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!MNH_LIC Copyright 1994-2021 CNRS, Meteo-France and Universite Paul Sabatier
!MNH_LIC This is part of the Meso-NH software governed by the CeCILL-C licence
!MNH_LIC version 1. See LICENSE, CeCILL-C_V1-en.txt and CeCILL-C_V1-fr.txt
!MNH_LIC for details. version 1.
MODULE MODE_TURB_VER_SV_FLUX
IMPLICIT NONE
CONTAINS
RODIER Quentin
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SUBROUTINE TURB_VER_SV_FLUX(D,CST,CSTURB,ONOMIXLG, &
KSV,KSV_LGBEG,KSV_LGEND, &
RODIER Quentin
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OTURB_FLX,HTURBDIM,OHARAT,OBLOWSNOW,OLES_CALL,&
PIMPL,PEXPL, &
PTSTEP, &
TPFILE, &
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PDZZ,PDIRCOSZW, &
PRHODJ,PWM, &
PSFSVM,PSFSVP, &
PSVM, &
PTKEM,PLM,MFMOIST,PPSI_SV, &
PRSVS,PWSV )
!
!
!
!!**** *TURB_VER_SV_FLUX* -compute the source terms due to the vertical turbulent
!! fluxes.
!!
!! PURPOSE
!! -------
! The purpose of this routine is to compute the vertical turbulent
! fluxes of the evolutive variables and give back the source
! terms to the main program. In the case of large horizontal meshes,
! the divergence of these vertical turbulent fluxes represent the whole
! effect of the turbulence but when the three-dimensionnal version of
! the turbulence scheme is activated (CTURBDIM="3DIM"), these divergences
! are completed in the next routine TURB_HOR.
! An arbitrary degree of implicitness has been implemented for the
! temporal treatment of these diffusion terms.
! The vertical boundary conditions are as follows:
! * at the bottom, the surface fluxes are prescribed at the same
! as the other turbulent fluxes
! * at the top, the turbulent fluxes are set to 0.
! It should be noted that the condensation has been implicitely included
! in this turbulence scheme by using conservative variables and computing
! the subgrid variance of a statistical variable s indicating the presence
! or not of condensation in a given mesh.
!
!!** METHOD
!! ------
!! 1D type calculations are made;
!! The vertical turbulent fluxes are computed in an off-centered
!! implicit scheme (a Crank-Nicholson type with coefficients different
!! than 0.5), which allows to vary the degree of implicitness of the
!! formulation.
!! The different prognostic variables are treated one by one.
!! The contributions of each turbulent fluxes are cumulated into the
!! tendency PRvarS, and into the dynamic and thermal production of
!! TKE if necessary.
!!
!! In section 2 and 3, the thermodynamical fields are considered.
!! Only the turbulent fluxes of the conservative variables
!! (Thetal and Rnp stored in PRx(:,:,:,1)) are computed.
!! Note that the turbulent fluxes at the vertical
!! boundaries are given either by the soil scheme for the surface one
!! ( at the same instant as the others fluxes) and equal to 0 at the
!! top of the model. The thermal production is computed by vertically
!! averaging the turbulent flux and multiply this flux at the mass point by
!! a function ETHETA or EMOIST, which preform the transformation from the
!! conservative variables to the virtual potential temperature.
!!
!! In section 4, the variance of the statistical variable
!! s indicating presence or not of condensation, is determined in function
!! of the turbulent moments of the conservative variables and its
!! squarred root is stored in PSIGS. This information will be completed in
!! the horizontal turbulence if the turbulence dimensionality is not
!! equal to "1DIM".
!!
!! In section 5, the x component of the stress tensor is computed.
!! The surface flux <u'w'> is computed from the value of the surface
!! fluxes computed in axes linked to the orography ( i", j" , k"):
!! i" is parallel to the surface and in the direction of the maximum
!! slope
!! j" is also parallel to the surface and in the normal direction of
!! the maximum slope
!! k" is the normal to the surface
!! In order to prevent numerical instability, the implicit scheme has
!! been extended to the surface flux regarding to its dependence in
!! function of U. The dependence in function of the other components
!! introduced by the different rotations is only explicit.
!! The turbulent fluxes are used to compute the dynamic production of
!! TKE. For the last TKE level ( located at PDZZ(:,:,IKB)/2 from the
!! ground), an harmonic extrapolation from the dynamic production at
!! PDZZ(:,:,IKB) is used to avoid an evaluation of the gradient of U
!! in the surface layer.
!!
!! In section 6, the same steps are repeated but for the y direction
!! and in section 7, a diagnostic computation of the W variance is
!! performed.
!!
!! In section 8, the turbulent fluxes for the scalar variables are
!! computed by the same way as the conservative thermodynamical variables
!!
!!
!! EXTERNAL
!! --------
!! GX_U_M, GY_V_M, GZ_W_M : cartesian gradient operators
!! GX_U_UW,GY_V_VW (X,Y,Z) represent the direction of the gradient
!! _(M,U,...)_ represent the localization of the
!! field to be derivated
!! _(M,UW,...) represent the localization of the
!! field derivated
!!
!!
!! MXM,MXF,MYM,MYF,MZM,MZF
!! : Shuman functions (mean operators)
!! DXF,DYF,DZF,DZM
!! : Shuman functions (difference operators)
!!
!! SUBROUTINE TRIDIAG : to compute the split implicit evolution
!! of a variable located at a mass point
!!
!! SUBROUTINE TRIDIAG_WIND: to compute the split implicit evolution
!! of a variable located at a wind point
!!
!! FUNCTIONs ETHETA and EMOIST :
!! allows to compute:
!! - the coefficients for the turbulent correlation between
!! any variable and the virtual potential temperature, of its
!! correlations with the conservative potential temperature and
!! the humidity conservative variable:
!! ------- ------- -------
!! A' Thv' = ETHETA A' Thl' + EMOIST A' Rnp'
!!
!!
!! IMPLICIT ARGUMENTS
!! ------------------
!! Module MODD_CST : contains physical constants
!!
RODIER Quentin
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!! CST%XG : gravity constant
!!
!! Module MODD_CTURB: contains the set of constants for
!! the turbulence scheme
!!
RODIER Quentin
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!! CSTURB%XCMFS,XCMFB : cts for the momentum flux
!! CSTURB%XCSHF : ct for the sensible heat flux
!! CSTURB%XCHF : ct for the moisture flux
!! CSTURB%XCTV,CSTURB%XCHV : cts for the T and moisture variances
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!!
!! Module MODD_PARAMETERS
!!
!! JPVEXT_TURB : number of vertical external points
!! JPHEXT : number of horizontal external points
!!
!!
!! REFERENCE
!! ---------
!! Book 1 of documentation (Chapter: Turbulence)
!!
!! AUTHOR
!! ------
!! Joan Cuxart * INM and Meteo-France *
!!
!! MODIFICATIONS
!! -------------
!! Original August 19, 1994
!! Modifications: February 14, 1995 (J.Cuxart and J.Stein)
!! Doctorization and Optimization
!! Modifications: March 21, 1995 (J.M. Carriere)
!! Introduction of cloud water
!! Modifications: June 14, 1995 (J.Cuxart and J. Stein)
!! Phi3 and Psi3 at w-point + bug in the all
!! or nothing condens.
!! Modifications: Sept 15, 1995 (J.Cuxart and J. Stein)
!! Change the DP computation at the ground
!! Modifications: October 10, 1995 (J.Cuxart and J. Stein)
!! Psi for scal var and LES tools
!! Modifications: November 10, 1995 (J. Stein)
!! change the surface relations
!! Modifications: February 20, 1995 (J. Stein) optimization
!! Modifications: May 21, 1996 (J. Stein)
!! bug in the vertical flux of the V wind
!! component for explicit computation
!! Modifications: May 21, 1996 (N. wood)
!! modify the computation of the vertical
!! part or the surface tangential flux
!! Modifications: May 21, 1996 (P. Jabouille)
!! same modification in the Y direction
!!
!! Modifications: Sept 17, 1996 (J. Stein) change the moist case by using
!! Pi instead of Piref + use Atheta and Amoist
!!
!! Modifications: Nov 24, 1997 (V. Masson) removes the DO loops
!! Modifications: Mar 31, 1998 (V. Masson) splits the routine TURB_VER_SV_FLUX
!! Modifications: Dec 01, 2000 (V. Masson) conservation of scalar emission
!! from surface in 1DIM case
!! when slopes are present
!! Jun 20, 2001 (J Stein) case of lagragian variables
!! Nov 06, 2002 (V. Masson) LES budgets
!! October 2009 (G. Tanguy) add ILENCH=LEN(YCOMMENT) after
!! change of YCOMMENT
!! Feb 2012(Y. Seity) add possibility to run with reversed
!! vertical levels
RODIER Quentin
committed
!! Modifications: July 2015 (Wim de Rooy) OHARAT switch
!! Feb 2017(M. Leriche) add initialisation of ZSOURCE
!! to avoid unknwon values outside physical domain
!! and avoid negative values in sv tendencies
!! Philippe Wautelet: 05/2016-04/2018: new data structures and calls for I/O
!!--------------------------------------------------------------------------
!
!* 0. DECLARATIONS
! ------------
!
USE PARKIND1, ONLY : JPRB
USE YOMHOOK , ONLY : LHOOK, DR_HOOK
!
RODIER Quentin
committed
USE MODD_CST, ONLY: CST_t
USE MODD_CTURB, ONLY: CSTURB_t
USE MODD_DIMPHYEX, ONLY: DIMPHYEX_t
USE MODD_FIELD, ONLY: TFIELDDATA, TYPEREAL
USE MODD_IO, ONLY: TFILEDATA
RODIER Quentin
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USE MODD_PARAMETERS, ONLY: JPVEXT_TURB
USE MODD_LES
RODIER Quentin
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USE MODD_BLOWSNOW, ONLY: XRSNOW
USE MODE_IO_FIELD_WRITE, ONLY: IO_FIELD_WRITE_PHY
USE SHUMAN_PHY , ONLY : DZM_PHY, MZM_PHY, MZF_PHY
USE MODE_GRADIENT_W_PHY, ONLY: GZ_W_M_PHY
USE MODE_GRADIENT_M_PHY, ONLY: GZ_M_W_PHY
USE MODE_TRIDIAG, ONLY: TRIDIAG
USE MODE_EMOIST, ONLY: EMOIST
USE MODE_ETHETA, ONLY: ETHETA
USE MODI_LES_MEAN_SUBGRID_PHY
USE MODI_SECOND_MNH
!
IMPLICIT NONE
!
!* 0.1 declarations of arguments
!
!
TYPE(DIMPHYEX_t), INTENT(IN) :: D
TYPE(CST_t), INTENT(IN) :: CST
TYPE(CSTURB_t), INTENT(IN) :: CSTURB
INTEGER, INTENT(IN) :: KSV, &
KSV_LGBEG, KSV_LGEND ! number of scalar variables
LOGICAL, INTENT(IN) :: OTURB_FLX ! switch to write the
! turbulent fluxes in the syncronous FM-file
RODIER Quentin
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LOGICAL, INTENT(IN) :: ONOMIXLG ! to use turbulence for lagrangian variables (modd_conf)
CHARACTER(LEN=4), INTENT(IN) :: HTURBDIM ! dimensionality of the
! turbulence scheme
RODIER Quentin
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LOGICAL, INTENT(IN) :: OHARAT
RODIER Quentin
committed
LOGICAL, INTENT(IN) :: OLES_CALL ! compute the LES diagnostics at current time-step
LOGICAL, INTENT(IN) :: OBLOWSNOW ! switch to activate pronostic blowing snow
REAL, INTENT(IN) :: PIMPL, PEXPL ! Coef. for temporal disc.
REAL, INTENT(IN) :: PTSTEP ! Double Time Step
TYPE(TFILEDATA), INTENT(IN) :: TPFILE ! Output file
REAL, DIMENSION(D%NIJT,D%NKT), INTENT(IN) :: PDZZ
! Metric coefficients
REAL, DIMENSION(D%NIJT), INTENT(IN) :: PDIRCOSZW ! Director Cosinus of the
! normal to the ground surface
!
REAL, DIMENSION(D%NIJT,D%NKT), INTENT(IN) :: PRHODJ ! dry density * grid volum
REAL, DIMENSION(D%NIJT,D%NKT), INTENT(IN) :: MFMOIST ! moist mf dual scheme
REAL, DIMENSION(D%NIJT,KSV), INTENT(IN) :: PSFSVM ! t - deltat
REAL, DIMENSION(D%NIJT,KSV), INTENT(IN) :: PSFSVP ! t + deltat
REAL, DIMENSION(D%NIJT,D%NKT,KSV), INTENT(IN) :: PSVM ! scalar var. at t-Delta t
REAL, DIMENSION(D%NIJT,D%NKT), INTENT(IN) :: PWM ! vertical wind
REAL, DIMENSION(D%NIJT,D%NKT), INTENT(IN) :: PTKEM ! TKE at time t
REAL, DIMENSION(D%NIJT,D%NKT), INTENT(IN) :: PLM ! Turb. mixing length
REAL, DIMENSION(D%NIJT,D%NKT,KSV), INTENT(IN) :: PPSI_SV ! Inv.Turb.Sch.for scalars
REAL, DIMENSION(D%NIJT,D%NKT,KSV), INTENT(INOUT) :: PRSVS
! cumulated sources for the prognostic variables
REAL, DIMENSION(D%NIJT,D%NKT,KSV), INTENT(OUT) :: PWSV ! scalar flux
!
!* 0.2 declaration of local variables
!
!
REAL, DIMENSION(D%NIJT,D%NKT) :: &
ZA, & ! under diagonal elements of the tri-diagonal matrix involved
! in the temporal implicit scheme (also used to store coefficient
! J in Section 5)
ZRES, & ! guess of the treated variable at t+ deltat when the turbu-
! lence is the only source of evolution added to the ones
! considered in ZSOURCE
ZFLXZ, & ! vertical flux of the treated variable
ZSOURCE, & ! source of evolution for the treated variable
ZKEFF, & ! effectif diffusion coeff = LT * SQRT( TKE )
ZWORK1,ZWORK2,&
ZWORK3,ZWORK4! working var. for shuman operators (array syntax)
INTEGER :: IKT ! array size in k direction
INTEGER :: IIJB,IIJE,IKB,IKE ! index value for the mass points of the domain
INTEGER :: IKTB,IKTE ! start, end of k loops in physical domain
INTEGER :: JSV ! loop counters
!
REAL :: ZTIME1, ZTIME2
REAL :: ZCSVP = 4.0 ! constant for scalar flux presso-correlation (RS81)
REAL :: ZCSV !constant for the scalar flux
!
TYPE(TFIELDDATA) :: TZFIELD
!----------------------------------------------------------------------------
!
!* 1. PRELIMINARIES
! -------------
!
REAL(KIND=JPRB) :: ZHOOK_HANDLE
IF (LHOOK) CALL DR_HOOK('TURB_VER_SV_FLUX',0,ZHOOK_HANDLE)
!
IKT=D%NKT
IKTB=D%NKTB
IKTE=D%NKTE
IKB=D%NKB
IKE=D%NKE
IIJE=D%NIJE
IIJB=D%NIJB
RODIER Quentin
committed
IF (OHARAT) THEN
!$mnh_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ZKEFF(IIJB:IIJE,IKB:IKE) = PLM(IIJB:IIJE,IKB:IKE) * SQRT(PTKEM(IIJB:IIJE,IKB:IKE)) &
+ 50.*MFMOIST(IIJB:IIJE,IKB:IKE)
!$mnh_end_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
!$mnh_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ZWORK1(IIJB:IIJE,1:D%NKT) = PLM(IIJB:IIJE,1:D%NKT)*SQRT(PTKEM(IIJB:IIJE,1:D%NKT))
!$mnh_end_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
CALL MZM_PHY(D,ZWORK1,ZKEFF)
ENDIF
!
RODIER Quentin
committed
IF(OBLOWSNOW) THEN
! See Vionnet (PhD, 2012) for a complete discussion around the value of the Schmidt number for blowing snow variables
ZCSV=CSTURB%XCHF/XRSNOW
ELSE
ENDIF
!----------------------------------------------------------------------------
!
!* 8. SOURCES OF PASSIVE SCALAR VARIABLES
! -----------------------------------
!
CALL MZM_PHY(D,PRHODJ,ZWORK1)
RODIER Quentin
committed
DO JSV=1,KSV
RODIER Quentin
committed
IF (ONOMIXLG .AND. JSV >= KSV_LGBEG .AND. JSV<= KSV_LGEND) CYCLE
!
! Preparation of the arguments for TRIDIAG
RODIER Quentin
committed
IF (OHARAT) THEN
!$mnh_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ZA(IIJB:IIJE,IKB:IKE) = -PTSTEP * ZKEFF(IIJB:IIJE,IKB:IKE) * ZWORK1(IIJB:IIJE,IKB:IKE) &
/ PDZZ(IIJB:IIJE,IKB:IKE)**2
!$mnh_end_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ELSE
!$mnh_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ZA(IIJB:IIJE,IKB:IKE) = -PTSTEP*ZCSV*PPSI_SV(IIJB:IIJE,IKB:IKE,JSV) * &
ZKEFF(IIJB:IIJE,IKB:IKE) * ZWORK1(IIJB:IIJE,IKB:IKE) / PDZZ(IIJB:IIJE,IKB:IKE)**2
!$mnh_end_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ENDIF
ZSOURCE(IIJB:IIJE,IKB:IKE) = 0.
!
! Compute the sources for the JSVth scalar variable
!* in 3DIM case, a part of the flux goes vertically, and another goes horizontally
! (in presence of slopes)
!* in 1DIM case, the part of energy released in horizontal flux
! is taken into account in the vertical part
IF (HTURBDIM=='3DIM') THEN
!$mnh_expand_array(JIJ=IIJB:IIJE)
ZSOURCE(IIJB:IIJE,IKB) = (PIMPL*PSFSVP(IIJB:IIJE,JSV) + PEXPL*PSFSVM(IIJB:IIJE,JSV)) / &
PDZZ(IIJB:IIJE,IKB) * PDIRCOSZW(IIJB:IIJE) &
* 0.5 * (1. + PRHODJ(IIJB:IIJE,D%NKA) / PRHODJ(IIJB:IIJE,IKB))
!$mnh_end_expand_array(JIJ=IIJB:IIJE)
!$mnh_expand_array(JIJ=IIJB:IIJE)
ZSOURCE(IIJB:IIJE,IKB) = (PIMPL*PSFSVP(IIJB:IIJE,JSV) + PEXPL*PSFSVM(IIJB:IIJE,JSV)) / &
PDZZ(IIJB:IIJE,IKB) / PDIRCOSZW(IIJB:IIJE) &
* 0.5 * (1. + PRHODJ(IIJB:IIJE,D%NKA) / PRHODJ(IIJB:IIJE,IKB))
!$mnh_end_expand_array(JIJ=IIJB:IIJE)
ZSOURCE(IIJB:IIJE,IKTB+1:IKTE-1) = 0.
ZSOURCE(IIJB:IIJE,IKE) = 0.
! Obtention of the split JSV scalar variable at t+ deltat
CALL TRIDIAG(D,PSVM(:,:,JSV),ZA,PTSTEP,PEXPL,PIMPL,PRHODJ,ZSOURCE,ZRES)
!
! Compute the equivalent tendency for the JSV scalar variable
!$mnh_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
PRSVS(IIJB:IIJE,IKB:IKE,JSV)= PRSVS(IIJB:IIJE,IKB:IKE,JSV)+ &
PRHODJ(IIJB:IIJE,IKB:IKE)*(ZRES(IIJB:IIJE,IKB:IKE)-PSVM(IIJB:IIJE,IKB:IKE,JSV))/PTSTEP
!$mnh_end_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
RODIER Quentin
committed
IF ( (OTURB_FLX .AND. TPFILE%LOPENED) .OR. OLES_CALL ) THEN
! Diagnostic of the cartesian vertical flux
!
!$mnh_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ZWORK1(IIJB:IIJE,1:D%NKT) = PLM(IIJB:IIJE,1:D%NKT)*SQRT(PTKEM(IIJB:IIJE,1:D%NKT))
ZWORK2(IIJB:IIJE,1:D%NKT) = PIMPL*ZRES(IIJB:IIJE,1:D%NKT) + PEXPL*PSVM(IIJB:IIJE,1:D%NKT,JSV)
!$mnh_end_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
CALL MZM_PHY(D,ZWORK1,ZWORK3)
CALL DZM_PHY(D,ZWORK2,ZWORK4)
!$mnh_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ZFLXZ(IIJB:IIJE,IKB:IKE) = -ZCSV * PPSI_SV(IIJB:IIJE,IKB:IKE,JSV) * ZWORK3(IIJB:IIJE,IKB:IKE) &
/ PDZZ(IIJB:IIJE,IKB:IKE) * &
ZWORK4(IIJB:IIJE,IKB:IKE)
!$mnh_end_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
! surface flux
!* in 3DIM case, a part of the flux goes vertically, and another goes horizontally
! (in presence of slopes)
!* in 1DIM case, the part of energy released in horizontal flux
! is taken into account in the vertical part
IF (HTURBDIM=='3DIM') THEN
!$mnh_expand_array(JIJ=IIJB:IIJE)
ZFLXZ(IIJB:IIJE,IKB) = (PIMPL*PSFSVP(IIJB:IIJE,JSV) + PEXPL*PSFSVM(IIJB:IIJE,JSV)) &
* PDIRCOSZW(IIJB:IIJE)
!$mnh_end_expand_array(JIJ=IIJB:IIJE)
!$mnh_expand_array(JIJ=IIJB:IIJE)
ZFLXZ(IIJB:IIJE,IKB) = (PIMPL*PSFSVP(IIJB:IIJE,JSV) + PEXPL*PSFSVM(IIJB:IIJE,JSV)) &
/ PDIRCOSZW(IIJB:IIJE)
!$mnh_end_expand_array(JIJ=IIJB:IIJE)
END IF
! extrapolates the flux under the ground so that the vertical average with
! the IKB flux gives the ground value
!$mnh_expand_array(JIJ=IIJB:IIJE)
ZFLXZ(IIJB:IIJE,D%NKA) = ZFLXZ(IIJB:IIJE,IKB)
!$mnh_end_expand_array(JIJ=IIJB:IIJE)
DO JK=IKTB+1,IKTE-1
!$mnh_expand_array(JIJ=IIJB:IIJE)
PWSV(IIJB:IIJE,JK,JSV)=0.5*(ZFLXZ(IIJB:IIJE,JK)+ZFLXZ(IIJB:IIJE,JK+D%NKL))
!$mnh_end_expand_array(JIJ=IIJB:IIJE)
!$mnh_expand_array(JIJ=IIJB:IIJE)
PWSV(IIJB:IIJE,IKB,JSV)=0.5*(ZFLXZ(IIJB:IIJE,IKB)+ZFLXZ(IIJB:IIJE,IKB+D%NKL))
PWSV(IIJB:IIJE,IKE,JSV)=PWSV(IIJB:IIJE,IKE-D%NKL,JSV)
!$mnh_end_expand_array(JIJ=IIJB:IIJE)
END IF
!
IF (OTURB_FLX .AND. TPFILE%LOPENED) THEN
! stores the JSVth vertical flux
WRITE(TZFIELD%CMNHNAME,'("WSV_FLX_",I3.3)') JSV
TZFIELD%CSTDNAME = ''
TZFIELD%CLONGNAME = TRIM(TZFIELD%CMNHNAME)
!PW: TODO: use the correct units of the JSV variable (and multiply it by m s-1)
TZFIELD%CUNITS = 'SVUNIT m s-1'
TZFIELD%CDIR = 'XY'
TZFIELD%CCOMMENT = 'X_Y_Z_'//TRIM(TZFIELD%CMNHNAME)
TZFIELD%NGRID = 4
TZFIELD%NTYPE = TYPEREAL
TZFIELD%NDIMS = 3
TZFIELD%LTIMEDEP = .TRUE.
!
CALL IO_FIELD_WRITE_PHY(D,TPFILE,TZFIELD,ZFLXZ)
END IF
!
! Storage in the LES configuration
!
RODIER Quentin
committed
IF (OLES_CALL) THEN
CALL SECOND_MNH(ZTIME1)
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!
CALL MZF_PHY(D,ZFLXZ,ZWORK1)
CALL LES_MEAN_SUBGRID_PHY(D,ZWORK1, X_LES_SUBGRID_WSv(:,:,:,JSV) )
!
CALL GZ_W_M_PHY(D,PWM,PDZZ,ZWORK2)
!$mnh_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ZWORK3(IIJB:IIJE,1:D%NKT) = ZWORK2(IIJB:IIJE,1:D%NKT) * ZWORK1(IIJB:IIJE,1:D%NKT)
!$mnh_end_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
CALL LES_MEAN_SUBGRID_PHY(D,ZWORK3, X_LES_RES_ddxa_W_SBG_UaSv(:,:,:,JSV) )
!
CALL GZ_M_W_PHY(D,PSVM(:,:,JSV),PDZZ,ZWORK1)
!$mnh_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ZWORK2(IIJB:IIJE,1:D%NKT) = ZWORK1(IIJB:IIJE,1:D%NKT) * ZFLXZ(IIJB:IIJE,1:D%NKT)
!$mnh_end_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
CALL MZF_PHY(D,ZWORK2,ZWORK3)
CALL LES_MEAN_SUBGRID_PHY(D,ZWORK3, X_LES_RES_ddxa_Sv_SBG_UaSv(:,:,:,JSV) )
!
CALL MZF_PHY(D,ZFLXZ,ZWORK1)
!$mnh_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ZWORK2(IIJB:IIJE,1:D%NKT) = -ZCSVP*SQRT(PTKEM(IIJB:IIJE,1:D%NKT))/PLM(IIJB:IIJE,1:D%NKT)*ZWORK1(IIJB:IIJE,1:D%NKT)
!$mnh_end_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
CALL LES_MEAN_SUBGRID_PHY(D,ZWORK2, X_LES_SUBGRID_SvPz(:,:,:,JSV) )
!
!$mnh_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
ZWORK1(IIJB:IIJE,1:D%NKT) = PWM(IIJB:IIJE,1:D%NKT)*ZFLXZ(IIJB:IIJE,1:D%NKT)
!$mnh_end_expand_array(JIJ=IIJB:IIJE,JK=1:D%NKT)
CALL MZF_PHY(D,ZWORK1,ZWORK2)
CALL LES_MEAN_SUBGRID_PHY(D,ZWORK2, X_LES_RES_W_SBG_WSv(:,:,:,JSV) )
!
CALL SECOND_MNH(ZTIME2)
XTIME_LES = XTIME_LES + ZTIME2 - ZTIME1
END IF
!
END DO ! end of scalar loop
!
!----------------------------------------------------------------------------
!
IF (LHOOK) CALL DR_HOOK('TURB_VER_SV_FLUX',1,ZHOOK_HANDLE)
END SUBROUTINE TURB_VER_SV_FLUX
END MODULE MODE_TURB_VER_SV_FLUX