Last change
on this file since 1682 was
1682,
checked in by emillour, 8 years ago
|
All GCMs: set things up to enable pluging physics with dynamico
- dyn3d
- gcm.F90 : move I/O initialization (dates) to be done before physics
initialization
- dyn3dpar
- gcm.F : move I/O initialization (dates) to be done before physics
initialization
- dynphy_lonlat:
- inigeomphy_mod.F90 : add ind_cell_glo computation and transfer
to init_geometry
- phy_common:
- geometry_mod.F90 : add ind_cell_glo module variable to store global
column index
- print_control_mod.F90 : make initialization occur via init_print_control_mod
to avoid circular module dependencies
- init_print_control_mod.F90 : added to initialize print_control_mod module
variables
- mod_phys_lmdz_mpi_data.F90 : use print_control_mod (rather than iniprint.h)
- mod_phys_lmdz_para.F90 : use print_control_mod (rather than iniprint.h)
- mod_phys_lmdz_omp_data.F90 : add is_omp_master (alias of is_omp_root) module
variable and use print_control_mod (rather than
iniprint.h)
- physics_distribution_mod.F90 : add call to init_dimphy in
init_physics_distribution
- xios_writefield.F90 : generic routine to output field with XIOS (for debug)
- misc:
- handle_err_m.F90 : call abort_physic, rather than abort_gcm
- wxios.F90 : updates to enable unstructured grids
set module variable g_ctx_name to "LMDZ"
wxios_init(): remove call to wxios_context_init
wxios_context_init(): call xios_context_initialize with COMM_LMDZ_PHY
add routine wxios_set_context() to get handle and set context to XIOS
wxios_domain_param(): change arguments and generate the domain in-place
add wxios_domain_param_unstructured(): generate domain for unstructured case
NB: access is via "domain group" (whereas it is via "domain" in
wxios_domain_param)
- dynphy_lonlat/phy[std|mars|venus|titan]:
- iniphysiq_mod.F90 : Remove call to init_dimphy (which is now done in
phy_common/physics_distribution_mod.F90)
EM
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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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