1 | ! %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
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2 | ! Copyright (c) 2015, Regents of the University of Colorado |
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3 | ! All rights reserved. |
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4 | ! |
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5 | ! Redistribution and use in source and binary forms, with or without modification, are |
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6 | ! permitted provided that the following conditions are met: |
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7 | ! |
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8 | ! 1. Redistributions of source code must retain the above copyright notice, this list of |
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9 | ! conditions and the following disclaimer. |
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10 | ! |
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11 | ! 2. Redistributions in binary form must reproduce the above copyright notice, this list |
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12 | ! of conditions and the following disclaimer in the documentation and/or other |
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13 | ! materials provided with the distribution. |
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14 | ! |
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15 | ! 3. Neither the name of the copyright holder nor the names of its contributors may be |
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16 | ! used to endorse or promote products derived from this software without specific prior |
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17 | ! written permission. |
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18 | ! |
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19 | ! THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS" AND ANY |
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20 | ! EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF |
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21 | ! MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL |
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22 | ! THE COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, |
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23 | ! SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT |
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24 | ! OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS |
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25 | ! INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT |
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26 | ! LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE |
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27 | ! OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. |
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28 | ! |
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29 | ! History: |
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30 | ! 05/01/15 Dustin Swales - Original version |
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31 | ! |
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32 | ! %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
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33 | module cosp_optics |
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34 | USE COSP_KINDS, ONLY: wp,dp |
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35 | USE COSP_MATH_CONSTANTS, ONLY: pi |
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36 | USE COSP_PHYS_CONSTANTS, ONLY: rholiq,km,rd,grav |
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37 | USE MOD_MODIS_SIM, ONLY: get_g_nir,get_ssa_nir,phaseIsLiquid,phaseIsIce |
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38 | implicit none |
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39 | |
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40 | real(wp),parameter :: & ! |
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41 | ice_density = 0.93_wp ! Ice density used in MODIS phase partitioning |
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42 | |
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43 | interface cosp_simulator_optics |
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44 | module procedure cosp_simulator_optics2D, cosp_simulator_optics3D |
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45 | end interface cosp_simulator_optics |
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46 | |
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47 | contains |
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48 | ! ########################################################################## |
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49 | ! COSP_SIMULATOR_OPTICS |
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50 | ! |
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51 | ! Used by: ISCCP, MISR and MODIS simulators |
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52 | ! ########################################################################## |
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53 | subroutine cosp_simulator_optics2D(dim1,dim2,dim3,flag,varIN1,varIN2,varOUT) |
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54 | ! INPUTS |
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55 | integer,intent(in) :: & |
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56 | dim1, & ! Dimension 1 extent (Horizontal) |
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57 | dim2, & ! Dimension 2 extent (Subcolumn) |
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58 | dim3 ! Dimension 3 extent (Vertical) |
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59 | real(wp),intent(in),dimension(dim1,dim2,dim3) :: & |
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60 | flag ! Logical to determine the of merge var1IN and var2IN |
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61 | real(wp),intent(in),dimension(dim1, dim3) :: & |
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62 | varIN1, & ! Input field 1 |
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63 | varIN2 ! Input field 2 |
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64 | ! OUTPUTS |
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65 | real(wp),intent(out),dimension(dim1,dim2,dim3) :: & |
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66 | varOUT ! Merged output field |
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67 | ! LOCAL VARIABLES |
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68 | integer :: j |
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69 | |
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70 | varOUT(1:dim1,1:dim2,1:dim3) = 0._wp |
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71 | do j=1,dim2 |
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72 | where(flag(:,j,:) .eq. 1) |
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73 | varOUT(:,j,:) = varIN2 |
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74 | endwhere |
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75 | where(flag(:,j,:) .eq. 2) |
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76 | varOUT(:,j,:) = varIN1 |
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77 | endwhere |
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78 | enddo |
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79 | end subroutine cosp_simulator_optics2D |
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80 | subroutine cosp_simulator_optics3D(dim1,dim2,dim3,flag,varIN1,varIN2,varOUT) |
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81 | ! INPUTS |
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82 | integer,intent(in) :: & |
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83 | dim1, & ! Dimension 1 extent (Horizontal) |
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84 | dim2, & ! Dimension 2 extent (Subcolumn) |
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85 | dim3 ! Dimension 3 extent (Vertical) |
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86 | real(wp),intent(in),dimension(dim1,dim2,dim3) :: & |
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87 | flag ! Logical to determine the of merge var1IN and var2IN |
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88 | real(wp),intent(in),dimension(dim1,dim2,dim3) :: & |
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89 | varIN1, & ! Input field 1 |
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90 | varIN2 ! Input field 2 |
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91 | ! OUTPUTS |
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92 | real(wp),intent(out),dimension(dim1,dim2,dim3) :: & |
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93 | varOUT ! Merged output field |
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94 | |
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95 | varOUT(1:dim1,1:dim2,1:dim3) = 0._wp |
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96 | where(flag(:,:,:) .eq. 1) |
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97 | varOUT(:,:,:) = varIN2 |
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98 | endwhere |
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99 | where(flag(:,:,:) .eq. 2) |
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100 | varOUT(:,:,:) = varIN1 |
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101 | endwhere |
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102 | |
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103 | end subroutine cosp_simulator_optics3D |
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104 | |
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105 | ! ############################################################################## |
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106 | ! MODIS_OPTICS_PARTITION |
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107 | ! |
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108 | ! For the MODIS simulator, there are times when only a sinlge optical depth |
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109 | ! profile, cloud-ice and cloud-water are provided. In this case, the optical |
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110 | ! depth is partitioned by phase. |
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111 | ! ############################################################################## |
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112 | subroutine MODIS_OPTICS_PARTITION(npoints,nlev,ncolumns,cloudWater,cloudIce,waterSize, & |
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113 | iceSize,tau,tauL,tauI) |
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114 | ! INPUTS |
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115 | INTEGER,intent(in) :: & |
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116 | npoints, & ! Number of horizontal gridpoints |
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117 | nlev, & ! Number of levels |
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118 | ncolumns ! Number of subcolumns |
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119 | REAL(wp),intent(in),dimension(npoints,nlev,ncolumns) :: & |
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120 | cloudWater, & ! Subcolumn cloud water content |
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121 | cloudIce, & ! Subcolumn cloud ice content |
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122 | waterSize, & ! Subcolumn cloud water effective radius |
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123 | iceSize, & ! Subcolumn cloud ice effective radius |
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124 | tau ! Optical thickness |
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125 | |
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126 | ! OUTPUTS |
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127 | real(wp),intent(out),dimension(npoints,nlev,ncolumns) :: & |
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128 | tauL, & ! Partitioned liquid optical thickness. |
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129 | tauI ! Partitioned ice optical thickness. |
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130 | ! LOCAL VARIABLES |
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131 | real(wp),dimension(nlev,ncolumns) :: fracL |
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132 | integer :: i |
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133 | |
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134 | |
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135 | do i=1,npoints |
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136 | where(cloudIce(i,:, :) <= 0.) |
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137 | fracL(:, :) = 1._wp |
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138 | elsewhere |
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139 | where (cloudWater(i,:, :) <= 0.) |
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140 | fracL(:, :) = 0._wp |
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141 | elsewhere |
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142 | ! Geometic optics limit - tau as LWP/re (proportional to LWC/re) |
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143 | fracL(:, :) = (cloudWater(i,:, :)/waterSize(i,:, :)) / & |
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144 | (cloudWater(i,:, :)/waterSize(i,:, :) + cloudIce(i,:, :)/(ice_density * iceSize(i,:, :)) ) |
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145 | end where |
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146 | end where |
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147 | tauL(i,:, :) = fracL(:, :) * tau(i,:, :) |
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148 | tauI(i,:, :) = tau(i,:, :) - tauL(i,:, :) |
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149 | enddo |
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150 | |
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151 | end subroutine MODIS_OPTICS_PARTITION |
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152 | ! ######################################################################################## |
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153 | ! MODIS_OPTICS |
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154 | ! |
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155 | ! ######################################################################################## |
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156 | subroutine modis_optics(nPoints,nLevels,nSubCols,tauLIQ,sizeLIQ,tauICE,sizeICE,fracLIQ, g, w0) |
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157 | ! INPUTS |
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158 | integer, intent(in) :: nPoints,nLevels,nSubCols |
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159 | real(wp),intent(in),dimension(nPoints,nSubCols,nLevels) :: tauLIQ, sizeLIQ, tauICE, sizeICE |
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160 | ! OUTPUTS |
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161 | real(wp),intent(out),dimension(nPoints,nSubCols,nLevels) :: g,w0,fracLIQ |
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162 | ! LOCAL VARIABLES |
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163 | real(wp), dimension(nLevels) :: water_g, water_w0, ice_g, ice_w0,tau |
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164 | integer :: i,j |
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165 | |
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166 | ! Initialize |
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167 | g(1:nPoints,1:nSubCols,1:nLevels) = 0._wp |
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168 | w0(1:nPoints,1:nSubCols,1:nLevels) = 0._wp |
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169 | |
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170 | do j =1,nPoints |
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171 | do i=1,nSubCols |
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172 | water_g(1:nLevels) = get_g_nir( phaseIsLiquid, sizeLIQ(j,i,1:nLevels)) |
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173 | water_w0(1:nLevels) = get_ssa_nir(phaseIsLiquid, sizeLIQ(j,i,1:nLevels)) |
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174 | ice_g(1:nLevels) = get_g_nir( phaseIsIce, sizeICE(j,i,1:nLevels)) |
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175 | ice_w0(1:nLevels) = get_ssa_nir(phaseIsIce, sizeICE(j,i,1:nLevels)) |
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176 | |
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177 | ! Combine ice and water optical properties |
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178 | tau(1:nLevels) = tauICE(j,i,1:nLevels) + tauLIQ(j,i,1:nLevels) |
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179 | where (tau(1:nLevels) > 0) |
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180 | g(j,i,1:nLevels) = (tauLIQ(j,i,1:nLevels)*water_g(1:nLevels) + tauICE(j,i,1:nLevels)*ice_g(1:nLevels)) / & |
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181 | tau(1:nLevels) |
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182 | w0(j,i,1:nLevels) = (tauLIQ(j,i,1:nLevels)*water_g(1:nLevels)*water_w0(1:nLevels) + tauICE(j,i,1:nLevels) * & |
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183 | ice_g(1:nLevels) * ice_w0(1:nLevels)) / (g(j,i,1:nLevels) * tau(1:nLevels)) |
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184 | end where |
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185 | enddo |
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186 | enddo |
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187 | |
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188 | ! Compute the total optical thickness and the proportion due to liquid in each cell |
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189 | do i=1,npoints |
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190 | where(tauLIQ(i,1:nSubCols,1:nLevels) + tauICE(i,1:nSubCols,1:nLevels) > 0.) |
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191 | fracLIQ(i,1:nSubCols,1:nLevels) = tauLIQ(i,1:nSubCols,1:nLevels)/ & |
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192 | (tauLIQ(i,1:nSubCols,1:nLevels) + tauICE(i,1:nSubCols,1:nLevels)) |
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193 | elsewhere |
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194 | fracLIQ(i,1:nSubCols,1:nLevels) = 0._wp |
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195 | end where |
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196 | enddo |
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197 | |
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198 | end subroutine modis_optics |
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199 | |
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200 | ! ###################################################################################### |
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201 | ! SUBROUTINE lidar_optics |
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202 | ! ###################################################################################### |
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203 | subroutine lidar_optics(npoints,ncolumns,nlev,npart,ice_type,q_lsliq, q_lsice, & |
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204 | q_cvliq, q_cvice,ls_radliq,ls_radice,cv_radliq,cv_radice, & |
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205 | pres,presf,temp,beta_mol,betatot,tau_mol,tautot, & |
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206 | tautot_S_liq,tautot_S_ice,betatot_ice,betatot_liq, & |
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207 | tautot_ice,tautot_liq) |
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208 | ! #################################################################################### |
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209 | ! NOTE: Using "grav" from cosp_constants.f90, instead of grav=9.81, introduces |
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210 | ! changes of up to 2% in atb532 adn 0.003% in parasolRefl and lidarBetaMol532. |
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211 | ! This also results in small changes in the joint-histogram, cfadLidarsr532. |
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212 | ! #################################################################################### |
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213 | |
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214 | ! INPUTS |
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215 | INTEGER,intent(in) :: & |
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216 | npoints, & ! Number of gridpoints |
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217 | ncolumns, & ! Number of subcolumns |
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218 | nlev, & ! Number of levels |
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219 | npart, & ! Number of cloud meteors (stratiform_liq, stratiform_ice, conv_liq, conv_ice). |
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220 | ice_type ! Ice particle shape hypothesis (0 for spheres, 1 for non-spherical) |
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221 | REAL(WP),intent(in),dimension(npoints,nlev) :: & |
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222 | temp, & ! Temperature of layer k |
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223 | pres, & ! Pressure at full levels |
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224 | ls_radliq, & ! Effective radius of LS liquid particles (meters) |
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225 | ls_radice, & ! Effective radius of LS ice particles (meters) |
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226 | cv_radliq, & ! Effective radius of CONV liquid particles (meters) |
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227 | cv_radice ! Effective radius of CONV ice particles (meters) |
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228 | REAL(WP),intent(in),dimension(npoints,ncolumns,nlev) :: & |
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229 | q_lsliq, & ! LS sub-column liquid water mixing ratio (kg/kg) |
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230 | q_lsice, & ! LS sub-column ice water mixing ratio (kg/kg) |
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231 | q_cvliq, & ! CONV sub-column liquid water mixing ratio (kg/kg) |
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232 | q_cvice ! CONV sub-column ice water mixing ratio (kg/kg) |
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233 | REAL(WP),intent(in),dimension(npoints,nlev+1) :: & |
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234 | presf ! Pressure at half levels |
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235 | |
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236 | ! OUTPUTS |
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237 | REAL(WP),intent(out),dimension(npoints,ncolumns,nlev) :: & |
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238 | betatot, & ! |
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239 | tautot ! Optical thickess integrated from top |
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240 | REAL(WP),intent(out),dimension(npoints,ncolumns,nlev) :: & |
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241 | betatot_ice, & ! Backscatter coefficient for ice particles |
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242 | betatot_liq, & ! Backscatter coefficient for liquid particles |
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243 | tautot_ice, & ! Total optical thickness of ice |
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244 | tautot_liq ! Total optical thickness of liq |
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245 | REAL(WP),intent(out),dimension(npoints,nlev) :: & |
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246 | beta_mol, & ! Molecular backscatter coefficient |
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247 | tau_mol ! Molecular optical depth |
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248 | REAL(WP),intent(out),dimension(npoints,ncolumns) :: & |
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249 | tautot_S_liq, & ! TOA optical depth for liquid |
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250 | tautot_S_ice ! TOA optical depth for ice |
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251 | |
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252 | ! LOCAL VARIABLES |
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253 | REAL(WP),dimension(npart) :: rhopart |
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254 | REAL(WP),dimension(npart,5) :: polpart |
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255 | REAL(WP),dimension(npoints,nlev) :: rhoair,alpha_mol |
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256 | REAL(WP),dimension(npoints,nlev+1) :: zheight |
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257 | REAL(WP),dimension(npoints,nlev,npart) :: rad_part,kp_part,qpart |
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258 | REAL(WP),dimension(npoints,ncolumns,nlev,npart) :: alpha_part,tau_part |
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259 | INTEGER :: i,k,icol |
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260 | |
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261 | ! Local data |
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262 | REAL(WP),PARAMETER :: rhoice = 0.5e+03 ! Density of ice (kg/m3) |
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263 | REAL(WP),PARAMETER :: Cmol = 6.2446e-32 ! Wavelength dependent |
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264 | REAL(WP),PARAMETER :: rdiffm = 0.7_wp ! Multiple scattering correction parameter |
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265 | REAL(WP),PARAMETER :: Qscat = 2.0_wp ! Particle scattering efficiency at 532 nm |
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266 | ! Local indicies for large-scale and convective ice and liquid |
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267 | INTEGER,PARAMETER :: INDX_LSLIQ = 1 |
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268 | INTEGER,PARAMETER :: INDX_LSICE = 2 |
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269 | INTEGER,PARAMETER :: INDX_CVLIQ = 3 |
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270 | INTEGER,PARAMETER :: INDX_CVICE = 4 |
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271 | |
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272 | ! Polarized optics parameterization |
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273 | ! Polynomial coefficients for spherical liq/ice particles derived from Mie theory. |
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274 | ! Polynomial coefficients for non spherical particles derived from a composite of |
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275 | ! Ray-tracing theory for large particles (e.g. Noel et al., Appl. Opt., 2001) |
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276 | ! and FDTD theory for very small particles (Yang et al., JQSRT, 2003). |
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277 | ! We repeat the same coefficients for LS and CONV cloud to make code more readable |
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278 | REAL(WP),PARAMETER,dimension(5) :: & |
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279 | polpartCVLIQ = (/ 2.6980e-8_wp, -3.7701e-6_wp, 1.6594e-4_wp, -0.0024_wp, 0.0626_wp/), & |
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280 | polpartLSLIQ = (/ 2.6980e-8_wp, -3.7701e-6_wp, 1.6594e-4_wp, -0.0024_wp, 0.0626_wp/), & |
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281 | polpartCVICE0 = (/-1.0176e-8_wp, 1.7615e-6_wp, -1.0480e-4_wp, 0.0019_wp, 0.0460_wp/), & |
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282 | polpartLSICE0 = (/-1.0176e-8_wp, 1.7615e-6_wp, -1.0480e-4_wp, 0.0019_wp, 0.0460_wp/), & |
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283 | polpartCVICE1 = (/ 1.3615e-8_wp, -2.04206e-6_wp, 7.51799e-5_wp, 0.00078213_wp, 0.0182131_wp/), & |
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284 | polpartLSICE1 = (/ 1.3615e-8_wp, -2.04206e-6_wp, 7.51799e-5_wp, 0.00078213_wp, 0.0182131_wp/) |
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285 | ! ############################################################################## |
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286 | |
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287 | ! Liquid/ice particles |
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288 | rhopart(INDX_LSLIQ) = rholiq |
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289 | rhopart(INDX_LSICE) = rhoice |
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290 | rhopart(INDX_CVLIQ) = rholiq |
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291 | rhopart(INDX_CVICE) = rhoice |
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292 | |
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293 | ! LS and CONV Liquid water coefficients |
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294 | polpart(INDX_LSLIQ,1:5) = polpartLSLIQ |
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295 | polpart(INDX_CVLIQ,1:5) = polpartCVLIQ |
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296 | ! LS and CONV Ice water coefficients |
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297 | if (ice_type .eq. 0) then |
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298 | polpart(INDX_LSICE,1:5) = polpartLSICE0 |
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299 | polpart(INDX_CVICE,1:5) = polpartCVICE0 |
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300 | endif |
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301 | if (ice_type .eq. 1) then |
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302 | polpart(INDX_LSICE,1:5) = polpartLSICE1 |
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303 | polpart(INDX_CVICE,1:5) = polpartCVICE1 |
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304 | endif |
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305 | |
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306 | ! Effective radius particles: |
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307 | rad_part(1:npoints,1:nlev,INDX_LSLIQ) = ls_radliq(1:npoints,1:nlev) |
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308 | rad_part(1:npoints,1:nlev,INDX_LSICE) = ls_radice(1:npoints,1:nlev) |
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309 | rad_part(1:npoints,1:nlev,INDX_CVLIQ) = cv_radliq(1:npoints,1:nlev) |
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310 | rad_part(1:npoints,1:nlev,INDX_CVICE) = cv_radice(1:npoints,1:nlev) |
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311 | rad_part(1:npoints,1:nlev,1:npart) = MAX(rad_part(1:npoints,1:nlev,1:npart),0._wp) |
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312 | rad_part(1:npoints,1:nlev,1:npart) = MIN(rad_part(1:npoints,1:nlev,1:npart),70.0e-6_wp) |
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313 | |
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314 | ! Density (clear-sky air) |
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315 | rhoair(1:npoints,1:nlev) = pres(1:npoints,1:nlev)/(rd*temp(1:npoints,1:nlev)) |
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316 | |
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317 | ! Altitude at half pressure levels: |
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318 | zheight(1:npoints,nlev+1) = 0._wp |
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319 | do k=nlev,1,-1 |
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320 | zheight(1:npoints,k) = zheight(1:npoints,k+1) & |
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321 | -(presf(1:npoints,k)-presf(1:npoints,k+1))/(rhoair(1:npoints,k)*grav) |
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322 | enddo |
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323 | |
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324 | ! ############################################################################## |
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325 | ! *) Molecular alpha, beta and optical thickness |
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326 | ! ############################################################################## |
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327 | |
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328 | beta_mol(1:npoints,1:nlev) = pres(1:npoints,1:nlev)/km/temp(1:npoints,1:nlev)*Cmol |
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329 | alpha_mol(1:npoints,1:nlev) = 8._wp*pi/3._wp * beta_mol(1:npoints,1:nlev) |
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330 | |
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331 | ! Optical thickness of each layer (molecular) |
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332 | tau_mol(1:npoints,1:nlev) = alpha_mol(1:npoints,1:nlev)*(zheight(1:npoints,1:nlev)-& |
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333 | zheight(1:npoints,2:nlev+1)) |
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334 | |
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335 | ! Optical thickness from TOA to layer k (molecular) |
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336 | DO k = 2,nlev |
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337 | tau_mol(1:npoints,k) = tau_mol(1:npoints,k) + tau_mol(1:npoints,k-1) |
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338 | ENDDO |
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339 | |
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340 | betatot (1:npoints,1:ncolumns,1:nlev) = spread(beta_mol(1:npoints,1:nlev), dim=2, NCOPIES=ncolumns) |
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341 | tautot (1:npoints,1:ncolumns,1:nlev) = spread(tau_mol (1:npoints,1:nlev), dim=2, NCOPIES=ncolumns) |
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342 | betatot_liq(1:npoints,1:ncolumns,1:nlev) = betatot(1:npoints,1:ncolumns,1:nlev) |
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343 | betatot_ice(1:npoints,1:ncolumns,1:nlev) = betatot(1:npoints,1:ncolumns,1:nlev) |
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344 | tautot_liq (1:npoints,1:ncolumns,1:nlev) = tautot(1:npoints,1:ncolumns,1:nlev) |
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345 | tautot_ice (1:npoints,1:ncolumns,1:nlev) = tautot(1:npoints,1:ncolumns,1:nlev) |
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346 | |
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347 | ! ############################################################################## |
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348 | ! *) Particles alpha, beta and optical thickness |
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349 | ! ############################################################################## |
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350 | ! Polynomials kp_lidar derived from Mie theory |
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351 | do i = 1, npart |
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352 | where (rad_part(1:npoints,1:nlev,i) .gt. 0.0) |
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353 | kp_part(1:npoints,1:nlev,i) = & |
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354 | polpart(i,1)*(rad_part(1:npoints,1:nlev,i)*1e6)**4 & |
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355 | + polpart(i,2)*(rad_part(1:npoints,1:nlev,i)*1e6)**3 & |
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356 | + polpart(i,3)*(rad_part(1:npoints,1:nlev,i)*1e6)**2 & |
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357 | + polpart(i,4)*(rad_part(1:npoints,1:nlev,i)*1e6) & |
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358 | + polpart(i,5) |
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359 | elsewhere |
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360 | kp_part(1:npoints,1:nlev,i) = 0._wp |
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361 | endwhere |
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362 | enddo |
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363 | |
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364 | ! Loop over all subcolumns |
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365 | do icol=1,ncolumns |
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366 | ! ############################################################################## |
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367 | ! Mixing ratio particles in each subcolum |
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368 | ! ############################################################################## |
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369 | qpart(1:npoints,1:nlev,INDX_LSLIQ) = q_lsliq(1:npoints,icol,1:nlev) |
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370 | qpart(1:npoints,1:nlev,INDX_LSICE) = q_lsice(1:npoints,icol,1:nlev) |
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371 | qpart(1:npoints,1:nlev,INDX_CVLIQ) = q_cvliq(1:npoints,icol,1:nlev) |
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372 | qpart(1:npoints,1:nlev,INDX_CVICE) = q_cvice(1:npoints,icol,1:nlev) |
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373 | |
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374 | ! ############################################################################## |
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375 | ! Alpha and optical thickness (particles) |
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376 | ! ############################################################################## |
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377 | ! Alpha of particles in each subcolumn: |
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378 | do i = 1, npart |
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379 | where (rad_part(1:npoints,1:nlev,i) .gt. 0.0) |
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380 | alpha_part(1:npoints,icol,1:nlev,i) = 3._wp/4._wp * Qscat & |
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381 | * rhoair(1:npoints,1:nlev) * qpart(1:npoints,1:nlev,i) & |
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382 | / (rhopart(i) * rad_part(1:npoints,1:nlev,i) ) |
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383 | elsewhere |
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384 | alpha_part(1:npoints,icol,1:nlev,i) = 0._wp |
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385 | endwhere |
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386 | enddo |
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387 | |
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388 | ! Optical thicknes |
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389 | tau_part(1:npoints,icol,1:nlev,1:npart) = rdiffm * alpha_part(1:npoints,icol,1:nlev,1:npart) |
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390 | do i = 1, npart |
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391 | ! Optical thickness of each layer (particles) |
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392 | tau_part(1:npoints,icol,1:nlev,i) = tau_part(1:npoints,icol,1:nlev,i) & |
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393 | & * (zheight(1:npoints,1:nlev)-zheight(1:npoints,2:nlev+1) ) |
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394 | ! Optical thickness from TOA to layer k (particles) |
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395 | do k=2,nlev |
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396 | tau_part(1:npoints,icol,k,i) = tau_part(1:npoints,icol,k,i) + tau_part(1:npoints,icol,k-1,i) |
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397 | enddo |
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398 | enddo |
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399 | |
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400 | ! ############################################################################## |
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401 | ! Beta and optical thickness (total=molecular + particules) |
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402 | ! ############################################################################## |
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403 | |
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404 | DO i = 1, npart |
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405 | betatot(1:npoints,icol,1:nlev) = betatot(1:npoints,icol,1:nlev) + & |
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406 | kp_part(1:npoints,1:nlev,i)*alpha_part(1:npoints,icol,1:nlev,i) |
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407 | tautot(1:npoints,icol,1:nlev) = tautot(1:npoints,icol,1:nlev) + & |
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408 | tau_part(1:npoints,icol,1:nlev,i) |
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409 | ENDDO |
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410 | |
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411 | ! ############################################################################## |
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412 | ! Beta and optical thickness (liquid/ice) |
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413 | ! ############################################################################## |
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414 | ! Ice |
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415 | betatot_ice(1:npoints,icol,1:nlev) = betatot_ice(1:npoints,icol,1:nlev)+ & |
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416 | kp_part(1:npoints,1:nlev,INDX_LSICE)*alpha_part(1:npoints,icol,1:nlev,INDX_LSICE)+ & |
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417 | kp_part(1:npoints,1:nlev,INDX_CVICE)*alpha_part(1:npoints,icol,1:nlev,INDX_CVICE) |
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418 | tautot_ice(1:npoints,icol,1:nlev) = tautot_ice(1:npoints,icol,1:nlev) + & |
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419 | tau_part(1:npoints,icol,1:nlev,INDX_LSICE) + & |
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420 | tau_part(1:npoints,icol,1:nlev,INDX_CVICE) |
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421 | |
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422 | ! Liquid |
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423 | betatot_liq(1:npoints,icol,1:nlev) = betatot_liq(1:npoints,icol,1:nlev)+ & |
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424 | kp_part(1:npoints,1:nlev,INDX_LSLIQ)*alpha_part(1:npoints,icol,1:nlev,INDX_LSLIQ)+ & |
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425 | kp_part(1:npoints,1:nlev,INDX_CVLIQ)*alpha_part(1:npoints,icol,1:nlev,INDX_CVLIQ) |
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426 | tautot_liq(1:npoints,icol,1:nlev) = tautot_liq(1:npoints,icol,1:nlev) + & |
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427 | tau_part(1:npoints,icol,1:nlev,INDX_LSLIQ) + & |
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428 | tau_part(1:npoints,icol,1:nlev,INDX_CVLIQ) |
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429 | enddo |
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430 | |
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431 | ! ############################################################################## |
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432 | ! Optical depths used by the PARASOL simulator |
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433 | ! ############################################################################## |
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434 | tautot_S_liq(1:npoints,1:ncolumns) = 0._wp |
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435 | tautot_S_ice(1:npoints,1:ncolumns) = 0._wp |
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436 | do icol=1,ncolumns |
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437 | tautot_S_liq(1:npoints,icol) = tautot_S_liq(1:npoints,icol)+tau_part(1:npoints,icol,nlev,1)+tau_part(1:npoints,icol,nlev,3) |
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438 | tautot_S_ice(1:npoints,icol) = tautot_S_ice(1:npoints,icol)+tau_part(1:npoints,icol,nlev,2)+tau_part(1:npoints,icol,nlev,4) |
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439 | enddo |
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440 | |
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441 | end subroutine lidar_optics |
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442 | end module cosp_optics |
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