CCG_FM3x
- Combines data lines using a fast median
Description:
This routine accepts an array consisting a series of (vectorised)
lines of data. The data values in the lines are then combined to
form a (fast) median line. This method uses no weights and
returns no variances.
The method used is based on Wirth's algorithm for selecting the
Kth value, which is very fast compared to a full sort.
The output medians are returned in the array RESULT.
Invocation:
CALL CCG_FM3x( NPIX, NLINES, STACK, MINPIX, RESULT, WRK1, NCON,
POINT, USED, NCON, NBAD, STATUS )
Arguments:
NPIX = INTEGER (Given)
The number of pixels in a line of data.
NLINES = INTEGER (Given)
The number of lines of data in the stack.
STACK( NPIX, NLINES ) = ? (Given)
The array of lines which are to be combined into a single line.
MINPIX = INTEGER (Given)
The minimum number of pixels required to contribute to an
output pixel.
RESULT( NPIX ) = ? (Returned)
The output line of data.
WRK1( NLINES ) = ? (Returned)
Workspace for calculations.
POINT( NLINES ) = INTEGER (Returned)
Workspace to hold pointers to the original positions of the
data before extraction and conversion in to the WRK1 array.
USED( NLINES ) = LOGICAL (Returned)
Workspace used to indicate which values have been used in
estimating a resultant value.
NCON( NLINES ) = DOUBLE PRECISION (Returned)
The actual number of contributing pixels from each input line
to the output line.
NBAD = INTEGER (Returned)
The number of bad values in the output array created while
forming the statistics. It excludes those bad values whose
corresponding values along the collapse axis are all bad.
STATUS = INTEGER (Given and Returned)
The global status.
Notes:
There is a routine for real and double-precision: replace "x"
in the routine name by D or R as appropriate. The STACK, RESULT,
and WRK1 arguments supplied to the routine must have the data type
specified.
KAPLIBS -- Internal subroutines used within the KAPPA package. Starlink User Note 238 D.S. Berry Malcolm J. Currie 9th March 2009 E-mail:ussc@star.rl.ac.uk