2.2.6 spase://CNES/NumericalOutput/CDPP-AMDA/TAO/Venus/tao-venus-dsc SW / Input DSCOVR Tao SW Venus / Input DSCOVR 2017-07-08T16:49:29Z DSCOVR FC solar wind 1-min data is used as model input. Calculation : IRAP. TBD spase://CNES/Person/Chihiro.Tao PrincipalInvestigator spase://CNES/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/CNES/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://CNES/SimulationRun/CDPP-AMDA/TAO/Venus ThermalPlasma 1990-01-01T01:00:00Z 2018-11-14T00:00:00Z PT1H Venus Note an important parameter - angle Venus-Sun-Earth - which could be considered as quality flag. spase://CDPP/NumericalData/AMDA/DSCOVR/FC/dsc-fc-1m density venus_dsc_n Solar Wind Proton Number Density, scalar cm^-3 NaN Proton NumberDensity velocity venus_dsc_v Solar Wind Bulk Speed km/s 3 V r Component.I 1 venus_dsc_v(0) V t Component.J 2 venus_dsc_v(1) NaN Proton Velocity temperature venus_dsc_t eV NaN Proton Temperature dynamic pressure venus_dsc_pdyn nPa NaN Proton Pressure b tangential venus_dsc_b nT NaN Magnetic angle Venus-Sun-Earth venus_dsc_da deg NaN Positional