source: LMDZ6/trunk/libf/dyn3d/integrd.f90 @ 5274

!
! $Id: integrd.f90 5272 2024-10-24 15:53:15Z abarral $
!
SUBROUTINE integrd &
        (  nq,vcovm1,ucovm1,tetam1,psm1,massem1, &
        dv,du,dteta,dq,dp,vcov,ucov,teta,q,ps,masse,phis & !,finvmaold
        )

  use control_mod, only : planet_type
  use comconst_mod, only: pi
  USE logic_mod, ONLY: leapf
  use comvert_mod, only: ap, bp
  USE temps_mod, ONLY: dt

  USE dimensions_mod, ONLY: iim, jjm, llm, ndm
USE paramet_mod_h, ONLY: iip1, iip2, iip3, jjp1, llmp1, llmp2, llmm1, kftd, ip1jm, ip1jmp1, &
          ip1jmi1, ijp1llm, ijmllm, mvar, jcfil, jcfllm
IMPLICIT NONE


  !=======================================================================
  !
  !   Auteur:  P. Le Van
  !   -------
  !
  !   objet:
  !   ------
  !
  !   Incrementation des tendances dynamiques
  !
  !=======================================================================
  !-----------------------------------------------------------------------
  !   Declarations:
  !   -------------



  include "comgeom.h"
  include "iniprint.h"

  !   Arguments:
  !   ----------

  integer,intent(in) :: nq ! number of tracers to handle in this routine
  real,intent(inout) :: vcov(ip1jm,llm) ! covariant meridional wind
  real,intent(inout) :: ucov(ip1jmp1,llm) ! covariant zonal wind
  real,intent(inout) :: teta(ip1jmp1,llm) ! potential temperature
  real,intent(inout) :: q(ip1jmp1,llm,nq) ! advected tracers
  real,intent(inout) :: ps(ip1jmp1) ! surface pressure
  real,intent(inout) :: masse(ip1jmp1,llm) ! atmospheric mass
  real,intent(in) :: phis(ip1jmp1) ! ground geopotential !!! unused
  ! ! values at previous time step
  real,intent(inout) :: vcovm1(ip1jm,llm)
  real,intent(inout) :: ucovm1(ip1jmp1,llm)
  real,intent(inout) :: tetam1(ip1jmp1,llm)
  real,intent(inout) :: psm1(ip1jmp1)
  real,intent(inout) :: massem1(ip1jmp1,llm)
  ! ! the tendencies to add
  real,intent(in) :: dv(ip1jm,llm)
  real,intent(in) :: du(ip1jmp1,llm)
  real,intent(in) :: dteta(ip1jmp1,llm)
  real,intent(in) :: dp(ip1jmp1)
  real,intent(in) :: dq(ip1jmp1,llm,nq) !!! unused
   ! real,intent(out) :: finvmaold(ip1jmp1,llm) !!! unused

  !   Local:
  !   ------

  REAL :: vscr( ip1jm ),uscr( ip1jmp1 ),hscr( ip1jmp1 ),pscr(ip1jmp1)
  REAL :: massescr( ip1jmp1,llm )
   ! REAL finvmasse(ip1jmp1,llm)
  REAL :: p(ip1jmp1,llmp1)
  REAL :: tpn,tps,tppn(iim),tpps(iim)
  REAL :: qpn,qps,qppn(iim),qpps(iim)
  REAL :: deltap( ip1jmp1,llm )

  INTEGER :: l,ij,iq,i,j

  REAL :: SSUM

  !-----------------------------------------------------------------------

  DO  l = 1,llm
    DO  ij = 1,iip1
     ucov(    ij    , l) = 0.
     ucov( ij +ip1jm, l) = 0.
     uscr(     ij      ) = 0.
     uscr( ij +ip1jm   ) = 0.
    ENDDO
  ENDDO


  !    ............    integration  de       ps         ..............

  CALL SCOPY(ip1jmp1*llm, masse, 1, massescr, 1)

  DO ij = 1,ip1jmp1
   pscr (ij)    = ps(ij)
   ps (ij)      = psm1(ij) + dt * dp(ij)
  ENDDO
  !
  DO ij = 1,ip1jmp1
    IF( ps(ij).LT.0. ) THEN
     write(lunout,*) "integrd: negative surface pressure ",ps(ij)
     write(lunout,*) " at node ij =", ij
     ! ! since ij=j+(i-1)*jjp1 , we have
     j=modulo(ij,jjp1)
     i=1+(ij-j)/jjp1
     write(lunout,*) " lon = ",rlonv(i)*180./pi, " deg", &
           " lat = ",rlatu(j)*180./pi, " deg"
     call abort_gcm("integrd", "", 1)
    ENDIF
  ENDDO
  !
  DO  ij    = 1, iim
   tppn(ij) = aire(   ij   ) * ps(  ij    )
   tpps(ij) = aire(ij+ip1jm) * ps(ij+ip1jm)
  ENDDO
   tpn      = SSUM(iim,tppn,1)/apoln
   tps      = SSUM(iim,tpps,1)/apols
  DO ij   = 1, iip1
   ps(   ij   )  = tpn
   ps(ij+ip1jm)  = tps
  ENDDO
  !
  !  ... Calcul  de la nouvelle masse d'air au dernier temps integre t+1 ...
  !
  CALL pression ( ip1jmp1, ap, bp, ps, p )
  CALL massdair (     p  , masse         )

  ! Ehouarn : we don't use/need finvmaold and finvmasse,
        ! so might as well not compute them
   ! CALL   SCOPY( ijp1llm  , masse, 1, finvmasse,  1      )
   ! CALL filtreg( finvmasse, jjp1, llm, -2, 2, .TRUE., 1  )
  !

  !    ............   integration  de  ucov, vcov,  h     ..............

  DO l = 1,llm

   DO ij = iip2,ip1jm
    uscr( ij )   =  ucov( ij,l )
    ucov( ij,l ) = ucovm1( ij,l ) + dt * du( ij,l )
   ENDDO

   DO ij = 1,ip1jm
    vscr( ij )   =  vcov( ij,l )
    vcov( ij,l ) = vcovm1( ij,l ) + dt * dv( ij,l )
   ENDDO

   DO ij = 1,ip1jmp1
    hscr( ij )    =  teta(ij,l)
    teta ( ij,l ) = tetam1(ij,l) *  massem1(ij,l) / masse(ij,l) &
          + dt * dteta(ij,l) / masse(ij,l)
   ENDDO

  !   ....  Calcul de la valeur moyenne, unique  aux poles pour  teta    ......
  !
  !
   DO  ij   = 1, iim
    tppn(ij) = aire(   ij   ) * teta(  ij    ,l)
    tpps(ij) = aire(ij+ip1jm) * teta(ij+ip1jm,l)
   ENDDO
    tpn      = SSUM(iim,tppn,1)/apoln
    tps      = SSUM(iim,tpps,1)/apols

   DO ij   = 1, iip1
    teta(   ij   ,l)  = tpn
    teta(ij+ip1jm,l)  = tps
   ENDDO
  !

   IF(leapf)  THEN
     CALL SCOPY ( ip1jmp1, uscr(1), 1, ucovm1(1, l), 1 )
     CALL SCOPY (   ip1jm, vscr(1), 1, vcovm1(1, l), 1 )
     CALL SCOPY ( ip1jmp1, hscr(1), 1, tetam1(1, l), 1 )
   END IF

  ENDDO ! of DO l = 1,llm


  !
  !   .......  integration de   q   ......
  !
  !$$$      IF( iadv(1).NE.3.AND.iadv(2).NE.3 )    THEN
  !$$$c
  !$$$       IF( forward.OR. leapf )  THEN
  !$$$        DO iq = 1,2
  !$$$        DO  l = 1,llm
  !$$$        DO ij = 1,ip1jmp1
  !$$$        q(ij,l,iq) = ( q(ij,l,iq)*finvmaold(ij,l) + dtvr *dq(ij,l,iq) )/
  !$$$     $                            finvmasse(ij,l)
  !$$$        ENDDO
  !$$$        ENDDO
  !$$$        ENDDO
  !$$$       ELSE
  !$$$         DO iq = 1,2
  !$$$         DO  l = 1,llm
  !$$$         DO ij = 1,ip1jmp1
  !$$$         q( ij,l,iq ) = q( ij,l,iq ) * finvmaold(ij,l) / finvmasse(ij,l)
  !$$$         ENDDO
  !$$$         ENDDO
  !$$$         ENDDO
  !$$$
  !$$$       END IF
  !$$$c
  !$$$      ENDIF

  if (planet_type.eq."earth") then
  ! Earth-specific treatment of first 2 tracers (water)
    DO l = 1, llm
      DO ij = 1, ip1jmp1
        deltap(ij,l) =  p(ij,l) - p(ij,l+1)
      ENDDO
    ENDDO

    CALL qminimum( q, nq, deltap )

  !
  !    .....  Calcul de la valeur moyenne, unique  aux poles pour  q .....
  !

   DO iq = 1, nq
    DO l = 1, llm

       DO ij = 1, iim
         qppn(ij) = aire(   ij   ) * q(   ij   ,l,iq)
         qpps(ij) = aire(ij+ip1jm) * q(ij+ip1jm,l,iq)
       ENDDO
         qpn  =  SSUM(iim,qppn,1)/apoln
         qps  =  SSUM(iim,qpps,1)/apols

       DO ij = 1, iip1
         q(   ij   ,l,iq)  = qpn
         q(ij+ip1jm,l,iq)  = qps
       ENDDO

    ENDDO
   ENDDO

  ! Ehouarn: forget about finvmaold
   ! CALL  SCOPY( ijp1llm , finvmasse, 1, finvmaold, 1 )

  endif ! of if (planet_type.eq."earth")
  !
  !
  ! .....   FIN  de l'integration  de   q    .......

  !    .................................................................


  IF( leapf )  THEN
     CALL SCOPY (    ip1jmp1 ,  pscr   , 1,   psm1  , 1 )
     CALL SCOPY ( ip1jmp1*llm, massescr, 1,  massem1, 1 )
  END IF

  RETURN
END SUBROUTINE integrd