<?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>0035-001X</journal-id>
<journal-title><![CDATA[Revista mexicana de física]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. mex. fis.]]></abbrev-journal-title>
<issn>0035-001X</issn>
<publisher>
<publisher-name><![CDATA[Sociedad Mexicana de Física]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0035-001X2009000600006</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Monte Carlo simulations of drop growth by coalescence and collision-induced breakup]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Alfonso]]></surname>
<given-names><![CDATA[L.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Raga]]></surname>
<given-names><![CDATA[G.B.]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Baumgardner]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad Autónoma de la Ciudad de México  ]]></institution>
<addr-line><![CDATA[Mexico ]]></addr-line>
<country>México</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Universidad Nacional Autónoma de México Centro de Ciencias de la Atmósfera ]]></institution>
<addr-line><![CDATA[Mexico ]]></addr-line>
<country>México</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>12</month>
<year>2009</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>12</month>
<year>2009</year>
</pub-date>
<volume>55</volume>
<numero>6</numero>
<fpage>437</fpage>
<lpage>442</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2009000600006&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2009000600006&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2009000600006&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[A Monte Carlo framework to simulate the evolution of drop spectra by coalescence and collision-induced breakup is presented. The stochastic algorithm of Gillespie [1] for chemical reactions in the formulation proposed by Laurenzi and Diamond [2] was used to simulate the kinetic behavior of the drop population. Within Gillespie's framework, the collision-induced breakup process is modeled as a new "chemical reaction". The results of the Monte Carlo simulations were compared with the analytical solution to the collection-breakup equation obtained by Feingold et. al. [3], for an exponential distribution of satellite drops, and a constant collection and breakup kernels. A good correspondence between the analytical and the stochastic algorithm was found for this case.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Se presenta un algoritmo de Monte Carlo para simular la evolución del espectro de gotas por coalescencia y rompimiento inducido por colisiones. El algoritmo estocástico de Gillespie [1] para las reacciones químicas en la formulación propuesta por Laurenzi y Diamond [2] fue utilizado para simular la cinética de la población de gotas. El rompimiento inducido por colisiones es modelado en el formalismo de Gillespie [1] como una nueva "reacción química". Los resultados fueron comparados con la solución analítica para la ecuación de rompimiento encontrada por Feingold et. al. [3] para una distribución exponencial de las gotas satélites, y kernels de colección y rompimiento constantes. Se encontró una buena correspondencia entre la solución analítica y el algoritmo estocástico para este caso.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Cloud microphysics]]></kwd>
<kwd lng="en"><![CDATA[Monte Carlo simulation]]></kwd>
<kwd lng="en"><![CDATA[breakup process]]></kwd>
<kwd lng="es"><![CDATA[Microfísica de nubes]]></kwd>
<kwd lng="es"><![CDATA[simulación de Monte Carlo]]></kwd>
<kwd lng="es"><![CDATA[proceso de rompimiento]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="justify"><font face="verdana" size="4">Investigaci&oacute;n</font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="4"><b>Monte Carlo simulations of drop growth by coalescence and collision&#150;induced breakup</b></font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>L. Alfonso &ordf;, G.B. Raga<sup> b</sup> and D. Baumgardner <sup>b</sup></b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><i>&ordf; Universidad Aut&oacute;noma de la Ciudad de M&eacute;xico, Mexico City, 09790 M&eacute;xico, </i>e&#150;mail: <a href="mailto:esterson@yahoo.com">lesterson@yahoo.com</a></font></p>     <p align="justify"><font face="verdana" size="2"><i><sup>b</sup> Centro de Ciencias de la Atm&oacute;sfera, Universidad Nacional Aut&oacute;noma de M&eacute;xico, Mexico City, 04510, M&eacute;xico.</i></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Recibido el 7 de mayo de 2009    ]]></body>
<body><![CDATA[<br>   Aceptado el 29 de septiembre de 2009</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">A Monte Carlo framework to simulate the evolution of drop spectra by coalescence and collision&#150;induced breakup is presented. The stochastic algorithm of Gillespie &#91;1&#93; for chemical reactions in the formulation proposed by Laurenzi and Diamond &#91;2&#93; was used to simulate the kinetic behavior of the drop population. Within Gillespie's framework, the collision&#150;induced breakup process is modeled as a new "chemical reaction". The results of the Monte Carlo simulations were compared with the analytical solution to the collection&#150;breakup equation obtained by Feingold <i>et. al. </i>&#91;3&#93;, for an exponential distribution of satellite drops, and a constant collection and breakup kernels. A good correspondence between the analytical and the stochastic algorithm was found for this case.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Keywords:</b>  Cloud microphysics; Monte Carlo simulation; breakup process.</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>     <p align="justify"><font face="verdana" size="2">Se presenta un algoritmo de Monte Carlo para simular la evoluci&oacute;n del espectro de gotas por coalescencia y rompimiento inducido por colisiones. El algoritmo estoc&aacute;stico de Gillespie &#91;1&#93; para las reacciones qu&iacute;micas en la formulaci&oacute;n propuesta por Laurenzi y Diamond &#91;2&#93; fue utilizado para simular la cin&eacute;tica de la poblaci&oacute;n de gotas. El rompimiento inducido por colisiones es modelado en el formalismo de Gillespie &#91;1&#93; como una nueva "reacci&oacute;n qu&iacute;mica". Los resultados fueron comparados con la soluci&oacute;n anal&iacute;tica para la ecuaci&oacute;n de rompimiento encontrada por Feingold <i>et. al. </i>&#91;3&#93; para una distribuci&oacute;n exponencial de las gotas sat&eacute;lites, y kernels de colecci&oacute;n y rompimiento constantes. Se encontr&oacute; una buena correspondencia entre la soluci&oacute;n anal&iacute;tica y el algoritmo estoc&aacute;stico para este caso.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Descriptores:</b>  Microf&iacute;sica de nubes; simulaci&oacute;n de Monte Carlo; proceso de rompimiento.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2">PACS: 92.60.N; 92.60.Nv</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><a href="/pdf/rmf/v55n6/v55n6a6.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>References</b></font></p>     <!-- ref --><p align="justify"><font face="verdana" size="2">1. D.T. Gillespie, <i>J. Comput. Phys. </i><b>22</b> (1976) 403.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8357547&pid=S0035-001X200900060000600001&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">2. I.J. Laurenzi and S.L. Diamond, <i>Phys. Rev. E. </i><b>67</b> (2003) 051103.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8357548&pid=S0035-001X200900060000600002&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">3. G. Feingold, S. Tzivion, and Z. Levin, <i>J. Atmos. Sci. </i><b>45</b> (1988) 3387.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8357549&pid=S0035-001X200900060000600003&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">4. D.T. Gillespie, <i>J. Atmos. Sci. </i><b>32</b> (1975) 1977.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8357550&pid=S0035-001X200900060000600004&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">5. R. List and J.R. Gillespie, <i>J. Atmos. Sci. </i><b>33</b> (1976) 2007.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8357551&pid=S0035-001X200900060000600005&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">6. I.J. Laurenzi, L. Scott, and S.L. Diamond,<i> Biophys. J.</i><b> 77</b> (1999) 1733.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8357552&pid=S0035-001X200900060000600006&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">7. I.J. Laurenzi, S.L. Bartels, and S.L. Diamond, <i>J. Comput. Phys. </i><b>177</b> (2002) 418.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8357553&pid=S0035-001X200900060000600007&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">8. T.B. Low and R. List, <i>J. Atmos .Sci. </i><b>39</b> (1982) 1607</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8357554&pid=S0035-001X200900060000600008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">9. W.T. Scott, J. <i>Atoms. Sci. </i><b>25</b> (1968) 54.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8357555&pid=S0035-001X200900060000600009&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">10. A.M. Golovin, <i>Bull. Acad. Sci. USSR, Geophys. Ser. </i><b>5</b> (1963) 482.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8357556&pid=S0035-001X200900060000600010&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --> ]]></body><back>
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