2.2.6 spase://CNES/NumericalOutput/CDPP-AMDA/TAO/Cassini/tao-cass-sw SW / Input OMNI Tao SW Cassini / Input OMNI : Cruise Phase 2019-08-30T09:39:04Z OMNI solar wind 1-hour data is used as model input. Calculation : IRAP. TBD spase://CNES/Person/CDPP-AMDA/Chihiro.Tao PrincipalInvestigator spase://SMWG/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 CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi tao-cass-sw Web Service to this product using the HAPI interface. CSV Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA Web application https://amda.cdpp.eu Access to Data via CDPP/AMDA Web application. CSV VOTable CDF PNG Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. spase://CNES/SimulationRun/CDPP-AMDA/TAO/Cassini ThermalPlasma 1998-01-01T01:00:00Z 2004-07-04T00:00:00Z PT1H Cassini Note an important parameter - angle Cassini-Sun-Earth - which could be considered as quality flag. spase://CNES/NumericalData/AMDA/OMNI/omni-hour-all density cass_sw_n Solar Wind Proton Number Density, scalar cm^-3 NaN Proton NumberDensity velocity cass_sw_v Solar Wind Bulk Speed km/s 3 V r Component.I 1 cass_sw_v(0) V t Component.J 2 cass_sw_v(1) NaN Proton Velocity temperature cass_sw_t eV NaN Proton Temperature dynamic pressure cass_sw_pdyn nPa NaN Proton Pressure b tangential cass_sw_b nT NaN Magnetic b radial cass_sw_bx br along parker spiral computed with tao model outputs nT NaN Magnetic angle Cassini-Sun-Earth cass_sw_da deg NaN Positional