source: trunk/LMDZ.PLUTO.old/deftank/gcm/callphys.def @ 3594

Last change on this file since 3594 was 3175, checked in by emillour, 12 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: 3.3 KB
RevLine 
[3175]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   = .true.
8# Seasonal cycle ? if season=false, Ls stays constant, to value set in "start"
9season    = .true.
10# Run 1D or 3D version (false) / fast version volatile transport (true)
11fast    = .false.
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
21## Radiative transfer options
22## ~~~~~~~~~~~~~~~~~~~~~~~~~~
23# call radiative transfer?
24callrad    = .true.
25# the rad. transfer is computed every "iradia" physical timestep
26iradia     = 5
27# call multilayer correlated-k radiative transfer ?
28corrk      = .true.
29ch4fix = .true.
30vmrch4fix = 0.5
31nlte=.false.
32# folder in which correlated-k data is stored ?
33corrkdir   = pluton_ch4var_COfix
34# call visible gaseous absorption in radiative transfer ?
35callgasvis = .true.
36# Output spectral OLR in 3D?
37specOLR    = .false.
38# Output global radiative balance in file 'olr.txt' - slow for 1D!!
39meanOLR    = .false.
40
41## Star type (inherited from generic model)
42## ~~~~~~~~~
43startype = 1
44# ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
45# The choices are:
46#
47#       startype = 1            Sol        (G2V-class main sequence)
48#       startype = 2            Ad Leo     (M-class, synthetic)
49#       startype = 3            GJ644
50#       startype = 4            HD128167
51# ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
52# Stellar flux at 1 AU. Examples:
53# 1366.0 W m-2          Sol today
54# 1017.0 W m-2          Sol today x 0.75 = weak early Sun
55# 18.462 W m-2          The feeble Gl581
56Fat1AU = 1366.0
57
58## Tracer and aerosol options
59## ~~~~~~~~~~~~~~~~~~~~~~~~~~
60# Call N2 condensation ?
61N2cond       = .true.
62# Gravitational sedimentation of tracers ?
63sedimentation = .true.
64# Compute glacial flow (for fast option only)?
65glaflow = .false.
66# Compute methane cycle ?
67methane = .true.
68# Compute CO cycle ?
69carbox = .true.
70# Compute methane clouds ?
71metcloud = .true.
72# Compute CO clouds ?
73monoxcloud = .true.
74# Haze production ?
75haze          = .true.
76# source additional haze ?
77source_haze= .false.
78# number mixing ratio of haze particles for ch4 clouds
79Nmix_ch4      = 100000.
80# number mixing ratio of haze particles for co clouds
81Nmix_co      = 100000.
82# Radiatively active haze ?
83aerohaze=.false.
84# fractal particle ?
85fractal=.false.
86# Day fraction for limited cold trap in SP?
87dayfrac=0.
88# geothermal flux at the bottom layer
89fluxgeo = 0.
90
91## Surface properties
92## ~~~~~~~~~~~~~~~~~~~~~~~~~~
93constalb=.true.
94alb_n2b=0.7
95alb_n2a=0.7
96alb_ch4_eq=0.5
97alb_ch4=0.5
98alb_co=0.4
99alb_tho=0.2
100alb_tho_eq=0.1
101emis_n2b=0.8
102emis_n2a=0.8
103emis_ch4=0.8
104emis_co=0.8
105emis_tho=1.0
106emis_tho_eq=1.0
107
108# Change TI with time
109changeti=.false.
110ITCH4=800.
111ITN2=800
112ITH2O=800.
113
114## Other physics options
115## ~~~~~~~~~~~~~~~~~~~~~
116# call turbulent vertical diffusion ?
117calldifv = .true.
118# call convective adjustment ?
119calladj  = .true.
120# call thermal conduction in the soil ?
121callsoil = .true.
122# call thermal conduction
123callconduct=.true.
124# call molecular viscosity 3D only
125callmolvis=.true.
126# call molecular diffusion
127callmoldiff=.true.
128# flux qui arrive au-dessus de latmosphere
129phitop=0.
130
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