source: trunk/LMDZ.COMMON/libf/dyn3dpar/gr_dyn_fi_p.F @ 1243

Last change on this file since 1243 was 1019, checked in by emillour, 11 years ago

Common dynamics; keep up with updates (seq and ) in LMDZ5 (up tio rev 1845):

  • General stuff:
  • makelmdz_fcm: add options -j # (compile using # threads) and -full, and to keep up

with Earth model, possibility to compile with various versions of orchidee

  • bld.cfg: adaptations to enable compiling using multiple threads
  • build_gcm: adaptations to enable compiling using multiple threads
  • makelmdz: keep up with Earth model: possibility to compile with various versions of orchidee + cosmetic changes + library directory name change
  • bibio:
  • wxios.F90 : Added for possible future use of XIOS library
  • filtrez:
  • mkl_dft_type.f90 & mkl_dfti.f90 : MKL (for MKL FFT) interface definitions
  • filtreg_mod : limit use of FFT to parallel mode
  • mod_filtre_fft.F90 & mod_filtre_fft_lov.F90 : swich to use parallel_lmdz
  • dyn3d:
  • abort_gcm.F : add things for xios
  • advtrac.F90 : minor change in CFL outputs
  • ce0l.F90 : indicesol.h is now module indice_sol_mod
  • comvert.h : cosmetic change on comments
  • gcm.F : add xios and use module indice_sol_mod (for INCA)
  • inigeom.F : move two computations outside loop
  • dyn3dpar:
  • parallel.F90 => parallel_lmdz.F90 : and change all the "use parallel" into "use parallel_lmdz" in all files in dyn3dpar
  • comvert.h : cosmetic change on comments
  • gcm.F : add xios and use module indice_sol_mod (for INCA)
  • leapfrog_p.F : add xios + correction for times in Newtonian case
  • ce0l.F90 : indicesol.h is now module indice_sol_mod
  • inigeom.F : move two computations outside loop

EM
File size: 1.1 KB
Line 
1!
2! $Id: gr_dyn_fi_p.F 1615 2012-02-10 15:42:26Z emillour $
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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