Changeset 1949 for trunk/LMDZ.MARS/deftank
- Timestamp:
- Jun 19, 2018, 12:06:14 PM (6 years ago)
- Location:
- trunk/LMDZ.MARS/deftank
- Files:
-
- 2 deleted
- 5 edited
- 2 moved
Legend:
- Unmodified
- Added
- Removed
-
trunk/LMDZ.MARS/deftank/callphys.def.MCD5
r1686 r1949 5 5 6 6 #Directory where external input files are: 7 datadir=/ planeto/emlmd/run_mcd5.v0_new/datadir7 datadir=/users/lmdz/WWW/planets/mars/datadir 8 8 9 9 #Diurnal cycle ? if diurnal=False, diurnal averaged solar heating … … 27 27 # =4 Mars Year 24 from TES assimilation (old version of MY24; dust_tes.nc file) 28 28 # =6 "cold" (low dust) scenario ; =7 "warm" (high dust) scenario 29 # =8 "climatology" (our best guess of a typical Mars year) scenario 29 30 # =24 Mars Year 24 ; =25 Mars Year 25 (year with a global dust storm) ; ... 30 31 # =30 Mars Year 30 -
trunk/LMDZ.MARS/deftank/callphys.def.watercycle
r1922 r1949 20 20 21 21 #Directory where external input files are: 22 datadir=/users/ forget/WWW/datagcm/datafile/22 datadir=/users/lmdz/WWW/planets/mars/datadir 23 23 24 24 ## Dust scenario. Used if the dust is prescribed (i.e. if tracer=F or active=F) … … 27 27 # =4 Mars Year 24 from TES assimilation (old version of MY24; dust_tes.nc file) 28 28 # =6 "cold" (low dust) scenario ; =7 "warm" (high dust) scenario 29 # =8 "climatology" (our best guess of a typical Mars year) scenario 29 30 # =24 Mars Year 24 ; =25 Mars Year 25 (year with a global dust storm) ; ... 30 31 # =30 Mars Year 30 … … 45 46 # call NLTE radiative schemes ? matters only if callrad=T 46 47 callnlte = .true. 48 # NLTE 15um scheme to use. 49 # 0-> Old scheme, static oxygen 50 # 1-> Old scheme, dynamic oxygen 51 # 2-> New scheme 52 nltemodel = 0 47 53 # call CO2 NIR absorption ? matters only if callrad=T 48 54 callnirco2 = .true. 55 # NIR NLTE correction ? matters only if callnirco2=T 56 nircorr=0 49 57 # call turbulent vertical diffusion ? 50 58 calldifv = .true. 51 59 # call convective adjustment ? 52 60 calladj = .true. 61 # Thermals 62 calltherm = .true. 63 callrichsl = .true. 53 64 # call CO2 condensation ? 54 65 callcond =.true. … … 60 71 TESicealbedo = .true. 61 72 ## Coefficient for Northern cap albedoes 62 TESice_Ncoef=1. 473 TESice_Ncoef=1.6 63 74 ## Coefficient for Southern cap albedoes 64 TESice_Scoef=1. 475 TESice_Scoef=1.6 65 76 66 77 … … 130 141 # call thermal conduction ? (only if callthermos=.true.) 131 142 callconduct = .false. 132 # call EUV heating ? (only if callthermos=.true.)133 calleuv=.false.134 143 # call molecular viscosity ? (only if callthermos=.true.) 135 144 callmolvis = .false. … … 138 147 # call thermospheric photochemistry ? (only if callthermos=.true.) 139 148 thermochem = .false. 140 # date for solar flux calculation: (1985 < date < 2002) 141 ## (Solar min=1996.4 ave=1993.4 max=1990.6) 142 solarcondate = 1993.4 143 144 ## Thermals 145 ## ~~~~~~~~ 146 calltherm = .true. 147 callrichsl = .true. 149 # call EUV heating ? (only if callthermos=.true.) 150 calleuv=.false. 151 #Method to include solar variability? 152 #0-> Fixed EUV input 1-> Variability with E10.7 as observed 153 solvarmod=0 154 # fixed E10.7 value (for solvarmod=0) 155 # (min=80 , ave=140, max=320) 156 fixed_euv_value=140 157 #Solar variability as observed for MY? (must be between MY23 and MY32) 158 # (only matters if solvarmod=1) 159 solvaryear=24 160 # value for the UV heating efficiency 161 ##(experimental values between 0.19 and 0.23, lower values may 162 ## be used to compensate for low 15 um cooling) 163 euveff = 0.21 148 164 165 -
trunk/LMDZ.MARS/deftank/run.def.32x24x25
r1480 r1949 3 3 #GCM run control parameters: 4 4 #--------------------------- 5 6 # planet type 7 planet_type=mars 5 8 6 9 # Number of days to run model for -
trunk/LMDZ.MARS/deftank/run.def.32x24x32
r1480 r1949 3 3 #GCM run control parameters: 4 4 #--------------------------- 5 6 # planet type 7 planet_type=mars 5 8 6 9 # Number of days to run model for -
trunk/LMDZ.MARS/deftank/run.def.64x48x32
r575 r1949 1 1 # 2 2 #----------------------------------------------------------------------- 3 # Parametres de controle du run:4 #--------------------------- ---3 #GCM run control parameters: 4 #--------------------------- 5 5 6 # Nombre de jours d'integration 6 # planet type 7 planet_type=mars 8 9 # Number of days to run model for 7 10 nday=9999 8 11 9 # nombre de pas par jour (multiple de iperiod) ( ici pour dt = 1 min )12 # Number of dynamical steps per day (must be a multiple of iperiod) 10 13 day_step = 960 11 14 12 # periode pour le pas Matsuno (en pas)15 # Apply a Matsuno step every iperiod dynamical step 13 16 iperiod=5 14 17 15 # periode de sortie des variables de controle (en pas)18 # Control output information in the dynamics every iconser dynamical steps 16 19 iconser=120 17 20 18 # periode d'ecriture du fichier histoire (en jour) 19 iecri=100 20 21 # periode de stockage fichier histmoy (en jour) 22 periodav=60. 23 24 # periode de la dissipation (en pas) 21 # Apply dissipation every idissip dynamical steps 25 22 idissip=5 26 23 27 # choix de l'operateur de dissipation (star ou non star )24 # dissipation operator to use (star or non-star) 28 25 lstardis=.true. 29 26 30 # avec ou sans coordonnee hybrides27 # use hybrid vertical coordinate (else will use sigma levels) 31 28 hybrid=.true. 32 29 33 # nombre d'iterations de l'operateur de dissipation gradiv30 # use hybrid vertical coordinate (else will use sigma levels) 34 31 nitergdiv=1 35 32 36 # nombre d'iterations de l'operateur de dissipation nxgradrot33 # iterate lateral dissipation operator nxgradrot nitergrot times 37 34 nitergrot=2 38 35 39 # nombre d'iterations de l'operateur de dissipation divgrad36 # iterate lateral dissipation operator divgrad niterh times 40 37 niterh=2 41 38 42 # t emps de dissipation des plus petites long.d ondes pour u,v (gradiv)39 # time scale (s) for shortest wavelengths for u,v (gradiv) 43 40 tetagdiv= 4000. 44 41 45 # t emps de dissipation des plus petites long.d ondes pour u,v(nxgradrot)42 # time scale (s) for shortest wavelengths for u,v (nxgradrot) 46 43 tetagrot=5000. 47 44 48 # t emps de dissipation des plus petites long.d ondes pour h ( divgrad)45 # time scale (s) for shortest wavelengths for h (divgrad) 49 46 tetatemp=5000. 50 47 51 # coefficient pour gamdissip48 # coefficient for gamdissip 52 49 coefdis=0. 53 50 54 # choix du shema d'integration temporelle (Matsuno ou Matsuno-leapfrog)51 # time marching scheme (Matsuno if purmats is true, else Matsuno-Leapfrog) 55 52 purmats=.false. 56 53 57 # avec ou sans physique54 # run with (true) or without (false) physics 58 55 physic=.true. 59 56 60 # periode de la physique (en pas)61 iphysiq= 2057 # call physics every iphysiq dynamical steps 58 iphysiq=10 62 59 63 # choix d'une grille reguliere60 # Use a regular grid 64 61 grireg=.true. 65 62 66 # frequence (en pas) de l'ecriture du fichier diagfi63 # Output in diagfi file every ecritphy dynamical steps 67 64 ecritphy=240 68 65 69 # longitude en degres du centre du zoom66 # longitude (degrees) of zoom center 70 67 clon=63. 71 68 72 # latitude en degres du centre du zoom69 # latitude (degrees) of zoom center 73 70 clat=0. 74 71 75 # facteur de grossissement du zoom,selon longitude72 # enhancement factor of zoom, along longitudes 76 73 grossismx=1. 77 74 78 # facteur de grossissement du zoom ,selon latitude75 # enhancement factor of zoom, along latitudes 79 76 grossismy=1. 80 77 81 # Fonction f(y) hyperbolique si = .true. , sinon sinusoidale78 # Use an hyperbolic function f(y) if .true., else use a sine 82 79 fxyhypb=.false. 83 80 84 # exten sion en longitude de la zone du zoom ( fraction de la zone totale)81 # extention along longitudes of zoom region (fraction of global domain) 85 82 dzoomx= 0. 86 83 87 # exten sion en latitude de la zone du zoom ( fraction de la zone totale)84 # extention along latitudes of zoom region (fraction of global domain) 88 85 dzoomy=0. 89 86 90 # raideur du zoom en X87 # zoom stiffness along longitudes 91 88 taux=2. 92 89 93 # raideur du zoom en Y90 # zoom stiffness along latitudes 94 91 tauy=2. 95 92 96 # Fonction f(y) a vec y = Sin(latit.) si = .TRUE. , Sinon y = latit.93 # Fonction f(y) as y = Sin(latitude) if = .true. , else y = latitude 97 94 ysinus= .false. 98 95 99 # Avecsponge layer96 # Use a sponge layer 100 97 callsponge = .true. 101 98 99 # Sponge layer extends over topmost nsponge layers 100 nsponge = 3 101 102 102 # Sponge: mode0(u=v=0), mode1(u=umoy,v=0), mode2(u=umoy,v=vmoy) 103 mode_sponge= 2103 mode_sponge= 3 104 104 105 # Sponge : tetasponge (secondes)105 # Sponge layer time scale (s): tetasponge 106 106 tetasponge = 30000 107 107 -
trunk/LMDZ.MARS/deftank/traceur.def.watercycle
r38 r1949 1 2 1 7 2 co2 3 dust_number 4 dust_mass 5 ccn_number 6 ccn_mass 2 7 h2o_ice 3 8 h2o_vap
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