2.2.6 spase://CNES/NumericalOutput/CDPP-AMDA/TAO/Rosetta/tao-ros-sw SW / Input OMNI Tao SW Rosetta @ C-G / Input OMNI 2017-07-08T16:49:29Z OMNI solar wind 1-hour 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/Rosetta ThermalPlasma 2014-01-01T00:00:00Z 2016-10-01T00:00:00Z PT1H Comet Note an important parameter - angle Rosetta-Sun-Earth - which could be considered as quality flag. spase://CDPP/NumericalData/AMDA/OMNI/omni-hour-all density ros_sw_n Solar Wind Proton Number Density, scalar cm^-3 NaN Proton NumberDensity velocity ros_sw_v Solar Wind Bulk Speed km/s 3 V r Component.I 1 ros_sw_v(0) V t Component.J 2 ros_sw_v(1) NaN Proton Velocity temperature ros_sw_t eV NaN Proton Temperature dynamic pressure ros_sw_pdyn nPa NaN Proton Pressure b tangential ros_sw_b nT NaN Magnetic angle Ros-Sun-Earth ros_sw_da deg NaN Positional