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+*Add halo_size argument to wave_speeds
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  Replace the optional full_halos logical argument to wave_speed and wave_speeds
with an optional halo_size integer argument, following the pattern used
elsewhere in the MOM6 code, with a similar change to itidal_lowmode_loss.  This
halo_size argument is used in the call to thickness_to_dz in wave_speeds, and
the call to wave_speeds in propagate_int_tides was modified accordingly.  In
addition, the loop bounds in the MOM_internal_tides code were modified to avoid
excessive calculations over the full data domain, some of which would use
uninitialized variables.  This commit changes the interfaces publicly visible
routines and it changes answers in cases when the internal_tides are used by
doing calculations of the wave speeds in halo points that are used in that code.
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Hallberg-NOAA committed Sep 28, 2023
1 parent c24be1c commit 13c54a5
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38 changes: 20 additions & 18 deletions src/diagnostics/MOM_wave_speed.F90
Original file line number Diff line number Diff line change
Expand Up @@ -63,7 +63,7 @@ module MOM_wave_speed
contains

!> Calculates the wave speed of the first baroclinic mode.
subroutine wave_speed(h, tv, G, GV, US, cg1, CS, full_halos, use_ebt_mode, mono_N2_column_fraction, &
subroutine wave_speed(h, tv, G, GV, US, cg1, CS, halo_size, use_ebt_mode, mono_N2_column_fraction, &
mono_N2_depth, modal_structure)
type(ocean_grid_type), intent(in) :: G !< Ocean grid structure
type(verticalGrid_type), intent(in) :: GV !< Vertical grid structure
Expand All @@ -73,8 +73,8 @@ subroutine wave_speed(h, tv, G, GV, US, cg1, CS, full_halos, use_ebt_mode, mono_
type(thermo_var_ptrs), intent(in) :: tv !< Thermodynamic variables
real, dimension(SZI_(G),SZJ_(G)), intent(out) :: cg1 !< First mode internal wave speed [L T-1 ~> m s-1]
type(wave_speed_CS), intent(in) :: CS !< Wave speed control struct
logical, optional, intent(in) :: full_halos !< If true, do the calculation
!! over the entire computational domain.
integer, optional, intent(in) :: halo_size !< Width of halo within which to
!! calculate wave speeds
logical, optional, intent(in) :: use_ebt_mode !< If true, use the equivalent
!! barotropic mode instead of the first baroclinic mode.
real, optional, intent(in) :: mono_N2_column_fraction !< The lower fraction
Expand Down Expand Up @@ -158,7 +158,7 @@ subroutine wave_speed(h, tv, G, GV, US, cg1, CS, full_halos, use_ebt_mode, mono_
logical :: better_est ! If true, use an improved estimate of the first mode internal wave speed.
logical :: merge ! If true, merge the current layer with the one above.
integer :: kc ! The number of layers in the column after merging
integer :: i, j, k, k2, itt, is, ie, js, je, nz
integer :: i, j, k, k2, itt, is, ie, js, je, nz, halo
real :: hw ! The mean of the adjacent layer thicknesses [H ~> m or kg m-2]
real :: sum_hc ! The sum of the layer thicknesses [H ~> m or kg m-2]
real :: gp ! A limited local copy of gprime [L2 H-1 T-2 ~> m s-2 or m4 s-1 kg-1]
Expand All @@ -173,14 +173,15 @@ subroutine wave_speed(h, tv, G, GV, US, cg1, CS, full_halos, use_ebt_mode, mono_
real :: ms_min, ms_max ! The minimum and maximum mode structure values returned from tdma6 [L2 T-2 ~> m2 s-2]
real :: ms_sq ! The sum of the square of the values returned from tdma6 [L4 T-4 ~> m4 s-4]

is = G%isc ; ie = G%iec ; js = G%jsc ; je = G%jec ; nz = GV%ke
is = G%isc ; ie = G%iec ; js = G%jsc ; je = G%jec ; nz = GV%ke ; halo = 0

if (.not. CS%initialized) call MOM_error(FATAL, "MOM_wave_speed / wave_speed: "// &
"Module must be initialized before it is used.")

if (present(full_halos)) then ; if (full_halos) then
is = G%isd ; ie = G%ied ; js = G%jsd ; je = G%jed
endif ; endif
if (present(halo_size)) then
halo = halo_size
is = G%isc - halo ; ie = G%iec + halo ; js = G%jsc - halo ; je = G%jec + halo
endif

l_use_ebt_mode = CS%use_ebt_mode
if (present(use_ebt_mode)) l_use_ebt_mode = use_ebt_mode
Expand Down Expand Up @@ -747,7 +748,7 @@ end subroutine tdma6

!> Calculates the wave speeds for the first few barolinic modes.
subroutine wave_speeds(h, tv, G, GV, US, nmodes, cn, CS, w_struct, u_struct, u_struct_max, u_struct_bot, Nb, int_w2, &
int_U2, int_N2w2, full_halos)
int_U2, int_N2w2, halo_size)
type(ocean_grid_type), intent(in) :: G !< Ocean grid structure
type(verticalGrid_type), intent(in) :: GV !< Vertical grid structure
type(unit_scale_type), intent(in) :: US !< A dimensional unit scaling type
Expand All @@ -772,8 +773,8 @@ subroutine wave_speeds(h, tv, G, GV, US, nmodes, cn, CS, w_struct, u_struct, u_s
real, dimension(SZI_(G),SZJ_(G),nmodes), intent(out) :: int_N2w2 !< depth-integrated buoyancy frequency
!! times vertical velocity profile
!! squared [H T-2 ~> m s-2 or kg m-2 s-2]
logical, optional, intent(in) :: full_halos !< If true, do the calculation
!! over the entire data domain.
integer, optional, intent(in) :: halo_size !< Width of halo within which to
!! calculate wave speeds

! Local variables
real, dimension(SZK_(GV)+1) :: &
Expand Down Expand Up @@ -872,7 +873,7 @@ subroutine wave_speeds(h, tv, G, GV, US, nmodes, cn, CS, w_struct, u_struct, u_s
logical :: sub_rootfound ! if true, subdivision has located root
integer :: kc ! The number of layers in the column after merging
integer :: sub, sub_it
integer :: i, j, k, k2, itt, is, ie, js, je, nz, iint, m
integer :: i, j, k, k2, itt, is, ie, js, je, nz, iint, m, halo
real, dimension(SZK_(GV)+1) :: modal_structure !< Normalized model structure [nondim]
real, dimension(SZK_(GV)) :: modal_structure_fder !< Normalized model structure [Z-1 ~> m-1]
real :: mode_struct(SZK_(GV)+1) ! The mode structure [nondim], but it is also temporarily
Expand All @@ -889,14 +890,15 @@ subroutine wave_speeds(h, tv, G, GV, US, nmodes, cn, CS, w_struct, u_struct, u_s
real, parameter :: a_int = 0.5 ! Integral total for normalization [nondim]
real :: renorm ! Normalization factor [T2 L-2 ~> s2 m-2]

is = G%isc ; ie = G%iec ; js = G%jsc ; je = G%jec ; nz = GV%ke
is = G%isc ; ie = G%iec ; js = G%jsc ; je = G%jec ; nz = GV%ke ; halo = 0

if (.not. CS%initialized) call MOM_error(FATAL, "MOM_wave_speed / wave_speeds: "// &
"Module must be initialized before it is used.")

if (present(full_halos)) then ; if (full_halos) then
is = G%isd ; ie = G%ied ; js = G%jsd ; je = G%jed
endif ; endif
if (present(halo_size)) then
halo = halo_size
is = G%isc - halo ; ie = G%iec + halo ; js = G%jsc - halo ; je = G%jec + halo
endif

g_Rho0 = GV%g_Earth * GV%H_to_Z / GV%Rho0
H_to_pres = GV%H_to_RZ * GV%g_Earth
Expand Down Expand Up @@ -940,7 +942,7 @@ subroutine wave_speeds(h, tv, G, GV, US, nmodes, cn, CS, w_struct, u_struct, u_s
do i=is,ie ; htot(i) = 0.0 ; enddo
do k=1,nz ; do i=is,ie ; htot(i) = htot(i) + h(i,j,k) ; enddo ; enddo

call thickness_to_dz(h, tv, dz_2d, j, G, GV)
call thickness_to_dz(h, tv, dz_2d, j, G, GV, halo_size=halo)

do i=is,ie
hmin(i) = htot(i)*min_h_frac ; kf(i) = 1 ; H_here(i) = 0.0 ; dz_here(i) = 0.0
Expand Down Expand Up @@ -1097,7 +1099,7 @@ subroutine wave_speeds(h, tv, G, GV, US, nmodes, cn, CS, w_struct, u_struct, u_s
! Merge layers to eliminate convective instabilities or exceedingly
! small reduced gravities. Merging layers reduces the estimated wave speed by
! (rho(2)-rho(1))*h(1)*h(2) / H_tot.
if (use_EOS .and. (.not.nonBous)) then
if (use_EOS) then
kc = 1
Hc(1) = Hf(1,i) ; dzc(1) = dzf(1,i) ; Tc(1) = Tf(1,i) ; Sc(1) = Sf(1,i)
do k=2,kf(i)
Expand Down
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