Data Set Information
DATA_SET_NAME ICE SOLAR WIND PLASMA ELECTRON ANALYSER DATA V1.0
DATA_SET_ID ICE-C-SWPLAS-3-RDR-GIACOBIN-ZIN-V1.0
NSSDC_DATA_SET_ID
DATA_SET_TERSE_DESCRIPTION
DATA_SET_DESCRIPTION Data Set Overview : These data were obtained from the LANL plasma experiment on ICE (Principal Investigator: S.J. Bame; data provided by J.T. Gosling, with assistance from K. Sofaly and S. Kedge). The instrument measures the 2-D electron distribution function in one spacecraft rotation (3 s) once every 24 s, by obtaining 16 evenly spaced energy spectra, each with 15 contiguous levels covering the energy range 8.5 eV to 1140 eV. From these 2-D distributions the density, velocity, and temperature of the electrons are then derived. A 2-D temperature matrix is calculated which is subsequently diagonalized. Then nominally the maximum temperature corresponds to the parallel temperature and the minimum temperature corresponds to the perpendicular temperature. This is done independently of the magnetic field measurements; however, the direction of maximum temperature determined in this manner is usually found to be within 15 degrees of the magnetic field direction inferred from the magnetometer measurements. The time resolution is 24 sec from the start of Day 253 (September 10) until Day 255 (September 12), 18:38. At that time the bit rate dropped from 1024 to 512 bps, and the nominal time resolution went to 48 sec.
DATA_SET_RELEASE_DATE 3000-01-01T00:00:00.000Z
START_TIME 1985-09-10T12:00:16.800Z
STOP_TIME 1985-09-14T08:46:53.200Z
MISSION_NAME INTERNATIONAL COMETARY EXPLORER
MISSION_START_DATE 1983-12-22T12:00:00.000Z
MISSION_STOP_DATE N/A (ongoing)
TARGET_NAME GIACOBINI-ZINNER
TARGET_TYPE COMET
INSTRUMENT_HOST_ID ICE
INSTRUMENT_NAME SOLAR WIND PLASMA EXPERIMENT
INSTRUMENT_ID SWP
INSTRUMENT_TYPE PLASMA EXPERIMENT
NODE_NAME Small Bodies
ARCHIVE_STATUS ARCHIVED
CONFIDENCE_LEVEL_NOTE Confidence Level Overview : N/A
CITATION_DESCRIPTION Bame, S.J., J.T. Gosling, K. Sofaly, S. Kedge, ICE SOLAR WIND PLASMA ELECTRON ANALYSER DATA V1.0, ICE-C-SWPLAS-3-RDR-GIACOBIN-ZIN-V1.0, NASA Planetary Data System, 1995.
ABSTRACT_TEXT These data were obtained from the LANL plasma experiment on ICE (Principal Investigator: S.J. Bame assistance from K. Sofaly and S. Kedge). The instrument measures the 2-D electron distribution function in one spacecraft rotation (3 s) once every 24 s, by obtaining 16 evenly spaced energy spectra, each with 15 contiguous levels covering the energy range 8.5 eV to 1140 eV. From these 2-D distributions the density, velocity, and temperature of the electrons are then derived. A 2-D temperature matrix is calculated which is subsequently diagonalized. Then nominally the maximum temperature corresponds to the parallel temperature and the minimum temperature corresponds to the perpendicular temperature. This is done independently of the magnetic field measurements however, the direction of maximum temperature determined in this manner is usually found to be within 15 degrees of the magnetic field direction inferred from the magnetometer measurements. The time resolution is 24 sec from the start of Day 253 (September 10) until Day 255 (September 12), 18:38. At that time the bit rate dropped from 1024 to 512 bps, and the nominal time resolution went to 48 sec.
PRODUCER_FULL_NAME INTERNATIONAL HALLEY WATCH
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