1 | program kcm1d |
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2 | |
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3 | use infotrac, only: nqtot |
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4 | use radinc_h, only: NAERKIND |
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5 | use radcommon_h, only: L_NSPECTI, L_NSPECTV, sigma, glat |
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6 | use watercommon_h, only: mH2O |
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7 | use ioipsl_getincom, only: getin |
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8 | use comsaison_h, only: mu0, fract, dist_star |
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9 | use planete_mod |
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10 | use callkeys_mod, only: check_cpp_match, pceil, tstrat, tracer, global1d |
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11 | use inifis_mod, only: inifis |
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12 | use comcstfi_mod |
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13 | use mod_grid_phy_lmdz, only : regular_lonlat |
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14 | use regular_lonlat_mod, only: init_regular_lonlat |
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15 | use physics_distribution_mod, only: init_physics_distribution |
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16 | use regular_lonlat_mod, only: init_regular_lonlat |
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17 | use mod_interface_dyn_phys, only: init_interface_dyn_phys |
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18 | use geometry_mod, only: init_geometry |
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19 | use dimphy, only : init_dimphy |
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20 | |
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21 | implicit none |
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22 | |
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23 | !================================================================== |
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24 | ! |
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25 | ! Purpose |
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26 | ! ------- |
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27 | ! Run the universal model radiative transfer once in a 1D column. |
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28 | ! Useful for climate evolution studies etc. |
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29 | ! |
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30 | ! It can be compiled with a command like (e.g. for 25 layers): |
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31 | ! "makegcm -p std -d 25 kcm1d" |
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32 | ! It requires the files "callphys.def", "gases.def" |
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33 | ! "traceur.def", and "run.def" with a line "INCLUDEDEF=callphys.def" |
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34 | ! |
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35 | ! Authors |
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36 | ! ------- |
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37 | ! - R. Wordsworth |
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38 | ! - updated by M. Turbet (June 2017) |
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39 | ! |
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40 | !================================================================== |
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41 | |
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42 | #include "dimensions.h" |
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43 | !#include "dimphys.h" |
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44 | |
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45 | ! -------------------------------------------------------------- |
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46 | ! Declarations |
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47 | ! -------------------------------------------------------------- |
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48 | |
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49 | integer nlayer,nlevel,nq |
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50 | integer ilay,ilev,iq,iw,iter |
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51 | real play(llm) ! Pressure at the middle of the layers [Pa] |
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52 | real zlay(llm) ! Altitude at middle of the layers [km] |
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53 | real plev(llm+1) ! Intermediate pressure levels [Pa] |
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54 | real temp(llm) ! temperature at the middle of the layers [K] |
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55 | real,allocatable :: q(:,:) ! tracer mixing ratio [kg/kg] |
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56 | real,allocatable :: vmr(:,:) ! tracer mixing ratio [mol/mol] |
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57 | real,allocatable :: qsurf(:) ! tracer surface budget [kg/kg] ???? |
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58 | real psurf,psurf_n,tsurf |
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59 | |
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60 | real emis, albedo, albedo_equivalent |
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61 | real albedo_wv(1,L_NSPECTV) |
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62 | |
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63 | real muvar(llm+1) |
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64 | |
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65 | real dtsw(llm) ! heating rate (K/s) due to SW |
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66 | real dtlw(llm) ! heating rate (K/s) due to LW |
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67 | real fluxsurf_lw ! incident LW flux to surf (W/m2) |
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68 | real fluxtop_lw ! outgoing LW flux to space (W/m2) |
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69 | real fluxsurf_sw ! incident SW flux to surf (W/m2) |
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70 | real fluxsurfabs_sw ! absorbed SW flux by the surf (W/m2) |
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71 | real fluxabs_sw ! SW flux absorbed by planet (W/m2) |
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72 | real fluxtop_dn ! incident top of atmosphere SW flux (W/m2) |
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73 | |
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74 | ! not used |
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75 | real cloudfrac(llm) |
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76 | real totcloudfrac |
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77 | real tau_col |
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78 | |
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79 | real dTstrat |
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80 | real aerosol(llm,naerkind) ! aerosol tau (kg/kg) |
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81 | real OLR_nu(1,L_NSPECTI) |
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82 | real OSR_nu(1,L_NSPECTV) |
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83 | real Eatmtot |
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84 | |
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85 | integer ierr |
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86 | logical firstcall,lastcall |
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87 | |
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88 | character*20,allocatable :: nametrac(:) ! name of the tracer (no need for adv trac common) |
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89 | |
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90 | real :: latitude(1), longitude(1), cell_area(1), phisfi(1) |
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91 | |
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92 | ! added by JVO and YJ to read modern traceur.def |
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93 | character(len=500) :: line ! to store a line of text |
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94 | LOGICAL :: moderntracdef=.false. ! JVO, YJ : modern traceur.def |
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95 | |
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96 | ! -------------- |
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97 | ! Initialisation |
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98 | ! -------------- |
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99 | |
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100 | pi=2.E+0*asin(1.E+0) |
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101 | |
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102 | cloudfrac(:) = 0.0 |
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103 | totcloudfrac = 0.0 |
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104 | |
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105 | |
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106 | nlayer=llm |
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107 | nlevel=nlayer+1 |
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108 | |
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109 | !! this is defined in comsaison_h |
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110 | ALLOCATE(mu0(1)) |
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111 | ALLOCATE(fract(1)) |
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112 | ALLOCATE(glat(1)) |
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113 | |
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114 | ! Load parameters from "run.def" |
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115 | ! ------------------------------- |
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116 | |
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117 | ! check if 'kcm1d.def' file is around (otherwise reading parameters |
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118 | ! from callphys.def via getin() routine won't work.) |
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119 | open(90,file='kcm1d.def',status='old',form='formatted',& |
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120 | iostat=ierr) |
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121 | if (ierr.ne.0) then |
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122 | write(*,*) 'Cannot find required file "kcm1d.def"' |
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123 | write(*,*) ' (which should contain some input parameters' |
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124 | write(*,*) ' along with the following line:' |
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125 | write(*,*) ' INCLUDEDEF=callphys.def' |
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126 | write(*,*) ' )' |
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127 | write(*,*) ' ... might as well stop here ...' |
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128 | stop |
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129 | else |
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130 | close(90) |
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131 | endif |
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132 | |
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133 | ! now, run.def is needed anyway. so we create a dummy temporary one |
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134 | ! for ioipsl to work. if a run.def is already here, stop the |
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135 | ! program and ask the user to do a bit of cleaning |
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136 | open(90,file='run.def',status='old',form='formatted',& |
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137 | iostat=ierr) |
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138 | if (ierr.eq.0) then |
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139 | close(90) |
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140 | write(*,*) 'There is already a run.def file.' |
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141 | write(*,*) 'This is not compatible with 1D runs.' |
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142 | write(*,*) 'Please remove the file and restart the run.' |
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143 | write(*,*) 'Runtime parameters are supposed to be in kcm1d.def' |
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144 | stop |
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145 | else |
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146 | call system('touch run.def') |
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147 | call system("echo 'INCLUDEDEF=callphys.def' >> run.def") |
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148 | call system("echo 'INCLUDEDEF=kcm1d.def' >> run.def") |
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149 | endif |
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150 | |
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151 | ! check if we are going to run with or without tracers |
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152 | write(*,*) "Run with or without tracer transport ?" |
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153 | tracer=.false. ! default value |
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154 | call getin("tracer",tracer) |
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155 | write(*,*) " tracer = ",tracer |
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156 | |
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157 | |
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158 | |
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159 | ! Tracer initialisation |
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160 | ! --------------------- |
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161 | if (tracer) then |
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162 | ! load tracer names from file 'traceur.def' |
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163 | open(90,file='traceur.def',status='old',form='formatted',& |
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164 | iostat=ierr) |
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165 | if (ierr.eq.0) then |
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166 | write(*,*) "kcm1d: Reading file traceur.def" |
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167 | ! read number of tracers: |
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168 | !! - Modif. by JVO and YJ for modern planetary traceur.def --------------- |
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169 | READ(90,'(A)') line |
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170 | IF (trim(line).ne.'#ModernTrac-v1') THEN ! Test modern traceur.def |
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171 | READ(line,*,iostat=ierr) nq ! Try standard traceur.def |
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172 | ELSE |
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173 | moderntracdef = .true. |
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174 | DO |
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175 | READ(90,'(A)',iostat=ierr) line |
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176 | IF (ierr.eq.0) THEN |
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177 | IF (index(line,'#').ne.1) THEN ! Allows arbitary number of comments lines in the header |
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178 | READ(line,*,iostat=ierr) nq |
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179 | EXIT |
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180 | ENDIF |
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181 | ELSE ! If pb, or if reached EOF without having found nbtr |
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182 | write(*,*) "rcm1d: error reading number of tracers" |
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183 | write(*,*) " (first line of traceur.def) " |
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184 | stop |
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185 | ENDIF |
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186 | ENDDO |
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187 | ENDIF ! if modern or standard traceur.def |
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188 | if (ierr.ne.0) then |
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189 | write(*,*) "kcm1d: error reading number of tracers" |
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190 | write(*,*) " (first line of traceur.def) " |
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191 | stop |
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192 | endif |
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193 | nqtot=nq |
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194 | ! allocate arrays which depend on number of tracers |
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195 | allocate(nametrac(nq)) |
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196 | allocate(q(nlayer,nq)) |
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197 | allocate(vmr(nlayer,nq)) |
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198 | allocate(qsurf(nq)) |
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199 | |
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200 | do iq=1,nq |
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201 | ! minimal version, just read in the tracer names, 1 per line |
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202 | read(90,*,iostat=ierr) nametrac(iq) |
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203 | write(*,*) 'tracer here is', nametrac(iq) |
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204 | if (ierr.ne.0) then |
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205 | write(*,*) 'kcm1d: error reading tracer names...' |
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206 | stop |
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207 | endif |
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208 | enddo !of do iq=1,nq |
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209 | close(90) |
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210 | endif |
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211 | |
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212 | call initracer(1,nq,nametrac) |
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213 | |
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214 | endif |
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215 | |
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216 | |
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217 | |
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218 | |
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219 | |
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220 | psurf_n=100000. ! default value for psurf |
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221 | print*,'Dry surface pressure (Pa)?' |
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222 | call getin("psurf",psurf_n) |
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223 | write(*,*) " psurf = ",psurf_n |
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224 | |
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225 | ! OK. now that run.def has been read once -- any variable is in memory. |
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226 | ! so we can dump the dummy run.def |
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227 | call system("rm -rf run.def") |
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228 | |
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229 | tsurf=300.0 ! default value for tsurf |
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230 | print*,'Surface temperature (K)?' |
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231 | call getin("tref",tsurf) |
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232 | write(*,*) " tsurf = ",tsurf |
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233 | |
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234 | g=10.0 ! default value for g |
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235 | print*,'Gravity ?' |
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236 | call getin("g",g) |
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237 | write(*,*) " g = ",g |
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238 | glat(1)=g |
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239 | |
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240 | periastr = 1.0 |
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241 | apoastr = 1.0 |
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242 | print*,'Periastron (AU)?' |
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243 | call getin("periastr",periastr) |
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244 | write(*,*) "periastron = ",periastr |
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245 | dist_star = periastr |
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246 | fract = 0.5 |
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247 | print*,'Apoastron (AU)?' |
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248 | call getin("apoastr",apoastr) |
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249 | write(*,*) "apoastron = ",apoastr |
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250 | |
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251 | albedo=0.2 ! default value for albedo |
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252 | print*,'Albedo of bare ground?' |
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253 | call getin("albedo",albedo) |
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254 | write(*,*) " albedo = ",albedo |
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255 | do iw=1,L_NSPECTV |
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256 | albedo_wv(1,iw)=albedo |
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257 | enddo |
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258 | |
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259 | emis=1.0 ! default value for emissivity |
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260 | PRINT *,'Emissivity of bare ground ?' |
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261 | call getin("emis",emis) |
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262 | write(*,*) " emis = ",emis |
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263 | |
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264 | pceil=100.0 ! Pascals |
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265 | PRINT *,'Ceiling pressure (Pa) ?' |
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266 | call getin("pceil",pceil) |
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267 | write(*,*) " pceil = ", pceil |
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268 | |
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269 | check_cpp_match = .false. |
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270 | call getin("check_cpp_match",check_cpp_match) |
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271 | if (check_cpp_match) then |
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272 | print*,"In 1D modeling, check_cpp_match is supposed to be F" |
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273 | print*,"Please correct callphys.def" |
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274 | stop |
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275 | endif |
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276 | |
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277 | |
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278 | !!! GEOGRAPHICAL INITIALIZATIONS |
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279 | !!! AREA. useless in 1D |
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280 | cell_area(1)=1.E+0 !JL+EM to have access to the area in the diagfi.nc files. |
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281 | !!! GEOPOTENTIAL. useless in 1D because control by surface pressure |
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282 | phisfi(1)=0.E+0 |
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283 | !!! LATITUDE. can be set. |
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284 | latitude=0 ! default value for latitude |
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285 | PRINT *,'latitude (in degrees) ?' |
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286 | call getin("latitude",latitude) |
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287 | write(*,*) " latitude = ",latitude |
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288 | latitude=latitude*pi/180.E+0 |
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289 | !!! LONGITUDE. useless in 1D. |
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290 | longitude=0.E+0 |
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291 | longitude=longitude*pi/180.E+0 |
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292 | |
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293 | rad=6400000. |
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294 | !rad = -99999. |
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295 | !PRINT *,'PLANETARY RADIUS in m ?' |
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296 | !call getin("rad",rad) |
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297 | ! Planetary radius is needed to compute shadow of the rings |
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298 | !IF (rad.eq.-99999. .and. rings_shadow .eqv. .true.) THEN |
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299 | ! PRINT *,"STOP. I NEED rad IN RCM1D.DEF." |
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300 | ! STOP |
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301 | !ELSE |
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302 | ! PRINT *,"--> rad = ",rad |
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303 | !ENDIF |
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304 | |
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305 | |
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306 | |
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307 | call init_physics_distribution(regular_lonlat,4,1,1,1,nlayer,1) |
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308 | call init_interface_dyn_phys |
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309 | CALL init_regular_lonlat(1,1,longitude,latitude,(/0.,0./),(/0.,0./)) |
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310 | call init_geometry(1,longitude,latitude,(/0.,0.,0.,0./),(/0.,0.,0.,0./),cell_area) |
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311 | call init_dimphy(1,nlayer) ! Initialize dimphy module |
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312 | |
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313 | !!! CALL INIFIS |
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314 | !!! - read callphys.def |
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315 | !!! - calculate sine and cosine of longitude and latitude |
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316 | !!! - calculate mugaz and cp |
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317 | !!! NB: some operations are being done dummily in inifis in 1D |
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318 | !!! - physical constants: nevermind, things are done allright below |
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319 | !!! - physical frequency: nevermind, in inifis this is a simple print |
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320 | |
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321 | cpp=1.d-7 !JL because we divide by cpp in inifis, there may be a more elegant solution |
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322 | CALL inifis(1,llm,nq,0,86400.0,1,1.0,latitude,longitude,cell_area,rad,g,r,cpp) |
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323 | |
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324 | if(.not.global1d)then |
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325 | print*,'Error, kcm1d must have global1d=.true. in kcm1d.def!' |
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326 | stop |
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327 | end if |
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328 | |
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329 | !write(*,*) 'BASE 1' |
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330 | !write(*,*) 1,llm,nq,0,86400.0,1,1.0,latitude,longitude,cell_area,rad,g,r,cpp |
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331 | |
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332 | do iq=1,nq |
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333 | do ilay=1,nlayer |
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334 | q(ilay,iq) = 0. |
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335 | enddo |
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336 | enddo |
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337 | |
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338 | do iq=1,nq |
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339 | qsurf(iq) = 0. |
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340 | enddo |
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341 | |
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342 | firstcall = .true. |
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343 | lastcall = .false. |
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344 | |
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345 | iter = 1 |
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346 | Tstrat = 150.0 |
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347 | dTstrat = 1000.0 |
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348 | |
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349 | ! --------- |
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350 | ! Run model |
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351 | ! --------- |
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352 | !do |
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353 | psurf = psurf_n |
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354 | |
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355 | ! Create vertical profiles |
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356 | call kcmprof_fn(nlayer,psurf,qsurf(1),tsurf, & |
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357 | tstrat,play,plev,zlay,temp,q(:,1),muvar(1)) |
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358 | |
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359 | |
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360 | !write(*,*) 'BASE 2' |
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361 | !write(*,*) nlayer,psurf,qsurf(1),tsurf, & |
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362 | ! tstrat |
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363 | !write(*,*) play |
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364 | !write(*,*) plev |
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365 | !write(*,*) zlay |
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366 | !write(*,*) temp |
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367 | !write(*,*) q(:,1),muvar(1) |
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368 | |
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369 | |
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370 | |
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371 | call iniaerosol() |
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372 | |
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373 | |
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374 | |
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375 | |
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376 | ! Run radiative transfer |
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377 | call callcorrk(1,nlayer,q,nq,qsurf, & |
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378 | albedo_wv,albedo_equivalent, & |
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379 | emis,mu0,plev,play,temp, & |
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380 | tsurf,fract,dist_star,aerosol,muvar, & |
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381 | dtlw,dtsw,fluxsurf_lw,fluxsurf_sw, & |
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382 | fluxsurfabs_sw,fluxtop_lw, & |
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383 | fluxabs_sw,fluxtop_dn,OLR_nu,OSR_nu,tau_col, & |
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384 | cloudfrac,totcloudfrac,.false.,firstcall,lastcall) |
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385 | |
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386 | !write(*,*) 'BASE 3' |
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387 | !write(*,*) 1,nlayer,'A',q,'B',nq,'C',qsurf, & |
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388 | ! albedo_wv,'D',albedo_equivalent,'E', & |
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389 | ! emis,'F',mu0,'G',plev,'H',play,'I',temp,'J', & |
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390 | ! tsurf,'K',fract,'L',dist_star,'M',aerosol,'N',muvar,'O', & |
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391 | ! dtlw,'P',dtsw,'Q',fluxsurf_lw,'R',fluxsurf_sw,'S', & |
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392 | ! fluxsurfabs_sw,'T',fluxtop_lw,'U', & |
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393 | ! fluxabs_sw,'V',fluxtop_dn,'W',OLR_nu,'X',OSR_nu,'Y',tau_col,'Z', & |
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394 | ! cloudfrac,'A1',totcloudfrac,'A2',.false.,'A3',firstcall,'A4',lastcall |
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395 | |
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396 | |
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397 | |
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398 | |
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399 | |
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400 | |
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401 | |
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402 | ! Iterate stratospheric temperature |
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403 | print*,'Tstrat = ',Tstrat |
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404 | dTstrat = Tstrat |
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405 | !Tstrat = Tsurf*(0.2786*(psurf/100000.)**(-1.123))**0.25 |
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406 | ! skin temperature (gray approx.) using analytic pure H2 expression |
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407 | !Tstrat = (fluxabs_sw/(2*sigma))**0.25 ! skin temperature (gray approx.) |
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408 | Tstrat = (fluxtop_lw/(2*sigma))**0.25 ! skin temperature (gray approx.) |
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409 | dTstrat = dTstrat-Tstrat |
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410 | |
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411 | !if(abs(dTstrat).lt.1.0)then |
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412 | ! print*,'dTstrat = ',dTstrat |
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413 | ! exit |
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414 | !endif |
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415 | |
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416 | !iter=iter+1 |
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417 | !if(iter.eq.100)then |
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418 | ! print*,'Stratosphere failed to converge after' |
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419 | ! print*,'100 iteration, aborting run.' |
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420 | ! call abort |
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421 | !endif |
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422 | |
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423 | !end do |
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424 | |
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425 | |
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426 | ! Run radiative transfer one last time to get OLR,OSR |
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427 | firstcall=.false. |
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428 | lastcall=.true. |
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429 | call callcorrk(1,nlayer,q,nq,qsurf, & |
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430 | albedo_wv,albedo_equivalent,emis,mu0,plev,play,temp, & |
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431 | tsurf,fract,dist_star,aerosol,muvar, & |
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432 | dtlw,dtsw,fluxsurf_lw,fluxsurf_sw,fluxsurfabs_sw, & |
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433 | fluxtop_lw, fluxabs_sw,fluxtop_dn,OLR_nu,OSR_nu, & |
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434 | tau_col, & |
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435 | cloudfrac,totcloudfrac,.false.,firstcall,lastcall) |
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436 | |
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437 | |
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438 | !write(*,*) 'BASE 4' |
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439 | !write(*,*) 1,nlayer,'A',q,'B',nq,'C',qsurf, & |
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440 | ! albedo_wv,'D',albedo_equivalent,'E', & |
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441 | ! emis,'F',mu0,'G',plev,'H',play,'I',temp,'J', & |
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442 | ! tsurf,'K',fract,'L',dist_star,'M',aerosol,'N',muvar,'O', & |
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443 | ! dtlw,'P',dtsw,'Q',fluxsurf_lw,'R',fluxsurf_sw,'S', & |
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444 | ! fluxsurfabs_sw,'T',fluxtop_lw,'U', & |
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445 | ! fluxabs_sw,'V',fluxtop_dn,'W',OLR_nu,'X',OSR_nu,'Y',tau_col,'Z', & |
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446 | ! cloudfrac,'A1',totcloudfrac,'A2',.false.,'A3',firstcall,'A4',lastcall |
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447 | |
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448 | |
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449 | |
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450 | |
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451 | |
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452 | |
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453 | |
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454 | ! Calculate total atmospheric energy |
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455 | Eatmtot=0.0 |
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456 | ! call calcenergy_kcm(nlayer,tsurf,temp,play,plev,qsurf,& |
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457 | ! q(:,1),muvar,Eatmtot) |
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458 | |
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459 | ! ------------------------ |
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460 | ! Save data to ascii files |
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461 | ! ------------------------ |
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462 | |
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463 | print*,'Saving profiles...' |
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464 | open(115,file='profpres.out',form='formatted') |
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465 | open(116,file='proftemp.out',form='formatted') |
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466 | open(117,file='profztab.out',form='formatted') |
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467 | open(118,file='profqvar.out',form='formatted') |
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468 | open(119,file='profvvar.out',form='formatted') |
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469 | |
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470 | write(115,*) psurf |
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471 | write(116,*) tsurf |
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472 | write(117,*) 0.0 |
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473 | write(118,*) qsurf(1) |
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474 | write(119,*) qsurf(1)*(muvar(1)/mH2O) |
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475 | do ilay=1,nlayer |
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476 | vmr(ilay,1) = q(ilay,1)*(muvar(ilay+1)/mH2O) |
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477 | write(115,*) play(ilay) |
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478 | write(116,*) temp(ilay) |
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479 | write(117,*) zlay(ilay) |
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480 | write(118,*) q(ilay,1) |
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481 | write(119,*) vmr(ilay,1) |
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482 | enddo |
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483 | close(115) |
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484 | close(116) |
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485 | close(117) |
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486 | close(118) |
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487 | close(119) |
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488 | |
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489 | print*, tsurf,psurf,fluxtop_dn,fluxabs_sw,fluxtop_lw |
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490 | |
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491 | print*,'Saving scalars...' |
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492 | open(116,file='surf_vals.out') |
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493 | write(116,*) tsurf,psurf,fluxtop_dn, & |
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494 | fluxabs_sw,fluxtop_lw |
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495 | close(116) |
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496 | open(111,file='ene_vals.out') |
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497 | write(111,*) tsurf,psurf,Eatmtot,Tstrat |
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498 | close(111) |
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499 | |
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500 | print*,'Saving spectra...' |
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501 | open(117,file='OLRnu.out') |
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502 | do iw=1,L_NSPECTI |
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503 | write(117,*) OLR_nu(1,iw) |
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504 | enddo |
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505 | close(117) |
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506 | |
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507 | open(127,file='OSRnu.out') |
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508 | do iw=1,L_NSPECTV |
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509 | write(127,*) OSR_nu(1,iw) |
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510 | enddo |
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511 | close(127) |
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512 | |
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513 | end program kcm1d |
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