1 | MODULE microphysics_mod |
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2 | |
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3 | !--------------------------------------------------------------------------------! |
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4 | ! This file is part of PALM. |
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5 | ! |
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6 | ! PALM is free software: you can redistribute it and/or modify it under the terms |
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7 | ! of the GNU General Public License as published by the Free Software Foundation, |
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8 | ! either version 3 of the License, or (at your option) any later version. |
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9 | ! |
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10 | ! PALM is distributed in the hope that it will be useful, but WITHOUT ANY |
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11 | ! WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR |
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12 | ! A PARTICULAR PURPOSE. See the GNU General Public License for more details. |
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13 | ! |
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14 | ! You should have received a copy of the GNU General Public License along with |
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15 | ! PALM. If not, see <http://www.gnu.org/licenses/>. |
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16 | ! |
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17 | ! Copyright 1997-2012 Leibniz University Hannover |
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18 | !--------------------------------------------------------------------------------! |
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19 | ! |
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20 | ! Current revisions: |
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21 | ! ------------------ |
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22 | ! |
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23 | ! |
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24 | ! Former revisions: |
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25 | ! ----------------- |
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26 | ! $Id: microphysics.f90 1116 2013-03-26 18:49:55Z witha $ |
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27 | ! |
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28 | ! 1115 2013-03-26 18:16:16Z hoffmann |
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29 | ! microphyical tendencies are calculated in microphysics_control in an optimized |
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30 | ! way; unrealistic values are prevented; bugfix in evaporation; some reformatting |
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31 | ! |
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32 | ! 1106 2013-03-04 05:31:38Z raasch |
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33 | ! small changes in code formatting |
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34 | ! |
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35 | ! 1092 2013-02-02 11:24:22Z raasch |
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36 | ! unused variables removed |
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37 | ! file put under GPL |
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38 | ! |
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39 | ! 1065 2012-11-22 17:42:36Z hoffmann |
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40 | ! Sedimentation process implemented according to Stevens and Seifert (2008). |
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41 | ! Turbulence effects on autoconversion and accretion added (Seifert, Nuijens |
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42 | ! and Stevens, 2010). |
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43 | ! |
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44 | ! 1053 2012-11-13 17:11:03Z hoffmann |
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45 | ! initial revision |
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46 | ! |
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47 | ! Description: |
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48 | ! ------------ |
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49 | ! Calculate cloud microphysics according to the two moment bulk |
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50 | ! scheme by Seifert and Beheng (2006). |
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51 | !------------------------------------------------------------------------------! |
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52 | |
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53 | PRIVATE |
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54 | PUBLIC microphysics_control |
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55 | |
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56 | INTERFACE microphysics_control |
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57 | MODULE PROCEDURE microphysics_control |
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58 | MODULE PROCEDURE microphysics_control_ij |
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59 | END INTERFACE microphysics_control |
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60 | |
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61 | INTERFACE adjust_cloud |
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62 | MODULE PROCEDURE adjust_cloud |
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63 | MODULE PROCEDURE adjust_cloud_ij |
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64 | END INTERFACE adjust_cloud |
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65 | |
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66 | INTERFACE autoconversion |
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67 | MODULE PROCEDURE autoconversion |
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68 | MODULE PROCEDURE autoconversion_ij |
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69 | END INTERFACE autoconversion |
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70 | |
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71 | INTERFACE accretion |
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72 | MODULE PROCEDURE accretion |
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73 | MODULE PROCEDURE accretion_ij |
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74 | END INTERFACE accretion |
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75 | |
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76 | INTERFACE selfcollection_breakup |
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77 | MODULE PROCEDURE selfcollection_breakup |
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78 | MODULE PROCEDURE selfcollection_breakup_ij |
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79 | END INTERFACE selfcollection_breakup |
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80 | |
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81 | INTERFACE evaporation_rain |
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82 | MODULE PROCEDURE evaporation_rain |
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83 | MODULE PROCEDURE evaporation_rain_ij |
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84 | END INTERFACE evaporation_rain |
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85 | |
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86 | INTERFACE sedimentation_cloud |
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87 | MODULE PROCEDURE sedimentation_cloud |
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88 | MODULE PROCEDURE sedimentation_cloud_ij |
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89 | END INTERFACE sedimentation_cloud |
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90 | |
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91 | INTERFACE sedimentation_rain |
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92 | MODULE PROCEDURE sedimentation_rain |
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93 | MODULE PROCEDURE sedimentation_rain_ij |
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94 | END INTERFACE sedimentation_rain |
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95 | |
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96 | CONTAINS |
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97 | |
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98 | |
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99 | !------------------------------------------------------------------------------! |
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100 | ! Call for all grid points |
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101 | !------------------------------------------------------------------------------! |
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102 | SUBROUTINE microphysics_control |
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103 | |
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104 | USE arrays_3d |
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105 | USE control_parameters |
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106 | USE indices |
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107 | USE statistics |
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108 | |
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109 | IMPLICIT NONE |
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110 | |
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111 | INTEGER :: i, j, k |
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112 | |
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113 | |
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114 | DO i = nxl, nxr |
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115 | DO j = nys, nyn |
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116 | DO k = nzb_s_inner(j,i)+1, nzt |
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117 | |
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118 | ENDDO |
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119 | ENDDO |
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120 | ENDDO |
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121 | |
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122 | END SUBROUTINE microphysics_control |
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123 | |
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124 | SUBROUTINE adjust_cloud |
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125 | |
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126 | USE arrays_3d |
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127 | USE cloud_parameters |
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128 | USE indices |
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129 | |
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130 | IMPLICIT NONE |
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131 | |
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132 | INTEGER :: i, j, k |
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133 | |
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134 | |
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135 | DO i = nxl, nxr |
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136 | DO j = nys, nyn |
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137 | DO k = nzb_s_inner(j,i)+1, nzt |
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138 | |
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139 | ENDDO |
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140 | ENDDO |
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141 | ENDDO |
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142 | |
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143 | END SUBROUTINE adjust_cloud |
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144 | |
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145 | |
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146 | SUBROUTINE autoconversion |
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147 | |
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148 | USE arrays_3d |
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149 | USE cloud_parameters |
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150 | USE control_parameters |
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151 | USE grid_variables |
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152 | USE indices |
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153 | |
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154 | IMPLICIT NONE |
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155 | |
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156 | INTEGER :: i, j, k |
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157 | |
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158 | |
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159 | DO i = nxl, nxr |
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160 | DO j = nys, nyn |
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161 | DO k = nzb_s_inner(j,i)+1, nzt |
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162 | |
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163 | ENDDO |
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164 | ENDDO |
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165 | ENDDO |
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166 | |
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167 | END SUBROUTINE autoconversion |
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168 | |
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169 | |
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170 | SUBROUTINE accretion |
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171 | |
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172 | USE arrays_3d |
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173 | USE cloud_parameters |
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174 | USE control_parameters |
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175 | USE indices |
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176 | |
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177 | IMPLICIT NONE |
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178 | |
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179 | INTEGER :: i, j, k |
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180 | |
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181 | |
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182 | DO i = nxl, nxr |
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183 | DO j = nys, nyn |
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184 | DO k = nzb_s_inner(j,i)+1, nzt |
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185 | |
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186 | ENDDO |
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187 | ENDDO |
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188 | ENDDO |
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189 | |
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190 | END SUBROUTINE accretion |
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191 | |
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192 | |
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193 | SUBROUTINE selfcollection_breakup |
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194 | |
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195 | USE arrays_3d |
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196 | USE cloud_parameters |
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197 | USE control_parameters |
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198 | USE indices |
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199 | |
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200 | IMPLICIT NONE |
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201 | |
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202 | INTEGER :: i, j, k |
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203 | |
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204 | |
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205 | DO i = nxl, nxr |
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206 | DO j = nys, nyn |
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207 | DO k = nzb_s_inner(j,i)+1, nzt |
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208 | |
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209 | ENDDO |
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210 | ENDDO |
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211 | ENDDO |
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212 | |
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213 | END SUBROUTINE selfcollection_breakup |
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214 | |
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215 | |
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216 | SUBROUTINE evaporation_rain |
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217 | |
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218 | USE arrays_3d |
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219 | USE cloud_parameters |
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220 | USE constants |
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221 | USE control_parameters |
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222 | USE indices |
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223 | |
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224 | IMPLICIT NONE |
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225 | |
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226 | INTEGER :: i, j, k |
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227 | |
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228 | |
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229 | DO i = nxl, nxr |
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230 | DO j = nys, nyn |
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231 | DO k = nzb_s_inner(j,i)+1, nzt |
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232 | |
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233 | ENDDO |
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234 | ENDDO |
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235 | ENDDO |
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236 | |
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237 | END SUBROUTINE evaporation_rain |
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238 | |
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239 | |
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240 | SUBROUTINE sedimentation_cloud |
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241 | |
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242 | USE arrays_3d |
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243 | USE cloud_parameters |
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244 | USE constants |
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245 | USE control_parameters |
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246 | USE indices |
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247 | |
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248 | IMPLICIT NONE |
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249 | |
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250 | INTEGER :: i, j, k |
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251 | |
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252 | |
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253 | DO i = nxl, nxr |
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254 | DO j = nys, nyn |
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255 | DO k = nzb_s_inner(j,i)+1, nzt |
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256 | |
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257 | ENDDO |
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258 | ENDDO |
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259 | ENDDO |
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260 | |
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261 | END SUBROUTINE sedimentation_cloud |
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262 | |
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263 | |
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264 | SUBROUTINE sedimentation_rain |
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265 | |
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266 | USE arrays_3d |
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267 | USE cloud_parameters |
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268 | USE constants |
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269 | USE control_parameters |
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270 | USE indices |
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271 | USE statistics |
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272 | |
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273 | IMPLICIT NONE |
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274 | |
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275 | INTEGER :: i, j, k |
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276 | |
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277 | |
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278 | DO i = nxl, nxr |
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279 | DO j = nys, nyn |
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280 | DO k = nzb_s_inner(j,i)+1, nzt |
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281 | |
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282 | ENDDO |
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283 | ENDDO |
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284 | ENDDO |
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285 | |
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286 | END SUBROUTINE sedimentation_rain |
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287 | |
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288 | |
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289 | !------------------------------------------------------------------------------! |
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290 | ! Call for grid point i,j |
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291 | !------------------------------------------------------------------------------! |
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292 | |
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293 | SUBROUTINE microphysics_control_ij( i, j ) |
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294 | |
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295 | USE arrays_3d |
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296 | USE cloud_parameters |
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297 | USE control_parameters |
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298 | USE statistics |
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299 | |
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300 | IMPLICIT NONE |
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301 | |
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302 | INTEGER :: i, j |
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303 | |
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304 | dt_micro = dt_3d * weight_pres(intermediate_timestep_count) |
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305 | ! |
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306 | !-- Adjust unrealistic values |
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307 | IF ( precipitation ) CALL adjust_cloud( i,j ) |
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308 | ! |
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309 | !-- Use 1-d arrays |
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310 | q_1d(:) = q(:,j,i) |
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311 | pt_1d(:) = pt(:,j,i) |
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312 | qc_1d(:) = qc(:,j,i) |
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313 | nc_1d(:) = nc_const |
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314 | IF ( precipitation ) THEN |
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315 | qr_1d(:) = qr(:,j,i) |
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316 | nr_1d(:) = nr(:,j,i) |
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317 | ENDIF |
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318 | ! |
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319 | !-- Compute cloud physics |
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320 | IF ( precipitation ) THEN |
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321 | CALL autoconversion( i,j ) |
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322 | CALL accretion( i,j ) |
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323 | CALL selfcollection_breakup( i,j ) |
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324 | CALL evaporation_rain( i,j ) |
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325 | CALL sedimentation_rain( i,j ) |
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326 | ENDIF |
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327 | |
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328 | IF ( drizzle ) CALL sedimentation_cloud( i,j ) |
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329 | ! |
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330 | !-- Derive tendencies |
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331 | tend_q(:,j,i) = ( q_1d(:) - q(:,j,i) ) / dt_micro |
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332 | tend_pt(:,j,i) = ( pt_1d(:) - pt(:,j,i) ) / dt_micro |
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333 | IF ( precipitation ) THEN |
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334 | tend_qr(:,j,i) = ( qr_1d(:) - qr(:,j,i) ) / dt_micro |
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335 | tend_nr(:,j,i) = ( nr_1d(:) - nr(:,j,i) ) / dt_micro |
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336 | ENDIF |
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337 | |
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338 | END SUBROUTINE microphysics_control_ij |
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339 | |
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340 | SUBROUTINE adjust_cloud_ij( i, j ) |
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341 | |
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342 | USE arrays_3d |
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343 | USE cloud_parameters |
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344 | USE indices |
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345 | |
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346 | IMPLICIT NONE |
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347 | |
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348 | INTEGER :: i, j, k |
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349 | ! |
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350 | !-- Adjust number of raindrops to avoid nonlinear effects in |
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351 | !-- sedimentation and evaporation of rain drops due to too small or |
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352 | !-- too big weights of rain drops (Stevens and Seifert, 2008). |
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353 | !-- The same procedure is applied to cloud droplets if they are determined |
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354 | !-- prognostically. |
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355 | DO k = nzb_s_inner(j,i)+1, nzt |
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356 | |
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357 | IF ( qr(k,j,i) <= eps_sb ) THEN |
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358 | qr(k,j,i) = 0.0 |
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359 | nr(k,j,i) = 0.0 |
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360 | ELSE |
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361 | ! |
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362 | !-- Adjust number of raindrops to avoid nonlinear effects in |
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363 | !-- sedimentation and evaporation of rain drops due to too small or |
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364 | !-- too big weights of rain drops (Stevens and Seifert, 2008). |
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365 | IF ( nr(k,j,i) * xrmin > qr(k,j,i) * hyrho(k) ) THEN |
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366 | nr(k,j,i) = qr(k,j,i) * hyrho(k) / xrmin |
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367 | ELSEIF ( nr(k,j,i) * xrmax < qr(k,j,i) * hyrho(k) ) THEN |
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368 | nr(k,j,i) = qr(k,j,i) * hyrho(k) / xrmax |
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369 | ENDIF |
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370 | |
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371 | ENDIF |
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372 | |
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373 | ENDDO |
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374 | |
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375 | END SUBROUTINE adjust_cloud_ij |
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376 | |
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377 | |
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378 | SUBROUTINE autoconversion_ij( i, j ) |
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379 | |
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380 | USE arrays_3d |
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381 | USE cloud_parameters |
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382 | USE control_parameters |
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383 | USE grid_variables |
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384 | USE indices |
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385 | |
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386 | IMPLICIT NONE |
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387 | |
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388 | INTEGER :: i, j, k |
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389 | REAL :: alpha_cc, autocon, epsilon, k_au, l_mix, nu_c, phi_au, & |
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390 | r_cc, rc, re_lambda, selfcoll, sigma_cc, tau_cloud, xc |
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391 | |
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392 | |
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393 | k_au = k_cc / ( 20.0 * x0 ) |
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394 | |
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395 | DO k = nzb_s_inner(j,i)+1, nzt |
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396 | |
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397 | IF ( qc_1d(k) > eps_sb ) THEN |
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398 | ! |
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399 | !-- Intern time scale of coagulation (Seifert and Beheng, 2006): |
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400 | !-- (1.0 - qc(k,j,i) / ( qc(k,j,i) + qr_1d(k) )) |
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401 | tau_cloud = 1.0 - qc_1d(k) / ( qr_1d(k) + qc_1d(k) ) |
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402 | ! |
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403 | !-- Universal function for autoconversion process |
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404 | !-- (Seifert and Beheng, 2006): |
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405 | phi_au = 600.0 * tau_cloud**0.68 * ( 1.0 - tau_cloud**0.68 )**3 |
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406 | ! |
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407 | !-- Shape parameter of gamma distribution (Geoffroy et al., 2010): |
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408 | !-- (Use constant nu_c = 1.0 instead?) |
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409 | nu_c = 1.0 !MAX( 0.0, 1580.0 * hyrho(k) * qc(k,j,i) - 0.28 ) |
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410 | ! |
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411 | !-- Mean weight of cloud droplets: |
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412 | xc = hyrho(k) * qc_1d(k) / nc_1d(k) |
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413 | ! |
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414 | !-- Parameterized turbulence effects on autoconversion (Seifert, |
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415 | !-- Nuijens and Stevens, 2010) |
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416 | IF ( turbulence ) THEN |
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417 | ! |
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418 | !-- Weight averaged radius of cloud droplets: |
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419 | rc = 0.5 * ( xc * dpirho_l )**( 1.0 / 3.0 ) |
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420 | |
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421 | alpha_cc = ( a_1 + a_2 * nu_c ) / ( 1.0 + a_3 * nu_c ) |
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422 | r_cc = ( b_1 + b_2 * nu_c ) / ( 1.0 + b_3 * nu_c ) |
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423 | sigma_cc = ( c_1 + c_2 * nu_c ) / ( 1.0 + c_3 * nu_c ) |
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424 | ! |
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425 | !-- Mixing length (neglecting distance to ground and stratification) |
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426 | l_mix = ( dx * dy * dzu(k) )**( 1.0 / 3.0 ) |
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427 | ! |
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428 | !-- Limit dissipation rate according to Seifert, Nuijens and |
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429 | !-- Stevens (2010) |
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430 | epsilon = MIN( 0.06, diss(k,j,i) ) |
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431 | ! |
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432 | !-- Compute Taylor-microscale Reynolds number: |
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433 | re_lambda = 6.0 / 11.0 * ( l_mix / c_const )**( 2.0 / 3.0 ) * & |
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434 | SQRT( 15.0 / kin_vis_air ) * epsilon**( 1.0 / 6.0 ) |
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435 | ! |
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436 | !-- The factor of 1.0E4 is needed to convert the dissipation rate |
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437 | !-- from m2 s-3 to cm2 s-3. |
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438 | k_au = k_au * ( 1.0 + & |
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439 | epsilon * 1.0E4 * ( re_lambda * 1.0E-3 )**0.25 * & |
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440 | ( alpha_cc * EXP( -1.0 * ( ( rc - r_cc ) / & |
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441 | sigma_cc )**2 ) + beta_cc ) ) |
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442 | ENDIF |
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443 | ! |
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444 | !-- Autoconversion rate (Seifert and Beheng, 2006): |
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445 | autocon = k_au * ( nu_c + 2.0 ) * ( nu_c + 4.0 ) / & |
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446 | ( nu_c + 1.0 )**2 * qc_1d(k)**2 * xc**2 * & |
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447 | ( 1.0 + phi_au / ( 1.0 - tau_cloud )**2 ) * & |
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448 | rho_surface |
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449 | autocon = MIN( autocon, qc_1d(k) / dt_micro ) |
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450 | |
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451 | qr_1d(k) = qr_1d(k) + autocon * dt_micro |
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452 | qc_1d(k) = qc_1d(k) - autocon * dt_micro |
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453 | nr_1d(k) = nr_1d(k) + autocon / x0 * hyrho(k) * dt_micro |
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454 | |
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455 | ENDIF |
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456 | |
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457 | ENDDO |
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458 | |
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459 | END SUBROUTINE autoconversion_ij |
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460 | |
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461 | |
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462 | SUBROUTINE accretion_ij( i, j ) |
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463 | |
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464 | USE arrays_3d |
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465 | USE cloud_parameters |
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466 | USE control_parameters |
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467 | USE indices |
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468 | |
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469 | IMPLICIT NONE |
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470 | |
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471 | INTEGER :: i, j, k |
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472 | REAL :: accr, k_cr, phi_ac, tau_cloud, xc |
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473 | |
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474 | DO k = nzb_s_inner(j,i)+1, nzt |
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475 | IF ( ( qc_1d(k) > eps_sb ) .AND. ( qr_1d(k) > eps_sb ) ) THEN |
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476 | ! |
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477 | !-- Intern time scale of coagulation (Seifert and Beheng, 2006): |
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478 | tau_cloud = 1.0 - qc_1d(k) / ( qc_1d(k) + qr_1d(k) ) |
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479 | ! |
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480 | !-- Universal function for accretion process |
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481 | !-- (Seifert and Beheng, 2001): |
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482 | phi_ac = tau_cloud / ( tau_cloud + 5.0E-5 ) |
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483 | phi_ac = ( phi_ac**2 )**2 |
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484 | ! |
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485 | !-- Parameterized turbulence effects on autoconversion (Seifert, |
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486 | !-- Nuijens and Stevens, 2010). The factor of 1.0E4 is needed to |
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487 | !-- convert the dissipation (diss) from m2 s-3 to cm2 s-3. |
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488 | IF ( turbulence ) THEN |
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489 | k_cr = k_cr0 * ( 1.0 + 0.05 * & |
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490 | MIN( 600.0, diss(k,j,i) * 1.0E4 )**0.25 ) |
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491 | ELSE |
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492 | k_cr = k_cr0 |
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493 | ENDIF |
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494 | ! |
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495 | !-- Accretion rate (Seifert and Beheng, 2006): |
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496 | accr = k_cr * qc_1d(k) * qr_1d(k) * phi_ac * & |
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497 | SQRT( rho_surface * hyrho(k) ) |
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498 | accr = MIN( accr, qc_1d(k) / dt_micro ) |
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499 | |
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500 | qr_1d(k) = qr_1d(k) + accr * dt_micro |
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501 | qc_1d(k) = qc_1d(k) - accr * dt_micro |
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502 | |
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503 | ENDIF |
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504 | |
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505 | ENDDO |
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506 | |
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507 | END SUBROUTINE accretion_ij |
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508 | |
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509 | |
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510 | SUBROUTINE selfcollection_breakup_ij( i, j ) |
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511 | |
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512 | USE arrays_3d |
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513 | USE cloud_parameters |
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514 | USE control_parameters |
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515 | USE indices |
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516 | |
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517 | IMPLICIT NONE |
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518 | |
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519 | INTEGER :: i, j, k |
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520 | REAL :: breakup, dr, phi_br, selfcoll |
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521 | |
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522 | DO k = nzb_s_inner(j,i)+1, nzt |
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523 | IF ( qr_1d(k) > eps_sb ) THEN |
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524 | ! |
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525 | !-- Selfcollection rate (Seifert and Beheng, 2001): |
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526 | selfcoll = k_rr * nr_1d(k) * qr_1d(k) * & |
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527 | SQRT( hyrho(k) * rho_surface ) |
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528 | ! |
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529 | !-- Weight averaged diameter of rain drops: |
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530 | dr = ( hyrho(k) * qr_1d(k) / nr_1d(k) * dpirho_l )**( 1.0 / 3.0 ) |
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531 | ! |
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532 | !-- Collisional breakup rate (Seifert, 2008): |
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533 | IF ( dr >= 0.3E-3 ) THEN |
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534 | phi_br = k_br * ( dr - 1.1E-3 ) |
---|
535 | breakup = selfcoll * ( phi_br + 1.0 ) |
---|
536 | ELSE |
---|
537 | breakup = 0.0 |
---|
538 | ENDIF |
---|
539 | |
---|
540 | selfcoll = MAX( breakup - selfcoll, -nr_1d(k) / dt_micro ) |
---|
541 | nr_1d(k) = nr_1d(k) + selfcoll * dt_micro |
---|
542 | |
---|
543 | ENDIF |
---|
544 | ENDDO |
---|
545 | |
---|
546 | END SUBROUTINE selfcollection_breakup_ij |
---|
547 | |
---|
548 | |
---|
549 | SUBROUTINE evaporation_rain_ij( i, j ) |
---|
550 | ! |
---|
551 | !-- Evaporation of precipitable water. Condensation is neglected for |
---|
552 | !-- precipitable water. |
---|
553 | |
---|
554 | USE arrays_3d |
---|
555 | USE cloud_parameters |
---|
556 | USE constants |
---|
557 | USE control_parameters |
---|
558 | USE indices |
---|
559 | |
---|
560 | IMPLICIT NONE |
---|
561 | |
---|
562 | INTEGER :: i, j, k |
---|
563 | REAL :: alpha, dr, e_s, evap, evap_nr, f_vent, g_evap, lambda_r, & |
---|
564 | mu_r, mu_r_2, mu_r_5d2, nr_0, q_s, sat, t_l, temp, xr |
---|
565 | |
---|
566 | DO k = nzb_s_inner(j,i)+1, nzt |
---|
567 | IF ( qr_1d(k) > eps_sb ) THEN |
---|
568 | ! |
---|
569 | !-- Actual liquid water temperature: |
---|
570 | t_l = t_d_pt(k) * pt_1d(k) |
---|
571 | ! |
---|
572 | !-- Saturation vapor pressure at t_l: |
---|
573 | e_s = 610.78 * EXP( 17.269 * ( t_l - 273.16 ) / ( t_l - 35.86 ) ) |
---|
574 | ! |
---|
575 | !-- Computation of saturation humidity: |
---|
576 | q_s = 0.622 * e_s / ( hyp(k) - 0.378 * e_s ) |
---|
577 | alpha = 0.622 * l_d_r * l_d_cp / ( t_l * t_l ) |
---|
578 | q_s = q_s * ( 1.0 + alpha * q_1d(k) ) / ( 1.0 + alpha * q_s ) |
---|
579 | ! |
---|
580 | !-- Supersaturation: |
---|
581 | sat = MIN( 0.0, ( q_1d(k) - qr_1d(k) - qc_1d(k) ) / q_s - 1.0 ) |
---|
582 | ! |
---|
583 | !-- Actual temperature: |
---|
584 | temp = t_l + l_d_cp * ( qc_1d(k) + qr_1d(k) ) |
---|
585 | |
---|
586 | g_evap = 1.0 / ( ( l_v / ( r_v * temp ) - 1.0 ) * l_v / & |
---|
587 | ( thermal_conductivity_l * temp ) + r_v * temp / & |
---|
588 | ( diff_coeff_l * e_s ) ) |
---|
589 | ! |
---|
590 | !-- Mean weight of rain drops |
---|
591 | xr = hyrho(k) * qr_1d(k) / nr_1d(k) |
---|
592 | ! |
---|
593 | !-- Weight averaged diameter of rain drops: |
---|
594 | dr = ( xr * dpirho_l )**( 1.0 / 3.0 ) |
---|
595 | ! |
---|
596 | !-- Compute ventilation factor and intercept parameter |
---|
597 | !-- (Seifert and Beheng, 2006; Seifert, 2008): |
---|
598 | IF ( ventilation_effect ) THEN |
---|
599 | ! |
---|
600 | !-- Shape parameter of gamma distribution (Milbrandt and Yau, 2005; |
---|
601 | !-- Stevens and Seifert, 2008): |
---|
602 | mu_r = 10.0 * ( 1.0 + TANH( 1.2E3 * ( dr - 1.4E-3 ) ) ) |
---|
603 | ! |
---|
604 | !-- Slope parameter of gamma distribution (Seifert, 2008): |
---|
605 | lambda_r = ( ( mu_r + 3.0 ) * ( mu_r + 2.0 ) * & |
---|
606 | ( mu_r + 1.0 ) )**( 1.0 / 3.0 ) / dr |
---|
607 | |
---|
608 | mu_r_2 = mu_r + 2.0 |
---|
609 | mu_r_5d2 = mu_r + 2.5 |
---|
610 | f_vent = a_vent * gamm( mu_r_2 ) * & |
---|
611 | lambda_r**( -mu_r_2 ) + & |
---|
612 | b_vent * schmidt_p_1d3 * & |
---|
613 | SQRT( a_term / kin_vis_air ) * gamm( mu_r_5d2 ) * & |
---|
614 | lambda_r**( -mu_r_5d2 ) * & |
---|
615 | ( 1.0 - 0.5 * ( b_term / a_term ) * & |
---|
616 | ( lambda_r / & |
---|
617 | ( c_term + lambda_r ) )**mu_r_5d2 - & |
---|
618 | 0.125 * ( b_term / a_term )**2 * & |
---|
619 | ( lambda_r / & |
---|
620 | ( 2.0 * c_term + lambda_r ) )**mu_r_5d2 - & |
---|
621 | 0.0625 * ( b_term / a_term )**3 * & |
---|
622 | ( lambda_r / & |
---|
623 | ( 3.0 * c_term + lambda_r ) )**mu_r_5d2 - & |
---|
624 | 0.0390625 * ( b_term / a_term )**4 * & |
---|
625 | ( lambda_r / & |
---|
626 | ( 4.0 * c_term + lambda_r ) )**mu_r_5d2 ) |
---|
627 | nr_0 = nr_1d(k) * lambda_r**( mu_r + 1.0 ) / & |
---|
628 | gamm( mu_r + 1.0 ) |
---|
629 | ELSE |
---|
630 | f_vent = 1.0 |
---|
631 | nr_0 = nr_1d(k) * dr |
---|
632 | ENDIF |
---|
633 | ! |
---|
634 | !-- Evaporation rate of rain water content (Seifert and Beheng, 2006): |
---|
635 | evap = 2.0 * pi * nr_0 * g_evap * f_vent * sat / & |
---|
636 | hyrho(k) |
---|
637 | |
---|
638 | evap = MAX( evap, -qr_1d(k) / dt_micro ) |
---|
639 | evap_nr = MAX( c_evap * evap / xr * hyrho(k), & |
---|
640 | -nr_1d(k) / dt_micro ) |
---|
641 | |
---|
642 | qr_1d(k) = qr_1d(k) + evap * dt_micro |
---|
643 | nr_1d(k) = nr_1d(k) + evap_nr * dt_micro |
---|
644 | ENDIF |
---|
645 | |
---|
646 | ENDDO |
---|
647 | |
---|
648 | END SUBROUTINE evaporation_rain_ij |
---|
649 | |
---|
650 | |
---|
651 | SUBROUTINE sedimentation_cloud_ij( i, j ) |
---|
652 | |
---|
653 | USE arrays_3d |
---|
654 | USE cloud_parameters |
---|
655 | USE constants |
---|
656 | USE control_parameters |
---|
657 | USE indices |
---|
658 | |
---|
659 | IMPLICIT NONE |
---|
660 | |
---|
661 | INTEGER :: i, j, k |
---|
662 | REAL :: sed_qc_const |
---|
663 | |
---|
664 | REAL, DIMENSION(nzb:nzt+1) :: sed_qc |
---|
665 | |
---|
666 | ! |
---|
667 | !-- Sedimentation of cloud droplets (Heus et al., 2010): |
---|
668 | sed_qc_const = k_st * ( 3.0 / ( 4.0 * pi * rho_l ))**( 2.0 / 3.0 ) * & |
---|
669 | EXP( 5.0 * LOG( sigma_gc )**2 ) |
---|
670 | |
---|
671 | sed_qc(nzt+1) = 0.0 |
---|
672 | |
---|
673 | DO k = nzt, nzb_s_inner(j,i)+1, -1 |
---|
674 | IF ( qc_1d(k) > eps_sb ) THEN |
---|
675 | sed_qc(k) = sed_qc_const * nc_1d(k)**( -2.0 / 3.0 ) * & |
---|
676 | ( qc_1d(k) * hyrho(k) )**( 5.0 / 3.0 ) |
---|
677 | ELSE |
---|
678 | sed_qc(k) = 0.0 |
---|
679 | ENDIF |
---|
680 | |
---|
681 | sed_qc(k) = MIN( sed_qc(k), hyrho(k) * dzu(k+1) * q_1d(k) / & |
---|
682 | dt_micro + sed_qc(k+1) ) |
---|
683 | |
---|
684 | q_1d(k) = q_1d(k) + ( sed_qc(k+1) - sed_qc(k) ) * ddzu(k+1) / & |
---|
685 | hyrho(k) * dt_micro |
---|
686 | qc_1d(k) = qc_1d(k) + ( sed_qc(k+1) - sed_qc(k) ) * ddzu(k+1) / & |
---|
687 | hyrho(k) * dt_micro |
---|
688 | pt_1d(k) = pt_1d(k) - ( sed_qc(k+1) - sed_qc(k) ) * ddzu(k+1) / & |
---|
689 | hyrho(k) * l_d_cp * pt_d_t(k) * dt_micro |
---|
690 | |
---|
691 | ENDDO |
---|
692 | |
---|
693 | END SUBROUTINE sedimentation_cloud_ij |
---|
694 | |
---|
695 | |
---|
696 | SUBROUTINE sedimentation_rain_ij( i, j ) |
---|
697 | |
---|
698 | USE arrays_3d |
---|
699 | USE cloud_parameters |
---|
700 | USE constants |
---|
701 | USE control_parameters |
---|
702 | USE indices |
---|
703 | USE statistics |
---|
704 | |
---|
705 | IMPLICIT NONE |
---|
706 | |
---|
707 | INTEGER :: i, j, k, k_run |
---|
708 | REAL :: c_run, d_max, d_mean, d_min, dr, dt_sedi, flux, lambda_r, & |
---|
709 | mu_r, z_run |
---|
710 | |
---|
711 | REAL, DIMENSION(nzb:nzt+1) :: c_nr, c_qr, d_nr, d_qr, nr_slope, & |
---|
712 | qr_slope, sed_nr, sed_qr, w_nr, w_qr |
---|
713 | ! |
---|
714 | !-- Computation of sedimentation flux. Implementation according to Stevens |
---|
715 | !-- and Seifert (2008). |
---|
716 | IF ( intermediate_timestep_count == 1 ) prr(:,j,i) = 0.0 |
---|
717 | ! |
---|
718 | !-- Compute velocities |
---|
719 | DO k = nzb_s_inner(j,i)+1, nzt |
---|
720 | IF ( qr_1d(k) > eps_sb ) THEN |
---|
721 | ! |
---|
722 | !-- Weight averaged diameter of rain drops: |
---|
723 | dr = ( hyrho(k) * qr_1d(k) / nr_1d(k) * dpirho_l )**( 1.0 / 3.0 ) |
---|
724 | ! |
---|
725 | !-- Shape parameter of gamma distribution (Milbrandt and Yau, 2005; |
---|
726 | !-- Stevens and Seifert, 2008): |
---|
727 | mu_r = 10.0 * ( 1.0 + TANH( 1.2E3 * ( dr - 1.4E-3 ) ) ) |
---|
728 | ! |
---|
729 | !-- Slope parameter of gamma distribution (Seifert, 2008): |
---|
730 | lambda_r = ( ( mu_r + 3.0 ) * ( mu_r + 2.0 ) * & |
---|
731 | ( mu_r + 1.0 ) )**( 1.0 / 3.0 ) / dr |
---|
732 | |
---|
733 | w_nr(k) = MAX( 0.1, MIN( 20.0, a_term - b_term * ( 1.0 + & |
---|
734 | c_term / lambda_r )**( -1.0 * ( mu_r + 1.0 ) ) ) ) |
---|
735 | w_qr(k) = MAX( 0.1, MIN( 20.0, a_term - b_term * ( 1.0 + & |
---|
736 | c_term / lambda_r )**( -1.0 * ( mu_r + 4.0 ) ) ) ) |
---|
737 | ELSE |
---|
738 | w_nr(k) = 0.0 |
---|
739 | w_qr(k) = 0.0 |
---|
740 | ENDIF |
---|
741 | ENDDO |
---|
742 | ! |
---|
743 | !-- Adjust boundary values |
---|
744 | w_nr(nzb_s_inner(j,i)) = w_nr(nzb_s_inner(j,i)+1) |
---|
745 | w_qr(nzb_s_inner(j,i)) = w_qr(nzb_s_inner(j,i)+1) |
---|
746 | w_nr(nzt+1) = 0.0 |
---|
747 | w_qr(nzt+1) = 0.0 |
---|
748 | ! |
---|
749 | !-- Compute Courant number |
---|
750 | DO k = nzb_s_inner(j,i)+1, nzt |
---|
751 | c_nr(k) = 0.25 * ( w_nr(k-1) + 2.0 * w_nr(k) + w_nr(k+1) ) * & |
---|
752 | dt_micro * ddzu(k) |
---|
753 | c_qr(k) = 0.25 * ( w_qr(k-1) + 2.0 * w_qr(k) + w_qr(k+1) ) * & |
---|
754 | dt_micro * ddzu(k) |
---|
755 | ENDDO |
---|
756 | ! |
---|
757 | !-- Limit slopes with monotonized centered (MC) limiter (van Leer, 1977): |
---|
758 | IF ( limiter_sedimentation ) THEN |
---|
759 | |
---|
760 | DO k = nzb_s_inner(j,i)+1, nzt |
---|
761 | d_mean = 0.5 * ( qr_1d(k+1) + qr_1d(k-1) ) |
---|
762 | d_min = qr_1d(k) - MIN( qr_1d(k+1), qr_1d(k), qr_1d(k-1) ) |
---|
763 | d_max = MAX( qr_1d(k+1), qr_1d(k), qr_1d(k-1) ) - qr_1d(k) |
---|
764 | |
---|
765 | qr_slope(k) = SIGN(1.0, d_mean) * MIN ( 2.0 * d_min, 2.0 * d_max, & |
---|
766 | ABS( d_mean ) ) |
---|
767 | |
---|
768 | d_mean = 0.5 * ( nr_1d(k+1) + nr_1d(k-1) ) |
---|
769 | d_min = nr_1d(k) - MIN( nr_1d(k+1), nr_1d(k), nr_1d(k-1) ) |
---|
770 | d_max = MAX( nr_1d(k+1), nr_1d(k), nr_1d(k-1) ) - nr_1d(k) |
---|
771 | |
---|
772 | nr_slope(k) = SIGN(1.0, d_mean) * MIN ( 2.0 * d_min, 2.0 * d_max, & |
---|
773 | ABS( d_mean ) ) |
---|
774 | ENDDO |
---|
775 | |
---|
776 | ELSE |
---|
777 | |
---|
778 | nr_slope = 0.0 |
---|
779 | qr_slope = 0.0 |
---|
780 | |
---|
781 | ENDIF |
---|
782 | |
---|
783 | sed_nr(nzt+1) = 0.0 |
---|
784 | sed_qr(nzt+1) = 0.0 |
---|
785 | ! |
---|
786 | !-- Compute sedimentation flux |
---|
787 | DO k = nzt, nzb_s_inner(j,i)+1, -1 |
---|
788 | ! |
---|
789 | !-- Sum up all rain drop number densities which contribute to the flux |
---|
790 | !-- through k-1/2 |
---|
791 | flux = 0.0 |
---|
792 | z_run = 0.0 ! height above z(k) |
---|
793 | k_run = k |
---|
794 | c_run = MIN( 1.0, c_nr(k) ) |
---|
795 | DO WHILE ( c_run > 0.0 .AND. k_run <= nzt ) |
---|
796 | flux = flux + hyrho(k_run) * & |
---|
797 | ( nr_1d(k_run) + nr_slope(k_run) * ( 1.0 - c_run ) * & |
---|
798 | 0.5 ) * c_run * dzu(k_run) |
---|
799 | z_run = z_run + dzu(k_run) |
---|
800 | k_run = k_run + 1 |
---|
801 | c_run = MIN( 1.0, c_nr(k_run) - z_run * ddzu(k_run) ) |
---|
802 | ENDDO |
---|
803 | ! |
---|
804 | !-- It is not allowed to sediment more rain drop number density than |
---|
805 | !-- available |
---|
806 | flux = MIN( flux, & |
---|
807 | hyrho(k) * dzu(k+1) * nr_1d(k) + sed_nr(k+1) * dt_micro ) |
---|
808 | |
---|
809 | sed_nr(k) = flux / dt_micro |
---|
810 | nr_1d(k) = nr_1d(k) + ( sed_nr(k+1) - sed_nr(k) ) * ddzu(k+1) / & |
---|
811 | hyrho(k) * dt_micro |
---|
812 | ! |
---|
813 | !-- Sum up all rain water content which contributes to the flux |
---|
814 | !-- through k-1/2 |
---|
815 | flux = 0.0 |
---|
816 | z_run = 0.0 ! height above z(k) |
---|
817 | k_run = k |
---|
818 | c_run = MIN( 1.0, c_qr(k) ) |
---|
819 | |
---|
820 | DO WHILE ( c_run > 0.0 .AND. k_run <= nzt-1 ) |
---|
821 | |
---|
822 | flux = flux + hyrho(k_run) * & |
---|
823 | ( qr_1d(k_run) + qr_slope(k_run) * ( 1.0 - c_run ) * & |
---|
824 | 0.5 ) * c_run * dzu(k_run) |
---|
825 | z_run = z_run + dzu(k_run) |
---|
826 | k_run = k_run + 1 |
---|
827 | c_run = MIN( 1.0, c_qr(k_run) - z_run * ddzu(k_run) ) |
---|
828 | |
---|
829 | ENDDO |
---|
830 | ! |
---|
831 | !-- It is not allowed to sediment more rain water content than available |
---|
832 | flux = MIN( flux, & |
---|
833 | hyrho(k) * dzu(k) * qr_1d(k) + sed_qr(k+1) * dt_micro ) |
---|
834 | |
---|
835 | sed_qr(k) = flux / dt_micro |
---|
836 | |
---|
837 | qr_1d(k) = qr_1d(k) + ( sed_qr(k+1) - sed_qr(k) ) * ddzu(k+1) / & |
---|
838 | hyrho(k) * dt_micro |
---|
839 | q_1d(k) = q_1d(k) + ( sed_qr(k+1) - sed_qr(k) ) * ddzu(k+1) / & |
---|
840 | hyrho(k) * dt_micro |
---|
841 | pt_1d(k) = pt_1d(k) - ( sed_qr(k+1) - sed_qr(k) ) * ddzu(k+1) / & |
---|
842 | hyrho(k) * l_d_cp * pt_d_t(k) * dt_micro |
---|
843 | ! |
---|
844 | !-- Compute the rain rate |
---|
845 | prr(k,j,i) = prr(k,j,i) + sed_qr(k) / hyrho(k) * & |
---|
846 | weight_substep(intermediate_timestep_count) |
---|
847 | ENDDO |
---|
848 | |
---|
849 | ! |
---|
850 | !-- Precipitation amount |
---|
851 | IF ( intermediate_timestep_count == intermediate_timestep_count_max & |
---|
852 | .AND. ( dt_do2d_xy - time_do2d_xy ) < & |
---|
853 | precipitation_amount_interval ) THEN |
---|
854 | |
---|
855 | precipitation_amount(j,i) = precipitation_amount(j,i) + & |
---|
856 | prr(nzb_s_inner(j,i)+1,j,i) * & |
---|
857 | hyrho(nzb_s_inner(j,i)+1) * dt_3d |
---|
858 | ENDIF |
---|
859 | |
---|
860 | END SUBROUTINE sedimentation_rain_ij |
---|
861 | |
---|
862 | |
---|
863 | ! |
---|
864 | !-- This function computes the gamma function (Press et al., 1992). |
---|
865 | !-- The gamma function is needed for the calculation of the evaporation |
---|
866 | !-- of rain drops. |
---|
867 | FUNCTION gamm( xx ) |
---|
868 | |
---|
869 | USE cloud_parameters |
---|
870 | |
---|
871 | IMPLICIT NONE |
---|
872 | |
---|
873 | REAL :: gamm, ser, tmp, x_gamm, xx, y_gamm |
---|
874 | INTEGER :: j |
---|
875 | |
---|
876 | |
---|
877 | x_gamm = xx |
---|
878 | y_gamm = x_gamm |
---|
879 | tmp = x_gamm + 5.5 |
---|
880 | tmp = ( x_gamm + 0.5 ) * LOG( tmp ) - tmp |
---|
881 | ser = 1.000000000190015 |
---|
882 | |
---|
883 | DO j = 1, 6 |
---|
884 | y_gamm = y_gamm + 1.0 |
---|
885 | ser = ser + cof( j ) / y_gamm |
---|
886 | ENDDO |
---|
887 | |
---|
888 | ! |
---|
889 | !-- Until this point the algorithm computes the logarithm of the gamma |
---|
890 | !-- function. Hence, the exponential function is used. |
---|
891 | ! gamm = EXP( tmp + LOG( stp * ser / x_gamm ) ) |
---|
892 | gamm = EXP( tmp ) * stp * ser / x_gamm |
---|
893 | |
---|
894 | RETURN |
---|
895 | |
---|
896 | END FUNCTION gamm |
---|
897 | |
---|
898 | END MODULE microphysics_mod |
---|