2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Galileo/MAG/gll-mag-ga flybys ganymede 2012-03-06T18:42:41Z Magnetic field data from the Galileo magnetometer during Ganymede flybys, obtained from NASA/PDS plasma node, in various coordinate systems * 1996-06-27T06:07:09 1996-06-27T06:52:37 * 1996-09-06T18:32:45 1996-09-06T19:28:22 * 1997-04-05T06:44:41 1997-04-05T07:40:18 * 1997-05-07T15:36:54 1997-05-07T16:22:23 * 1997-06-26T16:50:00 1997-06-26T17:49:56 * 1997-12-15T09:30:24 1997-12-15T10:30:00 * 2000-05-20T09:40:04 2000-05-20T10:40:41 * 2000-12-28T07:54:42 2000-12-28T08:55:20 Coordinate systems * System III : R is along the Jupiter to spacecraft line, positive away from Jupiter. Phi is parallel to the Jovigraphic equator (Omega x R). Theta completes the right-handed set (positive southward). * IRC - Inertial Rotor coordinates : Z is along the spacecraft spin axis (positive opposite the high-gain antenna). X is roughly parallel to the south ecliptic normal. Y completes the right handed set (pointing roughly dawnward). * GPHIO - Ganymede Phi-Omega coordinates : X is in the direction of corotational flow (System III Phi). Z is parallel to the Jovian spin axis (Omega). Y completes the right handed set. * GSPRH - spherical Ganymede-centered 'planetocentric' right-handed coordinates : R is along the satellite to spacecraft line, positive away from the satellite. Phi is parellel to the satellite's planetographic equator and positive in a right-handed sense. Theta completes the right-handed set (positive southward) spase://SMWG/Person/Margaret.Galland.Kivelson PrincipalInvestigator spase://CNES/Person/CDPP-AMDA/Steven.Joy DataProducer spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi gll-mag-ga 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. PDS GO-J-MAG-3-RDR-HIGHRES-V1.0 spase://CNES/Instrument/CDPP-AMDA/Galileo/MAG MagneticField 1996-06-27T06:07:08Z 2000-12-28T08:55:20Z PT0.3S Jupiter.Ganymede Jupiter Ganymede GALILEO b_irc gll_mag_gairc Magnetic field vector components in IRC coordinates phys.magField nT TimeSeries 3 bx 1 gll_mag_gairc(0) by 2 gll_mag_gairc(1) bz 3 gll_mag_gairc(2) Vector Magnetic b_gphio gll_mag_gagphio Magnetic field vector components in Ganymede-centered Phi-Omega coordinates phys.magField nT TimeSeries 3 bx 1 gll_mag_gagphio(0) by 2 gll_mag_gagphio(1) bz 3 gll_mag_gagphio(2) Vector Magnetic b gsprh gll_mag_gagsprh Magnetic field vector components in Ganymede-centered spherical coordinates nT 3 br 1 gll_mag_gagsprh(0) btheta 2 gll_mag_gagsprh(1) bphi 3 gll_mag_gagsprh(2) Vector Magnetic b_sys3 gll_mag_gasys3 Magnetic field vector components in SYS3 spherical coordinates phys.magField nT TimeSeries 3 br 1 gll_mag_gasys3(0) btheta 2 gll_mag_gasys3(1) bphi 3 gll_mag_gasys3(2) Vector Magnetic |b| gll_mag_gamagnitude Magnetic field vector magnitude phys.magField nT TimeSeries Magnitude Magnetic