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

! This file is part of Code_Saturne, a general-purpose CFD tool.
!
! Copyright (C) 1998-2016 EDF S.A.
!
! This program is free software; you can redistribute it and/or modify it under
! the terms of the GNU General Public License as published by the Free Software
! Foundation; either version 2 of the License, or (at your option) any later
! version.
!
! This program is distributed in the hope that it will be useful, but WITHOUT
! ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS
! FOR A PARTICULAR PURPOSE.  See the GNU General Public License for more
! details.
!
! You should have received a copy of the GNU General Public License along with
! this program; if not, write to the Free Software Foundation, Inc., 51 Franklin
! Street, Fifth Floor, Boston, MA 02110-1301, USA.

!-------------------------------------------------------------------------------
!> \file solvar.f90
!> \brief Atmospheric soil module - Compute ground level variables
!
!> \brief   Soil / atmosphere interface routine
!>   Compute the following surface variables :
!>-     temperature with a prognostic equation of the "force-restore" type
!>                       (deardorff 1978)
!>-     humidity with a two reservoirs method
!
!-------------------------------------------------------------------------------
! Arguments
!______________________________________________________________________________.
!  mode           name          role
!______________________________________________________________________________!
!> \param[in]   temp    temperature
!> \param[in]   qv      specific humidity
!> \param[in]   rom     Density
!> \param[in]   dt      ratio of the local time step to the reference one
!> \param[in]   rcodcl  Boundary conditions type
!-------------------------------------------------------------------------------
subroutine solvar ( temp , qv ,rom , dt, rcodcl )

!===============================================================================
! Module files
!===============================================================================

use paramx
use dimens
use numvar
use optcal
use cstphy
use cstnum
use entsor
use parall
use period
use ppppar
use ppthch
use ppincl
use atincl
use atsoil
use mesh
use field


implicit none

!===============================================================================

integer idim2
parameter ( idim2 = 26 )
!==============================================================================


!... declaration des variables externes


double precision rcodcl(nfabor,nvarcl,3)

double precision temp(ncelet)
double precision qv(ncelet)
double precision rom(ncelet),dt(ncelet)


!... declaration des variables internes

integer ifac,iel,isol
double precision rcodcx, rcodcy, rcodcz, rcodsn
double precision rnx, rny, rnz
double precision tx, ty, tz, txn
double precision vtmod, upx, upy, upz, usn
integer ichal
integer iseuil
double precision zreel
double precision b,c,d,tau1,precip,evapor,albedo
double precision emis,csol,veg,c1w,c2w,z0t,tprof
double precision act,rib,fh,fhden,rscp1,rscp2
double precision pres1,tpot1,tpot2,tpotv1,tpotv2
double precision cphum,cht,chq,tsplus,qvsplu,w1plus,w2plus
double precision w1num,w1den,w2num,w2den
double precision hu,esat,cstder,qsat,dqsat,rapsat
double precision tssol,qvsol,w1,w2,foir,fos
double precision ray1,chas1,chal1,rapp1,premem
double precision ray2,chas2,chal2,rapp2,secmem
double precision w1min,w1max,w2min,w2max
double precision r1,r2,tseuil,dum

double precision, dimension(:,:), pointer :: vel

!===============================================================================

! Map field arrays
call field_get_val_v(ivarfl(iu), vel)

!     ==========================
!     1) initialisations locales
!     ==========================

b = 5.d0
c = 5.d0
d = 5.d0

tau1 = 86400.d0

w1min = 0.d0
w1max = 1.d0
w2min = 0.d0
w2max = 1.d0

!  pas de precipitations pour l'instant
precip = 0.d0

!  tseuil pour le flux anthropogenique (m.a. atwater 1975)
tseuil = 16.d0 + tkelvi

do isol = 1, nfmodsol
  ifac = indsol(isol)

  tssol = solution_sol(isol)%temp_sol + tkelvi
  qvsol = solution_sol(isol)%total_water
  w1    = solution_sol(isol)%w1
  w2    = solution_sol(isol)%w2

  z0t    = solution_sol(isol)%constantes%rugthe
  emis   = solution_sol(ifac)%constantes%emissi
  albedo = solution_sol(ifac)%constantes%albedo
  csol   = solution_sol(isol)%constantes%csol
  veg    = solution_sol(isol)%constantes%vegeta
  c1w    = solution_sol(isol)%constantes%c1w
  c2w    = solution_sol(isol)%constantes%c2w
  r1     = solution_sol(isol)%constantes%r1
  r2     = solution_sol(isol)%constantes%r2
  tprof  = solution_sol(isol)%constantes%tprof

  foir = soilvert(1)%foir
  fos  = soilvert(1)%fos

  !     ==================================================================
  !     2) calcul du vecteur vitesse tangent (identique a celui fait ds fr
  !     ==================================================================

  ! ---> NORMALE UNITAIRE

  rnx = surfbo(1,ifac)/surfbn(ifac)
  rny = surfbo(2,ifac)/surfbn(ifac)
  rnz = surfbo(3,ifac)/surfbn(ifac)

  ! ---> PROJECTION DE LA VITESSE DE DEFILEMENT
  !           (utilisee plusieurs fois ensuite)

  rcodcx = rcodcl(ifac,iu,1)
  rcodcy = rcodcl(ifac,iv,1)
  rcodcz = rcodcl(ifac,iw,1)

  rcodsn = rcodcx*rnx + rcodcy*rny + rcodcz*rnz
  rcodcl(ifac,iu,1) = rcodcx - rcodsn*rnx
  rcodcl(ifac,iv,1) = rcodcy - rcodsn*rny
  rcodcl(ifac,iw,1) = rcodcz - rcodsn*rnz

  ! ---> VITESSE TANGENTIELLE RELATIVE

  upx = vel(1,ifabor(ifac))
  upy = vel(2,ifabor(ifac))
  upz = vel(3,ifabor(ifac))

  usn = upx*rnx + upy*rny + upz*rnz
  tx  = upx - usn*rnx
  ty  = upy - usn*rny
  tz  = upz - usn*rnz
  tx  = tx - rcodcl(ifac,iu,1)
  ty  = ty - rcodcl(ifac,iv,1)
  tz  = tz - rcodcl(ifac,iw,1)
  txn = sqrt(tx**2 + ty**2 + tz**2)
  vtmod = txn

  iel = ifabor(ifac)
  zreel = xyzcen(3,iel)

  if (pourcent_sol(isol,1) > 50) then

    !     ====================================
    !     3) cas particulier des points de mer
    !     ====================================

    ! on impose t = tmer et hr = 100 %
    esat = 610.78d0*exp(17.2694d0*tmer/(tmer + tkelvi-35.86d0))

    if (imeteo.eq.0) then
      call atmstd(zreel,pres1,dum,dum)
    else
      call intprf                                                       &
         !==========
         (nbmett, nbmetm,                                               &
          ztmet, tmmet, phmet, zreel, ttcabs, pres1)
    endif

    tsplus = tmer + tkelvi
    qvsplu = esat/(rvsra*pres1 + esat*(1.d0 - rvsra))

  else

    !     ============================================
    !     4) calcul du richardson et de la fonction fh
    !     ============================================

    act = xkappa/log((distb(ifac) + z0t)/z0t)

    rscp1 = (rair/cp0)*(1.d0 + (rvsra - cpvcpa)*qvsol)
    rscp2 = (rair/cp0)*(1.d0 + (rvsra - cpvcpa)*qv(iel))

    if (imeteo.eq.0) then
      call atmstd(zreel,pres1,dum,dum)
    else
      call intprf                                                       &
         !==========
         (nbmett, nbmetm,                                               &
          ztmet, tmmet, phmet, zreel, ttcabs, pres1)
    endif

    tpot1 = solution_sol(isol)%tempp
    tpot2 = temp(iel)

    tpotv1 = tpot1*(1.d0 + (rvsra - 1.d0)*qvsol)
    tpotv2 = tpot2*(1.d0 + (rvsra - 1.d0)*qv(iel))

    rib = 2.d0*abs(gz)*distb(ifac)*(tpotv2 - tpotv1)/(tpotv1 + tpotv2)      &
         /vtmod/vtmod
    if(rib.ge.0.d0) then
      fh = 1.d0/(1.d0 + 3.d0*b*rib*sqrt(1.d0 + d*rib))
    else
      fhden = 3.d0*b*c*act*act*sqrt((distb(ifac) + z0t)/z0t)
      fh = 1.d0 - (3.d0*b*rib)/(1.d0 + fhden*sqrt(abs(rib)))
    endif

    !     ==================================================================
    !     5) calcul des coefficients pour flux de chaleur sensible et latent
    !     ==================================================================

    cphum = cp0*(1.d0 + (cpvcpa-1.d0)*qvsol)
    cht = rom(iel)*cphum*act*act*fh*vtmod*((ps/pres1)**rscp1)
    chq = rom(iel)*act*act*fh*vtmod*(clatev - 2370.d0*(tssol - tkelvi))

    !     ==================================================================
    !     6) calcul des teneurs en eau des reservoirs superficiel et profond
    !     ==================================================================

    evapor = -rom(iel)*act*act*fh*vtmod*(qv(iel) - qvsol)

    w1num = w1 + dt(iel)*(precip - evapor)/c1w +                        &
            w2*dt(iel)/(tau1 + c2w*dt(iel))

    w1den = 1.d0 + 1.d0/(tau1/dt(iel) + c2w)
    w1plus = w1num/w1den
    w1plus = max(w1plus,w1min)
    w1plus = min(w1plus,w1max)
    w2num = w2*tau1 + w1plus*dt(iel)*c2w
    w2den = tau1 + dt(iel)*c2w
    w2plus = w2num/w2den
    w2plus = max(w2plus,w2min)
    w2plus = min(w2plus,w2max)
    solution_sol(isol)%w1 = w1plus
    solution_sol(isol)%w2 = w2plus
    hu = 0.5d0*(1.d0-cos(pi*w1plus))

    !     ==================================================================
    !     7) calcul de la pression de vapeur saturante esat et de d(qsat)/dt
    !     ==================================================================

    esat = 610.78d0*exp(17.2694d0*(tssol - tkelvi)/(tssol - 35.86d0))
    rapsat = rvsra*pres1+esat*(1.d0-rvsra)
    qsat = esat/rapsat
    cstder = 17.2694d0*(tkelvi - 35.86d0)
    dqsat = pres1*rvsra/rapsat/rapsat*cstder*esat                     &
         /(tssol - 35.86d0)/(tssol - 35.86d0)

    !     ===========================================================
    !     8) calcul du premier membre de l'equation d'evolution de tssol
    !     ===========================================================

    !  prise en compte du flux anthropogenique
    !  en-dessous de tseuil, ce flux depend de la temperature
    iseuil = 0
    if(tssol.lt.tseuil) iseuil = 1

    ichal = 1
    !  si e0 < 0 pas de contribution du flux de chaleur latente dans le bilan
    !     if(evapor    .lt.0.) ichal=0

    ray1 = 4.d0*emis*stephn*(tssol**3)
    chas1 = cht
    chal1 = chq*hu*dqsat
    rapp1 = 2.d0*pi/tau1

    premem = csol*(ray1 + chas1 + chal1*ichal + r2*iseuil) + rapp1

    !     ==========================================================
    !     9) calcul du second membre de l'equation d'evolution de tssol
    !     ==========================================================

    !  !! fos contient deja le facteur (1-albedo) !
    ray2 = fos + emis*foir + 3.d0*emis*stephn*(tssol**4)
    chas2 = cht*tpot2*((pres1/ps)**rscp1)
    chal2 = chq*(qv(iel)*(1.d0 - veg*(1.d0 - hu)) - hu*(qsat - tssol*dqsat))
    rapp2 = 2.d0*pi*(tprof + tkelvi)/tau1

    secmem = csol*(ray2 + chas2+chal2*ichal + r1 + tseuil*r2*iseuil)            &
           + rapp2
    !     ===========================================
    !     10) calcul des nouveaux parametres du sol
    !     ===========================================

    tsplus = (tssol + dt(iel)*secmem) /                                 &
         (1.d0 + dt(iel)*premem)

    qvsplu = hu*(qsat+dqsat*(tsplus - tssol))                           &
         + veg*qv(iel)*(1.d0 - hu)

    !  cas d'un flux de rosee
    !      if(qv(i,j,k+1).gt.qsat.and.hu.ne.1.d0) then
    !        hu=1.d0
    !        qvsplu=qsat
    !      endif

  endif

  !     (indicateur terre/mer)

  !     ================================
  !     11) mise a jour du tableau solva
  !     ================================

  solution_sol(isol)%temp_sol = tsplus - tkelvi
  solution_sol(isol)%tempp = tsplus*((ps/pres1)**((rair/cp0)*           &
       (1.d0+(rvsra-cpvcpa)*qvsplu)))
  solution_sol(isol)%total_water = qvsplu

enddo

return

end subroutine solvar
