source: trunk/LMDZ.PLUTO/libf/phypluto/sfluxv_pluto_mod.F @ 3917

      module sfluxv_pluto_mod

      implicit none

      contains

      SUBROUTINE SFLUXV_PLUTO(DTAUV,TAUV,TAUCUMV,RSFV,DWNV,WBARV,COSBV,
     *                UBAR0,STEL,NFLUXTOPV,NFLUXTOPV_nu,
     *                FMNETV,fmnetv_nu,FLUXUPV,FLUXDNV,FZEROV,taugsurf)

      use radinc_h, only: L_TAUMAX, L_LEVELS, L_NSPECTV, L_NGAUSS
      use radinc_h, only: L_NLAYRAD, L_NLEVRAD
      use radcommon_h, only: tlimit, gweight
      use gfluxv_mod, only: gfluxv

      implicit none

      real*8 FMNETV(L_NLAYRAD)
      real*8 FMNETV_NU(L_NLAYRAD,L_NSPECTV)
      real*8 TAUCUMV(L_LEVELS,L_NSPECTV,L_NGAUSS)
      real*8 TAUV(L_NLEVRAD,L_NSPECTV,L_NGAUSS)
      real*8 DTAUV(L_NLAYRAD,L_NSPECTV,L_NGAUSS), DWNV(L_NSPECTV)
      real*8 FMUPV(L_NLAYRAD), FMDV(L_NLAYRAD)
      real*8 COSBV(L_NLAYRAD,L_NSPECTV,L_NGAUSS)
      real*8 WBARV(L_NLAYRAD,L_NSPECTV,L_NGAUSS)
      real*8 STEL(L_NSPECTV)
      real*8 FLUXUPV(L_NLAYRAD), FLUXDNV(L_NLAYRAD)
      real*8 NFLUXTOPV, FLUXUP, FLUXDN
      real*8 NFLUXTOPV_nu(L_NSPECTV)


      integer L, NG, NW, NG1,k
      real*8  rsfv, ubar0, f0pi, btop, bsurf, taumax, eterm
      real*8 FZEROV(L_NSPECTV)

      real*8 DIFFV, DIFFVT

      real*8 taugsurf(L_NSPECTV,L_NGAUSS-1), fzero

C======================================================================C

      TAUMAX = L_TAUMAX

C     ZERO THE NET FLUXES

      NFLUXTOPV = 0.0


      DO L=1,L_NLAYRAD
        FMNETV(L)  = 0.0
        FLUXUPV(L) = 0.0
        FLUXDNV(L) = 0.0
      END DO
      DO NW=1,L_NSPECTV
        NFLUXTOPV_nu(nw) = 0.
        DO L=1,L_NLAYRAD
           FMNETV_nu(L,NW)  = 0.0
        END DO
      END DO


      DIFFVT = 0.0

C     WE NOW ENTER A MAJOR LOOP OVER SPECTRAL INTERVALS IN THE VISIBLE
C     TO CALCULATE THE NET FLUX IN EACH SPECTRAL INTERVAL

      DO 500 NW=1,L_NSPECTV

        F0PI = STEL(NW)


        FZERO = FZEROV(NW)
        IF(FZERO.ge.0.99) goto 40
        DO NG=1,L_NGAUSS-1

          if(TAUGSURF(NW,NG) .lt. TLIMIT) then

            fzero = fzero + (1.0-FZEROV(NW))*GWEIGHT(NG)

            goto 30
          end if

C         SET UP THE UPPER AND LOWER BOUNDARY CONDITIONS ON THE VISIBLE

          BTOP = 0.0

C         LOOP OVER THE NTERMS BEGINNING HERE

          ETERM = MIN(TAUV(L_NLEVRAD,NW,NG),TAUMAX)
          BSURF = RSFV*UBAR0*STEL(NW)*EXP(-ETERM/UBAR0)


C         WE CAN NOW SOLVE FOR THE COEFFICIENTS OF THE TWO STREAM
C         CALL A SUBROUTINE THAT SOLVES  FOR THE FLUX TERMS
C         WITHIN EACH INTERVAL AT THE MIDPOINT WAVENUMBER
C
C         FUW AND FDW ARE WORKING FLUX ARRAYS THAT WILL BE USED TO
C         RETURN FLUXES FOR A GIVEN NT



          CALL GFLUXV(DTAUV(1,NW,NG),TAUV(1,NW,NG),TAUCUMV(1,NW,NG),
     *                WBARV(1,NW,NG),COSBV(1,NW,NG),UBAR0,F0PI,RSFV,
     *                BTOP,BSURF,FMUPV,FMDV,DIFFV,FLUXUP,FLUXDN)


C         NOW CALCULATE THE CUMULATIVE VISIBLE NET FLUX

          NFLUXTOPV = NFLUXTOPV+(FLUXUP-FLUXDN)*GWEIGHT(NG)*
     *                          (1.0-FZEROV(NW))
          DO L=1,L_NLAYRAD
            FMNETV(L)=FMNETV(L)+( FMUPV(L)-FMDV(L) )*
     *                           GWEIGHT(NG)*(1.0-FZEROV(NW))
            FMNETV_nu(L,NW)=FMNETV_nu(L,NW)+( FMUPV(L)-FMDV(L) )*
     *                           GWEIGHT(NG)*(1.0-FZEROV(NW))
            FLUXUPV(L) = FLUXUPV(L) + FMUPV(L)*GWEIGHT(NG)*
     *                   (1.0-FZEROV(NW))
            FLUXDNV(L) = FLUXDNV(L) + FMDV(L)*GWEIGHT(NG)*
     *                   (1.0-FZEROV(NW))
          END DO

c         and same thing by spectral band... (RDW)
          NFLUXTOPV_nu(NW) = NFLUXTOPV_nu(NW)
     *      +(FLUXUP-FLUXDN)*GWEIGHT(NG)*
     *                          (1.0-FZEROV(NW))

C         THE DIFFUSE COMPONENT OF THE DOWNWARD STELLAR FLUX

          DIFFVT = DIFFVT + DIFFV*GWEIGHT(NG)*(1.0-FZEROV(NW))

   30     CONTINUE

        END DO   ! the Gauss loop

   40   continue
C       Special 17th Gauss point

        NG = L_NGAUSS

C       SET UP THE UPPER AND LOWER BOUNDARY CONDITIONS ON THE VISIBLE

        BTOP = 0.0

C       LOOP OVER THE NTERMS BEGINNING HERE

        ETERM = MIN(TAUV(L_NLEVRAD,NW,NG),TAUMAX)
        BSURF = RSFV*UBAR0*STEL(NW)*EXP(-ETERM/UBAR0)


C       WE CAN NOW SOLVE FOR THE COEFFICIENTS OF THE TWO STREAM
C       CALL A SUBROUTINE THAT SOLVES  FOR THE FLUX TERMS
C       WITHIN EACH INTERVAL AT THE MIDPOINT WAVENUMBER
C
C       FUW AND FDW ARE WORKING FLUX ARRAYS THAT WILL BE USED TO
C       RETURN FLUXES FOR A GIVEN NT

        CALL GFLUXV(DTAUV(1,NW,NG),TAUV(1,NW,NG),TAUCUMV(1,NW,NG),
     *              WBARV(1,NW,NG),COSBV(1,NW,NG),UBAR0,F0PI,RSFV,
     *              BTOP,BSURF,FMUPV,FMDV,DIFFV,FLUXUP,FLUXDN)


C       NOW CALCULATE THE CUMULATIVE VISIBLE NET FLUX




        NFLUXTOPV = NFLUXTOPV+(FLUXUP-FLUXDN)*FZERO
        DO L=1,L_NLAYRAD
          FMNETV(L)=FMNETV(L)+( FMUPV(L)-FMDV(L) )*FZERO
          FMNETV_nu(L,NW)=FMNETV_nu(L,NW)+( FMUPV(L)-FMDV(L) )*FZERO
          FLUXUPV(L) = FLUXUPV(L) + FMUPV(L)*FZERO
          FLUXDNV(L) = FLUXDNV(L) + FMDV(L)*FZERO
        END DO

c         and same thing by spectral band... (RDW)
          NFLUXTOPV_nu(NW) = NFLUXTOPV_nu(NW)
     *      +(FLUXUP-FLUXDN)*FZERO


C       THE DIFFUSE COMPONENT OF THE DOWNWARD STELLAR FLUX

        DIFFVT = DIFFVT + DIFFV*FZERO


  500 CONTINUE

C     *** END OF MAJOR SPECTRAL INTERVAL LOOP IN THE VISIBLE*****


      END SUBROUTINE SFLUXV_PLUTO

      end module sfluxv_pluto_mod