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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_THERMO_FLUX
IMPLICIT NONE
CONTAINS
SUBROUTINE TURB_VER_THERMO_FLUX(D,CST,CSTURB,TURBN, &
KKA,KKU,KKL,KRR,KRRL,KRRI,KSV, &
RODIER Quentin
committed
OTURB_FLX,HTURBDIM,HTOM,OOCEAN,ODEEPOC,OHARAT,&
OCOUPLES,OLES_CALL, OCOMPUTE_SRC, &
RODIER Quentin
committed
PIMPL,PEXPL,PTSTEP,HPROGRAM, &
TPFILE, &
PDXX,PDYY,PDZZ,PDZX,PDZY,PDIRCOSZW,PZZ, &
PRHODJ,PTHVREF, &
PSFTHM,PSFRM,PSFTHP,PSFRP, &
PWM,PTHLM,PRM,PSVM, &
PTKEM,PLM,PLEPS, &
PLOCPEXNM,PATHETA,PAMOIST,PSRCM,PFRAC_ICE, &
PBETA, PSQRT_TKE, PDTH_DZ, PDR_DZ, PRED2TH3, &
PRED2R3, PRED2THR3, PBLL_O_E, PETHETA, &
PEMOIST, PREDTH1, PREDR1, PPHI3, PPSI3, PD, &
PFWTH,PFWR,PFTH2,PFR2,PFTHR,MFMOIST,PBL_DEPTH,&
PWTHV,PRTHLS,PRRS,PTHLP,PRP,PTP,PWTH,PWRC )
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! ###############################################################
!
!
!!**** *TURB_VER_THERMO_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_THERMO_FLUX
!! Modifications: Oct 18, 2000 (V. Masson) LES computations
!! Modifications: Dec 01, 2000 (V. Masson) conservation of energy from
!! surface flux in 1DIM case
!! when slopes are present
!! Nov 06, 2002 (V. Masson) LES budgets
!! Feb 20, 2003 (JP Pinty) Add PFRAC_ICE
!! May 20, 2003 (JP Pinty) Correction of ETHETA
!! and EMOIST calls
!! July 2005 (S. Tomas, V. Masson)
!! Add 3rd order moments
!! and implicitation of PHI3 and PSI3
!! October 2009 (G. Tanguy) add ILENCH=LEN(YCOMMENT) after
!! change of YCOMMENT
!! 2012-02 (Y. Seity) add possibility to run with reversed
!! vertical levels
RODIER Quentin
committed
!! Modifications July 2015 (Wim de Rooy) OHARAT switch
!! Philippe Wautelet: 05/2016-04/2018: new data structures and calls for I/O
!! 2021 (D. Ricard) last version of HGRAD turbulence scheme
!! Leronard terms instead of Reynolds terms
!! applied to vertical fluxes of r_np and Thl
!! for implicit version of turbulence scheme
!! corrections and cleaning
!! June 2020 (B. Vie) Patch preventing negative rc and ri in 2.3 and 3.3
!! JL Redelsperger : 03/2021: Ocean and Autocoupling O-A LES Cases
!! Sfc flux shape for LDEEPOC Case
!!--------------------------------------------------------------------------
!
!* 0. DECLARATIONS
! ------------
!
USE PARKIND1, ONLY : JPRB
USE YOMHOOK , ONLY : LHOOK, DR_HOOK
!
RODIER Quentin
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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_GRID_n, ONLY: XZS, XXHAT, XYHAT
USE MODD_IO, ONLY: TFILEDATA
USE MODD_METRICS_n, ONLY: XDXX, XDYY, XDZX, XDZY, XDZZ
USE MODD_PARAMETERS, ONLY: JPVEXT_TURB, JPHEXT
USE MODD_TURB_n, ONLY: TURB_t
USE MODD_LES
RODIER Quentin
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USE MODD_DIM_n, ONLY: NIMAX_ll, NJMAX_ll
USE MODD_OCEANH, ONLY: XSSTFL
USE MODD_TURB_n, ONLY: TURB_t
RODIER Quentin
committed
USE MODD_FRC, ONLY: XCENTX_OC, XCENTY_OC, XRADX_OC,XRADY_OC
!
USE MODI_GRADIENT_U
USE MODI_GRADIENT_V
USE MODI_GRADIENT_W
USE MODI_GRADIENT_M
USE MODI_SHUMAN , ONLY : DZF, DZM, MZF, MZM, MYF, MXF
USE MODI_LES_MEAN_SUBGRID
USE MODE_TRIDIAG_THERMO, ONLY: TRIDIAG_THERMO
USE MODE_TM06_H, ONLY: TM06_H
USE MODE_IO_FIELD_WRITE, ONLY: IO_FIELD_WRITE
USE MODE_PRANDTL
!
USE MODI_SECOND_MNH
USE MODE_ll
USE MODE_GATHER_ll
!
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
TYPE(TURB_t), INTENT(IN) :: TURBN
INTEGER, INTENT(IN) :: KKA !near ground array index
INTEGER, INTENT(IN) :: KKU !uppest atmosphere array index
INTEGER, INTENT(IN) :: KKL !vert. levels type 1=MNH -1=ARO
INTEGER, INTENT(IN) :: KRR ! number of moist var.
INTEGER, INTENT(IN) :: KSV ! number of scalar var.
INTEGER, INTENT(IN) :: KRRL ! number of liquid water var.
INTEGER, INTENT(IN) :: KRRI ! number of ice water var.
LOGICAL, INTENT(IN) :: OTURB_FLX ! switch to write the
! turbulent fluxes in the syncronous FM-file
LOGICAL, INTENT(IN) :: OOCEAN ! switch for Ocean model version
RODIER Quentin
committed
LOGICAL, INTENT(IN) :: ODEEPOC ! activates sfc forcing for ideal ocean deep conv
RODIER Quentin
committed
LOGICAL, INTENT(IN) :: OHARAT
LOGICAL, INTENT(IN) :: OCOMPUTE_SRC ! flag to define dimensions of SIGS and
CHARACTER(LEN=4), INTENT(IN) :: HTURBDIM ! dimensionality of the
! turbulence scheme
RODIER Quentin
committed
CHARACTER(LEN=6), INTENT(IN) :: HPROGRAM ! CPROGRAM is the program currently running (modd_conf)
CHARACTER(LEN=4), INTENT(IN) :: HTOM ! type of Third Order Moment
REAL, INTENT(IN) :: PIMPL, PEXPL ! Coef. for temporal disc.
REAL, INTENT(IN) :: PTSTEP ! Double Time Step
TYPE(TFILEDATA), INTENT(IN) :: TPFILE ! Output file
RODIER Quentin
committed
LOGICAL, INTENT(IN) :: OLES_CALL ! compute the LES diagnostics at current time-step
LOGICAL, INTENT(IN) :: OCOUPLES ! switch to activate atmos-ocean LES version
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PDZZ, PDXX, PDYY, PDZX, PDZY
! Metric coefficients
REAL, DIMENSION(D%NIT,D%NJT), INTENT(IN) :: PDIRCOSZW ! Director Cosinus of the
! normal to the ground surface
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PZZ ! altitudes
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PRHODJ ! dry density * grid volum
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: MFMOIST ! moist mass flux dual scheme
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PTHVREF ! ref. state Virtual
! Potential Temperature
!
REAL, DIMENSION(D%NIT,D%NJT), INTENT(IN) :: PSFTHM,PSFRM ! surface fluxes at time
! ! t - deltat
!
REAL, DIMENSION(D%NIT,D%NJT), INTENT(IN) :: PSFTHP,PSFRP ! surface fluxes at time
! ! t + deltat
!
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PWM
! Vertical wind
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PTHLM
! potential temperature at t-Delta t
REAL, DIMENSION(D%NIT,D%NJT,D%NKT,KRR), INTENT(IN) :: PRM ! Mixing ratios
! at t-Delta t
REAL, DIMENSION(D%NIT,D%NJT,D%NKT,KSV), INTENT(IN) :: PSVM ! Mixing ratios
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PTKEM ! TKE at time t
RODIER Quentin
committed
! In case OHARAT=TRUE, PLM already includes all stability corrections
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PLM ! Turb. mixing length
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PLEPS ! dissipative length
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PLOCPEXNM ! Lv(T)/Cp/Exnref at time t-1
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PATHETA ! coefficients between
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PAMOIST ! s and Thetal and Rnp
REAL, DIMENSION(MERGE(D%NIT,0,OCOMPUTE_SRC),&
MERGE(D%NJT,0,OCOMPUTE_SRC),&
MERGE(D%NKT,0,OCOMPUTE_SRC)), INTENT(IN) :: PSRCM ! normalized
! 2nd-order flux s'r'c/2Sigma_s2 at t-1 multiplied by Lambda_3
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REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PFRAC_ICE ! ri fraction of rc+ri
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PBETA ! buoyancy coefficient
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PSQRT_TKE ! sqrt(e)
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PDTH_DZ ! d(th)/dz
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PDR_DZ ! d(rt)/dz
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PRED2TH3 ! 3D Redeslperger number R*2_th
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PRED2R3 ! 3D Redeslperger number R*2_r
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PRED2THR3 ! 3D Redeslperger number R*2_thr
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PBLL_O_E ! beta * Lk * Leps / tke
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PETHETA ! Coefficient for theta in theta_v computation
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PEMOIST ! Coefficient for r in theta_v computation
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PREDTH1 ! 1D Redelsperger number for Th
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PREDR1 ! 1D Redelsperger number for r
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PPHI3 ! Prandtl number for temperature
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PPSI3 ! Prandtl number for vapor
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PD ! Denominator in Prandtl numbers
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PFWTH ! d(w'2th' )/dz (at flux point)
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PFWR ! d(w'2r' )/dz (at flux point)
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PFTH2 ! d(w'th'2 )/dz (at mass point)
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PFR2 ! d(w'r'2 )/dz (at mass point)
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(IN) :: PFTHR ! d(w'th'r')/dz (at mass point)
REAL, DIMENSION(MERGE(D%NIT,0,HTOM=='TMO6'),&
MERGE(D%NJT,0,HTOM=='TMO6')), INTENT(INOUT):: PBL_DEPTH ! BL depth
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(OUT) :: PWTHV ! buoyancy flux
!
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(INOUT) :: PRTHLS ! cumulated source for theta
REAL, DIMENSION(D%NIT,D%NJT,D%NKT,KRR), INTENT(INOUT) :: PRRS ! cumulated source for rt
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(OUT) :: PTHLP ! guess of thl at t+ deltat
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(OUT) :: PRP ! guess of r at t+ deltat
!
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(OUT) :: PTP ! Dynamic and thermal
! TKE production terms
!
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(OUT) :: PWTH ! heat flux
REAL, DIMENSION(D%NIT,D%NJT,D%NKT), INTENT(OUT) :: PWRC ! cloud water flux
!
!
!* 0.2 declaration of local variables
!
!
REAL, DIMENSION(D%NIT,D%NJT,D%NKT) :: &
ZA, & ! work variable for wrc or LES computation
ZFLXZ, & ! vertical flux of the treated variable
ZSOURCE, & ! source of evolution for the treated variable
ZKEFF, & ! effectif diffusion coeff = LT * SQRT( TKE )
ZF, & ! Flux in dTh/dt =-dF/dz (evaluated at t-1)(or rt instead of Th)
ZDFDDTDZ, & ! dF/d(dTh/dz)
ZDFDDRDZ, & ! dF/d(dr/dz)
Z3RDMOMENT,& ! 3 order term in flux or variance equation
ZF_LEONARD,& ! Leonard terms
ZRWTHL, &
ZRWRNP, &
ZCLD_THOLD, ZALT
!
INTEGER :: IKB,IKE ! I index values for the Beginning and End
! mass points of the domain in the 3 direct.
INTEGER :: IKT ! array size in k direction
INTEGER :: IKTB,IKTE ! start, end of k loops in physical domain
INTEGER :: JI, JJ ! loop indexes
!
INTEGER :: IIB,IJB ! Lower bounds of the physical
! sub-domain in x and y directions
INTEGER :: IIE,IJE ! Upper bounds of the physical
! sub-domain in x and y directions
!
RODIER Quentin
committed
! TODO TO BE REMOVED OUTSIDE OF TURB ? : SHOULD BE NI/JMAX_ll+2*JPHEXT
! WARNING WRONG DIMENSION, NIMAX_ll not initialized with AROME
REAL, DIMENSION(1) :: ZXHAT_ll ! Position x in the conformal
! plane (array on the complete domain)
RODIER Quentin
committed
REAL, DIMENSION(1) :: ZYHAT_ll ! Position y in the conformal
! plane (array on the complete domain)
REAL :: ZTIME1, ZTIME2
REAL :: ZDELTAX
REAL :: ZXBEG,ZXEND,ZYBEG,ZYEND ! Forcing size for ocean deep convection
REAL, DIMENSION(D%NIT,D%NJT) :: ZDIST ! distance
! from the center of the cooling
REAL :: ZFLPROV
INTEGER :: JKM ! vertical index loop
INTEGER :: JSW
REAL :: ZSWA ! index for time flux interpolation
!
INTEGER :: IIU, IJU
INTEGER :: IRESP
INTEGER :: JK
LOGICAL :: GUSERV ! flag to use water
LOGICAL :: GFTH2 ! flag to use w'th'2
LOGICAL :: GFWTH ! flag to use w'2th'
LOGICAL :: GFR2 ! flag to use w'r'2
LOGICAL :: GFWR ! flag to use w'2r'
LOGICAL :: GFTHR ! flag to use w'th'r'
TYPE(TFIELDDATA) :: TZFIELD
!----------------------------------------------------------------------------
!
!* 1. PRELIMINARIES
! -------------
!
REAL(KIND=JPRB) :: ZHOOK_HANDLE
IF (LHOOK) CALL DR_HOOK('TURB_VER_THERMO_FLUX',0,ZHOOK_HANDLE)
!
! Size for a given proc & a given model
IIU=D%NIT
IJU=D%NJT
!
!! Compute Shape of sfc flux for Oceanic Deep Conv Case
!
RODIER Quentin
committed
IF (OOCEAN .AND. ODEEPOC) THEN
!* COMPUTES THE PHYSICAL SUBDOMAIN BOUNDS
!compute ZXHAT_ll = position in the (0:Lx) domain 1 (Lx=Size of domain1 )
!compute XXHAT_ll = position in the (L0_subproc,Lx_subproc) domain for the current subproc
! L0_subproc as referenced in the full domain 1
CALL GATHERALL_FIELD_ll('XX',XXHAT,ZXHAT_ll,IRESP)
CALL GATHERALL_FIELD_ll('YY',XYHAT,ZYHAT_ll,IRESP)
CALL GET_DIM_EXT_ll('B',IIU,IJU)
CALL GET_INDICE_ll(IIB,IJB,IIE,IJE,IIU,IJU)
DO JJ = IJB,IJE
DO JI = IIB,IIE
ZDIST(JI,JJ) = SQRT( &
(( (XXHAT(JI)+XXHAT(JI+1))*0.5 - XCENTX_OC ) / XRADX_OC)**2 + &
(( (XYHAT(JJ)+XYHAT(JJ+1))*0.5 - XCENTY_OC ) / XRADY_OC)**2 &
)
END DO
END DO
DO JJ=IJB,IJE
DO JI=IIB,IIE
IF ( ZDIST(JI,JJ) > 1.) XSSTFL(JI,JJ)=0.
END DO
END DO
END IF !END DEEP OCEAN CONV CASE
!
IKT=D%NKT
IKTB=D%NKTB
IKTE=D%NKTE
IKB=D%NKB
IKE=D%NKE
!
GUSERV = (KRR/=0)
!
! compute the coefficients for the uncentred gradient computation near the
! ground
!
RODIER Quentin
committed
IF (OHARAT) THEN
! OHARAT so TKE and length scales at half levels!
ZKEFF(:,:,:) = PLM(:,:,:) * SQRT(PTKEM(:,:,:)) +50.*MFMOIST(:,:,:)
ZKEFF(:,:,:) = MZM(PLM(:,:,:) * SQRT(PTKEM(:,:,:)), D%NKA, KKU, KKL)
ENDIF
!
! Define a cloud mask with ri and rc (used after with a threshold) for Leonard terms
!
IF(TURBN%LHGRAD) THEN
IF ( KRRL >= 1 ) THEN
IF ( KRRI >= 1 ) THEN
ZCLD_THOLD(:,:,:) = PRM(:,:,:,2) + PRM(:,:,:,4)
ELSE
ZCLD_THOLD(:,:,:) = PRM(:,:,:,2)
END IF
END IF
END IF
492
493
494
495
496
497
498
499
500
501
502
503
504
505
506
507
508
509
510
511
512
513
514
515
516
517
!
! Flags for 3rd order quantities
!
GFTH2 = .FALSE.
GFR2 = .FALSE.
GFTHR = .FALSE.
GFWTH = .FALSE.
GFWR = .FALSE.
!
IF (HTOM/='NONE') THEN
GFTH2 = ANY(PFTH2/=0.)
GFR2 = ANY(PFR2 /=0.) .AND. GUSERV
GFTHR = ANY(PFTHR/=0.) .AND. GUSERV
GFWTH = ANY(PFWTH/=0.)
GFWR = ANY(PFWR /=0.) .AND. GUSERV
END IF
!----------------------------------------------------------------------------
!
!* 2. SOURCES OF CONSERVATIVE POTENTIAL TEMPERATURE AND
! PARTIAL THERMAL PRODUCTION
! ---------------------------------------------------------------
!
!* 2.1 Splitted value for cons. potential temperature at t+deltat
!
! Compute the turbulent flux F and F' at time t-dt.
!
RODIER Quentin
committed
IF (OHARAT) THEN
ZF (:,:,:) = -ZKEFF*DZM(PTHLM, D%NKA, KKU, KKL)/PDZZ
ZDFDDTDZ(:,:,:) = -ZKEFF
ZF (:,:,:) = -CSTURB%XCSHF*PPHI3*ZKEFF*DZM(PTHLM, D%NKA, KKU, KKL)/PDZZ
ZDFDDTDZ(:,:,:) = -CSTURB%XCSHF*ZKEFF*D_PHI3DTDZ_O_DDTDZ(D,CSTURB,PPHI3,PREDTH1,PREDR1,PRED2TH3,PRED2THR3,HTURBDIM,GUSERV)
END IF
!
IF (TURBN%LHGRAD) THEN
! Compute the Leonard terms for thl
ZDELTAX= XXHAT(3) - XXHAT(2)
ZF_LEONARD (:,:,:)= TURBN%XCOEFHGRADTHL*ZDELTAX*ZDELTAX/12.0*( &
MXF(GX_W_UW(PWM(:,:,:), XDXX,XDZZ,XDZX,D%NKA,KKU,KKL))&
*MZM(GX_M_M(PTHLM(:,:,:),XDXX,XDZZ,XDZX,D%NKA, KKU, KKL), D%NKA, KKU, KKL) &
+ MYF(GY_W_VW(PWM(:,:,:), XDYY,XDZZ,XDZY,D%NKA,KKU,KKL)) &
*MZM(GY_M_M(PTHLM(:,:,:),XDYY,XDZZ,XDZY,D%NKA, KKU, KKL), D%NKA, KKU, KKL) )
END IF
!
! Effect of 3rd order terms in temperature flux (at flux point)
!
! d(w'2th')/dz
IF (GFWTH) THEN
Z3RDMOMENT= M3_WTH_W2TH(D,CSTURB,D%NKA,KKU,KKL,PREDTH1,PREDR1,PD,ZKEFF,PTKEM)
!
ZF = ZF + Z3RDMOMENT * PFWTH
ZDFDDTDZ = ZDFDDTDZ + D_M3_WTH_W2TH_O_DDTDZ(D,CSTURB,D%NKA,KKU,KKL,PREDTH1,PREDR1,&
& PD,PBLL_O_E,PETHETA,ZKEFF,PTKEM) * PFWTH
END IF
!
! d(w'th'2)/dz
IF (GFTH2) THEN
Z3RDMOMENT= M3_WTH_WTH2(D,CSTURB,PREDTH1,PREDR1,PD,PBLL_O_E,PETHETA)
ZF = ZF + Z3RDMOMENT * MZM(PFTH2, D%NKA, KKU, KKL)
ZDFDDTDZ = ZDFDDTDZ + D_M3_WTH_WTH2_O_DDTDZ(D,CSTURB,Z3RDMOMENT,PREDTH1,PREDR1,&
& PD,PBLL_O_E,PETHETA) * MZM(PFTH2, D%NKA, KKU, KKL)
END IF
!
! d(w'2r')/dz
IF (GFWR) THEN
ZF = ZF + M3_WTH_W2R(D,CSTURB,D%NKA,KKU,KKL,PD,ZKEFF,&
& PTKEM,PBLL_O_E,PEMOIST,PDTH_DZ) * PFWR
ZDFDDTDZ = ZDFDDTDZ + D_M3_WTH_W2R_O_DDTDZ(D,CSTURB,D%NKA,KKU,KKL,PREDTH1,PREDR1,&
& PD,ZKEFF,PTKEM,PBLL_O_E,PEMOIST) * PFWR
END IF
!
! d(w'r'2)/dz
IF (GFR2) THEN
ZF = ZF + M3_WTH_WR2(D,CSTURB,D%NKA,KKU,KKL,PD,ZKEFF,PTKEM,&
& PSQRT_TKE,PBLL_O_E,PBETA,PLEPS,PEMOIST,PDTH_DZ) * MZM(PFR2, D%NKA, KKU, KKL)
ZDFDDTDZ = ZDFDDTDZ + D_M3_WTH_WR2_O_DDTDZ(D,CSTURB,D%NKA,KKU,KKL,PREDTH1,PREDR1,PD,&
& ZKEFF,PTKEM,PSQRT_TKE,PBLL_O_E,PBETA,PLEPS,PEMOIST) * MZM(PFR2, D%NKA, KKU, KKL)
END IF
!
! d(w'th'r')/dz
IF (GFTHR) THEN
Z3RDMOMENT= M3_WTH_WTHR(D,CSTURB,D%NKA,KKU,KKL,PREDR1,PD,ZKEFF,PTKEM,PSQRT_TKE,PBETA,&
& PLEPS,PEMOIST)
!
ZF = ZF + Z3RDMOMENT * MZM(PFTHR, D%NKA, KKU, KKL)
ZDFDDTDZ = ZDFDDTDZ + D_M3_WTH_WTHR_O_DDTDZ(D,CSTURB,Z3RDMOMENT,PREDTH1,&
& PREDR1,PD,PBLL_O_E,PETHETA) * MZM(PFTHR, D%NKA, KKU, KKL)
! compute interface flux
RODIER Quentin
committed
IF (OCOUPLES) THEN ! Autocoupling O-A LES
IF (OOCEAN) THEN ! ocean model in coupled case
ZF(:,:,IKE) = (TURBN%XSSTFL_C(:,:,1)+TURBN%XSSRFL_C(:,:,1)) &
*0.5* ( 1. + PRHODJ(:,:,KKU)/PRHODJ(:,:,IKE) )
ELSE ! atmosph model in coupled case
ZF(:,:,IKB) = TURBN%XSSTFL_C(:,:,1) &
*0.5* ( 1. + PRHODJ(:,:,D%NKA)/PRHODJ(:,:,IKB) )
ENDIF
!
ELSE ! No coupling O and A cases
! atmosp bottom
!*In 3D, a part of the flux goes vertically,
! and another goes horizontally (in presence of slopes)
!*In 1D, part of energy released in horizontal flux is taken into account in the vertical part
IF (HTURBDIM=='3DIM') THEN
ZF(:,:,IKB) = ( PIMPL*PSFTHP(:,:) + PEXPL*PSFTHM(:,:) ) &
* PDIRCOSZW(:,:) &
* 0.5 * (1. + PRHODJ(:,:,D%NKA) / PRHODJ(:,:,IKB))
ELSE
ZF(:,:,IKB) = ( PIMPL*PSFTHP(:,:) + PEXPL*PSFTHM(:,:) ) &
/ PDIRCOSZW(:,:) &
* 0.5 * (1. + PRHODJ(:,:,D%NKA) / PRHODJ(:,:,IKB))
END IF
IF (OOCEAN) THEN
ZF(:,:,IKE) = XSSTFL(:,:) *0.5*(1. + PRHODJ(:,:,KKU) / PRHODJ(:,:,IKE))
ELSE !end ocean case (in nocoupled case)
! atmos top
#ifdef REPRO48
#else
ZF(:,:,IKE)=0.
#endif
END IF
END IF !end no coupled cases
! Compute the split conservative potential temperature at t+deltat
CALL TRIDIAG_THERMO(D,D%NKA,KKU,KKL,PTHLM,ZF,ZDFDDTDZ,PTSTEP,PIMPL,PDZZ,&
PRHODJ,PTHLP)
!
! Compute the equivalent tendency for the conservative potential temperature
!
ZRWTHL(:,:,:)= PRHODJ(:,:,:)*(PTHLP(:,:,:)-PTHLM(:,:,:))/PTSTEP
! replace the flux by the Leonard terms above ZALT and ZCLD_THOLD
IF (TURBN%LHGRAD) THEN
DO JK=1,KKU
ZALT(:,:,JK) = PZZ(:,:,JK)-XZS(:,:)
END DO
WHERE ( (ZCLD_THOLD(:,:,:) >= TURBN%XCLDTHOLD) .AND. ( ZALT(:,:,:) >= TURBN%XALTHGRAD) )
ZRWTHL(:,:,:) = -GZ_W_M(MZM(PRHODJ(:,:,:), D%NKA, KKU, KKL)*ZF_LEONARD(:,:,:),XDZZ,&
D%NKA, KKU, KKL)
END WHERE
END IF
!
PRTHLS(:,:,:)= PRTHLS(:,:,:) + ZRWTHL(:,:,:)
!
!* 2.2 Partial Thermal Production
!
! Conservative potential temperature flux :
!
ZFLXZ(:,:,:) = ZF &
+ PIMPL * ZDFDDTDZ * DZM(PTHLP - PTHLM, D%NKA, KKU, KKL) / PDZZ
! replace the flux by the Leonard terms
IF (TURBN%LHGRAD) THEN
WHERE ( (ZCLD_THOLD(:,:,:) >= TURBN%XCLDTHOLD) .AND. ( ZALT(:,:,:) >= TURBN%XALTHGRAD) )
ZFLXZ(:,:,:) = ZF_LEONARD(:,:,:)
END WHERE
END IF
ZFLXZ(:,:,D%NKA) = ZFLXZ(:,:,IKB)
IF (OOCEAN) THEN
ZFLXZ(:,:,KKU) = ZFLXZ(:,:,IKE)
END IF
DO JK=IKTB+1,IKTE-1
PWTH(:,:,JK)=0.5*(ZFLXZ(:,:,JK)+ZFLXZ(:,:,JK+KKL))
END DO
!
PWTH(:,:,IKB)=0.5*(ZFLXZ(:,:,IKB)+ZFLXZ(:,:,IKB+KKL))
!
IF (OOCEAN) THEN
PWTH(:,:,IKE)=0.5*(ZFLXZ(:,:,IKE)+ZFLXZ(:,:,IKE+KKL))
PWTH(:,:,D%NKA)=0.
PWTH(:,:,KKU)=ZFLXZ(:,:,KKU)
ELSE
PWTH(:,:,D%NKA)=0.5*(ZFLXZ(:,:,D%NKA)+ZFLXZ(:,:,D%NKA+KKL))
PWTH(:,:,IKE)=PWTH(:,:,IKE-KKL)
END IF
!
IF ( OTURB_FLX .AND. TPFILE%LOPENED ) THEN
! stores the conservative potential temperature vertical flux
TZFIELD%CMNHNAME = 'THW_FLX'
TZFIELD%CSTDNAME = ''
TZFIELD%CLONGNAME = 'THW_FLX'
TZFIELD%CUNITS = 'K m s-1'
TZFIELD%CDIR = 'XY'
TZFIELD%CCOMMENT = 'Conservative potential temperature vertical flux'
TZFIELD%NGRID = 4
TZFIELD%NTYPE = TYPEREAL
TZFIELD%NDIMS = 3
TZFIELD%LTIMEDEP = .TRUE.
CALL IO_Field_write(TPFILE,TZFIELD,ZFLXZ)
END IF
!
! Contribution of the conservative temperature flux to the buoyancy flux
IF (OOCEAN) THEN
PTP(:,:,:)= CST%XG*CST%XALPHAOC * MZF(ZFLXZ,D%NKA, KKU, KKL )
IF (KRR /= 0) THEN
PTP(:,:,:) = PBETA * MZF( MZM(PETHETA,D%NKA, KKU, KKL) * ZFLXZ,D%NKA, KKU, KKL )
PTP(:,:,IKB)= PBETA(:,:,IKB) * PETHETA(:,:,IKB) * &
0.5 * ( ZFLXZ (:,:,IKB) + ZFLXZ (:,:,IKB+KKL) )
ELSE
PTP(:,:,:)= PBETA * MZF( ZFLXZ,D%NKA, KKU, KKL )
END IF
END IF
!
! Buoyancy flux at flux points
!
PWTHV = MZM(PETHETA, D%NKA, KKU, KKL) * ZFLXZ
PWTHV(:,:,IKB) = PETHETA(:,:,IKB) * ZFLXZ(:,:,IKB)
!
IF (OOCEAN) THEN
! temperature contribution to Buy flux
PWTHV(:,:,IKE) = PETHETA(:,:,IKE) * ZFLXZ(:,:,IKE)
END IF
!* 2.3 Partial vertical divergence of the < Rc w > flux
! Correction for qc and qi negative in AROME
RODIER Quentin
committed
IF(HPROGRAM/='AROME ') THEN
IF ( KRRL >= 1 ) THEN
IF ( KRRI >= 1 ) THEN
PRRS(:,:,:,2) = PRRS(:,:,:,2) - &
PRHODJ*PATHETA*2.*PSRCM*DZF(ZFLXZ/PDZZ, D%NKA, KKU, KKL) &
*(1.0-PFRAC_ICE(:,:,:))
PRRS(:,:,:,4) = PRRS(:,:,:,4) - &
PRHODJ*PATHETA*2.*PSRCM*DZF(ZFLXZ/PDZZ, D%NKA, KKU, KKL) &
*PFRAC_ICE(:,:,:)
ELSE
PRRS(:,:,:,2) = PRRS(:,:,:,2) - &
PRHODJ*PATHETA*2.*PSRCM*DZF(ZFLXZ/PDZZ, D%NKA, KKU, KKL)
END IF
END IF
END IF
!
!* 2.4 Storage in LES configuration
!
RODIER Quentin
committed
IF (OLES_CALL) THEN
CALL SECOND_MNH(ZTIME1)
CALL LES_MEAN_SUBGRID(MZF(ZFLXZ, D%NKA, KKU, KKL), X_LES_SUBGRID_WThl )
CALL LES_MEAN_SUBGRID(MZF(PWM*ZFLXZ, D%NKA, KKU, KKL), X_LES_RES_W_SBG_WThl )
CALL LES_MEAN_SUBGRID(GZ_W_M(PWM,PDZZ, D%NKA, KKU, KKL)*MZF(ZFLXZ, D%NKA, KKU, KKL),&
& X_LES_RES_ddxa_W_SBG_UaThl )
CALL LES_MEAN_SUBGRID(MZF(PDTH_DZ*ZFLXZ, D%NKA, KKU, KKL), X_LES_RES_ddxa_Thl_SBG_UaThl )
CALL LES_MEAN_SUBGRID(-CSTURB%XCTP*PSQRT_TKE/PLM*MZF(ZFLXZ, D%NKA, KKU, KKL), X_LES_SUBGRID_ThlPz )
CALL LES_MEAN_SUBGRID(MZF(MZM(PETHETA, D%NKA, KKU, KKL)*ZFLXZ, D%NKA, KKU, KKL), X_LES_SUBGRID_WThv )
IF (KRR>=1) THEN
CALL LES_MEAN_SUBGRID(MZF(PDR_DZ*ZFLXZ, D%NKA, KKU, KKL), X_LES_RES_ddxa_Rt_SBG_UaThl )
END IF
!* diagnostic of mixing coefficient for heat
ZA = DZM(PTHLP, D%NKA, KKU, KKL)
WHERE (ZA==0.) ZA=1.E-6
ZA = - ZFLXZ / ZA * PDZZ
RODIER Quentin
committed
ZA(:,:,IKB) = CSTURB%XCSHF*PPHI3(:,:,IKB)*ZKEFF(:,:,IKB)
ZA = MZF(ZA, D%NKA, KKU, KKL)
ZA = MIN(MAX(ZA,-1000.),1000.)
CALL LES_MEAN_SUBGRID( ZA, X_LES_SUBGRID_Kh )
!
CALL SECOND_MNH(ZTIME2)
XTIME_LES = XTIME_LES + ZTIME2 - ZTIME1
END IF
!
!* 2.5 New boundary layer depth for TOMs
!
IF (HTOM=='TM06') CALL TM06_H(IKB,IKTB,IKTE,PTSTEP,PZZ,ZFLXZ,PBL_DEPTH)
!
!----------------------------------------------------------------------------
!
!
!* 3. SOURCES OF CONSERVATIVE AND CLOUD MIXING RATIO AND
! COMPLETE THERMAL PRODUCTION
! ------------------------------------------------------
!
!* 3.1 Splitted value for cons. mixing ratio at t+deltat
!
!
IF (KRR /= 0) THEN
! Compute the turbulent flux F and F' at time t-dt.
!
RODIER Quentin
committed
IF (OHARAT) THEN
ZF (:,:,:) = -ZKEFF*DZM(PRM(:,:,:,1), D%NKA, KKU, KKL)/PDZZ
ZDFDDRDZ(:,:,:) = -ZKEFF
ELSE
ZF (:,:,:) = -CSTURB%XCSHF*PPSI3*ZKEFF*DZM(PRM(:,:,:,1), D%NKA, KKU, KKL)/PDZZ
ZDFDDRDZ(:,:,:) = -CSTURB%XCSHF*ZKEFF*D_PSI3DRDZ_O_DDRDZ(D,CSTURB,PPSI3,PREDR1,PREDTH1,PRED2R3,PRED2THR3,HTURBDIM,GUSERV)
ENDIF
!
! Compute Leonard Terms for Cloud mixing ratio
IF (TURBN%LHGRAD) THEN
ZDELTAX= XXHAT(3) - XXHAT(2)
ZF_LEONARD (:,:,:)= TURBN%XCOEFHGRADRM*ZDELTAX*ZDELTAX/12.0*( &
MXF(GX_W_UW(PWM(:,:,:), XDXX,XDZZ,XDZX,D%NKA,KKU,KKL)) &
*MZM(GX_M_M(PRM(:,:,:,1),XDXX,XDZZ,XDZX,D%NKA,KKU,KKL),D%NKA,KKU,KKL) &
+MYF(GY_W_VW(PWM(:,:,:), XDYY,XDZZ,XDZY,D%NKA,KKU,KKL)) &
*MZM(GY_M_M(PRM(:,:,:,1),XDYY,XDZZ,XDZY,D%NKA,KKU,KKL),D%NKA,KKU,KKL) )
END IF
!
! Effect of 3rd order terms in temperature flux (at flux point)
!
! d(w'2r')/dz
IF (GFWR) THEN
Z3RDMOMENT= M3_WR_W2R(D,CSTURB,D%NKA,KKU,KKL,PREDR1,PREDTH1,PD,ZKEFF,PTKEM)
!
ZF = ZF + Z3RDMOMENT * PFWR
ZDFDDRDZ = ZDFDDRDZ + D_M3_WR_W2R_O_DDRDZ(D,CSTURB,D%NKA,KKU,KKL,PREDR1,PREDTH1,PD,&
& PBLL_O_E,PEMOIST,ZKEFF,PTKEM) * PFWR
END IF
!
! d(w'r'2)/dz
IF (GFR2) THEN
Z3RDMOMENT= M3_WR_WR2(D,CSTURB,PREDR1,PREDTH1,PD,PBLL_O_E,PEMOIST)
ZF = ZF + Z3RDMOMENT * MZM(PFR2, D%NKA, KKU, KKL)
ZDFDDRDZ = ZDFDDRDZ + D_M3_WR_WR2_O_DDRDZ(D,CSTURB,Z3RDMOMENT,PREDR1,&
& PREDTH1,PD,PBLL_O_E,PEMOIST) * MZM(PFR2, D%NKA, KKU, KKL)
END IF
!
! d(w'2th')/dz
IF (GFWTH) THEN
ZF = ZF + M3_WR_W2TH(D,CSTURB,D%NKA,KKU,KKL,PD,ZKEFF,&
& PTKEM,PBLL_O_E,PETHETA,PDR_DZ) * PFWTH
ZDFDDRDZ = ZDFDDRDZ + D_M3_WR_W2TH_O_DDRDZ(D,CSTURB,D%NKA,KKU,KKL,PREDR1,PREDTH1,&
& PD,ZKEFF,PTKEM,PBLL_O_E,PETHETA) * PFWTH
END IF
!
! d(w'th'2)/dz
IF (GFTH2) THEN
ZF = ZF + M3_WR_WTH2(D,CSTURB,D%NKA,KKU,KKL,PD,ZKEFF,PTKEM,&
& PSQRT_TKE,PBLL_O_E,PBETA,PLEPS,PETHETA,PDR_DZ) * MZM(PFTH2, D%NKA, KKU, KKL)
ZDFDDRDZ = ZDFDDRDZ + D_M3_WR_WTH2_O_DDRDZ(D,CSTURB,D%NKA,KKU,KKL,PREDR1,PREDTH1,PD,&
&ZKEFF,PTKEM,PSQRT_TKE,PBLL_O_E,PBETA,PLEPS,PETHETA) * MZM(PFTH2, D%NKA, KKU, KKL)
END IF
!
! d(w'th'r')/dz
IF (GFTHR) THEN
Z3RDMOMENT= M3_WR_WTHR(D,CSTURB,D%NKA,KKU,KKL,PREDTH1,PD,ZKEFF,PTKEM,PSQRT_TKE,PBETA,&
& PLEPS,PETHETA)
!
ZF = ZF + Z3RDMOMENT * MZM(PFTHR, D%NKA, KKU, KKL)
ZDFDDRDZ = ZDFDDRDZ + D_M3_WR_WTHR_O_DDRDZ(D,CSTURB,D%NKA,KKU,KKL,Z3RDMOMENT,PREDR1, &
& PREDTH1,PD,PBLL_O_E,PEMOIST) * MZM(PFTHR, D%NKA, KKU, KKL)
END IF
!
! compute interface flux
RODIER Quentin
committed
IF (OCOUPLES) THEN ! coupling NH O-A
IF (OOCEAN) THEN ! ocean model in coupled case
! evap effect on salinity to be added later !!!
ZF(:,:,IKE) = 0.
ELSE ! atmosph model in coupled case
ZF(:,:,IKB) = 0.
! AJOUTER FLUX EVAP SUR MODELE ATMOS
ENDIF
ELSE ! No coupling NH OA case
! atmosp bottom
!* 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
ZF(:,:,IKB) = ( PIMPL*PSFRP(:,:) + PEXPL*PSFRM(:,:) ) &
* PDIRCOSZW(:,:) &
* 0.5 * (1. + PRHODJ(:,:,D%NKA) / PRHODJ(:,:,IKB))
ELSE
ZF(:,:,IKB) = ( PIMPL*PSFRP(:,:) + PEXPL*PSFRM(:,:) ) &
/ PDIRCOSZW(:,:) &
* 0.5 * (1. + PRHODJ(:,:,D%NKA) / PRHODJ(:,:,IKB))
END IF
!
IF (OOCEAN) THEN
! General ocean case
! salinity/evap effect to be added later !!!!!
ZF(:,:,IKE) = 0.
ELSE !end ocean case (in nocoupled case)
! atmos top
#ifdef REPRO48
#else
ZF(:,:,IKE)=0.
#endif
END IF
END IF!end no coupled cases
! Compute the split conservative potential temperature at t+deltat
CALL TRIDIAG_THERMO(D,D%NKA,KKU,KKL,PRM(:,:,:,1),ZF,ZDFDDRDZ,PTSTEP,PIMPL,&
PDZZ,PRHODJ,PRP)
!
! Compute the equivalent tendency for the conservative mixing ratio
!
ZRWRNP (:,:,:) = PRHODJ(:,:,:)*(PRP(:,:,:)-PRM(:,:,:,1))/PTSTEP
!
! replace the flux by the Leonard terms above ZALT and ZCLD_THOLD
IF (TURBN%LHGRAD) THEN
DO JK=1,KKU
ZALT(:,:,JK) = PZZ(:,:,JK)-XZS(:,:)
END DO
WHERE ( (ZCLD_THOLD(:,:,:) >= TURBN%XCLDTHOLD ) .AND. ( ZALT(:,:,:) >= TURBN%XALTHGRAD ) )
ZRWRNP (:,:,:) = -GZ_W_M(MZM(PRHODJ(:,:,:),D%NKA,KKU,KKL)*ZF_LEONARD(:,:,:),XDZZ,D%NKA,KKU,KKL)
END WHERE
END IF
!
PRRS(:,:,:,1) = PRRS(:,:,:,1) + ZRWRNP (:,:,:)
!
!* 3.2 Complete thermal production
!
! cons. mixing ratio flux :
!
ZFLXZ(:,:,:) = ZF &
+ PIMPL * ZDFDDRDZ * DZM(PRP - PRM(:,:,:,1), D%NKA, KKU, KKL) / PDZZ
! replace the flux by the Leonard terms above ZALT and ZCLD_THOLD
IF (TURBN%LHGRAD) THEN
WHERE ( (ZCLD_THOLD(:,:,:) >= TURBN%XCLDTHOLD ) .AND. ( ZALT(:,:,:) >= TURBN%XALTHGRAD ) )
ZFLXZ(:,:,:) = ZF_LEONARD(:,:,:)
END WHERE
END IF
!
ZFLXZ(:,:,D%NKA) = ZFLXZ(:,:,IKB)
!
DO JK=IKTB+1,IKTE-1
PWRC(:,:,JK)=0.5*(ZFLXZ(:,:,JK)+ZFLXZ(:,:,JK+KKL))
END DO
PWRC(:,:,IKB)=0.5*(ZFLXZ(:,:,IKB)+ZFLXZ(:,:,IKB+KKL))
PWRC(:,:,D%NKA)=0.5*(ZFLXZ(:,:,D%NKA)+ZFLXZ(:,:,D%NKA+KKL))
PWRC(:,:,IKE)=PWRC(:,:,IKE-KKL)
!
!
IF ( OTURB_FLX .AND. TPFILE%LOPENED ) THEN
! stores the conservative mixing ratio vertical flux
TZFIELD%CMNHNAME = 'RCONSW_FLX'
TZFIELD%CSTDNAME = ''
TZFIELD%CLONGNAME = 'RCONSW_FLX'
TZFIELD%CUNITS = 'kg m s-1 kg-1'
TZFIELD%CDIR = 'XY'
TZFIELD%CCOMMENT = 'Conservative mixing ratio vertical flux'
TZFIELD%NGRID = 4
TZFIELD%NTYPE = TYPEREAL
TZFIELD%NDIMS = 3
TZFIELD%LTIMEDEP = .TRUE.
CALL IO_Field_write(TPFILE,TZFIELD,ZFLXZ)
END IF
!
! Contribution of the conservative water flux to the Buoyancy flux
IF (OOCEAN) THEN
ZA(:,:,:)= -CST%XG*CST%XBETAOC * MZF(ZFLXZ, D%NKA, KKU, KKL )
ELSE
ZA(:,:,:) = PBETA * MZF( MZM(PEMOIST, D%NKA, KKU, KKL) * ZFLXZ,D%NKA,KKU,KKL )
ZA(:,:,IKB) = PBETA(:,:,IKB) * PEMOIST(:,:,IKB) * &
0.5 * ( ZFLXZ (:,:,IKB) + ZFLXZ (:,:,IKB+KKL) )
PTP(:,:,:) = PTP(:,:,:) + ZA(:,:,:)
END IF
!
! Buoyancy flux at flux points
!
PWTHV = PWTHV + MZM(PEMOIST, D%NKA, KKU, KKL) * ZFLXZ
PWTHV(:,:,IKB) = PWTHV(:,:,IKB) + PEMOIST(:,:,IKB) * ZFLXZ(:,:,IKB)
IF (OOCEAN) THEN
PWTHV(:,:,IKE) = PWTHV(:,:,IKE) + PEMOIST(:,:,IKE)* ZFLXZ(:,:,IKE)
END IF
!
!* 3.3 Complete vertical divergence of the < Rc w > flux
! Correction of qc and qi negative for AROME
RODIER Quentin
committed
IF(HPROGRAM/='AROME ') THEN
IF ( KRRL >= 1 ) THEN
IF ( KRRI >= 1 ) THEN
PRRS(:,:,:,2) = PRRS(:,:,:,2) - &
PRHODJ*PAMOIST*2.*PSRCM*DZF(ZFLXZ/PDZZ,D%NKA,KKU,KKL ) &
*(1.0-PFRAC_ICE(:,:,:))
PRRS(:,:,:,4) = PRRS(:,:,:,4) - &
PRHODJ*PAMOIST*2.*PSRCM*DZF(ZFLXZ/PDZZ,D%NKA,KKU,KKL ) &
*PFRAC_ICE(:,:,:)
ELSE
PRRS(:,:,:,2) = PRRS(:,:,:,2) - &
PRHODJ*PAMOIST*2.*PSRCM*DZF(ZFLXZ/PDZZ,D%NKA,KKU,KKL )
END IF
END IF
END IF
!
!* 3.4 Storage in LES configuration
!
RODIER Quentin
committed
IF (OLES_CALL) THEN
CALL SECOND_MNH(ZTIME1)
CALL LES_MEAN_SUBGRID(MZF(ZFLXZ, D%NKA, KKU, KKL), X_LES_SUBGRID_WRt )
CALL LES_MEAN_SUBGRID(MZF(PWM*ZFLXZ, D%NKA, KKU, KKL), X_LES_RES_W_SBG_WRt )
CALL LES_MEAN_SUBGRID(GZ_W_M(PWM,PDZZ, D%NKA, KKU, KKL)*MZF(ZFLXZ, D%NKA, KKU, KKL),&
& X_LES_RES_ddxa_W_SBG_UaRt )
CALL LES_MEAN_SUBGRID(MZF(PDTH_DZ*ZFLXZ, D%NKA, KKU, KKL), X_LES_RES_ddxa_Thl_SBG_UaRt )
CALL LES_MEAN_SUBGRID(MZF(PDR_DZ*ZFLXZ, D%NKA, KKU, KKL), X_LES_RES_ddxa_Rt_SBG_UaRt )
CALL LES_MEAN_SUBGRID(MZF(MZM(PEMOIST, D%NKA, KKU, KKL)*ZFLXZ, D%NKA, KKU, KKL), X_LES_SUBGRID_WThv , .TRUE. )
CALL LES_MEAN_SUBGRID(-CSTURB%XCTP*PSQRT_TKE/PLM*MZF(ZFLXZ, D%NKA, KKU, KKL), X_LES_SUBGRID_RtPz )
CALL SECOND_MNH(ZTIME2)
XTIME_LES = XTIME_LES + ZTIME2 - ZTIME1
END IF
!
END IF
!
!----------------------------------------------------------------------------
!
!
!* 4. TURBULENT CORRELATIONS : <w Rc>
! -------------------------------
!
!
!* 4.1 <w Rc>
!
RODIER Quentin
committed
IF ( ((OTURB_FLX .AND. TPFILE%LOPENED) .OR. OLES_CALL) .AND. (KRRL > 0) ) THEN
!
! recover the Conservative potential temperature flux :
RODIER Quentin
committed
! With OHARAT is true tke and length scales at half levels
! yet modify to use length scale and tke at half levels from vdfexcuhl
RODIER Quentin
committed
IF (OHARAT) THEN
ZA(:,:,:) = DZM(PIMPL * PTHLP + PEXPL * PTHLM, D%NKA, KKU, KKL) / PDZZ * &