1 | ! radiation_adding_ica_lw.F90 - Longwave adding method in independent column approximation |
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2 | ! |
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3 | ! (C) Copyright 2015- 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 | ! 2017-07-12 R. Hogan Fast adding method for if only clouds scatter |
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18 | ! 2017-10-23 R. Hogan Renamed single-character variables |
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19 | |
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20 | module radiation_adding_ica_lw |
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21 | |
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22 | public |
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23 | |
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24 | contains |
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25 | |
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26 | !--------------------------------------------------------------------- |
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27 | ! Use the scalar "adding" method to compute longwave flux profiles, |
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28 | ! including scattering, by successively adding the contribution of |
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29 | ! layers starting from the surface to compute the total albedo and |
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30 | ! total upward emission of the increasingly larger block of |
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31 | ! atmospheric layers. |
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32 | subroutine adding_ica_lw(ncol, nlev, & |
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33 | & reflectance, transmittance, source_up, source_dn, emission_surf, albedo_surf, & |
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34 | & flux_up, flux_dn) |
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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, jphook |
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38 | |
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39 | implicit none |
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40 | |
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41 | ! Inputs |
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42 | integer, intent(in) :: ncol ! number of columns (may be spectral intervals) |
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43 | integer, intent(in) :: nlev ! number of levels |
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44 | |
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45 | ! Surface emission (W m-2) and albedo |
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46 | real(jprb), intent(in), dimension(ncol) :: emission_surf, albedo_surf |
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47 | |
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48 | ! Diffuse reflectance and transmittance of each layer |
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49 | real(jprb), intent(in), dimension(ncol, nlev) :: reflectance, transmittance |
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50 | |
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51 | ! Emission from each layer in an upward and downward direction |
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52 | real(jprb), intent(in), dimension(ncol, nlev) :: source_up, source_dn |
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53 | |
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54 | ! Resulting fluxes (W m-2) at half-levels: diffuse upwelling and |
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55 | ! downwelling |
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56 | real(jprb), intent(out), dimension(ncol, nlev+1) :: flux_up, flux_dn |
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57 | |
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58 | ! Albedo of the entire earth/atmosphere system below each half |
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59 | ! level |
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60 | real(jprb), dimension(ncol, nlev+1) :: albedo |
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61 | |
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62 | ! Upwelling radiation at each half-level due to emission below |
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63 | ! that half-level (W m-2) |
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64 | real(jprb), dimension(ncol, nlev+1) :: source |
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65 | |
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66 | ! Equal to 1/(1-albedo*reflectance) |
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67 | real(jprb), dimension(ncol, nlev) :: inv_denominator |
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68 | |
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69 | ! Loop index for model level and column |
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70 | integer :: jlev, jcol |
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71 | |
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72 | real(jphook) :: hook_handle |
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73 | |
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74 | if (lhook) call dr_hook('radiation_adding_ica_lw:adding_ica_lw',0,hook_handle) |
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75 | |
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76 | albedo(:,nlev+1) = albedo_surf |
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77 | |
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78 | ! At the surface, the source is thermal emission |
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79 | source(:,nlev+1) = emission_surf |
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80 | |
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81 | ! Work back up through the atmosphere and compute the albedo of |
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82 | ! the entire earth/atmosphere system below that half-level, and |
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83 | ! also the "source", which is the upwelling flux due to emission |
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84 | ! below that level |
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85 | do jlev = nlev,1,-1 |
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86 | ! Next loop over columns. We could do this by indexing the |
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87 | ! entire inner dimension as follows, e.g. for the first line: |
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88 | ! inv_denominator(:,jlev) = 1.0_jprb / (1.0_jprb-albedo(:,jlev+1)*reflectance(:,jlev)) |
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89 | ! and similarly for subsequent lines, but this slows down the |
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90 | ! routine by a factor of 2! Rather, we do it with an explicit |
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91 | ! loop. |
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92 | do jcol = 1,ncol |
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93 | ! Lacis and Hansen (1974) Eq 33, Shonk & Hogan (2008) Eq 10: |
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94 | inv_denominator(jcol,jlev) = 1.0_jprb & |
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95 | & / (1.0_jprb-albedo(jcol,jlev+1)*reflectance(jcol,jlev)) |
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96 | ! Shonk & Hogan (2008) Eq 9, Petty (2006) Eq 13.81: |
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97 | albedo(jcol,jlev) = reflectance(jcol,jlev) + transmittance(jcol,jlev)*transmittance(jcol,jlev) & |
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98 | & * albedo(jcol,jlev+1) * inv_denominator(jcol,jlev) |
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99 | ! Shonk & Hogan (2008) Eq 11: |
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100 | source(jcol,jlev) = source_up(jcol,jlev) & |
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101 | & + transmittance(jcol,jlev) * (source(jcol,jlev+1) & |
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102 | & + albedo(jcol,jlev+1)*source_dn(jcol,jlev)) & |
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103 | & * inv_denominator(jcol,jlev) |
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104 | end do |
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105 | end do |
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106 | |
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107 | ! At top-of-atmosphere there is no diffuse downwelling radiation |
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108 | flux_dn(:,1) = 0.0_jprb |
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109 | |
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110 | ! At top-of-atmosphere, all upwelling radiation is due to emission |
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111 | ! below that level |
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112 | flux_up(:,1) = source(:,1) |
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113 | |
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114 | ! Work back down through the atmosphere computing the fluxes at |
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115 | ! each half-level |
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116 | do jlev = 1,nlev |
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117 | do jcol = 1,ncol |
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118 | ! Shonk & Hogan (2008) Eq 14 (after simplification): |
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119 | flux_dn(jcol,jlev+1) & |
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120 | & = (transmittance(jcol,jlev)*flux_dn(jcol,jlev) & |
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121 | & + reflectance(jcol,jlev)*source(jcol,jlev+1) & |
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122 | & + source_dn(jcol,jlev)) * inv_denominator(jcol,jlev) |
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123 | ! Shonk & Hogan (2008) Eq 12: |
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124 | flux_up(jcol,jlev+1) = albedo(jcol,jlev+1)*flux_dn(jcol,jlev+1) & |
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125 | & + source(jcol,jlev+1) |
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126 | end do |
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127 | end do |
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128 | |
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129 | if (lhook) call dr_hook('radiation_adding_ica_lw:adding_ica_lw',1,hook_handle) |
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130 | |
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131 | end subroutine adding_ica_lw |
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132 | |
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133 | |
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134 | !--------------------------------------------------------------------- |
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135 | ! Use the scalar "adding" method to compute longwave flux profiles, |
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136 | ! including scattering in cloudy layers only. |
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137 | subroutine fast_adding_ica_lw(ncol, nlev, & |
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138 | & reflectance, transmittance, source_up, source_dn, emission_surf, albedo_surf, & |
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139 | & is_clear_sky_layer, i_cloud_top, flux_dn_clear, & |
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140 | & flux_up, flux_dn) |
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141 | |
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142 | use parkind1, only : jprb |
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143 | use yomhook, only : lhook, dr_hook, jphook |
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144 | |
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145 | implicit none |
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146 | |
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147 | ! Inputs |
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148 | integer, intent(in) :: ncol ! number of columns (may be spectral intervals) |
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149 | integer, intent(in) :: nlev ! number of levels |
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150 | |
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151 | ! Surface emission (W m-2) and albedo |
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152 | real(jprb), intent(in), dimension(ncol) :: emission_surf, albedo_surf |
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153 | |
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154 | ! Diffuse reflectance and transmittance of each layer |
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155 | real(jprb), intent(in), dimension(ncol, nlev) :: reflectance, transmittance |
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156 | |
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157 | ! Emission from each layer in an upward and downward direction |
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158 | real(jprb), intent(in), dimension(ncol, nlev) :: source_up, source_dn |
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159 | |
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160 | ! Determine which layers are cloud-free |
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161 | logical, intent(in) :: is_clear_sky_layer(nlev) |
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162 | |
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163 | ! Index to highest cloudy layer |
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164 | integer, intent(in) :: i_cloud_top |
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165 | |
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166 | ! Pre-computed clear-sky downwelling fluxes (W m-2) at half-levels |
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167 | real(jprb), intent(in), dimension(ncol, nlev+1) :: flux_dn_clear |
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168 | |
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169 | ! Resulting fluxes (W m-2) at half-levels: diffuse upwelling and |
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170 | ! downwelling |
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171 | real(jprb), intent(out), dimension(ncol, nlev+1) :: flux_up, flux_dn |
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172 | |
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173 | ! Albedo of the entire earth/atmosphere system below each half |
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174 | ! level |
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175 | real(jprb), dimension(ncol, nlev+1) :: albedo |
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176 | |
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177 | ! Upwelling radiation at each half-level due to emission below |
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178 | ! that half-level (W m-2) |
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179 | real(jprb), dimension(ncol, nlev+1) :: source |
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180 | |
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181 | ! Equal to 1/(1-albedo*reflectance) |
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182 | real(jprb), dimension(ncol, nlev) :: inv_denominator |
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183 | |
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184 | ! Loop index for model level and column |
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185 | integer :: jlev, jcol |
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186 | |
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187 | real(jphook) :: hook_handle |
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188 | |
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189 | if (lhook) call dr_hook('radiation_adding_ica_lw:fast_adding_ica_lw',0,hook_handle) |
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190 | |
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191 | ! Copy over downwelling fluxes above cloud from clear sky |
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192 | flux_dn(:,1:i_cloud_top) = flux_dn_clear(:,1:i_cloud_top) |
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193 | |
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194 | albedo(:,nlev+1) = albedo_surf |
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195 | |
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196 | ! At the surface, the source is thermal emission |
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197 | source(:,nlev+1) = emission_surf |
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198 | |
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199 | ! Work back up through the atmosphere and compute the albedo of |
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200 | ! the entire earth/atmosphere system below that half-level, and |
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201 | ! also the "source", which is the upwelling flux due to emission |
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202 | ! below that level |
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203 | do jlev = nlev,i_cloud_top,-1 |
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204 | if (is_clear_sky_layer(jlev)) then |
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205 | ! Reflectance of this layer is zero, simplifying the expression |
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206 | do jcol = 1,ncol |
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207 | albedo(jcol,jlev) = transmittance(jcol,jlev)*transmittance(jcol,jlev)*albedo(jcol,jlev+1) |
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208 | source(jcol,jlev) = source_up(jcol,jlev) & |
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209 | & + transmittance(jcol,jlev) * (source(jcol,jlev+1) & |
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210 | & + albedo(jcol,jlev+1)*source_dn(jcol,jlev)) |
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211 | end do |
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212 | else |
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213 | ! Loop over columns; explicit loop seems to be faster |
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214 | do jcol = 1,ncol |
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215 | ! Lacis and Hansen (1974) Eq 33, Shonk & Hogan (2008) Eq 10: |
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216 | inv_denominator(jcol,jlev) = 1.0_jprb & |
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217 | & / (1.0_jprb-albedo(jcol,jlev+1)*reflectance(jcol,jlev)) |
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218 | ! Shonk & Hogan (2008) Eq 9, Petty (2006) Eq 13.81: |
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219 | albedo(jcol,jlev) = reflectance(jcol,jlev) + transmittance(jcol,jlev)*transmittance(jcol,jlev) & |
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220 | & * albedo(jcol,jlev+1) * inv_denominator(jcol,jlev) |
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221 | ! Shonk & Hogan (2008) Eq 11: |
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222 | source(jcol,jlev) = source_up(jcol,jlev) & |
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223 | & + transmittance(jcol,jlev) * (source(jcol,jlev+1) & |
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224 | & + albedo(jcol,jlev+1)*source_dn(jcol,jlev)) & |
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225 | & * inv_denominator(jcol,jlev) |
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226 | end do |
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227 | end if |
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228 | end do |
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229 | |
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230 | ! Compute the fluxes above the highest cloud |
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231 | flux_up(:,i_cloud_top) = source(:,i_cloud_top) & |
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232 | & + albedo(:,i_cloud_top)*flux_dn(:,i_cloud_top) |
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233 | do jlev = i_cloud_top-1,1,-1 |
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234 | flux_up(:,jlev) = transmittance(:,jlev)*flux_up(:,jlev+1) + source_up(:,jlev) |
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235 | end do |
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236 | |
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237 | ! Work back down through the atmosphere from cloud top computing |
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238 | ! the fluxes at each half-level |
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239 | do jlev = i_cloud_top,nlev |
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240 | if (is_clear_sky_layer(jlev)) then |
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241 | do jcol = 1,ncol |
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242 | flux_dn(jcol,jlev+1) = transmittance(jcol,jlev)*flux_dn(jcol,jlev) & |
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243 | & + source_dn(jcol,jlev) |
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244 | flux_up(jcol,jlev+1) = albedo(jcol,jlev+1)*flux_dn(jcol,jlev+1) & |
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245 | & + source(jcol,jlev+1) |
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246 | end do |
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247 | else |
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248 | do jcol = 1,ncol |
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249 | ! Shonk & Hogan (2008) Eq 14 (after simplification): |
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250 | flux_dn(jcol,jlev+1) & |
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251 | & = (transmittance(jcol,jlev)*flux_dn(jcol,jlev) & |
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252 | & + reflectance(jcol,jlev)*source(jcol,jlev+1) & |
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253 | & + source_dn(jcol,jlev)) * inv_denominator(jcol,jlev) |
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254 | ! Shonk & Hogan (2008) Eq 12: |
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255 | flux_up(jcol,jlev+1) = albedo(jcol,jlev+1)*flux_dn(jcol,jlev+1) & |
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256 | & + source(jcol,jlev+1) |
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257 | end do |
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258 | end if |
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259 | end do |
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260 | |
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261 | if (lhook) call dr_hook('radiation_adding_ica_lw:fast_adding_ica_lw',1,hook_handle) |
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262 | |
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263 | end subroutine fast_adding_ica_lw |
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264 | |
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265 | |
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266 | !--------------------------------------------------------------------- |
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267 | ! If there is no scattering then fluxes may be computed simply by |
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268 | ! passing down through the atmosphere computing the downwelling |
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269 | ! fluxes from the transmission and emission of each layer, and then |
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270 | ! passing back up through the atmosphere to compute the upwelling |
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271 | ! fluxes in the same way. |
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272 | subroutine calc_fluxes_no_scattering_lw(ncol, nlev, & |
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273 | & transmittance, source_up, source_dn, emission_surf, albedo_surf, flux_up, flux_dn) |
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274 | |
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275 | use parkind1, only : jprb |
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276 | use yomhook, only : lhook, dr_hook, jphook |
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277 | |
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278 | implicit none |
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279 | |
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280 | ! Inputs |
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281 | integer, intent(in) :: ncol ! number of columns (may be spectral intervals) |
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282 | integer, intent(in) :: nlev ! number of levels |
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283 | |
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284 | ! Surface emission (W m-2) and albedo |
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285 | real(jprb), intent(in), dimension(ncol) :: emission_surf, albedo_surf |
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286 | |
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287 | ! Diffuse reflectance and transmittance of each layer |
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288 | real(jprb), intent(in), dimension(ncol, nlev) :: transmittance |
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289 | |
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290 | ! Emission from each layer in an upward and downward direction |
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291 | real(jprb), intent(in), dimension(ncol, nlev) :: source_up, source_dn |
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292 | |
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293 | ! Resulting fluxes (W m-2) at half-levels: diffuse upwelling and |
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294 | ! downwelling |
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295 | real(jprb), intent(out), dimension(ncol, nlev+1) :: flux_up, flux_dn |
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296 | |
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297 | ! Loop index for model level |
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298 | integer :: jlev, jcol |
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299 | |
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300 | real(jphook) :: hook_handle |
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301 | |
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302 | if (lhook) call dr_hook('radiation_adding_ica_lw:calc_fluxes_no_scattering_lw',0,hook_handle) |
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303 | |
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304 | ! At top-of-atmosphere there is no diffuse downwelling radiation |
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305 | flux_dn(:,1) = 0.0_jprb |
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306 | |
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307 | ! Work down through the atmosphere computing the downward fluxes |
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308 | ! at each half-level |
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309 | ! Added for DWD (2020) |
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310 | !NEC$ outerloop_unroll(8) |
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311 | do jlev = 1,nlev |
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312 | do jcol = 1,ncol |
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313 | flux_dn(jcol,jlev+1) = transmittance(jcol,jlev)*flux_dn(jcol,jlev) + source_dn(jcol,jlev) |
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314 | end do |
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315 | end do |
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316 | |
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317 | ! Surface reflection and emission |
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318 | flux_up(:,nlev+1) = emission_surf + albedo_surf * flux_dn(:,nlev+1) |
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319 | |
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320 | ! Work back up through the atmosphere computing the upward fluxes |
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321 | ! at each half-level |
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322 | ! Added for DWD (2020) |
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323 | !NEC$ outerloop_unroll(8) |
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324 | do jlev = nlev,1,-1 |
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325 | do jcol = 1,ncol |
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326 | flux_up(jcol,jlev) = transmittance(jcol,jlev)*flux_up(jcol,jlev+1) + source_up(jcol,jlev) |
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327 | end do |
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328 | end do |
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329 | |
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330 | if (lhook) call dr_hook('radiation_adding_ica_lw:calc_fluxes_no_scattering_lw',1,hook_handle) |
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331 | |
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332 | end subroutine calc_fluxes_no_scattering_lw |
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333 | |
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334 | end module radiation_adding_ica_lw |
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