source: LMDZ6/trunk/libf/dyn3d_common/diagedyn.f90 @ 5423

!
! $Id: diagedyn.f90 5285 2024-10-28 13:33:29Z evignon $
!

!======================================================================
SUBROUTINE diagedyn(tit,iprt,idiag,idiag2,dtime &
        , ucov    , vcov , ps, p ,pk , teta , q, ql)
  !======================================================================
  !
  ! Purpose:
  !    Calcul la difference d'enthalpie et de masse d'eau entre 2 appels,
  !    et calcul le flux de chaleur et le flux d'eau necessaire a ces
  !    changements. Ces valeurs sont moyennees sur la surface de tout
  !    le globe et sont exprime en W/2 et kg/s/m2
  !    Outil pour diagnostiquer la conservation de l'energie
  !    et de la masse dans la dynamique.
  !
  !
  !======================================================================
  ! Arguments:
  ! tit-----imput-A15- Comment added in PRINT (CHARACTER*15)
  ! iprt----input-I-  PRINT level ( <=1 : no PRINT)
  ! idiag---input-I- indice dans lequel sera range les nouveaux
  !              bilans d' entalpie et de masse
  ! idiag2--input-I-les nouveaux bilans d'entalpie et de masse
  !             sont compare au bilan de d'enthalpie de masse de
  !             l'indice numero idiag2
  !             Cas parriculier : si idiag2=0, pas de comparaison, on
  !             sort directement les bilans d'enthalpie et de masse
  ! dtime----input-R- time step (s)
  ! uconv, vconv-input-R- vents covariants (m/s)
  ! ps-------input-R- Surface pressure (Pa)
  ! p--------input-R- pressure at the interfaces
  ! pk-------input-R- pk= (p/Pref)**kappa
  ! teta-----input-R- potential temperature (K)
  ! q--------input-R- vapeur d'eau (kg/kg)
  ! ql-------input-R- liquid watter (kg/kg)
  ! aire-----input-R- mesh surafce (m2)
  !
  ! the following total value are computed by UNIT of earth surface
  !
  ! d_h_vcol--output-R- Heat flux (W/m2) define as the Enthalpy
  !        change (J/m2) during one time step (dtime) for the whole
  !        atmosphere (air, watter vapour, liquid and solid)
  ! d_qt------output-R- total water mass flux (kg/m2/s) defined as the
  !       total watter (kg/m2) change during one time step (dtime),
  ! d_qw------output-R- same, for the watter vapour only (kg/m2/s)
  ! d_ql------output-R- same, for the liquid watter only (kg/m2/s)
  ! d_ec------output-R- Cinetic Energy Budget (W/m2) for vertical air column
  !
  !
  ! J.L. Dufresne, July 2002
  !======================================================================

  USE iniprint_mod_h
  USE comgeom_mod_h
  USE control_mod, ONLY : planet_type

  USE dimensions_mod, ONLY: iim, jjm, llm, ndm
USE paramet_mod_h
IMPLICIT NONE
  !



  ! Ehouarn: for now set these parameters to what is in Earth physics...
   !     (cf ../phylmd/suphel.h)
   !     this should be generalized...
  REAL,PARAMETER :: RCPD= &
        3.5*(1000.*(6.0221367E+23*1.380658E-23)/28.9644)
  REAL,PARAMETER :: RCPV= &
        4.*(1000.*(6.0221367E+23*1.380658E-23)/18.0153)
  REAL,PARAMETER :: RCS=RCPV
  REAL,PARAMETER :: RCW=RCPV
  REAL,PARAMETER :: RLSTT=2.8345E+6
  REAL,PARAMETER :: RLVTT=2.5008E+6
  !
  !
  INTEGER :: imjmp1
  PARAMETER( imjmp1=iim*jjp1)
  ! Input variables
  CHARACTER(len=15) :: tit
  INTEGER :: iprt,idiag, idiag2
  REAL :: dtime
  REAL :: vcov(ip1jm,llm),ucov(ip1jmp1,llm) ! vents covariants
  REAL :: ps(ip1jmp1)                       ! pression  au sol
  REAL :: p (ip1jmp1,llmp1  )  ! pression aux interfac.des couches
  REAL :: pk (ip1jmp1,llm  )  ! = (p/Pref)**kappa
  REAL :: teta(ip1jmp1,llm)                 ! temperature potentielle
  REAL :: q(ip1jmp1,llm)               ! champs eau vapeur
  REAL :: ql(ip1jmp1,llm)               ! champs eau liquide


  ! Output variables
  REAL :: d_h_vcol, d_qt, d_qw, d_ql, d_qs, d_ec
  !
  ! Local variables
  !
  REAL :: h_vcol_tot, h_dair_tot, h_qw_tot, h_ql_tot &
        , h_qs_tot, qw_tot, ql_tot, qs_tot , ec_tot
  ! h_vcol_tot--  total enthalpy of vertical air column
         ! (air with watter vapour, liquid and solid) (J/m2)
  ! h_dair_tot-- total enthalpy of dry air (J/m2)
  ! h_qw_tot----  total enthalpy of watter vapour (J/m2)
  ! h_ql_tot----  total enthalpy of liquid watter (J/m2)
  ! h_qs_tot----  total enthalpy of solid watter  (J/m2)
  ! qw_tot------  total mass of watter vapour (kg/m2)
  ! ql_tot------  total mass of liquid watter (kg/m2)
  ! qs_tot------  total mass of solid watter (kg/m2)
  ! ec_tot------  total cinetic energy (kg/m2)
  !
  REAL :: masse(ip1jmp1,llm)                ! masse d'air
  REAL :: vcont(ip1jm,llm),ucont(ip1jmp1,llm)
  REAL :: ecin(ip1jmp1,llm)

  REAL :: zaire(imjmp1)
  REAL :: zps(imjmp1)
  REAL :: zairm(imjmp1,llm)
  REAL :: zecin(imjmp1,llm)
  REAL :: zpaprs(imjmp1,llm)
  REAL :: zpk(imjmp1,llm)
  REAL :: zt(imjmp1,llm)
  REAL :: zh(imjmp1,llm)
  REAL :: zqw(imjmp1,llm)
  REAL :: zql(imjmp1,llm)
  REAL :: zqs(imjmp1,llm)

  REAL :: zqw_col(imjmp1)
  REAL :: zql_col(imjmp1)
  REAL :: zqs_col(imjmp1)
  REAL :: zec_col(imjmp1)
  REAL :: zh_dair_col(imjmp1)
  REAL :: zh_qw_col(imjmp1), zh_ql_col(imjmp1), zh_qs_col(imjmp1)
  !
  REAL :: d_h_dair, d_h_qw, d_h_ql, d_h_qs
  !
  REAL :: airetot, zcpvap, zcwat, zcice
  !
  INTEGER :: i, k, jj, ij , l ,ip1jjm1
  !
  INTEGER :: ndiag     ! max number of diagnostic in parallel
  PARAMETER (ndiag=10)
  integer :: pas(ndiag)
  save pas
  data pas/ndiag*0/
  !
  REAL :: h_vcol_pre(ndiag), h_dair_pre(ndiag), h_qw_pre(ndiag) &
        , h_ql_pre(ndiag), h_qs_pre(ndiag), qw_pre(ndiag) &
        , ql_pre(ndiag), qs_pre(ndiag) , ec_pre(ndiag)
  SAVE      h_vcol_pre, h_dair_pre, h_qw_pre, h_ql_pre &
        , h_qs_pre, qw_pre, ql_pre, qs_pre , ec_pre


  !#ifdef CPP_EARTH
  IF (planet_type=="earth") THEN

  !======================================================================
  ! Compute Kinetic enrgy
  CALL covcont  ( llm    , ucov    , vcov , ucont, vcont        )
  CALL enercin ( vcov   , ucov  , vcont     , ucont  , ecin  )
  CALL massdair( p, masse )
  !======================================================================
  !
  !
  print*,'MAIS POURQUOI DONC DIAGEDYN NE MARCHE PAS ?'
  return
  ! On ne garde les donnees que dans les colonnes i=1,iim
  DO jj = 1,jjp1
    ip1jjm1=iip1*(jj-1)
    DO ij =  1,iim
      i=iim*(jj-1)+ij
      zaire(i)=aire(ij+ip1jjm1)
      zps(i)=ps(ij+ip1jjm1)
    ENDDO
  ENDDO
  ! 3D arrays
  DO l  =  1, llm
    DO jj = 1,jjp1
      ip1jjm1=iip1*(jj-1)
      DO ij =  1,iim
        i=iim*(jj-1)+ij
        zairm(i,l) = masse(ij+ip1jjm1,l)
        zecin(i,l) = ecin(ij+ip1jjm1,l)
        zpaprs(i,l) = p(ij+ip1jjm1,l)
        zpk(i,l) = pk(ij+ip1jjm1,l)
        zh(i,l) = teta(ij+ip1jjm1,l)
        zqw(i,l) = q(ij+ip1jjm1,l)
        zql(i,l) = ql(ij+ip1jjm1,l)
        zqs(i,l) = 0.
      ENDDO
    ENDDO
  ENDDO
  !
  ! Reset variables
  DO i = 1, imjmp1
    zqw_col(i)=0.
    zql_col(i)=0.
    zqs_col(i)=0.
    zec_col(i) = 0.
    zh_dair_col(i) = 0.
    zh_qw_col(i) = 0.
    zh_ql_col(i) = 0.
    zh_qs_col(i) = 0.
  ENDDO
  !
  zcpvap=RCPV
  zcwat=RCW
  zcice=RCS
  !
  ! Compute vertical sum for each atmospheric column
  ! ================================================
  DO k = 1, llm
    DO i = 1, imjmp1
      ! Watter mass
      zqw_col(i) = zqw_col(i) + zqw(i,k)*zairm(i,k)
      zql_col(i) = zql_col(i) + zql(i,k)*zairm(i,k)
      zqs_col(i) = zqs_col(i) + zqs(i,k)*zairm(i,k)
      ! Cinetic Energy
      zec_col(i) =  zec_col(i) &
            +zecin(i,k)*zairm(i,k)
      ! Air enthalpy
      zt(i,k)= zh(i,k) * zpk(i,k) / RCPD
      zh_dair_col(i) = zh_dair_col(i) &
            + RCPD*(1.-zqw(i,k)-zql(i,k)-zqs(i,k))*zairm(i,k)*zt(i,k)
      zh_qw_col(i) = zh_qw_col(i) &
            + zcpvap*zqw(i,k)*zairm(i,k)*zt(i,k)
      zh_ql_col(i) = zh_ql_col(i) &
            + zcwat*zql(i,k)*zairm(i,k)*zt(i,k) &
            - RLVTT*zql(i,k)*zairm(i,k)
      zh_qs_col(i) = zh_qs_col(i) &
            + zcice*zqs(i,k)*zairm(i,k)*zt(i,k) &
            - RLSTT*zqs(i,k)*zairm(i,k)

    END DO
  ENDDO
  !
  ! Mean over the planete surface
  ! =============================
  qw_tot = 0.
  ql_tot = 0.
  qs_tot = 0.
  ec_tot = 0.
  h_vcol_tot = 0.
  h_dair_tot = 0.
  h_qw_tot = 0.
  h_ql_tot = 0.
  h_qs_tot = 0.
  airetot=0.
  !
  do i=1,imjmp1
    qw_tot = qw_tot + zqw_col(i)
    ql_tot = ql_tot + zql_col(i)
    qs_tot = qs_tot + zqs_col(i)
    ec_tot = ec_tot + zec_col(i)
    h_dair_tot = h_dair_tot + zh_dair_col(i)
    h_qw_tot = h_qw_tot + zh_qw_col(i)
    h_ql_tot = h_ql_tot + zh_ql_col(i)
    h_qs_tot = h_qs_tot + zh_qs_col(i)
    airetot=airetot+zaire(i)
  END DO
  !
  qw_tot = qw_tot/airetot
  ql_tot = ql_tot/airetot
  qs_tot = qs_tot/airetot
  ec_tot = ec_tot/airetot
  h_dair_tot = h_dair_tot/airetot
  h_qw_tot = h_qw_tot/airetot
  h_ql_tot = h_ql_tot/airetot
  h_qs_tot = h_qs_tot/airetot
  !
  h_vcol_tot = h_dair_tot+h_qw_tot+h_ql_tot+h_qs_tot
  !
  ! Compute the change of the atmospheric state compare to the one
  ! stored in "idiag2", and convert it in flux. THis computation
  ! is performed IF idiag2 /= 0 and IF it is not the first CALL
  ! for "idiag"
  ! ===================================
  !
  IF ( (idiag2.gt.0) .and. (pas(idiag2) .ne. 0) ) THEN
    d_h_vcol  = (h_vcol_tot - h_vcol_pre(idiag2) )/dtime
    d_h_dair = (h_dair_tot- h_dair_pre(idiag2))/dtime
    d_h_qw   = (h_qw_tot  - h_qw_pre(idiag2)  )/dtime
    d_h_ql   = (h_ql_tot  - h_ql_pre(idiag2)  )/dtime
    d_h_qs   = (h_qs_tot  - h_qs_pre(idiag2)  )/dtime
    d_qw     = (qw_tot    - qw_pre(idiag2)    )/dtime
    d_ql     = (ql_tot    - ql_pre(idiag2)    )/dtime
    d_qs     = (qs_tot    - qs_pre(idiag2)    )/dtime
    d_ec     = (ec_tot    - ec_pre(idiag2)    )/dtime
    d_qt = d_qw + d_ql + d_qs
  ELSE
    d_h_vcol = 0.
    d_h_dair = 0.
    d_h_qw   = 0.
    d_h_ql   = 0.
    d_h_qs   = 0.
    d_qw     = 0.
    d_ql     = 0.
    d_qs     = 0.
    d_ec     = 0.
    d_qt     = 0.
  ENDIF
  !
  IF (iprt.ge.2) THEN
    WRITE(6,9000) tit,pas(idiag),d_qt,d_qw,d_ql,d_qs
 9000   format('Dyn3d. Watter Mass Budget (kg/m2/s)',A15 &
              ,1i6,10(1pE14.6))
    WRITE(6,9001) tit,pas(idiag), d_h_vcol
 9001   format('Dyn3d. Enthalpy Budget (W/m2) ',A15,1i6,10(F8.2))
    WRITE(6,9002) tit,pas(idiag), d_ec
 9002   format('Dyn3d. Cinetic Energy Budget (W/m2) ',A15,1i6,10(F8.2))
     ! WRITE(6,9003) tit,pas(idiag), ec_tot
 9003   format('Dyn3d. Cinetic Energy (W/m2) ',A15,1i6,10(E15.6))
    WRITE(6,9004) tit,pas(idiag), d_h_vcol+d_ec
 9004   format('Dyn3d. Total Energy Budget (W/m2) ',A15,1i6,10(F8.2))
  END IF
  !
  ! Store the new atmospheric state in "idiag"
  !
  pas(idiag)=pas(idiag)+1
  h_vcol_pre(idiag)  = h_vcol_tot
  h_dair_pre(idiag) = h_dair_tot
  h_qw_pre(idiag)   = h_qw_tot
  h_ql_pre(idiag)   = h_ql_tot
  h_qs_pre(idiag)   = h_qs_tot
  qw_pre(idiag)     = qw_tot
  ql_pre(idiag)     = ql_tot
  qs_pre(idiag)     = qs_tot
  ec_pre (idiag)    = ec_tot
  !
  !#else
  ELSE
    write(lunout,*)'diagedyn: set to function with Earth parameters'
  ENDIF ! of if (planet_type=="earth")
  !#endif
  ! #endif of #ifdef CPP_EARTH
  RETURN
END SUBROUTINE diagedyn