1 | subroutine optci(PLEV,TLEV,DTAUI,TAUCUMI, & |
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2 | QXIAER,QSIAER,GIAER,COSBI,WBARI,TAUAERO, & |
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3 | TMID,PMID,TAUGSURF,QVAR) |
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4 | |
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5 | |
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6 | use radinc_h |
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7 | use radcommon_h, only: gasi, tlimit, wrefVAR, Cmk,tgasref,pfgasref,wnoi |
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8 | implicit none |
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9 | |
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10 | !================================================================== |
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11 | ! |
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12 | ! Purpose |
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13 | ! ------- |
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14 | ! Calculates longwave optical constants at each level. For each |
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15 | ! layer and spectral interval in the IR it calculates WBAR, DTAU |
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16 | ! and COSBAR. For each level it calculates TAU. |
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17 | ! |
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18 | ! TAUI(L,LW) is the cumulative optical depth at level L (or alternatively |
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19 | ! at the *bottom* of layer L), LW is the spectral wavelength interval. |
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20 | ! |
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21 | ! TLEV(L) - Temperature at the layer boundary (i.e., level) |
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22 | ! PLEV(L) - Pressure at the layer boundary (i.e., level) |
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23 | ! |
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24 | ! Authors |
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25 | ! ------- |
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26 | ! Adapted from the NASA Ames code by R. Wordsworth (2009) |
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27 | ! |
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28 | !================================================================== |
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29 | |
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30 | |
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31 | #include "comcstfi.h" |
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32 | #include "callkeys.h" |
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33 | |
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34 | |
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35 | real*8 DTAUI(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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36 | real*8 DTAUKI(L_LEVELS+1,L_NSPECTI,L_NGAUSS) |
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37 | real*8 TAUI(L_NLEVRAD,L_NSPECTI,L_NGAUSS) |
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38 | real*8 TAUCUMI(L_LEVELS,L_NSPECTI,L_NGAUSS) |
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39 | real*8 PLEV(L_LEVELS) |
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40 | real*8 TLEV(L_LEVELS) |
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41 | real*8 TMID(L_LEVELS), PMID(L_LEVELS) |
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42 | real*8 COSBI(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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43 | real*8 WBARI(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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44 | |
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45 | ! For aerosols |
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46 | real*8 QXIAER(L_LEVELS+1,L_NSPECTI,NAERKIND) |
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47 | real*8 QSIAER(L_LEVELS+1,L_NSPECTI,NAERKIND) |
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48 | real*8 GIAER(L_LEVELS+1,L_NSPECTI,NAERKIND) |
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49 | real*8 TAUAERO(L_LEVELS+1,NAERKIND) |
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50 | real*8 TAUAEROLK(L_LEVELS+1,L_NSPECTI,NAERKIND) |
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51 | real*8 TAEROS(L_LEVELS,L_NSPECTI,NAERKIND) |
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52 | |
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53 | integer L, NW, NG, K, LK, IAER |
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54 | integer MT(L_LEVELS), MP(L_LEVELS), NP(L_LEVELS) |
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55 | real*8 ANS, TAUGAS |
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56 | real*8 DPR(L_LEVELS), U(L_LEVELS) |
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57 | real*8 LCOEF(4), LKCOEF(L_LEVELS,4) |
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58 | |
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59 | real*8 taugsurf(L_NSPECTI,L_NGAUSS-1) |
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60 | real*8 dco2 |
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61 | |
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62 | ! mixing ratio variables |
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63 | real*8 QVAR(L_LEVELS), WRATIO(L_LEVELS) |
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64 | real*8 KCOEF(4) |
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65 | integer NVAR(L_LEVELS) |
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66 | |
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67 | ! temporary variables for multiple aerosol calculation |
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68 | real*8 atemp |
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69 | real*8 btemp(L_NLAYRAD,L_NSPECTI) |
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70 | |
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71 | ! variables for k in units m^-1 |
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72 | real*8 rho, dz |
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73 | |
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74 | !======================================================================= |
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75 | ! Determine the total gas opacity throughout the column, for each |
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76 | ! spectral interval, NW, and each Gauss point, NG. |
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77 | |
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78 | ! write(*,*)'L_LEVELS',L_LEVELS |
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79 | ! write(*,*)'L_NSPECTI',L_NSPECTI |
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80 | DTAUI(:,:,:)=0. |
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81 | DTAUKI(:,:,:)=0. |
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82 | |
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83 | DO NG=1,L_NGAUSS-1 |
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84 | do NW=1,L_NSPECTI |
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85 | TAUGSURF(NW,NG) = 0.0D0 |
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86 | end do |
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87 | end do |
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88 | do K=2,L_LEVELS |
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89 | DPR(k) = PLEV(K)-PLEV(K-1) |
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90 | |
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91 | ! rho = PLEV(K)/(R*TMID(K)) |
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92 | rho = PMID(K)/(R*TMID(K)) |
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93 | dz = -DPR(k)/(g*rho) |
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94 | !print*,'rho=',rho |
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95 | !print*,'dz=',dz |
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96 | |
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97 | U(k) = Cmk*DPR(k) ! only Cmk line in optci.F |
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98 | ! soon to be replaced by m^-1 !!! |
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99 | |
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100 | call tpindex(PMID(K),TMID(K),QVAR(K),pfgasref,tgasref,WREFVAR, & |
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101 | LCOEF,MT(K),MP(K),NVAR(K),WRATIO(K)) |
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102 | |
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103 | do LK=1,4 |
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104 | LKCOEF(K,LK) = LCOEF(LK) |
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105 | end do |
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106 | |
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107 | DO NW=1,L_NSPECTI |
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108 | do iaer=1,naerkind |
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109 | TAEROS(K,NW,IAER) = TAUAERO(K,IAER) * QXIAER(K,NW,IAER) |
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110 | ! write(22,*) 'TB17 Taero IR:',K,NW,IAER,TAEROS(K,NW,IAER) |
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111 | end do |
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112 | END DO |
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113 | end do ! levels |
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114 | |
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115 | |
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116 | do K=2,L_LEVELS |
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117 | do nw=1,L_NSPECTI |
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118 | |
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119 | DCO2 = 0.0 ! continuum absorption (no longer used) |
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120 | |
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121 | do ng=1,L_NGAUSS-1 |
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122 | |
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123 | ! Now compute TAUGAS |
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124 | ! Interpolate between mixing ratios |
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125 | ! WRATIO = 0.0 if the requested amount is equal to, or outside the |
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126 | ! the data range |
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127 | |
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128 | |
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129 | if (L_REFVAR.eq.1)then ! added by RW for special no variable case |
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130 | KCOEF(1) = GASI(MT(K),MP(K),1,NW,NG) |
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131 | KCOEF(2) = GASI(MT(K),MP(K)+1,1,NW,NG) |
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132 | KCOEF(3) = GASI(MT(K)+1,MP(K)+1,1,NW,NG) |
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133 | KCOEF(4) = GASI(MT(K)+1,MP(K),1,NW,NG) |
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134 | else |
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135 | |
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136 | KCOEF(1) = GASI(MT(K),MP(K),NVAR(K),NW,NG) + WRATIO(K)* & |
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137 | (GASI(MT(K),MP(K),NVAR(K)+1,NW,NG) - & |
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138 | GASI(MT(K),MP(K),NVAR(K),NW,NG)) |
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139 | |
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140 | KCOEF(2) = GASI(MT(K),MP(K)+1,NVAR(K),NW,NG)+ WRATIO(K)* & |
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141 | (GASI(MT(K),MP(K)+1,NVAR(K)+1,NW,NG) - & |
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142 | GASI(MT(K),MP(K)+1,NVAR(K),NW,NG)) |
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143 | |
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144 | KCOEF(3)=GASI(MT(K)+1,MP(K)+1,NVAR(K),NW,NG)+WRATIO(K)* & |
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145 | (GASI(MT(K)+1,MP(K)+1,NVAR(K)+1,NW,NG) - & |
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146 | GASI(MT(K)+1,MP(K)+1,NVAR(K),NW,NG)) |
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147 | |
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148 | KCOEF(4) =GASI(MT(K)+1,MP(K),NVAR(K),NW,NG) + WRATIO(K)* & |
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149 | (GASI(MT(K)+1,MP(K),NVAR(K)+1,NW,NG) - & |
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150 | GASI(MT(K)+1,MP(K),NVAR(K),NW,NG)) |
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151 | endif |
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152 | |
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153 | ! Interpolate the gaseous k-coefficients to the requested T,P values |
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154 | |
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155 | ANS = LKCOEF(K,1)*KCOEF(1) + LKCOEF(K,2)*KCOEF(2) + & |
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156 | LKCOEF(K,3)*KCOEF(3) + LKCOEF(K,4)*KCOEF(4) |
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157 | |
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158 | TAUGAS = U(k)*ANS |
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159 | |
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160 | TAUGSURF(NW,NG) = TAUGSURF(NW,NG) + TAUGAS |
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161 | |
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162 | DTAUKI(K,nw,ng) = TAUGAS |
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163 | do iaer=1,naerkind |
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164 | DTAUKI(K,nw,ng) = DTAUKI(K,nw,ng) + TAEROS(K,NW,IAER) & |
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165 | + DCO2 ! For Kasting CIA |
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166 | end do |
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167 | |
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168 | end do |
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169 | |
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170 | ! Now fill in the "clear" part of the spectrum (NG = L_NGAUSS), |
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171 | ! which holds continuum opacity only |
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172 | |
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173 | NG = L_NGAUSS |
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174 | DTAUKI(K,nw,ng) = 0.0 |
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175 | do iaer=1,naerkind |
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176 | DTAUKI(K,nw,ng) = DTAUKI(K,nw,ng) + TAEROS(K,NW,IAER) & |
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177 | + DCO2 ! For parameterized continuum absorption |
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178 | end do ! a bug was found here!! |
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179 | |
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180 | end do |
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181 | end do |
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182 | |
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183 | |
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184 | !======================================================================= |
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185 | ! Now the full treatment for the layers, where besides the opacity |
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186 | ! we need to calculate the scattering albedo and asymmetry factors |
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187 | |
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188 | DO NW=1,L_NSPECTI |
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189 | DO K=2,L_LEVELS |
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190 | do iaer=1,naerkind |
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191 | TAUAEROLK(K,NW,IAER) = TAUAERO(K,IAER)*QSIAER(K,NW,IAER) |
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192 | end do |
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193 | ENDDO |
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194 | ENDDO |
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195 | |
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196 | DO NW=1,L_NSPECTI |
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197 | NG = L_NGAUSS |
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198 | DO L=1,L_NLAYRAD-1 |
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199 | |
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200 | K = 2*L+1 |
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201 | DTAUI(L,nw,ng) = DTAUKI(K,NW,NG) + DTAUKI(K+1,NW,NG)! + 1.e-50 |
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202 | |
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203 | atemp = 0. |
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204 | btemp(L,NW) = 0. |
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205 | do iaer=1,naerkind |
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206 | atemp = atemp + & |
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207 | GIAER(K,NW,IAER) * TAUAEROLK(K,NW,IAER) + & |
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208 | GIAER(K+1,NW,IAER) * TAUAEROLK(K+1,NW,IAER) |
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209 | btemp(L,NW) = btemp(L,NW) + TAUAEROLK(K,NW,IAER) + TAUAEROLK(K+1,NW,IAER) |
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210 | ! * + 1.e-10 |
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211 | end do |
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212 | |
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213 | if(DTAUI(L,NW,NG) .GT. 1.0E-9) then |
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214 | WBARI(L,nw,ng) = btemp(L,NW) / DTAUI(L,NW,NG) |
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215 | else |
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216 | WBARI(L,nw,ng) = 0.0D0 |
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217 | DTAUI(L,NW,NG) = 1.0E-9 |
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218 | endif |
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219 | |
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220 | if(btemp(L,NW) .GT. 0.0) then |
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221 | cosbi(L,NW,NG) = atemp/btemp(L,NW) |
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222 | else |
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223 | cosbi(L,NW,NG) = 0.0D0 |
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224 | end if |
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225 | |
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226 | END DO ! L vertical loop |
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227 | ! Last level |
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228 | |
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229 | L = L_NLAYRAD |
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230 | K = 2*L+1 |
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231 | DTAUI(L,nw,ng) = DTAUKI(K,NW,NG) ! + 1.e-50 |
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232 | btemp(L,NW) = 0 |
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233 | do iaer=1,naerkind |
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234 | btemp(L,NW) = btemp(L,NW) + TAUAEROLK(K,NW,IAER) |
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235 | enddo |
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236 | |
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237 | atemp = 0. |
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238 | if(DTAUI(L,NW,NG) .GT. 1.0D-9) then |
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239 | do iaer=1,naerkind |
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240 | atemp = atemp + GIAER(K,NW,IAER) * TAUAEROLK(K,NW,IAER) |
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241 | end do |
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242 | WBARI(L,nw,ng) = btemp(L,NW) / DTAUI(L,NW,NG) |
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243 | else |
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244 | WBARI(L,nw,ng) = 0.0D0 |
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245 | DTAUI(L,NW,NG) = 1.0D-9 |
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246 | endif |
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247 | |
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248 | if(btemp(L,NW) .GT. 0.0d0) then |
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249 | cosbi(L,NW,NG) = atemp/btemp(L,NW) |
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250 | else |
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251 | cosbi(L,NW,NG) = 0.0D0 |
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252 | end if |
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253 | |
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254 | ! Now the other Gauss points, if needed. |
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255 | |
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256 | DO NG=1,L_NGAUSS-1 |
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257 | IF(TAUGSURF(NW,NG) .gt. TLIMIT) THEN |
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258 | |
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259 | DO L=1,L_NLAYRAD |
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260 | K = 2*L+1 |
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261 | DTAUI(L,nw,ng) = DTAUKI(K,NW,NG)+DTAUKI(K+1,NW,NG)! + 1.e-50 |
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262 | |
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263 | if(DTAUI(L,NW,NG) .GT. 1.0E-9) then |
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264 | WBARI(L,nw,ng) = btemp(L,NW) / DTAUI(L,NW,NG) |
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265 | else |
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266 | WBARI(L,nw,ng) = 0.0D0 |
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267 | DTAUI(L,NW,NG) = 1.0E-9 |
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268 | endif |
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269 | |
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270 | cosbi(L,NW,NG) = cosbi(L,NW,L_NGAUSS) |
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271 | END DO ! L vertical loop |
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272 | END IF |
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273 | |
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274 | END DO ! NG Gauss loop |
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275 | END DO ! NW spectral loop |
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276 | |
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277 | ! Total extinction optical depths |
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278 | |
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279 | DO NW=1,L_NSPECTI |
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280 | DO NG=1,L_NGAUSS ! full gauss loop |
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281 | TAUI(1,NW,NG)=0.0D0 |
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282 | DO L=1,L_NLAYRAD |
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283 | TAUI(L+1,NW,NG)=TAUI(L,NW,NG)+DTAUI(L,NW,NG) |
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284 | END DO |
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285 | |
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286 | TAUCUMI(1,NW,NG)=0.0D0 |
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287 | DO K=2,L_LEVELS |
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288 | TAUCUMI(K,NW,NG)=TAUCUMI(K-1,NW,NG)+DTAUKI(K,NW,NG) |
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289 | END DO |
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290 | END DO ! end full gauss loop |
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291 | END DO |
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292 | |
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293 | |
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294 | return |
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295 | end subroutine optci |
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296 | |
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