|
Last change
on this file since 1632 was
1543,
checked in by emillour, 10 years ago
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|
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
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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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