1 | ! radiation_homogeneous_lw.F90 - Longwave homogeneous-column (no cloud fraction) solver |
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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 | ! 2017-04-11 R. Hogan Receive emission/albedo rather than planck/emissivity |
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17 | ! 2017-04-22 R. Hogan Store surface fluxes at all g-points |
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18 | ! 2017-10-23 R. Hogan Renamed single-character variables |
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19 | ! 2019-01-14 R. Hogan Save spectral flux profile if required |
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20 | |
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21 | module radiation_homogeneous_lw |
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22 | |
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23 | public |
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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 | ! Longwave homogeneous solver, in which clouds are assumed to fill |
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29 | ! the gridbox horizontally |
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30 | subroutine solver_homogeneous_lw(nlev,istartcol,iendcol, & |
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31 | & config, cloud, & |
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32 | & od, ssa, g, od_cloud, ssa_cloud, g_cloud, planck_hl, & |
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33 | & emission, albedo, & |
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34 | & flux) |
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35 | |
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36 | use parkind1, only : jprb |
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37 | use yomhook, only : lhook, dr_hook |
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38 | |
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39 | use radiation_config, only : config_type |
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40 | use radiation_cloud, only : cloud_type |
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41 | use radiation_flux, only : flux_type, indexed_sum_profile |
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42 | use radiation_two_stream, only : calc_two_stream_gammas_lw, & |
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43 | & calc_reflectance_transmittance_lw, & |
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44 | & calc_no_scattering_transmittance_lw |
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45 | use radiation_adding_ica_lw, only : adding_ica_lw, calc_fluxes_no_scattering_lw |
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46 | use radiation_lw_derivatives, only : calc_lw_derivatives_ica |
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47 | |
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48 | implicit none |
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49 | |
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50 | ! Inputs |
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51 | integer, intent(in) :: nlev ! number of model levels |
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52 | integer, intent(in) :: istartcol, iendcol ! range of columns to process |
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53 | type(config_type), intent(in) :: config |
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54 | type(cloud_type), intent(in) :: cloud |
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55 | |
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56 | ! Gas and aerosol optical depth, single-scattering albedo and |
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57 | ! asymmetry factor at each longwave g-point |
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58 | real(jprb), intent(in), dimension(config%n_g_lw, nlev, istartcol:iendcol) :: & |
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59 | & od |
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60 | real(jprb), intent(in), dimension(config%n_g_lw_if_scattering, nlev, istartcol:iendcol) :: & |
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61 | & ssa, g |
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62 | |
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63 | ! Cloud and precipitation optical depth, single-scattering albedo and |
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64 | ! asymmetry factor in each longwave band |
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65 | real(jprb), intent(in), dimension(config%n_bands_lw,nlev,istartcol:iendcol) :: & |
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66 | & od_cloud |
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67 | real(jprb), intent(in), dimension(config%n_bands_lw_if_scattering, & |
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68 | & nlev,istartcol:iendcol) :: ssa_cloud, g_cloud |
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69 | |
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70 | ! Planck function at each half-level and the surface |
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71 | real(jprb), intent(in), dimension(config%n_g_lw,nlev+1,istartcol:iendcol) :: & |
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72 | & planck_hl |
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73 | |
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74 | ! Emission (Planck*emissivity) and albedo (1-emissivity) at the |
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75 | ! surface at each longwave g-point |
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76 | real(jprb), intent(in), dimension(config%n_g_lw, istartcol:iendcol) & |
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77 | & :: emission, albedo |
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78 | |
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79 | ! Output |
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80 | type(flux_type), intent(inout):: flux |
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81 | |
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82 | ! Local variables |
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83 | |
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84 | ! Diffuse reflectance and transmittance for each layer in clear |
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85 | ! and all skies |
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86 | real(jprb), dimension(config%n_g_lw, nlev) :: reflectance, transmittance |
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87 | |
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88 | ! Emission by a layer into the upwelling or downwelling diffuse |
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89 | ! streams, in clear and all skies |
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90 | real(jprb), dimension(config%n_g_lw, nlev) :: source_up, source_dn |
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91 | |
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92 | ! Fluxes per g point |
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93 | real(jprb), dimension(config%n_g_lw, nlev+1) :: flux_up, flux_dn |
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94 | |
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95 | ! Combined gas+aerosol+cloud optical depth, single scattering |
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96 | ! albedo and asymmetry factor |
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97 | real(jprb), dimension(config%n_g_lw) :: od_total, ssa_total, g_total |
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98 | |
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99 | ! Two-stream coefficients |
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100 | real(jprb), dimension(config%n_g_lw) :: gamma1, gamma2 |
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101 | |
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102 | ! Optical depth of cloud in g-point space |
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103 | real(jprb), dimension(config%n_g_lw) :: od_cloud_g |
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104 | |
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105 | ! Is there any cloud in the profile? |
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106 | logical :: is_cloudy_profile |
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107 | |
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108 | ! Number of g points |
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109 | integer :: ng |
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110 | |
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111 | ! Loop indices for level and column |
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112 | integer :: jlev, jcol |
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113 | |
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114 | real(jprb) :: hook_handle |
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115 | |
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116 | if (lhook) call dr_hook('radiation_homogeneous_lw:solver_homogeneous_lw',0,hook_handle) |
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117 | |
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118 | ng = config%n_g_lw |
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119 | |
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120 | ! Loop through columns |
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121 | do jcol = istartcol,iendcol |
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122 | |
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123 | ! Is there any cloud in the profile? |
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124 | is_cloudy_profile = .false. |
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125 | do jlev = 1,nlev |
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126 | if (cloud%fraction(jcol,jlev) >= config%cloud_fraction_threshold) then |
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127 | is_cloudy_profile = .true. |
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128 | exit |
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129 | end if |
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130 | end do |
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131 | |
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132 | ! If clear-sky fluxes need to be computed then we first compute |
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133 | ! the reflectance and transmittance of all layers, neglecting |
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134 | ! clouds. If clear-sky fluxes are not required then we only do |
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135 | ! the clear-sky layers since these will be needed when we come |
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136 | ! to do the total-sky fluxes. |
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137 | do jlev = 1,nlev |
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138 | if (config%do_clear .or. cloud%fraction(jcol,jlev) & |
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139 | & < config%cloud_fraction_threshold) then |
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140 | if (config%do_lw_aerosol_scattering) then |
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141 | ! Scattering case: first compute clear-sky reflectance, |
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142 | ! transmittance etc at each model level |
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143 | ssa_total = ssa(:,jlev,jcol) |
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144 | g_total = g(:,jlev,jcol) |
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145 | call calc_two_stream_gammas_lw(ng, ssa_total, g_total, & |
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146 | & gamma1, gamma2) |
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147 | call calc_reflectance_transmittance_lw(ng, & |
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148 | & od(:,jlev,jcol), gamma1, gamma2, & |
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149 | & planck_hl(:,jlev,jcol), planck_hl(:,jlev+1,jcol), & |
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150 | & reflectance(:,jlev), transmittance(:,jlev), & |
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151 | & source_up(:,jlev), source_dn(:,jlev)) |
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152 | else |
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153 | ! Non-scattering case: use simpler functions for |
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154 | ! transmission and emission |
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155 | call calc_no_scattering_transmittance_lw(ng, od(:,jlev,jcol), & |
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156 | & planck_hl(:,jlev,jcol), planck_hl(:,jlev+1, jcol), & |
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157 | & transmittance(:,jlev), source_up(:,jlev), source_dn(:,jlev)) |
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158 | ! Ensure that clear-sky reflectance is zero since it may be |
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159 | ! used in cloudy-sky case |
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160 | reflectance(:,jlev) = 0.0_jprb |
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161 | end if |
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162 | |
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163 | end if |
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164 | end do |
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165 | |
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166 | if (config%do_clear) then |
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167 | if (config%do_lw_aerosol_scattering) then |
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168 | ! Then use adding method to compute fluxes |
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169 | call adding_ica_lw(ng, nlev, & |
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170 | & reflectance, transmittance, source_up, source_dn, & |
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171 | & emission(:,jcol), albedo(:,jcol), & |
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172 | & flux_up, flux_dn) |
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173 | else |
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174 | ! Simpler down-then-up method to compute fluxes |
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175 | call calc_fluxes_no_scattering_lw(ng, nlev, & |
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176 | & transmittance, source_up, source_dn, & |
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177 | & emission(:,jcol), albedo(:,jcol), & |
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178 | & flux_up, flux_dn) |
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179 | |
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180 | end if |
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181 | |
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182 | ! Sum over g-points to compute broadband fluxes |
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183 | flux%lw_up_clear(jcol,:) = sum(flux_up,1) |
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184 | flux%lw_dn_clear(jcol,:) = sum(flux_dn,1) |
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185 | ! Store surface spectral downwelling fluxes |
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186 | flux%lw_dn_surf_clear_g(:,jcol) = flux_dn(:,nlev+1) |
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187 | |
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188 | ! Save the spectral fluxes if required |
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189 | if (config%do_save_spectral_flux) then |
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190 | call indexed_sum_profile(flux_up, config%i_spec_from_reordered_g_lw, & |
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191 | & flux%lw_up_clear_band(:,jcol,:)) |
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192 | call indexed_sum_profile(flux_dn, config%i_spec_from_reordered_g_lw, & |
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193 | & flux%lw_dn_clear_band(:,jcol,:)) |
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194 | end if |
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195 | |
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196 | end if ! Do clear-sky calculations |
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197 | |
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198 | ! Now the total-sky calculation. If this is a clear profile and |
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199 | ! clear-sky fluxes have been calculated then we can simply copy |
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200 | ! over the clear-sky fluxes, otherwise we need to compute fluxes |
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201 | ! now. |
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202 | if (is_cloudy_profile .or. .not. config%do_clear) then |
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203 | do jlev = 1,nlev |
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204 | ! Compute combined gas+aerosol+cloud optical properties; |
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205 | ! note that for clear layers, the reflectance and |
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206 | ! transmittance have already been calculated |
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207 | if (cloud%fraction(jcol,jlev) >= config%cloud_fraction_threshold) then |
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208 | od_cloud_g = od_cloud(config%i_band_from_reordered_g_lw,jlev,jcol) |
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209 | od_total = od(:,jlev,jcol) + od_cloud_g |
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210 | ssa_total = 0.0_jprb |
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211 | g_total = 0.0_jprb |
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212 | |
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213 | if (config%do_lw_cloud_scattering) then |
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214 | ! Scattering case: calculate reflectance and |
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215 | ! transmittance at each model level |
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216 | if (config%do_lw_aerosol_scattering) then |
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217 | where (od_total > 0.0_jprb) |
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218 | ssa_total = (ssa(:,jlev,jcol)*od(:,jlev,jcol) & |
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219 | & + ssa_cloud(config%i_band_from_reordered_g_lw,jlev,jcol) & |
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220 | & * od_cloud_g) & |
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221 | & / od_total |
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222 | end where |
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223 | where (ssa_total > 0.0_jprb .and. od_total > 0.0_jprb) |
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224 | g_total = (g(:,jlev,jcol)*ssa(:,jlev,jcol)*od(:,jlev,jcol) & |
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225 | & + g_cloud(config%i_band_from_reordered_g_lw,jlev,jcol) & |
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226 | & * ssa_cloud(config%i_band_from_reordered_g_lw,jlev,jcol) & |
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227 | & * od_cloud_g) & |
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228 | & / (ssa_total*od_total) |
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229 | end where |
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230 | else |
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231 | where (od_total > 0.0_jprb) |
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232 | ssa_total = ssa_cloud(config%i_band_from_reordered_g_lw,jlev,jcol) & |
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233 | & * od_cloud_g / od_total |
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234 | end where |
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235 | where (ssa_total > 0.0_jprb .and. od_total > 0.0_jprb) |
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236 | g_total = g_cloud(config%i_band_from_reordered_g_lw,jlev,jcol) & |
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237 | & * ssa_cloud(config%i_band_from_reordered_g_lw,jlev,jcol) & |
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238 | & * od_cloud_g / (ssa_total*od_total) |
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239 | end where |
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240 | end if |
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241 | |
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242 | ! Compute cloudy-sky reflectance, transmittance etc at |
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243 | ! each model level |
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244 | call calc_two_stream_gammas_lw(ng, ssa_total, g_total, & |
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245 | & gamma1, gamma2) |
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246 | call calc_reflectance_transmittance_lw(ng, & |
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247 | & od_total, gamma1, gamma2, & |
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248 | & planck_hl(:,jlev,jcol), planck_hl(:,jlev+1,jcol), & |
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249 | & reflectance(:,jlev), transmittance(:,jlev), & |
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250 | & source_up(:,jlev), source_dn(:,jlev)) |
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251 | else |
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252 | ! No-scattering case: use simpler functions for |
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253 | ! transmission and emission |
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254 | call calc_no_scattering_transmittance_lw(ng, od_total, & |
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255 | & planck_hl(:,jlev,jcol), planck_hl(:,jlev+1, jcol), & |
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256 | & transmittance(:,jlev), source_up(:,jlev), source_dn(:,jlev)) |
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257 | end if |
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258 | end if ! is cloudy layer |
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259 | end do |
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260 | |
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261 | if (config%do_lw_cloud_scattering) then |
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262 | ! Use adding method to compute fluxes for an overcast sky |
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263 | call adding_ica_lw(ng, nlev, reflectance, transmittance, source_up, source_dn, & |
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264 | & emission(:,jcol), albedo(:,jcol), & |
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265 | & flux_up, flux_dn) |
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266 | else |
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267 | ! Simpler down-then-up method to compute fluxes |
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268 | call calc_fluxes_no_scattering_lw(ng, nlev, & |
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269 | & transmittance, source_up, source_dn, emission(:,jcol), albedo(:,jcol), & |
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270 | & flux_up, flux_dn) |
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271 | end if |
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272 | |
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273 | ! Store overcast broadband fluxes |
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274 | flux%lw_up(jcol,:) = sum(flux_up,1) |
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275 | flux%lw_dn(jcol,:) = sum(flux_dn,1) |
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276 | ! Store surface spectral downwelling fluxes |
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277 | flux%lw_dn_surf_g(:,jcol) = flux_dn(:,nlev+1) |
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278 | |
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279 | ! Save the spectral fluxes if required |
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280 | if (config%do_save_spectral_flux) then |
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281 | call indexed_sum_profile(flux_up, config%i_spec_from_reordered_g_lw, & |
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282 | & flux%lw_up_band(:,jcol,:)) |
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283 | call indexed_sum_profile(flux_dn, config%i_spec_from_reordered_g_lw, & |
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284 | & flux%lw_dn_band(:,jcol,:)) |
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285 | end if |
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286 | |
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287 | else |
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288 | ! No cloud in profile and clear-sky fluxes already |
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289 | ! calculated: copy them over |
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290 | flux%lw_up(jcol,:) = flux%lw_up_clear(jcol,:) |
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291 | flux%lw_dn(jcol,:) = flux%lw_dn_clear(jcol,:) |
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292 | flux%lw_dn_surf_g(:,jcol) = flux%lw_dn_surf_clear_g(:,jcol) |
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293 | |
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294 | if (config%do_save_spectral_flux) then |
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295 | flux%lw_up_band(:,jcol,:) = flux%lw_up_clear_band(:,jcol,:) |
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296 | flux%lw_dn_band(:,jcol,:) = flux%lw_dn_clear_band(:,jcol,:) |
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297 | end if |
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298 | |
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299 | end if |
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300 | |
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301 | ! Compute the longwave derivatives needed by Hogan and Bozzo |
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302 | ! (2015) approximate radiation update scheme, using clear-sky |
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303 | ! transmittance if no clouds were present in the profile, |
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304 | ! all-sky transmittance otherwise |
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305 | if (config%do_lw_derivatives) then |
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306 | call calc_lw_derivatives_ica(ng, nlev, jcol, transmittance, flux_up(:,nlev+1), & |
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307 | & flux%lw_derivatives) |
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308 | |
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309 | end if |
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310 | |
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311 | end do |
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312 | |
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313 | if (lhook) call dr_hook('radiation_homogeneous_lw:solver_homogeneous_lw',1,hook_handle) |
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314 | |
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315 | end subroutine solver_homogeneous_lw |
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316 | |
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317 | end module radiation_homogeneous_lw |
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