<?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>0016-7169</journal-id>
<journal-title><![CDATA[Geofísica internacional]]></journal-title>
<abbrev-journal-title><![CDATA[Geofís. Intl]]></abbrev-journal-title>
<issn>0016-7169</issn>
<publisher>
<publisher-name><![CDATA[Universidad Nacional Autónoma de México, Instituto de Geofísica]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0016-71692016000100069</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[The Mexican Meteor Network: A Preliminary Proposal]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Cordero-Tercero]]></surname>
<given-names><![CDATA[Guadalupe]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Velázquez-Villegas]]></surname>
<given-names><![CDATA[Fernando]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Vázquez-Hernández]]></surname>
<given-names><![CDATA[Carlos Francisco]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Ramírez-Cruz]]></surname>
<given-names><![CDATA[José Luis]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Arévalo-Vieyra]]></surname>
<given-names><![CDATA[Alejandro]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Mendoza-San-Agustín]]></surname>
<given-names><![CDATA[Asahel]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Camacho-Martínez]]></surname>
<given-names><![CDATA[Fernando]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
</contrib-group>
<aff id="Af1">
<institution><![CDATA[,Universidad Nacional Autónoma de México Instituto de Geofísica Departamento de Ciencias Espaciales]]></institution>
<addr-line><![CDATA[México D.F.]]></addr-line>
<country>Mexico</country>
</aff>
<aff id="Af2">
<institution><![CDATA[,Universidad Nacional Autónoma de México Centro de Ingeniería Avanzada ]]></institution>
<addr-line><![CDATA[México D.F.]]></addr-line>
<country>Mexico</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>03</month>
<year>2016</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>03</month>
<year>2016</year>
</pub-date>
<volume>55</volume>
<numero>1</numero>
<fpage>69</fpage>
<lpage>77</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0016-71692016000100069&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0016-71692016000100069&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0016-71692016000100069&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[Abstract: The study of asteroidal and cometary material entering into Earth's atmosphere has scientific and social importance. The observation and study of the impact of meteoroids with our planet is a way of studying geophysics and planetary geology without spaceships. This article describes the progress of the installation of the Mexican Meteor Network (Citlalin Tlamina). At medium and long term, the aim of this network is to cover the entire national territory with stations that allow us to record the entry of meteoroids into Earth's atmosphere. This seeks to: a) study the meteoroid-atmosphere interaction, b) determine impactor's physical properties; c) analyze flows and Radiant deviations of known meteor showers, d) find or ratify new meteor showers; e) recover and study meteorites, f) study the interaction of the shock wave with the ground by analyzing seismograms; g) report people in real time (or near) the occurrence of fireballs and fragmentation of meteoroids in the atmosphere, avoiding the fear of this phenomenon and provide support for Civil Protection, h) find areas of opportunity that can use the images captured by the cameras (weather, bird migration, etc.). In this paper, it is shown the prototype of the base to house the cameras whose purpose is to protect them from the environment, prevent condensation within the container and keep the cameras below 25 °C.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Resumen: El estudio de la entrada a la atmósfera terrestre de material asteroidal y cometario tiene importancia científica y social. La observación y estudio del impacto de meteoroides con nuestro planeta es una forma de estudiar geofísica y geología planetarias sin naves espaciales. En este artículo se muestran los avances de la instalación de la Red Mexicana de Meteoros (Citlalin Tlamina) cuyo objetivo, a mediano y largo plazo, es poder cubrir todo el territorio nacional con estaciones que nos permitan registrar la entrada de meteoroides a la atmósfera terrestre. Con esto se busca: a) estudiar en detalle la interacción meteoroideatmósfera, b) determinar propiedades físicas de los impactores; c) analizar flujos y desviaciones del radiante de las lluvias de estrellas conocidas, d) encontrar o ratificar nuevas lluvias de estrellas; e) recuperar y estudiar meteoritas, f) estudiar la interacción de la onda de choque con el suelo mediante el análisis de sismogramas; g) informar en tiempo real (o casi) a las personas la ocurrencia de bólidos y fragmentación de meteoroides en la atmósfera, evitando el miedo hacia este tipo de fenómenos y servir de apoyo a Protección Civil y h) encontrar áreas de oportunidad que puedan hacer uso de las imágenes captadas por las cámaras (meteorología, migración de aves, etc.). En este trabajo se muestra el prototipo de la base que albergará las cámaras y cuyo propósito es protegerlas del medio ambiente, evitar la condensación dentro de los contenedores de las cámaras y mantenerlas a una temperatura inferior a los 25 °C.v.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[meteor]]></kwd>
<kwd lng="en"><![CDATA[meteorite]]></kwd>
<kwd lng="en"><![CDATA[meteoroid]]></kwd>
<kwd lng="en"><![CDATA[small bodies]]></kwd>
<kwd lng="en"><![CDATA[video network]]></kwd>
<kwd lng="en"><![CDATA[Civil Protection]]></kwd>
<kwd lng="es"><![CDATA[meteoro]]></kwd>
<kwd lng="es"><![CDATA[meteorita]]></kwd>
<kwd lng="es"><![CDATA[meteoroide]]></kwd>
<kwd lng="es"><![CDATA[cuerpos pequeños]]></kwd>
<kwd lng="es"><![CDATA[red de cámaras]]></kwd>
<kwd lng="es"><![CDATA[Protección Civil]]></kwd>
</kwd-group>
</article-meta>
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