Last change
on this file since 2757 was
1572,
checked in by emillour, 8 years ago
|
All GCMs:
Further adaptations to keep up with changes in LMDZ5 concerning
physics/dynamics separation (up to rev r2500 of LMDZ5)
- arch:
- remove ifort debug option '-check all', replace it with
'-check bounds,format,output_conversion,pointers,uninit' (i.e.
get it to stop complaining about copying into temporary arrays)
- dyn3d_common:
- comconst_mod.F90 : add ngroup
- dyn3d:
- gcm.F90 : minor bug fix (arguments to a call_abort())
- leapfrog.F90 : recompute geopotential for bilan_dyn outputs
- conf_gcm.F90 : read "ngroup" from run.def
- groupe.F , groupeun.F : ngroup no longer a local parameter
- dyn3d_par:
- conf_gcm.F90 : read "ngroup" from run.def
- groupe_p.F , groupeun_p.F : ngroup no longer a local parameter
- misc:
- regr1_step_av_m.F90 : removed (not used)
- phy_common:
- mod_phys_lmdz_mpi_transfert.F90 , mod_phys_lmdz_mpi_data.F90 : change
is_north_pole and is_south_pole to is_north_pole_dyn and is_south_pole_dyn
- mod_phys_lmdz_omp_data.F90 : introduce is_nort_pole_phy and is_south_pole_phy
- dynphy_lonlat:
- mod_interface_dyn_phys.F90 : use is_north_pole_dyn and is_south_pole_dyn
- calfis_p.F : use is_north_pole_dyn and is_south_pole_dyn
- phyvenus:
- physiq_mod , write_hist*.h : use is_north_pole_phy and is_south_pole_phy
to correctly compute mesh area at poles to send to hist*nc files.
- phytitan:
- physiq_mod , write_hist*.h : use is_north_pole_phy and is_south_pole_phy
to correctly compute mesh area at poles to send to hist*nc files.
EM
|
File size:
1.2 KB
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1 | ! |
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2 | ! $Id: mod_interface_dyn_phys.F90 2351 2015-08-25 15:14:59Z emillour $ |
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3 | ! |
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4 | MODULE mod_interface_dyn_phys |
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5 | INTEGER,SAVE,dimension(:),allocatable :: index_i |
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6 | INTEGER,SAVE,dimension(:),allocatable :: index_j |
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7 | |
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8 | |
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9 | CONTAINS |
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10 | |
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11 | #ifdef CPP_PARA |
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12 | ! Interface with parallel physics, |
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13 | SUBROUTINE Init_interface_dyn_phys |
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14 | USE mod_phys_lmdz_mpi_data |
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15 | IMPLICIT NONE |
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16 | include 'dimensions.h' |
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17 | |
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18 | INTEGER :: i,j,k |
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19 | |
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20 | ALLOCATE(index_i(klon_mpi)) |
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21 | ALLOCATE(index_j(klon_mpi)) |
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22 | |
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23 | k=1 |
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24 | IF (is_north_pole_dyn) THEN |
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25 | index_i(k)=1 |
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26 | index_j(k)=1 |
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27 | k=2 |
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28 | ELSE |
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29 | DO i=ii_begin,iim |
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30 | index_i(k)=i |
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31 | index_j(k)=jj_begin |
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32 | k=k+1 |
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33 | ENDDO |
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34 | ENDIF |
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35 | |
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36 | DO j=jj_begin+1,jj_end-1 |
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37 | DO i=1,iim |
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38 | index_i(k)=i |
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39 | index_j(k)=j |
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40 | k=k+1 |
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41 | ENDDO |
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42 | ENDDO |
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43 | |
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44 | IF (is_south_pole_dyn) THEN |
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45 | index_i(k)=1 |
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46 | index_j(k)=jj_end |
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47 | ELSE |
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48 | DO i=1,ii_end |
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49 | index_i(k)=i |
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50 | index_j(k)=jj_end |
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51 | k=k+1 |
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52 | ENDDO |
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53 | ENDIF |
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54 | |
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55 | END SUBROUTINE Init_interface_dyn_phys |
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56 | #else |
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57 | SUBROUTINE Init_interface_dyn_phys |
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58 | ! dummy routine for seq case |
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59 | END SUBROUTINE Init_interface_dyn_phys |
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60 | #endif |
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61 | ! of #ifdef CPP_PARA |
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62 | END MODULE mod_interface_dyn_phys |
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