F I G S 4 2 2
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.
Command parameters -
'HCUBE' (Character) The name of the hypercube to be processed.
'XSTART' (Real) The start of the wavelength range to be included.
'XEND' (Real) The end of the wavelength range to be included.
'CYSTART' (Integer) The first cycle to be included.
'CYEND' (Integer) The last cycle to be included.
'IMAGE' (Character) The name of the resulting image.
Command keywords -
'SPLIT' If set, FIGS422 will create a number of output
files, one for each cycle in the specified range,
rather than just one with all the cycles in the range
summed. In this case, the output files will be named
using the name specified using 'IMAGE', but with the
cycle number appended.
Input data -
HCUBE is assumed is the actual hypercube data.
This routine assumes that the first axis of the cube 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 AXIS(1) structure of the hypercube represents
wavelength, the AXIS(2) represents the image X axis and so forth)
and the fourth axis represents scan cycle number.
Output data -
IMAGE is created with the same structure as HCUBE
except that the main data array will only have 2 dimensions, and any
AXIS sub-structures that HCUBE has will be
deleted/renamed as appropriate.
KS / AAO 6th Jan 1985
FIGARO A general data reduction system