2.2.6
spase://CNES/SimulationRun/CDPP-AMDA/TAO/Juno
Tao Model
SW propagated from Earth to Juno
2014-07-08T14:48:29Z
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
spase://CNES/Person/Chihiro.Tao
PrincipalInvestigator
spase://CDPP/SimulationModel/AMDA/Tao
Juno
Cartesian
RTN
2
AU
Density
Proton
Velocity
Proton
Magnetic Field
Magnetic