1 | ## Directory where external input files are |
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2 | levels## ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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3 | #datadir = /d5/aslmd/DATAGENERIC |
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4 | datadir = /planeto/sglmd/datagcm |
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5 | |
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6 | ## Orbit / general options |
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7 | ## ~~~~~~~~~~~~~~~~~~~~~~~ |
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8 | # Run with or without tracer transport ? |
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9 | tracer = .false. |
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10 | # Diurnal cycle ? if diurnal=false, diurnally averaged solar heating |
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11 | diurnal = .false. |
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12 | # Seasonal cycle ? if season=false, Ls stays constant, to value set in "start" |
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13 | season = .true. |
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14 | # Tidally resonant orbit ? must have diurnal=false, correct rotation rate in newstart |
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15 | tlocked = .false. |
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16 | # Tidal resonance ratio ? ratio T_orbit to T_rotation |
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17 | nres = 1 |
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18 | # Planet with rings? |
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19 | rings_shadow = .false. |
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20 | # Compute latitude-dependent gravity field?? |
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21 | oblate = .true. |
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22 | # Flattening (a-b)/a |
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23 | flatten = 0.06487 |
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24 | # Needed if oblate=.true.: J2 |
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25 | J2 = 0.01470 |
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26 | # Needed if oblate=.true.: Planet mean radius (m) |
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27 | Rmean = 69911000. |
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28 | # Needed if oblate=.true.: Mass of the planet (*1e24 kg) |
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29 | MassPlanet = 1898.3 |
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30 | # Write some more output on the screen ? |
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31 | lwrite = .false. |
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32 | # Save statistics in file "stats.nc" ? |
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33 | callstats = .false. |
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34 | # Test energy conservation of model physics ? |
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35 | enertest = .true. |
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36 | # Check to see if cpp, mugaz values used match gas mixture defined in gases.def (recommended) ? |
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37 | check_cpp_match=.false. |
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38 | # |
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39 | ## Radiative transfer options |
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40 | ## ~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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41 | # call radiative transfer? |
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42 | callrad = .true. |
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43 | # the rad. transfer is computed every "iradia" physical timestep |
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44 | iradia = 8 |
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45 | # call multilayer correlated-k radiative transfer ? |
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46 | corrk = .true. |
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47 | # Include continuum absorption in radiative transfer (note CO2 is treated separately) ? |
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48 | continuum = .true. |
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49 | # folder in which correlated-k data is stored ? |
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50 | corrkdir = Jupiter_NewMOSES_NH3_HITRAN2012_REY_ISO_ge-12_NoKarko |
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51 | # call visible gaseous absorption in radiative transfer ? |
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52 | callgasvis = .true. |
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53 | # Include Rayleigh scattering in the visible ? |
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54 | rayleigh = .true. |
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55 | # Uniform absorption coefficient in IR ? |
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56 | graybody = .false. |
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57 | # Characteristic planetary equilibrium (black body) temperature |
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58 | # This is used only in the aerosol radiative transfer setup. (see aerave.F) |
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59 | tplanet = 100. |
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60 | # Use Newtonian cooling in place of radiative transfer ? |
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61 | newtonian = .false. |
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62 | # Radiative timescale for Newtonian cooling ? [only if newtonian = T] |
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63 | tau_relax = 30.00000 |
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64 | # Test physics timescale in 1D ? |
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65 | testradtimes = .false. |
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66 | # Output spectral OLR in 1D/3D? |
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67 | specOLR = .true. |
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68 | # Output global radiative balance in file 'rad_bal.out' - slow for 1D!! |
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69 | meanOLR = .false. |
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70 | # Variable gas species: Radiatively active ? |
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71 | varactive = .false. |
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72 | # Variable gas species: Fixed vertical distribution ? |
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73 | varfixed = .false. |
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74 | # Variable gas species: Saturation percentage value at ground ? |
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75 | satval = 0.0 |
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76 | # Use fixed vertical profile, 1 step, no iteration ? |
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77 | kastprof = .false. |
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78 | # Use blackbody for stellar spectrum ? |
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79 | stelbbody = .false. |
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80 | # Stellar blackbody temperature ? |
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81 | stelTbb = 5800.000 |
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82 | # Force specific heat capacity and molecular mass values |
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83 | force_cpp = .true. |
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84 | # Specific heat capacity in J K-1 kg-1 [only used if force_cpp = T] |
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85 | cpp = 11500 |
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86 | # Molecular mass in g mol-1 [only used if force_cpp = T] |
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87 | mugaz = 2.343 |
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88 | #Call conduction in upper atmosphere? |
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89 | callconduc = .false. |
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90 | #Flux from thermosphere (if callconduc)? |
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91 | phitop = 1.e-3 |
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92 | |
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93 | ## Star type |
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94 | ## ~~~~~~~~~ |
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95 | startype = 1 |
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96 | # ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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97 | # The choices are: |
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98 | # |
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99 | # startype = 1 Sol (G2V-class main sequence) |
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100 | # startype = 2 Ad Leo (M-class, synthetic) |
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101 | # startype = 3 GJ644 |
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102 | # startype = 4 HD128167 |
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103 | # ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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104 | # Stellar flux at 1 AU. Examples: |
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105 | # 1366.0 W m-2 Sol today |
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106 | # 1024.5 W m-2 Sol today x 0.75 = weak Sun 3.8 GYa |
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107 | # 18.462 W m-2 The feeble GJ581 |
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108 | # 19.960 W m-2 GJ581 with e=0.38 orbital average |
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109 | Fat1AU = 1366.0 |
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110 | |
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111 | ## Tracer and aerosol options |
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112 | ## ~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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113 | # Gravitational sedimentation of tracers (KEEP FALSE FOR NOW) ? |
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114 | sedimentation = .false. |
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115 | |
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116 | ## Other physics options |
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117 | ## ~~~~~~~~~~~~~~~~~~~~~ |
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118 | # call turbulent vertical diffusion ? |
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119 | calldifv = .true. |
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120 | # use turbdiff instead of vdifc ? |
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121 | UseTurbDiff = .true. |
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122 | # call convective adjustment ? |
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123 | calladj = .true. |
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124 | # call thermal conduction in the soil ? |
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125 | callsoil = .false. |
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126 | # Internal heat flux (matters only if callsoil=F) |
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127 | intheat = 5.44 |
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128 | # Remove lower boundary (e.g. for gas giant sims) |
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129 | nosurf = .true. |
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130 | |
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131 | ######################################################################### |
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132 | ## extra non-standard definitions for Gliese 581d / Early Mars |
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133 | ######################################################################### |
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134 | |
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135 | ## Tracer and aerosol options |
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136 | ## ~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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137 | # Radiatively active CO2 aerosol? |
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138 | aeroco2 = .false. |
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139 | |
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140 | # Ammonia cloud (Saturn/Jupiter)? |
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141 | aeronh3 = .true. |
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142 | size_nh3_cloud = 15.e-6 |
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143 | pres_nh3_cloud = 80000 |
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144 | tau_nh3_cloud = 7.0 |
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145 | # Radiatively active aerosol (Saturn/Jupiter)? |
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146 | aeroback2lay = .true. |
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147 | obs_tau_col_tropo= 2.0 |
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148 | size_tropo= 1.e-6 |
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149 | pres_bottom_tropo=80000. |
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150 | pres_top_tropo=18000. |
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151 | obs_tau_col_strato= 0.1D0 |
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152 | |
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153 | # Auroral aerosols (Saturn/Jupiter)? |
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154 | aeroaurora = .true. |
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155 | |
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156 | # Fixed CO2 aerosol distribution? |
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157 | aerofixco2 = .false. |
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158 | # Radiatively active water aerosol? |
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159 | aeroh2o = .false. |
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160 | # Fixed water aerosol distribution? |
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161 | aerofixh2o = .false. |
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162 | # Varying H2O cloud fraction? |
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163 | CLFvarying = .false. |
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164 | # H2O cloud fraction? |
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165 | CLFfixval = 0.0 |
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166 | # number mixing ratio of CO2 ice particles |
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167 | Nmix_co2 = 100000. |
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168 | # number mixing ratio of water ice particles |
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169 | Nmix_h2o = 100000. |
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170 | # basic dust opacity |
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171 | dusttau = 0.0 |
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172 | # water cloud pressure level (norm. by psurf) |
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173 | cloudlvl = 0.0 |
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174 | |
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175 | |
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176 | ## Water options |
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177 | ## ~~~~~~~~~~~~~ |
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178 | # Model water cycle |
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179 | water = .false. |
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180 | # Model water cloud formation |
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181 | watercond = .false. |
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182 | # Model water precipitation (including coagulation etc.) |
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183 | waterrain = .false. |
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184 | # Precipitation threshold (simple scheme only) ? |
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185 | rainthreshold = 0.011 |
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186 | # Surface hydrology? |
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187 | hydrology = .false. |
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188 | # H2O snow (and ice) albedo ? |
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189 | albedosnow = 0.6 |
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190 | # Maximum sea ice thickness (m) ? |
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191 | maxicethick = 2.0 |
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192 | # Freezing point of seawater (degrees C) ? |
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193 | Tsaldiff = 0.0 |
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194 | # Evolve surface water sources ? |
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195 | sourceevol = .false. |
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196 | |
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197 | ## CO2 options |
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198 | ## ~~~~~~~~~~~ |
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199 | # call CO2 condensation ? |
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200 | co2cond = .false. |
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201 | # Set initial temperature profile to 1 K above CO2 condensation everywhere? |
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202 | nearco2cond = .false. |
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