source: trunk/LMDZ.MARS/deftank/callphys.def.MCD5 @ 3493

Last change on this file since 3493 was 3468, checked in by emillour, 2 months ago

Mars PCM:
Remove obsolete/depreciated lwrite flag (which would trigger some very specific
extra text outputs), in code and in reference callphys.def files.
EM

File size: 5.0 KB
RevLine 
[758]1##General options
2##~~~~~~~~~~~~~~~
3
[3369]4# Number of outputs per sol for diagfi.nc files
5outputs_per_sol=4
6
[758]7#Directory where external input files are:
[1949]8datadir=/users/lmdz/WWW/planets/mars/datadir
[758]9
10#Diurnal cycle ?  if diurnal=False, diurnal averaged solar heating
11diurnal=.true.
12
13#Seasonal cycle ? if season=False, Ls stays constant, to value set in "start"
14season = .true.   
15
16#Save statistics in file "stats.nc" ?
17callstats =.true.
18
19#Save EOF profiles in file "profiles" for Climate Database?
20calleofdump = .false.
21
[3448]22## Dust scenario. Used if the dust is prescribed (i.e. if active=F)
[758]23## ~~~~~~~~~~~~~
24#  =1 Dust opt.deph read in startfi; =2 Viking scenario; =3 MGS scenario,
25#  =4 Mars Year 24 from TES assimilation (old version of MY24; dust_tes.nc file)
26#  =6 "cold" (low dust) scenario ; =7 "warm" (high dust) scenario
[1949]27#  =8 "climatology" (our best guess of a typical Mars year) scenario
[758]28#  =24 Mars Year 24  ; =25 Mars Year 25 (year with a global dust storm) ; ...
29#  =30 Mars Year 30
30iaervar = 24
31# Dust opacity at 610 Pa (when constant, i.e. for the iaervar=1 case)
32tauvis=0.1
33# Dust vertical distribution:
34# (=0: old distrib. (Pollack90), =1: top set by "topdustref",
35#  =2: Viking scenario; =3 MGS scenario)
36iddist  = 3
37# Dust top altitude (km). (Matters only if iddist=1)
38topdustref = 55.
39
40## Physical Parameterizations :
41## ~~~~~~~~~~~~~~~~~~~~~~~~~~
42# call radiative transfer ?
43callrad   = .true.
44# call NLTE radiative schemes ?   matters only if callrad=T
45callnlte = .true.
46# NLTE 15um scheme to use.
47# 0-> Old scheme, static oxygen
48# 1-> Old scheme, dynamic oxygen
49# 2-> New scheme
50nltemodel = 2
51# call CO2 NIR absorption ?   matters only if callrad=T
52callnirco2 = .true.
53# NIR NLTE correction ? matters only if callnirco2=T
54nircorr=1
55# call turbulent vertical diffusion ?
56calldifv  = .true.
57# call convective adjustment ?
58calladj  = .true.
59# Thermals
60calltherm = .true.
61callrichsl = .true.
62# call CO2 condensation ?
63callcond =.true.
64# call thermal conduction in the soil ?
65callsoil = .true.
66# call Lott's gravity wave/subgrid topography scheme ?
67calllott  = .true.
68# Impose polar cap surface albedos as observed by TES?
69TESicealbedo = .true.
70## Coefficient for Northern cap albedoes
71TESice_Ncoef=1.6
72## Coefficient for Southern cap albedoes
73TESice_Scoef=1.6
74
75
76## Radiative transfer options :
77## ~~~~~~~~~~~~~~~~~~~~~~~~~~
78# the rad.transfer is computed every "iradia" physical timestep
79iradia    = 1
80# Output of the exchange coefficient mattrix ? for diagnostic only
81callg2d  = .false.
82# Rayleigh scattering : (should be .false. for now)
83rayleigh  = .false.
84
[3448]85## Tracer (dust water, ice and/or chemical species) options :
86## ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
[758]87# DUST: Transported dust ? (if >0, use 'dustbin' dust bins)
88dustbin    = 2
89# DUST: Radiatively active dust ? (matters if dustbin>0)
90active  = .true.
91# DUST: use mass and number mixing ratios to predict dust size ?
92doubleq   = .true.
93# DUST: lifted by GCM surface winds ?
94lifting = .true.
95# DUST: lifted by dust devils ?
96callddevil = .false.
97# DUST: Scavenging by H2O/CO2 snowfall ?
98scavenging = .true.
99# DUST/WATERICE: Gravitationnal sedimentation ?
100sedimentation = .true.
101# WATERICE: Radiatively active transported atmospheric water ice ?
102activice   = .true.
103# WATER: Compute water cycle
104water = .true.
105# WATER: Microphysical scheme for water-ice clouds?
106microphys = .true.
107# WATER: parameter contact
108mteta = 0.95
[940]109# WATER: Effective variance for sedimentation for the log-normal
110#        distribution of ice particles ?
111nuice_sed=0.1
[758]112# WATER: current permanent caps at both poles. True IS RECOMMENDED
113#        (with .true., North cap is a source of water and South pole
114#         is a cold trap)
115caps  = .true.
116# WATER: Water ice albedo ?
117albedo_h2o_ice = 0.35
118# WATER: Water ice thermal inertia
119inert_h2o_ice = 800
120# WATER: Frost thickness threshold for albedo
121frost_albedo_threshold = 0.005
122# PHOTOCHEMISTRY: include chemical species
123photochem  = .true.
124
[1246]125# SCATTERERS: set number of scatterers. must be compliant with preceding options.
126naerkind = 2
127
128
[3448]129## Thermospheric options :
130##~~~~~~~~~~~~~~~~~~~~~~
[758]131# call thermosphere ?
132callthermos = .true.
133# WATER: included without cycle (only if water=.false.)
134thermoswater = .false.
135# call thermal conduction ? (only if callthermos=.true.)
136callconduct = .true.
137# call molecular viscosity ? (only if callthermos=.true.)
138callmolvis = .true.
139# call molecular diffusion ? (only if callthermos=.true.)
140callmoldiff = .true.
141# call thermospheric photochemistry ? (only if callthermos=.true.)
142thermochem = .true.
143# call EUV heating ? (only if callthermos=.true.)
144calleuv=.true.
145#Method to include solar variability?
[1686]146#0-> Fixed EUV input  1-> Variability with E10.7 as observed
[758]147solvarmod=0
[1686]148# fixed E10.7 value (for solvarmod=0)
149# (min=80 , ave=140, max=320)
150fixed_euv_value=140
151#Solar variability as observed for MY? (must be between MY23 and MY32)
[758]152# (only matters if solvarmod=1)
153solvaryear=24
154# value for the UV heating efficiency
155##(experimental values between 0.19 and 0.23, lower values may
156## be used to compensate for low 15 um cooling)
157euveff = 0.21       
158
159
160
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