1 | MODULE optci_mod |
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2 | |
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3 | IMPLICIT NONE |
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4 | |
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5 | CONTAINS |
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6 | |
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7 | subroutine optci(PLEV,TLEV,DTAUI,TAUCUMI, & |
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8 | QXIAER,QSIAER,GIAER,COSBI,WBARI,TAUAERO, & |
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9 | TMID,PMID,TAUGSURF,QVAR,MUVAR) |
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10 | |
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11 | use radinc_h, only: L_LEVELS, L_NLAYRAD, L_NSPECTI, L_NGAUSS, & |
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12 | L_NLEVRAD, L_REFVAR, naerkind |
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13 | use radcommon_h, only: gasi,tlimit,wrefVAR,Cmk,tgasref,pfgasref,wnoi,scalep,indi,glat_ig |
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14 | use gases_h, only: gfrac, ngasmx, igas_N2, igas_He, igas_H2O, igas_H2, & |
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15 | igas_CH4, igas_N2 |
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16 | use comcstfi_mod, only: g, r, mugaz |
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17 | use callkeys_mod, only: kastprof,continuum,graybody |
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18 | use recombin_corrk_mod, only: corrk_recombin, gasi_recomb |
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19 | use tpindex_mod, only: tpindex |
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20 | |
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21 | implicit none |
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22 | |
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23 | !================================================================== |
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24 | ! |
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25 | ! Purpose |
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26 | ! ------- |
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27 | ! Calculates longwave optical constants at each level. For each |
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28 | ! layer and spectral interval in the IR it calculates WBAR, DTAU |
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29 | ! and COSBAR. For each level it calculates TAU. |
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30 | ! |
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31 | ! TAUCUMI(L,LW) is the cumulative optical depth at level L (or alternatively |
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32 | ! at the *bottom* of layer L), LW is the spectral wavelength interval. |
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33 | ! |
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34 | ! TLEV(L) - Temperature at the layer boundary (i.e., level) |
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35 | ! PLEV(L) - Pressure at the layer boundary (i.e., level) |
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36 | ! |
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37 | ! Authors |
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38 | ! ------- |
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39 | ! Adapted from the NASA Ames code by R. Wordsworth (2009) |
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40 | ! |
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41 | !================================================================== |
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42 | |
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43 | |
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44 | real*8,intent(out) :: DTAUI(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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45 | real*8 DTAUKI(L_LEVELS,L_NSPECTI,L_NGAUSS) |
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46 | real*8 TAUI(L_NLEVRAD,L_NSPECTI,L_NGAUSS) |
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47 | real*8,intent(out) :: TAUCUMI(L_LEVELS,L_NSPECTI,L_NGAUSS) |
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48 | real*8,intent(in) :: PLEV(L_LEVELS) |
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49 | real*8,intent(in) :: TLEV(L_LEVELS) ! not used |
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50 | real*8,intent(in) :: TMID(L_LEVELS) |
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51 | real*8,intent(in) :: PMID(L_LEVELS) |
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52 | real*8,intent(out) :: COSBI(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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53 | real*8,intent(out) :: WBARI(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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54 | |
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55 | ! for aerosols |
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56 | real*8,intent(in) :: QXIAER(L_LEVELS,L_NSPECTI,NAERKIND) |
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57 | real*8,intent(in) :: QSIAER(L_LEVELS,L_NSPECTI,NAERKIND) |
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58 | real*8,intent(in) :: GIAER(L_LEVELS,L_NSPECTI,NAERKIND) |
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59 | real*8,intent(in) :: TAUAERO(L_LEVELS,NAERKIND) |
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60 | |
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61 | ! local variables (saved for convenience as need be allocated) |
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62 | real*8,save,allocatable :: TAUAEROLK(:,:,:) |
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63 | real*8,save,allocatable :: TAEROS(:,:,:) |
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64 | !$OMP THREADPRIVATE(TAUAEROLK,TAEROS) |
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65 | |
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66 | integer L, NW, NG, K, LK, IAER |
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67 | integer MT(L_LEVELS), MP(L_LEVELS), NP(L_LEVELS) |
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68 | real*8 ANS, TAUGAS |
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69 | real*8 DPR(L_LEVELS), U(L_LEVELS) |
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70 | real*8 LCOEF(4), LKCOEF(L_LEVELS,4) |
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71 | |
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72 | real*8,intent(out) :: taugsurf(L_NSPECTI,L_NGAUSS-1) |
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73 | real*8 DCONT,DAERO |
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74 | double precision wn_cont, p_cont, p_air, T_cont, dtemp, dtempc |
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75 | double precision p_cross |
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76 | |
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77 | ! variable species mixing ratio variables |
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78 | real*8,intent(in) :: QVAR(L_LEVELS) |
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79 | real*8,intent(in) :: MUVAR(L_LEVELS) |
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80 | real*8 WRATIO(L_LEVELS) |
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81 | real*8 KCOEF(4) |
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82 | integer NVAR(L_LEVELS) |
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83 | |
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84 | ! temporary variables to reduce memory access time to gasi |
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85 | real*8 tmpk(2,2) |
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86 | real*8 tmpkvar(2,2,2) |
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87 | |
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88 | ! temporary variables for multiple aerosol calculation |
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89 | real*8 atemp |
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90 | real*8 btemp(L_NLAYRAD,L_NSPECTI) |
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91 | |
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92 | ! variables for k in units m^-1 |
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93 | real*8 dz(L_LEVELS) |
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94 | !real*8 rho !! see test below |
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95 | |
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96 | integer igas, jgas |
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97 | |
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98 | integer interm |
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99 | |
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100 | logical :: firstcall=.true. |
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101 | !$OMP THREADPRIVATE(firstcall) |
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102 | |
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103 | !--- Kasting's CIA ---------------------------------------- |
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104 | !real*8, parameter :: Ci(L_NSPECTI)=[ & |
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105 | ! 3.8E-5, 1.2E-5, 2.8E-6, 7.6E-7, 4.5E-7, 2.3E-7, & |
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106 | ! 5.4E-7, 1.6E-6, 0.0, & |
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107 | ! 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, & |
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108 | ! 0.0, 4.0E-7, 4.0E-6, 1.4E-5, & |
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109 | ! 1.0E-5, 1.2E-6, 2.0E-7, 5.0E-8, 3.0E-8, 0.0 ] |
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110 | !real*8, parameter :: Ti(L_NSPECTI)=[ -2.2, -1.9, & |
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111 | ! -1.7, -1.7, -1.7, -1.7, -1.7, -1.7, & |
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112 | ! 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, & |
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113 | ! -1.7,-1.7,-1.7,-1.7,-1.7,-1.7,-1.7, -1.7,0.0 ] |
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114 | !---------------------------------------------------------- |
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115 | |
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116 | if (firstcall) then |
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117 | ! allocate local arrays of size "naerkind" (which are also |
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118 | ! "saved" so that this is done only once in for all even if |
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119 | ! we don't need to store the value from a time step to the next) |
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120 | allocate(TAUAEROLK(L_LEVELS,L_NSPECTI,NAERKIND)) |
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121 | allocate(TAEROS(L_LEVELS,L_NSPECTI,NAERKIND)) |
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122 | firstcall=.false. |
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123 | endif ! of if (firstcall) |
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124 | |
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125 | !! AS: to save time in computing continuum (see bilinearbig) |
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126 | IF (.not.ALLOCATED(indi)) THEN |
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127 | ALLOCATE(indi(L_NSPECTI,ngasmx,ngasmx)) |
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128 | indi = -9999 ! this initial value means "to be calculated" |
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129 | ENDIF |
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130 | |
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131 | !======================================================================= |
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132 | ! Determine the total gas opacity throughout the column, for each |
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133 | ! spectral interval, NW, and each Gauss point, NG. |
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134 | |
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135 | taugsurf(:,:) = 0.0 |
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136 | dpr(:) = 0.0 |
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137 | lkcoef(:,:) = 0.0 |
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138 | |
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139 | do K=2,L_LEVELS |
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140 | DPR(k) = PLEV(K)-PLEV(K-1) |
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141 | |
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142 | !--- Kasting's CIA ---------------------------------------- |
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143 | !dz(k)=dpr(k)*189.02*TMID(K)/(0.03720*PMID(K)) |
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144 | ! this is N2 path length (in cm) as written by Francois |
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145 | ! delta_z = delta_p * R_specific * T / (g * P) |
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146 | ! But Kasting states that W is in units of _atmosphere_ cm |
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147 | ! So we do |
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148 | !dz(k)=dz(k)*(PMID(K)/1013.25) |
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149 | !dz(k)=dz(k)/100.0 ! in m for SI calc |
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150 | !---------------------------------------------------------- |
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151 | |
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152 | ! if we have continuum opacities, we need dz |
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153 | if(kastprof)then |
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154 | dz(k) = dpr(k)*(1000.0d0*8.3145d0/muvar(k))*TMID(K)/(g*PMID(K)) |
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155 | U(k) = Cmk*DPR(k)*mugaz/muvar(k) |
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156 | else |
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157 | dz(k) = dpr(k)*R*TMID(K)/(glat_ig*PMID(K))*mugaz/muvar(k) |
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158 | U(k) = Cmk*DPR(k)*mugaz/muvar(k) ! only Cmk line in optci.F |
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159 | !JL13 the mugaz/muvar factor takes into account water meanmolecular weight if water is present |
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160 | endif |
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161 | |
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162 | call tpindex(PMID(K),TMID(K),QVAR(K),pfgasref,tgasref,WREFVAR, & |
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163 | LCOEF,MT(K),MP(K),NVAR(K),WRATIO(K)) |
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164 | |
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165 | do LK=1,4 |
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166 | LKCOEF(K,LK) = LCOEF(LK) |
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167 | end do |
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168 | end do ! levels |
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169 | |
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170 | ! Spectral dependance of aerosol absorption |
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171 | do iaer=1,naerkind |
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172 | DO NW=1,L_NSPECTI |
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173 | do K=2,L_LEVELS |
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174 | TAEROS(K,NW,IAER) = TAUAERO(K,IAER) * QXIAER(K,NW,IAER) |
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175 | end do ! levels |
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176 | END DO |
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177 | end do |
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178 | |
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179 | do NW=1,L_NSPECTI |
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180 | |
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181 | do K=2,L_LEVELS |
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182 | |
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183 | DAERO=SUM(TAEROS(K,NW,1:naerkind)) ! aerosol absorption |
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184 | |
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185 | DCONT = 0.0d0 ! continuum absorption |
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186 | |
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187 | if(continuum.and.(.not.graybody))then |
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188 | ! include continua if necessary |
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189 | wn_cont = dble(wnoi(nw)) |
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190 | T_cont = dble(TMID(k)) |
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191 | do igas=1,ngasmx |
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192 | |
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193 | if(gfrac(igas).eq.-1)then ! variable |
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194 | p_cont = dble(PMID(k)*scalep*QVAR(k)) ! qvar = mol/mol |
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195 | else |
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196 | p_cont = dble(PMID(k)*scalep*gfrac(igas)*(1.-QVAR(k))) |
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197 | endif |
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198 | |
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199 | dtemp=0.0d0 |
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200 | if(igas.eq.igas_N2)then |
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201 | |
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202 | interm = indi(nw,igas,igas) |
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203 | call interpolateN2N2(wn_cont,T_cont,p_cont,dtemp,.false.,interm) |
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204 | indi(nw,igas,igas) = interm |
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205 | |
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206 | ! elseif(igas.eq.igas_H2)then !AF24: removed |
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207 | |
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208 | elseif(igas.eq.igas_CH4)then |
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209 | |
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210 | ! first do self-induced absorption |
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211 | interm = indi(nw,igas,igas) |
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212 | call interpolateCH4CH4(wn_cont,T_cont,p_cont,dtemp,.false.,interm) |
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213 | indi(nw,igas,igas) = interm |
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214 | |
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215 | ! then cross-interactions with other gases !AF24: removed |
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216 | |
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217 | ! elseif(igas.eq.igas_H2O.and.T_cont.gt.100.0)then !AF24: removed |
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218 | |
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219 | endif |
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220 | DCONT = DCONT + dtemp |
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221 | enddo |
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222 | |
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223 | ! Oobleck test |
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224 | !rho = PMID(k)*scalep / (TMID(k)*286.99) |
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225 | !if(WNOI(nw).gt.300.0 .and. WNOI(nw).lt.500.0)then |
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226 | ! DCONT = rho * 0.125 * 4.6e-4 |
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227 | !elseif(WNOI(nw).gt.500.0 .and. WNOI(nw).lt.700.0)then |
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228 | ! DCONT = 1000*dpr(k) * 1.0 * 4.6e-4 / g |
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229 | ! DCONT = rho * 1.0 * 4.6e-4 |
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230 | !elseif(WNOI(nw).gt.700.0 .and. WNOI(nw).lt.900.0)then |
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231 | ! DCONT = rho * 0.125 * 4.6e-4 |
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232 | !endif |
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233 | |
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234 | DCONT = DCONT*dz(k) |
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235 | |
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236 | endif |
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237 | |
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238 | do ng=1,L_NGAUSS-1 |
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239 | |
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240 | ! Now compute TAUGAS |
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241 | |
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242 | ! Interpolate between water mixing ratios |
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243 | ! WRATIO = 0.0 if the requested water amount is equal to, or outside the |
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244 | ! the water data range |
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245 | |
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246 | if(L_REFVAR.eq.1)then ! added by RW for special no variable case |
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247 | |
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248 | ! JVO 2017 : added tmpk because the repeated calls to gasi/v increased dramatically |
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249 | ! the execution time of optci/v -> ~ factor 2 on the whole radiative |
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250 | ! transfer on the tested simulations ! |
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251 | |
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252 | IF (corrk_recombin) THEN ! added by JVO |
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253 | tmpk = GASI_RECOMB(MT(K):MT(K)+1,MP(K):MP(K)+1,1,NW,NG) ! contains the mix of recombined species |
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254 | ELSE |
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255 | tmpk = GASI(MT(K):MT(K)+1,MP(K):MP(K)+1,1,NW,NG) |
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256 | ENDIF |
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257 | |
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258 | KCOEF(1) = tmpk(1,1) ! KCOEF(1) = GASI(MT(K),MP(K),1,NW,NG) |
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259 | KCOEF(2) = tmpk(1,2) ! KCOEF(2) = GASI(MT(K),MP(K)+1,1,NW,NG) |
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260 | KCOEF(3) = tmpk(2,2) ! KCOEF(3) = GASI(MT(K)+1,MP(K)+1,1,NW,NG) |
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261 | KCOEF(4) = tmpk(2,1) ! KCOEF(4) = GASI(MT(K)+1,MP(K),1,NW,NG) |
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262 | |
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263 | else |
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264 | |
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265 | IF (corrk_recombin) THEN ! added by JVO |
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266 | tmpkvar = GASI_RECOMB(MT(K):MT(K)+1,MP(K):MP(K)+1,NVAR(K):NVAR(K)+1,NW,NG) |
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267 | ELSE |
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268 | tmpkvar = GASI(MT(K):MT(K)+1,MP(K):MP(K)+1,NVAR(K):NVAR(K)+1,NW,NG) |
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269 | ENDIF |
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270 | |
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271 | KCOEF(1) = tmpkvar(1,1,1) + WRATIO(K) * & |
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272 | ( tmpkvar(1,1,2)-tmpkvar(1,1,1) ) |
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273 | |
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274 | KCOEF(2) = tmpkvar(1,2,1) + WRATIO(K) * & |
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275 | ( tmpkvar(1,2,2)-tmpkvar(1,2,1) ) |
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276 | |
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277 | KCOEF(3) = tmpkvar(2,2,1) + WRATIO(K) * & |
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278 | ( tmpkvar(2,2,2)-tmpkvar(2,2,1) ) |
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279 | |
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280 | KCOEF(4) = tmpkvar(2,1,1) + WRATIO(K) * & |
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281 | ( tmpkvar(2,1,2)-tmpkvar(2,1,1) ) |
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282 | |
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283 | endif |
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284 | |
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285 | ! Interpolate the gaseous k-coefficients to the requested T,P values |
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286 | |
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287 | ANS = LKCOEF(K,1)*KCOEF(1) + LKCOEF(K,2)*KCOEF(2) + & |
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288 | LKCOEF(K,3)*KCOEF(3) + LKCOEF(K,4)*KCOEF(4) |
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289 | |
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290 | TAUGAS = U(k)*ANS |
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291 | |
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292 | TAUGSURF(NW,NG) = TAUGSURF(NW,NG) + TAUGAS + DCONT |
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293 | DTAUKI(K,nw,ng) = TAUGAS & |
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294 | + DCONT & ! For parameterized continuum absorption |
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295 | + DAERO ! For aerosol absorption |
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296 | |
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297 | end do |
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298 | |
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299 | ! Now fill in the "clear" part of the spectrum (NG = L_NGAUSS), |
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300 | ! which holds continuum opacity only |
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301 | |
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302 | NG = L_NGAUSS |
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303 | DTAUKI(K,nw,ng) = 0.d0 & |
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304 | + DCONT & ! For parameterized continuum absorption |
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305 | + DAERO ! For aerosol absorption |
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306 | |
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307 | end do |
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308 | end do |
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309 | |
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310 | !======================================================================= |
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311 | ! Now the full treatment for the layers, where besides the opacity |
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312 | ! we need to calculate the scattering albedo and asymmetry factors |
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313 | |
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314 | do iaer=1,naerkind |
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315 | DO NW=1,L_NSPECTI |
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316 | DO K=2,L_LEVELS |
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317 | TAUAEROLK(K,NW,IAER) = TAUAERO(K,IAER)*QSIAER(K,NW,IAER) ! effect of scattering albedo |
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318 | ENDDO |
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319 | ENDDO |
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320 | end do |
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321 | |
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322 | DO NW=1,L_NSPECTI |
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323 | DO L=1,L_NLAYRAD-1 |
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324 | K = 2*L+1 |
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325 | btemp(L,NW) = SUM(TAUAEROLK(K,NW,1:naerkind)) + SUM(TAUAEROLK(K+1,NW,1:naerkind)) |
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326 | END DO ! L vertical loop |
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327 | |
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328 | ! Last level |
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329 | L = L_NLAYRAD |
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330 | K = 2*L+1 |
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331 | btemp(L,NW) = SUM(TAUAEROLK(K,NW,1:naerkind)) |
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332 | |
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333 | END DO ! NW spectral loop |
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334 | |
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335 | |
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336 | DO NW=1,L_NSPECTI |
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337 | NG = L_NGAUSS |
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338 | DO L=1,L_NLAYRAD-1 |
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339 | |
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340 | K = 2*L+1 |
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341 | DTAUI(L,nw,ng) = DTAUKI(K,NW,NG) + DTAUKI(K+1,NW,NG)! + 1.e-50 |
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342 | |
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343 | atemp = 0. |
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344 | if(DTAUI(L,NW,NG) .GT. 1.0D-9) then |
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345 | do iaer=1,naerkind |
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346 | atemp = atemp + & |
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347 | GIAER(K,NW,IAER) * TAUAEROLK(K,NW,IAER) + & |
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348 | GIAER(K+1,NW,IAER) * TAUAEROLK(K+1,NW,IAER) |
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349 | end do |
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350 | WBARI(L,nw,ng) = btemp(L,nw) / DTAUI(L,NW,NG) |
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351 | else |
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352 | WBARI(L,nw,ng) = 0.0D0 |
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353 | DTAUI(L,NW,NG) = 1.0D-9 |
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354 | endif |
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355 | |
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356 | if(btemp(L,nw) .GT. 0.0d0) then |
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357 | cosbi(L,NW,NG) = atemp/btemp(L,nw) |
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358 | else |
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359 | cosbi(L,NW,NG) = 0.0D0 |
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360 | end if |
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361 | |
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362 | END DO ! L vertical loop |
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363 | |
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364 | ! Last level |
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365 | |
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366 | L = L_NLAYRAD |
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367 | K = 2*L+1 |
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368 | DTAUI(L,nw,ng) = DTAUKI(K,NW,NG) ! + 1.e-50 |
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369 | |
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370 | atemp = 0. |
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371 | if(DTAUI(L,NW,NG) .GT. 1.0D-9) then |
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372 | do iaer=1,naerkind |
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373 | atemp = atemp + GIAER(K,NW,IAER) * TAUAEROLK(K,NW,IAER) |
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374 | end do |
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375 | WBARI(L,nw,ng) = btemp(L,nw) / DTAUI(L,NW,NG) |
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376 | else |
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377 | WBARI(L,nw,ng) = 0.0D0 |
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378 | DTAUI(L,NW,NG) = 1.0D-9 |
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379 | endif |
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380 | |
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381 | if(btemp(L,nw) .GT. 0.0d0) then |
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382 | cosbi(L,NW,NG) = atemp/btemp(L,nw) |
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383 | else |
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384 | cosbi(L,NW,NG) = 0.0D0 |
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385 | end if |
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386 | |
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387 | |
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388 | ! Now the other Gauss points, if needed. |
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389 | |
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390 | DO NG=1,L_NGAUSS-1 |
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391 | IF(TAUGSURF(NW,NG) .gt. TLIMIT) THEN |
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392 | |
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393 | DO L=1,L_NLAYRAD-1 |
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394 | K = 2*L+1 |
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395 | DTAUI(L,nw,ng) = DTAUKI(K,NW,NG)+DTAUKI(K+1,NW,NG)! + 1.e-50 |
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396 | |
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397 | if(DTAUI(L,NW,NG) .GT. 1.0D-9) then |
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398 | |
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399 | WBARI(L,nw,ng) = btemp(L,nw) / DTAUI(L,NW,NG) |
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400 | |
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401 | else |
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402 | WBARI(L,nw,ng) = 0.0D0 |
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403 | DTAUI(L,NW,NG) = 1.0D-9 |
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404 | endif |
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405 | |
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406 | cosbi(L,NW,NG) = cosbi(L,NW,L_NGAUSS) |
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407 | END DO ! L vertical loop |
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408 | |
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409 | ! Last level |
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410 | L = L_NLAYRAD |
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411 | K = 2*L+1 |
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412 | DTAUI(L,nw,ng) = DTAUKI(K,NW,NG)! + 1.e-50 |
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413 | |
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414 | if(DTAUI(L,NW,NG) .GT. 1.0D-9) then |
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415 | |
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416 | WBARI(L,nw,ng) = btemp(L,nw) / DTAUI(L,NW,NG) |
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417 | |
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418 | else |
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419 | WBARI(L,nw,ng) = 0.0D0 |
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420 | DTAUI(L,NW,NG) = 1.0D-9 |
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421 | endif |
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422 | |
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423 | cosbi(L,NW,NG) = cosbi(L,NW,L_NGAUSS) |
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424 | |
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425 | END IF |
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426 | |
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427 | END DO ! NG Gauss loop |
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428 | END DO ! NW spectral loop |
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429 | |
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430 | ! Total extinction optical depths |
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431 | |
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432 | DO NG=1,L_NGAUSS ! full gauss loop |
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433 | DO NW=1,L_NSPECTI |
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434 | TAUCUMI(1,NW,NG)=0.0D0 |
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435 | DO K=2,L_LEVELS |
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436 | TAUCUMI(K,NW,NG)=TAUCUMI(K-1,NW,NG)+DTAUKI(K,NW,NG) |
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437 | END DO |
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438 | END DO ! end full gauss loop |
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439 | END DO |
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440 | |
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441 | ! be aware when comparing with textbook results |
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442 | ! (e.g. Pierrehumbert p. 218) that |
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443 | ! taucumi does not take the <cos theta>=0.5 factor into |
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444 | ! account. It is the optical depth for a vertically |
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445 | ! ascending ray with angle theta = 0. |
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446 | |
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447 | !open(127,file='taucum.out') |
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448 | !do nw=1,L_NSPECTI |
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449 | ! write(127,*) taucumi(L_LEVELS,nw,L_NGAUSS) |
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450 | !enddo |
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451 | !close(127) |
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452 | |
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453 | ! print*,'WBARI' |
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454 | ! print*,WBARI |
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455 | ! print*,'DTAUI' |
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456 | ! print*,DTAUI |
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457 | ! call abort |
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458 | |
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459 | end subroutine optci |
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460 | |
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461 | END MODULE optci_mod |
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462 | |
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