source: trunk/LMDZ.TITAN/deftank/callphys.def @ 3000

## Orbit / general options
## ~~~~~~~~~~~~~~~~~~~~~~~
# Run with or without tracer transport ?
tracer    = .false.
# 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.

## 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     = 5
# 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   = 23x23
# use corr-k recombination instead of pre-mixed ?
corrk_recombin = .false.
# 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. 


# Compute effective variations of gravity field with altitude in physics ?
## Better be true if you run with chemistry
eff_gz = .true.

## Chemistry
## ~~~~~~~~~
# call chemistry ? (must have tracer=true)
callchim = .false.
# Activate zonal mean ? 
moyzon_ch = .false.
# chemistry is computed every "ichim" phys. timestep
ichim = 200

## Microphysics
## ~~~~~~~~~~~~
# use haze seasonal model ? ( if you run without coupled microphysics )
seashaze = .false.
# call microphysics ? (must have tracer=true)
callmufi = .false.
## If yes, compute clouds ?
callclouds = .false.
### If yes, number of ices ? (must be compatible with traceur.def AND microphysical model )
nices = 3
# Desactivate radiative coupling of microphysics ( i.e. use mean opacity profile )
uncoupl_optic_haze = .true.
# ~~~~~ 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 = 2.0e-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.