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           <title>DRIFT-PHOENIX models</title>
           <shortName>DRIFT-PHOENIX</shortName>
           <identifier>ivo://svo.cab/models/drift</identifier>
           <curation>
              <publisher ivo-id="ivo://svo.cab">SVO CAB</publisher>
              <creator>
                 <name>Woitke P., Helling C., 2003, A&amp;A, 399, 297</name>
              </creator>
              <version>1.0</version>
              <contact>
                 <name>Enrique Solano, LAEFF Archive Support Team</name>
                 <email>esm@cab.inta-csic.es</email>
              </contact>
           </curation>
           <content>
              <subject>star</subject>
              <description>Drift-Phoenix is a computer code that simulates the structure of an atmosphere including the formation of clouds. The code is part of the Phoenix-code family. Drift describes the formation of mineral clouds and allows to predict cloud details, like the size of the cloud particles and their composition.</description>
              <source>http://adsabs.harvard.edu/abs/2003A%26A...399..297W</source>
              <referenceURL>http://svo.cab.inta-csic.es/</referenceURL>
              <type>Simulation</type>
              <contentLevel>Research</contentLevel>
           </content>
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