1 | ## $Header$ |
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2 | # |
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3 | ## Include diurnal cycle or not |
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4 | cycle_diurne=y |
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5 | ## Include soil model or not |
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6 | soil_model=y |
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7 | ## Use orodr or not for orography |
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8 | ok_orodr=n |
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9 | ## Use orolf or not for orography |
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10 | ok_orolf=n |
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11 | ## Use non-orographic Gravity Waves of not |
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12 | ok_gw_nonoro=n |
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13 | ## Number of calls to the radiative transfer (per day) |
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14 | nbapp_rad=24000 |
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15 | ## Number of calls to the chemistry routines (per day) |
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16 | nbapp_chem=24000 |
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17 | ## Flag for convection : 1 pour LMD, 2 pour Tiedtke, 3 KE(new version JYG), 30 KE(version IPCC AR4), 4 KE vect |
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18 | iflag_con=0 |
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19 | # |
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20 | # orbital parameters |
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21 | ##~~~~~~~~~~~~~~~~~~ |
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22 | # |
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23 | # VENUS ## |
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24 | # R_ecc = 0.006787 |
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25 | R_ecc = 0. |
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26 | R_peri = 0. |
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27 | # R_incl = 177.4 |
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28 | R_incl = 0. |
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29 | # solar: effective flux, given at 1 UA |
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30 | solaire = 328. |
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31 | # |
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32 | # parameters for the tracers |
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33 | ##~~~~~~~~~~~~~~~~~~~~~~~~~ |
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34 | # |
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35 | # 0: nothing (passive tracers) |
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36 | # 1: pseudo-chemistry relaxation (phytrac_relax) |
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37 | # 2: surface emission (phytrac_emiss) |
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38 | # 3: full chemistry (phytrac_chem) |
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39 | tr_scheme = 0 |
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40 | # |
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41 | # Reinitialization of tracer abundances |
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42 | reinit_trac=n |
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43 | # |
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44 | # Parameters for Age of air |
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45 | ##~~~~~~~~~~~~~~~~~~~~~~~~~ |
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46 | # Compute age of air (requires that there is an "aoa" tracer; default: n) |
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47 | ok_aoa=n |
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48 | # Reinitialize age of air tracer (default: y) |
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49 | reinit_aoa=n |
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50 | # Emission altitude (in model layers) of aoa tracer emission (default: 1) |
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51 | lev_aoa=1 |
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52 | # |
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53 | # parameters for chemistry and microphysics |
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54 | ##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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55 | # |
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56 | # use chemistry ? |
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57 | ok_chem=n |
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58 | # use clouds ? (needed for chemistry) |
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59 | ok_cloud=n |
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60 | # if yes, which scheme: |
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61 | # 1 => simple scheme (Aurelien Stolzenbach) |
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62 | # 2 => full microphysical scheme (Sabrina Guilbon) |
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63 | cl_scheme=1 |
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64 | # use sedimentation (goes with clouds) |
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65 | ok_sedim=n |
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66 | nb_mode=3 |
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67 | # |
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68 | # parameters for the boundary layer |
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69 | ##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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70 | # |
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71 | iflag_pbl=8 |
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72 | z0 = 0.01 |
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73 | lmixmin = 35. |
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74 | ksta = 1.e-7 |
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75 | ok_kzmin=n |
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76 | # |
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77 | # Surface thermal inertia |
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78 | inertie=2000 |
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79 | # |
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80 | # dry convection parameters |
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81 | ##~~~~~~~~~~~~~~~~~~~~~~~~~ |
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82 | # |
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83 | iflag_ajs = 1 |
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84 | |
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85 | # Solar radiation module |
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86 | ##~~~~~~~~~~~~~~~~~~~~~~ |
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87 | ## 1 = Rainer Haus Tables |
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88 | ## 2 = Generic solar module |
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89 | # |
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90 | solarchoice=1 |
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91 | |
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92 | # Thermosphere and nlte parameters |
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93 | ##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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94 | # |
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95 | ## Compute non-LTE or not |
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96 | callnlte=n |
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97 | ## choice of species profile to use |
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98 | nltemodel=2 |
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99 | ## Compute CO2 IR absorption or not |
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100 | callnirco2=n |
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101 | ##CO2 IR Absorption model |
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102 | nircorr=0 |
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103 | ##include thermosphere or not |
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104 | callthermos=n |
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105 | |
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106 | ## Thermospheric options |
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107 | ##~~~~~~~~~~~~~~~~~~~~~~ |
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108 | ## Tuning of photochemistry for oxygen production ? |
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109 | tuneupperatm = n |
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110 | |
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111 | #Method to include solar variability? |
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112 | #0-> Old method 1-> Variability with E10.7 as observed |
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113 | solvarmod=0 |
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114 | |
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115 | ## (Solar min=70 ave=140 max=300) |
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116 | fixed_euv_value = 140. |
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117 | |
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118 | # value for the UV heating efficiency |
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119 | ##(experimental values between 0.19 and 0.23, lower values may |
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120 | ## be used to compensate for low 15 um cooling) |
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121 | euveff = 0.195 |
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122 | # |
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123 | # |
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124 | # |
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125 | # |
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126 | # Parameters for IOIPSL output files |
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127 | ##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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128 | ## OLD. Now we use XIOS => see context_lmdz_physics.xml to taylor the output files |
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129 | # |
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130 | ### OK_journe= y for daily output file histday.nc, =n no histday.nc output |
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131 | ### Meaningless for Venus |
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132 | OK_journe=n |
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133 | ### OK_mensuel= y for monthly output file histmth.nc, =n no histmth.nc |
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134 | ### For Venus, only these averaged outputs |
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135 | OK_mensuel=n |
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136 | ## rate (in days) at which the Venus histmth file is to be written |
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137 | # sets the output rate in histmth and/or histins |
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138 | ecritphy=0.1 |
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139 | ### OK_instan=y, make some "instantaneous" outputs (same rate as histmth) |
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140 | OK_instan=n |
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141 | # |
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142 | # Output levels for the various output files |
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143 | # |
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144 | # output level for "day" lev_histday |
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145 | # - lev_hist*=1 => baseline 2D fields |
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146 | # - lev_hist*=2 => baseline 3D fields (default) |
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147 | # - lev_hist*=3 => radiative transfert |
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148 | # - lev_hist*=4 => 3D tendencies |
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149 | # - lev_hist*=5 => tracers and others |
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150 | lev_histday=2 |
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151 | #output level for "mth" lev_histmth |
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152 | lev_histmth=2 |
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153 | #output level for "ins" lev_histins |
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154 | lev_histins=2 |
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155 | |
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