<?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>0256-7024</journal-id>
<journal-title><![CDATA[Revista Geológica de América Central]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. Geol. Amér. Central]]></abbrev-journal-title>
<issn>0256-7024</issn>
<publisher>
<publisher-name><![CDATA[Universidad de Costa Rica]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0256-70242011000200003</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Progress and Challenges Using 40Ar/39Ar Geochronology in Costa Rica and Nicaragua]]></article-title>
<article-title xml:lang="es"><![CDATA[Progreso y retos de la geocronología 40Ar/39Ar en Costa Rica y Nicaragua]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Saginor¹]]></surname>
<given-names><![CDATA[Ian]]></given-names>
</name>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Gazel]]></surname>
<given-names><![CDATA[Esteban]]></given-names>
</name>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Michael J]]></surname>
<given-names><![CDATA[Carr]]></given-names>
</name>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Swisher III]]></surname>
<given-names><![CDATA[Carl C]]></given-names>
</name>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Turrin]]></surname>
<given-names><![CDATA[Brent]]></given-names>
</name>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Keystone College  ]]></institution>
<addr-line><![CDATA[La Plume PA]]></addr-line>
</aff>
<aff id="A02">
<institution><![CDATA[,Virginia Tech Department of Geological Sciences ]]></institution>
<addr-line><![CDATA[Blacksburg VA]]></addr-line>
</aff>
<aff id="A03">
<institution><![CDATA[,Rutgers University Department of Geological Sciences ]]></institution>
<addr-line><![CDATA[Piscataway NJ]]></addr-line>
</aff>
<aff id="A04">
<institution><![CDATA[,Autor para contacto  ]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>12</month>
<year>2011</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>12</month>
<year>2011</year>
</pub-date>
<numero>45</numero>
<fpage>75</fpage>
<lpage>85</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.sa.cr/scielo.php?script=sci_arttext&amp;pid=S0256-70242011000200003&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.sa.cr/scielo.php?script=sci_abstract&amp;pid=S0256-70242011000200003&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.sa.cr/scielo.php?script=sci_pdf&amp;pid=S0256-70242011000200003&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[To better estimate the extrusive flux of the Central American Arc, from 2002-2008, we obtained sixty one high precision 40Ar/39Ar ages on geographically well-situated lavas and tephra from Costa Rica and Nicaragua. Here, we describe a number of observations encountered during this study using four examples that well document the precision, accuracy and general reliability of the 40Ar/39Ar ages. First, low K2O values, particularly in samples from Nicaragua, is a major limitation in or attempts to obtain reliable dates on samples under 1 My. Second, extensive weathering of samples due to the tropical climate of Central America has resulted in various levels of argon loss even when the hand sample appeared unaltered. Third, our field and geochronological data lead us to conclude that eruptive rates have not been constant over the past 15 to 20 My, but rather appears punctuated by gaps of up to several million years. We attempted to address the temporal gaps in several ways. First, geochemical analyses were used to identify samples that may have erupted during time periods without known volcanism. For example, U/Th values in the active Central American arc are significantly higher than those obtained from the Miocene Coyol Group except for four samples with intermediate values that were dated to determine if their ages were intermediate as well. However, all of these samples were found to be from a period with known volcanism. Second, we sought to locate the oldest sections of the active arc and the youngest sections of the Coyol Group in order to better constrain the timing and duration of the apparent gap in volcanic productivity. This approach also failed to locate samples from periods without known volcanism. When these methods proved largely unsuccessful, our focus shifted to dating regions of minor volcanism between the active and Coyol volcanic fronts as well as between Cosigüina and San Cristóbal, the longest stretch of the Central American Volcanic Front without active volcanism. This effort yielded ages on samples ranging from 1.1 to 3.6 Ma and, thus, substantially reduced the apparent volcanic gap in Nicaragua.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Con el principal objetivo de realizar mejores cálculos de la producción volcánica, en el Arco Volcánico de América Central, realizamos 61 dataciones 40Ar/39Ar en tefras y lavas en localidades de frente volcánico de Costa Rica y Nicaragua por medio de varias campañas de campo y análisis de laboratorio (preparación de muestras, envió al reactor nuclear, espectroscopía de masas de las muestras radiactivas, al laboratorio de gases nobles del Departamento de Ciencias de la Tierra y Planetarias de la Universidad Rutgers) del 2002-2008. En este artículo presentamos diferentes observaciones que resultaron de este estudio donde se describe la precisión, exactitud y la confiabilidad de las edades 40Ar/39Ar. El primer resultado muestra las limitaciones de esta técnica en muestras baja en K2O con edades < 1 Ma, especialmente en Nicaragua. El segundo resultado muestra los efectos de la pérdida de Ar por los procesos de meteorización típicos del trópico, inclusive afectando las muestras sanas a nivel críptico. El tercer resultado sugiere que las razones eruptivas del frente volcánico no han sido constantes durante los últimos 15-20 Ma, sino más bien representan ciclos eruptivos. Con el propósito de evaluar los hitos entre diferentes ciclos eruptivos, evaluamos los datos geoquímicos a lo largo del frente volcánico, en especial las relaciones U/Th, cuyos valores son inferiores (Grupo Coyol) en Nicaragua, comparados con el frente volcánico activo. Sin embargo, las muestras seleccionadas con base en geoquímica, resultaron ser de edades conocidas y no produjeron datos que llenan los hiatos entre ciclos de actividad volcánica. La siguiente estrategia que manejamos fue extender el muestreo en el Grupo Coyol, inmediatamente detrás del frente volcánico activo, sin embargo, esta estrategia no fue exitosa para encontrar muestras que llenaran los hiatos de actividad. No obstante, obtuvimos edades de 1.1-3,6 Ma entre los volcanes Cosiguina and San Cristóbal, los cuales limitan el hiato de actividad y mejoran nuestra percepción de los ciclos de actividad volcánica en América Central.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Central American Volcanic Front]]></kwd>
<kwd lng="en"><![CDATA[Geocrhonology]]></kwd>
<kwd lng="en"><![CDATA[40Ar/39Ar]]></kwd>
<kwd lng="es"><![CDATA[Frente Volcánico de América Central]]></kwd>
<kwd lng="es"><![CDATA[Geocronología]]></kwd>
<kwd lng="es"><![CDATA[40Ar/39Ar]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <div style="text-align: justify;">     <div style="text-align: center;"><font  style="font-family: verdana; font-weight: bold;" size="4">Progress and Challenges Using </font><font  style="font-family: verdana; font-weight: bold;" size="4"><sup>40</sup>Ar</font><font  style="font-family: verdana; font-weight: bold;" size="4">/<sup>39</sup>Ar Geochronology in Costa Rica and Nicaragua</font><br style="font-family: verdana; font-weight: bold;"> <br style="font-family: verdana; font-weight: bold;"> <font style="font-family: verdana; font-weight: bold;" size="4">Progreso y retos de la geocronolog&iacute;a <sup>40</sup>Ar/<sup>39</sup>Ar en Costa Rica y Nicaragua</font><br style="font-family: verdana; font-weight: bold;"> <br style="font-family: verdana; font-weight: bold;"> <font style="font-family: verdana;" size="2">Ian Saginor<sup><a  href="#1">1</a><a name="4"></a>*</sup>, Esteban Gazel<sup><a href="#2">2</a><a name="5"></a>*</sup>, Michael J. Carr<sup><a href="#3">3</a><a name="6"></a>*</sup>, Carl C. Swisher III<a href="#3"><sup>3</sup></a> &amp; Brent Turrin<a href="#3"><sup>3</sup></a></font><br  style="font-family: verdana;"> <font style="font-family: verdana;" size="2"><a  href="mailto:ian.saginor@keystone.edu"></a></font>    <br> </div> <font style="font-family: verdana;" size="2"><a name="correspondencia2"></a>*<a  href="#correspondencia1">Direcci&oacute;n de correspondencia</a></font><br style="font-family: verdana;"> </div> <hr  style="width: 100%; height: 2px; margin-left: 0px; margin-right: 0px;">     <div style="text-align: justify;"><font  style="font-family: verdana; font-weight: bold;" size="3">Abstract</font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">To better estimate the extrusive flux of the Central American Arc, from 2002-2008, we obtained sixty one high precision <sup>40</sup>Ar/<sup>39</sup>Ar ages on geographically well-situated lavas and tephra from Costa Rica and Nicaragua. Here, we describe a number of observations encountered during this study using four examples that well document the precision, accuracy and general reliability of the <sup>40</sup>Ar/<sup>39</sup>Ar ages. First, low K<sub>2</sub>O values, particularly in samples from Nicaragua, is a major limitation in or attempts to obtain reliable dates on samples under 1 My. Second, extensive weathering of samples due to the tropical climate of Central America has resulted in various levels of argon loss even when the hand sample appeared unaltered. Third, our field and geochronological data lead us to conclude that eruptive rates have not been constant over the past 15 to 20 My, but rather appears punctuated by gaps of up to several million years. We attempted to address the temporal gaps in several ways. First, geochemical analyses were used to identify samples that may have erupted during time periods without known volcanism. For example, U/Th values in the active Central American arc are significantly higher than those obtained from the Miocene Coyol Group except for four samples with intermediate values that were dated to determine if their ages were intermediate as well. However, all of these samples were found to be from a period with known volcanism. Second, we sought to locate the oldest sections of the active arc and the youngest sections of the Coyol Group in order to better constrain the timing and duration of the apparent gap in volcanic productivity. This approach also failed to locate samples from periods without known volcanism. When these methods proved largely unsuccessful, our focus shifted to dating regions of minor volcanism between the active and Coyol volcanic fronts as well as between Cosig&uuml;ina and San Crist&oacute;bal, the longest stretch of the Central American Volcanic Front without active volcanism. This effort yielded ages on samples ranging from 1.1 to 3.6 Ma and, thus, substantially reduced the apparent volcanic gap in Nicaragua.</font><br  style="font-family: verdana;"> <br style="font-family: verdana; font-weight: bold;"> <font style="font-family: verdana;" size="2"><span  style="font-weight: bold;">Keywords: </span>Central American Volcanic Front, Geocrhonology, </font><font style="font-family: verdana;"  size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font  style="font-family: verdana;" size="2"> </font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana; font-weight: bold;" size="3">Resumen</font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">Con el principal objetivo de realizar mejores c&aacute;lculos de la producci&oacute;n volc&aacute;nica, en el Arco Volc&aacute;nico de Am&eacute;rica Central, realizamos 61 dataciones </font><font  style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font  style="font-family: verdana;" size="2"> en tefras y lavas en localidades de frente volc&aacute;nico de Costa Rica y Nicaragua por medio de varias campa&ntilde;as de campo y an&aacute;lisis de laboratorio (preparaci&oacute;n de muestras, envi&oacute; al reactor nuclear, espectroscop&iacute;a de masas de las muestras radiactivas, al laboratorio de gases nobles del Departamento de Ciencias de la Tierra y Planetarias de la Universidad Rutgers) del 2002-2008. En este art&iacute;culo presentamos diferentes observaciones que resultaron de este estudio donde se describe la precisi&oacute;n, exactitud y la confiabilidad de las edades </font><font  style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font  style="font-family: verdana;" size="2">. El primer resultado muestra las limitaciones de esta t&eacute;cnica en muestras baja en K<sub>2</sub>O con edades &lt; 1 Ma, especialmente en Nicaragua. El segundo resultado muestra los efectos de la p&eacute;rdida de Ar por los procesos de meteorizaci&oacute;n t&iacute;picos del tr&oacute;pico, inclusive afectando las muestras sanas a nivel cr&iacute;ptico. El tercer resultado sugiere que las razones eruptivas del frente volc&aacute;nico no han sido constantes durante los &uacute;ltimos 15-20 Ma, sino m&aacute;s bien representan ciclos eruptivos. Con el prop&oacute;sito de evaluar los hitos entre diferentes ciclos eruptivos, evaluamos los datos geoqu&iacute;micos a lo largo del frente volc&aacute;nico, en especial las relaciones U/Th, cuyos valores son inferiores (Grupo Coyol) en Nicaragua, comparados con el frente volc&aacute;nico activo. Sin embargo, las muestras seleccionadas con base en geoqu&iacute;mica, resultaron ser de edades conocidas y no produjeron datos que llenan los hiatos entre ciclos de actividad volc&aacute;nica. La siguiente estrategia que manejamos fue extender el muestreo en el Grupo Coyol, inmediatamente detr&aacute;s del frente volc&aacute;nico activo, sin embargo, esta estrategia no fue exitosa para encontrar muestras que llenaran los hiatos de actividad. No obstante, obtuvimos edades de 1.1-3,6 Ma entre los volcanes Cosiguina and San Crist&oacute;bal, los cuales limitan el hiato de actividad y mejoran nuestra percepci&oacute;n de los ciclos de actividad volc&aacute;nica en Am&eacute;rica Central.</font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2"><span  style="font-weight: bold;">Palabras Clave: </span>Frente Volc&aacute;nico de Am&eacute;rica Central, Geocronolog&iacute;a, </font><font style="font-family: verdana;"  size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> </div> <hr  style="width: 100%; height: 2px; margin-left: 0px; margin-right: 0px;">     <div style="text-align: justify;"><font      style="font-family: verdana; font-weight: bold;" size="3">Introduction</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">The development of </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font     ]]></body>
<body><![CDATA[ style="font-family: verdana;" size="2"> dating methods made it     possible to obtain     high precision ages from a wide variety of igneous material.     Radiometric dates appear simple to interpret, but this accessibility     often leads to misunderstandings about how these dates are obtained and     even what geologic events in the rock&#8217;s history the dates refer to. It     is therefore important to be clear about what argon ages mean, how they     are derived, and what affects their reliability. </font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     ]]></body>
<body><![CDATA[<font style="font-family: verdana;" size="2">The basis of the </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2"> dating technique is a     modification of the     40K/40Ar dating method based on the decay of </font><font      style="font-family: verdana;" size="2"><sup>40</sup>K</font><font      style="font-family: verdana;" size="2"> to </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2"> with a     half-life of 1.26 Ga (Beckinsale and Gale, 1969). </font><br     ]]></body>
<body><![CDATA[ style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">The</font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2"> technique differs from the     40K/40Ar method in that the K     of a sample, is measured by conversion of</font><font      style="font-family: verdana;" size="2"> <sup>39</sup></font><font      style="font-family: verdana;" size="2">K to </font><font      style="font-family: verdana;" size="2"><sup>39</sup>Ar</font><font     ]]></body>
<body><![CDATA[ style="font-family: verdana;" size="2"> by neutron     bombardment in nuclear reactor. Since the ratio of&nbsp;</font><font      style="font-family: verdana;" size="2"> <sup>39</sup></font><font      style="font-family: verdana;" size="2">K</font><font      style="font-family: verdana;" size="2"> to </font><font      style="font-family: verdana;" size="2"><sup>40</sup>K</font><font      style="font-family: verdana;" size="2"> is known,     the derived </font><font style="font-family: verdana;" size="2"><sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2"> can be used as proxy for </font><font      style="font-family: verdana;" size="2"><sup>40</sup>K</font><font     ]]></body>
<body><![CDATA[ style="font-family: verdana;" size="2"> measurement (Merrihue and     Turner, 1966). This technique has an advantage over conventional K-Ar     dating, because both the radioactive parent </font><font      style="font-family: verdana;" size="2"><sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2"> and the daughter </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2">     can be measured by the same method, mass spectrometry, on the same     sample split at the same time. This permits the measurement of smaller     sample sizes (since splits are not needed for K and Ar measurement) and     ]]></body>
<body><![CDATA[reduces measurement errors associated with weighing and homogeneity.     Since these are now direct ratio measurements, not recombined yields     per sample weight, samples can be incrementally heated, yielding series     of relative increasing temperature ages that yield insight into the     thermal history of the sample. Likewise these data can be plotted on     isochron plots that give added information as to the initial argon     concentration of the sample at the time of cooling.</font><br      style="font-family: verdana;">     <font style="font-family: verdana;" size="2"></font><br      style="font-family: verdana;">     ]]></body>
<body><![CDATA[<font style="font-family: verdana;" size="2">The </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2"> technique can be applied to     any K-bearing igneous rock or     mineral phase that has not experienced extensive weathering or     reheating since its formation. Within each rock, </font><font      style="font-family: verdana;" size="2"><sup>40</sup>K</font><font      style="font-family: verdana;" size="2"> is perpetually     decaying, however </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2"> will not begin to accumulate     ]]></body>
<body><![CDATA[until the material     drops below its &#8220;blocking&#8221; temperature; the temperature below which     crystal structure is strong enough to block the diffusion of argon. </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2"> is a relatively large atom and     cannot escape the typical silicate     mineral crystal lattice unless the sample is reheated or physically     abraded. Once the mineral has cooled beneath its blocking temperature,     the &#8220;clock&#8221; begins and the daughter </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font     ]]></body>
<body><![CDATA[ style="font-family: verdana;" size="2"> accumulates. Blocking     temperatures vary for different minerals, with amphibole ~500&ordm;C     (Hanson and Gast, 1967), biotite ~400&ordm;C, and plagioclase     ~200&ordm;C (Berger and York, 1981). It is important to note that when     we refer to a </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2"> &#8220;age&#8221;, we are referring to     this moment in time     and not necessarily the formation age. For example, plutonic rocks can     remain above their blocking temperature for millions of years and     metamorphic rocks can have their radiometric clocks reset by subsequent     ]]></body>
<body><![CDATA[reheating, which means that the protolith of these rocks can form long     before the radiometric clock begins (Berger and York, 1981). In     contrast, extrusive volcanic rocks typically cool below their blocking     temperature soon after the time of eruption and can yield true     formation ages. All ages referred to in this paper are considered to be     eruption ages.</font><br style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">While 40Ar/39Ar dating is     an extremely useful tool, it is not without     its drawbacks, particularly in Central America and obtaining reliable     ]]></body>
<body><![CDATA[dates is dependant on a number of factors, each of which can affect the     reliability of the resulting age data.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana; font-weight: bold;" size="2">Radiogenic     Argon</font><br style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">Prior to the eruption of a     lava or tephra, the magma is generally well     above the blocking temperature of most K-bearing minerals, and normally     ]]></body>
<body><![CDATA[is in equilibration with the </font><font style="font-family: verdana;"      size="2"><sup>40</sup>Ar/<sup>36</sup>AR</font><font      style="font-family: verdana;" size="2"> ratio of the atmosphere     (295.5,     Steiger and Jager, 1977). All extrusive volcanic rocks therefore     contain some 40Ar at the time of formation, but 40Ar of radiogenic     origin (abbreviated </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2">*) only begins to accumulate     after they cool     below their blocking temperature. A reliable date can be obtained if     ]]></body>
<body><![CDATA[sufficient amounts of </font><font style="font-family: verdana;"      size="2"><sup>40</sup>Ar</font><font style="font-family: verdana;"      size="2">* accumulates to distinguish from </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2">     derived from equilibration with the atmosphere.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">The accumulation of </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font     ]]></body>
<body><![CDATA[ style="font-family: verdana;" size="2">* is controlled by two main     factors: The     initial potassium content of the sample and the elapsed time since it     dropped below the blocking temperature. A high potassium sample can     accumulate sufficient </font><font style="font-family: verdana;"      size="2"><sup>40</sup>Ar</font><font style="font-family: verdana;"      size="2">* to yield a reliable age in less time than a     low potassium sample. A problem arises however, when trying to date     young rocks with low potassium content, because there is very little </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font     ]]></body>
<body><![CDATA[ style="font-family: verdana;" size="2">* to measure.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">While potassium contents     of Central American arc basalts are comparable     to basalts from other arcs (generally between 0.5 and 2 wt.%, Luff,     1982; Marsh, 1982; Smith et al., 1980; Wills, 1974), there is     significant internal variability with central Costa Rican values almost     doubling those in northwest Nicaragua (<a      href="img/revistas/rgac/n45/a03i1.jpg">Figure 1</a>, Carr et al.,     ]]></body>
<body><![CDATA[2003).     Northwest Costa Rican samples are also higher on average than those     from Nicaragua, although there is significant overlap. </font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">Volcanic material as young     as a few thousand years has been     successfully dated using </font><font style="font-family: verdana;"      size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2"> dating techniques (Renne et     ]]></body>
<body><![CDATA[al.,     1997; Lanphere et al., 1999), but those samples had potassium levels at     least 10 times that of typical in Central America. It is likely the     combination of young age and low potassium content that makes dating     Nicaraguan volcanic front samples challenging. Thirty one Nicaraguan     volcanic front samples have been dated at the Rutgers University     Geochronology Lab and of those, only eight yielded reliable ages.     Thirty five Costa Rican volcanic front samples have been dated at the     Rutgers University Geochronology Lab and of those, thirty three yielded     reliable ages, a significantly higher percentage than the Nicaraguan     ]]></body>
<body><![CDATA[samples. Measuring K<sub>2</sub>O contents and selecting only those     samples with     the highest levels can help solve this problem.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">Weathering and     hydrothermal alteration can also be problematic for     argon geochronology of lavas, because both of these processes can cause     the release of </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2">* that has been building up     ]]></body>
<body><![CDATA[since the time of     eruption or differential K and Ar loss during weathering. This is     common in volcanic rocks, particularly in the tropical climate of     Central America, and often affects only the phases that crystallized at     the lowest temperatures as well as secondary phases, such as zeolites     that are the result of low temperature alteration or metamorphism     (<a href="img/revistas/rgac/n45/a03i2.jpg">Figure 2</a>; Ching-Hua et     al., 1994). Under certain conditions,     weathering and hydrothermal alteration can cause the release of all     pre-eruption </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font     ]]></body>
<body><![CDATA[ style="font-family: verdana;" size="2">*, even in samples less than     100 ka. For example, on     the southern flank of San Crist&oacute;bal, one smooth, lobe-shaped     lava was found (12.7315&ordm;N/87.0540&ordm;W) to be so hydrothermally     altered that it could be easily broken by hand. This sample was not     collected, but is a reminder of how quickly alteration can occur. Kis     often lost from glass phases during weathering and hydration.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">Another factor that can     ]]></body>
<body><![CDATA[cause unreliable dates is incomplete degassing     or trapping of pre-eruption 40Ar. When erupted lava is allowed to fully     equilibrate with the atmosphere, the initial ratio of </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2"> to <sup>36</sup>Ar will     be 295.5. However, if preeruption </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2"> is not allowed to degass, the     sample is said to have &#8220;excess&#8221; argon. This can be seen in an isochron     diagram of sample VE-071605-2 (<a href="img/revistas/rgac/n45/a03i2.jpg">Figure     ]]></body>
<body><![CDATA[2</a>), which is described later in     this paper.</font><br style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana; font-weight: bold;" size="3">Methods</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">Samples for 40Ar/39Ar     dating discussed here, were obtained from the     cores of large boulders or lava blocks collected from the study areas.     Samples were observed under binocular and petrographic microscopes and     ]]></body>
<body><![CDATA[those that showed clear evidence of weathering or alteration were     eliminated. For most samples, only the fine-grained matrix (composed     mainly of microlitic plagioclase) was analyzed, because its lack of     phenocrysts suggest that it was formed at the time of eruption.     Phenocrysts were removed through a combination of hand picking and     magnetic separation. A biotite mineral separate was analyzed for sample     C-06-NIC-2, a biotite rich tephra. Samples were prepared and analyzed     following methods outlined in Carr et al. (2007) and therefore it will     not be described in detail here.</font><br style="font-family: verdana;">     <br style="font-family: verdana;">     ]]></body>
<body><![CDATA[<font style="font-family: verdana;" size="2">It is worth noting that     all ages are based on either matrix or mineral     separates as opposed to whole rock analysis. The main difference is     that with the whole rock method, the entire sample is analyzed and may     include radiogenic argon from weathered phases, pre eruption     phenocrysts, or xenolithic contamination. By analyzing only the     fine-grained matrix, we minimize these factors and limit the     possibility of obtaining anomalously old ages. Even with this     precaution, it can be difficult to eliminate pre-eruption phases     entirely, particularly if they are small and of the same minerals that     ]]></body>
<body><![CDATA[make up the matrix. Low temperature alteration can also be difficult to     completely eliminate during sample preparation. </font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">For these reasons, samples     were incrementally heated with up to 15     increasing temperature steps and the released gases measured each time.     Each temperature step is based on an increase in laser power wattage     (typically between 2 and 32 watts) and those power limits have been     empirically determined to vary the temperature of the sample between     ]]></body>
<body><![CDATA[500&ordm;C and 1150&ordm;C. This method yielded the incremental heating     release spectra diagrams seen throughout this paper as opposed to total     fusion ages, which are generated by releasing trapped argon with a     single high temperature step. Total fusion analysis includes the     radiogenic argon component of the entire sample in a single measurement     and can mask internal variability and evidence of weathering and     xenolithic contamination. Release spectra diagrams plot the apparent     age of each individual temperature step, which may or may not be the     same throughout the sample. Ideally, apparent ages from consecutive     temperature steps representing at least 50% of the total </font><font     ]]></body>
<body><![CDATA[ style="font-family: verdana;" size="2"><sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2"> would     form an age plateau at the 95% confidence level. Typically, the plateau     age (if there is one) is reported along with the integrated age, which     is simply the weighted average of each individual temperature step and     is essentially the same as a total fusion age.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">The incremental-heating     method is also beneficial because multiple     ]]></body>
<body><![CDATA[steps can be plotted on an inverse isochron diagram (examples in <a      href="img/revistas/rgac/n45/a03i2.jpg">Figure     2</a>). In this type of diagram, </font><font      style="font-family: verdana;" size="2"><sup><sub>36</sub></sup>Ar/<sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2"> is plotted against </font><font      style="font-family: verdana;" size="2"><sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2">/</font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2"> In     an ideal sample, the individual temperature steps plot along a single     ]]></body>
<body><![CDATA[line, such that the slope provides the age and the y-intercept provides     the initial <sup><sub>36</sub></sup>Ar/<sup>40</sup>Ar value.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana; font-weight: bold;" size="2">Case     Studies</font><br style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">The first sample case     study is RO-4 (<a href="img/revistas/rgac/n45/a03i2.jpg">Figure 2A</a>),     a lava collected from     ]]></body>
<body><![CDATA[Rota Volcano in Nicaragua (Figure 5, Carr et al., 2007). RO-4&#8217;s     extremely low radiogenic argon yields (&#8211;1.1 to 1.9%) is typical of     Nicaraguan active front lavas. Negative values simply reflect the fact     that the error exceeds the amount of the measured gas. This can be     clearly seen in the first temperature step, which accounts for     approximately 30% of the total released </font><font      style="font-family: verdana;" size="2"><sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2">, yet the apparent age is     below 0. The low </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2">* yield is most likely due to     ]]></body>
<body><![CDATA[its relatively young     age (the present Nicaraguan front is no more than 350 ka, Carr et al.,     2007) rather than it&#8217;s potassium content, which at 1.22 wt.% (Carr et     al., 2003), is one of the highest in Nicaragua. Although evidence of     weathering was not detected in hand sample or thin section, due to the     sample&#8217;s location in a tropical climate and proximity to active     volcanism (and therefore sources of hydrothermal activity),     low-temperature alteration cannot be entirely ruled out. In addition,     the apparent age seems to increase in the last 5 temperature steps,     which could suggest that radiogenic argon was released only at the     ]]></body>
<body><![CDATA[lower temperature phases. This sample is considered not to have yielded     a reliable date and is included here only to illustrate the difficulty     in evaluating the age of a sample when the radiogenic argon yield is     low.</font><br style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">In the absence of a     reliable plateau, how should this data be     interpreted? The isochron yields a negative age and an atmospheric     initial </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>36</sup>Ar</font><font      style="font-family: verdana;" size="2">, so we can conclude that there     ]]></body>
<body><![CDATA[is simply too little     radiogenic argon to obtain a reliable age. In the absence of clear     evidence of chemical or physical alteration, we can simply conclude     that the sample is of very recent age, or more precisely, that the     sample&#8217;s age is indistinguishable from 0.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">The next sample case study     is CR-TE-04- 8b (<a href="img/revistas/rgac/n45/a03i2.jpg">Figure 2B</a>),     a lava     ]]></body>
<body><![CDATA[collected from Tenorio Volcano along the Costa Rican volcanic front     (<a href="img/revistas/rgac/n45/a03i3.jpg">Figure 3</a>, Carr et al.,     2007). All temperature steps form a 0.369     &plusmn; 0.012 Ma plateau at the 95% confidence level and the </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2">*     yields range from 4 to 16%. The isochron age agrees with the plateau     age within the margin of error at 0.39 &plusmn; 0.03 Ma and the initial     </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>36</sup>Ar</font><font      style="font-family: verdana;" size="2"> ratio is within the range of     ]]></body>
<body><![CDATA[atmospheric values at 294     &plusmn; 3. In addition, the mean squared weighted deviation (MSWD) of     the individual steps is only 0.47, which means that the errors fully     account for the scatter about the isochron line. The large plateau and     the high </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2">* yield (relative to Nicaraguan     volcanic front samples) is     consistent with the majority of other Costa Rican samples. For all of     these reasons,this is considered to be an excellent example of a     reliable age in contrast to the previous sample RO-4.</font><br     ]]></body>
<body><![CDATA[ style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">The third case study is a     pillow basalt from Isla Venado off Costa     Rica&#8217;s Nicoya Peninsula (VE-07165-2; <a      href="img/revistas/rgac/n45/a03i2.jpg">Figure 2C</a>). This sample is     overlain by a unit of reworked volcaniclastic sediments that was dated     using biostratigraphy to 100 m.y.. This sample had an initial </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>36</sup>Ar</font><font      style="font-family: verdana;" size="2">     ]]></body>
<body><![CDATA[ratio of 326 &plusmn; 14, higher than atmospheric ratios and evidence     of excess argon and is likely due to its submarine eruption, which     prevented complete degassing and equilibration with the atmosphere. The     release spectra (<a href="img/revistas/rgac/n45/a03i2.jpg">Figure 2C</a>)     show the individual temperature steps     falling from 105 Ma to 45 Ma throughout the analysis. Not only does     this sample lack a plateau, but the isochron is also problematic with a     mean squared weighted deviation of 14, well above the variation     accounted for by the errors. One could attempt to refit the isochron     with a different line by including only the high temperature steps that     ]]></body>
<body><![CDATA[appear to be approaching a plateau. This approach would increase the     age and the initial </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>36</sup>Ar</font><font      style="font-family: verdana;" size="2"> ratio, but we believe that     would be over     interpreting very low-quality data. Although a reliable age cannot be     obtained from this sample, the high initial </font><font      style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>36</sup>Ar</font><font      style="font-family: verdana;" size="2"> ratio suggests     that it the age is probably much younger than the &gt;100 Ma estimate     based on field data. This may simply mean that the contact between the     ]]></body>
<body><![CDATA[pillow basalts and the overlying unit is a thrust fault and not     depositional, however further fieldwork is needed to make this     determination. Given the glassy nature of pillow basalts, the spectra     may also reflect K-loss during hydrothermal alteration. It may also be     that the formation is a pillow dike and not a lava flow.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">The last sample case study     is C-51 (<a href="img/revistas/rgac/n45/a03i2.jpg">Figure 2D</a>), a     lava collected from a     ]]></body>
<body><![CDATA[low lying area between the volcanic front volcanoes of Cosig&uuml;ina     and San Crist&oacute;bal in northwest Nicaragua. This sample has a     plateau age of 3.59 &plusmn; 0.03 in agreement with an isochron age of     3.54 &plusmn; 0.05. These ages were first reported in Carr et al.     (2007) and are included here as an example of how low degrees of     weathering or alteration can affect the release spectra of a sample.     Although, the plateau includes 98% of the total released </font><font      style="font-family: verdana;" size="2"><sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2">, the     first temperature step is not included and is almost 2 Ma younger than     ]]></body>
<body><![CDATA[the rest of the plateau. This is common even in samples with robust     ages and is evidence of low-temperature alteration, which releases     radiogenic argon trapped in low-temperature phases within the lava.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana; font-weight: bold;" size="2">Volcanic     History</font><br style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">Previous geochronological     work in Nicaragua (Ehrenborg, 1996; Elming et     ]]></body>
<body><![CDATA[al., 2001; Plank et al., 2002, Carr et al., 2007, Saginor et al., 2011)     suggest that the NW/SE trending Coyol Arc migrated steadily toward the     southwest until ~7 Ma when volcanic production abruptly ceased. The     Coyol volcanic front lasted from 25 Ma to 7 Ma (Plank et al., 2002) and     consists of extensive lavas and ignimbrites throughout the Nicaraguan     Highlands. Volcanism wouldn&#8217;t resume until 3.6 Ma and then only between     Cosig&uuml;ina and San Crist&oacute;bal (Carr et al., 2007, Saginor et     al., 2011). Several attempts were made aimed at filling in this missing     period in the volcanic record. </font><br style="font-family: verdana;">     <br style="font-family: verdana;">     ]]></body>
<body><![CDATA[<font style="font-family: verdana;" size="2">First, U/Th values in     Nicaraguan volcanics experienced a significant     increase between the Miocene and present arc (<a      href="img/revistas/rgac/n45/a03i3.jpg">Figure 3</a>, Plank et al.,     2002), however there were three samples thought to be Miocene that had     U/Th values between those typical for the Miocene and active arcs.     These samples were selected for dating, because their intermediate U/Th     values raised the possibility that their ages were intermediate as     well. Sample LL-4 is from the Las Lajas volcano just east of the     Nicaraguan depression and samples Bal-8 and Bal-10 are from the Balsamo     ]]></body>
<body><![CDATA[Formation in El Salvador. LL-4 was found to be 9.5 Ma, which places it     firmly within the Coyol Group (Carr et al., 2007). Samples Bal-8 and     Bal-10 were found to be older than the active volcanic front and     yielded ages of 1.3 and 1.1 Ma, respectively.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">Second, an attempt was     made to constrain both the timing and duration     of this apparent hiatus in Nicaraguan volcanism by refining estimates     for the youngest material within the Coyol Group as well as the oldest     ]]></body>
<body><![CDATA[sections of the active arc. For the latter task, satellite images     (https://zulu.ssc.nasa.gov/mrsid/) and topographic maps were used to     identify areas within the active arc where the morphology suggested the     oldest material could be found.</font><br style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font      style="font-family: verdana;" size="2"> ages obtained using this     method were reported in Carr et al.     (2007), with a maximum age of 330 ka. Plank et al. (2002) suggested     that Miocene volcanism in Nicaragua ceased ~7 Ma after the Coyol     ]]></body>
<body><![CDATA[volcanic front migrated towards the southwest for at least 5 m.y. In an     effort to locate Coyol volcanics younger than 7 Ma, fieldwork was     focused between the active arc and the westernmost Coyol lavas (<a      href="img/revistas/rgac/n45/a03i4.jpg">Figure     4</a>, Carr et al., 2007). </font><br style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">This approach extended the     geographic distribution of the Coyol Group     ~10 km into the Nicaraguan Depression, although did not extend its     temporal range. Two samples were found in this area with ages of 1.13     ]]></body>
<body><![CDATA[and 1.48, which places them in the Tinajas unit as defined in Saginor     et al. (Saginor et al., 2011). </font><br style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">We also collected samples     between Cosig&uuml;ina and San     Crist&oacute;bal, the longest stretch of the volcanic front without an     active volcano. This effort revealed two previously unknown volcanic     units: The Tinajas (2.5-1.3 Ma) and the Encanto (3.6-3.2 Ma). Both of     these are described in Saginor et al. (2011). These two units also     decreased the duration of the temporal gap in Nicaragua, leaving only     ]]></body>
<body><![CDATA[3.4 Ma (7 to 3.6 Ma) without known volcanism.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana; font-weight: bold;" size="3">Acknowledgements</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">The authors acknowledge     revisions and comments by Dr Guillermo Alvarado     and the editorial work of Dr. Percy Denyer. This work was partially     supported through the NSF Margins Program, grants EAR0203388 and NSF     ]]></body>
<body><![CDATA[OCE 0505924 to MC.</font><br style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana; font-weight: bold;" size="3">Conclusions</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">Samples from the     Nicaraguan volcanic front are generally lower in K<sub>2</sub>O     than samples from the Costa Rican front. In addition, the front may be     slightly younger in Nicaragua than Costa Rica. These two factors make     obtaining reliable Nicaraguan </font><font     ]]></body>
<body><![CDATA[ style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>49</sup>Ar</font><font      style="font-family: verdana;" size="2"> ages difficult because it     leads     to lower </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar</font><font      style="font-family: verdana;" size="2">* yields.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     <font style="font-family: verdana;" size="2">The volcanic history in     Nicaragua is incomplete and several attempts     have been made to locate samples that fill in these temporal gaps.     ]]></body>
<body><![CDATA[First, samples with U/Th values between the Miocene and active volcanic     fronts were analyzed to see if their ages were intermediate as well.     Second, satellite imagery was used to direct fieldwork toward the most     weathered sections of the active Nicaraguan volcanoes and to a     topographic low just behind the active front. Third, volcanic material     was collected between Cosig&uuml;ina and San Crist&oacute;bal, the     longest stretch of the volcanic front without an active volcano. These     efforts decreased the duration of the temporal gap in Nicaragua to     about 3.4 Ma, which lasted from 7 to 3.6 Ma. It is also important that     detailed geologic maps of northwest Nicaragua be developed to fully     ]]></body>
<body><![CDATA[understand the volcanic history of the region.</font><br      style="font-family: verdana;">     <br style="font-family: verdana;">     </div>     <hr      style="width: 100%; height: 2px; margin-left: 0px; margin-right: 0px;">     <!-- ref --><div style="text-align: justify;"><font  style="font-family: verdana; font-weight: bold;" size="3">References</font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">BECKINSALE, R.D., &amp; GALE, N.H. 1969: A reappraisal of the decay constants and branching ratio of <sup>40</sup>K.- Earth Plan. Sci. Lett. 6: 289-294.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031567&pid=S0256-7024201100020000300001&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">BERGER, G.W., &amp; YORK, D. 1981: Geothermometry from </font><font style="font-family: verdana;"  size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font  style="font-family: verdana;" size="2"> dating experiments.- Geochim. Cosmochim. Acta. 45: 795-811.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031568&pid=S0256-7024201100020000300002&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">CARR, M.J., FEIGENSON, M.D., PATINO, L.C., &amp; WALKER, J.A. 2003: Volcanism and geochemistry in Central America: progress and problem.- In Eiler, J. &amp; G. Abers (Eds): Inside the Subduction Factory.- AGU Geophysical Monograph 138: 153-179.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031569&pid=S0256-7024201100020000300003&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">CARR, M.J., SAGINOR, I., ALVARADO, G.E., BOLGE, L.L., LINDSAY, F.N., MILLIDAKIS, K., TURRIN, B.D., FEIGENSON, M.D., &amp; SWISHER III, C.C. 2007: Element fluxes from the volcanic front of Nicaragua and Costa Rica.- Geochem. Geophysics Geosystems. 8(6): 1525-2027.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031570&pid=S0256-7024201100020000300004&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">CHING-HUA, L., ONSTOTT, T.C., CHIANGHWA C., &amp; TPHOON, L. 1994: An assessment of </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font  style="font-family: verdana;" size="2"> dating for the whole- rock volcanic samples from the Luzon Arc near Taiwan.- Chem. Geol. 114(1-2): 157-178.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031571&pid=S0256-7024201100020000300005&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">CONDIE, C. 2005: Continuity (Ba) and change (U) in Central American geochemistry: New evidence from the Miocene Balsamo Formation in El Salvador.- Rutgers University [Tesis Maestr&iacute;a].    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031572&pid=S0256-7024201100020000300006&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">EHRENBORG, J. 1996: A new stratigraphy for the Tertiary volcanic rocks of the Nicaraguan highland.- Geol. Soc. Am. Bull. 108: 830- 842.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031573&pid=S0256-7024201100020000300007&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">ELMING, S.A., LAYER, P., &amp; UBIETA, K. 2001: A paleomagnetic study of Tertiary rocks in Nicaragua, Central America.- Geophys. J. Int. 147: 294-309.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031574&pid=S0256-7024201100020000300008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">HANSON, G.N., &amp; GAST, P.W. 1967: Kinetic studies in contact metamorphic zones.- Geochim. Cosmochim. Acta, 31: 1119- 1153.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031575&pid=S0256-7024201100020000300009&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">LANPHERE, M. 2000: Comparison of conventional K&#8211;Ar and </font><font  style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font  style="font-family: verdana;" size="2"> dating of young mafic volcanic rocks.- Quat. Res. 53(3): 294-301.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031576&pid=S0256-7024201100020000300010&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">LUFF, I.W. 1982: Petrogenesis of the island arc tholeiite series of the South Sandwich Islands.- University of Leeds, U.K. Tesis Doc.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031577&pid=S0256-7024201100020000300011&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">MARSH, B.D. 1982: The Aleutians. In Andesites: Orogenic andesites and related rocks.-R.S. Thorpe (ed.), Chichester, Wiley: 99-114.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031578&pid=S0256-7024201100020000300012&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">MERRIHUE, C., &amp; TURNER, G. 1966: Potassium-Argon dating by activation with fast neutrons.- J. Geophys. Res. 71: 2852-2857.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031579&pid=S0256-7024201100020000300013&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">PECERILLO, R., &amp; TAYLOR, S.R. 1976: Geochemistry of Eocene calc-alkaline rocks from the Kastamonu Area, northern Turkey.- Contrib. Min. Pet. 58: 63-81.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031580&pid=S0256-7024201100020000300014&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">PLANK, T., BALZER, V., &amp; CARR, M.J. 2002: Nicaraguan volcanoes record paleoceanographic changes accompanying closure of the Panama Gateway.- Geol. 30: 1087-1090.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031581&pid=S0256-7024201100020000300015&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">RENNE, P.R., SHARP, W.D., DEINO, A.L., ORSI, G., &amp; CIVETTA, L. 1997: </font><font style="font-family: verdana;" size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font  style="font-family: verdana;" size="2"> dating into the historical realm: Calibration against Pliny the Younger.- Science, 277: 1279-1280.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031582&pid=S0256-7024201100020000300016&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">SAGINOR, I, GAZEL, E., CARR, M., SWISHER, C., &amp; TURRIN, B. 2011: New Pliocene&#8211; Pleistocene </font><font style="font-family: verdana;"  size="2"><sup>40</sup>Ar/<sup>39</sup>Ar</font><font  style="font-family: verdana;" size="2"> ages fill in temporal gaps in the Nicaraguan volcanic record.- J. Volc. Geothermal Res. 202: 143-152.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031583&pid=S0256-7024201100020000300017&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">STEIGER, R.H., &amp; JAGER, E. 1977: Subcommision on geochronology: Convention on the use of decay constants.-Earth Plan. Sci. Lett. 36: 359-362.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031584&pid=S0256-7024201100020000300018&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">SMITH, A.L., ROOBAL, M.J., &amp; GUNN, B.M. 1980: The Lesser Antilles &#8211; A discussion of the Island arc magmatism.- Bull. Volc. 43: 287-302.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031585&pid=S0256-7024201100020000300019&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --></font><br  style="font-family: verdana;"> <br style="font-family: verdana;"> <font style="font-family: verdana;" size="2">WILLS, J.K. 1974: The geological history of southern Dominica, and plutonic nodules from the Lesser Antilles.- University of Durham, U.K. Tesis Doc.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=1031586&pid=S0256-7024201100020000300020&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --> </font>    <br>     <br> <font style="font-family: verdana;" size="2"><a name="correspondencia1"></a><a  href="#correspondencia2">*</a>Correspondencia: </font><font style="font-family: verdana;" size="2">Ian Saginor: </font><font  style="font-family: verdana;" size="2">Keystone College, Natural Sciences and Mathematics, One College Green, La Plume, PA 18440. </font><small><span style="font-family: verdana;">Autor para contacto: <a href="mailto:ian.saginor@keystone.edu">ian.saginor@keystone.edu</a></span></small>    <br> <font style="font-family: verdana;" size="2">Esteban Gazel: </font><font  style="font-family: verdana;" size="2">Virginia Tech, Department of Geological Sciences, 4044 Derring Hall (0420), Blacksburg, VA 24061</font>    ]]></body>
<body><![CDATA[<br> <font style="font-family: verdana;" size="2">Michael J. Carr: </font><font  style="font-family: verdana;" size="2">Rutgers University, Department of Geological Sciences, 610 Taylor Rd., Piscataway NJ 08854</font>    <br> <font style="font-family: verdana;" size="2">Carl C. Swisher III: </font><font style="font-family: verdana;" size="2">Rutgers University, Department of Geological Sciences, 610 Taylor Rd., Piscataway NJ 08854</font>    <br> <font style="font-family: verdana;" size="2">Brent Turrin: </font><font  style="font-family: verdana;" size="2">Rutgers University, Department of Geological Sciences, 610 Taylor Rd., Piscataway NJ 08854    <br>     <br> </font><font style="font-family: verdana;" size="2"><sup><a name="1"></a><a  href="#4">1</a></sup>Keystone College, Natural Sciences and Mathematics, One College Green, La Plume, PA 18440</font><br style="font-family: verdana;"> <font style="font-family: verdana;" size="2"><sup><a name="2"></a><a  href="#5">2</a></sup>Virginia Tech, Department of Geological Sciences, 4044 Derring Hall (0420), Blacksburg, VA 24061</font><br style="font-family: verdana;"> <font style="font-family: verdana;" size="2"><sup><a name="3"></a><a  href="#6">3</a></sup>Rutgers University, Department of Geological Sciences, 610 Taylor Rd., Piscataway NJ 08854</font><br style="font-family: verdana;"> <font style="font-family: verdana;" size="2"><sup>*</sup>Autor para contacto: <a href="mailto:ian.saginor@keystone.edu">ian.saginor@keystone.edu</a></font>    <br> <font style="font-family: verdana;" size="2"></font> </div> <hr  style="width: 100%; height: 2px; margin-left: 0px; margin-right: 0px;">     <div style="text-align: center;"><font  style="font-family: verdana; font-weight: bold;" size="2">(Recibido: 16/07/2011; aceptado: 28/11/2011)</font>    <br> </div>      ]]></body><back>
<ref-list>
<ref id="B1">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[BECKINSALE]]></surname>
<given-names><![CDATA[R.D]]></given-names>
</name>
<name>
<surname><![CDATA[GALE]]></surname>
<given-names><![CDATA[N.H]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[A reappraisal of the decay constants and branching ratio of 40K]]></article-title>
<source><![CDATA[Earth Plan. Sci. Lett]]></source>
<year>1969</year>
<volume>6</volume>
<page-range>289-294</page-range></nlm-citation>
</ref>
<ref id="B2">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[BERGER]]></surname>
<given-names><![CDATA[G.W]]></given-names>
</name>
<name>
<surname><![CDATA[YORK]]></surname>
<given-names><![CDATA[D]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Geothermometry from 40Ar/39Ar dating experiments]]></article-title>
<source><![CDATA[Geochim. Cosmochim. Acta.]]></source>
<year>1981</year>
<volume>45</volume>
<page-range>795-811</page-range></nlm-citation>
</ref>
<ref id="B3">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[CARR]]></surname>
<given-names><![CDATA[M.J]]></given-names>
</name>
<name>
<surname><![CDATA[FEIGENSON]]></surname>
<given-names><![CDATA[M.D]]></given-names>
</name>
<name>
<surname><![CDATA[PATINO]]></surname>
<given-names><![CDATA[L.C]]></given-names>
</name>
<name>
<surname><![CDATA[WALKER]]></surname>
<given-names><![CDATA[J.A]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Volcanism and geochemistry in Central America: progress and problem]]></article-title>
<person-group person-group-type="editor">
<name>
<surname><![CDATA[Eiler]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
<name>
<surname><![CDATA[Abers]]></surname>
<given-names><![CDATA[G]]></given-names>
</name>
</person-group>
<source><![CDATA[AGU Geophysical MonographInside the Subduction Factory]]></source>
<year>2003</year>
<volume>138</volume>
<page-range>153-179</page-range></nlm-citation>
</ref>
<ref id="B4">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[CARR]]></surname>
<given-names><![CDATA[M.J]]></given-names>
</name>
<name>
<surname><![CDATA[SAGINOR]]></surname>
<given-names><![CDATA[I]]></given-names>
</name>
<name>
<surname><![CDATA[ALVARADO]]></surname>
<given-names><![CDATA[G.E]]></given-names>
</name>
<name>
<surname><![CDATA[BOLGE]]></surname>
<given-names><![CDATA[L.L]]></given-names>
</name>
<name>
<surname><![CDATA[LINDSAY]]></surname>
<given-names><![CDATA[F.N]]></given-names>
</name>
<name>
<surname><![CDATA[MILLIDAKIS]]></surname>
<given-names><![CDATA[K]]></given-names>
</name>
<name>
<surname><![CDATA[TURRIN]]></surname>
<given-names><![CDATA[B.D]]></given-names>
</name>
<name>
<surname><![CDATA[FEIGENSON]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[SWISHER III]]></surname>
<given-names><![CDATA[C.C]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Element fluxes from the volcanic front of Nicaragua and Costa Rica]]></article-title>
<source><![CDATA[Geochem. Geophysics Geosystems]]></source>
<year>2007</year>
<volume>8</volume>
<numero>6</numero>
<issue>6</issue>
<page-range>1525-2027</page-range></nlm-citation>
</ref>
<ref id="B5">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[CHING-HUA]]></surname>
<given-names><![CDATA[L]]></given-names>
</name>
<name>
<surname><![CDATA[ONSTOTT]]></surname>
<given-names><![CDATA[T.C.]]></given-names>
</name>
<name>
<surname><![CDATA[CHIANGHWA]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
<name>
<surname><![CDATA[TPHOON]]></surname>
<given-names><![CDATA[L]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[An assessment of 40Ar/39Ar dating for the whole- rock volcanic samples from the Luzon Arc near Taiwan]]></article-title>
<source><![CDATA[Chem. Geol.]]></source>
<year>1994</year>
<volume>114</volume>
<numero>1-2</numero>
<issue>1-2</issue>
<page-range>157-178</page-range></nlm-citation>
</ref>
<ref id="B6">
<nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[CONDIE]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
</person-group>
<source><![CDATA[Continuity (Ba) and change (U) in Central American geochemistry: New evidence from the Miocene Balsamo Formation in El Salvador]]></source>
<year>2005</year>
</nlm-citation>
</ref>
<ref id="B7">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[EHRENBORG]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[A new stratigraphy for the Tertiary volcanic rocks of the Nicaraguan highland]]></article-title>
<source><![CDATA[Geol. Soc. Am. Bull.]]></source>
<year>1996</year>
<volume>108</volume>
<page-range>830- 842</page-range></nlm-citation>
</ref>
<ref id="B8">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[ELMING]]></surname>
<given-names><![CDATA[S.A]]></given-names>
</name>
<name>
<surname><![CDATA[LAYER]]></surname>
<given-names><![CDATA[P]]></given-names>
</name>
<name>
<surname><![CDATA[UBIETA]]></surname>
<given-names><![CDATA[K]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[A paleomagnetic study of Tertiary rocks in Nicaragua, Central America]]></article-title>
<source><![CDATA[Geophys. J. Int]]></source>
<year>2001</year>
<volume>147</volume>
<page-range>294-309</page-range></nlm-citation>
</ref>
<ref id="B9">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[HANSON]]></surname>
<given-names><![CDATA[G.N]]></given-names>
</name>
<name>
<surname><![CDATA[GAST]]></surname>
<given-names><![CDATA[P.W]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Kinetic studies in contact metamorphic zones]]></article-title>
<source><![CDATA[Geochim. Cosmochim. Acta]]></source>
<year>1967</year>
<volume>31</volume>
<page-range>1119- 1153</page-range></nlm-citation>
</ref>
<ref id="B10">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[LANPHERE]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Comparison of conventional K-Ar and 40Ar/39Ar dating of young mafic volcanic rocks]]></article-title>
<source><![CDATA[Quat. Res.]]></source>
<year>2000</year>
<volume>53</volume>
<numero>3</numero>
<issue>3</issue>
<page-range>294-301</page-range></nlm-citation>
</ref>
<ref id="B11">
<nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[LUFF]]></surname>
<given-names><![CDATA[I.W]]></given-names>
</name>
</person-group>
<source><![CDATA[Petrogenesis of the island arc tholeiite series of the South Sandwich Islands]]></source>
<year>1982</year>
</nlm-citation>
</ref>
<ref id="B12">
<nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[MARSH]]></surname>
<given-names><![CDATA[B.D]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[The Aleutians]]></article-title>
<person-group person-group-type="editor">
<name>
<surname><![CDATA[Thorpe]]></surname>
<given-names><![CDATA[R.S]]></given-names>
</name>
</person-group>
<source><![CDATA[Andesites: Orogenic andesites and related rocks]]></source>
<year>1982</year>
<page-range>99-114</page-range><publisher-loc><![CDATA[Chichester^eWiley Wiley]]></publisher-loc>
</nlm-citation>
</ref>
<ref id="B13">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[MERRIHUE]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
<name>
<surname><![CDATA[TURNER]]></surname>
<given-names><![CDATA[G]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Potassium-Argon dating by activation with fast neutrons]]></article-title>
<source><![CDATA[J. Geophys. Res.]]></source>
<year>1966</year>
<volume>71</volume>
<page-range>2852-2857</page-range></nlm-citation>
</ref>
<ref id="B14">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[PECERILLO]]></surname>
<given-names><![CDATA[R]]></given-names>
</name>
<name>
<surname><![CDATA[TAYLOR]]></surname>
<given-names><![CDATA[S.R]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Geochemistry of Eocene calc-alkaline rocks from the Kastamonu Area, northern Turkey]]></article-title>
<source><![CDATA[Contrib. Min. Pet]]></source>
<year>1976</year>
<volume>58</volume>
<numero>63-81</numero>
<issue>63-81</issue>
</nlm-citation>
</ref>
<ref id="B15">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[PLANK]]></surname>
<given-names><![CDATA[T]]></given-names>
</name>
<name>
<surname><![CDATA[BALZER]]></surname>
<given-names><![CDATA[V]]></given-names>
</name>
<name>
<surname><![CDATA[CARR]]></surname>
<given-names><![CDATA[M.J]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Nicaraguan volcanoes record paleoceanographic changes accompanying closure of the Panama Gateway]]></article-title>
<source><![CDATA[Geol.]]></source>
<year>2002</year>
<volume>30</volume>
<page-range>1087-1090</page-range></nlm-citation>
</ref>
<ref id="B16">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[RENNE]]></surname>
<given-names><![CDATA[P.R]]></given-names>
</name>
<name>
<surname><![CDATA[SHARP]]></surname>
<given-names><![CDATA[W.D]]></given-names>
</name>
<name>
<surname><![CDATA[DEINO]]></surname>
<given-names><![CDATA[A.L]]></given-names>
</name>
<name>
<surname><![CDATA[ORSI]]></surname>
<given-names><![CDATA[G]]></given-names>
</name>
<name>
<surname><![CDATA[CIVETTA]]></surname>
<given-names><![CDATA[L]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[40Ar/39Ar dating into the historical realm: Calibration against Pliny the Younger]]></article-title>
<source><![CDATA[Science]]></source>
<year>1997</year>
<volume>277</volume>
<page-range>1279-1280</page-range></nlm-citation>
</ref>
<ref id="B17">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[SAGINOR]]></surname>
<given-names><![CDATA[I]]></given-names>
</name>
<name>
<surname><![CDATA[GAZEL]]></surname>
<given-names><![CDATA[E]]></given-names>
</name>
<name>
<surname><![CDATA[CARR]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
<name>
<surname><![CDATA[SWISHER]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
<name>
<surname><![CDATA[TURRIN]]></surname>
<given-names><![CDATA[B]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[New Pliocene- Pleistocene 40Ar/39Ar ages fill in temporal gaps in the Nicaraguan volcanic record]]></article-title>
<source><![CDATA[J. Volc. Geothermal Res]]></source>
<year>2011</year>
<volume>202</volume>
<page-range>143-152</page-range></nlm-citation>
</ref>
<ref id="B18">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[STEIGER]]></surname>
<given-names><![CDATA[R.H]]></given-names>
</name>
<name>
<surname><![CDATA[JAGER]]></surname>
<given-names><![CDATA[E]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Subcommision on geochronology: Convention on the use of decay constants]]></article-title>
<source><![CDATA[Earth Plan. Sci. Lett]]></source>
<year>1977</year>
<volume>36</volume>
<page-range>359-362</page-range></nlm-citation>
</ref>
<ref id="B19">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[SMITH]]></surname>
<given-names><![CDATA[A.L]]></given-names>
</name>
<name>
<surname><![CDATA[ROOBAL]]></surname>
<given-names><![CDATA[M.J]]></given-names>
</name>
<name>
<surname><![CDATA[GUNN]]></surname>
<given-names><![CDATA[B.M.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[The Lesser Antilles: A discussion of the Island arc magmatism]]></article-title>
<source><![CDATA[Bull. Volc.]]></source>
<year>1980</year>
<volume>43</volume>
<page-range>287-302</page-range></nlm-citation>
</ref>
<ref id="B20">
<nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[WILLS]]></surname>
<given-names><![CDATA[J.K]]></given-names>
</name>
</person-group>
<source><![CDATA[The geological history of southern Dominica, and plutonic nodules from the Lesser Antilles]]></source>
<year>1974</year>
</nlm-citation>
</ref>
</ref-list>
</back>
</article>
