source: trunk/LMDZ.COMMON/libf/dyn3dpar/gr_fi_dyn_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: 1.3 KB
Line 
1!
2! $Id: gr_fi_dyn_p.F 1615 2012-02-10 15:42:26Z emillour $
3!
4      SUBROUTINE gr_fi_dyn_p(nfield,ngrid,im,jm,pfi,pdyn)
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,ifield,ig
24
25c-----------------------------------------------------------------------
26c   calcul:
27c   -------
28c$OMP DO SCHEDULE(STATIC,OMP_CHUNK)
29      DO ifield=1,nfield
30
31        do ig=1,klon
32          i=index_i(ig)
33          j=index_j(ig)
34          pdyn(i,j,ifield)=pfi(ig,ifield)
35          if (i==1) pdyn(im,j,ifield)=pdyn(i,j,ifield)
36        enddo
37
38c   traitement des poles
39      if (pole_nord) then
40        do i=1,im
41          pdyn(i,1,ifield)=pdyn(1,1,ifield)
42        enddo
43      endif
44       
45      if (pole_sud) then
46        do i=1,im
47          pdyn(i,jm,ifield)=pdyn(1,jm,ifield)
48        enddo
49      endif
50     
51      ENDDO
52c$OMP END DO NOWAIT
53#endif
54! of #ifdef CPP_PHYS
55      RETURN
56      END
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