2.2.6 spase://CDPP/NumericalOutput/AMDA/TAO/Jupiter/tao-jup-dsc SW / Input DSCOVR Tao SW Jupiter / Input DSCOVR 2017-07-08T16:49:29Z DSCOVR FC solar wind 1-min data is used as model input. Calculation : IRAP. TBD spase://CDPP/Person/Chihiro.Tao PrincipalInvestigator spase://CDPP/Person/Elena.Budnik TechnicalContact Model Description http://www.astro.phys.s.chiba-u.ac.jp/netlab/astro/index2-e.html Model Article http://onlinelibrary.wiley.com/doi/10.1029/2004JA010959/abstract spase://SMWG/Repository/CDPP/AMDA Online Open AMDA at CDPP http://amda.cdpp.eu Text.ASCII AMDA is a science analysis system provided by the Centre de Donnees de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Universite Paul Sabatier, Toulouse spase://CDPP/SimulationRun/AMDA/TAO/Jupiter ThermalPlasma 1990-01-01T01:00:00Z 2018-11-14T00:00:00Z PT1H Jupiter Note an important parameter - angle Jup-Sun-Earth - which could be considered as quality flag. spase://CDPP/NumericalData/AMDA/DSCOVR/FC/dsc-fc-1m density jup_dsc_n Solar Wind Proton Number Density, scalar cm^-3 NaN Proton NumberDensity velocity jup_dsc_v Solar Wind Bulk Speed km/s 3 V r Component.I 1 jup_dsc_v(0) V t Component.J 2 jup_dsc_v(1) NaN Proton Velocity temperature jup_dsc_t eV NaN Proton Temperature dynamic pressure jup_dsc_pdyn nPa NaN Proton Pressure b tangential jup_dsc_b nT NaN Magnetic angle Jup-Sun-Earth jup_dsc_da NaN Positional