2.2.6 spase://CDPP/NumericalOutput/AMDA/TAO/Mercury/tao-mercury-stb SW / Input STB Tao SW Mercury / Input Stereo-B 2017-07-08T16:49:29Z Stereo-B PLASTIC 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/Mercury ThermalPlasma 1990-01-01T01:00:00Z 2018-11-14T00:00:00Z PT1H Mercury Note an important parameter - angle Mercury-Sun-STB - which could be considered as quality flag. spase://CDPP/NumericalData/AMDA/STEREO-B/PLASTIC/stb-l2-pla density mercury_stb_n Solar Wind Proton Number Density, scalar cm^-3 NaN Proton NumberDensity velocity mercury_stb_v Solar Wind Bulk Speed km/s 3 V r Component.I 1 mercury_stb_v(0) V t Component.J 2 mercury_stb_v(1) NaN Proton Velocity temperature mercury_stb_t eV NaN Proton Temperature dynamic pressure mercury_stb_pdyn nPa NaN Proton Pressure b tangential mercury_stb_b nT NaN Magnetic angle Mercury-Sun-STB mercury_stb_da NaN Positional