C @(#)rctscl.for	17.1.1.1 (ES0-DMD) 01/25/02 17:19:01
C===========================================================================
C Copyright (C) 1995 European Southern Observatory (ESO)
C
C This program is free software; you can redistribute it and/or 
C modify it under the terms of the GNU General Public License as 
C published by the Free Software Foundation; either version 2 of 
C the License, or (at your option) any later version.
C
C This program is distributed in the hope that it will be useful,
C but WITHOUT ANY WARRANTY; without even the implied warranty of
C MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the
C GNU General Public License for more details.
C
C You should have received a copy of the GNU General Public 
C License along with this program; if not, write to the Free 
C Software Foundation, Inc., 675 Massachusetss Ave, Cambridge, 
C MA 02139, USA.
C
C Corresponding concerning ESO-MIDAS should be addressed as follows:
C	Internet e-mail: midas@eso.org
C	Postal address: European Southern Observatory
C			Data Management Division 
C			Karl-Schwarzschild-Strasse 2
C			D 85748 Garching bei Muenchen 
C			GERMANY
C===========================================================================
C
      SUBROUTINE RCTSCL(SUB,IN)
C +++
C.PURPOSE: This subroutine compares the sum of the fluxes in the individual
C          subpixels to the flux in the original input pixel. The fluxes in
C          the subpixels are then scaled such that their sum equals the
C          original flux. Hence, flux conservation should be achieved on the
C          pixel scale.
C ---
      IMPLICIT   NONE
      REAL       SUB(3,3)
      REAL       IN
C
      REAL       SUM,SCALE
      INTEGER    K
      INTEGER    L
C
      SCALE  = 1
      SUM    = SUB(1,1) + SUB(1,2) + SUB(1,3) + SUB(2,1) + SUB(2,2) +
     +         SUB(2,3) + SUB(3,1) + SUB(3,2) + SUB(3,3)
C  
      IF (SUM.NE.0) THEN     ! assume sum does not vanish due to neg. fluxes ...
         SCALE  = IN/SUM 
      ENDIF
C
      DO 20 K = 1,3
         DO 10 L = 1,3
            SUB(K,L) = SUB(K,L)*SCALE
   10    CONTINUE
   20 CONTINUE
C
      RETURN
      END