SUBROUTINE lmd_swfrac_tile (ng, tile,                             &
     &                            LBi, UBi, LBj, UBj,                   &
     &                            IminS, ImaxS, JminS, JmaxS,           &
     &                            Zscale, Z, swdk)
!
!git $Id$
!svn $Id: lmd_swfrac.F 1151 2023-02-09 03:08:53Z arango $
!================================================== Hernan G. Arango ===
!  Copyright (c) 2002-2023 The ROMS/TOMS Group                         !
!    Licensed under a MIT/X style license                              !
!    See License_ROMS.md                                               !
!=======================================================================
!                                                                      !
!  This subroutine computes the  fraction  of  solar shortwave flux    !
!  penetrating to specified depth (times Zscale) due to exponential    !
!  decay in Jerlov water type.                                         !
!                                                                      !
!  On Input:                                                           !
!                                                                      !
!     Zscale   scale factor to apply to depth array.                   !
!     Z        vertical height (meters, negative) for                  !
!              desired solar short-wave fraction.                      !
!                                                                      !
!  On Output:                                                          !
!                                                                      !
!     swdk     shortwave (radiation) fractional decay.                 !
!                                                                      !
!  Reference:                                                          !
!                                                                      !
!  Paulson, C.A., and J.J. Simpson, 1977: Irradiance meassurements     !
!     in the upper ocean, J. Phys. Oceanogr., 7, 952-956.              !
!                                                                      !
!  This routine was adapted from Bill Large 1995 code.                 !
!                                                                      !
!=======================================================================
!
      USE mod_param
      USE mod_mixing
      USE mod_scalars
!
      implicit none
!
!  Imported variable declarations.
!
      integer, intent(in) :: ng, tile
      integer, intent(in) :: LBi, UBi, LBj, UBj
      integer, intent(in) :: IminS, ImaxS, JminS, JmaxS
      real(r8), intent(in) :: Zscale
      real(r8), intent(in) :: Z(IminS:ImaxS,JminS:JmaxS)
      real(r8), intent(out) :: swdk(IminS:ImaxS,JminS:JmaxS)
!
!  Local variable declarations.
!
      integer :: Jindex, i, j
      real(r8), dimension(IminS:ImaxS) :: fac1, fac2, fac3
!
!-----------------------------------------------------------------------
!  Set lower and upper tile bounds and staggered variables bounds for
!  this horizontal domain partition.  Notice that if tile=-1, it will
!  set the values for the global grid.
!-----------------------------------------------------------------------
!
      integer :: Istr, IstrB, IstrP, IstrR, IstrT, IstrM, IstrU
      integer :: Iend, IendB, IendP, IendR, IendT
      integer :: Jstr, JstrB, JstrP, JstrR, JstrT, JstrM, JstrV
      integer :: Jend, JendB, JendP, JendR, JendT
      integer :: Istrm3, Istrm2, Istrm1, IstrUm2, IstrUm1
      integer :: Iendp1, Iendp2, Iendp2i, Iendp3
      integer :: Jstrm3, Jstrm2, Jstrm1, JstrVm2, JstrVm1
      integer :: Jendp1, Jendp2, Jendp2i, Jendp3
!
      Istr   =BOUNDS(ng) % Istr   (tile)
      IstrB  =BOUNDS(ng) % IstrB  (tile)
      IstrM  =BOUNDS(ng) % IstrM  (tile)
      IstrP  =BOUNDS(ng) % IstrP  (tile)
      IstrR  =BOUNDS(ng) % IstrR  (tile)
      IstrT  =BOUNDS(ng) % IstrT  (tile)
      IstrU  =BOUNDS(ng) % IstrU  (tile)
      Iend   =BOUNDS(ng) % Iend   (tile)
      IendB  =BOUNDS(ng) % IendB  (tile)
      IendP  =BOUNDS(ng) % IendP  (tile)
      IendR  =BOUNDS(ng) % IendR  (tile)
      IendT  =BOUNDS(ng) % IendT  (tile)
      Jstr   =BOUNDS(ng) % Jstr   (tile)
      JstrB  =BOUNDS(ng) % JstrB  (tile)
      JstrM  =BOUNDS(ng) % JstrM  (tile)
      JstrP  =BOUNDS(ng) % JstrP  (tile)
      JstrR  =BOUNDS(ng) % JstrR  (tile)
      JstrT  =BOUNDS(ng) % JstrT  (tile)
      JstrV  =BOUNDS(ng) % JstrV  (tile)
      Jend   =BOUNDS(ng) % Jend   (tile)
      JendB  =BOUNDS(ng) % JendB  (tile)
      JendP  =BOUNDS(ng) % JendP  (tile)
      JendR  =BOUNDS(ng) % JendR  (tile)
      JendT  =BOUNDS(ng) % JendT  (tile)
!
      Istrm3 =BOUNDS(ng) % Istrm3 (tile)            ! Istr-3
      Istrm2 =BOUNDS(ng) % Istrm2 (tile)            ! Istr-2
      Istrm1 =BOUNDS(ng) % Istrm1 (tile)            ! Istr-1
      IstrUm2=BOUNDS(ng) % IstrUm2(tile)            ! IstrU-2
      IstrUm1=BOUNDS(ng) % IstrUm1(tile)            ! IstrU-1
      Iendp1 =BOUNDS(ng) % Iendp1 (tile)            ! Iend+1
      Iendp2 =BOUNDS(ng) % Iendp2 (tile)            ! Iend+2
      Iendp2i=BOUNDS(ng) % Iendp2i(tile)            ! Iend+2 interior
      Iendp3 =BOUNDS(ng) % Iendp3 (tile)            ! Iend+3
      Jstrm3 =BOUNDS(ng) % Jstrm3 (tile)            ! Jstr-3
      Jstrm2 =BOUNDS(ng) % Jstrm2 (tile)            ! Jstr-2
      Jstrm1 =BOUNDS(ng) % Jstrm1 (tile)            ! Jstr-1
      JstrVm2=BOUNDS(ng) % JstrVm2(tile)            ! JstrV-2
      JstrVm1=BOUNDS(ng) % JstrVm1(tile)            ! JstrV-1
      Jendp1 =BOUNDS(ng) % Jendp1 (tile)            ! Jend+1
      Jendp2 =BOUNDS(ng) % Jendp2 (tile)            ! Jend+2
      Jendp2i=BOUNDS(ng) % Jendp2i(tile)            ! Jend+2 interior
      Jendp3 =BOUNDS(ng) % Jendp3 (tile)            ! Jend+3
!
!-----------------------------------------------------------------------
!  Use Paulson and Simpson (1977) two wavelength bands solar
!  absorption model.
!-----------------------------------------------------------------------
!
      DO j=Jstr,Jend
        DO i=Istr,Iend
          Jindex=INT(MIXING(ng)%Jwtype(i,j))
          fac1(i)=Zscale/lmd_mu1(Jindex)
          fac2(i)=Zscale/lmd_mu2(Jindex)
          fac3(i)=lmd_r1(Jindex)
        END DO
        DO i=Istr,Iend
          swdk(i,j)=EXP(Z(i,j)*fac1(i))*fac3(i)+                        &
     &              EXP(Z(i,j)*fac2(i))*(1.0_r8-fac3(i))
        END DO
      END DO
      RETURN
      END SUBROUTINE lmd_swfrac_tile