<?xml version="1.0" encoding="UTF-8"?>
<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema  http://www.spase-group.org/data/simulation/schema/spase-sim-1_0_0.xsd" xmlns="http://www.spase-group.org/data/schema">
    <Version>2.2.6</Version>
    <SimulationModel>
        <ResourceID>spase://CNES/SimulationModel/CDPP-AMDA/Tao</ResourceID>
        <ResourceHeader>
            <ResourceName>Tao SW propagation Model</ResourceName>
            <ReleaseDate>2014-07-08T14:48:29Z</ReleaseDate>
            <Description>1D MHD Model. The model code is based on the Coordinated Astronomical Numerical Software (CANS) by JSTModel details, evaluations compared with observation data, and limitations are described in Tao et al. 2005, J. Geophys. Res., 110, A11208, doi:10.1029/2004JA010959</Description>
            <Contact>
                <PersonID>spase://CNES/Person/Chihiro.Tao</PersonID>
                <Role>PrincipalInvestigator</Role>
            </Contact>
           <Association>
               <AssociationID>SW_Propagation_Model</AssociationID>
               <AssociationType>PartOf</AssociationType>
               <Note>Solar Wind Propagation Models</Note>
           </Association>
        </ResourceHeader> 
        <SimulationType>MHD</SimulationType>        
    </SimulationModel>
</Spase>