#_# Orbit / general options ## ~~~~~~~~~~~~~~~~~~~~~~~ # Run with or without tracer transport ? tracer = .true. # Diurnal cycle ? if diurnal=false, diurnally averaged solar heating diurnal = .true. # Seasonal cycle ? if season=false, Ls stays constant, to value set in "start" season = .true. # Tidally resonant orbit ? must have diurnal=false, correct rotation rate in newstart tlocked = .false. # Tidal resonance ratio ? ratio T_orbit to T_rotation nres = 1 # Write some more output on the screen ? lwrite = .false. # Save statistics in file "stats.nc" ? callstats = .false. # Test energy conservation of model physics ? enertest = .false. # check if cpp and mugaz from start.nc are consistent with values computed by comp_cpp_mugaz with gases.def check_cpp_match = .true. ### run with triton orbit ? ##triton = .false. ### conservation n2 ##conservn2=.false. ## Directory where external input files are ## ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ datadir = datadir ## Radiative transfer options ## ~~~~~~~~~~~~~~~~~~~~~~~~~~ # call radiative transfer? callrad = .true. # the rad. transfer is computed every "iradia" physical timestep iradia = 5 # call multilayer correlated-k radiative transfer ? corrk = .true. # folder in which correlated-k data is stored ? corrkdir = pluton_ch4var_COfix # strictboundcorrk strictboundcorrk = .true. # call visible gaseous absorption in radiative transfer ? callgasvis = .true. # call continuum in radiative transfer ? continuum = .false. # Include Rayleigh scattering in the visible ? rayleigh = .true. # Test physics timescale in 1D ? testradtimes = .false. # Output spectral OLR in 1D/3D? specOLR = .false. # Output global radiative balance in file 'rad_bal.out' - slow for 1D!! meanOLR = .false. # Variable gas species: Radiatively active ? varactive = .true. # Variable gas species: Fixed vertical distribution ? # (not to be used in time integration mode) varfixed = .false. # Variable gas species: Saturation percentage value at ground ? satval = .8 # Use fixed vertical profile, 1 step, no iteration ? kastprof = .false. ## Star type ## ~~~~~~~~~ startype = 1 # ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ # The choices are: # # startype = 1 Sol (G2V-class main sequence) # startype = 2 Ad Leo (M-class, synthetic) # startype = 3 GJ644 # startype = 4 HD128167 # ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ # Stellar flux at 1 AU. Examples: # 1366.0 W m-2 Sol today # 1024.5 W m-2 Sol today x 0.75 = weak early Sun # 18.462 W m-2 The feeble Gl581 # 19.960 W m-2 Gl581 with e=0.38 orbital average Fat1AU = 1366.0 ## Tracer and aerosol options ## ~~~~~~~~~~~~~~~~~~~~~~~~~~ # Gravitational sedimentation of tracers (just H2O ice for now) ? sedimentation = .true. naerkind = 1 hazeprop_file = optprop_tholins_fractal100nm.dat ## Other physics options ## ~~~~~~~~~~~~~~~~~~~~~ # call turbulent vertical diffusion ? calldifv = .true. # use turbdiff instead of vdifc ? UseTurbDiff = .true. # call convective adjustment ? calladj = .true. # call thermal conduction in the soil ? callsoil = .true. lay1_soil = 1.4e-2 ######################################################################### ## extra non-standard definitions for Earth ######################################################################### ## Tracer and aerosol options ## ~~~~~~~~~~~~~~~~~~~~~~~~~~ # atm mass update due to tracer evaporation/condensation? mass_redistrib = .false. ## Radiatively active CH4 aerosol? #aeroch4 = .false. # haze production? haze = .false. # Radiatively active haze aerosol? aerohcaer = .false. # Fixed haze distribution? aerofixhcaer = .false. # haze particule mean radius #rad_hcaer = 10e-9 ## Condensation ## ~~~~~~~~~~~ # call N2 condensation ? n2cond = .false. # Set initial temperature profile to 1 K above N2 condensation everywhere? #nearn2cond = .false.