| [1279] | 1 | ! |
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| 2 | ! $Id: gr_fi_dyn_p.F 1279 2009-12-10 09:02:56Z jghattas $ |
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| 3 | ! |
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| [630] | 4 | SUBROUTINE gr_fi_dyn_p(nfield,ngrid,im,jm,pfi,pdyn) |
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| [1279] | 5 | #ifdef CPP_EARTH |
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| 6 | ! Interface with parallel physics, |
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| 7 | ! for now this routine only works with Earth physics |
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| [774] | 8 | USE mod_interface_dyn_phys |
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| 9 | USE dimphy |
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| [630] | 10 | use parallel |
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| 11 | IMPLICIT NONE |
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| 12 | c======================================================================= |
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| 13 | c passage d'un champ de la grille scalaire a la grille physique |
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| 14 | c======================================================================= |
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| 15 | |
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| 16 | c----------------------------------------------------------------------- |
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| 17 | c declarations: |
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| 18 | c ------------- |
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| 19 | |
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| 20 | INTEGER im,jm,ngrid,nfield |
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| 21 | REAL pdyn(im,jm,nfield) |
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| 22 | REAL pfi(ngrid,nfield) |
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| 23 | |
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| 24 | INTEGER i,j,ifield,ig |
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| 25 | |
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| 26 | c----------------------------------------------------------------------- |
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| 27 | c calcul: |
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| 28 | c ------- |
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| [764] | 29 | c$OMP DO SCHEDULE(STATIC,OMP_CHUNK) |
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| [630] | 30 | DO ifield=1,nfield |
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| 31 | |
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| 32 | do ig=1,klon |
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| [774] | 33 | i=index_i(ig) |
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| 34 | j=index_j(ig) |
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| [630] | 35 | pdyn(i,j,ifield)=pfi(ig,ifield) |
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| 36 | if (i==1) pdyn(im,j,ifield)=pdyn(i,j,ifield) |
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| 37 | enddo |
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| 38 | |
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| 39 | c traitement des poles |
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| 40 | if (pole_nord) then |
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| 41 | do i=1,im |
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| 42 | pdyn(i,1,ifield)=pdyn(1,1,ifield) |
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| 43 | enddo |
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| 44 | endif |
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| 45 | |
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| 46 | if (pole_sud) then |
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| 47 | do i=1,im |
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| 48 | pdyn(i,jm,ifield)=pdyn(1,jm,ifield) |
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| 49 | enddo |
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| 50 | endif |
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| 51 | |
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| 52 | ENDDO |
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| [764] | 53 | c$OMP END DO NOWAIT |
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| [1279] | 54 | #else |
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| 55 | write(lunout,*) "gr_fi_dyn_p : This routine should not be called", |
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| 56 | & "without parallelized physics" |
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| 57 | stop |
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| 58 | #endif |
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| 59 | ! of #ifdef CPP_EARTH |
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| [630] | 60 | RETURN |
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| 61 | END |
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