source: trunk/LMDZ.PLUTO.old/deftank/nogcm/callphys.def @ 3438

Last change on this file since 3438 was 3175, checked in by emillour, 11 months ago

Pluto PCM:
Add the old Pluto LMDZ for reference (required prior step to making
an LMDZ.PLUTO using the same framework as the other physics packages).
TB+EM

File size: 3.2 KB
Line 
1datadir=/home1/tbertran/MODELES/KBO/datagcm/
2## Orbit / general options
3## ~~~~~~~~~~~~~~~~~~~~~~~
4# Run with or without tracer transport ?
5tracer    = .true.
6# Diurnal cycle ?  if diurnal=false, diurnally averaged solar heating
7diurnal   = .false.
8# Seasonal cycle ? if season=false, Ls stays constant, to value set in "start"
9season    = .true.
10# Run 3D version (false) / fast version (true)
11fast    = .true.
12# Write some more output on the screen ?
13lwrite    = .false.
14# Save statistics in file "stats.nc" ?
15callstats = .false.
16# Test energy conservation of model physics ?
17enertest  = .false.
18# run with triton orbit ?
19triton = .false.
20# specific paleo run ?
21paleo = .false.
22# nb Earth years as paleoclimate step ? (if paleo = true)
23paleoyears = 50000.
24
25## Radiative transfer options
26## ~~~~~~~~~~~~~~~~~~~~~~~~~~
27# call radiative transfer?
28callrad    = .true.
29# the rad. transfer is computed every "iradia" physical timestep
30iradia     = 1
31# call multilayer correlated-k radiative transfer ?
32corrk      = .false.
33# folder in which correlated-k data is stored ?
34corrkdir   = pluton_ch4var_COfix
35# call visible gaseous absorption in radiative transfer ?
36callgasvis = .false.
37# Output spectral OLR in 3D?
38specOLR    = .false.
39# Output global radiative balance in file 'olr.txt' - slow for 1D!!
40meanOLR    = .false.
41
42## Star type (inherited from generic model)
43## ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
44startype = 1
45# ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
46# The choices are:
47#
48#       startype = 1            Sol        (G2V-class main sequence)
49#       startype = 2            Ad Leo     (M-class, synthetic)
50#       startype = 3            GJ644
51#       startype = 4            HD128167
52# ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
53# Stellar flux at 1 AU. Examples:
54# 1366.0 W m-2          Sol today
55# 1017.0 W m-2          Sol today x 0.75 = weak early Sun
56# 18.462 W m-2          The feeble Gl581
57Fat1AU = 1366.0
58
59## Tracer and aerosol options
60## ~~~~~~~~~~~~~~~~~~~~~~~~~~
61# Call N2 condensation ?
62N2cond       = .true.
63# N2 condensation subtimestep ?
64nbcond = 20
65# Gravitational sedimentation of tracers ?
66sedimentation = .false.
67# Compute glacial flow (for fast option only)?
68glaflow = .true.
69# Compute methane cycle ?
70methane = .true.
71# Compute CO cycle ?
72carbox = .false.
73# Haze production ?
74haze          = .false.
75# Fast haze production (with option fast=.true.) ?
76fasthaze          = .false.
77# number mixing ratio of haze particles for ch4 clouds
78Nmix_ch4      = 100000.
79# number mixing ratio of haze particles for co clouds
80Nmix_co      = 100000.
81# atmospheric redistribution : spring constant (s)
82tau_n2 = 1.
83tau_ch4 = 1.E6
84tau_co = 1. !E5
85# day fraction for blocking CH4/CO condensation in SP (0 by default) (with methane or carbox=.true.)
86dayfrac=1.0
87# geothermal flux at the bottom layer
88fluxgeo = 0.
89
90## Surface properties
91## ~~~~~~~~~~~~~~~~~~~~~~~~~~
92# constant albedo with time
93constalb=.false.
94
95alb_n2b=0.7
96alb_n2a=0.7
97alb_ch4_eq=0.5
98alb_ch4=0.5
99alb_co=0.4
100alb_tho=0.1
101alb_tho_eq=0.1
102emis_n2b=0.8
103emis_n2a=0.8
104emis_ch4=0.8
105emis_co=0.8
106emis_tho=0.8
107emis_tho_eq=0.8
108
109# Change TI with time
110changeti=.false.
111ITCH4=800.
112ITN2=800
113ITH2O=800.
114
115## Other physics options
116## ~~~~~~~~~~~~~~~~~~~~~
117# call thermal conduction in the soil ?
118callsoil = .true.
119# flux qui arrive au-dessus de latmosphere
120phitop=0.
121
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