urn:nasa:pds:cassini-mag-cal:data-full-rtn:00053_fgm_rtn 1.0 1.20.0.0 Product_Observational Dougherty, Michele K.; Kellock, Stephen; Slootweg, A. Peter; Achilleos, Nicholas; Joy, Steven P.; Mafi, Joseph N. 2023 Cassini magnetic-field data in the highest time resolution available, from the Fluxgate Magnetometer (FGM) instrument, for 2000-02-22 (053) in RTN coordinates. 2023-11-09 1.0 This data file, 00053_FGM_RTN.LBL, was originally not a part of the PDS3 CO-E/SW/J/S-MAG-3-RDR-FULL-RES-V2.0 dataset. The meta-data have been migrated to PDS4. 2000-02-22T19:24:25.203Z 2000-02-22T20:51:53.234Z Science Calibrated Fields Magnetic Background Cassini-Huygens Mission urn:nasa:pds:context:investigation:mission.cassini-huygens data_to_investigation Cassini Orbiter Host urn:nasa:pds:context:instrument_host:spacecraft.co is_instrument_host Dual Technique Magnetometer Instrument urn:nasa:pds:context:instrument:mag.co is_instrument Solar Wind Plasma Stream urn:nasa:pds:context:target:plasma_stream.solar_wind data_to_target Outer Cruise 1/1329939180.218 1/1329944428.235 1 urn:nasa:pds:cassini-mag-cal:document:data-full-rtn-desc data_to_document Document containing a description of the Cassini MAG Calibrated Full Res. Data in RTN Coords. Collection. 10.17189/1520114 Elson, L.S., C.H. Acton, D.L. Conner and B.V. Semenov, Cassini SPICE Kernels V1.0, CO-S/J/E/V-SPICE-6-V1.0, NASA Planetary Data System, 2005. https://doi.org/10.17189/1520114 This product was processed using the following kernels using the data set referenced above: CO-E/SW/J/S-MAG-3-RDR-FULL-RES-V2.0:00053_FGM_RTN:00053_FGM_RTN.TAB data_to_calibrated_source_product 10.17189/1521151 PDS Planetary Plasma Interactions Node This is the first version converted to PDS4. The DOI provided references the PDS3 source data set. 00053_FGM_RTN.TAB 2023-08-23T17:10:41.000Z 9272576 8dc6ccb96cb75741de6d1cfc7dd0c748 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). These MAG data were processed (calibrated, and rotated into RTN coordinates) by the Cassini MAG team at Imperial College. They were acquired by the PDS PPI node at UCLA where they were converted from binary to ASCII, and the B-field magnitude, and position data removed. These data have been processed using an updated calibration that was produced using the Proximal Orbit data. The original binary data file contained a large number of backwards time steps. Due to the large number and overlap in these timing errors, these data have been sorted by time. For more information on the timing errors, and on this and previous versions of the data, please refer to the collection description file for this collection (data-full-rtn.txt). 0 159872 Carriage-Return Line-Feed 4 0 58 TIME 1 1 ASCII_Date_Time_YMD 23 Spacecraft event time of the sample. BR 2 25 ASCII_Real 10 nT RTN radial component of the magnetic-field component in nT. The radial component (R) points from the Sun to the spacecraft, positive away from the Sun. 44000.000 -44000.000 BT 3 36 ASCII_Real 10 nT RTN tangential component of the magnetic field component in nT. The tangential component (T) is parallel to the Solar Equatorial plane (Omega Sun x R). 44000.000 -44000.000 BN 4 47 ASCII_Real 10 nT RTN normal component of the magnetic field component in nT. The normal component (N) completes the right handed set, and is roughly normal to the Solar Equatorial plane (R x Phi). 44000.000 -44000.000