HESSI SCIENCE OPERATIONS
Telemetry to CD production:
Start with telemetry files: vc1 and vc3 per contact. (vc1 = instrument State of Health, vc3 = Science)
hsi_contact2fits combines vc1 and vc3 packets, splits files into files per each orbit, named hsi_yyyymmdd_hhmm_nnn.fits. The date and time, yyyymmdd_hhmm, corresponds to the start of the orbit. For this, we need access to the ehpemeris data, to be provided by the GDS in ASCII files.
The "nnn" is a version number, for instances in which a file is generated that has the same yyyymmdd_hhmm as a previous file.
The catalog data will be generated as part of hsi_contact2fits, and appended to the hsi_yyyymmdd_hhmm_nnn.fits files.
These files are then written to CD.
Contents of the various files:
Inputs to hsi_contact2fits:
- contact files contain telemetry frames:
- vc1 files contain stored instrument/state of health packets
- vc3 files contain stored science data
- ephemeris files contain:
- position and velocity of spacecraft at 10 sec intervals
- times of spacecraft day and night, and SAA pasage
Outputs from hsi_contact2fits:
- FITS file contains (as binary table extensions):
- vc1 & vc3 packets
- Catalog for the given time interval
- Catalog contains (in binary table extensions):
- Observing Summary: (Implemented)
- spin-averaged count rates in 8 energy bands, summed over detectors
- monitor rates
- modulation variance, 2 Coarsest collimators
- data gap start and end times
- S/C position
- Instrument Log: (Not Implemented)
- Housekeeping, State of Health data for the Imager, Spectrometer, Particle Monitor, etc...
- Flare List: (Partially Implemented)
- Id number
- Start, peak and end times, in energy range [3.0, 20.0] keV
- peak count rate
- total counts
- Highest energy of observed photons
- Flare position, arcsec from Sun center
- Flags for flares that start/end in Eclipse or SAA
- Spectral catalog: (Not Implemented)
- count and photon spectra as a function of time
- Thermal + double power law photon spectra,
- dE = E/2 energy resolution.
- Image catalog: (Not Implemented)
- Images in the 8 energy bands given by the Observing Summary, If possible, Cadence determined by Count Rate
Other database files needed by hsi_contact2fits:
- The Calibration database contains the data needed for spectral response matrices. From /ssw/hessi/dbase
- The Grid response database contains the data needed for grid response matrices. From /ssw/hessi/dbase
- The Stellar position database contains the position of stars used by the RAS/SAS SW to determine the aspect solution. From /ssw/hessi/dbase
- The Solar ephemeris database contains the position, size, and orientation of the Sun.
Other data to be generated after contact:
- Real-time Science data catalog: Generated by hsi_contact2fits from vc2 packets for each contact. Posted on the HESSI ftp site for quick access.
- Whole-Mission HESSI catalog: During catalog generation by hsi_contact2fits, the catalog extensions are saved in separate files (hsicat_yyyymmdd....etc) and are appended to form weekly files (or possibly monthly:TBD). These will be accessible for web-based browsing.
- Contact2fits file database: A list of each FITS file generated including the filename the start and end times for the file, and the contact from which it came.
Distribution:
- The FITS files are hopefully sent via internet to SDAC and ETH. CDs are mailed. The data is stored locally on a RAID system.
16-Oct-1999, jmm