Last change
on this file since 1543 was
1543,
checked in by emillour, 9 years ago
|
All models: Further adaptations to keep up with changes in LMDZ5 concerning
physics/dynamics separation:
- dyn3d:
- adapted gcm.F so that all physics initializations are now done in iniphysiq.
- dyn3dpar:
- adapted gcm.F so that all physics initializations are now done in iniphysiq.
- updated calfis_p.F to follow up with changes.
- copied over updated "bands.F90" from LMDZ5.
- dynphy_lonlat:
- calfis_p.F90, mod_interface_dyn_phys.F90,
follow up of changes in phy_common/mod_* routines
- phy_common:
- added "geometry_mod.F90" to store information about the grid (replaces
phy*/comgeomphy.F90) and give variables friendlier names: rlond =>
longitude , rlatd => latitude, airephy => cell_area,
cuphy => dx , cvphy => dy
- added "physics_distribution_mod.F90"
- updated "mod_grid_phy_lmdz.F90", "mod_phys_lmdz_mpi_data.F90",
"mod_phys_lmdz_para.F90", "mod_phys_lmdz_mpi_transfert.F90",
"mod_grid_phy_lmdz.F90", "mod_phys_lmdz_omp_data.F90",
"mod_phys_lmdz_omp_transfert.F90", "write_field_phy.F90"
and "ioipsl_getin_p_mod.F90" to LMDZ5 versions.
- phy[venus/titan/mars/std]:
- removed "init_phys_lmdz.F90", "comgeomphy.F90"; adapted routines to use
geometry_mod (longitude, latitude, cell_area, etc.)
EM
|
File size:
1.1 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) 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) 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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