### 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 = .true. # Check if cpp matches gases.def (should be false in 1d) check_cpp_match = .false. # Force cpp and mugaz values from gases.def (should be false in 1d) force_cpp = .false. # Compute effective variations of gravity field with altitude in physics ? # Better be true if you run with chemistry eff_gz = .false. ### Directory where external input files are ### ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ datadir = ../../datagcm ### Radiative transfer options ### ~~~~~~~~~~~~~~~~~~~~~~~~~~ # Call radiative transfer? callrad = .true. # The rad. transfer is computed every "iradia" physical timestep iradia = 4 # Use blackbody for stellar spectrum ? stelbbody = .false. # Stellar blackbody temperature ? stelTbb = 2000.000 # Call multilayer correlated-k radiative transfer ? corrk = .true. # Folder in which correlated-k data is stored ? corrkdir = recombin # Use corr-k recombination instead of pre-mixed ? corrk_recombin = .true. # Call visible gaseous absorption in radiative transfer ? callgasvis = .true. # Call continuum in radiative transfer ? Continuum = .true. # Allow temperatures above kmatrix tmax strictboundcorrk = .false. # Include Rayleigh scattering in the visible ? rayleigh = .true. # Uniform absorption coefficient in radiative transfer? graybody = .false. # Constant absorption coefficient in visible # (in m^2/kg; only if graybody=true): # tau_surf= kappa*P/g kappa_VI = 0. # Constant absorption coefficient in IR # (in m^2/kg; only if graybody=true): kappa_IR = 0. # Use Newtonian cooling in place of radiative transfer ? newtonian = .false. # Radiative timescale for Newtonian cooling ? [only if newtonian = T] tau_relax = 30.00000 # Test physics timescale in 1D ? testradtimes = .false. # Characteristic planetary equilibrium (black body) temperature # This is used only in the aerosol radiative transfer setup. (see aerave.F) tplanet = 94. # Output spectral OLR in 1D/3D? specOLR = .false. # Output global radiative balance in file 'rad_bal.out' - slow for 1D!! meanOLR = .false. # Remove lower boundary (e.g. for gas giant sims) noradsurf = .false. # Output optical diagnostics (in otpcv & optci) ? diagdtau = .false. ### Chemistry ### ~~~~~~~~~ # Call chemistry ? (must have tracer = .true.) callchim = .true. # Activate zonal mean ? moyzon_ch = .true. # Chemistry is computed every "ichim" phys. timestep ichim = 20 # Infinite tank of CH4 ? (.false. == lakes at the poles) resCH4_inf = .false. ### Microphysics ### ~~~~~~~~~~~~ # Call microphysics ? (must have tracer = .true.) callmufi = .true. # Activate zonal mean ? (must be .true. if callmufi by now ?) moyzon_mu = .false. # If yes, compute clouds ? callclouds = .true. # If yes, number of ices ? (must be compatible with traceur.def AND microphysical model) nices = 4 # Use new optics for clouds ? opt4clouds = .true. # Cloudy fraction in the Clear / Dark column method ? Fcloudy = 0.2 # Adjustment of ssca albedo for cloudy dropplet ? Fssa = 0.90 # Adjustment of aerosol properties in the VIS ? FHVIS = 1.0 # Adjustment of aerosol properties in the IR ? FHIR = 1.0 # Desactivate radiative coupling of microphysics (i.e. use mean opacity profile) uncoupl_optic_haze = .false. # Use haze seasonal model ? (if you run without coupled microphysics) seashaze = .false. # ~~~~~ Parameters for microphysics ~~~~~ # Path to microphys. config file ? config_mufi = ../../datagcm/microphysics/config.ne15.cfg # Pressure level of aer. production (Pa) ? p_prod = 1.0 # Aer. production rate (kg.m-2.s-1) ? tx_prod = 3.5e-13 # Equivalent radius production (m) ? rc_prod = 1.0e-8 # Radius of air (nitrogen) molecule (m) ? air_rad = 1.75e-10 ### Star type ### ~~~~~~~~~ startype = 1 # ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ # The choices are: # # startype = 1 Sol (G2V-class main sequence) # ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ # 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 Fat1AU = 1366.0 ### 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. # Call nudging of zonal wind ? nudging_u = .true. # Nudging relaxation time (secondes) ? nudging_dt = 9.3e8