2</a>). The vast majority of the flow is a basaltic trachyandesite and, in addition, it contains minor pockets of trachytic compositions which are discerned in the field just by a slight change in color. The most evolved rocks are those of Blocky Trachytes and Vitreous Trachytes litho&#45;facies belonging to the Post&#45;caldera Trachytes unit, along with very few representatives of pre&#45;caldera trachytes. The tendency of the alkaline series is towards the rhyolite or phonolite fields, and in the particular case of the Pay&uacute;n Matr&uacute; Volcanic Field, the trachytes contain up to 14% of normative quartz and the most silicic ones plot close to the rhyolite field in the TAS diagram, suggesting that the evolution is towards more silicic compositions rather than to more alkaline products. Basaltic and trachybasaltic lavas from the basaltic fields are olivine and nepheline normative (6.6&#45;10.1% and 0.6&#45;4.2%, respectively, see <a href="/fbpe/img/andgeol/v39n1/t08-02.html" target="_blank">Table 1</a>), as expected for alkaline basalts. Stern <i>et al.</i> (1990) reported the chemistry and <sup>s7</sup>Sry<sup>86</sup>Sr isotopic ratio of a basalt from 'Los Volcanes', having similar values as the analysis reported in the present work.</font></p> 	    
<p align="center"><font size="2" face="Verdana"><a name="img11"></a>    <br> 	</font></p> 	<table width="55%" border="0" align="center">       <tr>         <td align="center"><font size="2" face="Verdana"><img src="/fbpe/img/andgeol/v39n1/fig08-11.jpg" width="482" height="343"></font></td>       </tr>       <tr>         <td><font size="2" face="Verdana">FIG. 11. TAS classification diagram for volcanic rock ( Le Maitre <em>et al.</em>, 1989). Line separating the alkaline and subalkaline series according to Irving and Baragar (1971).</font></td>       </tr>     </table> 	    
<p align="justify"><font size="2" face="Verdana"><a href="#img12">Figure 12</a> shows variation diagrams for major elements, where the samples define linear trends. K<sub>2</sub>O and Na<sub>2</sub>O have positive correlations with SiO<sub>2</sub> while MgO, Fe<sub>2</sub>O<sub>3</sub> (T), CaO and TiO<sub>2</sub> (not shown) have negative correlations. Al<sub>2</sub>O<sub>3</sub> is relatively constant with the increment of SiO<sub>2</sub> content in basic and intermediate compositions, decreasing in the more silicic rocks (around 66% SiO<sub>2</sub>) belonging to the Blocky Trachytes and Vitreous Trachytes lithofacies, and in a few Pre&#45;caldera Trachytic lavas.</font></p> 	    <p align="center"><font size="2" face="Verdana"><a name="img12"></a>    <br> 	</font></p> 	<table width="55%" border="0" align="center">       <tr>         <td align="center"><font size="2" face="Verdana"><img src="/fbpe/img/andgeol/v39n1/fig08-12.jpg" width="521" height="399"></font></td>       </tr>       <tr>         <td><font size="2" face="Verdana">FIG. 12. Harker diagrams for major elements, showing a linear and continuous trend. See<a href="#img11"> figure 11</a> for references.</font></td>       </tr>     </table> 	    
]]></body>
<body><![CDATA[<p align="justify"><font size="2" face="Verdana">The analysis of the <sup>87</sup>Sr/<sup>86</sup>Sr isotopic ratio in the 9 samples indicates a narrow range in their values, between 0.703766 and 0.704288 (<a href="/fbpe/img/andgeol/v39n1/t08-02.html" target="_blank">Table 2</a>). These values correspond to both the basaltic lavas (Pre&#45;caldera Basalts and Post&#45;caldera Basalts II units) of the basaltic fields, and to the basaltic trachyandesitic to trachytic lavas (Pre&#45;caldera Trachytes, Post&#45;caldera Trachyandesites and Post&#45;caldera Trachytes units) of the Pay&uacute;n Matr&uacute; volcano (see <a href="/fbpe/img/andgeol/v39n1/t08-02.html" target="_blank">Table 2</a>). The <sup>87</sup>Sr/<sup>86</sup>Sr isotopic ratio indicates that the magmas were originated in the mantle, as previously proposed for the basaltic lavas of Payenia (Kay <i>et al</i>., 2004).</font></p>  	    
<p align="justify"><font size="3" face="Verdana"><b>5. &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Discussion</b></font></p>  	    <p align="justify"><font size="2" face="Verdana"><b>5.1. &nbsp;&nbsp;&nbsp;Volcanic stratigraphy</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">The volcanic stratigraphy of the Pay&uacute;n Matr&uacute; Volcanic Field was modified from Llamb&iacute;as (1966) on the basis of new field, petrographic and geochemical information. The Portezuelo Ignimbrite lead to the separation in a pre&#45;, syn&#45;, and post&#45;caldera stages (<a href="#img06">Fig. 6</a>). In the pre&#45;caldera stage, basaltic eruptions took place in the eastern and western basaltic field and basaltic trachyandesitic to trachytic magmas formed the pre&#45;caldera Pay&uacute;n Matr&uacute; edifice, along with the neighboring Pay&uacute;n Liso stratovolcano. The syn&#45;caldera stage is represented by the Portezuelo Ignimbrite and the formation of the 8 km wide caldera. The post&#45;caldera stage continued in Pay&uacute;n Matr&uacute;, the basaltic fields (mostly in the western field), and not at all in Pay&uacute;n Liso. The Post&#45;caldera Trachy&#45;andesites were grouped originally along with some of the Post&#45;caldera Basalts I lavas (Llamb&iacute;as, 1966). We postulate the definition of a new unit &#45;Post&#45;caldera Trachyandesites&#45; due to their different composition and their belonging to the Pay&uacute;n Matr&uacute; volcano. The remaining post&#45;caldera rocks (Post&#45;caldera Trachytes unit, with its three lithofacies&#45; Blocky Trachytes, Pumice cones and Vitreous Trachytes) are defined similarly as in Llamb&iacute;as (1966), but we grouped them in a different way due to their homogeneous trachytic compositions and their complex stratigraphic relationships (<a href="#img06">Fig. 6</a>). The post&#45;caldera basaltic lavas and scoria cones from the eastern and western basaltic fields were also grouped differently than the corresponding ones from Llamb&iacute;as (1966), according to the geological map presented and the contemporaneity of the basaltic fisural eruptions with the eruptions in the Pay&uacute;n Matr&uacute; volcano.</font></p>  	    <p align="justify"><font size="2" face="Verdana"><b>5.2. &nbsp;&nbsp;&nbsp;Evidence of magma mixing and mingling</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">In the Pay&uacute;n Matr&uacute; Volcanic Field there are several lines of evidence for magma mixing and/ or mingling, at different scales. For instance, the numerous E&#45;W and NW&#45;SE fisural basaltic eruptions are interrupted by the presence of a trachytic Pay&uacute;n Matr&uacute; composite volcano (<a href="#img03">Figs. 3a</a> and <a href="/fbpe/img/andgeol/v39n1/img08-05.html" target="_blank">5</a>). The absence of basaltic lavas in the caldera region suggests that the basaltic magmas were unable to reach the surface, most probably due to the presence of a magmatic chamber below the Pay&uacute;n Matr&uacute; caldera. This chamber would have acted as a barrier for the basaltic lavas rising from deeper levels if the chamber had been sufficiently melted, a likely condition as proved by the contemporaneity of both types of volcanism.</font></p>  	    
<p align="justify"><font size="2" face="Verdana">On the other hand, the petrographic study of the different units allowed us to discern several disequilibrium textures, the majority of which are attributed to magma mixing. According to experimental studies, the dusty zones in plagioclase phenocrysts are formed by partial dissolution of a plagioclase which is more sodic than the one that would be in equilibrium with the melt (Tsuchiyama, 1985). The conservation of the euhedral shape means that the crystal was below the liquidus curve for the plagioclase, and the rounding of crystals occurs if they were above the liquidus curve (Tsuchiyama, 1985).</font></p>  	    <p align="justify"><font size="2" face="Verdana">A sieve texture in plagioclase, coarser than dusty zones but not as coarse as the coarse sieve texture, has been reproduced in hydrous experiments (Nakamura and Shimakita, 1998). This texture was interpreted as a partial dissolution of the plagioclase crystals, as in the anhydrous experiments carried out by Tsuchiyama (1985). The proposed scenario for this coarse sieved dissolution texture is magma mixing and frequently sieved and unsieved phenocrysts occur side by side, due to the mixing processes (Tsuchiyama, 1985; Stimac and Pearce, 1992; Tepley III <i>et al.,</i> 1999; Nakamura and Shimakita, 1998).</font></p>  	    <p align="justify"><font size="2" face="Verdana">Coarse sieve textures in plagioclase are interpreted as a result of rapid decompression with minor heat loss, rather than magma mixing (Nelson and Montana, 1992). The decompression of the system takes the plagioclase equilibrium composition to a more calcic composition, and this change is greater with the addition of the diopside component to the system, a likely condition in the Pay&uacute;n Matr&uacute; Volcanic Field as seen in the widespread occurrence of clinopyroxene in all its volcanic products (Nelson and Montana, 1992).</font></p>  	    <p align="justify"><font size="2" face="Verdana">Mafic minerals may also show disequilibrium textures, but because of the faster diffusion of Fe&#45;Mg with respect to the diffusion of CaAl&#45;NaSi, these textures are less likely to be preserved (Nakamura and Shimakita, 1998). Biotite breaks down into a reaction rim of anhydrous minerals by a number of reasons, such as changes in the H<sub>2</sub>O content of the melt or bulk composition or pressure. An accepted explanation to this is by rising the temperature of the host magma due to the intrusion of a mafic magma batch at the base of a magma chamber (Feeley and Sharp, 1996; Tepley III <i>et al.,</i> 1999). Considering the mineral textures and association where the dehydrated biotite crystals occur, the most reasonable explanation for the reaction rims in biotite is magma mixing.</font></p>  	    ]]></body>
<body><![CDATA[<p align="justify"><font size="2" face="Verdana">Opaque rims in amphiboles are common in volcanic rocks and are not necessarily related to magma mixing processes. In magmas ascending slowly from the storage zone at depth, the decompression and the loss of volatiles can produce the instability of amphibole and the reaction rim (Tepley III <i>et al.,</i> 1999, Rutherford and Hill, 1993), which may be due to decompression or by mixing with another magma poor in volatiles (Kus&ccedil;u and Floyd, 2001). Clinopyroxene destabilizes by nucleating Fe&#45;Ti oxides and rendering it opaque, in decompression experiments (Nelson and Montana, 1992).</font></p>  	    <p align="justify"><font size="2" face="Verdana">These mineralogical disequilibrium textures considered above, formed either by decompression or magma mixing, occur widely in the pre&#45;caldera stage of Pay&uacute;n Matr&uacute;. The occurrence of dusty and coarse sieved zones in plagioclase phenocrysts is common (<a href="#img09">Fig. 9a</a>), as the reaction rims with anhydrous minerals in biotite (<a href="#img09">Fig. 9b</a>) and the opaque rim in amphibole (<a href="#img09">Fig. 9c</a>), when these minerals are present. A few cases of magma mingling are present in the Pre&#45;caldera Trachytes unit, showing the same mineralogical disequilibria textures named above (<a href="#img09">Fig. 9d</a>).</font></p>  	    <p align="justify"><font size="2" face="Verdana">The origin of the explosive eruption that deposited the Portezuelo Ignimbrite is somehow obscure. There have been cases in which the intrusion of mafic magma into a more silicic chamber triggered the explosive eruption, by producing the heating of the silicic magma and the exsolution of volatiles. This, in turn, would increase the pressure in the relatively shallow magmatic chamber and provide the energy required for the eruption (Kuritani, 2001; Kennet and Eichelberg, 1997; Snyder, 2000; Leonard <i>et al.,</i> 2002; Shane <i>et al.,</i> 2007). Also, the release of volatiles from the dehydration of amphibole and biotite can produce the vesiculation of the magma and the subsequent eruption (Tepley III <i>et al.,</i> 1999). Considering the widespread occurrence of magma mixing and mingling in the pre&#45;caldera stage, this explanation would seem the most reasonable one for the origin of the explosive eruption. Nevertheless, the petrography of the Portezuelo Ignimbrite does not show the same mineralogical disequilibrium textures of the Pre&#45;caldera Trachytes unit, with the exception of some coarse sieved feldspars (<a href="#img09">Fig. 9e</a>). Biotite crystals do not show signs of thermal instabilities (<a href="#img09">Fig. 9f</a>). If the intrusion of mafic magma into the trachytic magma chamber of Pay&uacute;n Matr&uacute; was the triggering factor for the explosive phase of the Portezuelo Ignimbrite, it may be possible that these magmas formed a not mixed cap in the top of the magma chamber. This matter is still under consideration and needs further studies.</font></p>  	    <p align="justify"><font size="2" face="Verdana">In the early post&#45;caldera stage, represented by the Post&#45;caldera Trachyandesites unit, the abundance of dusty zones in euhedral and also in rounded pla&#45;gioclases is widespread, and they are present along with clean and euhedral plagioclases (<a href="#img10">Fig. 10a, b</a>). The large variety of plagioclase textures and their abundance is a characteristic that is compatible with magma mixing processes. In the intra&#45;caldera basaltic trachyandesitic lava flow, the mingling process, although not very discernible in the field,</font></p>  	    <p align="justify"><font size="2" face="Verdana">is evident in a microscopic scale and also in whole rock geochemical analysis (samples PM 13 and 34, <a href="/fbpe/img/andgeol/v39n1/t08-02.html" target="_blank">Table 2</a>), with pockets of trachytic magma immersed in basaltic trachyandesitic lava (<a href="#img09">Fig. 9d</a>). Mixing processes were much more common than mingling ones, indicating that the proportion of the mafic end&#45;member was high (&gt;30%) or, less likely, that the compositional differences were low (&lt;10% SiO<sub>2</sub>), otherwise, mafic enclaves would have formed in the more silicic magma (Stimac and Pearce, 1992; Tepley III <i>et al,</i> 1999; Kus&ccedil;u and Floyd, 2001).</font></p>  	    
<p align="justify"><font size="2" face="Verdana">The late post&#45;caldera stage, represented by the Post&#45;caldera Trachytes unit with its three lithofacies, does not show reabsorption textures characteristic of magma mixing (<a href="#img10">Fig. 10e and 10f</a>). Although the eruption style of the lithofacies changed from effusive to slightly explosive and again to effusive, the whole rock trachytic composition of the magmas remained relatively constant. Based on their morphology and textural characteristics of the deposits, the Pumice cones lithofacies is interpreted as very proximal pyroclastic fall deposits, analogous to their mafic equivalents, the scoria cones. The Vitreous Trachytes lithofacies is interpreted to be the degasified equivalent of the magma that formed the pumiceous cones, considering the field relations and petrographic characteristics.</font></p>  	    <p align="justify"><font size="2" face="Verdana">The values of the initial <sup>87</sup>Sr/<sup>86</sup>Sr isotopic ratio of both basalts and trachytes lie close to the present day mean mantle values of 0.704, and show narrow ranges, suggesting little contamination with radiogenic crust. Only in the younger post&#45;caldera trachytes of the Post&#45;caldera Trachytes unit there is a slight increase in this value. The homogeneous <sup>87</sup>Sry<sup>86</sup>Sr isotopic ratio along with the linear trends in the TAS and Harker diagrams for major elements (<a href="#img11">Figs. 11</a> and <a href="#img12">12</a>) are consistent with the idea that the trachytic lavas are differentiated products of the basalts. The <sup>87</sup>Sr/<sup>86</sup>Sr isotopic ratio of Pay&uacute;n Matr&uacute; Volcanic Field rocks indicates that either the magmas are fractioned from mantle derived magmas, or that they are mixtures of mantle derived magmas and melts of magmas with isotopic ratios like the mantle magmas. The silicic lavas could be partial melts of underplated mantle derived basalt.</font></p>  	    <p align="justify"><font size="2" face="Verdana">Since in bivariate diagrams hybrid magmas must lie along a tie line connecting the end&#45;members of the mixing products, the Post&#45;caldera Trachyandesites and some hybrid Pre&#45;caldera Trachytes unit lavas would represent a mixture between magmas of basaltic and trachytic compositions, being the evolved member of pre&#45;caldera trachytes type and not of post&#45;caldera trachytes type. This is easily discernible in the Harker diagram for Al<sub>2</sub>O<sub>3</sub> (<a href="#img12">Fig. 12</a>), where the younger trachytes have a significantly lower value of Al<sub>2</sub>O<sub>3</sub> than it would be expected for the more silicic end&#45;member of the mixed products. Post&#45;caldera Trachyandesites unit lavas and the hybrid or mingled lavas of the Pre&#45;caldera Trachytes unit do not coincide with the tie line connecting the Post&#45;caldera Trachytes and basaltic extreme compositions.</font></p>  	    <p align="justify"><font size="3" face="Verdana"><b>6. &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Conclusions</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">The Pay&uacute;n Matr&uacute; Volcanic Field is one of the two basaltic fields of the Payenia Basaltic Province, the largest Quaternary basaltic province present in the Andes back&#45;arc of South America. The Pay&uacute;n Matr&uacute; Volcanic Field comprises two composite volcanoes (Pay&uacute;n Matr&uacute; with a circular summit caldera and Pay&uacute;n Liso stratovolcano) along with basaltic fields east and west of the Pay&uacute;n Matr&uacute; caldera.</font></p>  	    ]]></body>
<body><![CDATA[<p align="justify"><font size="2" face="Verdana">The Pay&uacute;n Matr&uacute; Volcanic Field is a notable example of magma mixing, where the end&#45;members of this mixing process are side by side in the field, showing two contrasting styles of volcanic activity: one forming a volcanic field with numerous monogenic basaltic cones and lava flows, and the other forming a polygenic volcano with a single shield&#45;shaped edifice built by successive effusive and explosive eruptions, the Pay&uacute;n Matr&uacute;. Basaltic magmas originated in the mantle were erupted forming basaltic fields, with their eruptions controlled by NW&#45;SE and E&#45;W fissures. The trachytic Pay&uacute;n Matr&uacute; volcano is a product of the differentiation of these basaltic magmas. With the exception of the latest stage when the more evolved trachytes erupted, the Pay&uacute;n Matr&uacute; history was marked by recurrent mixing processes of basaltic and trachytic magmas. Thus, magma mixing is the result of injection of basaltic magma coming from depth into a cogenetic trachytic magma chamber near the surface.</font></p>  	    <p align="justify"><font size="2" face="Verdana"><b>Acknowledgements</b></font></p>  	    <p align="justify"><font size="2" face="Verdana">We are grateful to the staff of Recursos Naturales Renovables of Malarg&uuml;e, Argentina, for their support in the successive field work. We would like to thank A. Schiuma, L. Oliva, M. Galina, G. P&aacute;ez and F. Gonz&aacute;lez Soto (Universidad Nacional de La Plata, Argentina) for their contributions in the field work. Special thanks to J. Franzese and A. Benialgo (Centro de Investigaciones Geol&oacute;gicas, La Plata, Argentina) for the enlightening revision of the manuscript and for helping with the satellite imagery, respectively, and also to A. Richter (Universidad Nacional de La Plata, Argentina) for the revision of the manuscript. We also thank V Garc&iacute;a and R. Varela (Centro de Investigaciones Geol&oacute;gicas, La Plata, Argentina) for helping in the laboratory procedures and techniques. Thanks to L. G&oacute;mez Peral (Centro de Investigaciones Geol&oacute;gicas, La Plata, Argentina) for providing a processed satellite image. Finally, we would like to thank the reviewers for the comments and suggestions that improved the article. This study was funded by projects UNLP N547 and N620 and CONICET PIP 0119, Argentina.</font></p> 	    <p align="justify">&nbsp;</p> 	    <p align="justify"><font size="3" face="Verdana"><b>References</b></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Berm&uacute;dez, A.; Delpino, D. 1989. La provincia bas&aacute;ltica andino cuyana. Revista de la Asociaci&oacute;n Geol&oacute;gica Argentina 44 (1&#45;4): 35&#45;55.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800001&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Berm&uacute;dez, A.; Delpino, D.; Frey, F.; Saal, A. 1993. Los basaltos de retroarco extraandinos. <i>In</i> Congreso Geol&oacute;gico Argentino, No. 12 and Congreso de Exploraci&oacute;n de Hidrocarburos, No. 2. Geolog&iacute;a y Recursos Naturales de Mendoza (Ramos, V.A.; editor), Relatorio I (13): 161&#45;172. Mendoza.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800002&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Feeley, T.C.; Sharp, Z.D. 1996. Chemical and hydrogen isotopic evidence for <i>in situ</i> dehydrogenation of biotite in silicic magma chamber. Geology 24: 1021&#45;1024.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800003&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Folguera, A.; Naranjo, J.A.; Orihashi, Y.; Sumino, H.; Nagao, K. 2009. Retroarc volcanism in the northern San Rafael Block (34&deg;&#45;35&deg;30'S), southern Central Andes: Occurrence, age, and tectonic setting. Journal of Volcanology and Geothermal Research 186: 169&#45;185.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800004&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Galland, O.; Hallot, E.; Cobbold, P.R.; Buffet, G. 2007. Volcanism in a compressional Andean setting: A structural and geochronological study of Tromen volcano (Neuqu&eacute;n province, Argentina). Tectonics 26 TC4010: 1&#45;24.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800005&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Germa, A.; Quidelleur, X.; Gillot, P. Y.; Tchilinguirian, P. 2010. Volcanic evolution of the back&#45;arc Pleistocene Payun Matru volcanic field (Argentina). Journal of South American Earth Sciences 29: 717&#45;730.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800006&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Gonz&aacute;lez D&iacute;az, E. 1970. Rasgos morfol&oacute;gicos del &aacute;rea volc&aacute;nica del cerro&#45;volc&aacute;n Pay&uacute;n Matr&uacute;. Opera Lilloana 20: 102 p.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800007&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Gonz&aacute;lez D&iacute;az, E. 1972. Descripci&oacute;n geol&oacute;gica de la Hoja 30d Pay&uacute;n Matr&uacute;. Direcci&oacute;n Nacional de Geolog&iacute;a y Miner&iacute;a, Bolet&iacute;n 130: 92 p.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800008&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Hernando, I.R.; Llamb&iacute;as, E.J.; Garc&iacute;a, V 2011. Caracterizaci&oacute;n geoqu&iacute;mica del volc&aacute;n Pay&uacute;n Matr&uacute;, retroarco andino al sur de la provincia de Mendoza. <i>In</i> Congreso Geol&oacute;gico Argentino, No. 18, Actas: 486&#45;487. Neuqu&eacute;n.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800009&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Inbar, M.; Risso, C. 2001a. A morphological and morphometric an&aacute;lisis of a high density cinder cone volcanic field &#45; Payun Matru, south&#45;central Andes, Argentina. Zeitschrift f&uuml;r Geomorfologie 45 (3): 321&#45;343.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800010&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Inbar, M.; Risso, C. 2001b. Holocene yardangs in volcanic terrains in the southern Andes. Earth Surface Processes and Landforms 26: 657&#45;666.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800011&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Irvine, T.N.; Baragar, W.R.A. 1971. A guide to the chemical ckassification of the common volcanic rocks. Canadian Journal of Earth Sciences 8: 523&#45;548.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800012&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Kay, S.M. 2002. Magmatic sources, tectonic setting and causes of tertiary to recent Patagonian plateau magmatism (36&deg;S to 52&deg;S latitude). <i>In</i> Congreso Geol&oacute;gico Argentino, No. 15, Actas 3: 95&#45;100. Calafate.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800013&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Kay, S.M.; Gorring, M.; Ramos, V.A. 2004. Magmatic sources, setting and causes of Eocene to recent Patagonian plateau magmatism (36&deg;S to 52&deg;S latitude). Revista de la Asociaci&oacute;n Geol&oacute;gica Argentina 59 (4): 556&#45;568.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800014&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Kay, S.M.; Burns, W.M.; Copeland, P.; Mancilla, O. 2006a. Upper Cretaceous to Holocene magmatism and evidence for transient Miocene shallowing of the Andean subduction zone under the northern Neuqu&eacute;n Basin. <i>In</i> Evolution of an Andean margin: A tectonic and magmatic view from the Andes to the Neuqu&eacute;n Basin (35&deg;&#45;39&deg;S latitude) (Kay, S.M.; Ramos, V.A.; editors). Geological Society of America, Special Paper 407: 19&#45;60. Colorado.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800015&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p> 	    <!-- ref --><p align="justify"><font size="2" face="Verdana"> Kay, S.M.; Mancilla, O.; Copeland, P. 2006b. Evolution of the late Miocene Chachahu&eacute;n volcanic complex at 37&deg;S over a transient shallow subduction zone under the Neuqu&eacute;n Andes. <i>In</i> Evolution of an Andean Margin: A tectonic and magmatic view from the Andes to the Neuqu&eacute;n Basin (35&deg;&#45;39&deg;S lat.) (Kay, S.M.; Ramos, V.A.; editors). Geological Society of America, Special Paper 407: 215&#45;246. Colorado.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800016&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p> 	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Kennet, J.W; Eichelberg, J.C. 1997. Syneruptive mixing, degassing and crystallization at Redoubt volcano, eruption of december, 1989 to may 1990. Journal of Volcanology and Geothermal Research 75: 19&#45;37.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800017&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Kuritani, T. 2001. Replenishment of a mafic magma in a zoned mafic magma chamber beneath Rishiri Volcano, Japan. Bulletin of Volcanology 62: 533&#45;548.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800018&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Kus&ccedil;u, G.G.; Floyd, P.A. 2001. Mineral compositional and textural evidence for magma mingling in the Saraykent volcanics. Lithos 56: 207&#45;230.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800019&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Le Maitre, R.W.; Bateman, P.; Dudek, A.; Keller, J.; Lameyre, J.; Le Bas, M.J.; Sabine, P.A.; Schmid, R.; Sorensen, H.&nbsp;; Streckeisen, A.; Woolley, A.R.; Zanettin, B. 1989. A classification of igneous rocks and glossary of terms: Recommendations of the International Union of Geological Sciences Subcommission on the Systematics of Igneous Rocks. Blackwell Scientific: 193 p. Oxford.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800020&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Leonard, G.S.; Cole, J.W.; Nairn, I.A.; Self, S. 2002. Basalt triggering of the c. AD 1305 Kaharoa rhyolite eruption, Tarawera Volcanic Complex, New Zealand. Journal of Volcanology and Geothermal Research 115: 461&#45;486.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800021&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Llamb&iacute;as, E.J. 1966. Geolog&iacute;a y petrolog&iacute;a del volc&aacute;n Pay&uacute;n Matr&uacute;. Acta Geol&oacute;gica Lilloana 8: 265&#45;315.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800022&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Llamb&iacute;as, E.J.; Bertotto, G.W.; Risso, C.; Hernando, I.&nbsp;R. 2010. El volcanismo cuaternario en el retroarco de Payenia: una revisi&oacute;n. Revista de la asociaci&oacute;n Geol&oacute;gica Argentina 67 (2): 278&#45;300.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800023&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Nakamura, M.; Shimakita, S. 1998. Dissolution origin and syn&#45;entrapment compositional change of melt inclusion in plagioclase. Earth and Planetary Science Letters 161: 119&#45;133.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800024&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Nelson, S.T.; Montana, A. 1992. Sieve&#45;textured plagioclase in volcanic rocks produced by rapid decompression. American Mineralogist 77: 1242&#45;1249.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800025&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Pasquer&egrave;, G.; Bistacchi, A.; Francalanci, L.; Bertotto, G.W.; Boari, E.; Massironi, M.; Rossotti, A. 2008. Very long pahoehoe inflated basaltic lava flows in the Payenia Volcanic Province (Mendoza and La Pampa, Argentina). Revista de la Asociaci&oacute;n Geol&oacute;gica Argentina 63 (1): 131&#45;149.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800026&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Polanski, J. 1954. Rasgos geomorfol&oacute;gicos del territorio de la provincia de Mendoza. Instituto de Investigaciones Econ&oacute;micas y Tecnol&oacute;gicas, Cuadernos de Estudio e Investigaci&oacute;n 4: 10 p. Mendoza.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800027&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Ramos, V.A. 1978. Estructura. <i>In</i> Geolog&iacute;a y Recursos Naturales del Neuqu&eacute;n. <i>In</i> Congreso Geol&oacute;gico Argentino, No. 7, Relatorio: 99&#45;118. Neuqu&eacute;n.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800028&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Ramos, V.A.; Kay, S.M. 2006. Overview of the tectonic evolution of the southern Central Andes of Mendoza and Neuqu&eacute;n (35&deg;&#45;39&deg;S latitude). <i>In</i> Evolution of an Andean margin: A tectonic and magmatic view from the Andes to the Neuqu&eacute;n Basin (35&deg;&#45;39&deg;S latitude) (Kay, S.M.; Ramos, V.A.; editors) Geological Society of America, Special Paper 407: 1&#45;17. Colorado.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800029&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p> 	    <!-- ref --><p align="justify"><font size="2" face="Verdana"> Ramos, V.A.; Folguera, A. 2010. Payenia volcanic province in the Southern Andes: An appraisal of an exceptional Quaternary tectonic setting. Journal of Volcanology and Geothermal Research 201 (1&#45;4): 53&#45;64</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800030&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font size="2" face="Verdana">Rutherford, M.J.; Hill, P.M. 1993. Magma ascent rates from amphibole breakdown: An experimental study applied to the 1980&#45;1986 Mount St. Helens eruptions. Journal of Geophisical Research 98 (11): 667&#45;685.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800031&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Shane, P.; Martin, S.B.; Smith, V.C.; Beggs, K.F.; Darragh, M.B.; Cole, J.W.; Nairn, I.A. 2007. Multiple rhyolite magmas and basalt injection in the 17.7 ka Rerewhakaaitu eruption episode from Tarawera Volcanic Complex, New Zealand. Journal of Volcanology and Geothermal Research 164: 1&#45;26.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800032&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Snyder, D. 2000. Thermal effects of the intrusion of basaltic magma into a more silicic magma chamber and implications for eruption triggering. Earth and Planetary Science Letters 175: 257&#45;273.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800033&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    ]]></body>
<body><![CDATA[<!-- ref --><p align="justify"><font size="2" face="Verdana">Stern, C.R.; Frey, F.A.; Futa, K.; Zartman, R.E.; Peng, Z.; Kyser, T.K. 1990. Trace&#45;element and Sr, Nd, Pb, and O isotopic composition of Pliocene and Quaternary alkali basalts of the Patagonian Plateau lavas of southernmost South America. Contributions to Mineralogy and Petrology 104: 294&#45;308.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800034&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Stimac, J.A.; Pearce, T.H. 1992. Textural evidence of mafic&#45;felsic magma interaction in dacite lavas, Clear Lake, California. American Mineralogist 77: 795&#45;809.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800035&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Tepley III, F.J.; Davidson, J.P.; Clynne, M.A. 1999. Magmatic interactions as recorded in plagioclase phenocrysts of Chaos Crag, Lassen Volcanic Center, California. Journal of Petrology 40 (5): 787&#45;806.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800036&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Tsuchiyama, A. 1985. Dissolution kinetics of plagioclase in the melt of the system diopside&#45;albite&#45;anorthite, and origin of dusty plagioclase in andesites. Contributions to Mineralogy and Petrology 89: 1&#45;16.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800037&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font size="2" face="Verdana">Varela, R.; Roverano, D.; Sato, A.M. 2000. Granito El Pe&ntilde;&oacute;n, sierra de Umango: descripci&oacute;n, edad Rb/Sr e implicancias geotect&oacute;nicas. Revista de la Asociaci&oacute;n Geol&oacute;gica Argentina 55 (4): 407&#45;413.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scieloOrg/php/reflinks.php?refpid=S0718-7106201200010000800038&pid=S0718-71062012000100008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');"></a>&#160;]<!-- end-ref --></font></p> 	    ]]></body>
<body><![CDATA[<p align="justify">&nbsp;</p> 	    <p align="justify"><font size="2" face="Verdana">Manuscript received: January 11, 2011; revised/accepted: October 6, 2011; available online: October 25, 2011.</font></p>      ]]></body><back>
<ref-list>
<ref id="B1">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Bermúdez]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[Delpino]]></surname>
<given-names><![CDATA[D]]></given-names>
</name>
</person-group>
<article-title xml:lang="es"><![CDATA[La provincia basáltica andino cuyana]]></article-title>
<source><![CDATA[Revista de la Asociación Geológica Argentina]]></source>
<year>1989</year>
<volume>44</volume>
<numero>1-4</numero>
<issue>1-4</issue>
<page-range>35-55</page-range></nlm-citation>
</ref>
<ref id="B2">
<nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Bermúdez]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[Delpino]]></surname>
<given-names><![CDATA[D]]></given-names>
</name>
<name>
<surname><![CDATA[Frey]]></surname>
<given-names><![CDATA[F]]></given-names>
</name>
<name>
<surname><![CDATA[Saal]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
</person-group>
<article-title xml:lang="es"><![CDATA[Los basaltos de retroarco extraandinos]]></article-title>
<person-group person-group-type="editor">
<name>
<surname><![CDATA[Ramos]]></surname>
<given-names><![CDATA[V.A]]></given-names>
</name>
</person-group>
<source><![CDATA[Congreso Geológico Argentino, No. 12 and Congreso de Exploración de Hidrocarburos, No. 2: Geología y Recursos Naturales de Mendoza]]></source>
<year>1993</year>
<page-range>161-172</page-range><publisher-loc><![CDATA[Mendoza ]]></publisher-loc>
</nlm-citation>
</ref>
<ref id="B3">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Feeley]]></surname>
<given-names><![CDATA[T.C]]></given-names>
</name>
<name>
<surname><![CDATA[Sharp]]></surname>
<given-names><![CDATA[Z.D]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Chemical and hydrogen isotopic evidence for in situ dehydrogenation of biotite in silicic magma chamber]]></article-title>
<source><![CDATA[Geology]]></source>
<year>1996</year>
<volume>24</volume>
<page-range>1021-1024</page-range></nlm-citation>
</ref>
<ref id="B4">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Folguera]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[Naranjo]]></surname>
<given-names><![CDATA[J.A]]></given-names>
</name>
<name>
<surname><![CDATA[Orihashi]]></surname>
<given-names><![CDATA[Y]]></given-names>
</name>
<name>
<surname><![CDATA[Sumino]]></surname>
<given-names><![CDATA[H]]></given-names>
</name>
<name>
<surname><![CDATA[Nagao]]></surname>
<given-names><![CDATA[K]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Retroarc volcanism in the northern San Rafael Block (34°-35°30'S), southern Central Andes: Occurrence, age, and tectonic setting]]></article-title>
<source><![CDATA[Journal of Volcanology and Geothermal Research]]></source>
<year>2009</year>
<volume>186</volume>
<page-range>169-185</page-range></nlm-citation>
</ref>
<ref id="B5">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Galland]]></surname>
<given-names><![CDATA[O]]></given-names>
</name>
<name>
<surname><![CDATA[Hallot]]></surname>
<given-names><![CDATA[E]]></given-names>
</name>
<name>
<surname><![CDATA[Cobbold]]></surname>
<given-names><![CDATA[P.R]]></given-names>
</name>
<name>
<surname><![CDATA[Buffet]]></surname>
<given-names><![CDATA[G]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Volcanism in a compressional Andean setting: A structural and geochronological study of Tromen volcano (Neuquén province, Argentina)]]></article-title>
<source><![CDATA[Tectonics]]></source>
<year>2007</year>
<volume>26</volume>
<numero>TC4010</numero>
<issue>TC4010</issue>
<page-range>1-24</page-range></nlm-citation>
</ref>
<ref id="B6">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Germa]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[Quidelleur]]></surname>
<given-names><![CDATA[X]]></given-names>
</name>
<name>
<surname><![CDATA[Gillot]]></surname>
<given-names><![CDATA[P. Y]]></given-names>
</name>
<name>
<surname><![CDATA[Tchilinguirian]]></surname>
<given-names><![CDATA[P]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Volcanic evolution of the back-arc Pleistocene Payun Matru volcanic field (Argentina)]]></article-title>
<source><![CDATA[Journal of South American Earth Sciences]]></source>
<year>2010</year>
<volume>29</volume>
<page-range>717-730</page-range></nlm-citation>
</ref>
<ref id="B7">
<nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[González Díaz]]></surname>
<given-names><![CDATA[E]]></given-names>
</name>
</person-group>
<source><![CDATA[Rasgos morfológicos del área volcánica del cerro-volcán Payún Matrú: Opera Lilloana]]></source>
<year>1970</year>
<volume>20</volume>
</nlm-citation>
</ref>
<ref id="B8">
<nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[González Díaz]]></surname>
<given-names><![CDATA[E]]></given-names>
</name>
</person-group>
<source><![CDATA[Descripción geológica de la Hoja 30d Payún Matrú]]></source>
<year>1972</year>
<volume>130</volume>
<publisher-name><![CDATA[Dirección Nacional de Geología y Minería]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B9">
<nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Hernando]]></surname>
<given-names><![CDATA[I.R]]></given-names>
</name>
<name>
<surname><![CDATA[Llambías]]></surname>
<given-names><![CDATA[E.J]]></given-names>
</name>
<name>
<surname><![CDATA[García]]></surname>
<given-names><![CDATA[V]]></given-names>
</name>
</person-group>
<article-title xml:lang="es"><![CDATA[Caracterización geoquímica del volcán Payún Matrú, retroarco andino al sur de la provincia de Mendoza]]></article-title>
<source><![CDATA[Congreso Geológico Argentino, No. 18: Actas]]></source>
<year>2011</year>
<page-range>486-487</page-range><publisher-loc><![CDATA[Neuquén ]]></publisher-loc>
</nlm-citation>
</ref>
<ref id="B10">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Inbar]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
<name>
<surname><![CDATA[Risso]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[A morphological and morphometric análisis of a high density cinder cone volcanic field - Payun Matru, south-central Andes, Argentina]]></article-title>
<source><![CDATA[Zeitschrift für Geomorfologie]]></source>
<year>2001</year>
<month>a</month>
<volume>45</volume>
<numero>3</numero>
<issue>3</issue>
<page-range>321-343</page-range></nlm-citation>
</ref>
<ref id="B11">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Inbar]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
<name>
<surname><![CDATA[Risso]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Holocene yardangs in volcanic terrains in the southern Andes]]></article-title>
<source><![CDATA[Earth Surface Processes and Landforms]]></source>
<year>2001</year>
<month>b</month>
<volume>26</volume>
<page-range>657-666</page-range></nlm-citation>
</ref>
<ref id="B12">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Irvine]]></surname>
<given-names><![CDATA[T.N]]></given-names>
</name>
<name>
<surname><![CDATA[Baragar]]></surname>
<given-names><![CDATA[W.R.A]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[A guide to the chemical ckassification of the common volcanic rocks]]></article-title>
<source><![CDATA[Canadian Journal of Earth Sciences]]></source>
<year>1971</year>
<volume>8</volume>
<page-range>523-548</page-range></nlm-citation>
</ref>
<ref id="B13">
<nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Kay]]></surname>
<given-names><![CDATA[S.M]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Magmatic sources, tectonic setting and causes of tertiary to recent Patagonian plateau magmatism (36°S to 52°S latitude)]]></article-title>
<source><![CDATA[Congreso Geológico Argentino, No. 15: Actas]]></source>
<year>2002</year>
<volume>3</volume>
<page-range>95-100</page-range><publisher-loc><![CDATA[Calafate ]]></publisher-loc>
</nlm-citation>
</ref>
<ref id="B14">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Kay]]></surname>
<given-names><![CDATA[S.M]]></given-names>
</name>
<name>
<surname><![CDATA[Gorring]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
<name>
<surname><![CDATA[Ramos]]></surname>
<given-names><![CDATA[V.A]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Magmatic sources, setting and causes of Eocene to recent Patagonian plateau magmatism (36°S to 52°S latitude)]]></article-title>
<source><![CDATA[Revista de la Asociación Geológica Argentina]]></source>
<year>2004</year>
<volume>59</volume>
<numero>4</numero>
<issue>4</issue>
<page-range>556-568</page-range></nlm-citation>
</ref>
<ref id="B15">
<nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Kay]]></surname>
<given-names><![CDATA[S.M]]></given-names>
</name>
<name>
<surname><![CDATA[Burns]]></surname>
<given-names><![CDATA[W.M]]></given-names>
</name>
<name>
<surname><![CDATA[Copeland]]></surname>
<given-names><![CDATA[P]]></given-names>
</name>
<name>
<surname><![CDATA[Mancilla]]></surname>
<given-names><![CDATA[O]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Upper Cretaceous to Holocene magmatism and evidence for transient Miocene shallowing of the Andean subduction zone under the northern Neuquén Basin]]></article-title>
<person-group person-group-type="editor">
<name>
<surname><![CDATA[Kay]]></surname>
<given-names><![CDATA[S.M]]></given-names>
</name>
<name>
<surname><![CDATA[Ramos]]></surname>
<given-names><![CDATA[V.A]]></given-names>
</name>
</person-group>
<source><![CDATA[Evolution of an Andean margin: A tectonic and magmatic view from the Andes to the Neuquén Basin (35°-39°S latitude)]]></source>
<year>2006</year>
<month>a</month>
<volume>407</volume>
<page-range>19-60</page-range><publisher-loc><![CDATA[Colorado ]]></publisher-loc>
<publisher-name><![CDATA[Geological Society of America]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B16">
<nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Kay]]></surname>
<given-names><![CDATA[S.M]]></given-names>
</name>
<name>
<surname><![CDATA[Mancilla]]></surname>
<given-names><![CDATA[O]]></given-names>
</name>
<name>
<surname><![CDATA[Copeland]]></surname>
<given-names><![CDATA[P]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Evolution of the late Miocene Chachahuén volcanic complex at 37°S over a transient shallow subduction zone under the Neuquén Andes]]></article-title>
<person-group person-group-type="editor">
<name>
<surname><![CDATA[Kay]]></surname>
<given-names><![CDATA[S.M]]></given-names>
</name>
<name>
<surname><![CDATA[Ramos]]></surname>
<given-names><![CDATA[V.A]]></given-names>
</name>
</person-group>
<source><![CDATA[Evolution of an Andean Margin: A tectonic and magmatic view from the Andes to the Neuquén Basin (35°-39°S lat.)]]></source>
<year>2006</year>
<month>b</month>
<volume>407</volume>
<page-range>215-246</page-range><publisher-loc><![CDATA[Colorado ]]></publisher-loc>
<publisher-name><![CDATA[Geological Society of America]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B17">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Kennet]]></surname>
<given-names><![CDATA[J.W]]></given-names>
</name>
<name>
<surname><![CDATA[Eichelberg]]></surname>
<given-names><![CDATA[J.C]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Syneruptive mixing, degassing and crystallization at Redoubt volcano, eruption of december, 1989 to may 1990]]></article-title>
<source><![CDATA[Journal of Volcanology and Geothermal Research]]></source>
<year>1997</year>
<volume>75</volume>
<page-range>19-37</page-range></nlm-citation>
</ref>
<ref id="B18">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Kuritani]]></surname>
<given-names><![CDATA[T]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Replenishment of a mafic magma in a zoned mafic magma chamber beneath Rishiri Volcano, Japan]]></article-title>
<source><![CDATA[Bulletin of Volcanology]]></source>
<year>2001</year>
<volume>62</volume>
<page-range>533-548</page-range></nlm-citation>
</ref>
<ref id="B19">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Kusçu]]></surname>
<given-names><![CDATA[G.G]]></given-names>
</name>
<name>
<surname><![CDATA[Floyd]]></surname>
<given-names><![CDATA[P.A]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Mineral compositional and textural evidence for magma mingling in the Saraykent volcanics]]></article-title>
<source><![CDATA[Lithos]]></source>
<year>2001</year>
<volume>56</volume>
<page-range>207-230</page-range></nlm-citation>
</ref>
<ref id="B20">
<nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Le Maitre]]></surname>
<given-names><![CDATA[R.W]]></given-names>
</name>
<name>
<surname><![CDATA[Bateman]]></surname>
<given-names><![CDATA[P]]></given-names>
</name>
<name>
<surname><![CDATA[Dudek]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[Keller]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
<name>
<surname><![CDATA[Lameyre]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
<name>
<surname><![CDATA[Le Bas]]></surname>
<given-names><![CDATA[M.J]]></given-names>
</name>
<name>
<surname><![CDATA[Sabine]]></surname>
<given-names><![CDATA[P.A]]></given-names>
</name>
<name>
<surname><![CDATA[Schmid]]></surname>
<given-names><![CDATA[R]]></given-names>
</name>
<name>
<surname><![CDATA[Sorensen]]></surname>
<given-names><![CDATA[H]]></given-names>
</name>
<name>
<surname><![CDATA[Streckeisen]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[Woolley]]></surname>
<given-names><![CDATA[A.R]]></given-names>
</name>
<name>
<surname><![CDATA[Zanettin]]></surname>
<given-names><![CDATA[B]]></given-names>
</name>
</person-group>
<source><![CDATA[A classification of igneous rocks and glossary of terms: Recommendations of the International Union of Geological Sciences Subcommission on the Systematics of Igneous Rocks]]></source>
<year>1989</year>
<publisher-loc><![CDATA[Oxford ]]></publisher-loc>
<publisher-name><![CDATA[Blackwell Scientific]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B21">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Leonard]]></surname>
<given-names><![CDATA[G.S]]></given-names>
</name>
<name>
<surname><![CDATA[Cole]]></surname>
<given-names><![CDATA[J.W]]></given-names>
</name>
<name>
<surname><![CDATA[Nairn]]></surname>
<given-names><![CDATA[I.A]]></given-names>
</name>
<name>
<surname><![CDATA[Self]]></surname>
<given-names><![CDATA[S]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Basalt triggering of the c. AD 1305 Kaharoa rhyolite eruption, Tarawera Volcanic Complex, New Zealand]]></article-title>
<source><![CDATA[Journal of Volcanology and Geothermal Research]]></source>
<year>2002</year>
<volume>115</volume>
<page-range>461-486</page-range></nlm-citation>
</ref>
<ref id="B22">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Llambías]]></surname>
<given-names><![CDATA[E.J]]></given-names>
</name>
</person-group>
<article-title xml:lang="es"><![CDATA[Geología y petrología del volcán Payún Matrú]]></article-title>
<source><![CDATA[Acta Geológica Lilloana]]></source>
<year>1966</year>
<volume>8</volume>
<page-range>265-315</page-range></nlm-citation>
</ref>
<ref id="B23">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Llambías]]></surname>
<given-names><![CDATA[E.J]]></given-names>
</name>
<name>
<surname><![CDATA[Bertotto]]></surname>
<given-names><![CDATA[G.W]]></given-names>
</name>
<name>
<surname><![CDATA[Risso]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
<name>
<surname><![CDATA[Hernando]]></surname>
<given-names><![CDATA[I. R]]></given-names>
</name>
</person-group>
<article-title xml:lang="es"><![CDATA[El volcanismo cuaternario en el retroarco de Payenia: una revisión]]></article-title>
<source><![CDATA[Revista de la asociación Geológica Argentina]]></source>
<year>2010</year>
<volume>67</volume>
<numero>2</numero>
<issue>2</issue>
<page-range>278-300</page-range></nlm-citation>
</ref>
<ref id="B24">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Nakamura]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
<name>
<surname><![CDATA[Shimakita]]></surname>
<given-names><![CDATA[S]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Dissolution origin and syn-entrapment compositional change of melt inclusion in plagioclase]]></article-title>
<source><![CDATA[Earth and Planetary Science Letters]]></source>
<year>1998</year>
<volume>161</volume>
<page-range>119-133</page-range></nlm-citation>
</ref>
<ref id="B25">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Nelson]]></surname>
<given-names><![CDATA[S.T]]></given-names>
</name>
<name>
<surname><![CDATA[Montana]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Sieve-textured plagioclase in volcanic rocks produced by rapid decompression]]></article-title>
<source><![CDATA[American Mineralogist]]></source>
<year>1992</year>
<volume>77</volume>
<page-range>1242-1249</page-range></nlm-citation>
</ref>
<ref id="B26">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Pasquerè]]></surname>
<given-names><![CDATA[G]]></given-names>
</name>
<name>
<surname><![CDATA[Bistacchi]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[Francalanci]]></surname>
<given-names><![CDATA[L]]></given-names>
</name>
<name>
<surname><![CDATA[Bertotto]]></surname>
<given-names><![CDATA[G.W]]></given-names>
</name>
<name>
<surname><![CDATA[Boari]]></surname>
<given-names><![CDATA[E]]></given-names>
</name>
<name>
<surname><![CDATA[Massironi]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
<name>
<surname><![CDATA[Rossotti]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Very long pahoehoe inflated basaltic lava flows in the Payenia Volcanic Province (Mendoza and La Pampa, Argentina)]]></article-title>
<source><![CDATA[Revista de la Asociación Geológica Argentina]]></source>
<year>2008</year>
<volume>63</volume>
<numero>1</numero>
<issue>1</issue>
<page-range>131-149</page-range></nlm-citation>
</ref>
<ref id="B27">
<nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Polanski]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
</person-group>
<source><![CDATA[Rasgos geomorfológicos del territorio de la provincia de Mendoza]]></source>
<year>1954</year>
<volume>4</volume>
<publisher-loc><![CDATA[Mendoza ]]></publisher-loc>
<publisher-name><![CDATA[Instituto de Investigaciones Económicas y Tecnológicas]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B28">
<nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Ramos]]></surname>
<given-names><![CDATA[V.A]]></given-names>
</name>
</person-group>
<article-title xml:lang="es"><![CDATA[Estructura]]></article-title>
<source><![CDATA[Congreso Geológico Argentino, No. 7: Relatorio]]></source>
<year>1978</year>
<page-range>99-118</page-range><publisher-loc><![CDATA[Neuquén ]]></publisher-loc>
</nlm-citation>
</ref>
<ref id="B29">
<nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Ramos]]></surname>
<given-names><![CDATA[V.A]]></given-names>
</name>
<name>
<surname><![CDATA[Kay]]></surname>
<given-names><![CDATA[S.M]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Overview of the tectonic evolution of the southern Central Andes of Mendoza and Neuquén (35°-39°S latitude)]]></article-title>
<person-group person-group-type="editor">
<name>
<surname><![CDATA[Kay]]></surname>
<given-names><![CDATA[S.M]]></given-names>
</name>
<name>
<surname><![CDATA[Ramos]]></surname>
<given-names><![CDATA[V.A]]></given-names>
</name>
</person-group>
<source><![CDATA[Evolution of an Andean margin: A tectonic and magmatic view from the Andes to the Neuquén Basin (35°-39°S latitude)]]></source>
<year>2006</year>
<volume>407</volume>
<page-range>1-17</page-range><publisher-loc><![CDATA[Colorado ]]></publisher-loc>
<publisher-name><![CDATA[Geological Society of America]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B30">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Ramos]]></surname>
<given-names><![CDATA[V.A]]></given-names>
</name>
<name>
<surname><![CDATA[Folguera]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Payenia volcanic province in the Southern Andes: An appraisal of an exceptional Quaternary tectonic setting]]></article-title>
<source><![CDATA[Journal of Volcanology and Geothermal Research]]></source>
<year>2010</year>
<volume>201</volume>
<numero>1-4</numero>
<issue>1-4</issue>
<page-range>53-64</page-range></nlm-citation>
</ref>
<ref id="B31">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Rutherford]]></surname>
<given-names><![CDATA[M.J]]></given-names>
</name>
<name>
<surname><![CDATA[Hill]]></surname>
<given-names><![CDATA[P.M]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Magma ascent rates from amphibole breakdown: An experimental study applied to the 1980-1986 Mount St. Helens eruptions]]></article-title>
<source><![CDATA[Journal of Geophisical Research]]></source>
<year>1993</year>
<volume>98</volume>
<numero>11</numero>
<issue>11</issue>
<page-range>667-685</page-range></nlm-citation>
</ref>
<ref id="B32">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Shane]]></surname>
<given-names><![CDATA[P]]></given-names>
</name>
<name>
<surname><![CDATA[Martin]]></surname>
<given-names><![CDATA[S.B]]></given-names>
</name>
<name>
<surname><![CDATA[Smith]]></surname>
<given-names><![CDATA[V.C]]></given-names>
</name>
<name>
<surname><![CDATA[Beggs]]></surname>
<given-names><![CDATA[K.F]]></given-names>
</name>
<name>
<surname><![CDATA[Darragh]]></surname>
<given-names><![CDATA[M.B]]></given-names>
</name>
<name>
<surname><![CDATA[Cole]]></surname>
<given-names><![CDATA[J.W]]></given-names>
</name>
<name>
<surname><![CDATA[Nairn]]></surname>
<given-names><![CDATA[I.A]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Multiple rhyolite magmas and basalt injection in the 17.7 ka Rerewhakaaitu eruption episode from Tarawera Volcanic Complex, New Zealand]]></article-title>
<source><![CDATA[Journal of Volcanology and Geothermal Research]]></source>
<year>2007</year>
<volume>164</volume>
<page-range>1-26</page-range></nlm-citation>
</ref>
<ref id="B33">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Snyder]]></surname>
<given-names><![CDATA[D]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Thermal effects of the intrusion of basaltic magma into a more silicic magma chamber and implications for eruption triggering]]></article-title>
<source><![CDATA[Earth and Planetary Science Letters]]></source>
<year>2000</year>
<volume>175</volume>
<page-range>257-273</page-range></nlm-citation>
</ref>
<ref id="B34">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Stern]]></surname>
<given-names><![CDATA[C.R]]></given-names>
</name>
<name>
<surname><![CDATA[Frey]]></surname>
<given-names><![CDATA[F.A]]></given-names>
</name>
<name>
<surname><![CDATA[Futa]]></surname>
<given-names><![CDATA[K]]></given-names>
</name>
<name>
<surname><![CDATA[Zartman]]></surname>
<given-names><![CDATA[R.E]]></given-names>
</name>
<name>
<surname><![CDATA[Peng]]></surname>
<given-names><![CDATA[Z]]></given-names>
</name>
<name>
<surname><![CDATA[Kyser]]></surname>
<given-names><![CDATA[T.K]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Trace-element and Sr, Nd, Pb, and O isotopic composition of Pliocene and Quaternary alkali basalts of the Patagonian Plateau lavas of southernmost South America]]></article-title>
<source><![CDATA[Contributions to Mineralogy and Petrology]]></source>
<year>1990</year>
<volume>104</volume>
<page-range>294-308</page-range></nlm-citation>
</ref>
<ref id="B35">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Stimac]]></surname>
<given-names><![CDATA[J.A]]></given-names>
</name>
<name>
<surname><![CDATA[Pearce]]></surname>
<given-names><![CDATA[T.H]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Textural evidence of mafic-felsic magma interaction in dacite lavas, Clear Lake, California]]></article-title>
<source><![CDATA[American Mineralogist]]></source>
<year>1992</year>
<volume>77</volume>
<page-range>795-809</page-range></nlm-citation>
</ref>
<ref id="B36">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Tepley III]]></surname>
<given-names><![CDATA[F.J]]></given-names>
</name>
<name>
<surname><![CDATA[Davidson]]></surname>
<given-names><![CDATA[J.P]]></given-names>
</name>
<name>
<surname><![CDATA[Clynne]]></surname>
<given-names><![CDATA[M.A]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Magmatic interactions as recorded in plagioclase phenocrysts of Chaos Crag, Lassen Volcanic Center, California]]></article-title>
<source><![CDATA[Journal of Petrology]]></source>
<year>1999</year>
<volume>40</volume>
<numero>5</numero>
<issue>5</issue>
<page-range>787-806</page-range></nlm-citation>
</ref>
<ref id="B37">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Tsuchiyama]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Dissolution kinetics of plagioclase in the melt of the system diopside-albite-anorthite, and origin of dusty plagioclase in andesites]]></article-title>
<source><![CDATA[Contributions to Mineralogy and Petrology]]></source>
<year>1985</year>
<volume>89</volume>
<page-range>1-16</page-range></nlm-citation>
</ref>
<ref id="B38">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Varela]]></surname>
<given-names><![CDATA[R]]></given-names>
</name>
<name>
<surname><![CDATA[Roverano]]></surname>
<given-names><![CDATA[D]]></given-names>
</name>
<name>
<surname><![CDATA[Sato]]></surname>
<given-names><![CDATA[A.M]]></given-names>
</name>
</person-group>
<article-title xml:lang="es"><![CDATA[Granito El Peñón, sierra de Umango: descripción, edad Rb/Sr e implicancias geotectónicas]]></article-title>
<source><![CDATA[Revista de la Asociación Geológica Argentina]]></source>
<year>2000</year>
<volume>55</volume>
<numero>4</numero>
<issue>4</issue>
<page-range>407-413</page-range></nlm-citation>
</ref>
</ref-list>
</back>
</article>
