PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = " 2006-07-26, B. Harris, minor updates for version 3 standards; 2012-06-05, D. Kazden, removed unnecessary keywords; 2018-08-01, D. Kazden, removed aRCHIVE_STATUS keyword;" OBJECT = DATA_SET DATA_SET_ID = "GO-E-POS-6-SUMM-E2-GSE/GSM-COORDS-V1.0" OBJECT = DATA_SET_INFORMATION DATA_SET_NAME = "GALILEO EARTH2 TRAJECTORY V1.0" DATA_OBJECT_TYPE = "TABLE" ARCHIVE_STATUS = ARCHIVED DATA_SET_COLLECTION_MEMBER_FLG = N START_TIME = 1992-11-03T00:00:00 STOP_TIME = 1990-12-19T00:00:00 DATA_SET_RELEASE_DATE = 1995-04-18 PRODUCER_FULL_NAME = "DR. MARGARET G. KIVELSON" DETAILED_CATALOG_FLAG = N DATA_SET_TERSE_DESC = " This dataset contains the Galileo spacecraft trajectory during the Earth 2 flyby." ABSTRACT_DESC = " This dataset contains the Galileo spacecraft trajectory during the Earth 2 flyby. The data have been derived from SPICE kernels at a 1 minute sample rate. The data are provided in both Geocentric Solar Ecliptic (GSE) and Geocentric Solar Magnetic (GSM) coordinates and are given in units of earth radii where 1 Re = 6378 km." CITATION_DESC = " GALILEO EARTH2 TRAJECTORY V1.0, GO-E-POS-6-SUMM-E2-GSE/GSM-COORDS-V1.0, NASA Planetary Data System, 1995" DATA_SET_DESC = " Dataset Overview ================ This dataset contains the Galileo spacecraft trajectory during the Earth 2 flyby. The data have been derived from SPICE kernels at a 1 minute sample rate. The data are provided in both Geocentric Solar Ecliptic (GSE) and Geocentric Solar Magnetic (GSM) coordinates and are given in units of earth radii where 1 Re = 6378 km. Data Columns: time S/C event time (UT) given in seconds since 1966 scet S/C event time (UT) given in the form yyyy ddd mon day hh:mm:ss.sss X S/C position X component in GSE or GSM coordinate Y_gse S/C position Y component in GSE coordinates Z_gse S/C position Z component in GSE coordinates Y_gsm S/C position Y component in GSM coordinates Z_gsm S/C position Z component in GSM coordinates Coordinate Systems ================== The Galileo trajectory data are being archived in 2 coordinate systems. Geocentric Solar Ecliptic (GSE) and Geocentric Solar Magnetic (GSM) are related earth centered coordinate systems. Both the GSE and GSM X directions are taken along the Earth - Sun line, positive towards the Sun. The GSE Z direction is parallel to the ecliptic normal, positive northward, and Y completes the right-handed set (towards dusk). For GSM, the X-Z plane contains the Earth's dipole moment vector, positive northward, and Y completes the right-handed set. GSE coordinates are commonly used for analyzing the solar wind near the Earth and GSM coordinates are used when analyzing data inside the Earth's bow shock. Data Processing =============== These data have been derived from the PDS dataset: 'GO-J-SPICE-6-SPK-E2-V1.0' The SPK file used to dervied this product was: 'GLL920818.SPK' Data Quality ============ The data have been derived from the Galileo SPICE kernels using well tested software from the SPICELIB and GLLSPICE subroutine libraries. Each data point is computed using S/C and planetary ephemerides computed at the time of the dataset sample (not interpolated)." CONFIDENCE_LEVEL_NOTE = "NONE PROVIDED" END_OBJECT = DATA_SET_INFORMATION OBJECT = DATA_SET_TARGET TARGET_NAME = "EARTH" END_OBJECT = DATA_SET_TARGET OBJECT = DATA_SET_HOST INSTRUMENT_HOST_ID = GO INSTRUMENT_ID = MAG END_OBJECT = DATA_SET_HOST OBJECT = DATA_SET_MISSION MISSION_NAME = "GALILEO" END_OBJECT = DATA_SET_MISSION OBJECT = DATA_SET_REFERENCE_INFORMATION REFERENCE_KEY_ID = "N/A" END_OBJECT = DATA_SET_REFERENCE_INFORMATION END_OBJECT = DATA_SET END