!-------------------------------------------------------------------------------
! Code_Saturne version 6.0.0
! --------------------------
! This file is part of Code_Saturne, a general-purpose CFD tool.
!
! Copyright (C) 1998-2019 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 cs_user_physical_properties.f90
!>
!> \brief Definition of physical variable laws.
!>
!> See \subpage physical_properties for examples.
!>
!===============================================================================
!> \brief Definition of physical variable laws.
!>
!> \section Warning
!>
!> It is \b forbidden to modify turbulent viscosity \c visct here
!> (a specific subroutine is dedicated to that: \ref usvist)
!>
!> - icp = 0 must have been specified
!> in \ref usipsu if we wish to define a variable specific heat
!> cpro_cp (otherwise: memory overwrite).
!>
!> - the kivisl field integer key (diffusivity_id)
!> must have been specified
!> in \ref usipsu if we wish to define a variable viscosity
!> \c viscls.
!>
!>
!> \remarks
!> - This routine is called at the beginning of each time step
!> Thus, AT THE FIRST TIME STEP (non-restart case), the only
!> values initialized before this call are those defined
!> - in the GUI or \ref usipsu (cs_user_parameters.f90)
!> - density (initialized at \c ro0)
!> - viscosity (initialized at \c viscl0)
!> - in the GUI or \ref cs_user_initialization
!> - calculation variables (initialized at 0 by defaut
!> or to the value given in the GUI or in \ref cs_user_initialization)
!>
!> - We may define here variation laws for cell properties, for:
!> - density: rom kg/m3
!> - density at boundary faces: romb kg/m3)
!> - molecular viscosity: cpro_viscl kg/(m s)
!> - specific heat: cpro_cp J/(kg degrees)
!> - diffusivities associated with scalars: cpro_vscalt kg/(m s)
!>
!> \b Warning: if the scalar is the temperature, cpro_vscalt corresponds
!> to its conductivity (Lambda) in W/(m K)
!>
!>
!> The types of boundary faces at the previous time step are available
!> (except at the first time step, where arrays \c itypfb and \c itrifb have
!> not been initialized yet)
!>
!> It is recommended to keep only the minimum necessary in this file
!> (i.e. remove all unused example code)
!>
!>
!> \section usphyv_cell_id Cells identification
!>
!> Cells may be identified using the \ref getcel subroutine.
!> The syntax of this subroutine is described in the
!> \ref cs_user_boundary_conditions subroutine,
!> but a more thorough description can be found in the user guide.
!
!-------------------------------------------------------------------------------
!-------------------------------------------------------------------------------
! Arguments
!______________________________________________________________________________.
! mode name role !
!______________________________________________________________________________!
!> \param[in] nvar total number of variables
!> \param[in] nscal total number of scalars
!> \param[in] mbrom indicator of filling of romb array
!> \param[in] dt time step (per cell)
!_______________________________________________________________________________
subroutine usphyv &
( nvar , nscal , &
mbrom , &
dt )
!===============================================================================
!===============================================================================
! Module files
!===============================================================================
use paramx
use pointe
use numvar
use optcal
use cstphy
use cstnum
use entsor
use parall
use period
use ppppar
use ppthch
use ppincl
use field
use mesh
use lagran
use cs_c_bindings
!===============================================================================
implicit none
! Arguments
integer nvar , nscal
integer mbrom
integer ifcvsl, ncelt, icelt, iel
integer, allocatable, dimension(:) :: lstcel
double precision dt(ncelet)
double precision, dimension(:), pointer :: cpro_vscalT, cpro_cp, cpro_crom, cpro_viscl
!===============================================================================
!--------
! Formats
!--------
allocate(lstcel(ncel))
call field_get_val_s(icp, cpro_cp)
call field_get_val_s(icrom, cpro_crom)
call field_get_key_int(ivarfl(isca(iscalt)), kivisl, ifcvsl)
call field_get_val_s(ifcvsl, cpro_vscalT)
call field_get_val_s(iviscl, cpro_viscl)
call getcel('solid', ncelt, lstcel)
do icelt = 1, ncelt
iel = lstcel(icelt)
cpro_vscalT(iel) = 18.d0
cpro_cp(iel) = 525.d0
cpro_crom(iel) = 8027.d0
enddo
!----
! End
!----
return
end subroutine usphyv
!===============================================================================
!===============================================================================
!> \brief Modify turbulent viscosity
!>
!> This subroutine is called at beginning of each time step
!> after the computation of the turbulent viscosity
!> (physical quantities have already been computed in \ref usphyv).
!>
!> Turbulent viscosity \f$ \mu_T \f$ (kg/(m s)) can be modified.
!>
!> A modification of the turbulent viscosity can lead to very
!> significant differences betwwen solutions and even give wrong
!> results.
!>
!> This subroutine is therefore reserved to expert users.
!
!-------------------------------------------------------------------------------
!-------------------------------------------------------------------------------
! Arguments
!______________________________________________________________________________.
! mode name role !
!______________________________________________________________________________!
!> \param[in] nvar total number of variables
!> \param[in] nscal total number of scalars
!> \param[in] ncepdp number of cells with head loss
!> \param[in] ncesmp number of cells with mass source term
!> \param[in] icepdc head loss cell numbering
!> \param[in] icetsm numbering of cells with mass source term
!> \param[in] itypsm kind of mass source for each variable
!> (cf. \ref cs_user_mass_source_terms)
!> \param[in] dt time step (per cell)
!> \param[in] ckupdc work array for head loss terms
!> \param[in] smacel values of variables related to mass source
!> term. If ivar=ipr, smacel=mass flux
!_______________________________________________________________________________
subroutine usvist &
( nvar , nscal , ncepdp , ncesmp , &
icepdc , icetsm , itypsm , &
dt , &
ckupdc , smacel )
!===============================================================================
!===============================================================================
! Module files
!===============================================================================
use paramx
use numvar
use optcal
use cstphy
use entsor
use parall
use period
use mesh
use field
use field_operator
!===============================================================================
implicit none
! Arguments
integer nvar , nscal
integer ncepdp , ncesmp
integer icepdc(ncepdp)
integer icetsm(ncesmp), itypsm(ncesmp,nvar)
double precision dt(ncelet)
double precision ckupdc(6,ncepdp), smacel(ncesmp,nvar)
!===============================================================================
!--------
! Formats
!--------
!----
! End
!----
return
end subroutine usvist
!===============================================================================
!===============================================================================
!> \brief user modification of the Smagorinsky constant in the case of a
!> dynamic model
!>
!> SMAGOR = Mij.Lij / Mij.Mij
!>
!> The local avergaes of the numerator and denominator are done before calling
!> this subroutine, so
!>
!> SMAGOR = < Mij.Lij > / < Mij.Mij >
!>
!> In this subroutine, Mij.Lij and Mij.Mij are passed as arguments before
!> the local average.
!-------------------------------------------------------------------------------
! Arguments
!______________________________________________________________________________.
! mode name role !
!______________________________________________________________________________!
!> \param[in] nvar total number of variables
!> \param[in] nscal total number of scalars
!> \param[in] ncepdp number of cells with head loss
!> \param[in] ncesmp number of cells with mass source term
!> \param[in] icepdc head loss cell numbering
!> \param[in] icetsm numbering of cells with mass source term
!> \param[in] itypsm kind of mass source for each variable
!> (cf. \ref cs_user_mass_source_terms)
!> \param[in] dt time step (per cell)
!> \param[in] ckupdc work array for head loss terms
!> \param[in] smacel values of variables related to mass source
!> term. If ivar=ipr, smacel=mass flux
!> \param[in] mijlij mij.lij before the local averaging
!> \param[in] mijmij mij.mij before the local averaging
!_______________________________________________________________________________
subroutine ussmag &
( nvar , nscal , ncepdp , ncesmp , &
icepdc , icetsm , itypsm , &
dt , &
ckupdc , smacel , &
mijlij , mijmij )
!===============================================================================
!===============================================================================
! Module files
!===============================================================================
use paramx
use numvar
use cstnum
use optcal
use cstphy
use entsor
use parall
use field
use mesh
!===============================================================================
implicit none
! Arguments
integer nvar , nscal
integer ncepdp , ncesmp
integer icepdc(ncepdp)
integer icetsm(ncesmp), itypsm(ncesmp,nvar)
double precision dt(ncelet)
double precision ckupdc(6,ncepdp), smacel(ncesmp,nvar)
double precision mijlij(ncelet), mijmij(ncelet)
! Local
double precision, dimension(:), pointer :: cpro_smago
call field_get_val_s(ismago, cpro_smago)
!===============================================================================
!----
! End
!----
return
end subroutine ussmag
!===============================================================================
!===============================================================================
!> \brief User subroutine dedicated the use of ALE
!> (Arbitrary Lagrangian Eulerian Method): fills mesh viscosity arrays.
!>
!> Here one can modify mesh viscosity value to prevent cells and nodes
!> from huge displacements in awkward areas, such as boundary layer for example.
!>
!> This subroutine is called once per computation, before restart files
!> are read, so the mesh is always in the initial position at this stage.
!>
!> Note that by default, the mesh viscosity is initialized to a uniform
!> value of 1.
!
!-------------------------------------------------------------------------------
!-------------------------------------------------------------------------------
! Arguments
!______________________________________________________________________________.
! mode name role !
!______________________________________________________________________________!
!_______________________________________________________________________________
subroutine usvima
!===============================================================================
!===============================================================================
! Module files
!===============================================================================
use paramx
use pointe
use numvar
use optcal
use cstphy
use entsor
use parall
use period
use albase
use field
use mesh
use cs_c_bindings
!===============================================================================
implicit none
! Arguments
! Local
integer idftnp
double precision, dimension(:), pointer :: cpro_vism_s
double precision, dimension(:,:), pointer :: cpro_vism_v
type(var_cal_opt) :: vcopt
!===============================================================================
call field_get_key_struct_var_cal_opt(ivarfl(iuma), vcopt)
idftnp = vcopt%idften
if (iand(idftnp, ISOTROPIC_DIFFUSION).ne.0) then
call field_get_val_s(ivisma, cpro_vism_s)
else if (iand(idftnp, ANISOTROPIC_LEFT_DIFFUSION).ne.0) then
call field_get_val_v(ivisma, cpro_vism_v)
endif
!----
! Formats
!----
!----
! End
!----
return
end subroutine usvima
!===============================================================================
! Purpose:
! -------
!> usatph
!> \brief User subroutine dedicated to modifie physical properties of the
!> atmospheric module
!>
!> This subroutine is called at beginning of each time step at the end of
!> atphyv.
!
!-------------------------------------------------------------------------------
!-------------------------------------------------------------------------------
! Arguments
!______________________________________________________________________________.
! mode name role !
!______________________________________________________________________________!
!_______________________________________________________________________________
subroutine usatph
!===============================================================================
! Module files
!===============================================================================
use paramx
use pointe
use numvar
use optcal
use cstphy
use entsor
use parall
use period
use albase
use field
use mesh
!===============================================================================
implicit none
!----
! Formats
!----
!----
! End
!----
return
end subroutine usatph