F I G S 4 2 3
Given a FIGS image mode data hypercube, either sorted into
wavelength order (e.g. by FIGS424) or not, sums all the cycles
and wavelength planes within a specified wavelength range
to produce an image. Note that it is probably best to have
performed the wavelength sort first.
Command parameters -
'HCUBE' (Character) The name of the hypercube to be processed.
'CYSTART' (Integer) The first cycle to be included.
'CYEND' (Integer) The last cycle to be included.
'CUBE' (Character) The name of the resulting cube..
Input data -
This routine assumes that the first axis of the hcube data
represents wavelength, that the second and third represent the
X and Y dimensions of the image (this is an unfortunate,
since it means that the .X axis of the hypercube represents
wavelength, the .Y represents the image X axis and so forth)
and the fourth axis represents scan cycle number.
Output data -
CUBE is created with the same structure as HCUBE
except that the dta array will only have 3 dimensions, and any
AXIS(4) sub-structures that HCUBE has will be deleted.
KS / AAO 19th May 1986
FIGARO A general data reduction system