<?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>
    <SimulationRun>
        <ResourceID>spase://CNES/SimulationRun/CDPP-AMDA/TAO/Mercury</ResourceID>
        <ResourceHeader>
            <ResourceName>Tao Model</ResourceName>
            <AlternateName>SW propagated from Earth to Mercury</AlternateName>

            <DOI>https://doi.org/10.6096/2009</DOI>

            <ReleaseDate>2014-07-08T14:48:29Z</ReleaseDate>
            <Description>These data sets are the simulation outputs of solar wind variations observed near the Earth and propagated to the different destinations using a 1-dimensional 2-component (radial and azimuthal) magnetohydrodynamic (MHD) model.The model code is based on the Coordinated Astronomical Numerical Software (CANS) by JST.

		    Model details, evaluations compared with observation data, and limitations are described in Tao et al. 2005, J. Geophys. Res., 110, A11208, doi:10.1029/2004JA010959 
		    
		    The radial magnetic field along parker spirals is computed using :  
		    
		    br = mercury_input_b*mercury_input_v(0)*1000./(2*pi/25.38/86400)/(2.5*Rsun-r_mercury*AU)</Description> 

            <Contact>

                <PersonID>spase://CNES/Person/CDPP-AMDA/Chihiro.Tao</PersonID>

                <Role>PrincipalInvestigator</Role>
            </Contact>           
        </ResourceHeader>
        <Model>

            <ModelID>spase://CNES/SimulationModel/CDPP-AMDA/Tao</ModelID>

        </Model> 
        <SimulatedRegion>Mercury</SimulatedRegion>        
        <SimulationDomain>
            <CoordinateSystem>
                <CoordinateRepresentation>Cartesian</CoordinateRepresentation>
                <CoordinateSystemName>RTN</CoordinateSystemName>
            </CoordinateSystem>            
            <SpatialDimension>2</SpatialDimension>
            <Units>AU</Units>
        </SimulationDomain>
        <InputParameter>
            <Name>Density</Name>
            <Property>
                <PropertyQuantity>Proton</PropertyQuantity>
            </Property>
        </InputParameter>
        <InputParameter>
            <Name>Velocity</Name>
            <Property>
                <PropertyQuantity>Proton</PropertyQuantity>
            </Property>
        </InputParameter>
        <InputParameter>

            <Name>Tangential Field Component</Name>

            <Property>
                <PropertyQuantity>Magnetic</PropertyQuantity>
            </Property>
        </InputParameter>
    </SimulationRun>
</Spase>