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CCG_RMS3x
- Combines data lines using the root mean square
- Description:
- This routine accepts an array consisting a series of (vectorised)
lines of data. The data values in each lines are then combined to
form the roor mean square of the values. The output rot mean
squares are returned in the array RESULT.
- Invocation:
- CALL CCG_RMS3x( NPIX, NLINES, STACK, MINPIX, RESULT, RESVAR,
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.
-
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:
- This routine performs its work in double precision.
- There is a routine for each numeric data type: replace "x" in
the routine name by D, R, I, W, UW, B or UB as appropriate. The
STACK and RESULT arguments supplied to the routine must
have the data type specified.
Next: CCG_SCR1 - Combines data lines using a sigma-clipped mean
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Previous: CCG_RMS1x - Combines data lines using the root mean square
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
Copyright © 2010 Science and Technology Facilities Council