| Line | |
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| 1 | ! |
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| 2 | ! $Id$ |
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| 3 | ! |
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| 4 | SUBROUTINE gr_dyn_fi_p(nfield,im,jm,ngrid,pdyn,pfi) |
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| 5 | #ifdef CPP_PHYS |
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| 6 | ! Interface with parallel physics, |
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| 7 | USE mod_interface_dyn_phys |
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| 8 | USE dimphy |
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| 9 | USE PARALLEL |
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| 10 | IMPLICIT NONE |
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| 11 | c======================================================================= |
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| 12 | c passage d'un champ de la grille scalaire a la grille physique |
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| 13 | c======================================================================= |
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| 14 | |
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| 15 | c----------------------------------------------------------------------- |
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| 16 | c declarations: |
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| 17 | c ------------- |
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| 18 | |
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| 19 | INTEGER im,jm,ngrid,nfield |
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| 20 | REAL pdyn(im,jm,nfield) |
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| 21 | REAL pfi(ngrid,nfield) |
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| 22 | |
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| 23 | INTEGER i,j,ig,l |
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| 24 | |
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| 25 | c----------------------------------------------------------------------- |
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| 26 | c calcul: |
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| 27 | c ------- |
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| 28 | |
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| 29 | c IF(ngrid.NE.2+(jm-2)*(im-1)) STOP 'probleme de dim' |
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| 30 | c traitement des poles |
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| 31 | c traitement des point normaux |
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| 32 | c$OMP DO SCHEDULE(STATIC,OMP_CHUNK) |
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| 33 | DO l=1,nfield |
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| 34 | DO ig=1,klon |
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| 35 | i=index_i(ig) |
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| 36 | j=index_j(ig) |
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| 37 | pfi(ig,l)=pdyn(i,j,l) |
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| 38 | ENDDO |
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| 39 | ENDDO |
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| 40 | c$OMP END DO NOWAIT |
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| 41 | #endif |
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| 42 | ! of #ifdef CPP_PHYS |
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| 43 | RETURN |
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| 44 | END |
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