1 | #!/bin/bash |
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2 | |
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3 | function print() |
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4 | { |
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5 | # prints one comment line followed by any number of "key = value" lines |
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6 | echo "# $1 : $2 (default=$3)" |
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7 | shift; shift; shift; |
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8 | while (($# > 0)) ; do |
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9 | echo "$1 = $2" |
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10 | shift; shift; |
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11 | done |
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12 | echo |
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13 | } |
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14 | |
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15 | ################################### Planet ####################################### |
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16 | |
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17 | function radius { print 'Planetary radius' real 6371220 radius $1 |
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18 | } |
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19 | function g { print Gravity real 9.80616 g $1 |
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20 | } |
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21 | function omega { print 'Planetary rotation rate' real 7.292E-5 omega $1 |
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22 | } |
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23 | function kappa { print 'kappa=Rd/cpp' real 0.2857143 kappa $1 |
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24 | } |
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25 | function cpp { print 'Heat capacity at constant pressure' real 1004.70885 cpp $1 |
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26 | } |
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27 | function preff { print 'Reference pressure' real 101325 preff $1 |
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28 | } |
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29 | function scale_factor { print 'Scale factor for small planet experiment' real 1. scale_factor $1 |
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30 | } |
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31 | |
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32 | ##################################### Mesh ##################################### |
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33 | |
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34 | function nbp { print 'Number of subdivisions on a main triangle' integer 40 nbp $1 |
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35 | } |
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36 | function split { print 'Sub splitting of main rhombus' integer 1 nsplit_i $1 nsplit_j $2 |
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37 | } |
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38 | function llm { print 'Number of vertical layers' integer 19 llm $1 |
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39 | } |
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40 | function disvert { print 'Vertical grid' '[std|ncar|ncarl30]' std disvert $1 |
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41 | } |
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42 | function ncar_dz { print 'Model layer thickness in m, used if disvert=ncar' real 300 ncar_dz $1 |
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43 | } |
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44 | function optim_it { print 'Mesh optimisation : number of iterations' integer 0 optim_it $1 |
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45 | } |
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46 | |
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47 | ################################# Numerics ################################### |
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48 | |
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49 | function scheme { print 'Time-stepping scheme' '[euler|leapfrog_matsuno|runge_kutta]' runge_kutta scheme $1 |
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50 | } |
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51 | function time_step { print 'Time step in s' real 480 dt $1 |
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52 | } |
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53 | function matsuno { print 'Matsuno period' integer 5 matsuno_period $1 |
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54 | } |
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55 | function itau_adv { print 'Advection called every itau_adv time steps' integer 2 itau_adv $1 |
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56 | } |
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57 | function nqtot { print 'Number of tracers' integer 1 nqtot $1 |
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58 | } |
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59 | function caldyn { print 'Equations solved' '[gcm|adv]' gcm caldyn $1 |
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60 | } |
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61 | function caldyn_conserv { print 'Discretization of Coriolis term' '[energy|enstophy]' energy caldyn_conserv $1 |
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62 | } |
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63 | function caldyn_eta { print 'Vertical coordinate' '[eta_mass|eta_lag]' mass caldyn_eta $1 |
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64 | } |
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65 | function boussinesq { print 'Boussinesq approximation, requires eta_lag' '[.FALSE.|.TRUE.]' .FALSE. boussinesq $1 |
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66 | } |
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67 | ############################### Time and output ############################### |
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68 | |
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69 | function time_style() { print 'Time style' '[none|dcmip]' dcmip time_style $1 |
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70 | } |
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71 | function run_length() { print 'Run length in s' real ?? run_length $1 |
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72 | } |
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73 | function write_period { print 'Interval in s between two outputs' integer ?? write_period $1 |
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74 | } |
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75 | function out_pressure_level { print 'Pressure level to which interpolate T' real 0 out_pression_level $1 |
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76 | } |
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77 | |
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78 | ################################ Physics ###################################### |
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79 | |
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80 | function etat0 { |
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81 | OPTS=$(printf '\n# [jablonowsky06|academic|dcmip[1-4]|heldsz|dcmip2_schaer_noshear]') |
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82 | print 'Initial state' "$OPTS" jablonowsky06 etat0 $1 |
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83 | } |
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84 | function dissip |
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85 | { |
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86 | print 'Dissipation time for grad(div)' real 5000 tau_graddiv $1 |
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87 | print 'Exponent of grad(div) disspation' integer 1 nitergdiv $2 |
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88 | print 'Dissipation time for curl(curl)' real 5000 tau_gradrot $3 |
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89 | print 'Exponent of curl(curl) disspation' integer 1 nitergrot $4 |
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90 | print 'Dissipation time for div(grad)' real 5000 tau_divgrad $5 |
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91 | print 'Exponent of div(grad) disspation' integer 1 niterdivgrad $6 |
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92 | } |
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93 | # Standard dissipation values for a few nbp |
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94 | function dissip32() { dissip 21600 2 50000 2 50000 2 |
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95 | } |
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96 | function dissip40() { dissip 18000 2 18000 2 18000 2 |
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97 | } |
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98 | function dissip64() { dissip 10800 2 10800 2 10800 2 |
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99 | } |
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100 | function dissip80() { dissip 9000 2 9000 2 9000 2 |
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101 | } |
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102 | |
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103 | |
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104 | function guided_type { print 'Type of guiding terms' '[none|dcmip1]' none guided_type $1 |
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105 | } |
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106 | |
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107 | function rayleigh_friction_type { print 'Type of Rayleigh friction' '[none|dcmip21]' none rayleigh_friction_type $1 |
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108 | } |
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109 | |
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110 | function rayleigh_friction_tau { print 'Relaxation time for Rayleigh friction' '0' none rayleigh_friction_tau $1 |
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111 | } |
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112 | |
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113 | function guided_type { print 'Type of guiding terms' '[none|dcmip1]' none guided_type $1 |
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114 | } |
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115 | |
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116 | function physics { print 'Physics package' '[none|held_suarez|dcmip]' none physics $1 |
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117 | } |
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118 | |
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119 | function itau_physics { print 'Call physics every itau_physics time steps' 'integer' 1 itau_physics $1 |
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120 | } |
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121 | |
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122 | #################################### DCMIP ################################# |
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123 | |
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124 | function dcmip1_def() |
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125 | { |
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126 | etat0 dcmip1 |
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127 | OPTS=$(printf '\n# [const|slotted_cyl|cos_bell|dbl_cos_bell_q1|dbl_cos_bell_q2|complement|hadley|dcmip11]') |
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128 | print 'DCMIP 1.1 advection test, initial tracer field' "$OPTS" cos_bell dcmip1_shape $1 |
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129 | print 'DCMIP 1.1 advection test, wind field' '[solid|deform|hadley]' deform dcmip1_wind $2 |
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130 | } |
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131 | function dcmip_refs() |
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132 | { |
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133 | print 'Reference temperature T0 for DCMIP test cases' real 300 ncar_T0 $1 |
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134 | print 'Reference pressure p0 for DCMIP test cases, used by disvert if disver=ncar' real 1e5 ncar_p0 $2 |
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135 | print 'Exponent for B(eta), used by disvert if disvert=ncar' integer 1 ncar_disvert_c $3 |
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136 | } |
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137 | function dcmip_physics() |
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138 | { |
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139 | physics dcmip |
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140 | print 'DCMIP physics' '[0|1]' 1 dcmip_physics $1 |
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141 | } |
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142 | function dcmip4_testcase { print 'DCMIP 4 Test case' '[1|2]' 1 dcmip4_testcase $1 |
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143 | } |
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144 | |
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145 | ####################### Functions generating parameter files #################### |
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146 | |
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147 | function params { |
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148 | # executes any number of "command arg" commands |
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149 | while (($# > 0)) ; do |
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150 | $1 $2 |
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151 | shift; shift; |
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152 | done |
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153 | } |
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154 | |
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155 | function group { |
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156 | # prints one separation line then executes any number of "command arg" commands |
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157 | echo |
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158 | echo "#---------------- $1 ----------------" |
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159 | echo |
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160 | shift |
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161 | params $* |
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162 | } |
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163 | |
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164 | function williamson91() |
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165 | { |
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166 | group 'Mesh' nbp 40 llm 1 optim_it 100 ; split 2 2 |
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167 | group 'Numerics' time_step 480 caldyn_conserv enstrophy |
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168 | group 'Time and output' out_pressure_level 85000 write_period 21600 run_length 864000 |
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169 | group 'Physical parameters' radius 6.37122e6 g 9.80616 caldyn_eta eta_lag boussinesq .TRUE. etat0 williamson91.6 |
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170 | dissip 5000 2 5000 2 5000 2 |
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171 | } |
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172 | |
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173 | function held_suarez() |
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174 | { |
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175 | group 'Mesh' nbp 40 llm 19 disvert std optim_it 1000 ; split 2 2 |
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176 | group 'Numerics' itau_adv 1 time_step 480 nqtot 0 |
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177 | group 'Time and output' time_style none run_length 103680000 write_period 86400 |
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178 | group 'Planet' radius 6.371e6 g 9.8 omega 7.292e-5 kappa 0.2857143 cpp 1004 preff 1e5 |
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179 | group 'Physical parameters' etat0 held_suarez physics held_suarez |
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180 | dissip40 |
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181 | } |
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182 | |
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183 | function const_dcmip |
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184 | { |
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185 | group 'Planet' radius 6.37122e6 g 9.80616 kappa 0.2857143 cpp 1004.5 preff 1e5 omega $1 |
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186 | group 'Constants' ; dcmip_refs 300 1e5 1 |
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187 | } |
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188 | |
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189 | function dcmip11 |
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190 | { |
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191 | const_dcmip 0 |
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192 | group 'Mesh' nbp 80 llm 60 disvert ncar ncar_dz 200 optim_it 100 ; split 2 2 |
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193 | group 'Numerics' caldyn adv time_step 180 |
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194 | group 'Time' run_length 1036800 write_period 86400 |
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195 | group 'Physical parameters' nqtot 5 guided_type dcmip1 ; dcmip1_def dcmip11 deform |
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196 | } |
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197 | |
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198 | function dcmip20 |
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199 | { |
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200 | const_dcmip 0 # non-rotating |
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201 | group 'Mesh' nbp 64 llm 15 disvert ncar ncar_dz 800 optim_it 100 ; split 2 2 |
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202 | group 'Numerics' time_step 300 |
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203 | dissip64 |
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204 | group 'Time' run_length 518400 write_period 21600 |
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205 | group 'Physical parameters' scale_factor 1 etat0 dcmip2_mountain |
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206 | } |
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207 | |
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208 | function dcmip21 |
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209 | { |
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210 | # small planet : we define the unscaled time as T and the scaled time is T/X |
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211 | # time.f90 divides times and lengths scales by scale factor X |
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212 | # the DCMIP document uses the words "scaled" and "unscaled" ambiguously |
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213 | # at p.3 the "rescaled radius" is a/X |
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214 | # in the description of experiment 2.1 (p. 32) "T in unscaled time units" means T/X |
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215 | # and "T in scaled times units" means T |
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216 | # I understand the document as tau_rayleigh/X=25s |
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217 | const_dcmip 0 # non-rotating |
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218 | group 'Mesh' nbp 64 llm 60 disvert ncar ncar_dz 500 optim_it 100 ; split 2 2 |
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219 | group 'Numerics' time_step 300 |
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220 | dissip64 |
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221 | group 'Time' run_length 3.6e6 write_period 50000 |
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222 | group 'Physical parameters' scale_factor 500 etat0 dcmip2_schaer_noshear rayleigh_friction_tau 12500 rayleigh_friction_type dcmip2_schaer_noshear |
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223 | } |
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224 | |
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225 | function dcmip3 |
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226 | { |
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227 | const_dcmip 0 # non-rotating |
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228 | group 'Mesh' nbp 80 llm 10 disvert ncar ncar_dz 1000 optim_it 100 ; split 2 2 |
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229 | group 'Numerics' time_step 240 |
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230 | dissip80 |
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231 | group 'Time' run_length 4.5e5 write_period 12500 |
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232 | group 'Physical parameters' scale_factor 125 etat0 dcmip3 |
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233 | } |
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234 | |
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235 | # Next DCMIP test cases have rotation |
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236 | |
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237 | function dcmip4x |
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238 | { |
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239 | echo 'INCLUDEDEF = const.def' |
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240 | group 'Mesh' nbp 80 llm 30 disvert ncarl30 optim_it 100 ; split 2 2 |
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241 | group 'Numerics' time_step 240 |
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242 | dissip80 |
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243 | group 'Time' run_length 3.6e6 write_period 21600 |
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244 | group 'Physical parameters' nqtot 2 etat0 dcmip4 dcmip4_testcase $1 |
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245 | } |
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246 | |
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247 | function dcmip42 |
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248 | { |
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249 | dcmip4x 2 |
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250 | dcmip_physics 1 |
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251 | } |
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252 | |
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253 | function dcmip51 |
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254 | { |
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255 | echo 'INCLUDEDEF = const.def' |
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256 | group 'Mesh' nbp 64 llm 30 disvert ncarl30 optim_it 1000 ; split 2 2 |
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257 | group 'Numerics' time_step 300 |
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258 | dissip64 |
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259 | group 'Time' run_length 864000 write_period 7200 |
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260 | group 'Physical parameters' nqtot 1 etat0 dcmip5 dcmip_physics 0 itau_physics 6 |
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261 | } |
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262 | |
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263 | ########## Main program : generate all *.def files in param_sets ############## |
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264 | |
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265 | function mkcd { cd $ROOT ; mkdir -p $1 ; cd $1 |
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266 | } |
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267 | |
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268 | set -o errexit |
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269 | ROOT=$PWD |
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270 | |
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271 | mkcd climate/Held_Suarez |
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272 | held_suarez > run.def |
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273 | |
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274 | mkcd shallow_water/williamson91 |
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275 | williamson91 > run6.def |
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276 | |
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277 | mkcd dcmip2012 |
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278 | const_dcmip 7.292e-5 > const.def |
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279 | dcmip11 > run11.def |
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280 | dcmip20 > run20.def |
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281 | dcmip21 > run21.def |
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282 | dcmip3 > run3.def |
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283 | dcmip4x 1 > run41.def |
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284 | dcmip42 > run42.def |
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285 | dcmip51 > run51.def |
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