urn:nasa:pds:cassini-mag-cal:data-full-gse:99232_fgm_gse 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 1999-08-20 (232) in GSE coordinates. 2023-10-27 1.0 Original 99232_FGM_GSE.TAB, product version 5, from the PDS3 CO-E/SW/J/S-MAG-3-RDR-FULL-RES-V2.0 dataset, DATA directory, converted to PDS4. 1999-08-20T00:00:03.734Z 1999-08-21T00:00:00.126Z 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 Earth Planet urn:nasa:pds:context:target:planet.earth data_to_target Solar Wind Plasma Stream urn:nasa:pds:context:target:plasma_stream.solar_wind data_to_target Interplanetary Cruise 1/1313798812.117 1/1313885209.107 1 urn:nasa:pds:cassini-mag-cal:document:data-full-gse-desc data_to_document Document containing a description of the Cassini MAG Calibrated Full Res. Data in GSE 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: SPICE spacecraft orientation kernels: 99229_99239ra.bc Leapsecond (LSK) kernels: naif0012.tls PCK kernels: cpck15Dec2017.tpc Spacecraft clock kernels: cas00172.tsc 99232_FGM_GSE.TAB 2019-06-05T13:18:11.000Z 151640072 fd4ab98a3012243066d84d19491f3f71 GSE coordinates consist of X (Earth to Sun), Y (completes the right handed set), and Z (perpendicular to the ecliptic plane). These MAG data were processed (calibrated, and rotated into GSE 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. Note that some of the data files from this collection contain timing errors. This file, however, contains no identified timing errors. The data in this PRODUCT_VERSION_ID 5 data product have been processed using an updated calibration that was produced using the Proximal Orbit data. 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-gse-desc.txt). These spice kernels were used to process these data but are not archived: 171215R_SCPSEops_97288_17258.bsp 0 2614484 Carriage-Return Line-Feed 4 0 58 TIME 1 1 ASCII_Date_Time_YMD 23 Spacecraft event time of the sample. BX 2 25 ASCII_Real 10 nT GSE X component of the magnetic-field component in nT. X points from Earth to the Sun. 44000.000 -44000.000 BY 3 36 ASCII_Real 10 nT GSE Y component of the magnetic field component in nT. Y is parallel to the ecliptic plane and perpendicular to the Earth-Sun line, positive opposite to the direction of the Earth's motion. 44000.000 -44000.000 BZ 4 47 ASCII_Real 10 nT GSE Z component of the magnetic field component in nT. Z is perpendicular to the ecliptic plane. 44000.000 -44000.000