source: trunk/LMDZ.MARS/deftank/callphys.def @ 1733

Last change on this file since 1733 was 1246, checked in by aslmd, 11 years ago

LMDZ.MARS. Made number of scatterers a free dimension not in need to be prescribe at compiling time. Instead it must be set in callphys.def. See README for further information about this commit.

File size: 4.7 KB
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[38]1##General options
2##~~~~~~~~~~~~~~~
3#Run with or without tracer transport ?
4tracer=.false.
5
[677]6#Where are the external files (dust, topography; chemistry,...)
7#datadir=/u/forget/WWW/datagcm/datafile
8
[38]9#Diurnal cycle ?  if diurnal=False, diurnal averaged solar heating
10diurnal=.true.
11
12#Seasonal cycle ? if season=False, Ls stays constant, to value set in "start"
13season = .true.   
14
15#write some more output on the screen ?
16lwrite = .false.   
17
18#Save statistics in file "stats.nc" ?
19callstats =.true.
20
21#Save EOF profiles in file "profiles" for Climate Database?
22calleofdump = .false.
23
24## Dust scenario. Used if the dust is prescribed (i.e. if tracer=F or active=F)
25## ~~~~~~~~~~~~~
26#  =1 Dust opt.deph read in startfi; =2 Viking scenario; =3 MGS scenario,
27#  =4 Mars Year 24 from TES assimilation (old version of MY24; dust_tes.nc file)
[677]28#  =6 "cold" (low dust) scenario ; =7 "warm" (high dust) scenario
29#  =24 Mars Year 24  ; =25 Mars Year 25 (year with a global dust storm) ; ...
30#  =30 Mars Year 30
[38]31iaervar = 24
[627]32# Dust opacity at 610 Pa (when constant, i.e. for the iaervar=1 case)
[38]33tauvis=0.2
34# Dust vertical distribution:
35# (=0: old distrib. (Pollack90), =1: top set by "topdustref",
36#  =2: Viking scenario; =3 MGS scenario)
37iddist  = 3
38# Dust top altitude (km). (Matters only if iddist=1)
39topdustref = 55.
40
41## Physical Parameterizations :
42## ~~~~~~~~~~~~~~~~~~~~~~~~~~
43# call radiative transfer ?
44callrad   = .true.
45# call NLTE radiative schemes ?   matters only if callrad=T
46callnlte = .true.
[705]47# NLTE 15um scheme to use.
48# 0-> Old scheme, static oxygen
49# 1-> Old scheme, dynamic oxygen
50# 2-> New scheme
51nltemodel = 1
[38]52# call CO2 NIR absorption ?   matters only if callrad=T
53callnirco2 = .true.
[705]54# NIR NLTE correction ? matters only if callnirco2=T
55nircorr=1
[38]56# call turbulent vertical diffusion ?
57calldifv  = .true.
58# call convective adjustment ?
59calladj  = .true.
60# call CO2 condensation ?
61callcond =.true.
62# call thermal conduction in the soil ?
63callsoil = .true.
64# call Lott's gravity wave/subgrid topography scheme ?
65calllott  = .true.
66# Impose polar cap surface albedos as observed by TES?
67TESicealbedo = .true.
[705]68## Coefficient for Northern cap albedoes
69TESice_Ncoef=1.6
70## Coefficient for Southern cap albedoes
71TESice_Scoef=1.6
[38]72
[705]73
[38]74## Radiative transfer options :
75## ~~~~~~~~~~~~~~~~~~~~~~~~~~
76# the rad.transfer is computed every "iradia" physical timestep
77iradia    = 1
78# Output of the exchange coefficient mattrix ? for diagnostic only
79callg2d  = .false.
80# Rayleigh scattering : (should be .false. for now)
81rayleigh  = .false.
82
83## Tracer (dust water, ice and/or chemical species) options (used if tracer=T):
84## ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
85# DUST: Transported dust ? (if >0, use 'dustbin' dust bins)
86dustbin    = 0
87# DUST: Radiatively active dust ? (matters if dustbin>0)
88active  = .false.
89# DUST: use mass and number mixing ratios to predict dust size ?
90doubleq   = .false.
91# DUST: lifted by GCM surface winds ?
92lifting = .false.
93# DUST: lifted by dust devils ?
94callddevil = .false.
95# DUST: Scavenging by CO2 snowfall ?
96scavenging = .false.
97# DUST/WATERICE: Gravitationnal sedimentation ?
98sedimentation = .false.
99# WATERICE: Radiatively active transported atmospheric water ice ?
100activice   = .false.
101# WATER: Compute water cycle
102water = .false.
103# WATER: current permanent caps at both poles. True IS RECOMMENDED
104#        (with .true., North cap is a source of water and South pole
105#         is a cold trap)
106caps  = .true.
107# PHOTOCHEMISTRY: include chemical species
108photochem  = .false.
109
[1246]110# SCATTERERS: set number of scatterers. must be compliant with preceding options.
111naerkind = 1
112
[38]113## Thermospheric options (relevant if tracer=T) :
114##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
115# call thermosphere ?
116callthermos = .false.
117# WATER: included without cycle (only if water=.false.)
118thermoswater = .false.
119# call thermal conduction ? (only if callthermos=.true.)
120callconduct = .false.
121# call molecular viscosity ? (only if callthermos=.true.)
122callmolvis = .false.
123# call molecular diffusion ? (only if callthermos=.true.)
124callmoldiff = .false.
125# call thermospheric photochemistry ? (only if callthermos=.true.)
126thermochem = .false.
[705]127# call EUV heating ? (only if callthermos=.true.)
128calleuv=.false.
129#Method to include solar variability?
130#0-> Old method   1-> Variability with E10.7 as observed
131solvarmod=1
[38]132# date for solar flux calculation: (1985 < date < 2002)
[705]133## (Solar min=1996.4 ave=1993.4 max=1990.6) ; Only used if solvarmod=0
[38]134solarcondate = 1993.4
[705]135#Solar variability as observed for MY? (must bebetween MY23 and MY30)
136# (only matters if solvarmod=1)
137solvaryear=24
138# value for the UV heating efficiency
139##(experimental values between 0.19 and 0.23, lower values may
140## be used to compensate for low 15 um cooling)
141euveff = 0.21       
[38]142
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