urn:nasa:pds:cassini-caps-derived:data-ele-mom:els_3dmomt_2006101 1.0 1.16.0.0 Product_Observational Waite, J. H.; Furman, J. D. 2022 This file contains Cassini CAPS electron moments data, acquired at SATURN between 2006-101T00:00:14.000 and 2006-101T23:59:41.000 (orbit 023). 2022-02-24 1.0 This product, ELS_3DMOMT_2006101_00.TAB, was originally released as part of the PDS3 CO-E/J/S/SW-CAPS-5-DDR-ELE-MOMENTS-V1.0 data set. The metadata have been migrated to PDS4. The data themselves are unchanged. 2006-04-11T00:00:14.000Z 2006-04-11T23:59:41.000Z Science Derived Particles Electrons Plasma 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 Cassini Plasma Spectrometer Instrument urn:nasa:pds:context:instrument:caps.co is_instrument Saturn Planet urn:nasa:pds:context:target:planet.saturn data_to_target Tour 1/1523406630.223 1/1523492998.108 0.7 30 Electrons Density Electrons Temperature Electrons Velocity urn:nasa:pds:cassini-caps-derived:document:ele-moments-dataset data_to_document CO-E_J_S_SW-CAPS-5-DDR-DERIVED-V1.0:ELS_3DMOMT_2006101_00 data_to_derived_source_product 10.17189/1519609 PDS Planetary Plasma Interactions Node This is the first version of this product converted to PDS4. The DOI provided references the PDS3 source data set. Electron Moments. A description of how moments are generated can be found in the archive SIS. ELS_3DMOMT_2006101_00.TAB 2013-04-02T21:43:00.000Z 341884 e2d06f382b4f246790e86a69b06f4120 This data file is unmodified from the PDS3 version. 0 2692 Carriage-Return Line-Feed 13 0 127 START_TIME 1 ASCII_Date_Time_DOY 17 N/A Start of the sampling period, spacecraft event time, UTC, in ISOD format to second resolution. ISOD format is as follows: YYYY-DOYTHH:MM:SS 2030-001T00:00:00 2025-001T00:00:00 1997-288T10:43:00 END_TIME 19 ASCII_Date_Time_DOY 17 N/A End of the sampling period, spacecraft event time, UTC, in ISOD format to second resolution. ISOD format is as follows: YYYY-DOYTHH:MM:SS 2030-001T00:00:00 2025-001T00:00:00 1997-288T10:43:00 ANODE_USED 37 ASCII_Integer 1 Anode used to calculate moments. A value of 9 implies that multiple anodes were used. 0 9 1 SIGNAL_TO_NOISE 39 ASCII_Real 5 N/A Signal to noise ratio threshold. Only data values above this threshold go into the moments calculation. -9.99 10.00 0.00 SC_POTENTIAL 45 ASCII_Real 7 V Spacecraft potential during the time period given -999.99 100.00 -100.00 DENSITY 53 ASCII_Real 13 ELECTRONS/M^3 Density, summed over all energies. -9.000000E+00 1.000000E+10 -9.000000E+00 TEMPERATURE 67 ASCII_Real 12 eV Temperature, summed over all energies -9999.000000 99999.999999 -9999.000000 QUALITY_FACTOR 80 ASCII_Real 7 N/A The number of standard deviations, assuming Poisson counting statistics, that the peak of the Maxwellian corresponding to the determined moments lies above the ELS one-count level. The larger the value, the better. -99.000 100.000 -99.000 SC_CHARGE_STATE 88 ASCII_Integer 1 N/A Indicates whether the data is likely to be from a region in which the spacecraft is negatively charged. 0: likely positively charged 1: likely negatively charged 9 1 0 PENETRATING_RADIATION 90 ASCII_Integer 1 N/A Indicates whether the data is probably from a region in which there is penetrating radiation present. 0: not likely to be present 1: likely to be present 9 1 0 DENSITY_WITHOUT_PEN_RAD 92 ASCII_Real 13 ELECTRONS/M^3 Density, summed over all energies, but with penetrating radiation subtracted from the data before moments calculations were made. -9.000000E+00 1.000000E+10 -9.000000E+00 TEMPERATURE_WITHOUT_PEN_RAD 106 ASCII_Real 12 eV Temperature, summed over all energies, but with penetrating radiation subtracted from the data before moments calculations were made. -9999.000000 99999.999999 -9999.000000 QUALITY_FACTOR_WITHOUT_PEN_RAD 119 ASCII_Real 7 N/A The number of standard deviations, assuming Poisson counting statistics, that the peak of the Maxwellian corresponding to the determined moments lies above the ELS one-count level, but with penetrating radiation subtracted from the data before moments calculations were made. The larger the value, the better. -99.000 100.000 -99.000