ISOCAM Interactive Analysis User's Manual Version 5.0 - ISO - ESA

314 APPENDIX B. CIA COMMAND SHORT-LIST
sscd clean breaks an SPD SSCD into one SPD SSCD per CAM CONFIGURATION.
CIA> cleaned_sscd = sscd_clean( spd_sscd )
sscd elem returns a list of SCDs from an SSCD. In the example the list is stored in the string
array scds.
CIA> scds = sscd_elem( sscd )
scd del deletes SCDs from memory. In the example, delete the first SCD named in the string
array scds.
CIA> scd_del, scds[0]
get sscdraster creates a raster PDS from an SPD SSCD containing raster or micro-scan observation
data (CAM01).
CIA> raster_pds = get_sscdraster( spd_sscd, magnify=magnify )
get sscdstruct creates a general PDS from an SPD SSCD containing staring observation data
(CAM01).
CIA> staring_pds = get_sscdstruct( spd_sscd )
get sscdbs creates a BS PDS from an SPD SSCD containing beam-switch observation data
(CAM03).
CIA> bs_pds = get_sscdbs( spd_sscd )
get sscdcvf creates a CVF PDS from an SPD SSCD containing CVF data (CAM04).
CIA> cvf_pds = get_sscdcvf( spd_sscd )
B.2 Data calibration
All routines listed here that have the keyword method have a selection of different algorithms
that can be applied to the data. For an exhaustive list of methods see Chapter 20 or the on-line
help. In general the variable pds scd refers to an SCD, an SSCD or any flavour of PDS. The
variable pds refers to any flavour of PDS. An appropriate variable name will be used in examples
of routines which operate on a PDS of a particular flavour.
corr dark Remove dark current from IMAGEs in .CUBE using the method dark model.
CIA> corr_dark, pds_scd, method=’model’
deglitch Deglitch IMAGEs in .CUBE using the method mm.
CIA> deglitch, pds_scd, method=’mm’