source: LMDZ5/trunk/libf/dyn3dpar/gr_dyn_fi_p.F @ 1992

Last change on this file since 1992 was 1907, checked in by lguez, 11 years ago

Added a copyright property to every file of the distribution, except
for the fcm files (which have their own copyright). Use svn propget on
a file to see the copyright. For instance:

$ svn propget copyright libf/phylmd/physiq.F90
Name of program: LMDZ
Creation date: 1984
Version: LMDZ5
License: CeCILL version 2
Holder: Laboratoire de m\'et\'eorologie dynamique, CNRS, UMR 8539
See the license file in the root directory

Also added the files defining the CeCILL version 2 license, in French
and English, at the top of the LMDZ tree.

  • Property copyright set to
    Name of program: LMDZ
    Creation date: 1984
    Version: LMDZ5
    License: CeCILL version 2
    Holder: Laboratoire de m\'et\'eorologie dynamique, CNRS, UMR 8539
    See the license file in the root directory
  • Property svn:eol-style set to native
  • Property svn:keywords set to Author Date Id Revision
File size: 1.1 KB
Line 
1!
2! $Id: gr_dyn_fi_p.F 1907 2013-11-26 13:10:46Z lguez $
3!
4      SUBROUTINE gr_dyn_fi_p(nfield,im,jm,ngrid,pdyn,pfi)
5#ifdef CPP_PHYS
6! Interface with parallel physics,
7      USE mod_interface_dyn_phys
8      USE dimphy
9      USE parallel_lmdz
10      IMPLICIT NONE
11c=======================================================================
12c   passage d'un champ de la grille scalaire a la grille physique
13c=======================================================================
14
15c-----------------------------------------------------------------------
16c   declarations:
17c   -------------
18
19      INTEGER im,jm,ngrid,nfield
20      REAL pdyn(im,jm,nfield)
21      REAL pfi(ngrid,nfield)
22
23      INTEGER i,j,ig,l
24
25c-----------------------------------------------------------------------
26c   calcul:
27c   -------
28
29c      IF(ngrid.NE.2+(jm-2)*(im-1)) STOP 'probleme de dim'
30c   traitement des poles
31c   traitement des point normaux
32c$OMP DO SCHEDULE(STATIC,OMP_CHUNK)
33      DO l=1,nfield   
34       DO ig=1,klon
35         i=index_i(ig)
36         j=index_j(ig)
37         pfi(ig,l)=pdyn(i,j,l)
38       ENDDO
39      ENDDO
40c$OMP END DO NOWAIT
41#endif
42! of #ifdef CPP_PHYS
43      RETURN
44      END
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