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📄 lorenz.xmds

📁 XMDS is a code generator that integrates equations. You write them down in human readable form in a
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<?xml version="1.0"?><!-- Example simulation: lorenz --><!-- $Id: lorenz.xmds,v 1.8 2004/07/14 06:37:05 joehope Exp $ --><!--  Copyright (C) 2000-2004                                           --><!--                                                                    --><!--  Code contributed by Greg Collecutt, Joseph Hope and Paul Cochrane --><!--                                                                    --><!--  This file is part of xmds.                                        --><!--                                                                    --><!--  This program is free software; you can redistribute it and/or     --><!--  modify it under the terms of the GNU General Public License       --><!--  as published by the Free Software Foundation; either version 2    --><!--  of the License, or (at your option) any later version.            --><!--                                                                    --><!--  This program is distributed in the hope that it will be useful,   --><!--  but WITHOUT ANY WARRANTY; without even the implied warranty of    --><!--  MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the     --><!--  GNU General Public License for more details.                      --><!--                                                                    --><!--  You should have received a copy of the GNU General Public License --><!--  along with this program; if not, write to the Free Software       --><!--  Foundation, Inc., 59 Temple Place - Suite 330, Boston,            --><!--  MA  02111-1307, USA.                                              --><!-- Adapted from the example in "Numerical methods for physics"--><!-- by Alejandro L. Garcia, pg 78--><!-- Try the simulation for different values of xo, yo and zo --><!-- e.g.: xo = 1, yo = 1, zo = 20 --><!-- Note: this simulation can be run as a shell/Perl/Python script by --><!-- changing the values of xo, yo and zo using the command line arguments --><simulation>  <name>lorenz</name>  <author>Paul Cochrane</author>  <description>    Lorenz attractor example simulation.  Adapted from the example in    "Numerical methods for physics" by Alejandro L. Garcia, page 78.  </description>  <!-- Global system parameters and functionality -->  <prop_dim>t</prop_dim>  <stochastic>no</stochastic>  <!-- Global variables for the simulation -->  <globals>    <![CDATA[    const double sigma = 10.0;    const double b = 8.0/3.0;    const double r = 28.0;    ]]>  </globals>  <!-- Command line arguments -->  <argv>    <arg>      <name>xo</name>      <type>double</type>      <default_value>1.0</default_value>    </arg>    <arg>      <name>yo</name>      <type>double</type>      <default_value>1.0</default_value>    </arg>    <arg>      <name>zo</name>      <type>double</type>      <default_value>1.0</default_value>    </arg>  </argv>  <!-- Field to be integrated over -->  <field>    <samples>1</samples>    <vector>      <name>main</name>      <type>double</type>      <components>x y z</components>      <filename> lorenzInput.dat </filename>      <!-- <![CDATA[        x = xo;        y = yo;	z = zo;      ]]> -->    </vector>  </field>  <!-- The sequence of integrations to perform -->  <sequence>    <integrate>      <algorithm>RK4EX</algorithm>      <interval>15.0</interval>      <lattice>5000</lattice>      <samples>50</samples>      <![CDATA[        dx_dt = sigma*(y - x);        dy_dt = r*x - y - x*z;	dz_dt = x*y - b*z;      ]]>    </integrate>  </sequence>  <!-- The output to generate -->  <output format="ascii" precision="double">    <group>      <sampling>        <moments>xOut yOut zOut</moments>          xOut = x;	  yOut = y;	  zOut = z;      </sampling>    </group>  </output></simulation>

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