<?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>0185-1101</journal-id>
<journal-title><![CDATA[Revista mexicana de astronomía y astrofísica]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. mex. astron. astrofis]]></abbrev-journal-title>
<issn>0185-1101</issn>
<publisher>
<publisher-name><![CDATA[Universidad Nacional Autónoma de México, Instituto de Astronomía]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0185-11012010000100009</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[The green potential of the San Pedro Mártir observatory]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Bohigas]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Núñez]]></surname>
<given-names><![CDATA[J. M.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad Nacional Autónoma de México Instituto de Astronomía ]]></institution>
<addr-line><![CDATA[Ensenada B. C.]]></addr-line>
<country>México</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>04</month>
<year>2010</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>04</month>
<year>2010</year>
</pub-date>
<volume>46</volume>
<numero>1</numero>
<fpage>89</fpage>
<lpage>107</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0185-11012010000100009&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0185-11012010000100009&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0185-11012010000100009&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[Se analizan observaciones meteorológicas realizadas entre octubre 2004 y julio 2008 en el Observatorio Astronómico Nacional de México (OAN). En abril, mayo y junio la humedad fue inferior a 55% casi 90% del tiempo. La velocidad del viento fue mayor durante la noche y disminuyó entre marzo y noviembre. Las variaciones nocturnas, diarias y anuales de temperatura fueron cercanas a 2, 6 y 16°C, respectivamente. La altura de escala para la función que relaciona la velocidad del viento con la altura sobre el suelo está entre 0.55 y 0.67 metros. La operación normal del OAN produjo algo más que 750 toneladas de CO<img border=0 src="../../../../../img/revistas/rmaa/v46n1/a9s1.jpg"> al año, unas 3 veces más que las emitidas por una industria mediana típica del municipio de Ensenada, donde está ubicado el OAN. La energía eólica pudo ser utilizada para producir electricidad &#126; 60% del tiempo, siendo más abundante durante la noche y en los meses de invierno y primavera temprana. La energía solar y eólica parece bastar para cubrir todas las necesidades energéticas del observatorio, cerca de 110 kWh, incluyendo transporte.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[Weather observations carried out between October 2004 and July 2008 at the Mexican Observatorio Astronómico Nacional (OAN) are analyzed. Humidity in April, May and June was less than 55% nearly 90% of the time. Wind speed was larger at nightime and tended to decrease between March and November. Typical temperature variations during the night, for the entire day and for a whole year were about 2, 6 and 16° C, respectively. The scale height or roughness length for the function relating wind speed and height above ground is between 0.55 and 0.67 meters. Normal activities associated to OAN produced somewhat more than 750 tons of CO<img border=0 src="../../../../../img/revistas/rmaa/v46n1/a9s1.jpg"> a year, roughly 3 times more than a typical mid-scale industry in the district of Ensenada, where OAN is located. Wind energy could have been extracted to produce electricity &#126; 60% of the time, being more bountiful during the night and in the winter and early spring months. Solar and wind energy seem plentiful enough to supply the entire energy needs of the observatory, some 110 kWh including transportation.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[seeing]]></kwd>
<kwd lng="en"><![CDATA[site testing]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="center"><font face="verdana" size="4"><b>The green potential of the San Pedro M&aacute;rtir observatory</b></font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>J. Bohigas<sup>1</sup> and J. M. N&uacute;&ntilde;ez<sup>1</sup> </b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><i><sup>1</sup> Instituto de Astronom&iacute;a, Universidad Nacional Aut&oacute;noma de M&eacute;xico, Apdo. Postal 877, 22800 Ensenada, B. C., M&eacute;xico. (<a href="mailto:jbb@astrosen.unam.mx">jbb@astrosen.unam.mx</a>, <a href="mailto:jnunez@astrosen.unam.mx">jnunez@astrosen.unam.mx</a>).</i></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Received 2009 September 17    <br> Accepted 2009 November 23</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>RESUMEN</b></font></p>     ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2">Se analizan observaciones meteorol&oacute;gicas realizadas entre octubre 2004 y julio 2008 en el Observatorio Astron&oacute;mico Nacional de M&eacute;xico (OAN). En abril, mayo y junio la humedad fue inferior a 55% casi 90% del tiempo. La velocidad del viento fue mayor durante la noche y disminuy&oacute; entre marzo y noviembre. Las variaciones nocturnas, diarias y anuales de temperatura fueron cercanas a 2, 6 y 16&deg;C, respectivamente. La altura de escala para la funci&oacute;n que relaciona la velocidad del viento con la altura sobre el suelo est&aacute; entre 0.55 y 0.67 metros. La operaci&oacute;n normal del OAN produjo algo m&aacute;s que 750 toneladas de CO<img src="/img/revistas/rmaa/v46n1/a9s1.jpg"> al a&ntilde;o, unas 3 veces m&aacute;s que las emitidas por una industria mediana t&iacute;pica del municipio de Ensenada, donde est&aacute; ubicado el OAN. La energ&iacute;a e&oacute;lica pudo ser utilizada para producir electricidad &#126; 60% del tiempo, siendo m&aacute;s abundante durante la noche y en los meses de invierno y primavera temprana. La energ&iacute;a solar y e&oacute;lica parece bastar para cubrir todas las necesidades energ&eacute;ticas del observatorio, cerca de 110 kWh, incluyendo transporte.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>ABSTRACT</b></font></p>     <p align="justify"><font face="verdana" size="2">Weather observations carried out between October 2004 and July 2008 at the Mexican Observatorio Astron&oacute;mico Nacional (OAN) are analyzed. Humidity in April, May and June was less than 55% nearly 90% of the time. Wind speed was larger at nightime and tended to decrease between March and November. Typical temperature variations during the night, for the entire day and for a whole year were about 2, 6 and 16&deg; C, respectively. The scale height or roughness length for the function relating wind speed and height above ground is between 0.55 and 0.67 meters. Normal activities associated to OAN produced somewhat more than 750 tons of CO<img src="/img/revistas/rmaa/v46n1/a9s1.jpg"> a year, roughly 3 times more than a typical mid&#150;scale industry in the district of Ensenada, where OAN is located. Wind energy could have been extracted to produce electricity &#126; 60% of the time, being more bountiful during the night and in the winter and early spring months. Solar and wind energy seem plentiful enough to supply the entire energy needs of the observatory, some 110 kWh including transportation.</font></p>     <p align="justify"><font face="verdana" size="2"><b><i>Key Words: </i></b>seeing &#151; site testing.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><a href="/pdf/rmaa/v46n1/v46n1a9.pdf" target="_blank">DESCARGAR ART&Iacute;CULO EN FORMATO PDF</a></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>ACKNOWLEDGMENTS</b></font></p>     <p align="justify"><font face="verdana" size="2">This paper would have been impossible without the dedication, professionalism and generosity of the TMT and LSST site testing teams. We appreciate the cooperation of the technical and administrative staff of OAN, and in particular the labor of Tom&aacute;s Calvario, Osiris Escoboza, Francisco Guill&eacute;n and Francisco Lazo. Josu&eacute; Carlos Avelar, Desiderio Carrasco and Marco Mostalac assisted us with valuable information regarding energy use at OAN. We also thank Dr. Thomas Schlatter for his guidance regarding water vapor saturation pressure algorithms. The paper was benefited by comments and suggestions made by an anonymous referee. Support from DGAPA&#150;Universidad Nacional Aut&oacute;noma de M&eacute;xico project IN102607&#150;3 is gratefully acknowledged.</font></p>     ]]></body>
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