|
Last change
on this file since 2604 was
1572,
checked in by emillour, 9 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
|
| Line | |
|---|
| 1 | ! |
|---|
| 2 | ! $Id: mod_interface_dyn_phys.F90 2351 2015-08-25 15:14:59Z emillour $ |
|---|
| 3 | ! |
|---|
| 4 | MODULE mod_interface_dyn_phys |
|---|
| 5 | INTEGER,SAVE,dimension(:),allocatable :: index_i |
|---|
| 6 | INTEGER,SAVE,dimension(:),allocatable :: index_j |
|---|
| 7 | |
|---|
| 8 | |
|---|
| 9 | CONTAINS |
|---|
| 10 | |
|---|
| 11 | #ifdef CPP_PARA |
|---|
| 12 | ! Interface with parallel physics, |
|---|
| 13 | SUBROUTINE Init_interface_dyn_phys |
|---|
| 14 | USE mod_phys_lmdz_mpi_data |
|---|
| 15 | IMPLICIT NONE |
|---|
| 16 | include 'dimensions.h' |
|---|
| 17 | |
|---|
| 18 | INTEGER :: i,j,k |
|---|
| 19 | |
|---|
| 20 | ALLOCATE(index_i(klon_mpi)) |
|---|
| 21 | ALLOCATE(index_j(klon_mpi)) |
|---|
| 22 | |
|---|
| 23 | k=1 |
|---|
| 24 | IF (is_north_pole_dyn) THEN |
|---|
| 25 | index_i(k)=1 |
|---|
| 26 | index_j(k)=1 |
|---|
| 27 | k=2 |
|---|
| 28 | ELSE |
|---|
| 29 | DO i=ii_begin,iim |
|---|
| 30 | index_i(k)=i |
|---|
| 31 | index_j(k)=jj_begin |
|---|
| 32 | k=k+1 |
|---|
| 33 | ENDDO |
|---|
| 34 | ENDIF |
|---|
| 35 | |
|---|
| 36 | DO j=jj_begin+1,jj_end-1 |
|---|
| 37 | DO i=1,iim |
|---|
| 38 | index_i(k)=i |
|---|
| 39 | index_j(k)=j |
|---|
| 40 | k=k+1 |
|---|
| 41 | ENDDO |
|---|
| 42 | ENDDO |
|---|
| 43 | |
|---|
| 44 | IF (is_south_pole_dyn) THEN |
|---|
| 45 | index_i(k)=1 |
|---|
| 46 | index_j(k)=jj_end |
|---|
| 47 | ELSE |
|---|
| 48 | DO i=1,ii_end |
|---|
| 49 | index_i(k)=i |
|---|
| 50 | index_j(k)=jj_end |
|---|
| 51 | k=k+1 |
|---|
| 52 | ENDDO |
|---|
| 53 | ENDIF |
|---|
| 54 | |
|---|
| 55 | END SUBROUTINE Init_interface_dyn_phys |
|---|
| 56 | #else |
|---|
| 57 | SUBROUTINE Init_interface_dyn_phys |
|---|
| 58 | ! dummy routine for seq case |
|---|
| 59 | END SUBROUTINE Init_interface_dyn_phys |
|---|
| 60 | #endif |
|---|
| 61 | ! of #ifdef CPP_PARA |
|---|
| 62 | END MODULE mod_interface_dyn_phys |
|---|
Note: See
TracBrowser
for help on using the repository browser.