2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/MAG/so-mag-rtnhr 0.1 sec : rtn Magnetic Field in RTN : 0.1 sec 2024-09-28T06:24:26Z Publication quality. Take note of Quality Flag and refer to SOL-MAG-DPDD for exceptions ( see SolO Archive Support Data) Solar Orbiter magnetometer data was provided by Imperial College London and supported by the UK Space Agency spase://CNES/Person/CDPP-AMDA/Tim.Horbury PrincipalInvestigator SolO home page at Imperial College https://www.imperial.ac.uk/space-and-atmospheric-physics/research/missions-and-projects/space-missions/solar-orbiter/ SolO Archive Support Data https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data solo-mag-l2 PartOf L2 spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi so-mag-rtnhr 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. http://soar.esac.esa.int/soar MAG-RTN-NORMAL spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/MAG MagneticField 2020-04-15T00:00:00Z 2024-06-30T23:59:59Z PT0.1S Heliosphere.Inner Sun.Corona Flag setting: * 0: Bad data; * 1: Known problems use at your own risk; * 2: Survey data, possibly not publication quality; * 3: Good for publication subject to PI approval; * 4: Excellent data which has received special treatment; refer SOL-MAG-DPDD for more information on how these flags are generated." b_rtn solo_b_rtn_hr phys.magField nT 1e-9>T Cartesian RTN TimeSeries 3 br Component.I 1 solo_b_rtn_hr(0) bt Component.J 2 solo_b_rtn_hr(1) bn Component.K 3 solo_b_rtn_hr(2) Vector Component.I Component.J Component.K Magnetic |b| solo_b_rtn_hr_tot Magnetic field magnitude phys.magField nT 1e-9>T TimeSeries Magnetic phi solo_b_rtn_hr_phi Magnetic field phi angle phys.magField degrees 1e-9>T TimeSeries Magnetic theta solo_b_rtn_hr_theta Magnetic field theta angle phys.magField degrees 1e-9>T TimeSeries Magnetic quality solo_b_rtn_hr_qf Flag setting: 0: Bad data; 1: Known problems use at your own risk; 2: Survey data, possibly not publication quality; 3: Good for publication subject to PI approval; 4: Excellent data which has received special treatment TimeSeries DataQuality