NSSDCA ID: PSSB-00387
Availability: Archived at NSSDC, accessible from elsewhere
This description was generated automatically using input from the Planetary Data System.
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.
These data are available on-line from the Planetary Data System (PDS) at:
http://pdssbn.astro.umd.edu/holdings/ro-x-gia-2-cvp2-commissioning2-v1.0/
Questions and comments about this data collection can be directed to: Dr. David R. Williams
Name | Role | Original Affiliation | |
---|---|---|---|
Dr. Luigi Colangeli | Data Provider | Osservatorio Astronomico di Capodimonte | colangeli@na.astro.it |