source: branches/jerome/src_flexwrf_v3.1/calcmatrix.f90 @ 16

!***********************************************************************
!* Copyright 1998,1999,2000,2001,2002,2005,2007,2008,2009,2010         *
!* Andreas Stohl, Petra Seibert, A. Frank, Gerhard Wotawa,             *
!* Caroline Forster, Sabine Eckhardt, John Burkhart, Harald Sodemann   *
!*                                                                     *
!* This file is part of FLEXPART.                                      *
!*                                                                     *
!* FLEXPART 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 3 of the License, or   *
!* (at your option) any later version.                                 *
!*                                                                     *
!* FLEXPART 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 FLEXPART.  If not, see <http://www.gnu.org/licenses/>.   *
!***********************************************************************

      subroutine calcmatrix(lconv,delt,cbmf)
!                             o    i    o
!******************************************************************
!     This subroutine calculates the matrix describing convective 
!     redistribution of mass in a grid column, using the subroutine
!     convect43c.f provided by Kerry Emanuel.
!
!     Petra Seibert, Bernd C. Krueger, 2000-2001
!
!     changed by C. Forster, November 2003 - February 2004
!     array fmassfrac(nconvlevmax,nconvlevmax) represents
!     the convective redistribution matrix for the particles
!
!     20 Oct 2005 - R. Easter - added calc of pconv_hpa(nconvlev+1)
!     16 Nov 2005 - R. Easter - pconv,phconv are set in convmix
!                               using pph & pphn
!
!******************************************************************

! lconv        indicates whether there is convection in this cell, or not
! delt         time step for convection [s]
! cbmf         cloud base mass flux

!      include 'includepar'
!      include 'includecom'
!      include 'includeconv'
  use par_mod
  use com_mod
  use conv_mod

  implicit none

  real :: rlevmass,summe

  integer :: iflag, k, kk, kuvz

  !1-d variables for convection
  !variables for redistribution matrix
  real :: cbmfold, precip, qprime
  real :: tprime, wd, f_qvsat
  real :: delt,cbmf
  logical :: lconv

  lconv = .false.

   
! calculate pressure at eta levels for use in convect
! and assign temp & spec. hum. to 1D workspace
! -------------------------------------------------------

! pconv(1) is the pressure at the first level above ground
! phconv(k) is the pressure between levels k-1 and k 
! dp(k) is the pressure difference "around" tconv(k)
! phconv(kmax) must also be defined 1/2 level above pconv(kmax)
! Therefore, we define k = kuvz-1 and let kuvz start from 2
! top layer cannot be used for convection because p at top of this layer is
! not given


!     phconv(1) = psconv
! Emanuel subroutine needs pressure in hPa, therefore convert all pressures       
      do kuvz = 2,nuvz
        k = kuvz-1
!       pconv(k) = (akz(kuvz) + bkz(kuvz)*psconv)
!       phconv(kuvz) = (akm(kuvz) + bkm(kuvz)*psconv)
        dpr(k) = phconv(k) - phconv(kuvz)
        qsconv(k) = f_qvsat( pconv(k), tconv(k) )

! initialize mass fractions 
        do kk=1,nconvlev
          fmassfrac(k,kk)=0.
        enddo
      enddo


!     note that Emanuel says it is important
!     a. to set this =0. every grid point
!     b. to keep this value in the calling programme in the iteration

! CALL CONVECTION
!******************

        cbmfold = cbmf
! Convert pressures to hPa, as required by Emanuel scheme
!*********************************************************
        do k=1,nconvlev+1
          pconv_hpa(k)=pconv(k)/100.
        phconv_hpa(k)=phconv(k)/100.
         enddo
        pconv_hpa(nconvlev+1)=pconv(nconvlev+1)/100.
        phconv_hpa(nconvlev+1)=phconv(nconvlev+1)/100.
        call convect(nconvlevmax, nconvlev, delt, iflag, &
                  precip, wd, tprime, qprime, cbmf)

!      do not update fmassfrac and cloudbase massflux
!      if no convection takes place or
!      if a CFL criterion is violated in convect43c.f
       if (iflag .ne. 1 .and. iflag .ne. 4) then
         cbmf=cbmfold
         goto 200
       endif

!      do not update fmassfrac and cloudbase massflux
!      if the old and the new cloud base mass
!      fluxes are zero
       if (cbmf.le.0..and.cbmfold.le.0.) then
         cbmf=cbmfold
         goto 200
       endif

!      Update fmassfrac
!      account for mass displaced from level k to level k

   lconv = .true.
    do k=1,nconvtop
      rlevmass = dpr(k)/ga
      summe = 0.
      do kk=1,nconvtop
        fmassfrac(k,kk) = delt*fmass(k,kk)
        summe = summe + fmassfrac(k,kk)
      end do
      fmassfrac(k,k)=fmassfrac(k,k) + rlevmass - summe
    end do

200   continue

end subroutine calcmatrix