2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Cassini/MAG/cass-mag-jup flyby jupiter high resolution MAG data during Jupiter flyby 2019-08-23T10:50:36Z High-resolution magnetic field data from the Cassini magnetometer during the Jupiter flyby obtained from NASA/PDS plasma node * J3 - J3 (IAU_JUPITER) is a Jovicentric cartesian coordinate system consistent with the IAU 1997 definition of the System 3 prime meridian. It consists of X (in Jovian equatorial plane, along S3 1997 prime meridian), Y (completes right handed set), and Z (parallel to the Jovian spin axis). * JMXYZ - JMAG XYZ is a Jovicentric cartesian coordinate system which consists of X (in the plane containing Z and the S3 1997 Prime Meridian), Y (completes right handed set), and Z (the Jupiter dipole). * RTN - RTN coordinates consist of R (radial component, Sun to the spacecraft), T (tangential component, parallel to the Solar Equatorial plane and perpendicular to R), and N (normal component, completes right handed set). spase://CNES/Person/CDPP-AMDA/Michele.Dougherty PrincipalInvestigator spase://CNES/Person/CDPP-AMDA/Steve.Kellock DataProducer spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server http://amda.irap.omp.eu/service/hapi 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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA Web application http://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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. PDS CO-E_SW_J_S-MAG-3-RDR-FULL-RES-V2.0 spase://CNES/Instrument/CDPP-AMDA/Cassini/MAG MagneticField 2001-01-01T02:26:04Z 2001-03-02T06:32:37Z PT0.031S PT8S Jupiter These data contain persistent noise signals at 0.2, 8, 16 Hz, and associated harmonics. This noise was not observed during ground testing of the instruments and is anticipated to be interference arising from the spacecraft. Removal of these signals is at the user's discretion. b_j3 cass_bj3_jup Magnetic field vector components in Jup_IAU coordinates phys.magField nT TimeSeries 3 bx 1 cass_bj3_jup(0) by 2 cass_bj3_jup(1) bz 3 cass_bj3_jup(2) Vector Magnetic b_jm cass_bjm_jup Magnetic field vector components in JMAG coordinates phys.magField nT TimeSeries 3 bx 1 cass_bjm_jup(0) by 2 cass_bjm_jup(1) bz 3 cass_bjm_jup(2) Vector Magnetic b_rtn cass_b_jup Magnetic field vector components in RTN coordinates phys.magField nT TimeSeries 3 br 1 cass_b_jup(0) bt 2 cass_b_jup(1) bn 3 cass_b_jup(2) Vector Magnetic |b| cass_bmag_jup Magnetic field vector magnitude phys.magField nT TimeSeries Magnitude Magnetic phi cass_b_jup_phi Magnetic field phi angle phys.magField degrees 1e-9>T TimeSeries 1 Magnetic theta cass_b_jup_theta Magnetic field theta angle phys.magField degrees 1e-9>T TimeSeries 1 Magnetic