Data Set Information
DATA_SET_NAME ROSETTA-ORBITER CHECK GIADA 2 CR5 CRUISE5 V1.0
DATA_SET_ID RO-X-GIA-2-CR5-CRUISE5-V1.0
NSSDC_DATA_SET_ID NULL
DATA_SET_TERSE_DESCRIPTION Volume containing data from 'Cruise 5' and more specifically: 'Active Payload Checkout 12' (PC12) - 23-04-2010 and 4-05-2010
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 2011-02-15T00:00:00.000Z
START_TIME 2010-04-24T02:16:11.160Z
STOP_TIME 2010-04-25T01:56:00.186Z
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 IN_LIEN_RESOLUTION
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 RO_GIA_OACUPA_RP_115_1 (reported in DOCUMENTation dir) for
        evaluations on GIADA behaviour during this mission phase.
CITATION_DESCRIPTION A. Rotundi and the International GIADA Consortium, RO-X-GIA-2-CR5-CRUISE5-V1.0, NASA Planetary Data System, 2007.
ABSTRACT_TEXT Payload Checkout 12 (PC12) was an active checkout where a target independent opportunity to perform interactive operations and to request spacecraft pointing was given to all Rosetta payload teams. All Rosetta payload took part in this scenario The Active Payload Checkout 12 ran for 23 consecutive days starting on the 23th April 2010 until the 14th May 2010.During PC12 GIADA performs only a passive test (GD01) similar to the previous Passive Payload Checkouts. This passive test (GD01), which includes standard procedures and full functional verification, was executed by switching on Main and Redundant I/Fs in sequence and executing similar procedures for the two cases. 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
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