1 | subroutine nlte_ch4(ngrid,nlayer,nq,pplay,pplev,pt,vmrch4,eps23,eps33,eps76) |
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2 | |
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3 | use comgeomfi_h |
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4 | use callkeys_mod, only: strobel |
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5 | use tracer_h, only: igcm_n2,mmol |
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6 | use comcstfi_mod, only: pi, g, cpp,r |
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7 | implicit none |
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8 | |
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9 | !================================================================== |
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10 | ! Purpose |
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11 | ! ------- |
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12 | ! Calculation of epsilon - non LTE efficiency factor |
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13 | ! For CH4 heating and cooling rate calculation |
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14 | ! Cf Strobel et al 1996 |
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15 | ! |
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16 | ! Inputs |
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17 | ! ------ |
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18 | ! ngrid Number of vertical columns |
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19 | ! nlayer Number of layers |
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20 | ! pplay(ngrid,nlayer) Pressure layers |
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21 | ! pt |
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22 | ! |
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23 | ! Outputs |
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24 | ! ------- |
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25 | ! |
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26 | ! eps_sw ! efficiency factor for heating rate |
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27 | ! eps_lw ! efficiency factor for cooling rate |
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28 | ! |
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29 | ! Authors |
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30 | ! ------- |
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31 | ! Tanguy Bertrand (2015,2022) |
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32 | ! |
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33 | !================================================================== |
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34 | |
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35 | !----------------------------------------------------------------------- |
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36 | |
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37 | ! Arguments |
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38 | |
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39 | INTEGER ngrid, nlayer, nq |
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40 | REAL pplay(ngrid,nlayer) |
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41 | REAL pplev(ngrid,nlayer) |
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42 | REAL pt(ngrid,nlayer) |
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43 | REAL vmrch4(ngrid,nlayer) |
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44 | |
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45 | !----------------------------------------------------------------------- |
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46 | ! Local variables |
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47 | |
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48 | INTEGER l,ig |
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49 | |
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50 | REAL cbol ! Boltzman constant |
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51 | REAL avog ! avogadro constant |
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52 | REAL beta23 |
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53 | REAL beta33 |
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54 | REAL nd(ngrid,nlayer) ! density number cm-3 |
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55 | REAL na(ngrid,nlayer) ! column density number cm-2 |
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56 | REAL rho(ngrid,nlayer) ! density of atmosphere |
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57 | REAL kn3,k3,k2n4,k3n4,k4 |
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58 | REAL An3,A3,A2n4,A3n4,A4 |
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59 | REAL dphin3,dphi3,dphi2n4,dphi3n4,dphi4 |
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60 | REAL phin3(ngrid,nlayer) |
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61 | REAL phi3(ngrid,nlayer) |
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62 | REAL phi2n4(ngrid,nlayer) |
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63 | REAL phi3n4(ngrid,nlayer) |
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64 | REAL phi4(ngrid,nlayer) |
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65 | REAL phi4T(ngrid,nlayer) |
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66 | |
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67 | ! DATA from Strobel et al 1996 |
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68 | REAL, DIMENSION(22) :: gam2 ! band escape fonction 2.3 |
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69 | REAL, DIMENSION(22) :: Naval2 ! column density number 2.3 |
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70 | REAL, DIMENSION(22) :: gam3 ! band escape fonction 3.3 |
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71 | REAL, DIMENSION(22) :: Naval3 ! column density number 3.3 |
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72 | REAL gammafi23(nlayer),gammafi33(nlayer) ! Band espace fonction |
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73 | REAL gammafi23mod(nlayer),gammafi33mod(nlayer) ! Band espace fonction |
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74 | REAL vmr |
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75 | REAL k4zT ! function to calculate k4 depending on T and vmr |
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76 | REAL log_square ! log function |
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77 | REAL log_affine ! log function |
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78 | REAL ratio_affine ! linear approx function to calculate ratio for gamma calculation |
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79 | REAL ratio_square ! |
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80 | REAL ratio_sq,ratio_af |
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81 | |
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82 | ! Output |
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83 | REAL,intent(out) :: eps23(ngrid,nlayer) |
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84 | REAL,intent(out) :: eps33(ngrid,nlayer) |
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85 | REAL,intent(out) :: eps76(ngrid,nlayer) |
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86 | |
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87 | ! Option simplified coefficient |
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88 | REAL klw, ksw, eps_sw1Pa |
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89 | |
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90 | !----------------------------------------------------------------------- |
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91 | eps23(:,:)=1. |
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92 | eps33(:,:)=1. |
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93 | eps76(:,:)=1. |
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94 | |
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95 | IF (strobel) then |
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96 | |
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97 | ! Constantes |
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98 | cbol=1.3806488e-23 !Boltzman constant |
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99 | avog=6.022141e23 |
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100 | |
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101 | ! band 3 |
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102 | k3=2.8e-11 !cm-3 |
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103 | A3=25.2 |
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104 | dphi3=k3/A3 |
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105 | ! band n3 |
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106 | kn3=2.8e-11 !cm-3 |
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107 | An3=27.3 |
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108 | dphin3=kn3/An3 |
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109 | ! band 3n4 |
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110 | k3n4=1.16e-11 !cm-3 |
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111 | A3n4=2.12 |
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112 | dphi3n4=k3n4/(3.*A3n4) |
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113 | ! band 4 |
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114 | !! Here we use function k4zT instead of constant k4 |
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115 | k4=4.5e-16 !cm-3 |
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116 | A4=2.12 |
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117 | dphi4=k4/A4 |
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118 | ! band 2n4 |
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119 | k2n4=1.16e-11 |
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120 | A2n4=2.12 |
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121 | dphi2n4=k2n4/(2.*A2n4) |
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122 | |
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123 | ! 2.3 band : |
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124 | beta23=0.09 |
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125 | ! 3.3 band : |
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126 | beta33=0.13 |
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127 | |
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128 | ! Escape Function Gamma (Data Strobel et al) : |
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129 | ! 100 K 2.3 |
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130 | Naval2=(/1.00000000e+10,1.30000000e+15,2.92766055e+15,6.59322793e+15,1.48482564e+16,3.34389650e+16, & |
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131 | 7.53061067e+16,1.69592860e+17,3.81931020e+17,8.60126447e+17,1.93704482e+18,4.36231516e+18, & |
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132 | 9.82413694e+18,2.21244140e+19,4.98252108e+19,1.12208695e+20,2.52699209e+20,5.69090388e+20, & |
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133 | 1.28161806e+21,2.88626357e+21,6.50000000e+21,1.00000000e+24/) |
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134 | gam2=(/1.00000000e+00,1.00000000e+00,1.00000000e+00,1.00000000e+00,1.00000000e+00,9.90000000e-01, & |
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135 | 9.80000000e-01,9.50000000e-0,9.00000000e-01,8.00000000e-01,7.00000000e-01,5.00000000e-01, & |
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136 | 3.50000000e-01,2.20000000e-01,1.20000000e-01,6.50000000e-02,3.20000000e-02,1.40000000e-02, & |
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137 | 6.20000000e-03,2.50000000e-03,1.05000000e-03,4.83227951e-06/) |
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138 | |
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139 | ! 100 K 3.3 |
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140 | Naval3=(/1.00000000e+10,1.30000000e+15,2.92766055e+15,6.59322793e+15,1.48482564e+16,3.34389650e+16, & |
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141 | 7.53061067e+16,1.69592860e+17,3.81931020e+17,8.60126447e+17,1.93704482e+18,4.36231516e+18, & |
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142 | 9.82413694e+18,2.21244140e+19,4.98252108e+19,1.12208695e+20,2.52699209e+20,5.69090388e+20, & |
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143 | 1.28161806e+21,2.88626357e+21,6.50000000e+21,1.00000000e+24/) |
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144 | gam3=(/1.00000000e+00,9.80000000e-01,9.00000000e-01,8.50000000e-01,7.00000000e-01,5.00000000e-01, & |
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145 | 3.00000000e-01,1.50000000e-01,1.00000000e-01,6.00000000e-02,4.00000000e-02,2.30000000e-02, & |
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146 | 1.45000000e-02,9.00000000e-03,5.00000000e-03,3.00000000e-03,1.50000000e-03,8.00000000e-04, & |
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147 | 3.80000000e-04,1.80000000e-04,8.30000000e-05,6.81737544e-07/) |
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148 | |
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149 | DO ig=1,ngrid |
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150 | |
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151 | phi3n4(ig,:)=1. |
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152 | phi2n4(ig,:)=1. |
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153 | phin3(ig,:)=1. |
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154 | phi4(ig,:)=1. |
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155 | nd(ig,:)=1. |
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156 | na(ig,:)=1. |
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157 | |
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158 | !write(*,*) 'TB22 pplev=',pplev(1,:) |
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159 | !write(*,*) 'TB22 tlev=',pt(1,:) |
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160 | |
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161 | DO l=1,nlayer |
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162 | !!calculation of density |
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163 | rho(ig,l)=pplay(ig,l)/(r*pt(ig,l)) |
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164 | |
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165 | !!calculation of column number density for ch4 (cm-2) |
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166 | na(ig,l)=vmrch4(ig,l)/100./(mmol(igcm_n2)*1.e-3)* & |
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167 | pplev(ig,l)/g*avog*1.e-4 |
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168 | |
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169 | !!calculation of atmospheric number density (cm-3) for each layer |
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170 | nd(ig,l)=rho(ig,l)/(mmol(igcm_n2)*1.e-3)*avog*1.e-6 |
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171 | |
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172 | !!calculation of the phi : |
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173 | phin3(ig,l)=dphin3*nd(ig,l) |
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174 | phi3(ig,l)=dphi3*nd(ig,l) |
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175 | phi2n4(ig,l)=dphi2n4*nd(ig,l) |
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176 | phi3n4(ig,l)=dphi3n4*nd(ig,l) |
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177 | phi4(ig,l)=dphi4*nd(ig,l) |
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178 | !! Getting phi4 depending on T and vmr |
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179 | vmr=vmrch4(ig,l)/100. |
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180 | phi4T(ig,l)=k4zT(pt(ig,l),vmr)/A4*nd(ig,l) |
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181 | ENDDO |
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182 | !write(*,*) 'TB22 nd=',nd(1,:) |
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183 | !write(*,*) 'TB22 vmr=',vmrch4 |
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184 | !write(*,*) 'TB22 phi4T=',phi4T |
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185 | |
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186 | !! interpolation of na values in cm-2 from Strobel values for |
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187 | !the 100K model: |
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188 | CALL interp_line(Naval2,gam2,22,na(ig,:),gammafi23,nlayer) |
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189 | CALL interp_line(Naval3,gam3,22,na(ig,:),gammafi33,nlayer) |
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190 | |
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191 | !write(*,*) 'TB22rad na = ',na(1,:) |
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192 | !write(*,*) 'TB22rad gammafi = ',gammafi23 |
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193 | |
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194 | DO l=1,nlayer |
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195 | |
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196 | !! Getting ratio depending on temperature and n (cm-2) |
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197 | ratio_sq=ratio_square(pt(ig,l),na(ig,l)) |
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198 | ratio_af=ratio_affine(pt(ig,l),na(ig,l)) |
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199 | !! Modified gamma depending on T |
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200 | gammafi23mod(l)=min(ratio_sq*gammafi23(l),1.) |
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201 | gammafi33mod(l)=min(ratio_af*gammafi33(l),1.) |
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202 | |
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203 | !! Heating : cf Strobel 1996 and Zalucha 2011 |
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204 | ! eps 2.3 |
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205 | eps23(ig,l)=phin3(ig,l)/(phin3(ig,l)+gammafi23mod(l))* & |
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206 | (beta23+phi3n4(ig,l)/(phi3n4(ig,l)+1)* & |
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207 | phi4T(ig,l)/(phi4T(ig,l)+gammafi23mod(l))* & |
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208 | (3.*phi2n4(ig,l)+1.)/(1.+phi2n4(ig,l))*(1-beta23)/3.) |
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209 | |
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210 | ! eps 3.3 |
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211 | eps33(ig,l)=phi3(ig,l)/(phi3(ig,l)+gammafi33mod(l))* & |
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212 | (beta33+phi2n4(ig,l)/(phi2n4(ig,l)+1)* & |
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213 | phi4T(ig,l)/(phi4T(ig,l)+gammafi33mod(l))* & |
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214 | (1-beta33)) |
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215 | |
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216 | ! Cooling from Zalucha et al 2013 eq10 |
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217 | eps76(ig,l)=1./(1.+gammafi23mod(l)/(2.*phi4T(ig,l))) |
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218 | |
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219 | ENDDO |
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220 | !write(*,*) 'TB22rad eps23 = ',eps23(1,:) |
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221 | !write(*,*) 'TB22rad eps33 = ',eps33(1,:) |
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222 | !write(*,*) 'TB22rad gamma33 = ',gammafi33mod |
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223 | !write(*,*) 'TB22rad eps76 = ',eps76(1,:) |
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224 | |
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225 | ENDDO ! ngrid |
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226 | |
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227 | ELSE ! if (strobel) |
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228 | !if strobel = false |
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229 | |
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230 | klw = 3.6E-4 ! fit strobel |
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231 | !eps_sw1Pa = 0.6 ! fit strobel |
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232 | eps_sw1Pa = 0.90 ! to fit NH temperature en 1D [ch4]=0.5 |
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233 | !eps_sw1Pa = 0.98 ! to fit NH temperature en 3D = fit 1D [ch4]=0.25 |
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234 | |
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235 | ksw = 8.5E-5*(0.9/(eps_sw1Pa-0.1)-1.) |
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236 | do l=1, nlayer |
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237 | do ig=1, ngrid |
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238 | rho(ig,l)=pplay(ig,l)/(r*pt(ig,l)) |
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239 | eps23(ig,l) = 0.1+ 0.9/(1.+ksw/rho(ig,l)) |
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240 | eps76(ig,l) = 1./(1.+klw/rho(ig,l)) |
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241 | end do |
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242 | end do |
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243 | |
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244 | END IF |
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245 | |
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246 | end subroutine nlte_ch4 |
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247 | |
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248 | real function k4zT(temp,vmr) |
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249 | implicit none |
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250 | real, intent(in) :: temp,vmr |
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251 | k4zT=1.9e-15*exp((temp-240.)/70.)*(1+10.*vmr) |
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252 | return |
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253 | end function k4zT |
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254 | |
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255 | !! Log log affine and square function for ratio adjustment and extrapolation |
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256 | |
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257 | real function log_square(x,y1,y2,x1,x2,coef) |
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258 | implicit none |
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259 | real, intent(in) :: x,y1,y2,x1,x2,coef |
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260 | real aa,bb |
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261 | aa=(log(y2)-log(y1))/((log(coef*x2))**4-(log(coef*x1)**4)) |
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262 | bb=log(y2)-aa*(log(coef*x2))**4 |
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263 | log_square=exp(aa*(log(coef*x))**4+bb) |
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264 | return |
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265 | end function log_square |
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266 | |
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267 | real function log_affine(x,y1,y2,x1,x2) |
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268 | real, intent(in) :: x,y1,y2,x1,x2 |
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269 | real aa,bb |
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270 | aa=(log(y2)-log(y1))/(log(x2)-log(x1)) |
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271 | bb=log(y2)-aa*log(x2) |
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272 | log_affine=exp(aa*log(x)+bb) |
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273 | return |
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274 | end function log_affine |
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275 | |
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276 | !! Ratio of gamma depending on T. Linear approximation |
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277 | real function ratio_affine(temp,n) |
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278 | implicit none |
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279 | real, intent(in) :: temp,n |
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280 | real aa,bb,ratio0 |
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281 | real log_affine |
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282 | aa=(1.-0.2)/(100.-40.) |
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283 | bb=1.-aa*100. |
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284 | ratio0=aa*temp+bb |
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285 | ratio_affine=log_affine(n,1.,ratio0,1e15,1e22) |
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286 | return |
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287 | end function ratio_affine |
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288 | |
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289 | !! Ratio of gamma depending on T. Linear approximation |
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290 | real function ratio_square(temp,n) |
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291 | implicit none |
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292 | real, intent(in) :: temp,n |
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293 | real aa,bb,ratio0,coef |
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294 | real log_square |
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295 | coef=1.e-12 |
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296 | aa=(1.-0.2)/(100.-40.) |
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297 | bb=1.-aa*100. |
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298 | ratio0=aa*temp+bb |
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299 | ratio_square=log_square(n,1.,ratio0,1e15,1e22,coef) |
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300 | return |
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301 | end function ratio_square |
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302 | |
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303 | |
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304 | |
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