<?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://amda.irap.omp.eu/public/schemas/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>
            <Acknowledgement>These datasets have been derived and provided by the Planetary Space Weather Services (PSWS) Virtual Activity of the Europlanet H2020 Research Infrastructure funded by the European Union's Horizon 2020 research and innovation programme under grant agreement No 654208, and by the Sun Planet Interactions Digital Environment on Request (SPIDER) Virtual Activity of the Europlanet 2024 Research Infrastucture funded by the European Union's Horizon 2020 research and innovation programme under grant agreement No 871149. http://spider-europlanet.irap.omp.eu/</Acknowledgement>
            <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>