PDS_VERSION_ID = PDS3 RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 140 FILE_RECORDS = 11 DATA_SET_ID = "MGN-V-RSS-1-BSR-V1.0" PRODUCT_ID = "KEPELEMS.TAB" SPACECRAFT_NAME = MAGELLAN INSTRUMENT_ID = RSS TARGET_NAME = VENUS PRODUCT_CREATION_TIME = 1996-10-05T00:00:00Z MISSION_PHASE_NAME = {"MAPPING CYCLE 5","MAPPING CYCLE 6"} ORBIT_NUMBER = "N/A" START_TIME = 1993-10-03T13:24:14Z STOP_TIME = 1994-06-06T00:27:37Z DSN_STATION_NUMBER = {14,43,63} ^TABLE = "KEPELEMS.TAB" OBJECT = TABLE INTERCHANGE_FORMAT = ASCII ROWS = 11 COLUMNS = 7 ROW_BYTES = 140 ROW_SUFFIX_BYTES = 0 DESCRIPTION = "This table contains Keplerian elements for Magellan orbits during which bistatic radar experiments were conducted. Each row contains 7 columns of data, separated by commas; character fields are enclosed in double quotes. The data fields occupy 138 bytes; each row is delimited by an ASCII carriage- return line-feed pair." ^TABLE = "KEPELEMS.TAB" OBJECT = COLUMN COLUMN_NUMBER = 1 NAME = "SEMI-MAJOR AXIS" DATA_TYPE = ASCII_REAL START_BYTE = 1 BYTES = 16 FORMAT = "E16.10" UNIT = "KILOMETER" DESCRIPTION = "The semi-major axis of the orbit." END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 2 NAME = "ECCENTRICITY" DATA_TYPE = ASCII_REAL START_BYTE = 18 BYTES = 19 FORMAT = "E19.13" UNIT = "N/A" DESCRIPTION = "The eccentricity of the orbit." END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 3 NAME = "INCLINATION" DATA_TYPE = ASCII_REAL START_BYTE = 38 BYTES = 17 FORMAT = "E17.11" UNIT = "DEGREE" DESCRIPTION = "The inclination of the orbit." END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 4 NAME = "LONGITUDE OF ASCENDING NODE" DATA_TYPE = ASCII_REAL START_BYTE = 56 BYTES = 18 FORMAT = "E18.12" UNIT = "DEGREE" DESCRIPTION = "The longitude of the ascending node." END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 5 NAME = "ARGUMENT OF PERIAPSIS" DATA_TYPE = ASCII_REAL START_BYTE = 75 BYTES = 18 FORMAT = "E18.12" UNIT = "DEGREE" DESCRIPTION = "The argument of periapsis." END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 6 NAME = "EPOCH" DATA_TYPE = TIME START_BYTE = 94 BYTES = 23 UNIT = "N/A" DESCRIPTION = "The date and time at which the orbital elements are defined. See column 7 for the relationship between EPOCH and spacecraft Time of Periapsis" END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 7 NAME = "SOURCE" DATA_TYPE = CHARACTER START_BYTE = 119 BYTES = 19 UNIT = "N/A" DESCRIPTION = "The source of the orbital elements and the date on which they were obtained. If 'Cavender', the source was Jim Cavender of the Martin Marietta Astronautics Group (Denver) and EPOCH is Time of Descending Node. To obtain Time of Periapsis TPER, calculate period = sqrt(4.0d+00*pi*pi*axi*axi*axi/mu) true_anom = (1.8d+02-wper)*pi/1.8d+02 fac1 = sqrt((1.0d+00-ecc)/(1.0d+00+ecc)) ecc_anom = 2.0d+00*datan(fac1*tan(0.5d+00*true_anom)) mean_anom = ecc_anom-ecc*sin(ecc_anom) TPER = EPOCH - mean_anom*period/2.0d+00/pi/8.64d+04 where axi is SEMI-MAJOR AXIS ecc is ECCENTRICITY pi is 4*atan(1.) mu is GM for Venus (0.32485876561687E+06 km^3/kg^2/sec^2) wper is ARGUMENT OF PERIAPSIS and TPER and EPOCH are both expressed in Julian days. If 'Lyons', the source was Dan Lyons of the Magellan Project (JPL) and EPOCH is time of apoapsis. To obtain Time of Periapsis TPER, calculate period = sqrt(4.0d+00*pi*pi*axi*axi*axi/mu) TPER = EPOCH - 0.5*period/8.64d+04 and TPER and EPOCH are both expressed in Julian days. If 'Lock', the source was Rob Lock of the Magellan Project (JPL) and EPOCH is Time of Periapsis." END_OBJECT = COLUMN END_OBJECT = TABLE END