- Timestamp:
- Feb 23, 2014, 4:38:20 PM (11 years ago)
- Location:
- trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER
- Files:
-
- 2 deleted
- 4 edited
- 1 moved
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trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER/callphys.def.mars0
r1115 r1187 125 125 microphys = .true. 126 126 microphys = .false. 127 # WATER: microphysics sub-timestep 128 # imicro = 2 5 10 129 imicro = 1 127 130 # WATER: parameter contact 128 131 mteta = 0.95 -
trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER/callphys.def.mars11_radact
r1180 r1187 114 114 # WATERICE: Radiatively active transported atmospheric water ice ? 115 115 activice = .true. 116 #activice = .false. 116 117 # WATER: Compute water cycle 117 118 water = .true. … … 119 120 microphys = .true. 120 121 microphys = .false. 122 # WATER: microphysics sub-timestep 123 # imicro = 2 5 10 124 imicro = 1 121 125 # WATER: parameter contact 122 126 mteta = 0.95 -
trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER/callphys.def.mars1_radact
r1185 r1187 3 3 #Run with or without tracer transport ? 4 4 tracer=.true. 5 6 #Directory where external input files are: 7 datadir=/planeto/emlmd/run_mcd5.v0_new/datadir 8 #datadir = /san/home/spiga/DATAFILE 9 #datadir = /d5/aslmd/datafile 10 #datadir=/users/forget/WWW/datagcm/datafile 11 datadir = /home/spiga/datadir/ 5 12 6 13 #Diurnal cycle ? if diurnal=False, diurnal averaged solar heating … … 14 21 15 22 #Save statistics in file "stats.nc" ? 23 callstats =.true. 16 24 callstats =.false. 17 25 … … 23 31 # =1 Dust opt.deph read in startfi; =2 Viking scenario; =3 MGS scenario, 24 32 # =4 Mars Year 24 from TES assimilation (old version of MY24; dust_tes.nc file) 25 # = 24 Mars Year 24 from TES assimilation (ie: MCD reference case)26 # =2 5 Mars Year 25 from TES assimilation (ie: a year with a global dust storm)27 # = 26 Mars Year 26 from TES assimilation28 iaervar = 2 629 # Dust opacity at 700 Pa (when constant, i.e. for the iaervar=1 case)30 tauvis=0. 233 # =6 "cold" (low dust) scenario ; =7 "warm" (high dust) scenario 34 # =24 Mars Year 24 ; =25 Mars Year 25 (year with a global dust storm) ; ... 35 # =30 Mars Year 30 36 iaervar = 24 37 # Dust opacity at 610 Pa (when constant, i.e. for the iaervar=1 case) 38 tauvis=0.1 31 39 # Dust vertical distribution: 32 40 # (=0: old distrib. (Pollack90), =1: top set by "topdustref", … … 41 49 callrad = .true. 42 50 # call NLTE radiative schemes ? matters only if callrad=T 51 callnlte = .true. 43 52 callnlte = .false. 53 # NLTE 15um scheme to use. 54 # 0-> Old scheme, static oxygen 55 # 1-> Old scheme, dynamic oxygen 56 # 2-> New scheme 57 nltemodel = 2 58 nltemodel = 0 44 59 # call CO2 NIR absorption ? matters only if callrad=T 45 60 callnirco2 = .true. 61 # NIR NLTE correction ? matters only if callnirco2=T 62 nircorr=1 63 nircorr=0 46 64 # call turbulent vertical diffusion ? 47 65 calldifv = .true. 48 66 # call convective adjustment ? 49 67 calladj = .true. 68 # Thermals 69 calltherm = .true. 70 callrichsl = .true. 50 71 # call CO2 condensation ? 51 72 callcond =.true. … … 53 74 callsoil = .true. 54 75 # call Lott's gravity wave/subgrid topography scheme ? 76 calllott = .true. 55 77 calllott = .false. 56 78 # Impose polar cap surface albedos as observed by TES? 57 79 TESicealbedo = .true. 80 TESicealbedo = .false. 81 ## Coefficient for Northern cap albedoes 82 TESice_Ncoef=1.6 83 ## Coefficient for Southern cap albedoes 84 TESice_Scoef=1.6 85 58 86 59 87 ## Radiative transfer options : … … 69 97 ## ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 70 98 # DUST: Transported dust ? (if >0, use 'dustbin' dust bins) 99 dustbin = 2 71 100 dustbin = 0 72 101 # DUST: Radiatively active dust ? (matters if dustbin>0) 102 active = .true. 73 103 active = .false. 74 104 # DUST: use mass and number mixing ratios to predict dust size ? 105 doubleq = .true. 75 106 doubleq = .false. 76 107 # DUST: lifted by GCM surface winds ? 77 lifting = .false. 108 lifting = .true. 109 lifting = .false. 78 110 # DUST: lifted by dust devils ? 79 111 callddevil = .false. 80 # DUST: Scavenging by CO2 snowfall ? 112 # DUST: Scavenging by H2O/CO2 snowfall ? 113 scavenging = .true. 81 114 scavenging = .false. 82 115 # DUST/WATERICE: Gravitationnal sedimentation ? 83 116 sedimentation = .true. 84 117 # WATERICE: Radiatively active transported atmospheric water ice ? 85 activice = .false. 118 activice = .true. 119 #activice = .false. 86 120 # WATER: Compute water cycle 87 121 water = .true. 122 # WATER: Microphysical scheme for water-ice clouds? 123 microphys = .true. 124 microphys = .false. 125 # WATER: microphysics sub-timestep 126 # imicro = 2 5 10 127 imicro = 1 128 # WATER: parameter contact 129 mteta = 0.95 130 # WATER: Effective variance for sedimentation for the log-normal 131 # distribution of ice particles ? 132 nuice_sed=0.1 88 133 # WATER: current permanent caps at both poles. True IS RECOMMENDED 89 134 # (with .true., North cap is a source of water and South pole 90 135 # is a cold trap) 91 caps = .false. 136 caps = .true. 137 # WATER: Water ice albedo ? 138 albedo_h2o_ice = 0.35 139 # WATER: Water ice thermal inertia 140 inert_h2o_ice = 800 141 # WATER: Frost thickness threshold for albedo 142 frost_albedo_threshold = 0.005 92 143 # PHOTOCHEMISTRY: include chemical species 144 photochem = .true. 93 145 photochem = .false. 94 146 … … 96 148 ##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 97 149 # call thermosphere ? 150 callthermos = .true. 98 151 callthermos = .false. 99 152 # WATER: included without cycle (only if water=.false.) 100 153 thermoswater = .false. 101 154 # call thermal conduction ? (only if callthermos=.true.) 155 callconduct = .true. 102 156 callconduct = .false. 103 # call EUV heating ? (only if callthermos=.true.)104 calleuv=.false.105 157 # call molecular viscosity ? (only if callthermos=.true.) 158 callmolvis = .true. 106 159 callmolvis = .false. 107 160 # call molecular diffusion ? (only if callthermos=.true.) 161 callmoldiff = .true. 108 162 callmoldiff = .false. 109 163 # call thermospheric photochemistry ? (only if callthermos=.true.) 164 thermochem = .true. 110 165 thermochem = .false. 166 # call EUV heating ? (only if callthermos=.true.) 167 calleuv=.true. 168 calleuv=.false. 169 #Method to include solar variability? 170 #0-> Old method (fixed EUV input) 1-> Variability with E10.7 as observed 171 solvarmod=0 111 172 # date for solar flux calculation: (1985 < date < 2002) 112 ## (Solar min=1996.4 ave=1993.4 max=1990.6) 173 ## (Solar min=1996.4 ave=1993.4 max=1990.6) ; Only used if solvarmod=0 113 174 solarcondate = 1993.4 114 175 #Solar variability as observed for MY? (must bebetween MY23 and MY30) 176 # (only matters if solvarmod=1) 177 solvaryear=24 178 # value for the UV heating efficiency 179 ##(experimental values between 0.19 and 0.23, lower values may 180 ## be used to compensate for low 15 um cooling) 181 euveff = 0.21 115 182 116 183 184 -
trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER/callphys.def.mars2
r1042 r1187 9 9 #datadir = /d5/aslmd/datafile 10 10 #datadir=/users/forget/WWW/datagcm/datafile 11 datadir = /home/spiga/datadir/ 11 12 12 13 #Diurnal cycle ? if diurnal=False, diurnal averaged solar heating … … 20 21 21 22 #Save statistics in file "stats.nc" ? 23 callstats =.true. 22 24 callstats =.false. 23 25 … … 33 35 # =30 Mars Year 30 34 36 iaervar = 24 35 iaervar = 2636 37 # Dust opacity at 610 Pa (when constant, i.e. for the iaervar=1 case) 37 38 tauvis=0.1 … … 73 74 callsoil = .true. 74 75 # call Lott's gravity wave/subgrid topography scheme ? 76 calllott = .true. 75 77 calllott = .false. 76 78 # Impose polar cap surface albedos as observed by TES? … … 122 124 microphys = .true. 123 125 microphys = .false. 126 # WATER: microphysics sub-timestep 127 # imicro = 2 5 10 128 imicro = 1 124 129 # WATER: parameter contact 125 130 mteta = 0.95 -
trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER/callphys.def.mars3
r1115 r1187 121 121 microphys = .true. 122 122 microphys = .false. 123 # WATER: microphysics sub-timestep 124 # imicro = 2 5 10 125 imicro = 1 123 126 # WATER: parameter contact 124 127 mteta = 0.95
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