[4773] | 1 | ! radiation_regions.F90 -- Properties of horizontal regions in Tripleclouds & SPARTACUS |
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| 2 | ! |
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| 3 | ! (C) Copyright 2016- ECMWF. |
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| 4 | ! |
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| 5 | ! This software is licensed under the terms of the Apache Licence Version 2.0 |
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| 6 | ! which can be obtained at http://www.apache.org/licenses/LICENSE-2.0. |
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| 7 | ! |
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| 8 | ! In applying this licence, ECMWF does not waive the privileges and immunities |
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| 9 | ! granted to it by virtue of its status as an intergovernmental organisation |
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| 10 | ! nor does it submit to any jurisdiction. |
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| 11 | ! |
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| 12 | ! Author: Robin Hogan |
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| 13 | ! Email: r.j.hogan@ecmwf.int |
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| 14 | ! |
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| 15 | ! Modifications |
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| 16 | ! 2017-07-14 R. Hogan Incorporate gamma distribution option |
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| 17 | ! 2018-10-06 R. Hogan Merged from radiation_optical_depth_scaling.h and radiation_overlap.F90 |
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| 18 | |
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| 19 | module radiation_regions |
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| 20 | |
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| 21 | implicit none |
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| 22 | |
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| 23 | public :: calc_region_properties |
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| 24 | |
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| 25 | contains |
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| 26 | |
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| 27 | !--------------------------------------------------------------------- |
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| 28 | ! Compute the optical depth scalings for the optically "thick" and |
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| 29 | ! "thin" regions of a Tripleclouds representation of a sub-grid PDF |
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| 30 | ! of cloud optical depth. Following Shonk and Hogan (2008), the 16th |
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| 31 | ! percentile is used for the thin region, and the formulas estimate |
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| 32 | ! this for both lognormal and gamma distributions. However, an |
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| 33 | ! adjustment is needed for the gamma distribution at large |
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| 34 | ! fractional standard deviations. |
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| 35 | subroutine calc_region_properties(nlev, nreg, istartcol, iendcol, do_gamma, & |
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| 36 | & cloud_fraction, frac_std, reg_fracs, od_scaling, cloud_fraction_threshold) |
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| 37 | |
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| 38 | use parkind1, only : jprb |
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| 39 | use yomhook, only : lhook, dr_hook, jphook |
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| 40 | use radiation_io, only : nulerr, radiation_abort |
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| 41 | |
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| 42 | ! Minimum od_scaling in the case of a Gamma distribution |
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| 43 | real(jprb), parameter :: MinGammaODScaling = 0.025_jprb |
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| 44 | |
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| 45 | ! At large fractional standard deviations (FSDs), we cannot |
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| 46 | ! capture the behaviour of a gamma distribution with two equally |
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| 47 | ! weighted points; we need to weight the first ("lower") point |
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| 48 | ! more. The weight of the first point is normally 0.5, but for |
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| 49 | ! FSDs between 1.5 and 3.725 it rises linearly to 0.9, and for |
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| 50 | ! higher FSD it is capped at this value. The weight of the second |
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| 51 | ! point is one minus the first point. |
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| 52 | real(jprb), parameter :: MinLowerFrac = 0.5_jprb |
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| 53 | real(jprb), parameter :: MaxLowerFrac = 0.9_jprb |
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| 54 | real(jprb), parameter :: FSDAtMinLowerFrac = 1.5_jprb |
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| 55 | real(jprb), parameter :: FSDAtMaxLowerFrac = 3.725_jprb |
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| 56 | ! Between FSDAtMinLowerFrac and FSDAtMaxLowerFrac, |
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| 57 | ! LowerFrac=LowerFracFSDIntercept+FSD*LowerFracFSDGradient |
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| 58 | real(jprb), parameter :: LowerFracFSDGradient & |
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| 59 | & = (MaxLowerFrac-MinLowerFrac) / (FSDAtMaxLowerFrac-FSDAtMinLowerFrac) |
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| 60 | real(jprb), parameter :: LowerFracFSDIntercept & |
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| 61 | & = MinLowerFrac - FSDAtMinLowerFrac*LowerFracFSDGradient |
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| 62 | |
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| 63 | ! Number of levels and regions |
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| 64 | integer, intent(in) :: nlev, nreg |
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| 65 | |
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| 66 | ! Range of columns to process |
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| 67 | integer, intent(in) :: istartcol, iendcol |
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| 68 | |
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| 69 | ! Do we do a lognormal or gamma distribution? |
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| 70 | logical, intent(in) :: do_gamma |
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| 71 | |
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| 72 | ! Cloud fraction, i.e. the fraction of the gridbox assigned to all |
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| 73 | ! regions numbered 2 and above (region 1 is clear sky) |
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| 74 | real(jprb), intent(in), dimension(:,:) :: cloud_fraction ! (ncol,nlev) |
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| 75 | |
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| 76 | ! Fractional standard deviation of in-cloud water content |
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| 77 | real(jprb), intent(in), dimension(:,:) :: frac_std ! (ncol,nlev) |
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| 78 | |
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| 79 | ! Fractional area coverage of each region |
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| 80 | real(jprb), intent(out) :: reg_fracs(1:nreg,nlev,istartcol:iendcol) |
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| 81 | |
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| 82 | ! Optical depth scaling for the cloudy regions |
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| 83 | real(jprb), intent(out) :: od_scaling(2:nreg,nlev,istartcol:iendcol) |
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| 84 | |
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| 85 | ! Regions smaller than this are ignored |
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| 86 | real(jprb), intent(in), optional :: cloud_fraction_threshold |
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| 87 | |
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| 88 | ! In case the user doesn't supply cloud_fraction_threshold we use |
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| 89 | ! a default value |
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| 90 | real(jprb) :: frac_threshold |
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| 91 | |
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| 92 | ! Loop indices |
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| 93 | integer :: jcol, jlev |
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| 94 | |
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| 95 | real(jphook) :: hook_handle |
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| 96 | |
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| 97 | if (lhook) call dr_hook('radiation_region_properties:calc_region_properties',0,hook_handle) |
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| 98 | |
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| 99 | if (present(cloud_fraction_threshold)) then |
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| 100 | frac_threshold = cloud_fraction_threshold |
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| 101 | else |
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| 102 | frac_threshold = 1.0e-20_jprb |
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| 103 | end if |
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| 104 | |
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| 105 | if (nreg == 2) then |
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| 106 | ! Only one clear-sky and one cloudy region: cloudy region is |
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| 107 | ! homogeneous |
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| 108 | reg_fracs(2,1:nlev,istartcol:iendcol) = transpose(cloud_fraction(istartcol:iendcol,1:nlev)) |
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| 109 | reg_fracs(1,1:nlev,istartcol:iendcol) = 1.0_jprb - reg_fracs(2,1:nlev,istartcol:iendcol) |
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| 110 | od_scaling(2,1:nlev,istartcol:iendcol) = 1.0_jprb |
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| 111 | |
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| 112 | else if (nreg == 3) then |
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| 113 | ! Two cloudy regions with optical depth scaled by 1-x and |
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| 114 | ! 1+x. |
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| 115 | ! Simple version which fails when fractional_std >= 1: |
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| 116 | !od_scaling(2) = 1.0_jprb-cloud%fractional_std(jcol,jlev) |
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| 117 | ! According to Shonk and Hogan (2008), 1-FSD should correspond to |
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| 118 | ! the 16th percentile. |
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| 119 | if (.not. do_gamma) then |
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| 120 | ! If we treat the distribution as a lognormal such that the |
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| 121 | ! equivalent Normal has a mean mu and standard deviation |
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| 122 | ! sigma, then the 16th percentile of the lognormal is very |
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| 123 | ! close to exp(mu-sigma). |
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| 124 | do jcol = istartcol,iendcol |
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| 125 | do jlev = 1,nlev |
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| 126 | if (cloud_fraction(jcol,jlev) < frac_threshold) then |
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| 127 | reg_fracs(1,jlev,jcol) = 1.0_jprb |
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| 128 | reg_fracs(2:3,jlev,jcol) = 0.0_jprb |
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| 129 | od_scaling(2:3,jlev,jcol) = 1.0_jprb |
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| 130 | else |
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| 131 | reg_fracs(1,jlev,jcol) = 1.0_jprb - cloud_fraction(jcol,jlev) |
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| 132 | reg_fracs(2:3,jlev,jcol) = cloud_fraction(jcol,jlev)*0.5_jprb |
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| 133 | od_scaling(2,jlev,jcol) & |
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| 134 | & = exp(-sqrt(log(frac_std(jcol,jlev)**2+1))) & |
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| 135 | & / sqrt(frac_std(jcol,jlev)**2+1) |
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| 136 | od_scaling(3,jlev,jcol) = 2.0_jprb - od_scaling(2,jlev,jcol) |
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| 137 | end if |
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| 138 | end do |
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| 139 | end do |
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| 140 | else |
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| 141 | ! If we treat the distribution as a gamma then the 16th |
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| 142 | ! percentile is close to the following. Note that because it |
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| 143 | ! becomes vanishingly small for FSD >~ 2, we have a lower |
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| 144 | ! limit of 1/40, and for higher FSDs reduce the fractional |
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| 145 | ! cover of the denser region - see region_fractions routine |
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| 146 | ! below |
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| 147 | do jcol = istartcol,iendcol |
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| 148 | do jlev = 1,nlev |
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| 149 | if (cloud_fraction(jcol,jlev) < frac_threshold) then |
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| 150 | reg_fracs(1,jlev,jcol) = 1.0_jprb |
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| 151 | reg_fracs(2:3,jlev,jcol) = 0.0_jprb |
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| 152 | od_scaling(2:3,jlev,jcol) = 1.0_jprb |
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| 153 | else |
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| 154 | ! Fraction of the clear-sky region |
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| 155 | reg_fracs(1,jlev,jcol) = 1.0_jprb - cloud_fraction(jcol,jlev) |
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| 156 | !#define OLD_GAMMA_REGION_BEHAVIOUR 1 |
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| 157 | #ifdef OLD_GAMMA_REGION_BEHAVIOUR |
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| 158 | ! Use previous behaviour (ecRad version 1.1.5 and |
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| 159 | ! earlier): cloudy fractions are the same and there is |
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| 160 | ! no minimum optical depth scaling; this tends to lead |
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| 161 | ! to an overprediction of the reflection from scenes |
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| 162 | ! with a large fractional standard deviation of optical |
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| 163 | ! depth. |
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| 164 | ! Fraction and optical-depth scaling of the lower of the |
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| 165 | ! two cloudy regions |
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| 166 | reg_fracs(2,jlev,jcol) = cloud_fraction(jcol,jlev) * 0.5_jprb |
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| 167 | od_scaling(2,jlev,jcol) = & |
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| 168 | & exp(-frac_std(jcol,jlev)*(1.0_jprb + 0.5_jprb*frac_std(jcol,jlev) & |
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| 169 | & *(1.0_jprb+0.5_jprb*frac_std(jcol,jlev)))) |
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| 170 | |
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| 171 | #else |
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| 172 | ! Improved behaviour. |
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| 173 | ! Fraction and optical-depth scaling of the lower of the |
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| 174 | ! two cloudy regions |
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| 175 | reg_fracs(2,jlev,jcol) = cloud_fraction(jcol,jlev) & |
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| 176 | & * max(MinLowerFrac, min(MaxLowerFrac, & |
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| 177 | & LowerFracFSDIntercept + frac_std(jcol,jlev)*LowerFracFSDGradient)) |
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| 178 | od_scaling(2,jlev,jcol) = MinGammaODScaling & |
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| 179 | & + (1.0_jprb - MinGammaODScaling) & |
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| 180 | & * exp(-frac_std(jcol,jlev)*(1.0_jprb + 0.5_jprb*frac_std(jcol,jlev) & |
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| 181 | & *(1.0_jprb+0.5_jprb*frac_std(jcol,jlev)))) |
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| 182 | #endif |
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| 183 | ! Fraction of the upper of the two cloudy regions |
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| 184 | reg_fracs(3,jlev,jcol) = 1.0_jprb-reg_fracs(1,jlev,jcol)-reg_fracs(2,jlev,jcol) |
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| 185 | ! Ensure conservation of the mean optical depth |
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| 186 | od_scaling(3,jlev,jcol) = (cloud_fraction(jcol,jlev) & |
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| 187 | & -reg_fracs(2,jlev,jcol)*od_scaling(2,jlev,jcol)) / reg_fracs(3,jlev,jcol) |
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| 188 | end if |
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| 189 | end do |
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| 190 | end do |
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| 191 | end if |
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| 192 | else ! nreg > 3 |
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| 193 | write(nulerr,'(a)') '*** Error: only 2 or 3 regions may be specified' |
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| 194 | call radiation_abort() |
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| 195 | end if |
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| 196 | |
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| 197 | if (lhook) call dr_hook('radiation_region_properties:calc_region_properties',1,hook_handle) |
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| 198 | |
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| 199 | end subroutine calc_region_properties |
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| 200 | |
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| 201 | end module radiation_regions |
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| 202 | |
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