Changeset 1042 for trunk/MESOSCALE/LMD_MM_MARS/SIMU
- Timestamp:
- Sep 19, 2013, 2:15:35 AM (11 years ago)
- Location:
- trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER
- Files:
-
- 2 added
- 4 edited
- 2 copied
Legend:
- Unmodified
- Added
- Removed
-
trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER/callphys.def.mars0
r1041 r1042 1 1 ##General options 2 2 ##~~~~~~~~~~~~~~~ 3 #Directory where external input files are 4 datadir = /san/home/spiga/DATAFILE/ 5 datadir = /d5/aslmd/datafile/ 6 datadir=/users/forget/WWW/datagcm/datafile/ 3 #Run with or without tracer transport ? 4 tracer=.false. 7 5 8 #Run with or without tracer transport ? 9 tracer=.true. 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 10 11 11 12 #Diurnal cycle ? if diurnal=False, diurnal averaged solar heating … … 27 28 ## ~~~~~~~~~~~~~ 28 29 # =1 Dust opt.deph read in startfi; =2 Viking scenario; =3 MGS scenario, 29 # =4 Mars Year 24 from TES assimilation (same as =24 for now) 30 # =24 Mars Year 24 from TES assimilation (ie: MCD reference case) 31 # =25 Mars Year 25 from TES assimilation (ie: a year with a global dust storm) 32 # =26 Mars Year 26 from TES assimilation 33 iaervar = 26 34 # Dust opacity at 700 Pa (when constant, i.e. for the iaervar=1 case) 35 tauvis=0.2 30 # =4 Mars Year 24 from TES assimilation (old version of MY24; dust_tes.nc file) 31 # =6 "cold" (low dust) scenario ; =7 "warm" (high dust) scenario 32 # =24 Mars Year 24 ; =25 Mars Year 25 (year with a global dust storm) ; ... 33 # =30 Mars Year 30 34 iaervar = 24 35 iaervar = 26 36 # Dust opacity at 610 Pa (when constant, i.e. for the iaervar=1 case) 37 tauvis=0.1 36 38 # Dust vertical distribution: 37 39 # (=0: old distrib. (Pollack90), =1: top set by "topdustref", … … 46 48 callrad = .true. 47 49 # call NLTE radiative schemes ? matters only if callrad=T 48 callnlte = .false. #.true. 50 callnlte = .true. 51 callnlte = .false. 52 # NLTE 15um scheme to use. 53 # 0-> Old scheme, static oxygen 54 # 1-> Old scheme, dynamic oxygen 55 # 2-> New scheme 56 nltemodel = 2 57 nltemodel = 0 49 58 # call CO2 NIR absorption ? matters only if callrad=T 50 callnirco2 = .false. #.true. 59 callnirco2 = .true. 60 # NIR NLTE correction ? matters only if callnirco2=T 61 nircorr=1 62 nircorr=0 51 63 # call turbulent vertical diffusion ? 52 64 calldifv = .true. 53 65 # call convective adjustment ? 54 66 calladj = .true. 67 # Thermals 68 calltherm = .true. 69 callrichsl = .true. 55 70 # call CO2 condensation ? 56 71 callcond =.true. … … 61 76 # Impose polar cap surface albedos as observed by TES? 62 77 TESicealbedo = .true. 78 TESicealbedo = .false. 79 ## Coefficient for Northern cap albedoes 80 TESice_Ncoef=1.6 81 ## Coefficient for Southern cap albedoes 82 TESice_Scoef=1.6 83 63 84 64 85 ## Radiative transfer options : … … 74 95 ## ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 75 96 # DUST: Transported dust ? (if >0, use 'dustbin' dust bins) 76 dustbin = 0 97 dustbin = 2 98 dustbin = 0 77 99 # DUST: Radiatively active dust ? (matters if dustbin>0) 100 active = .true. 78 101 active = .false. 79 102 # DUST: use mass and number mixing ratios to predict dust size ? 80 doubleq = .false. 103 doubleq = .true. 104 doubleq = .false. 81 105 # DUST: lifted by GCM surface winds ? 106 lifting = .true. 82 107 lifting = .false. 83 108 # DUST: lifted by dust devils ? 84 109 callddevil = .false. 85 # DUST: Scavenging by CO2 snowfall ? 110 # DUST: Scavenging by H2O/CO2 snowfall ? 111 scavenging = .true. 86 112 scavenging = .false. 87 113 # DUST/WATERICE: Gravitationnal sedimentation ? 114 sedimentation = .true. 88 115 sedimentation = .false. 89 116 # WATERICE: Radiatively active transported atmospheric water ice ? 117 activice = .true. 90 118 activice = .false. 91 119 # WATER: Compute water cycle 120 water = .true. 92 121 water = .false. 93 122 # WATER: Microphysical scheme for water-ice clouds? 123 microphys = .true. 94 124 microphys = .false. 95 125 # WATER: parameter contact 96 126 mteta = 0.95 127 # WATER: Effective variance for sedimentation for the log-normal 128 # distribution of ice particles ? 129 nuice_sed=0.1 97 130 # WATER: current permanent caps at both poles. True IS RECOMMENDED 98 131 # (with .true., North cap is a source of water and South pole 99 132 # is a cold trap) 100 133 caps = .true. 134 caps = .false. 101 135 # WATER: Water ice albedo ? 102 136 albedo_h2o_ice = 0.35 … … 105 139 # WATER: Frost thickness threshold for albedo 106 140 frost_albedo_threshold = 0.005 107 nuice_sed=0.1108 icedryness=1109 nircorr=0110 imicro = 2111 imicro = 1112 141 # PHOTOCHEMISTRY: include chemical species 142 photochem = .true. 113 143 photochem = .false. 114 144 … … 116 146 ##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 117 147 # call thermosphere ? 148 callthermos = .true. 118 149 callthermos = .false. 119 150 # WATER: included without cycle (only if water=.false.) 120 151 thermoswater = .false. 121 152 # call thermal conduction ? (only if callthermos=.true.) 153 callconduct = .true. 122 154 callconduct = .false. 123 # call EUV heating ? (only if callthermos=.true.)124 calleuv=.false.125 155 # call molecular viscosity ? (only if callthermos=.true.) 156 callmolvis = .true. 126 157 callmolvis = .false. 127 158 # call molecular diffusion ? (only if callthermos=.true.) 159 callmoldiff = .true. 128 160 callmoldiff = .false. 129 161 # call thermospheric photochemistry ? (only if callthermos=.true.) 162 thermochem = .true. 130 163 thermochem = .false. 164 # call EUV heating ? (only if callthermos=.true.) 165 calleuv=.true. 166 calleuv=.false. 167 #Method to include solar variability? 168 #0-> Old method (fixed EUV input) 1-> Variability with E10.7 as observed 169 solvarmod=0 131 170 # date for solar flux calculation: (1985 < date < 2002) 132 ## (Solar min=1996.4 ave=1993.4 max=1990.6) 171 ## (Solar min=1996.4 ave=1993.4 max=1990.6) ; Only used if solvarmod=0 133 172 solarcondate = 1993.4 134 173 #Solar variability as observed for MY? (must bebetween MY23 and MY30) 174 # (only matters if solvarmod=1) 175 solvaryear=24 176 # value for the UV heating efficiency 177 ##(experimental values between 0.19 and 0.23, lower values may 178 ## be used to compensate for low 15 um cooling) 179 euveff = 0.21 135 180 136 ## Thermals 137 ## ~~~~~~~~ 138 calltherm = .true. 139 callrichsl = .true. 181 182 -
trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER/callphys.def.mars0.nothermals
r1041 r1042 3 3 #Run with or without tracer transport ? 4 4 tracer=.false. 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 5 11 6 12 #Diurnal cycle ? if diurnal=False, diurnal averaged solar heating … … 23 29 # =1 Dust opt.deph read in startfi; =2 Viking scenario; =3 MGS scenario, 24 30 # =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 # =25 Mars Year 25 from TES assimilation (ie: a year with a global dust storm) 27 # =26 Mars Year 26 from TES assimilation 28 iaervar = 26 29 # Dust opacity at 700 Pa (when constant, i.e. for the iaervar=1 case) 30 tauvis=0.2 31 # =6 "cold" (low dust) scenario ; =7 "warm" (high dust) scenario 32 # =24 Mars Year 24 ; =25 Mars Year 25 (year with a global dust storm) ; ... 33 # =30 Mars Year 30 34 iaervar = 24 35 iaervar = 26 36 # Dust opacity at 610 Pa (when constant, i.e. for the iaervar=1 case) 37 tauvis=0.1 31 38 # Dust vertical distribution: 32 39 # (=0: old distrib. (Pollack90), =1: top set by "topdustref", … … 41 48 callrad = .true. 42 49 # call NLTE radiative schemes ? matters only if callrad=T 50 callnlte = .true. 43 51 callnlte = .false. 52 # NLTE 15um scheme to use. 53 # 0-> Old scheme, static oxygen 54 # 1-> Old scheme, dynamic oxygen 55 # 2-> New scheme 56 nltemodel = 2 57 nltemodel = 0 44 58 # call CO2 NIR absorption ? matters only if callrad=T 45 59 callnirco2 = .true. 60 # NIR NLTE correction ? matters only if callnirco2=T 61 nircorr=1 62 nircorr=0 46 63 # call turbulent vertical diffusion ? 47 64 calldifv = .true. 48 65 # call convective adjustment ? 49 66 calladj = .true. 67 # Thermals 68 calltherm = .true. 69 callrichsl = .true. 70 calltherm = .false. 71 callrichsl = .false. 50 72 # call CO2 condensation ? 51 73 callcond =.true. … … 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 ? 116 sedimentation = .true. 83 117 sedimentation = .false. 84 118 # WATERICE: Radiatively active transported atmospheric water ice ? 119 activice = .true. 85 120 activice = .false. 86 121 # WATER: Compute water cycle 122 water = .true. 87 123 water = .false. 124 # WATER: Microphysical scheme for water-ice clouds? 125 microphys = .true. 126 microphys = .false. 127 # WATER: parameter contact 128 mteta = 0.95 129 # WATER: Effective variance for sedimentation for the log-normal 130 # distribution of ice particles ? 131 nuice_sed=0.1 88 132 # WATER: current permanent caps at both poles. True IS RECOMMENDED 89 133 # (with .true., North cap is a source of water and South pole 90 134 # is a cold trap) 135 caps = .true. 91 136 caps = .false. 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.mars11
r76 r1042 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 5 11 6 12 #Diurnal cycle ? if diurnal=False, diurnal averaged solar heating … … 23 29 # =1 Dust opt.deph read in startfi; =2 Viking scenario; =3 MGS scenario, 24 30 # =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 # =25 Mars Year 25 from TES assimilation (ie: a year with a global dust storm) 27 # =26 Mars Year 26 from TES assimilation 28 iaervar = 26 29 # Dust opacity at 700 Pa (when constant, i.e. for the iaervar=1 case) 30 tauvis=0.2 31 # =6 "cold" (low dust) scenario ; =7 "warm" (high dust) scenario 32 # =24 Mars Year 24 ; =25 Mars Year 25 (year with a global dust storm) ; ... 33 # =30 Mars Year 30 34 iaervar = 24 35 iaervar = 26 36 # Dust opacity at 610 Pa (when constant, i.e. for the iaervar=1 case) 37 tauvis=0.1 31 38 # Dust vertical distribution: 32 39 # (=0: old distrib. (Pollack90), =1: top set by "topdustref", … … 41 48 callrad = .true. 42 49 # call NLTE radiative schemes ? matters only if callrad=T 50 callnlte = .true. 43 51 callnlte = .false. 52 # NLTE 15um scheme to use. 53 # 0-> Old scheme, static oxygen 54 # 1-> Old scheme, dynamic oxygen 55 # 2-> New scheme 56 nltemodel = 2 57 nltemodel = 0 44 58 # call CO2 NIR absorption ? matters only if callrad=T 45 59 callnirco2 = .true. 60 # NIR NLTE correction ? matters only if callnirco2=T 61 nircorr=1 62 nircorr=0 46 63 # call turbulent vertical diffusion ? 47 64 calldifv = .true. 48 65 # call convective adjustment ? 49 66 calladj = .true. 67 # Thermals 68 calltherm = .true. 69 callrichsl = .true. 50 70 # call CO2 condensation ? 51 71 callcond =.true. … … 56 76 # Impose polar cap surface albedos as observed by TES? 57 77 TESicealbedo = .true. 78 TESicealbedo = .false. 79 ## Coefficient for Northern cap albedoes 80 TESice_Ncoef=1.6 81 ## Coefficient for Southern cap albedoes 82 TESice_Scoef=1.6 83 58 84 59 85 ## Radiative transfer options : … … 71 97 dustbin = 2 72 98 # DUST: Radiatively active dust ? (matters if dustbin>0) 73 active = . false.99 active = .true. 74 100 # DUST: use mass and number mixing ratios to predict dust size ? 75 doubleq = .true. 101 doubleq = .true. 76 102 # DUST: lifted by GCM surface winds ? 77 lifting = .true. 103 lifting = .true. 104 lifting = .false. 78 105 # DUST: lifted by dust devils ? 79 106 callddevil = .false. 80 # DUST: Scavenging by CO2 snowfall ? 107 # DUST: Scavenging by H2O/CO2 snowfall ? 108 scavenging = .true. 81 109 scavenging = .false. 82 110 # DUST/WATERICE: Gravitationnal sedimentation ? 83 111 sedimentation = .true. 84 112 # WATERICE: Radiatively active transported atmospheric water ice ? 113 activice = .true. 85 114 activice = .false. 86 115 # WATER: Compute water cycle 87 116 water = .true. 117 # WATER: Microphysical scheme for water-ice clouds? 118 microphys = .true. 119 microphys = .false. 120 # WATER: parameter contact 121 mteta = 0.95 122 # WATER: Effective variance for sedimentation for the log-normal 123 # distribution of ice particles ? 124 nuice_sed=0.1 88 125 # WATER: current permanent caps at both poles. True IS RECOMMENDED 89 126 # (with .true., North cap is a source of water and South pole 90 127 # is a cold trap) 91 caps = .false. #.true. 128 caps = .true. 129 # WATER: Water ice albedo ? 130 albedo_h2o_ice = 0.35 131 # WATER: Water ice thermal inertia 132 inert_h2o_ice = 800 133 # WATER: Frost thickness threshold for albedo 134 frost_albedo_threshold = 0.005 92 135 # PHOTOCHEMISTRY: include chemical species 136 photochem = .true. 93 137 photochem = .false. 94 138 … … 96 140 ##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 97 141 # call thermosphere ? 142 callthermos = .true. 98 143 callthermos = .false. 99 144 # WATER: included without cycle (only if water=.false.) 100 145 thermoswater = .false. 101 146 # call thermal conduction ? (only if callthermos=.true.) 147 callconduct = .true. 102 148 callconduct = .false. 103 # call EUV heating ? (only if callthermos=.true.)104 calleuv=.false.105 149 # call molecular viscosity ? (only if callthermos=.true.) 150 callmolvis = .true. 106 151 callmolvis = .false. 107 152 # call molecular diffusion ? (only if callthermos=.true.) 153 callmoldiff = .true. 108 154 callmoldiff = .false. 109 155 # call thermospheric photochemistry ? (only if callthermos=.true.) 156 thermochem = .true. 110 157 thermochem = .false. 158 # call EUV heating ? (only if callthermos=.true.) 159 calleuv=.true. 160 calleuv=.false. 161 #Method to include solar variability? 162 #0-> Old method (fixed EUV input) 1-> Variability with E10.7 as observed 163 solvarmod=0 111 164 # date for solar flux calculation: (1985 < date < 2002) 112 ## (Solar min=1996.4 ave=1993.4 max=1990.6) 165 ## (Solar min=1996.4 ave=1993.4 max=1990.6) ; Only used if solvarmod=0 113 166 solarcondate = 1993.4 114 167 #Solar variability as observed for MY? (must bebetween MY23 and MY30) 168 # (only matters if solvarmod=1) 169 solvaryear=24 170 # value for the UV heating efficiency 171 ##(experimental values between 0.19 and 0.23, lower values may 172 ## be used to compensate for low 15 um cooling) 173 euveff = 0.21 115 174 116 175 176 -
trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER/callphys.def.mars11_radact
r81 r1042 1 1 ##General options 2 2 ##~~~~~~~~~~~~~~~ 3 #Directory where external input files are4 datadir = /san/home/spiga/DATAFILE/5 6 3 #Run with or without tracer transport ? 7 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 8 11 9 12 #Diurnal cycle ? if diurnal=False, diurnal averaged solar heating … … 26 29 # =1 Dust opt.deph read in startfi; =2 Viking scenario; =3 MGS scenario, 27 30 # =4 Mars Year 24 from TES assimilation (old version of MY24; dust_tes.nc file) 28 # =24 Mars Year 24 from TES assimilation (ie: MCD reference case) 29 # =25 Mars Year 25 from TES assimilation (ie: a year with a global dust storm) 30 # =26 Mars Year 26 from TES assimilation 31 iaervar = 26 32 # Dust opacity at 700 Pa (when constant, i.e. for the iaervar=1 case) 33 tauvis=0.2 31 # =6 "cold" (low dust) scenario ; =7 "warm" (high dust) scenario 32 # =24 Mars Year 24 ; =25 Mars Year 25 (year with a global dust storm) ; ... 33 # =30 Mars Year 30 34 iaervar = 24 35 iaervar = 26 36 # Dust opacity at 610 Pa (when constant, i.e. for the iaervar=1 case) 37 tauvis=0.1 34 38 # Dust vertical distribution: 35 39 # (=0: old distrib. (Pollack90), =1: top set by "topdustref", … … 44 48 callrad = .true. 45 49 # call NLTE radiative schemes ? matters only if callrad=T 50 callnlte = .true. 46 51 callnlte = .false. 52 # NLTE 15um scheme to use. 53 # 0-> Old scheme, static oxygen 54 # 1-> Old scheme, dynamic oxygen 55 # 2-> New scheme 56 nltemodel = 2 57 nltemodel = 0 47 58 # call CO2 NIR absorption ? matters only if callrad=T 48 59 callnirco2 = .true. 60 # NIR NLTE correction ? matters only if callnirco2=T 61 nircorr=1 62 nircorr=0 49 63 # call turbulent vertical diffusion ? 50 64 calldifv = .true. 51 65 # call convective adjustment ? 52 66 calladj = .true. 67 # Thermals 68 calltherm = .true. 69 callrichsl = .true. 53 70 # call CO2 condensation ? 54 71 callcond =.true. … … 59 76 # Impose polar cap surface albedos as observed by TES? 60 77 TESicealbedo = .true. 78 TESicealbedo = .false. 79 ## Coefficient for Northern cap albedoes 80 TESice_Ncoef=1.6 81 ## Coefficient for Southern cap albedoes 82 TESice_Scoef=1.6 83 61 84 62 85 ## Radiative transfer options : … … 76 99 active = .true. 77 100 # DUST: use mass and number mixing ratios to predict dust size ? 78 doubleq = .true. 101 doubleq = .true. 79 102 # DUST: lifted by GCM surface winds ? 80 lifting = .true. 103 lifting = .true. 104 lifting = .false. 81 105 # DUST: lifted by dust devils ? 82 106 callddevil = .false. 83 # DUST: Scavenging by CO2 snowfall ? 107 # DUST: Scavenging by H2O/CO2 snowfall ? 108 scavenging = .true. 84 109 scavenging = .false. 85 110 # DUST/WATERICE: Gravitationnal sedimentation ? … … 89 114 # WATER: Compute water cycle 90 115 water = .true. 116 # WATER: Microphysical scheme for water-ice clouds? 117 microphys = .true. 118 microphys = .false. 119 # WATER: parameter contact 120 mteta = 0.95 121 # WATER: Effective variance for sedimentation for the log-normal 122 # distribution of ice particles ? 123 nuice_sed=0.1 91 124 # WATER: current permanent caps at both poles. True IS RECOMMENDED 92 125 # (with .true., North cap is a source of water and South pole 93 126 # is a cold trap) 94 127 caps = .true. 128 # WATER: Water ice albedo ? 129 albedo_h2o_ice = 0.35 130 # WATER: Water ice thermal inertia 131 inert_h2o_ice = 800 132 # WATER: Frost thickness threshold for albedo 133 frost_albedo_threshold = 0.005 95 134 # PHOTOCHEMISTRY: include chemical species 135 photochem = .true. 96 136 photochem = .false. 97 137 … … 99 139 ##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 100 140 # call thermosphere ? 141 callthermos = .true. 101 142 callthermos = .false. 102 143 # WATER: included without cycle (only if water=.false.) 103 144 thermoswater = .false. 104 145 # call thermal conduction ? (only if callthermos=.true.) 146 callconduct = .true. 105 147 callconduct = .false. 106 # call EUV heating ? (only if callthermos=.true.)107 calleuv=.false.108 148 # call molecular viscosity ? (only if callthermos=.true.) 149 callmolvis = .true. 109 150 callmolvis = .false. 110 151 # call molecular diffusion ? (only if callthermos=.true.) 152 callmoldiff = .true. 111 153 callmoldiff = .false. 112 154 # call thermospheric photochemistry ? (only if callthermos=.true.) 155 thermochem = .true. 113 156 thermochem = .false. 157 # call EUV heating ? (only if callthermos=.true.) 158 calleuv=.true. 159 calleuv=.false. 160 #Method to include solar variability? 161 #0-> Old method (fixed EUV input) 1-> Variability with E10.7 as observed 162 solvarmod=0 114 163 # date for solar flux calculation: (1985 < date < 2002) 115 ## (Solar min=1996.4 ave=1993.4 max=1990.6) 164 ## (Solar min=1996.4 ave=1993.4 max=1990.6) ; Only used if solvarmod=0 116 165 solarcondate = 1993.4 117 166 #Solar variability as observed for MY? (must bebetween MY23 and MY30) 167 # (only matters if solvarmod=1) 168 solvaryear=24 169 # value for the UV heating efficiency 170 ##(experimental values between 0.19 and 0.23, lower values may 171 ## be used to compensate for low 15 um cooling) 172 euveff = 0.21 118 173 119 174 175 -
trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER/callphys.def.mars2
r76 r1042 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 5 11 6 12 #Diurnal cycle ? if diurnal=False, diurnal averaged solar heating … … 23 29 # =1 Dust opt.deph read in startfi; =2 Viking scenario; =3 MGS scenario, 24 30 # =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 # =25 Mars Year 25 from TES assimilation (ie: a year with a global dust storm) 27 # =26 Mars Year 26 from TES assimilation 28 iaervar = 26 29 # Dust opacity at 700 Pa (when constant, i.e. for the iaervar=1 case) 30 tauvis=0.2 31 # =6 "cold" (low dust) scenario ; =7 "warm" (high dust) scenario 32 # =24 Mars Year 24 ; =25 Mars Year 25 (year with a global dust storm) ; ... 33 # =30 Mars Year 30 34 iaervar = 24 35 iaervar = 26 36 # Dust opacity at 610 Pa (when constant, i.e. for the iaervar=1 case) 37 tauvis=0.1 31 38 # Dust vertical distribution: 32 39 # (=0: old distrib. (Pollack90), =1: top set by "topdustref", … … 41 48 callrad = .true. 42 49 # call NLTE radiative schemes ? matters only if callrad=T 50 callnlte = .true. 43 51 callnlte = .false. 52 # NLTE 15um scheme to use. 53 # 0-> Old scheme, static oxygen 54 # 1-> Old scheme, dynamic oxygen 55 # 2-> New scheme 56 nltemodel = 2 57 nltemodel = 0 44 58 # call CO2 NIR absorption ? matters only if callrad=T 45 59 callnirco2 = .true. 60 # NIR NLTE correction ? matters only if callnirco2=T 61 nircorr=1 62 nircorr=0 46 63 # call turbulent vertical diffusion ? 47 64 calldifv = .true. 48 65 # call convective adjustment ? 49 66 calladj = .true. 67 # Thermals 68 calltherm = .true. 69 callrichsl = .true. 50 70 # call CO2 condensation ? 51 71 callcond =.true. … … 56 76 # Impose polar cap surface albedos as observed by TES? 57 77 TESicealbedo = .true. 78 TESicealbedo = .false. 79 ## Coefficient for Northern cap albedoes 80 TESice_Ncoef=1.6 81 ## Coefficient for Southern cap albedoes 82 TESice_Scoef=1.6 83 58 84 59 85 ## Radiative transfer options : … … 69 95 ## ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 70 96 # DUST: Transported dust ? (if >0, use 'dustbin' dust bins) 97 dustbin = 2 71 98 dustbin = 1 72 99 # DUST: Radiatively active dust ? (matters if dustbin>0) 100 active = .true. 73 101 active = .false. 74 102 # DUST: use mass and number mixing ratios to predict dust size ? 75 doubleq = .false. 103 doubleq = .true. 104 doubleq = .false. 76 105 # DUST: lifted by GCM surface winds ? 77 lifting = .true. #.false. 106 lifting = .true. 107 lifting = .false. 78 108 # DUST: lifted by dust devils ? 79 109 callddevil = .false. 80 # DUST: Scavenging by CO2 snowfall ? 110 # DUST: Scavenging by H2O/CO2 snowfall ? 111 scavenging = .true. 81 112 scavenging = .false. 82 113 # DUST/WATERICE: Gravitationnal sedimentation ? 83 114 sedimentation = .true. 84 115 # WATERICE: Radiatively active transported atmospheric water ice ? 116 activice = .true. 85 117 activice = .false. 86 118 # WATER: Compute water cycle 87 water = .false. #.true. 119 water = .true. 120 water = .false. 121 # WATER: Microphysical scheme for water-ice clouds? 122 microphys = .true. 123 microphys = .false. 124 # WATER: parameter contact 125 mteta = 0.95 126 # WATER: Effective variance for sedimentation for the log-normal 127 # distribution of ice particles ? 128 nuice_sed=0.1 88 129 # WATER: current permanent caps at both poles. True IS RECOMMENDED 89 130 # (with .true., North cap is a source of water and South pole 90 131 # is a cold trap) 91 caps = .false. #.true. 132 caps = .true. 133 caps = .false. 134 # WATER: Water ice albedo ? 135 albedo_h2o_ice = 0.35 136 # WATER: Water ice thermal inertia 137 inert_h2o_ice = 800 138 # WATER: Frost thickness threshold for albedo 139 frost_albedo_threshold = 0.005 92 140 # PHOTOCHEMISTRY: include chemical species 141 photochem = .true. 93 142 photochem = .false. 94 143 … … 96 145 ##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 97 146 # call thermosphere ? 147 callthermos = .true. 98 148 callthermos = .false. 99 149 # WATER: included without cycle (only if water=.false.) 100 150 thermoswater = .false. 101 151 # call thermal conduction ? (only if callthermos=.true.) 152 callconduct = .true. 102 153 callconduct = .false. 103 # call EUV heating ? (only if callthermos=.true.)104 calleuv=.false.105 154 # call molecular viscosity ? (only if callthermos=.true.) 155 callmolvis = .true. 106 156 callmolvis = .false. 107 157 # call molecular diffusion ? (only if callthermos=.true.) 158 callmoldiff = .true. 108 159 callmoldiff = .false. 109 160 # call thermospheric photochemistry ? (only if callthermos=.true.) 161 thermochem = .true. 110 162 thermochem = .false. 163 # call EUV heating ? (only if callthermos=.true.) 164 calleuv=.true. 165 calleuv=.false. 166 #Method to include solar variability? 167 #0-> Old method (fixed EUV input) 1-> Variability with E10.7 as observed 168 solvarmod=0 111 169 # date for solar flux calculation: (1985 < date < 2002) 112 ## (Solar min=1996.4 ave=1993.4 max=1990.6) 170 ## (Solar min=1996.4 ave=1993.4 max=1990.6) ; Only used if solvarmod=0 113 171 solarcondate = 1993.4 114 172 #Solar variability as observed for MY? (must bebetween MY23 and MY30) 173 # (only matters if solvarmod=1) 174 solvaryear=24 175 # value for the UV heating efficiency 176 ##(experimental values between 0.19 and 0.23, lower values may 177 ## be used to compensate for low 15 um cooling) 178 euveff = 0.21 115 179 116 180 181 -
trunk/MESOSCALE/LMD_MM_MARS/SIMU/DEF/newphys_THARSIS_WATER/callphys.def.mars3
r88 r1042 1 1 ##General options 2 2 ##~~~~~~~~~~~~~~~ 3 # Directory where external input files are4 datadir = /san/home/spiga/DATAFILE/ 3 #Run with or without tracer transport ? 4 tracer=.false. 5 5 6 #Run with or without tracer transport ? 7 tracer=.true. 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 8 11 9 12 #Diurnal cycle ? if diurnal=False, diurnal averaged solar heating … … 26 29 # =1 Dust opt.deph read in startfi; =2 Viking scenario; =3 MGS scenario, 27 30 # =4 Mars Year 24 from TES assimilation (old version of MY24; dust_tes.nc file) 28 # =24 Mars Year 24 from TES assimilation (ie: MCD reference case) 29 # =25 Mars Year 25 from TES assimilation (ie: a year with a global dust storm) 30 # =26 Mars Year 26 from TES assimilation 31 iaervar = 26 32 # Dust opacity at 700 Pa (when constant, i.e. for the iaervar=1 case) 33 tauvis=0.2 31 # =6 "cold" (low dust) scenario ; =7 "warm" (high dust) scenario 32 # =24 Mars Year 24 ; =25 Mars Year 25 (year with a global dust storm) ; ... 33 # =30 Mars Year 30 34 iaervar = 24 35 iaervar = 26 36 # Dust opacity at 610 Pa (when constant, i.e. for the iaervar=1 case) 37 tauvis=0.1 34 38 # Dust vertical distribution: 35 39 # (=0: old distrib. (Pollack90), =1: top set by "topdustref", … … 44 48 callrad = .true. 45 49 # call NLTE radiative schemes ? matters only if callrad=T 50 callnlte = .true. 46 51 callnlte = .false. 52 # NLTE 15um scheme to use. 53 # 0-> Old scheme, static oxygen 54 # 1-> Old scheme, dynamic oxygen 55 # 2-> New scheme 56 nltemodel = 2 57 nltemodel = 0 47 58 # call CO2 NIR absorption ? matters only if callrad=T 48 59 callnirco2 = .true. 60 # NIR NLTE correction ? matters only if callnirco2=T 61 nircorr=1 62 nircorr=0 49 63 # call turbulent vertical diffusion ? 50 64 calldifv = .true. 51 65 # call convective adjustment ? 52 66 calladj = .true. 67 # Thermals 68 calltherm = .true. 69 callrichsl = .true. 53 70 # call CO2 condensation ? 54 71 callcond =.true. … … 59 76 # Impose polar cap surface albedos as observed by TES? 60 77 TESicealbedo = .true. 78 TESicealbedo = .false. 79 ## Coefficient for Northern cap albedoes 80 TESice_Ncoef=1.6 81 ## Coefficient for Southern cap albedoes 82 TESice_Scoef=1.6 83 61 84 62 85 ## Radiative transfer options : … … 74 97 dustbin = 2 75 98 # DUST: Radiatively active dust ? (matters if dustbin>0) 76 active = .true. #.false.99 active = .true. 77 100 # DUST: use mass and number mixing ratios to predict dust size ? 78 doubleq = .true. #.false.101 doubleq = .true. 79 102 # DUST: lifted by GCM surface winds ? 80 lifting = .true. #.false. 103 lifting = .true. 104 lifting = .false. 81 105 # DUST: lifted by dust devils ? 82 106 callddevil = .false. 83 # DUST: Scavenging by CO2 snowfall ? 107 # DUST: Scavenging by H2O/CO2 snowfall ? 108 scavenging = .true. 84 109 scavenging = .false. 85 110 # DUST/WATERICE: Gravitationnal sedimentation ? 86 111 sedimentation = .true. 87 112 # WATERICE: Radiatively active transported atmospheric water ice ? 113 activice = .true. 88 114 activice = .false. 89 115 # WATER: Compute water cycle 90 water = .false. #.true. 116 water = .true. 117 water = .false. 118 # WATER: Microphysical scheme for water-ice clouds? 119 microphys = .true. 120 microphys = .false. 121 # WATER: parameter contact 122 mteta = 0.95 123 # WATER: Effective variance for sedimentation for the log-normal 124 # distribution of ice particles ? 125 nuice_sed=0.1 91 126 # WATER: current permanent caps at both poles. True IS RECOMMENDED 92 127 # (with .true., North cap is a source of water and South pole 93 128 # is a cold trap) 94 caps = .false. #.true. 129 caps = .true. 130 caps = .false. 131 # WATER: Water ice albedo ? 132 albedo_h2o_ice = 0.35 133 # WATER: Water ice thermal inertia 134 inert_h2o_ice = 800 135 # WATER: Frost thickness threshold for albedo 136 frost_albedo_threshold = 0.005 95 137 # PHOTOCHEMISTRY: include chemical species 138 photochem = .true. 96 139 photochem = .false. 97 140 … … 99 142 ##~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 100 143 # call thermosphere ? 144 callthermos = .true. 101 145 callthermos = .false. 102 146 # WATER: included without cycle (only if water=.false.) 103 147 thermoswater = .false. 104 148 # call thermal conduction ? (only if callthermos=.true.) 149 callconduct = .true. 105 150 callconduct = .false. 106 # call EUV heating ? (only if callthermos=.true.)107 calleuv=.false.108 151 # call molecular viscosity ? (only if callthermos=.true.) 152 callmolvis = .true. 109 153 callmolvis = .false. 110 154 # call molecular diffusion ? (only if callthermos=.true.) 155 callmoldiff = .true. 111 156 callmoldiff = .false. 112 157 # call thermospheric photochemistry ? (only if callthermos=.true.) 158 thermochem = .true. 113 159 thermochem = .false. 160 # call EUV heating ? (only if callthermos=.true.) 161 calleuv=.true. 162 calleuv=.false. 163 #Method to include solar variability? 164 #0-> Old method (fixed EUV input) 1-> Variability with E10.7 as observed 165 solvarmod=0 114 166 # date for solar flux calculation: (1985 < date < 2002) 115 ## (Solar min=1996.4 ave=1993.4 max=1990.6) 167 ## (Solar min=1996.4 ave=1993.4 max=1990.6) ; Only used if solvarmod=0 116 168 solarcondate = 1993.4 117 169 #Solar variability as observed for MY? (must bebetween MY23 and MY30) 170 # (only matters if solvarmod=1) 171 solvaryear=24 172 # value for the UV heating efficiency 173 ##(experimental values between 0.19 and 0.23, lower values may 174 ## be used to compensate for low 15 um cooling) 175 euveff = 0.21 118 176 119 177 178
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