forcing-perturbation/interpolation/rotateUVorca_sources/geo2ocean.f90

MODULE geo2ocean
   !!======================================================================
   !!                     ***  MODULE  geo2ocean  ***
   !! Ocean mesh    :  ???
   !!======================================================================
   !! History :  OPA  !  07-1996  (O. Marti)  Original code
   !!   NEMO     1.0  !  02-2008  (G. Madec)  F90: Free form
   !!            3.0  !  
   !!----------------------------------------------------------------------

   !!----------------------------------------------------------------------
   !!   repcmo      : 
   !!   angle       :
   !!   geo2oce     :
   !!----------------------------------------------------------------------
   USE dom_oce         ! mesh and scale factors
   USE phycst          ! physical constants
   USE par_kind        ! precision 
   USE lbclnk
   IMPLICIT NONE
   PRIVATE

   PUBLIC   rot_rep

   REAL(wp), DIMENSION(jpi,jpj) ::   &
      gsint, gcost,   &  ! cos/sin between model grid lines and NP direction at T point
      gsinu, gcosu,   &  ! cos/sin between model grid lines and NP direction at U point
      gsinv, gcosv,   &  ! cos/sin between model grid lines and NP direction at V point
      gsinf, gcosf       ! cos/sin between model grid lines and NP direction at F point

   LOGICAL ::   lmust_init = .TRUE.        !: used to initialize the cos/sin variables (se above)

   !! * Substitutions
   !!----------------------------------------------------------------------
   !! NEMO/OPA 3.0 , LOCEAN-IPSL (2008) 
   !! $Id: geo2ocean.F90 1833 2010-04-13 17:44:52Z smasson $ 
   !! Software governed by the CeCILL licence (modipsl/doc/NEMO_CeCILL.txt)
   !!----------------------------------------------------------------------

CONTAINS


   SUBROUTINE rot_rep ( pxin, pyin, cd_type, cdtodo, prot )
      !!----------------------------------------------------------------------
      !!                  ***  ROUTINE rot_rep  ***
      !!
      !! ** Purpose :   Rotate the Repere: Change vector componantes between
      !!                geographic grid <--> stretched coordinates grid.
      !!
      !! History :
      !!   9.2  !  07-04  (S. Masson)  
      !!                  (O. Marti ) Original code (repere and repcmo)
      !!----------------------------------------------------------------------
      REAL(wp), DIMENSION(jpi,jpj), INTENT( IN ) ::   pxin, pyin   ! vector componantes
      CHARACTER(len=1),             INTENT( IN ) ::   cd_type      ! define the nature of pt2d array grid-points
      CHARACTER(len=5),             INTENT( IN ) ::   cdtodo       ! specify the work to do:
      !!                                                           ! 'en->i' east-north componantes to model i componante
      !!                                                           ! 'en->j' east-north componantes to model j componante
      !!                                                           ! 'ij->e' model i-j componantes to east componante
      !!                                                           ! 'ij->n' model i-j componantes to east componante
      REAL(wp), DIMENSION(jpi,jpj), INTENT(out) ::   prot      

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

      ! Initialization of gsin* and gcos* at first call
      ! -----------------------------------------------

      IF( lmust_init ) THEN

         CALL angle       ! initialization of the transformation
         lmust_init = .FALSE.

      ENDIF 
      
      SELECT CASE (cdtodo)
      CASE ('en->i')      ! 'en->i' est-north componantes to model i componante
         SELECT CASE (cd_type)
         CASE ('T')   ;   prot(:,:) = pxin(:,:) * gcost(:,:) + pyin(:,:) * gsint(:,:)
         CASE ('U')   ;   prot(:,:) = pxin(:,:) * gcosu(:,:) + pyin(:,:) * gsinu(:,:)
         CASE ('V')   ;   prot(:,:) = pxin(:,:) * gcosv(:,:) + pyin(:,:) * gsinv(:,:)
         CASE ('F')   ;   prot(:,:) = pxin(:,:) * gcosf(:,:) + pyin(:,:) * gsinf(:,:)
         CASE DEFAULT   ;   STOP 'Only T, U, V and F grid points are coded' 
         END SELECT
      CASE ('en->j')      ! 'en->j' est-north componantes to model j componante
         SELECT CASE (cd_type)
         CASE ('T')   ;   prot(:,:) = pyin(:,:) * gcost(:,:) - pxin(:,:) * gsint(:,:)
         CASE ('U')   ;   prot(:,:) = pyin(:,:) * gcosu(:,:) - pxin(:,:) * gsinu(:,:)
         CASE ('V')   ;   prot(:,:) = pyin(:,:) * gcosv(:,:) - pxin(:,:) * gsinv(:,:)   
         CASE ('F')   ;   prot(:,:) = pyin(:,:) * gcosf(:,:) - pxin(:,:) * gsinf(:,:)   
         CASE DEFAULT   ;   STOP 'Only T, U, V and F grid points are coded'
         END SELECT
      CASE ('ij->e')      ! 'ij->e' model i-j componantes to est componante
         SELECT CASE (cd_type)
         CASE ('T')   ;   prot(:,:) = pxin(:,:) * gcost(:,:) - pyin(:,:) * gsint(:,:)
         CASE ('U')   ;   prot(:,:) = pxin(:,:) * gcosu(:,:) - pyin(:,:) * gsinu(:,:)
         CASE ('V')   ;   prot(:,:) = pxin(:,:) * gcosv(:,:) - pyin(:,:) * gsinv(:,:)
         CASE ('F')   ;   prot(:,:) = pxin(:,:) * gcosf(:,:) - pyin(:,:) * gsinf(:,:)
         CASE DEFAULT   ;   STOP 'Only T, U, V and F grid points are coded' 
         END SELECT
      CASE ('ij->n')      ! 'ij->n' model i-j componantes to est componante
         SELECT CASE (cd_type)
         CASE ('T')   ;   prot(:,:) = pyin(:,:) * gcost(:,:) + pxin(:,:) * gsint(:,:)
         CASE ('U')   ;   prot(:,:) = pyin(:,:) * gcosu(:,:) + pxin(:,:) * gsinu(:,:)
         CASE ('V')   ;   prot(:,:) = pyin(:,:) * gcosv(:,:) + pxin(:,:) * gsinv(:,:)
         CASE ('F')   ;   prot(:,:) = pyin(:,:) * gcosf(:,:) + pxin(:,:) * gsinf(:,:)
         CASE DEFAULT   ;   STOP 'Only T, U, V and F grid points are coded' 
         END SELECT
      CASE DEFAULT   ;   STOP 'rot_rep: Syntax Error in the definition of cdtodo' 
      END SELECT
      
   END SUBROUTINE rot_rep


   SUBROUTINE angle
      !!----------------------------------------------------------------------
      !!                  ***  ROUTINE angle  ***
      !! 
      !! ** Purpose :   Compute angles between model grid lines and the North direction
      !!
      !! ** Method  :
      !!
      !! ** Action  :   Compute (gsint, gcost, gsinu, gcosu, gsinv, gcosv, gsinf, gcosf) arrays:
      !!      sinus and cosinus of the angle between the north-south axe and the 
      !!      j-direction at t, u, v and f-points
      !!
      !! History :
      !!   7.0  !  96-07  (O. Marti )  Original code
      !!   8.0  !  98-06  (G. Madec )
      !!   8.5  !  98-06  (G. Madec )  Free form, F90 + opt.
      !!   9.2  !  07-04  (S. Masson)  Add T, F points and bugfix in cos lateral boundary
      !!----------------------------------------------------------------------
      INTEGER ::   ji, jj      ! dummy loop indices
      !!
      REAL(wp) ::   &
         zlam, zphi,            &  ! temporary scalars
         zlan, zphh,            &  !    "         "
         zxnpt, zynpt, znnpt,   &  ! x,y components and norm of the vector: T point to North Pole
         zxnpu, zynpu, znnpu,   &  ! x,y components and norm of the vector: U point to North Pole
         zxnpv, zynpv, znnpv,   &  ! x,y components and norm of the vector: V point to North Pole
         zxnpf, zynpf, znnpf,   &  ! x,y components and norm of the vector: F point to North Pole
         zxvvt, zyvvt, znvvt,   &  ! x,y components and norm of the vector: between V points below and above a T point
         zxffu, zyffu, znffu,   &  ! x,y components and norm of the vector: between F points below and above a U point
         zxffv, zyffv, znffv,   &  ! x,y components and norm of the vector: between F points left  and right a V point
         zxuuf, zyuuf, znuuf       ! x,y components and norm of the vector: between U points below and above a F point
      !!----------------------------------------------------------------------

      ! ============================= !
      ! Compute the cosinus and sinus !
      ! ============================= !
      ! (computation done on the north stereographic polar plane)
      
      DO jj = 2, (jpj-1)
!CDIR NOVERRCHK
         DO ji = 2, jpi   ! vector opt.

            ! north pole direction & modulous (at t-point)
            zlam = glamt(ji,jj)
            zphi = gphit(ji,jj)
            zxnpt = 0. - 2. * COS( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )
            zynpt = 0. - 2. * SIN( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )
            znnpt = zxnpt*zxnpt + zynpt*zynpt

            ! north pole direction & modulous (at u-point)
            zlam = glamu(ji,jj)
            zphi = gphiu(ji,jj)
            zxnpu = 0. - 2. * COS( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )
            zynpu = 0. - 2. * SIN( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )
            znnpu = zxnpu*zxnpu + zynpu*zynpu

            ! north pole direction & modulous (at v-point)
            zlam = glamv(ji,jj)
            zphi = gphiv(ji,jj)
            zxnpv = 0. - 2. * COS( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )
            zynpv = 0. - 2. * SIN( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )
            znnpv = zxnpv*zxnpv + zynpv*zynpv

            ! north pole direction & modulous (at f-point)
            zlam = glamf(ji,jj)
            zphi = gphif(ji,jj)
            zxnpf = 0. - 2. * COS( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )
            zynpf = 0. - 2. * SIN( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )
            znnpf = zxnpf*zxnpf + zynpf*zynpf

            ! j-direction: v-point segment direction (around t-point)
            zlam = glamv(ji,jj  )
            zphi = gphiv(ji,jj  )
            zlan = glamv(ji,jj-1)
            zphh = gphiv(ji,jj-1)
            zxvvt =  2. * COS( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )   &
               &  -  2. * COS( rad*zlan ) * TAN( rpi/4. - rad*zphh/2. )
            zyvvt =  2. * SIN( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )   &
               &  -  2. * SIN( rad*zlan ) * TAN( rpi/4. - rad*zphh/2. )
            znvvt = SQRT( znnpt * ( zxvvt*zxvvt + zyvvt*zyvvt )  )
            znvvt = MAX( znvvt, 1.e-14 )

            ! j-direction: f-point segment direction (around u-point)
            zlam = glamf(ji,jj  )
            zphi = gphif(ji,jj  )
            zlan = glamf(ji,jj-1)
            zphh = gphif(ji,jj-1)
            zxffu =  2. * COS( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )   &
               &  -  2. * COS( rad*zlan ) * TAN( rpi/4. - rad*zphh/2. )
            zyffu =  2. * SIN( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )   &
               &  -  2. * SIN( rad*zlan ) * TAN( rpi/4. - rad*zphh/2. )
            znffu = SQRT( znnpu * ( zxffu*zxffu + zyffu*zyffu )  )
            znffu = MAX( znffu, 1.e-14 )

            ! i-direction: f-point segment direction (around v-point)
            zlam = glamf(ji  ,jj)
            zphi = gphif(ji  ,jj)
            zlan = glamf(ji-1,jj)
            zphh = gphif(ji-1,jj)
            zxffv =  2. * COS( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )   &
               &  -  2. * COS( rad*zlan ) * TAN( rpi/4. - rad*zphh/2. )
            zyffv =  2. * SIN( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )   &
               &  -  2. * SIN( rad*zlan ) * TAN( rpi/4. - rad*zphh/2. )
            znffv = SQRT( znnpv * ( zxffv*zxffv + zyffv*zyffv )  )
            znffv = MAX( znffv, 1.e-14 )

            ! j-direction: u-point segment direction (around f-point)
            zlam = glamu(ji,jj+1)
            zphi = gphiu(ji,jj+1)
            zlan = glamu(ji,jj  )
            zphh = gphiu(ji,jj  )
            zxuuf =  2. * COS( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )   &
               &  -  2. * COS( rad*zlan ) * TAN( rpi/4. - rad*zphh/2. )
            zyuuf =  2. * SIN( rad*zlam ) * TAN( rpi/4. - rad*zphi/2. )   &
               &  -  2. * SIN( rad*zlan ) * TAN( rpi/4. - rad*zphh/2. )
            znuuf = SQRT( znnpf * ( zxuuf*zxuuf + zyuuf*zyuuf )  )
            znuuf = MAX( znuuf, 1.e-14 )

            ! cosinus and sinus using scalar and vectorial products
            gsint(ji,jj) = ( zxnpt*zyvvt - zynpt*zxvvt ) / znvvt
            gcost(ji,jj) = ( zxnpt*zxvvt + zynpt*zyvvt ) / znvvt

            gsinu(ji,jj) = ( zxnpu*zyffu - zynpu*zxffu ) / znffu
            gcosu(ji,jj) = ( zxnpu*zxffu + zynpu*zyffu ) / znffu

            gsinf(ji,jj) = ( zxnpf*zyuuf - zynpf*zxuuf ) / znuuf
            gcosf(ji,jj) = ( zxnpf*zxuuf + zynpf*zyuuf ) / znuuf

            ! (caution, rotation of 90 degres)
            gsinv(ji,jj) = ( zxnpv*zxffv + zynpv*zyffv ) / znffv
            gcosv(ji,jj) =-( zxnpv*zyffv - zynpv*zxffv ) / znffv

         END DO
      END DO

      ! =============== !
      ! Geographic mesh !
      ! =============== !

      DO jj = 2, (jpj-1)
         DO ji = 2, jpi   ! vector opt.
            IF( MOD( ABS( glamv(ji,jj) - glamv(ji,jj-1) ), 360. ) < 1.e-8 ) THEN
               gsint(ji,jj) = 0.
               gcost(ji,jj) = 1.
            ENDIF
            IF( MOD( ABS( glamf(ji,jj) - glamf(ji,jj-1) ), 360. ) < 1.e-8 ) THEN
               gsinu(ji,jj) = 0.
               gcosu(ji,jj) = 1.
            ENDIF
            IF(      ABS( gphif(ji,jj) - gphif(ji-1,jj) )         < 1.e-8 ) THEN
               gsinv(ji,jj) = 0.
               gcosv(ji,jj) = 1.
            ENDIF
            IF( MOD( ABS( glamu(ji,jj) - glamu(ji,jj+1) ), 360. ) < 1.e-8 ) THEN
               gsinf(ji,jj) = 0.
               gcosf(ji,jj) = 1.
            ENDIF
         END DO
      END DO

      ! =========================== !
      ! Lateral boundary conditions !
      ! =========================== !

      ! lateral boundary cond.: T-, U-, V-, F-pts, sgn
      CALL lbc_lnk( gcost, 'T', -1._wp )   ;   CALL lbc_lnk( gsint, 'T', -1._wp )
      CALL lbc_lnk( gcosu, 'U', -1._wp )   ;   CALL lbc_lnk( gsinu, 'U', -1._wp )
      CALL lbc_lnk( gcosv, 'V', -1._wp )   ;   CALL lbc_lnk( gsinv, 'V', -1._wp )
      CALL lbc_lnk( gcosf, 'F', -1._wp )   ;   CALL lbc_lnk( gsinf, 'F', -1._wp )

   END SUBROUTINE angle


END MODULE geo2ocean