source: trunk/LMDZ.MARS/deftank/callphys.def @ 1242

Last change on this file since 1242 was 705, checked in by emillour, 13 years ago

Mars GCM:

  • Added possibility to run with a varying EUV cycle following real one. The flag solvarmod=1 triggers this behaviour, with companion flag solvaryear=## , where ## is the Mars Year (from 23 to 30). Setting solvarmod=0 reverts to 'old' behaviour, where there is a constant EUV forcing throughout the run, set by the "solarcondate" flag.
  • Needs corresponding input data files ("param_v6" subdirectory of "EUV" subdirectory in "datadir").
  • Added files jthermcalc_e107.F and param_read_e107.F in "aeronomars", modified files euvheat.F90, hrtherm.F, chemthermos.F90, param_v4.h and param_read.F in "aeronomars" and files inifis.F, physiq.F and callkeys.h in "phymars".

FGG

File size: 4.6 KB
Line 
1##General options
2##~~~~~~~~~~~~~~~
3#Run with or without tracer transport ?
4tracer=.false.
5
6#Where are the external files (dust, topography; chemistry,...)
7#datadir=/u/forget/WWW/datagcm/datafile
8
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)
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
31iaervar = 24
32# Dust opacity at 610 Pa (when constant, i.e. for the iaervar=1 case)
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.
47# NLTE 15um scheme to use.
48# 0-> Old scheme, static oxygen
49# 1-> Old scheme, dynamic oxygen
50# 2-> New scheme
51nltemodel = 1
52# call CO2 NIR absorption ?   matters only if callrad=T
53callnirco2 = .true.
54# NIR NLTE correction ? matters only if callnirco2=T
55nircorr=1
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.
68## Coefficient for Northern cap albedoes
69TESice_Ncoef=1.6
70## Coefficient for Southern cap albedoes
71TESice_Scoef=1.6
72
73
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
110## Thermospheric options (relevant if tracer=T) :
111##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
112# call thermosphere ?
113callthermos = .false.
114# WATER: included without cycle (only if water=.false.)
115thermoswater = .false.
116# call thermal conduction ? (only if callthermos=.true.)
117callconduct = .false.
118# call molecular viscosity ? (only if callthermos=.true.)
119callmolvis = .false.
120# call molecular diffusion ? (only if callthermos=.true.)
121callmoldiff = .false.
122# call thermospheric photochemistry ? (only if callthermos=.true.)
123thermochem = .false.
124# call EUV heating ? (only if callthermos=.true.)
125calleuv=.false.
126#Method to include solar variability?
127#0-> Old method   1-> Variability with E10.7 as observed
128solvarmod=1
129# date for solar flux calculation: (1985 < date < 2002)
130## (Solar min=1996.4 ave=1993.4 max=1990.6) ; Only used if solvarmod=0
131solarcondate = 1993.4
132#Solar variability as observed for MY? (must bebetween MY23 and MY30)
133# (only matters if solvarmod=1)
134solvaryear=24
135# value for the UV heating efficiency
136##(experimental values between 0.19 and 0.23, lower values may
137## be used to compensate for low 15 um cooling)
138euveff = 0.21       
139
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