source: LMDZ5/branches/AI-cosp/libf/dyn3d_common/convmas.F90

Last change on this file was 2336, checked in by dcugnet, 9 years ago
  • Add parallel capability for ce0l.
  • Small bug in grid_noro fixed (smoothed topography was used instead of unsmoothed one for geopotential computation at north pole).
  • Removed average of mass at poles in etat0dyn_netcdf after start_init_dyn => different results in the zoomed grid case.
  • ok_etat0=n and ok_limit=y combination now works fine (if no initial state is needed, but only limit.nc file). This required:
    • to move grid_noro0 and start_init_noro0 subroutines from etat0dyn_netcdf.F90 to limit_netcdf.F90
    • to create init_ssrf_m.F90 file, so that sub-surfaces can be initialized from limit_netcdf.F90 without any etat0*_netcdf routines call).
  • Simplified somehow the corresponding code, in particular: 1) removed obsolete flags "oldice". 2) removed flag "ibar": barycentric interpolation is used everywhere (except in start_init_subsurf, still calling grille_m - to be changed soon). 3) removed useless CPP_PHY precompilation directives, considering the possibility to run ce0l without physics is useless (ce0l is dedicated to Earth physics).
  • Property copyright set to
    Name of program: LMDZ
    Creation date: 1984
    Version: LMDZ5
    License: CeCILL version 2
    Holder: Laboratoire de m\'et\'eorologie dynamique, CNRS, UMR 8539
    See the license file in the root directory
  • Property svn:eol-style set to native
  • Property svn:keywords set to Author Date Id Revision
File size: 1.3 KB
Line 
1SUBROUTINE convmas (pbaru, pbarv, convm)
2!
3!-------------------------------------------------------------------------------
4! Authors: P. Le Van , Fr. Hourdin.
5!-------------------------------------------------------------------------------
6! Purpose: Compute mass flux convergence at p levels.
7  IMPLICIT NONE
8  include "dimensions.h"
9  include "paramet.h"
10  include "comgeom.h"
11  include "logic.h"
12!===============================================================================
13! Arguments:
14  REAL, INTENT(IN)  :: pbaru(ip1jmp1,llm)
15  REAL, INTENT(IN)  :: pbarv(ip1jm  ,llm)
16  REAL, INTENT(OUT) :: convm(ip1jmp1,llm)
17!===============================================================================
18! Method used:   Computation from top to bottom.
19!   Mass convergence at level llm is equal to zero and is not stored in convm.
20!===============================================================================
21! Local variables:
22  INTEGER :: l
23!===============================================================================
24
25!--- Computation of - (d(pbaru)/dx + d(pbarv)/dy )
26  CALL convflu( pbaru, pbarv, llm, convm )
27
28!--- Filter
29  CALL filtreg( convm, jjp1, llm, 2, 2, .TRUE., 1 )
30
31!--- Mass convergence is integrated from top to bottom
32  DO l=llmm1,1,-1
33    convm(:,l) = convm(:,l) + convm(:,l+1)
34  END DO
35
36END SUBROUTINE convmas
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