source: trunk/LMDZ.COMMON/libf/dyn3d_common/convmas.F90

Last change on this file was 1523, checked in by emillour, 9 years ago

All models: More updates to make planetary codes (+Earth) setups converge.

  • in dyn3d_common:
  • convmas.F => convmas.F90
  • enercin.F => enercin.F90
  • flumass.F => flumass.F90
  • massbar.F => massbar.F90
  • tourpot.F => tourpot.F90
  • vitvert.F => vitvert.F90
  • in misc:
  • move "q_sat" from "dyn3d_common" to "misc" (in Earth model, it is also called by the physics)
  • move "write_field" from "dyn3d_common" to "misc"(may be called from physics or dynamics and depends on neither).
  • in phy_common:
  • move "write_field_phy" here since it may be called from any physics package)
  • add module "regular_lonlat_mod" to store global information on lon-lat grid
  • in dynlonlat_phylonlat/phy*:
  • turn "iniphysiq.F90" into module "iniphysiq_mod.F90" (and of course adapt gcm.F[90] and 1D models accordingly)

EM
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!===============================================================================
12! Arguments:
13  REAL, INTENT(IN)  :: pbaru(ip1jmp1,llm)
14  REAL, INTENT(IN)  :: pbarv(ip1jm  ,llm)
15  REAL, INTENT(OUT) :: convm(ip1jmp1,llm)
16!===============================================================================
17! Method used:   Computation from top to bottom.
18!   Mass convergence at level llm is equal to zero and is not stored in convm.
19!===============================================================================
20! Local variables:
21  INTEGER :: l
22!===============================================================================
23
24!--- Computation of - (d(pbaru)/dx + d(pbarv)/dy )
25  CALL convflu( pbaru, pbarv, llm, convm )
26
27!--- Filter
28  CALL filtreg( convm, jjp1, llm, 2, 2, .TRUE., 1 )
29
30!--- Mass convergence is integrated from top to bottom
31  DO l=llmm1,1,-1
32    convm(:,l) = convm(:,l) + convm(:,l+1)
33  END DO
34
35END SUBROUTINE convmas
Note: See TracBrowser for help on using the repository browser.