1 | !> @file calc_radiation_mod.f90 |
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2 | !--------------------------------------------------------------------------------! |
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3 | ! This file is part of PALM. |
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4 | ! |
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5 | ! PALM is free software: you can redistribute it and/or modify it under the terms |
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6 | ! of the GNU General Public License as published by the Free Software Foundation, |
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7 | ! either version 3 of the License, or (at your option) any later version. |
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8 | ! |
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9 | ! PALM is distributed in the hope that it will be useful, but WITHOUT ANY |
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10 | ! WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR |
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11 | ! A PARTICULAR PURPOSE. See the GNU General Public License for more details. |
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12 | ! |
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13 | ! You should have received a copy of the GNU General Public License along with |
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14 | ! PALM. If not, see <http://www.gnu.org/licenses/>. |
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15 | ! |
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16 | ! Copyright 1997-2016 Leibniz Universitaet Hannover |
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17 | !--------------------------------------------------------------------------------! |
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18 | ! |
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19 | ! Current revisions: |
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20 | ! ----------------- |
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21 | ! |
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22 | ! |
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23 | ! Former revisions: |
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24 | ! ----------------- |
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25 | ! $Id: calc_radiation_mod.f90 1851 2016-04-08 13:32:50Z hoffmann $ |
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26 | ! |
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27 | ! 1850 2016-04-08 13:29:27Z maronga |
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28 | ! Module renamed |
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29 | ! |
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30 | ! |
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31 | ! 1682 2015-10-07 23:56:08Z knoop |
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32 | ! Code annotations made doxygen readable |
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33 | ! |
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34 | ! 1353 2014-04-08 15:21:23Z heinze |
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35 | ! REAL constants provided with KIND-attribute |
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36 | ! |
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37 | ! 1322 2014-03-20 16:38:49Z raasch |
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38 | ! exponent 4.0 changed to integer |
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39 | ! |
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40 | ! 1320 2014-03-20 08:40:49Z raasch |
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41 | ! ONLY-attribute added to USE-statements, |
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42 | ! kind-parameters added to all INTEGER and REAL declaration statements, |
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43 | ! kinds are defined in new module kinds, |
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44 | ! revision history before 2012 removed, |
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45 | ! comment fields (!:) to be used for variable explanations added to |
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46 | ! all variable declaration statements |
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47 | ! |
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48 | ! 1036 2012-10-22 13:43:42Z raasch |
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49 | ! code put under GPL (PALM 3.9) |
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50 | ! |
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51 | ! Revision 1.1 2000/04/13 14:42:45 schroeter |
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52 | ! Initial revision |
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53 | ! |
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54 | ! |
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55 | ! Description: |
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56 | ! ------------- |
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57 | !> Calculation of the vertical divergences of the long-wave radiation-fluxes |
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58 | !> based on the parameterization of the cloud effective emissivity |
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59 | !------------------------------------------------------------------------------! |
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60 | MODULE calc_radiation_mod |
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61 | |
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62 | USE kinds |
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63 | |
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64 | PRIVATE |
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65 | PUBLIC calc_radiation |
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66 | |
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67 | LOGICAL, SAVE :: first_call = .TRUE. !< |
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68 | REAL(wp), SAVE :: sigma = 5.67E-08_wp !< |
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69 | |
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70 | REAL(wp), DIMENSION(:), ALLOCATABLE, SAVE :: lwp_ground !< |
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71 | REAL(wp), DIMENSION(:), ALLOCATABLE, SAVE :: lwp_top !< |
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72 | REAL(wp), DIMENSION(:), ALLOCATABLE, SAVE :: blackbody_emission !< |
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73 | |
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74 | INTERFACE calc_radiation |
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75 | MODULE PROCEDURE calc_radiation |
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76 | MODULE PROCEDURE calc_radiation_ij |
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77 | END INTERFACE calc_radiation |
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78 | |
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79 | CONTAINS |
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80 | |
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81 | |
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82 | !------------------------------------------------------------------------------! |
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83 | ! Description: |
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84 | ! ------------ |
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85 | !> Call for all grid points |
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86 | !------------------------------------------------------------------------------! |
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87 | SUBROUTINE calc_radiation |
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88 | |
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89 | USE arrays_3d, & |
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90 | ONLY: dzw, pt, ql, tend |
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91 | |
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92 | USE cloud_parameters, & |
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93 | ONLY: cp, l_d_cp, pt_d_t, t_d_pt |
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94 | |
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95 | USE control_parameters, & |
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96 | ONLY: rho_surface |
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97 | |
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98 | USE indices, & |
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99 | ONLY: nxl, nxr, nyn, nys, nzb, nzb_s_inner, nzt |
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100 | |
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101 | USE kinds |
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102 | |
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103 | USE pegrid |
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104 | |
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105 | |
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106 | IMPLICIT NONE |
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107 | |
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108 | INTEGER(iwp) :: i !< |
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109 | INTEGER(iwp) :: j !< |
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110 | INTEGER(iwp) :: k !< |
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111 | INTEGER(iwp) :: k_help !< |
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112 | |
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113 | REAL(wp) :: df_p !< |
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114 | REAL(wp) :: df_m !< |
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115 | REAL(wp) :: effective_emission_up_m !< |
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116 | REAL(wp) :: effective_emission_up_p !< |
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117 | REAL(wp) :: effective_emission_down_m !< |
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118 | REAL(wp) :: effective_emission_down_p !< |
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119 | REAL(wp) :: f_up_m !< |
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120 | REAL(wp) :: f_up_p !< |
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121 | REAL(wp) :: f_down_m !< |
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122 | REAL(wp) :: f_down_p !< |
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123 | REAL(wp) :: impinging_flux_at_top !< |
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124 | REAL(wp) :: temperature !< |
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125 | |
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126 | |
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127 | ! |
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128 | !-- On first call, allocate temporary arrays |
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129 | IF ( first_call ) THEN |
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130 | ALLOCATE( blackbody_emission(nzb:nzt+1), lwp_ground(nzb:nzt+1), & |
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131 | lwp_top(nzb:nzt+1) ) |
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132 | first_call = .FALSE. |
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133 | ENDIF |
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134 | |
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135 | |
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136 | DO i = nxl, nxr |
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137 | DO j = nys, nyn |
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138 | ! |
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139 | !-- Compute the liquid water path (LWP) and blackbody_emission |
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140 | !-- at all vertical levels |
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141 | lwp_ground(nzb) = 0.0_wp |
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142 | lwp_top(nzt+1) = rho_surface * ql(nzt+1,j,i) * dzw(nzt+1) |
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143 | |
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144 | temperature = pt(nzb,j,i) * t_d_pt(nzb) + l_d_cp * ql(nzb,j,i) |
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145 | blackbody_emission(nzb) = sigma * temperature**4 |
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146 | |
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147 | DO k = nzb_s_inner(j,i)+1, nzt |
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148 | |
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149 | k_help = ( nzt+nzb+1 ) - k |
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150 | lwp_ground(k) = lwp_ground(k-1) + rho_surface * ql(k,j,i) * & |
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151 | dzw(k) |
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152 | |
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153 | lwp_top(k_help) = lwp_top(k_help+1) + & |
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154 | rho_surface * ql(k_help,j,i) * dzw(k_help) |
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155 | |
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156 | temperature = pt(k,j,i) * t_d_pt(k) + l_d_cp * ql(k,j,i) |
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157 | blackbody_emission(k) = sigma * temperature**4 |
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158 | |
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159 | ENDDO |
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160 | |
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161 | lwp_ground(nzt+1) = lwp_ground(nzt) + & |
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162 | rho_surface * ql(nzt+1,j,i) * dzw(nzt+1) |
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163 | lwp_top(nzb) = lwp_top(nzb+1) |
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164 | |
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165 | temperature = pt(nzt+1,j,i) * t_d_pt(nzt+1) + l_d_cp * & |
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166 | ql(nzt+1,j,i) |
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167 | blackbody_emission(nzt+1) = sigma * temperature**4 |
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168 | |
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169 | ! |
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170 | !-- See Chlond '92, this is just a first guess |
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171 | impinging_flux_at_top = blackbody_emission(nzb) - 100.0_wp |
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172 | |
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173 | DO k = nzb_s_inner(j,i)+1, nzt |
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174 | ! |
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175 | !-- Save some computational time, but this may cause load |
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176 | !-- imbalances if ql is not distributed uniformly |
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177 | IF ( ql(k,j,i) /= 0.0_wp ) THEN |
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178 | ! |
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179 | !-- Compute effective emissivities |
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180 | effective_emission_up_p = 1.0_wp - & |
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181 | EXP( -130.0_wp * lwp_ground(k+1) ) |
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182 | effective_emission_up_m = 1.0_wp - & |
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183 | EXP( -130.0_wp * lwp_ground(k-1) ) |
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184 | effective_emission_down_p = 1.0_wp - & |
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185 | EXP( -158.0_wp * lwp_top(k+1) ) |
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186 | effective_emission_down_m = 1.0_wp - & |
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187 | EXP( -158.0_wp * lwp_top(k-1) ) |
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188 | |
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189 | ! |
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190 | !-- Compute vertical long wave radiation fluxes |
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191 | f_up_p = blackbody_emission(nzb) + & |
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192 | effective_emission_up_p * & |
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193 | ( blackbody_emission(k) - blackbody_emission(nzb) ) |
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194 | |
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195 | f_up_m = blackbody_emission(nzb) + & |
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196 | effective_emission_up_m * & |
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197 | ( blackbody_emission(k-1) - blackbody_emission(nzb) ) |
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198 | |
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199 | f_down_p = impinging_flux_at_top + & |
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200 | effective_emission_down_p * & |
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201 | ( blackbody_emission(k) - impinging_flux_at_top ) |
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202 | |
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203 | f_down_m = impinging_flux_at_top + & |
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204 | effective_emission_down_m * & |
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205 | ( blackbody_emission(k-1) - impinging_flux_at_top ) |
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206 | |
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207 | ! |
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208 | !-- Divergence of vertical long wave radiation fluxes |
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209 | df_p = f_up_p - f_down_p |
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210 | df_m = f_up_m - f_down_m |
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211 | |
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212 | ! |
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213 | !-- Compute tendency term |
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214 | tend(k,j,i) = tend(k,j,i) - & |
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215 | ( pt_d_t(k) / ( rho_surface * cp ) * & |
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216 | ( df_p - df_m ) / dzw(k) ) |
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217 | |
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218 | ENDIF |
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219 | |
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220 | ENDDO |
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221 | ENDDO |
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222 | ENDDO |
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223 | |
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224 | END SUBROUTINE calc_radiation |
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225 | |
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226 | |
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227 | !------------------------------------------------------------------------------! |
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228 | ! Description: |
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229 | ! ------------ |
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230 | !> Call for grid point i,j |
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231 | !------------------------------------------------------------------------------! |
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232 | SUBROUTINE calc_radiation_ij( i, j ) |
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233 | |
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234 | USE arrays_3d, & |
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235 | ONLY: dzw, pt, ql, tend |
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236 | |
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237 | USE cloud_parameters, & |
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238 | ONLY: cp, l_d_cp, pt_d_t, t_d_pt |
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239 | |
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240 | USE control_parameters, & |
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241 | ONLY: rho_surface |
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242 | |
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243 | USE indices, & |
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244 | ONLY: nzb, nzb_s_inner, nzt |
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245 | |
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246 | USE kinds |
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247 | |
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248 | USE pegrid |
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249 | |
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250 | |
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251 | IMPLICIT NONE |
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252 | |
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253 | INTEGER(iwp) :: i !< |
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254 | INTEGER(iwp) :: j !< |
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255 | INTEGER(iwp) :: k !< |
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256 | INTEGER(iwp) :: k_help !< |
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257 | |
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258 | REAL(wp) :: df_p !< |
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259 | REAL(wp) :: df_m !< |
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260 | REAL(wp) :: effective_emission_up_m !< |
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261 | REAL(wp) :: effective_emission_up_p !< |
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262 | REAL(wp) :: effective_emission_down_m !< |
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263 | REAL(wp) :: effective_emission_down_p !< |
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264 | REAL(wp) :: f_up_m !< |
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265 | REAL(wp) :: f_up_p !< |
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266 | REAL(wp) :: f_down_m !< |
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267 | REAL(wp) :: f_down_p !< |
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268 | REAL(wp) :: impinging_flux_at_top !< |
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269 | REAL(wp) :: temperature !< |
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270 | |
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271 | |
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272 | ! |
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273 | !-- On first call, allocate temporary arrays |
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274 | IF ( first_call ) THEN |
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275 | ALLOCATE( blackbody_emission(nzb:nzt+1), lwp_ground(nzb:nzt+1), & |
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276 | lwp_top(nzb:nzt+1) ) |
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277 | first_call = .FALSE. |
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278 | ENDIF |
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279 | |
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280 | ! |
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281 | !-- Compute the liquid water path (LWP) and blackbody_emission |
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282 | !-- at all vertical levels |
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283 | lwp_ground(nzb) = 0.0_wp |
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284 | lwp_top(nzt+1) = rho_surface * ql(nzt+1,j,i) * dzw(nzt+1) |
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285 | |
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286 | temperature = pt(nzb,j,i) * t_d_pt(nzb) + l_d_cp * ql(nzb,j,i) |
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287 | blackbody_emission(nzb) = sigma * temperature**4 |
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288 | |
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289 | DO k = nzb_s_inner(j,i)+1, nzt |
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290 | k_help = ( nzt+nzb+1 ) - k |
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291 | lwp_ground(k) = lwp_ground(k-1) + rho_surface * ql(k,j,i) * dzw(k) |
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292 | |
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293 | lwp_top(k_help) = lwp_top(k_help+1) + & |
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294 | rho_surface * ql(k_help,j,i) * dzw(k_help) |
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295 | |
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296 | temperature = pt(k,j,i) * t_d_pt(k) + l_d_cp * ql(k,j,i) |
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297 | blackbody_emission(k) = sigma * temperature**4 |
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298 | |
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299 | ENDDO |
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300 | lwp_ground(nzt+1) = lwp_ground(nzt) + & |
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301 | rho_surface * ql(nzt+1,j,i) * dzw(nzt+1) |
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302 | lwp_top(nzb) = lwp_top(nzb+1) |
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303 | |
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304 | temperature = pt(nzt+1,j,i) * t_d_pt(nzt+1) + l_d_cp * & |
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305 | ql(nzt+1,j,i) |
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306 | blackbody_emission(nzt+1) = sigma * temperature**4 |
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307 | |
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308 | ! |
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309 | !-- See Chlond '92, this is just a first guess |
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310 | impinging_flux_at_top = blackbody_emission(nzb) - 100.0_wp |
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311 | |
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312 | DO k = nzb_s_inner(j,i)+1, nzt |
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313 | ! |
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314 | !-- Store some computational time, |
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315 | !-- this may cause load imbalances if ql is not distributed uniformly |
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316 | IF ( ql(k,j,i) /= 0.0_wp ) THEN |
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317 | ! |
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318 | !-- Compute effective emissivities |
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319 | effective_emission_up_p = 1.0_wp - & |
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320 | EXP( -130.0_wp * lwp_ground(k+1) ) |
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321 | effective_emission_up_m = 1.0_wp - & |
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322 | EXP( -130.0_wp * lwp_ground(k-1) ) |
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323 | effective_emission_down_p = 1.0_wp - & |
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324 | EXP( -158.0_wp * lwp_top(k+1) ) |
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325 | effective_emission_down_m = 1.0_wp - & |
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326 | EXP( -158.0_wp * lwp_top(k-1) ) |
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327 | |
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328 | ! |
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329 | !-- Compute vertical long wave radiation fluxes |
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330 | f_up_p = blackbody_emission(nzb) + effective_emission_up_p * & |
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331 | ( blackbody_emission(k) - blackbody_emission(nzb) ) |
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332 | |
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333 | f_up_m = blackbody_emission(nzb) + effective_emission_up_m * & |
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334 | ( blackbody_emission(k-1) - blackbody_emission(nzb) ) |
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335 | |
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336 | f_down_p = impinging_flux_at_top + effective_emission_down_p * & |
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337 | ( blackbody_emission(k) - impinging_flux_at_top ) |
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338 | |
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339 | f_down_m = impinging_flux_at_top + effective_emission_down_m * & |
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340 | ( blackbody_emission(k-1) - impinging_flux_at_top ) |
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341 | |
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342 | ! |
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343 | !- Divergence of vertical long wave radiation fluxes |
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344 | df_p = f_up_p - f_down_p |
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345 | df_m = f_up_m - f_down_m |
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346 | |
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347 | ! |
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348 | !-- Compute tendency term |
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349 | tend(k,j,i) = tend(k,j,i) - ( pt_d_t(k) / ( rho_surface * cp ) * & |
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350 | ( df_p - df_m ) / dzw(k) ) |
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351 | |
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352 | ENDIF |
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353 | |
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354 | ENDDO |
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355 | |
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356 | END SUBROUTINE calc_radiation_ij |
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357 | |
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358 | END MODULE calc_radiation_mod |
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