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|
! Copyright (C) 2006 Imperial College London and others.
!
! Please see the AUTHORS file in the main source directory for a full list
! of copyright holders.
!
! Prof. C Pain
! Applied Modelling and Computation Group
! Department of Earth Science and Engineering
! Imperial College London
!
! amcgsoftware@imperial.ac.uk
!
! This library is free software; you can redistribute it and/or
! modify it under the terms of the GNU Lesser General Public
! License as published by the Free Software Foundation,
! version 2.1 of the License.
!
! This library 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
! Lesser General Public License for more details.
!
! You should have received a copy of the GNU Lesser General Public
! License along with this library; if not, write to the Free Software
! Foundation, Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307
! USA
! Note: many routines in this module were not written by the above authors.
! Where this is the case, the original authors are cited.
! All included modules conform the above licence, however.
#include "fdebug.h"
module bulk_parameterisations
use boundary_conditions
use fldebug
use quadrature
use elements
use fields
use field_options
use state_module
use spud
use global_parameters, only: OPTION_PATH_LEN
implicit none
private
public :: ncar_forcing, coare_forcing, kara_forcing
public :: bulk_parameterisations_check_options
public :: get_forcing_surface_element_list
! physical constants
real, parameter :: air_density = 1.22,&
vapour_latent = 2.5e6, &
air_specificHeat = 1000.5, &
alpha = 0.066, &
sb = 5.67e-8, &
fusion_latent = 3.337e5, &
q1 = 0.98*640380, &
q2 = -5107.4, &
ocean_density = 1027.0, &
OneOverDensity = 1.0 / ocean_density, &
ocean_heat_capacity = 4000.0, &
kelvin_centrigrade = 273.15, &
heat_convert = 1.0 / (ocean_density * ocean_heat_capacity), &
one_over_density = 1.0 / ocean_density
contains
!------------------------------------------------------------------------------
! These are the public routines. They take the following inputs:
! - points
! - speed
! - air_temp
! - sst
! - spec_humidity
! - sea_surface_humidity
! - U
! - V
! - ppt
! - runoff
! - salinity
!
! And output the following:
!
! - Q_solar
! - Q
! - F
! - tau_u
! - tau_v
!
! These outputs are for each node on the surface. See
! Boundary_conditions_from_options.F90 for how these are added to the mesh.
!------------------------------------------------------------------------------
! Wrapper around routine of Large and Yeager (2004),
! Turns the coefficients from the routine into fluxes
subroutine ncar_forcing(points, speed, air_temp, sst, spec_humidity, &
sea_surface_humidity, U, V, ppt, runoff, salinity, &
thermal, solar, Q_solar, Q, F, tau_u, tau_v)
implicit none
integer, intent(in) :: points
real, intent(in), dimension(points) :: speed, air_temp, sst, spec_humidity, sea_surface_humidity
real, intent(in), dimension(points) :: U, V, ppt, runoff, salinity, solar, thermal
real, intent(out), dimension(points) :: Q_solar, Q ! heat fluxes
real, intent(out), dimension(points) :: F ! Freshwater flux
real, intent(out), dimension(points) :: tau_u, tau_v ! momentum fluxes
real, parameter :: heat_convert = 1.0 / (ocean_density * ocean_heat_capacity)
real, parameter :: one_over_density = 1.0 / ocean_density
real :: tau_temp, E
real, dimension(points) :: z, ustar, bstar, cd, ce, ch
real :: Q_long, Q_latent, Q_sensible, Q_ppt
logical*1, dimension(points) :: avail
integer :: i
z = 2.0
avail = .true.
ewrite(2,*) "In NCAR bulk parameterisations"
call ncar_ocean_fluxes(points, speed, air_temp, sst, spec_humidity, sea_surface_humidity, &
z, avail, cd, ch, ce, ustar, bstar)
do i=1,points
! from cd, ce and ch, calculate fluxes
tau_temp = OneOverDensity * air_density * cd(i) * speed(i);
tau_u(i) = tau_temp * U(i)
tau_v(i) = tau_temp * V(i)
E = air_density * ce(i) * (spec_humidity(i) - sea_surface_humidity(i)) * speed(i) ! evap
Q_solar(i) = solar(i) * (1.0-alpha)
Q_long = thermal(i) - (sb * SST(i)**4.0)
Q_latent = vapour_latent * E
Q_sensible = air_density * air_specificHeat * ch(i) * &
(air_temp(i) - sst(i)) * speed(i)
Q_ppt = -fusion_latent * ppt(i)
! E seems to be about a factor of a thousand out of the ERA40 data when using
! it for the freshwater fluxes
! Dividing by ocean density appears to give the right answer...
E = E / ocean_density
F(i) = ppt(i) + E + runoff(i)
Q(i) = heat_convert * (Q_solar(i) + Q_long + Q_latent + Q_sensible + Q_ppt)
F(i) = -1.0 * salinity(i) * F(i)
end do
end subroutine ncar_forcing
! Wrapper around routine of Large and Yeager (2004),
! Turns the coefficients from the routine into fluxes
subroutine coare_forcing(points, speed, air_temp, sst, spec_humidity, &
sea_surface_humidity, U, V, ppt, runoff, salinity, &
thermal, solar, Q_solar, Q, F, tau_u, tau_v)
implicit none
integer, intent(in) :: points
real, intent(in), dimension(points) :: speed, spec_humidity, sea_surface_humidity
real, intent(inout), dimension(points) :: sst, air_temp !Need converting to C from K, hence the inout
real, intent(in), dimension(points) :: U, V, ppt, runoff, salinity, solar, thermal
real, intent(out), dimension(points) :: Q_solar, Q ! heat fluxes
real, intent(out), dimension(points) :: F ! Freshwater flux
real, intent(out), dimension(points) :: tau_u, tau_v ! momentum fluxes
real :: tau_temp, E
real, dimension(points) :: cd, ce, ch, hf, ef, rf ! DO WE NEED HF, EF RF ?!
real :: Q_long, Q_latent, Q_sensible, Q_ppt
integer :: i, r
real :: jwave = 0
real, dimension(points) :: lat
real :: zu, zt, zq
zu = 15.
zt = 15.
zq = 15.
lat = 0.
ewrite(2,*) "In COARE bulk parameterisations"
! coare v3.0: Temperatures are in C not K
do r=1, points
sst(r) = sst(r) - kelvin_centrigrade
air_temp(r) = air_temp(r) - kelvin_centrigrade
end do
call coare30_ocean_fluxes (points, speed, sst, air_temp, sea_surface_humidity, &
solar, thermal, ppt, zu, zt, zq, jwave, &
lat, hf, ef, rf, cd, ch, ce)
do i=1,points
! from cd, ce and ch, calculate fluxes
tau_temp = OneOverDensity * air_density * cd(i) * speed(i)
tau_u(i) = tau_temp * U(i)
tau_v(i) = tau_temp * V(i)
E = air_density * ce(i) * (spec_humidity(i) - sea_surface_humidity(i)) * speed(i) ! evap
Q_solar(i) = solar(i) * (1.0-alpha)
Q_long = thermal(i) - (sb * (SST(i) + kelvin_centrigrade)**4.0)
Q_latent = vapour_latent * E
Q_sensible = air_density * air_specificHeat * ch(i) * &
(air_temp(i) - sst(i)) * speed(i)
Q_ppt = -fusion_latent * ppt(i)
! E seems to be about a factor of a thousand out of the ERA40 data when using
! it for the freshwater fluxes
! Dividing by ocean density appears to give the right answer...
E = E / ocean_density
F(i) = ppt(i) + E + runoff(i)
Q(i) = heat_convert * (Q_solar(i) + Q_long + Q_latent + Q_sensible + Q_ppt)
F(i) = -1.0 * salinity(i) * F(i)
end do
end subroutine coare_forcing
subroutine kara_forcing (points, speed, air_temp, sst, spec_humidity, &
sea_surface_humidity, U, V, ppt, runoff, salinity, &
thermal, solar, Q_solar, Q, F, tau_u, tau_v)
implicit none
integer, intent(in) :: points
real, intent(in), dimension(points) :: spec_humidity, sea_surface_humidity
real, intent(in), dimension(points) :: U, V, ppt, runoff, salinity, solar, thermal
real, intent(inout), dimension(points) :: sst, air_temp
real, intent(inout), dimension(points) :: speed ! is inout in the private routine as it gets limited
real, intent(out), dimension(points) :: Q_solar, Q ! heat fluxes
real, intent(out), dimension(points) :: F ! Freshwater flux
real, intent(out), dimension(points) :: tau_u, tau_v ! momentum fluxes
real :: tau_temp, E
real, dimension(points) :: cd, ce, ch, lhf, shf, tau_r
real :: Q_long, Q_latent, Q_sensible, Q_ppt
integer :: i, r
ewrite(2,*) "In KARA bulk parameterisations"
! kara: Temperatures are in C not K
do r=1, points
sst(r) = sst(r) - kelvin_centrigrade
air_temp(r) = air_temp(r) - kelvin_centrigrade
end do
call kara_ocean_fluxes (points, U, V, ppt, air_temp, sst, speed, lhf, shf, tau_u, tau_v, tau_r, ce, cd, ch);
do i=1,points
! from cd, ce and ch, calculate fluxes
tau_temp = OneOverDensity * air_density * cd(i) * speed(i)
tau_u(i) = tau_temp * U(i)
tau_v(i) = tau_temp * V(i)
E = air_density * ce(i) * (spec_humidity(i) - sea_surface_humidity(i)) * speed(i) ! evap
Q_solar(i) = solar(i) * (1.0-alpha)
Q_long = thermal(i) - (sb * (SST(i) + kelvin_centrigrade)**4.0)
Q_latent = vapour_latent * E
Q_sensible = air_density * air_specificHeat * ch(i) * &
(air_temp(i) - sst(i)) * speed(i)
Q_ppt = -fusion_latent * ppt(i)
! E seems to be about a factor of a thousand out of the ERA40 data when using
! it for the freshwater fluxes
! Dividing by ocean density appears to give the right answer...
E = E / ocean_density
F(i) = ppt(i) + E + runoff(i)
! Q(i) = lhf(i) + shf(i)
Q(i) = heat_convert * (Q_solar(i) + Q_long + Q_latent + Q_sensible + Q_ppt)
F(i) = -1.0 * salinity(i) * F(i)
end do
end subroutine kara_forcing
subroutine get_forcing_surface_element_list(state, surface_element_list, &
& force_temperature, force_solar, force_velocity, force_salinity)
type(state_type), intent(in) :: state
integer, dimension(:), pointer, intent(out) :: surface_element_list
! set to the BC id of the field or -1 otherwise
integer, intent(out) :: force_temperature, force_solar, force_velocity, force_salinity
type(vector_field), pointer :: vfield
type(scalar_field), pointer :: sfield
character(len=OPTION_PATH_LEN) :: field_path, bc_path, bc_type, bc_path_i
integer :: nbcs, i, stat
logical :: found_bc = .false.
! Check potential bulk_force'd fields until we come across a "bulk_formulae" type
! bc - this will give us the required info to create our mesh
! We always have a velocity field, so let's try there first
vfield => extract_vector_field(state, "Velocity")
force_velocity = -1
field_path=vfield%option_path
if (have_option(trim(field_path)//'/prognostic')) then
! Get number of boundary conditions
bc_path = trim(field_path)//'/prognostic/boundary_conditions'
nbcs=option_count(trim(bc_path))
! Loop over boundary conditions
do i=0, nbcs-1
bc_path_i=trim(bc_path)//"["//int2str(i)//"]"
call get_option(trim(bc_path_i)//"/type[0]/name", bc_type)
if (trim(bc_type) .eq. "bulk_formulae") then
found_bc = .true.
call get_boundary_condition(vfield, i+1, surface_element_list=surface_element_list)
force_velocity = i+1
end if
end do
end if
sfield => extract_scalar_field(state, "Temperature")
force_temperature = -1
field_path=sfield%option_path
if (have_option(trim(field_path)//'/prognostic')) then
! Get number of boundary conditions
bc_path = trim(field_path)//'/prognostic/boundary_conditions'
nbcs=option_count(trim(bc_path))
! Loop over boundary conditions
do i=0, nbcs-1
bc_path_i=trim(bc_path)//"["//int2str(i)//"]"
call get_option(trim(bc_path_i)//"/type[0]/name", bc_type)
if (trim(bc_type) .eq. "bulk_formulae") then
force_temperature = i+1
if (.not. found_bc) then
found_bc = .true.
call get_boundary_condition(sfield, i+1, surface_element_list=surface_element_list)
end if
end if
end do
end if
sfield => extract_scalar_field(state, "PhotosyntheticRadiation",stat)
force_solar = -1
if (stat == 0) then
field_path=sfield%option_path
if (have_option(trim(field_path)//'/prognostic')) then
! Get number of boundary conditions
bc_path = trim(field_path)//'/prognostic/boundary_conditions'
nbcs=option_count(trim(bc_path))
! Loop over boundary conditions
do i=0, nbcs-1
bc_path_i=trim(bc_path)//"["//int2str(i)//"]"
call get_option(trim(bc_path_i)//"/type[0]/name", bc_type)
if (trim(bc_type) .eq. "bulk_formulae") then
force_solar = i+1
if (.not. found_bc) then
found_bc = .true.
call get_boundary_condition(sfield, i+1, surface_element_list=surface_element_list)
end if
end if
end do
end if
end if
! Salinity?!
sfield => extract_scalar_field(state, "Salinity",stat)
force_salinity = -1
if (stat == 0) then
field_path=sfield%option_path
if (have_option(trim(field_path)//'/prognostic')) then
! Get number of boundary conditions
bc_path = trim(field_path)//'/prognostic/boundary_conditions'
nbcs=option_count(trim(bc_path))
! Loop over boundary conditions
do i=0, nbcs-1
bc_path_i=trim(bc_path)//"["//int2str(i)//"]"
call get_option(trim(bc_path_i)//"/type[0]/name", bc_type)
if (trim(bc_type) .eq. "bulk_formulae") then
force_salinity = i+1
if (.not. found_bc) then
found_bc = .true.
call get_boundary_condition(sfield, i+1, surface_element_list=surface_element_list)
end if
end if
end do
end if
end if
! reset found_Bc to false, otherwise, next time we come around it's set to
! .true. for some reason I can't figure out!
found_bc = .false.
end subroutine get_forcing_surface_element_list
subroutine bulk_parameterisations_check_options
character(len=FIELD_NAME_LEN) :: buffer
integer :: stat
real :: nbcs
integer :: dimension
! Don't do BP if it's not included in the model!
if (.not.have_option("/ocean_forcing/bulk_formulae")) return
! Only 3 dimensional problems supported
call get_option("/geometry/dimension/", dimension)
if (dimension .ne. 3 .and. have_option("/ocean_forcing/bulk_formulae")) then
FLExit("Bulk parameterisations only supported for dimension == 3")
end if
call get_option("/problem_type", buffer)
if (buffer/="oceans") then
FLExit("GLS modelling is only supported for problem type oceans.")
end if
! checking for required fields
if (.not.have_option("/material_phase[0]/scalar_field::Temperature")) then
FLExit("You need a Temperature field for bulk forumlae")
end if
if (.not.have_option("/material_phase[0]/vector_field::Velocity")) then
FLExit("You need Velocity field for bulk forumlae")
end if
! check if the diagnostics are on same mesh as the velocity
if (have_option("/ocean_forcing/bulk_formulae/output_fluxes_diagnostics/scalar_field::PhotosyntheticRadiationDownward")) then
call get_option("/ocean_forcing/bulk_formulae/output_fluxes_diagnostics/scalar_field::PhotosyntheticRadiationDownward/diagnostic/mesh/name",buffer)
if (trim(buffer) .ne. "VelocityMesh") then
FLExit("The bulk_forcing diagnostic PhotosyntheticRadiationDownward must be on the velocity mesh")
end if
end if
if (have_option("/ocean_forcing/bulk_formulae/output_fluxes_diagnostics/scalar_field:SalinityFlux")) then
call get_option("/ocean_forcing/bulk_formulae/output_fluxes_diagnostics/scalar_field::SalinityFlux/diagnostic/mesh/name", buffer)
print trim(buffer)
if (trim(buffer) .ne. "VelocityMesh") then
FLExit("The bulk_forcing diagnostic SalinityFlux must be on the velocity mesh")
end if
end if
if (have_option("/ocean_forcing/bulk_formulae/output_fluxes_diagnostics/scalar_field:HeatFlux")) then
call get_option("/ocean_forcing/bulk_formulae/output_fluxes_diagnostics/scalar_field::HeatFlux/diagnostic/mesh/name", buffer)
if (trim(buffer) .ne. "VelocityMesh") then
FLExit("The bulk_forcing diagnostic HeatFlux must be on the velocity mesh")
end if
end if
if (have_option("/ocean_forcing/bulk_formulae/output_fluxes_diagnostics/vector_field::MomentumFlux")) then
call get_option("/ocean_forcing/bulk_formulae/output_fluxes_diagnostics/vector_field::MomentumFlux/diagnostic/mesh/name", buffer)
if (trim(buffer) .ne. "VelocityMesh") then
FLExit("The bulk_forcing diagnostic MomentumFlux must be on the velocity mesh")
end if
end if
end subroutine bulk_parameterisations_check_options
!-----------------------------------------------------------------------------
!
! Private routines - the actual bulk formula!
!
!-----------------------------------------------------------------------------
!~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~!
! Over-ocean fluxes following Large and Yeager (used in NCAR models) !
! Coded by Mike Winton (Michael.Winton@noaa.gov) in 2004
!
! A bug was found by Laurent Brodeau (brodeau@gmail.com) in 2007.
! Stephen.Griffies@noaa.gov updated the code with the bug fix.
!~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~!
!
subroutine ncar_ocean_fluxes (points,u_del, t, ts, q, qs, z, avail, &
cd, ch, ce, ustar, bstar )
implicit none
real, parameter :: gravity = 9.81
real, parameter :: VONKARM = 0.40
integer, intent(in) :: points
real , intent(in) , dimension(points) :: u_del, t, ts, q, qs, z
logical*1, intent(in) , dimension(points) :: avail
real , intent(inout), dimension(points) :: cd, ch, ce, ustar, bstar
real :: cd_n10, ce_n10, ch_n10, cd_n10_rt ! neutral 10m drag coefficients
real :: cd_rt ! full drag coefficients @ z
real :: zeta, x2, x, psi_m, psi_h ! stability parameters
real :: u, u10, tv, tstar, qstar, z0, xx, stab
integer, parameter :: n_itts = 2
integer i, j
! whats what for a non-ocean modeller:
! - u_del - wind speed relative to currents (currents usually ignored)
! - t - temperature
! - ts - SST
! - q - specific humidity
! - qs - saturating humidity
! - z - height of point i
! - avail - array of booleans to say if data is available at point i
! - cd - these are the coefficients calculated by the sub routine
! - ch - that are then used to calculate QH, E and Tau from
! - ce - Large and Yeager (2004), eq: 4a-d
! - ustar
! - bstar
do i=1,points
if (avail(i)) then
tv = t(i)*(1+0.608*q(i));
u = max(u_del(i), 0.5); ! 0.5 m/s floor on wind (undocumented NCAR)
u10 = u; ! first guess 10m wind
cd_n10 = (2.7/u10+0.142+0.0764*u10)/1e3; ! L-Y eqn. 6a
cd_n10_rt = sqrt(cd_n10);
ce_n10 = 34.6 *cd_n10_rt/1e3; ! L-Y eqn. 6b
stab = 0.5 + sign(0.5,t(i)-ts(i))
ch_n10 = (18.0*stab+32.7*(1-stab))*cd_n10_rt/1e3; ! L-Y eqn. 6c
cd(i) = cd_n10; ! first guess for exchange coeff's at z
ch(i) = ch_n10;
ce(i) = ce_n10;
do j=1,n_itts ! Monin-Obukhov iteration
cd_rt = sqrt(cd(i));
ustar(i) = cd_rt*u; ! L-Y eqn. 7a
tstar = (ch(i)/cd_rt)*(t(i)-ts(i)); ! L-Y eqn. 7b
qstar = (ce(i)/cd_rt)*(q(i)-qs(i)); ! L-Y eqn. 7c
bstar(i) = gravity*(tstar/tv+qstar/(q(i)+1/0.608));
zeta = vonkarm*bstar(i)*z(i)/(ustar(i)*ustar(i)); ! L-Y eqn. 8a
zeta = sign( min(abs(zeta),10.0), zeta ); ! undocumented NCAR
x2 = sqrt(abs(1-16*zeta)); ! L-Y eqn. 8b
x2 = max(x2, 1.0); ! undocumented NCAR
x = sqrt(x2);
if (zeta > 0) then
psi_m = -5*zeta; ! L-Y eqn. 8c
psi_h = -5*zeta; ! L-Y eqn. 8c
else
psi_m = log((1+2*x+x2)*(1+x2)/8)-2*(atan(x)-atan(1.0)); ! L-Y eqn. 8d
psi_h = 2*log((1+x2)/2); ! L-Y eqn. 8e
end if
u10 = u/(1+cd_n10_rt*(log(z(i)/10)-psi_m)/vonkarm); ! L-Y eqn. 9
cd_n10 = (2.7/u10+0.142+0.0764*u10)/1e3; ! L-Y eqn. 6a again
cd_n10_rt = sqrt(cd_n10);
ce_n10 = 34.6*cd_n10_rt/1e3; ! L-Y eqn. 6b again
stab = 0.5 + sign(0.5,zeta)
ch_n10 = (18.0*stab+32.7*(1-stab))*cd_n10_rt/1e3; ! L-Y eqn. 6c again
z0 = 10*exp(-vonkarm/cd_n10_rt); ! diagnostic
xx = (log(z(i)/10)-psi_m)/vonkarm;
cd(i) = cd_n10/(1+cd_n10_rt*xx)**2; ! L-Y 10a
xx = (log(z(i)/10)-psi_h)/vonkarm;
ch(i) = ch_n10/(1+ch_n10*xx/cd_n10_rt)*sqrt(cd(i)/cd_n10) ! 10b (corrected code aug2007)
ce(i) = ce_n10/(1+ce_n10*xx/cd_n10_rt)*sqrt(cd(i)/cd_n10) ! 10c (corrected code aug2007)
end do
end if
end do
end subroutine ncar_ocean_fluxes
subroutine coare30_ocean_fluxes (points, u_array, ts_array, t_array, q_array, rs_array, rl_array, rain_array, &
zu, zt, zq, jwave, xlat_array, &
hf_array, ef_array, rf_array, Cdn_array, Chn_array, Cen_array)
implicit none
integer, intent (in) :: points
real, intent (in), dimension(points) :: u_array, ts_array, t_array, q_array, rs_array, rl_array, rain_array, xlat_array
real, intent (inout), dimension(points) :: hf_array, ef_array, rf_array, Cdn_array, Chn_array, Cen_array
real, intent (inout) :: zu, zt, zq, jwave
real :: hwave
real :: x(19), y(30), hnet(30), hl_webb(30)
real :: u, tsnk, ta, qa, rs, rl, org, lat, msp
real :: jcool
real :: a, b, cd, cdn_10, ce, cen_10, ch, chn_10
real :: dqer, dter, hlb, hsb
integer :: ibg, l, le
real :: p, q, qs, qsr, rain, rf,rgas
real :: rhoa, rnl, rns, t, taub, tdk, intime, tkt, ts, tsea
real :: tsr, twave, us, usr, visa, wbar, wg, zi, zo, zoq, zot
! U true wind speed, m/s etl sonic anemometer
! tsnk sea snake temperature, C (0.05 m depth)
! ta air temperature, C (z=14.5 m)
! qa air specific humidity, g/kg (z=14.5 m)
! rs downward solar flux, W/m^2 (ETL units)
! rl downward IR flux, W/m^2 (ETL units)
! org rainrate, mm/hr (ETL STI optical rain gauge, uncorrected)
! lat latitude, deg (SCS pcode)
! msp 6-m deotg T from MSP, C
!zu=15 !anemometer ht
!zt=15 !air T height
!zq=15 !humidity height
jcool=1 ! DO WE WANT COOL LAYER CALCULATION ?
!jwave=0
!******************* set constants ****************
tdk=273.15
Rgas=287.1
dter=0.3
!*********** set variables not in data base ********
P=1008 !air pressure
us=0 !surface current
zi=600 !inversion ht
!****************** setup read data loop **********
do ibg = 1, points
u=u_array(ibg)
tsnk=ts_array(ibg)
ta=t_array(ibg)
qa=q_array(ibg)
rs=rs_array(ibg)
rl=rl_array(ibg)
org=rain_array(ibg)
lat=xlat_array(ibg)
msp=tsnk ! DO WE HAVE A 6 M DATA FOR THIS?!
!******** decode bulk met data ****
ts = tsnk ! if(ibg .eq. 1) ts=tsnk ! CHECK THIS OUT
tsea=tsnk !bulk sea surface temp
t=ta !air temp
qs=qsee(tsea, P) !bulk sea surface humidity
q=qa !air humidity
Rs=rs !downward solar flux
Rl=rl !doward IR flux
rain=org !rain rate
!********* set condition dependent stuff ******
Le=(2.501-.00237*tsea)*1e6
rhoa=P*100/(Rgas*(t+tdk)*(1+0.61*q/1000))
visa=1.326e-5*(1+6.542e-3*t+8.301e-6*t*t-4.84e-9*t*t*t)
ts=tsea
qs=qsee(ts, P)
a=.018
b=.729
twave=b*u
hwave=a*u**2.*(1+.015*u)
x=(/u, us, ts, t, qs, q, Rs, Rl, rain, zi, P, zu, zt, zq, lat, jcool, jwave, twave, hwave/)
!******** call modified LKB routine *******
call cor30a(x,y)
!****************** output from routine *****************************
hsb=y(1) !sensible heat flux W/m/m
hlb=y(2) !latent
taub=y(3) !stress
zo=y(4) !vel roughness
zot=y(5) !temp "
zoq=y(6) !hum "
L=y(7) !Ob Length
usr=y(8) !ustar
tsr=y(9) !tstar
qsr=y(10) !qstar [g/g]
dter=y(11) !cool skin delta T
dqer=y(12) ! " " " q
tkt=y(13) !thickness of cool skin
RF=y(14) !rain heat flux
wbar=y(15) !webb mean w
Cd=y(16) !drag @ zu
Ch=y(17)
Ce=y(18) !Dalton
Cdn_10=y(19) !neutral drag @ 10 [includes gustiness]
Chn_10=y(20)
Cen_10=y(21)
Wg=y(22)
!********** new values from this code
hnet(ibg)=Rns-Rnl-hsb-hlb-RF !total heat input to ocean
hl_webb=rhoa*Le*wbar*qa/1000
! OUR OUTPUT HERE - DO WE WANT ANY MORE OUTUPUT, IS Cdn, Chn and Cen stuff correct at 10
hf_array(ibg) = y(1)
ef_array(ibg) = y(2)
rf_array(ibg) = y(14)
Cdn_array(ibg) = y(19)
Chn_array(ibg) = y(20)
Cen_array(ibg) = y(21)
enddo
contains
subroutine cor30a(x,y)
!version with shortened iteration modified Rt and Rq
!uses wave information wave period in s and wave ht in m
!no wave, standard coare 2.6 charnock: jwave=0
!Oost et al. zo=50/2/pi L (u*/c)**4.5 if jwave=1
!taylor and yelland zo=1200 h*(L/h)**4.5 jwave=2
implicit none
real x(19), y(22)
real u,us,ts,t,Qs,Q,Rs,Rl,rain,zi,P,zu,zt,zq,lat,jcool,twave,hwave
real Beta,von,fdg,tdk,grav,Rgas,Le,cpa,cpv,rhoa,visa,Al,be,cpw,rhow,visw,tcw,bigc,wetc
real lwave,cwave,Rns,Rnl,du,dt,dq,qout,dels,qcol,alq,xlamx,alfac,bf,cc,cd10,ch10,charn,ct,ct10,dtmp,dwat,hl_webb
real jwave, l10,pi,ribcu,ribu,rr,ta,u10,ut,zet,zetu,zo10,zot10
real hsb, hlb, tau, zo, zot, zoq, L, usr, tsr, qsr, dter, dqer, tkt, RF, wbar, Cd, Ch, Ce, Cdn_10, Chn_10, Cen_10, ug
real p30
integer i,nits
u=x(1) !wind speed (m/s) at height zu (m)
us=x(2) !surface current speed in the wind direction (m/s)
ts=x(3) !bulk water temperature (C) if jcool=1, interface water T if jcool=0
t=x(4) !bulk air temperature (C), height zt
Qs=x(5)/1000 !bulk water spec hum (g/kg) if jcool=1, ...
Q=x(6)/1000 !bulk air spec hum (g/kg), height zq
Rs=x(7) !downward solar flux (W/m**2)
Rl=x(8) !downard IR flux (W/m**2)
rain=x(9) !rain rate (mm/hr)
zi=x(10) !PBL depth (m)
P=x(11) !Atmos surface pressure (mb)
zu=x(12) !wind speed measurement height (m)
zt=x(13) !air T measurement height (m)
zq=x(14) !air q measurement height (m)
lat=x(15) !latitude (deg, N=+)
jcool=x(16) !implement cool calculation skin switch, 0=no, 1=yes
jwave=x(17) !implement wave dependent roughness model
twave=x(18) !wave period (s)
hwave=x(19) !wave height (m)
!***************** set constants *************
Beta=1.2
von=0.4
fdg=1.00
tdk=273.15
pi = 3.141593
grav=grv(lat) !9.82
!************* air constants ************
Rgas=287.1
Le=(2.501-.00237*ts)*1e6
cpa=1004.67
cpv=cpa*(1+0.84*Q)
rhoa=P*100/(Rgas*(t+tdk)*(1+0.61*Q))
visa=1.326e-5*(1+6.542e-3*t+8.301e-6*t*t-4.84e-9*t*t*t)
!************ cool skin constants *******
Al=2.1e-5*(ts+3.2)**0.79
be=0.026
cpw=4000
rhow=1022
visw=1e-6
tcw=0.6
bigc=16*grav*cpw*(rhow*visw)**3/(tcw*tcw*rhoa*rhoa)
wetc=0.622*Le*Qs/(Rgas*(ts+tdk)**2)
!*************** wave parameters *********
lwave=grav/2/pi*twave**2
cwave=grav/2/pi*twave
!************** compute aux stuff *******
Rns=Rs*.945
Rnl=0.97*(5.67e-8*(ts-0.3*jcool+tdk)**4-Rl)
!*************** Begin bulk loop *******
!*************** first guess ************
du=u-us
dt=ts-t-.0098*zt
dq=Qs-Q
ta=t+tdk
ug=.5
dter=0.3
dqer=wetc*dter
ut=sqrt(du*du+ug*ug)
u10=ut*log(10/1e-4)/log(zu/1e-4)
usr=.035*u10
zo10=0.011*usr*usr/grav+0.11*visa/usr
Cd10=(von/log(10/zo10))**2
Ch10=0.00115
Ct10=Ch10/sqrt(Cd10)
zot10=10/exp(von/Ct10)
Cd=(von/log(zu/zo10))**2
Ct=von/log(zt/zot10)
CC=von*Ct/Cd
Ribcu=-zu/zi/.004/Beta**3
Ribu=-grav*zu/ta*((dt-dter*jcool)+.61*ta*dq)/ut**2
nits=3
if (Ribu .LT. 0) then
zetu=CC*Ribu/(1+Ribu/Ribcu)
else
zetu=CC*Ribu*(1+27/9*Ribu/CC)
endif
L10=zu/zetu
if (zetu .GT. 50) then
nits=1
endif
usr=ut*von/(log(zu/zo10)-psiuo(zu/L10))
tsr=-(dt-dter*jcool)*von*fdg/(log(zt/zot10)-psit_30(zt/L10))
qsr=-(dq-wetc*dter*jcool)*von*fdg/(log(zq/zot10)-psit_30(zq/L10))
tkt=.001
charn=0.011
if (ut .GT. 10) then
charn=0.011+(ut-10)/(18-10)*(0.018-0.011)
endif
if (ut .GT. 18) then
charn=0.018
endif
!*************** bulk loop ************
do i=1, nits
zet=von*grav*zu/ta*(tsr*(1+0.61*Q)+.61*ta*qsr)/(usr*usr)/(1+0.61*Q)
!disp(usr)
!disp(zet)
if (jwave .EQ. 0) zo=charn*usr*usr/grav+0.11*visa/usr
if (jwave .EQ. 1) zo=50/2/pi*lwave*(usr/cwave)**4.5+0.11*visa/usr !Oost et al
if (jwave .EQ. 2) zo=1200*hwave*(hwave/lwave)**4.5+0.11*visa/usr !Taylor and Yelland
rr=zo*usr/visa
L=zu/zet
zoq=min(1.15e-4,5.5e-5/rr**.6)
zot=zoq
usr=ut*von/(log(zu/zo)-psiuo(zu/L))
tsr=-(dt-dter*jcool)*von*fdg/(log(zt/zot)-psit_30(zt/L))
qsr=-(dq-wetc*dter*jcool)*von*fdg/(log(zq/zoq)-psit_30(zq/L))
Bf=-grav/ta*usr*(tsr+.61*ta*qsr)
if (Bf .GT. 0) then
ug=Beta*(Bf*zi)**.333
else
ug=.2
endif
ut=sqrt(du*du+ug*ug)
Rnl=0.97*(5.67e-8*(ts-dter*jcool+tdk)**4-Rl)
hsb=-rhoa*cpa*usr*tsr
hlb=-rhoa*Le*usr*qsr
qout=Rnl+hsb+hlb
dels=Rns*(.065+11*tkt-6.6e-5/tkt*(1-exp(-tkt/8.0e-4))) ! Eq.16 Shortwave
qcol=qout-dels
alq=Al*qcol+be*hlb*cpw/Le ! Eq. 7 Buoy flux water
if (alq .GT. 0) then
xlamx=6/(1+(bigc*alq/usr**4)**.75)**.333 ! Eq 13 Saunders
tkt=xlamx*visw/(sqrt(rhoa/rhow)*usr) !Eq.11 Sub. thk
else
xlamx=6.0
tkt=min(.01,xlamx*visw/(sqrt(rhoa/rhow)*usr)) !Eq.11 Sub. thk
endif
dter=qcol*tkt/tcw ! Eq.12 Cool skin
dqer=wetc*dter
! print *,' third guesses=',usr,tsr,qsr,ug,ut
enddo !bulk iter loop
tau=rhoa*usr*usr*du/ut !stress
hsb=-rhoa*cpa*usr*tsr
hlb=-rhoa*Le*usr*qsr
!**************** rain heat flux ********
dwat=2.11e-5*((t+tdk)/tdk)**1.94 !! water vapour diffusivity
dtmp=(1.+3.309e-3*t-1.44e-6*t*t)*0.02411/(rhoa*cpa) !!heat diffusivity
alfac= 1/(1+(wetc*Le*dwat)/(cpa*dtmp)) !! wet bulb factor
RF= rain*alfac*cpw*((ts-t-dter*jcool)+(Qs-Q-dqer*jcool)*Le/cpa)/3600
!**************** Webb et al. correection ************
wbar=1.61*hlb/Le/(1+1.61*Q)/rhoa+hsb/rhoa/cpa/ta !formulation in hlb already includes webb
!wbar=1.61*hlb/Le/rhoa+(1+1.61*Q)*hsb/rhoa/cpa/ta
hl_webb=rhoa*wbar*Q*Le
!************** compute transfer coeffs relative to ut @meas. ht **********
Cd=tau/rhoa/ut/max(.1,du)
Ch=-usr*tsr/ut/(dt-dter*jcool)
Ce=-usr*qsr/(dq-dqer*jcool)/ut
!************ 10-m neutral coeff realtive to ut ********
Cdn_10=von*von/log(10/zo)/log(10/zo)
Chn_10=von*von*fdg/log(10/zo)/log(10/zot)
Cen_10=von*von*fdg/log(10/zo)/log(10/zoq)
!**************** the Y array going back tom the main program ****************
y=(/hsb, hlb, tau, zo, zot, zoq, L, usr, tsr, qsr, dter, dqer, tkt, RF, wbar, Cd, Ch, Ce, Cdn_10, Chn_10, Cen_10, ug /)
! 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22
end subroutine
function qsee(ts,Pa)
real :: ts,Pa
real qsee
real x, es, p
x=ts
p=Pa
es=6.112*exp(17.502*x/(x+240.97))*.98*(1.0007+3.46e-6*p)
qsee=es*621.97/(p-.378*es)
end function qsee
function grv(lat)
real lat
real grv
real, parameter :: gamma=9.7803267715
real, parameter :: c1=0.0052790414
real, parameter :: c2=0.0000232718
real, parameter :: c3=0.0000001262
real, parameter :: c4=0.0000000007
real, parameter :: pi=3.141593
real phi, x
phi=lat*pi/180
x=sin(phi)
grv=gamma*(1+(c1*x**2)+(c2*x**4)+(c3*x**6)+(c4*x**8))
end function grv
function psiuo(zet)
real :: psiuo, zet, z, psik, psic, f, c, x
x=(1.-15.*zet)**.25
psik=2.*log((1.+x)/2.)+log((1.+x*x)/2.)-2.*atan(x)+2.*atan(1.)
x=(1.-10.15*zet)**.3333
psic=1.5*log((1.+x+x*x)/3.)-sqrt(3.)*atan((1.+2.*x)/sqrt(3.))+4.*atan(1.)/sqrt(3.)
f=zet*zet/(1+zet*zet)
psiuo=(1-f)*psik+f*psic
if(zet>0)then
c=min(50.,.35*zet)
psiuo=-((1+1.0*zet)**1.0+.667*(zet-14.28)/exp(c)+8.525)
endif
end function psiuo
function psit_30(zet)
real psit_30, zet, x, psik, psic, f, c
x=(1.-(15*zet))**.5
psik=2*log((1+x)/2)
x=(1.-(34.15*zet))**.3333
psic=1.5*log((1.+x+x*x)/3.)-sqrt(3.)*atan((1.+2.*x)/sqrt(3.))+4.*atan(1.)/sqrt(3.)
f=zet*zet/(1+zet*zet)
psit_30=(1-f)*psik+f*psic
if(zet>0)then
c=min(50.,.35*zet)
psit_30=-((1.+2./3.*zet)**1.5+.6667*(zet-14.28)/exp(c)+8.525)
endif
end function psit_30
end subroutine coare30_ocean_fluxes
subroutine kara_ocean_fluxes(points, u, v, R, Ta, Ts, Va, lhf, shf, &
tau_u, tau_v, tau_r, Ce, Cd, Ch)
implicit none
! INPUT:
! u = Zonal wins speed component (m s^-1)
! v = Meridional wins speed component (m s^-1)
! R = Rain rate (mm h^-1)
! Ta = Air temp at 10 m above sea level (C)
! Ts = Sea surface temperature (C)
! Va = Wind speed at 10 m above sea level (m s^-1)
! OUTPUT
! lhf = Latent heat flux (W m^-2)
! shf = Sensible heat flux (W m^-2)
! tau_u = Zonal component of wind stress (N m^-2)
! tau_v = Zonal component of wind stress (N m^-2)
! tau_r = Wind stress due to rain fall (N m^-2)
! Ce = Latent heat flux coefficient
! Cd = Wind stress drag coefficient
! Ch = Sensible heat flux coefficient
integer, intent(in) :: points
real , intent(in) , dimension(points) :: u, v, R, Ta, Ts
real , intent(inout), dimension(points) :: Va
real, intent(out), dimension(points) :: lhf, shf, tau_u, tau_v, tau_r, Ce, Cd, Ch
! Temp variables
real :: Cd0, Cd1, Ce0, Ce1, pa_i, qa, qs
integer :: i
! Constants here
real :: Cp, L, Pa, Rgas, absT
Cp = 1004.5 ! Specific heat of air (J kg^-1 K^-1)
L = 2.5*10.0**6.0 ! Latent heat of vaporisation (J kg^-1)
Pa = 1013.0 ! Atmospheric pressure at sea surface (mb)
Rgas = 287.1 ! Gas constant (J Kg^-1 K^-1)
absT = 273.16 ! Absolute Temperature
! Main loop
do i=1,points
Va(i) = max(2.5, min(32.5, Va(i)));
pa_i = 100.0*Pa/(Rgas*(Ta(i) + absT))
Cd0 = 1.0/1000*(0.862 + 0.088*Va(i) - 0.00089*(Va(i))**2)
Cd1 = 1.0/1000*(0.1034 - 0.00678*Va(i) + 0.0001147*(Va(i))**2)
Cd(i) = Cd0 + Cd1*(Ts(i) - Ta(i))
tau_u(i) = pa_i*Cd(i)*u(i)*sqrt(u(i)**2 + v(i)**2)
tau_v(i) = pa_i*Cd(i)*v(i)*sqrt(u(i)**2 + v(i)**2)
tau_r(i) = R(i)*Va(i)/3600
Ce0 = 1.0/1000*(0.994 + 0.061*Va(i) - 0.001*(Va(i))**2)
Ce1 = 1.0/1000*(-0.020 + 0.691*(1/Va(i)) - 0.817*(1/(Va(i)))**2)
Ce(i) = Ce0 + Ce1*(Ts(i) - Ta(i))
Ch(i) = 0.96*Ce(i)
shf(i) = Ch(i)*Cp*pa_i*Va(i)*(Ta(i) - Ts(i))
qa = R(i)*shf(i)*qsat(Ta(i), Pa)
qs = 0.98*qsat(Ts(i), Pa)
lhf(i) = Ce(i)*L*pa_i*Va(i)*(qa - qs)
end do
contains
function qsat (T, Pa)
real :: T, Pa, qsat
qsat = 0.622*es(T, Pa)/(Pa - 0.378*es(T, Pa))
end function qsat
function es (T, Pa)
real :: T, Pa, es
es = (1.0 + 3.46*(10.0**(-6))*Pa)*6.1121*exp(17.50*T/(240.97 + T))
end function es
end subroutine kara_ocean_fluxes
end module bulk_parameterisations
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