urn:nasa:pds:cassini-mag-cal:data-1sec-gse:99228_99258_fgm_gse_1s 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 1 second averages, from the Fluxgate Magnetometer (FGM), from 1999-08-16 - 1999-09-15, in GSE coordinates. GSE coordinates consist of X (Earth to Sun), Y (completes the right handed set), and Z (perpendicular to the ecliptic plane). 2023-11-08 1.0 Original 99228_99258_FGM_GSE_1S.TAB, product version 6, from the PDS3 CO-E/SW/J/S-MAG-4-SUMM-1SECAVG-V2.0 dataset, DATA directory, converted to PDS4. 1999-08-16T00:00:03.005Z 1999-09-15T11:34:07.005Z 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 1/1313453209.244 1/1316086871.066 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: 99221_99228rb.bc 99228_99235rb.bc 99229_99230rb.bc 99235_99242rb.bc 99249_99256rb.bc 99256_99263rb.bc Leapsecond (LSK) kernels: naif0007.tls naif0008.tls PCK kernels: cpck01Oct2002.tpc cpck05Mar2004.tpc cpck30Sep2004_jupiter.tpc Spacecraft clock kernels: cas00090.tsc cas00091.tsc cas00113.tsc Spacecraft ephemeris kernels: 000331r_sk_v2p12_ep15.bsp 010420r_scpse_ep1_jp83.bsp CO-E/SW/J/S-MAG-4-SUMM-1SECAVG-V2.0:99228_99258_FGM_GSE_1S:99228_99258_FGM_GSE_1S.TAB data_to_calibrated_source_product 10.17189/1519603 PDS Planetary Plasma Interactions Node This is the first version converted to PDS4. The DOI provided references the PDS3 source data set. 99228_99258_FGM_GSE_1S.TAB 2023-11-02T10:31:37.000Z 75835340 b6c2b31c7214b6f5d6680dc271261f19 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 averaged from the full-resolution MAG data at the PDS PPI node at UCLA. The full-res MAG data were processed (calibrated, rotated into GSE coordinates) by the Cassini MAG team at Imperial College and are archived as part of the data set: CO-E/SW/J/S-MAG-3-RDR-FULL-RES-V1.0. The full-res data were provided to PDS by the MAG team Co-I at UCLA. Trajectory and the number of points in the average were added at the PDS/PPI node. Note that for some of the data files associated with the PDS3 data set it was necessary to remove mistime-tagged data present in the full-res dayfiles prior to averaging. A complete list of full-res data files containing mistime-tagged intervals is provided in the file FGM_FULL_TIMING_ERRS.CSV, which is included in the 'Cassini Bundle, document-mag collection.' For more information on this data set please refer to the PDS catalog file for this data set (CO_MAG_CAL_1SEC_DS.CAT). 0 1083362 Carriage-Return Line-Feed 6 0 70 TIME 1 1 ASCII_Date_Time_YMD 21 Spacecraft event time of the sample. BX 2 23 ASCII_Real 10 nT GSE X component of the magnetic-field in nT. X points from Earth to the Sun. 44000.000 -44000.000 BY 3 34 ASCII_Real 10 nT GSE Y component of the magnetic-field 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 45 ASCII_Real 10 nT GSE Z component of the magnetic-field in nT. Z is perpendicular to the ecliptic plane. 44000.000 -44000.000 BTOTAL 5 56 ASCII_Real 10 nT Average value of the full-resolution magnetic-field magnitudes calculated over the averaging interval in nT. Note that this value may differ slightly from the square root of the sum of the squares of the averaged field components. 44000.000 0. NPTS 6 67 ASCII_Real 2 Number of points in the average.