1 | ## Orbit / general options |
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2 | ## ~~~~~~~~~~~~~~~~~~~~~~~ |
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3 | # Run with or without tracer transport ? |
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4 | tracer = .true. |
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5 | # Diurnal cycle ? if diurnal=false, diurnally averaged solar heating |
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6 | diurnal = .false. |
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7 | # Seasonal cycle ? if season=false, Ls stays constant, to value set in "start" |
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8 | season = .false. |
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9 | # Tidally resonant orbit ? must have diurnal=false, correct rotation rate in newstart |
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10 | tlocked = .true. |
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11 | # Tidal resonance ratio ? ratio T_orbit to T_rotation |
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12 | nres = 1. |
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13 | # Write some more output on the screen ? |
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14 | lwrite = .true. |
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15 | # Save statistics in file "stats.nc" ? |
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16 | callstats = .false. |
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17 | # Test energy conservation of model physics ? |
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18 | enertest = .true. |
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19 | # check if cpp and mugaz from start.nc are consistent with values computed by comp_cpp_mugaz with gases.def |
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20 | check_cpp_match = .false. |
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21 | |
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22 | ## Directory where external input files are |
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23 | ## ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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24 | #datadir = /planeto/mturbet/planeto2-mturbet/Maxence/SIMUS_Proxima_b |
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25 | #datadir = /home/leconte/datagcm |
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26 | datadir = ./datagcm |
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27 | |
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28 | ## Radiative transfer options |
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29 | ## ~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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30 | # call radiative transfer? |
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31 | callrad = .true. |
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32 | # the rad. transfer is computed every "iradia" physical timestep |
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33 | iradia = 1000 |
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34 | # Use blackbody for stellar spectrum ? |
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35 | stelbbody = .false. |
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36 | # Stellar blackbody temperature ? |
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37 | stelTbb = 3050.000 |
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38 | # call multilayer correlated-k radiative transfer ? |
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39 | corrk = .true. |
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40 | # folder in which correlated-k data is stored ? |
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41 | corrkdir = Earth_110-710K |
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42 | # corrkdir = megaCO2 |
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43 | # corrkdir = null_highT |
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44 | # call visible gaseous absorption in radiative transfer ? |
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45 | callgasvis = .true. |
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46 | # call continuum in radiative transfer ? |
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47 | continuum = .true. |
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48 | # Include Rayleigh scattering in the visible ? |
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49 | rayleigh = .true. |
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50 | # Uniform absorption coefficient in radiative transfer? |
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51 | graybody = .false. |
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52 | # Constant absorption coefficient in visible |
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53 | # (in m^2/kg; only if graybody=true): |
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54 | # tau_surf= kappa*P/g |
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55 | kappa_VI = 1.e-4 |
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56 | # Constant absorption coefficient in IR |
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57 | # (in m^2/kg; only if graybody=true): |
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58 | kappa_IR = 1.e-4 |
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59 | # Use Newtonian cooling in place of radiative transfer ? |
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60 | newtonian = .false. |
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61 | # Radiative timescale for Newtonian cooling ? [only if newtonian = T] |
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62 | tau_relax = 30.00000 |
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63 | # Test physics timescale in 1D ? |
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64 | testradtimes = .false. |
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65 | # Characteristic planetary equilibrium (black body) temperature |
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66 | # This is used only in the aerosol radiative transfer setup. (see aerave.F) |
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67 | tplanet = 215. |
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68 | # Output spectral OLR in 1D/3D? |
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69 | specOLR = .false. |
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70 | # Output global radiative balance in file 'rad_bal.out' - slow for 1D!! |
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71 | meanOLR = .false. |
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72 | # Variable gas species: Radiatively active ? |
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73 | varactive = .true. |
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74 | # Variable gas species: Fixed vertical distribution ? |
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75 | # (not to be used in time integration mode) |
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76 | varfixed = .false. |
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77 | # Variable gas species: Saturation percentage value at ground ? |
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78 | satval = 1. |
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79 | # Use fixed vertical profile, 1 step, no iteration ? |
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80 | kastprof = .false. |
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81 | # Remove lower boundary (e.g. for gas giant sims) |
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82 | nosurf = .false. |
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83 | intheat = 0. |
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84 | |
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85 | ## Star type |
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86 | ## ~~~~~~~~~ |
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87 | startype = 1 |
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88 | # ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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89 | # The choices are: |
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90 | # |
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91 | # startype = 1 Sol (G2V-class main sequence) |
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92 | # startype = 2 Ad Leo (M-class, synthetic) |
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93 | # startype = 3 GJ644 |
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94 | # startype = 4 HD128167 |
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95 | # ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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96 | # Stellar flux at 1 AU. Examples: |
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97 | # 1366.0 W m-2 Sol today |
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98 | # 1024.5 W m-2 Sol today x 0.75 = weak early Sun |
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99 | # 18.462 W m-2 The feeble Gl581 |
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100 | # 19.960 W m-2 Gl581 with e=0.38 orbital average |
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101 | # 1.58e6 W m-2 at Kepler 7 b distance |
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102 | Fat1AU = 1300.7 |
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103 | #Fat1AU = 1400.0 |
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104 | ##Fat1AU = 2000.0 |
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105 | |
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106 | ## Tracer and aerosol options |
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107 | ## ~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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108 | # Gravitational sedimentation of tracers (just H2O ice for now) ? |
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109 | sedimentation = .true. |
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110 | |
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111 | ## Other physics options |
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112 | ## ~~~~~~~~~~~~~~~~~~~~~ |
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113 | # call turbulent vertical diffusion ? |
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114 | calldifv = .true. |
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115 | # use turbdiff instead of vdifc ? |
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116 | UseTurbDiff = .true. |
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117 | # call convective adjustment ? |
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118 | calladj = .false. |
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119 | # call thermal conduction in the soil ? |
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120 | callsoil = .true. |
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121 | |
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122 | ######################################################################### |
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123 | ## extra non-standard definitions for Earth |
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124 | ######################################################################### |
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125 | |
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126 | ## Tracer and aerosol options |
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127 | ## ~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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128 | # Varying H2O cloud fraction? |
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129 | CLFvarying = .false. |
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130 | # H2O cloud fraction? |
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131 | CLFfixval = 1. |
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132 | # number mixing ratio of CO2 ice particles |
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133 | Nmix_co2 = 1.e5 |
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134 | # basic dust opacity |
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135 | dusttau = 0.0 |
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136 | # water cloud pressure level (norm. by psurf) |
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137 | cloudlvl = 0.0 |
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138 | # atm mass update due to tracer evaporation/condensation? |
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139 | mass_redistrib = .true. |
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140 | # Radiatively active CO2 aerosol? |
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141 | aeroco2 = .false. |
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142 | # Fixed CO2 aerosol distribution? |
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143 | aerofixco2 = .false. |
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144 | # Radiatively active water aerosol? |
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145 | aeroh2o = .true. |
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146 | # Fixed water aerosol distribution? |
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147 | aerofixh2o = .false. |
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148 | # Radiatively active sulfur aersol? |
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149 | aeroh2so4 = .false. |
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150 | # Radiatively active generic aerosol? |
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151 | aerogen = .false. |
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152 | # Fixed water aerosol distribution? |
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153 | aerofixgen = .false. |
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154 | # fixed radii for h2o cloud particles? |
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155 | radfixed=.false. |
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156 | # number mixing ratio of water particles (for rafixed=.false.) |
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157 | Nmix_h2o = 1.e7 |
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158 | # number mixing ratio of water ice particles (for rafixed=.false.) |
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159 | Nmix_h2o_ice = 1.e4 |
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160 | # radius of H2O water particles (for rafixed=.true.): |
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161 | rad_h2o=12.e-6 |
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162 | # radius of H2O ice particles (for rafixed=.true.): |
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163 | rad_h2o_ice=35.e-6 |
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164 | |
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165 | ## Water options |
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166 | ## ~~~~~~~~~~~~~ |
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167 | # Model water cycle |
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168 | water = .true. |
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169 | # Model water cloud formation |
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170 | watercond = .true. |
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171 | # Model water precipitation (including coagulation etc.) |
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172 | waterrain = .true. |
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173 | # Use simple precipitation scheme? |
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174 | precip_scheme=4 |
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175 | # multiplicative constant in Boucher 95 precip scheme |
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176 | Cboucher=2. |
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177 | # rain threshold. |
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178 | rainthreshold = 1e-3 |
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179 | # re-evaporate precipitations? |
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180 | evap_prec = .true. |
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181 | # ratqs ? |
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182 | ratqs = 1.0 |
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183 | # Include hydrology ? |
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184 | hydrology = .true. |
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185 | # H2O snow (and ice) albedo ? |
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186 | albedosnow = 0.70 |
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187 | albedo_spectral_mode = .true. |
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188 | # Maximum sea ice thickness ? |
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189 | maxicethick = 1. |
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190 | # Freezing point of seawater (degrees C) ? |
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191 | Tsaldiff = 0.0 |
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192 | # Evolve surface water sources ? |
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193 | sourceevol = .false. |
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194 | |
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195 | ## CO2 options |
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196 | ## ~~~~~~~~~~~ |
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197 | # call CO2 condensation ? |
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198 | co2cond = .false. |
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199 | # Set initial temperature profile to 1 K above CO2 condensation everywhere? |
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200 | nearco2cond = .false. |
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201 | |
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202 | ## generic tracer options |
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203 | ## ~~~~~~~~~~~ |
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204 | # call generic condensation ? |
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205 | generic_cond=.false. |
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206 | # Generic condensate specific latent heat divided by R |
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207 | latR_gencond= 4.4473d4 |
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208 | # Generic condensate reference pressure |
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209 | Pref_gencond= 1.d5 |
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210 | # Generic condensate reference temperature |
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211 | Tref_gencond= 3134.d0 |
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212 | # Generic condensate mean molecular weight |
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213 | mu_gencond= 55.8d0 |
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214 | # Generic condensate density |
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215 | rho_gencond=1.d4 |
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216 | # Generic condensate mean radius |
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217 | rad_gencond=5.d-6 |
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