! radiation_regions.F90 -- Properties of horizontal regions in Tripleclouds & SPARTACUS ! (C) Copyright 2016- ECMWF. ! This software is licensed under the terms of the Apache Licence Version 2.0 ! which can be obtained at http://www.apache.org/licenses/LICENSE-2.0. ! In applying this licence, ECMWF does not waive the privileges and immunities ! granted to it by virtue of its status as an intergovernmental organisation ! nor does it submit to any jurisdiction. ! Author: Robin Hogan ! Email: r.j.hogan@ecmwf.int ! Modifications ! 2017-07-14 R. Hogan Incorporate gamma distribution option ! 2018-10-06 R. Hogan Merged from radiation_optical_depth_scaling.h and radiation_overlap.F90 module radiation_regions implicit none public :: calc_region_properties contains !--------------------------------------------------------------------- ! Compute the optical depth scalings for the optically "thick" and ! "thin" regions of a Tripleclouds representation of a sub-grid PDF ! of cloud optical depth. Following Shonk and Hogan (2008), the 16th ! percentile is used for the thin region, and the formulas estimate ! this for both lognormal and gamma distributions. However, an ! adjustment is needed for the gamma distribution at large ! fractional standard deviations. subroutine calc_region_properties(nlev, nreg, istartcol, iendcol, do_gamma, & & cloud_fraction, frac_std, reg_fracs, od_scaling, cloud_fraction_threshold) use parkind1, only : jprb use yomhook, only : lhook, dr_hook, jphook use radiation_io, only : nulerr, radiation_abort ! Minimum od_scaling in the case of a Gamma distribution real(jprb), parameter :: MinGammaODScaling = 0.025_jprb ! At large fractional standard deviations (FSDs), we cannot ! capture the behaviour of a gamma distribution with two equally ! weighted points; we need to weight the first ("lower") point ! more. The weight of the first point is normally 0.5, but for ! FSDs between 1.5 and 3.725 it rises linearly to 0.9, and for ! higher FSD it is capped at this value. The weight of the second ! point is one minus the first point. real(jprb), parameter :: MinLowerFrac = 0.5_jprb real(jprb), parameter :: MaxLowerFrac = 0.9_jprb real(jprb), parameter :: FSDAtMinLowerFrac = 1.5_jprb real(jprb), parameter :: FSDAtMaxLowerFrac = 3.725_jprb ! Between FSDAtMinLowerFrac and FSDAtMaxLowerFrac, ! LowerFrac=LowerFracFSDIntercept+FSD*LowerFracFSDGradient real(jprb), parameter :: LowerFracFSDGradient & & = (MaxLowerFrac-MinLowerFrac) / (FSDAtMaxLowerFrac-FSDAtMinLowerFrac) real(jprb), parameter :: LowerFracFSDIntercept & & = MinLowerFrac - FSDAtMinLowerFrac*LowerFracFSDGradient ! Number of levels and regions integer, intent(in) :: nlev, nreg ! Range of columns to process integer, intent(in) :: istartcol, iendcol ! Do we do a lognormal or gamma distribution? logical, intent(in) :: do_gamma ! Cloud fraction, i.e. the fraction of the gridbox assigned to all ! regions numbered 2 and above (region 1 is clear sky) real(jprb), intent(in), dimension(:,:) :: cloud_fraction ! (ncol,nlev) ! Fractional standard deviation of in-cloud water content real(jprb), intent(in), dimension(:,:) :: frac_std ! (ncol,nlev) ! Fractional area coverage of each region real(jprb), intent(out) :: reg_fracs(1:nreg,nlev,istartcol:iendcol) ! Optical depth scaling for the cloudy regions real(jprb), intent(out) :: od_scaling(2:nreg,nlev,istartcol:iendcol) ! Regions smaller than this are ignored real(jprb), intent(in), optional :: cloud_fraction_threshold ! In case the user doesn't supply cloud_fraction_threshold we use ! a default value real(jprb) :: frac_threshold ! Loop indices integer :: jcol, jlev real(jphook) :: hook_handle if (lhook) call dr_hook('radiation_region_properties:calc_region_properties',0,hook_handle) if (present(cloud_fraction_threshold)) then frac_threshold = cloud_fraction_threshold else frac_threshold = 1.0e-20_jprb end if if (nreg == 2) then ! Only one clear-sky and one cloudy region: cloudy region is ! homogeneous reg_fracs(2,1:nlev,istartcol:iendcol) = transpose(cloud_fraction(istartcol:iendcol,1:nlev)) reg_fracs(1,1:nlev,istartcol:iendcol) = 1.0_jprb - reg_fracs(2,1:nlev,istartcol:iendcol) od_scaling(2,1:nlev,istartcol:iendcol) = 1.0_jprb else if (nreg == 3) then ! Two cloudy regions with optical depth scaled by 1-x and ! 1+x. ! Simple version which fails when fractional_std >= 1: !od_scaling(2) = 1.0_jprb-cloud%fractional_std(jcol,jlev) ! According to Shonk and Hogan (2008), 1-FSD should correspond to ! the 16th percentile. if (.not. do_gamma) then ! If we treat the distribution as a lognormal such that the ! equivalent Normal has a mean mu and standard deviation ! sigma, then the 16th percentile of the lognormal is very ! close to exp(mu-sigma). DO jcol = istartcol,iendcol DO jlev = 1,nlev if (cloud_fraction(jcol,jlev) < frac_threshold) then reg_fracs(1,jlev,jcol) = 1.0_jprb reg_fracs(2:3,jlev,jcol) = 0.0_jprb od_scaling(2:3,jlev,jcol) = 1.0_jprb else reg_fracs(1,jlev,jcol) = 1.0_jprb - cloud_fraction(jcol,jlev) reg_fracs(2:3,jlev,jcol) = cloud_fraction(jcol,jlev)*0.5_jprb od_scaling(2,jlev,jcol) & & = exp(-sqrt(log(frac_std(jcol,jlev)**2+1))) & & / sqrt(frac_std(jcol,jlev)**2+1) od_scaling(3,jlev,jcol) = 2.0_jprb - od_scaling(2,jlev,jcol) end if end do end do else ! If we treat the distribution as a gamma then the 16th ! percentile is close to the following. Note that because it ! becomes vanishingly small for FSD >~ 2, we have a lower ! limit of 1/40, and for higher FSDs reduce the fractional ! cover of the denser region - see region_fractions routine ! below DO jcol = istartcol,iendcol DO jlev = 1,nlev if (cloud_fraction(jcol,jlev) < frac_threshold) then reg_fracs(1,jlev,jcol) = 1.0_jprb reg_fracs(2:3,jlev,jcol) = 0.0_jprb od_scaling(2:3,jlev,jcol) = 1.0_jprb else ! Fraction of the clear-sky region reg_fracs(1,jlev,jcol) = 1.0_jprb - cloud_fraction(jcol,jlev) !#define OLD_GAMMA_REGION_BEHAVIOUR 1 #ifdef OLD_GAMMA_REGION_BEHAVIOUR ! Use previous behaviour (ecRad version 1.1.5 and ! earlier): cloudy fractions are the same and there is ! no minimum optical depth scaling; this tends to lead ! to an overprediction of the reflection from scenes ! with a large fractional standard deviation of optical ! depth. ! Fraction and optical-depth scaling of the lower of the ! two cloudy regions reg_fracs(2,jlev,jcol) = cloud_fraction(jcol,jlev) * 0.5_jprb od_scaling(2,jlev,jcol) = & & exp(-frac_std(jcol,jlev)*(1.0_jprb + 0.5_jprb*frac_std(jcol,jlev) & & *(1.0_jprb+0.5_jprb*frac_std(jcol,jlev)))) #else ! Improved behaviour. ! Fraction and optical-depth scaling of the lower of the ! two cloudy regions reg_fracs(2,jlev,jcol) = cloud_fraction(jcol,jlev) & & * max(MinLowerFrac, min(MaxLowerFrac, & & LowerFracFSDIntercept + frac_std(jcol,jlev)*LowerFracFSDGradient)) od_scaling(2,jlev,jcol) = MinGammaODScaling & & + (1.0_jprb - MinGammaODScaling) & & * exp(-frac_std(jcol,jlev)*(1.0_jprb + 0.5_jprb*frac_std(jcol,jlev) & & *(1.0_jprb+0.5_jprb*frac_std(jcol,jlev)))) #endif ! Fraction of the upper of the two cloudy regions reg_fracs(3,jlev,jcol) = 1.0_jprb-reg_fracs(1,jlev,jcol)-reg_fracs(2,jlev,jcol) ! Ensure conservation of the mean optical depth od_scaling(3,jlev,jcol) = (cloud_fraction(jcol,jlev) & & -reg_fracs(2,jlev,jcol)*od_scaling(2,jlev,jcol)) / reg_fracs(3,jlev,jcol) end if end do end do end if else ! nreg > 3 write(nulerr,'(a)') '*** Error: only 2 or 3 regions may be specified' call radiation_abort() end if if (lhook) call dr_hook('radiation_region_properties:calc_region_properties',1,hook_handle) end subroutine calc_region_properties end module radiation_regions