Neptune.xml
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<?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/Neptune</ResourceID>
<ResourceHeader>
<ResourceName>Tao Model</ResourceName>
<AlternateName>SW propagated from Earth to Neptune</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.
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 = nep_input_b*nep_input_v(0)*1000./(2*pi/25.38/86400)/(2.5*Rsun-r_nep*AU)</Description>
<Contact>
<PersonID>spase://CNES/Person/Chihiro.Tao</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
</ResourceHeader>
<Model>
<ModelID>spase://CNES/SimulationModel/CDPP-AMDA/Tao</ModelID>
</Model>
<SimulatedRegion>Neptune</SimulatedRegion>
<Caveats>The solar wind model does not include the additional contributions of the interaction between the solar wind and the neutral hydrogen of the
local interstellar medium, which becomes non-negligible in the outer heliosphere (beyond 10 AU) (see detail in Appendix A2 in Lamy et al., 2017JGR).
https://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2017JA023918
</Caveats>
<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>