code-saturne-data 4.3.3+repack-1build1 / usr / share / code_saturne / user / cs_user_physical_properties.f90

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

!                      Code_Saturne version 4.3.3
!                      --------------------------
! 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.

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

!===============================================================================
! Purpose:
! -------

!> \file cs_user_physical_properties.f90
!>
!> \brief Definition of physical variable laws.
!>
!> See \subpage physical_properties for examples.
!>

!===============================================================================
!> usphyv
!>
!> \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 = 1 must <b> have been specified </b>
!>    in \ref usipsu if we wish to define a variable specific heat
!>    cpro_cp (otherwise: memory overwrite).
!>
!> - the kivisl field integer key (scalar_diffusivity_id)
!>    must <b> have been specified </b>
!>    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, <b> AT THE FIRST TIME STEP </b> (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

double precision dt(ncelet)

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

!--------
! Formats
!--------

!----
! End
!----

return
end subroutine usphyv


!===============================================================================
!===============================================================================
! Purpose:
! -------

!> usvist
!> \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 dimens, only: ndimfb
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(ncepdp,6), smacel(ncesmp,nvar)

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

!--------
! Formats
!--------

!----
! End
!----

return
end subroutine usvist


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


subroutine ussmag &
!================

 ( nvar   , nscal  , ncepdp , ncesmp ,                            &
   icepdc , icetsm , itypsm ,                                     &
   dt     ,                                                       &
   ckupdc , smacel ,                                              &
   smagor , mijlij , mijmij )

!===============================================================================
!> FONCTION :
!>
!>
!> MODIFICATION UTILISATEUR DE LA CONSTANTE DE SMAGORINSKY
!> DANS LE CAS DE L'UTILISATION D'UN MODELE DYNAMIQUE
!>
!>              SMAGOR = Mij.Lij / Mij.Mij
!>
!> EN FAIT, DES MOYENNES LOCALES DU NUMERATEUR ET DU DENOMINATEUR
!> SONT REALISEES AVANT L'APPEL A USSMAG, SOIT
!>
!>              SMAGOR = < Mij.Lij > / < Mij.Mij >
!>
!> DANS CETTE ROUTINE, Mij.Lij ET Mij.Mij SONT PASSES EN ARGUMENT
!> AVANT LA MOYENNE LOCALE.

!-------------------------------------------------------------------------------
! 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]     smagor        smagorinsky constant in the case of a dynamic
!>                              model
!> \param[in]     mijlij        mij.lij before the local averaging
!> \param[in]     mijmij        mij.mij before the local averaging
!_______________________________________________________________________________

!===============================================================================
! 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(ncepdp,6), smacel(ncesmp,nvar)
double precision smagor(ncelet), mijlij(ncelet), mijmij(ncelet)

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

!----
! End
!----

return
end subroutine ussmag


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

!===============================================================================
! Purpose:
! -------

!> usvima
!> \brief User subroutine dedicated the use of ALE
!>  (Arbitrary Lagrangian Eulerian Method): fills mesh viscosity arrays.
!>
!> This subroutine is called at the beginning of each time step.
!>
!> Here one can modify mesh viscosity value to prevent cells and nodes
!> from huge displacements in awkward areas, such as boundary layer for example.
!>
!> IF variable IORTVM = 0, mesh viscosity modeling is isotropic therefore VISCMX
!> array only needs to be filled.
!> IF variable IORTVM = 1, mesh viscosity modeling is orthotropic therefore
!> all arrays VISCMX, VISCMY and VISCMZ need to be filled.
!>
!> Note that VISCMX, VISCMY and VISCMZ arrays are initialized at the first time step
!> to the value of 1.
!>
!> \section usvima_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]     dt            time step (per cell)
!> \param[out]    viscmx        mesh viscosity in X direction
!> \param[out]    viscmy        mesh viscosity in Y direction
!> \param[out]    viscmz        mesh viscosity in Z direction
!_______________________________________________________________________________

subroutine usvima &
 ( nvar   , nscal  ,                                              &
   dt     ,                                                       &
   viscmx , viscmy , viscmz )

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

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

use paramx
use dimens, only: ndimfb
use pointe
use numvar
use optcal
use cstphy
use entsor
use parall
use period
use albase
use field
use mesh

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

implicit none

! Arguments

integer          nvar   , nscal

double precision dt(ncelet)
double precision viscmx(ncelet), viscmy(ncelet), viscmz(ncelet)

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

!----
! 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 dimens, only: ndimfb
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