2.2.6 spase://CNES/NumericalOutput/CDPP-AMDA/TAO/Bepi/tao-bepi-sw SW / Input OMNI Tao SW Bepi / Input OMNI 2024-03-24T20:30:06Z 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-bepi-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/Bepi ThermalPlasma 2018-10-21T00:00:00Z 2024-02-14T00:00:00Z PT1H Heliosphere Note an important parameter - angle Bepi-Sun-Earth - which could be considered as quality flag. spase://CNES/NumericalData/AMDA/OMNI/omni-hour-all density bepi_sw_n Solar Wind Proton Number Density, scalar cm^-3 NaN Proton NumberDensity velocity bepi_sw_v Solar Wind Bulk Speed km/s 3 V r Component.I 1 bepi_sw_v(0) V t Component.J 2 bepi_sw_v(1) NaN Proton Velocity temperature bepi_sw_t eV NaN Proton Temperature dynamic pressure bepi_sw_pdyn nPa NaN Proton Pressure b tangential bepi_sw_b nT NaN Magnetic b radial bepi_sw_bx br along parker spiral computed with tao model outputs nT NaN Magnetic angle Bepi-Sun-Earth bepi_sw_da deg NaN Positional