urn:nasa:pds:cassini-mag-cal:data-full-gse:99225_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 1999-08-13 (225) in GSE coordinates. 2023-10-27 1.0 Original 99225_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. 1999-08-13T16:41:40.307Z 1999-08-13T16:44:11.383Z 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 Interplanetary Cruise 1/1313254105.116 1/1313254256.136 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: 99004_00003ra.bc Leapsecond (LSK) kernels: naif0012.tls PCK kernels: cpck15Dec2017.tpc Spacecraft clock kernels: cas00172.tsc 99225_FGM_GSE.TAB 2019-06-05T13:28:23.000Z 11600 458172fd53eb0c7a1dd360803758d98d 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 this data file contains timing errors including one or more backwards times. A list of mis-timed data intervals that have been identified for this file is provided below: Start Time Stop Time ======================= ======================= 1999-08-13T16:41:40.307 1999-08-13T16:41:56.176 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 0 200 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