Data Set Information
DATA_SET_NAME ROSETTA-ORBITER CHECK GIADA 2 CVP1 COMMISSIONING1 V1.0
DATA_SET_ID RO-X-GIA-2-CVP1-COMMISSIONING1-V1.0
NSSDC_DATA_SET_ID
DATA_SET_TERSE_DESCRIPTION
DATA_SET_DESCRIPTION The format of data reported in GIADA data sets is the same for all mission phases. Data reported by GDS and IS are due to noise as no dust event is expected in this mission phase. MBS frequency changes, once normalised for frequency vs. temperature dependence, if present, are due to deposition of contaminants existing in the S/C environment. Housekeeping and Calibration data from all GIADA sub-systems are useful to evaluate instrument health and behaviour when compared with similar data acquired during other mission phases.
DATA_SET_RELEASE_DATE 2009-05-01T00:00:00.000Z
START_TIME 2004-04-03T10:05:27.127Z
STOP_TIME 2004-04-04T03:25:52.694Z
MISSION_NAME INTERNATIONAL ROSETTA MISSION
MISSION_START_DATE 1995-03-01T12:00:00.000Z
MISSION_STOP_DATE N/A (ongoing)
TARGET_NAME UNKNOWN
TARGET_TYPE UNKNOWN
INSTRUMENT_HOST_ID RO
INSTRUMENT_NAME GRAIN IMPACT ANALYSER AND DUST ACCUMULATOR
INSTRUMENT_ID GIADA
INSTRUMENT_TYPE DUST DETECTOR
NODE_NAME Small Bodies
ARCHIVE_STATUS ARCHIVED
CONFIDENCE_LEVEL_NOTE The data reported in this data set have been converted from ADC counts to engineering values. The quality of the Housekeeping and Calibration data is good. Scientific data are due to noise, as no grain event is expected during this mission phase. These data must be only considered to evaluate GIADA behaviour and not as real scientific data. See GIA_GAL_RP_517.PDF (reported in DOCUMENT dir) for evaluations on GIADA behaviour during this mission phase.
CITATION_DESCRIPTION L. Colangeli and the International GIADA Consortium, RO-X-GIA-2-CVP1-COMMISSIONING1-V1.0, NASA Planetary Data System, 2007.
ABSTRACT_TEXT This volume contains Experiment Data acquired by GIADA during 'Commissioning 1' phase. More in detail it refers to the data provided during the following in-flight tests: 'First GIADA switch ON' held on 03/04-04-2004. It also contains documentation which describes the GIADA experiment. The data reported in this data set have been converted from ADC counts to engineering values. The quality of the Housekeeping and Calibration data is good. Scientific data are due to noise, as no grain event is expected during this mission phase. These data must be only considered to evaluate GIADA behaviour and not as real scientific data. Data reported by GDS and IS are due to noise as no dust event is expected during this mission phase. MBS frequency changes, once normalised for frequency vs. temperature dependence, if present, are due to deposition of contaminants existing in the S/C environment. Housekeeping and Calibration data from all GIADA sub-systems are useful to evaluate instrument health and behaviour when compared with similar data acquired during other mission phases.
PRODUCER_FULL_NAME GIADA TEAM
SEARCH/ACCESS DATA
  • SBN Comet Website
    		•