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SimulationRun/CDPP-AMDA/TAO/Mercury.xml 2.61 KB
dbc930ab   Elena.Budnik   redmine #7309
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<?xml version="1.0" encoding="UTF-8"?>
7e407638   Elena.Budnik   schema locally
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<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">
dbc930ab   Elena.Budnik   redmine #7309
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 <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>
            <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.
4acd80ba   Elena.Budnik   TAO : rm 6427 and...
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		    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> 
dbc930ab   Elena.Budnik   redmine #7309
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            <Contact>
                <PersonID>spase://CNES/Person/Chihiro.Tao</PersonID>
                <Role>PrincipalInvestigator</Role>
            </Contact>           
        </ResourceHeader>
        <Model>
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            <ModelID>spase://CNES/SimulationModel/CDPP-AMDA/Tao</ModelID>
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        </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>
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            <Name>Tangential Field Component</Name>
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            <Property>
                <PropertyQuantity>Magnetic</PropertyQuantity>
            </Property>
        </InputParameter>
    </SimulationRun>
</Spase>