Data Set Information
|
| DATA_SET_NAME |
ROSETTA-ORBITER CHECK GIADA 2 CVP2 COMMISSIONING2 V1.0
|
| DATA_SET_ID |
RO-X-GIA-2-CVP2-COMMISSIONING2-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 |
2004-09-20T11:47:04.867Z
|
| STOP_TIME |
2004-10-14T10:59:00.552Z
|
| 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_518, GIA_GAL_RP_519, GIA-GAL-RP-520, GIA_GAL_RP_521 and GIA_GAL_RP_522 (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-CVP2-COMMISSIONING2-V1.0, NASA Planetary Data System, 2007.
|
| ABSTRACT_TEXT |
This volume contains Experiment Data acquired by GIADA during 'Commissioning 2' phase. More in detail it refers to the data provided during the following in-flight scenarios: 'Interference 1' held on 20/21/22-09-2004; 'Pointing 1' held on 23-09-2004; 'Pointing 2' held on 30-09-2004; 'Interference 2' held on 12/13/14-10-2004. 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
|
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