1 | |
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2 | ! $Header$ |
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3 | |
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4 | SUBROUTINE suphel |
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5 | |
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6 | IMPLICIT NONE |
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7 | |
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8 | include "YOMCST.h" |
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9 | include "YOETHF.h" |
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10 | ! IM cf. JLD |
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11 | LOGICAL firstcall |
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12 | SAVE firstcall |
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13 | !$OMP THREADPRIVATE(firstcall) |
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14 | DATA firstcall/.TRUE./ |
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15 | |
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16 | IF (firstcall) THEN |
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17 | PRINT *, 'suphel initialise les constantes du GCM' |
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18 | firstcall = .FALSE. |
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19 | ELSE |
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20 | PRINT *, 'suphel DEJA APPELE ' |
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21 | RETURN |
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22 | END IF |
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23 | ! ----------------------------------------------------------------- |
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24 | |
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25 | ! * 1. DEFINE FUNDAMENTAL CONSTANTS. |
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26 | ! ----------------------------- |
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27 | |
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28 | WRITE (UNIT=6, FMT='(''0*** Constants of the ICM ***'')') |
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29 | rpi = 2.*asin(1.) |
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30 | rclum = 299792458. |
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31 | rhpla = 6.6260755E-34 |
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32 | rkbol = 1.380658E-23 |
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33 | rnavo = 6.0221367E+23 |
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34 | WRITE (UNIT=6, FMT='('' *** Fundamental constants ***'')') |
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35 | WRITE (UNIT=6, FMT='('' PI = '',E13.7,'' -'')') rpi |
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36 | WRITE (UNIT=6, FMT='('' c = '',E13.7,''m s-1'')') rclum |
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37 | WRITE (UNIT=6, FMT='('' h = '',E13.7,''J s'')') rhpla |
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38 | WRITE (UNIT=6, FMT='('' K = '',E13.7,''J K-1'')') rkbol |
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39 | WRITE (UNIT=6, FMT='('' N = '',E13.7,''mol-1'')') rnavo |
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40 | |
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41 | ! ---------------------------------------------------------------- |
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42 | |
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43 | ! * 2. DEFINE ASTRONOMICAL CONSTANTS. |
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44 | ! ------------------------------ |
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45 | |
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46 | rday = 86400. |
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47 | rea = 149597870000. |
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48 | repsm = 0.409093 |
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49 | |
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50 | rsiyea = 365.25*rday*2.*rpi/6.283076 |
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51 | rsiday = rday/(1.+rday/rsiyea) |
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52 | romega = 2.*rpi/rsiday |
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53 | |
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54 | ! exp1 R_ecc = 0.05 |
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55 | ! exp1 R_peri = 102.04 |
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56 | ! exp1 R_incl = 22.5 |
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57 | ! exp1 print*, 'Parametres orbitaux modifies' |
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58 | ! ref R_ecc = 0.016724 |
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59 | ! ref R_peri = 102.04 |
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60 | ! ref R_incl = 23.5 |
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61 | |
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62 | ! IM 161002 : pour avoir les ctes AMIP II |
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63 | ! IM 161002 R_ecc = 0.016724 |
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64 | ! IM 161002 R_peri = 102.04 |
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65 | ! IM 161002 R_incl = 23.5 |
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66 | ! IM on mets R_ecc, R_peri, R_incl dans conf_phys.F90 |
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67 | ! R_ecc = 0.016715 |
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68 | ! R_peri = 102.7 |
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69 | ! R_incl = 23.441 |
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70 | |
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71 | WRITE (UNIT=6, FMT='('' *** Astronomical constants ***'')') |
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72 | WRITE (UNIT=6, FMT='('' day = '',E13.7,'' s'')') rday |
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73 | WRITE (UNIT=6, FMT='('' half g. axis = '',E13.7,'' m'')') rea |
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74 | WRITE (UNIT=6, FMT='('' mean anomaly = '',E13.7,'' -'')') repsm |
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75 | WRITE (UNIT=6, FMT='('' sideral year = '',E13.7,'' s'')') rsiyea |
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76 | WRITE (UNIT=6, FMT='('' sideral day = '',E13.7,'' s'')') rsiday |
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77 | WRITE (UNIT=6, FMT='('' omega = '',E13.7,'' s-1'')') romega |
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78 | ! write(unit=6,fmt='('' excentricite = '',e13.7,''-'')')R_ecc |
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79 | ! write(unit=6,fmt='('' equinoxe = '',e13.7,''-'')')R_peri |
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80 | ! write(unit=6,fmt='('' inclinaison = '',e13.7,''-'')')R_incl |
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81 | |
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82 | ! ------------------------------------------------------------------ |
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83 | |
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84 | ! * 3. DEFINE GEOIDE. |
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85 | ! -------------- |
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86 | |
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87 | rg = 9.80665 |
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88 | ra = 6371229. |
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89 | r1sa = sngl(1.D0/dble(ra)) |
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90 | WRITE (UNIT=6, FMT='('' *** Geoide ***'')') |
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91 | WRITE (UNIT=6, FMT='('' Gravity = '',E13.7,'' m s-2'')') rg |
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92 | WRITE (UNIT=6, FMT='('' Earth radius = '',E13.7,'' m'')') ra |
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93 | WRITE (UNIT=6, FMT='('' Inverse E.R. = '',E13.7,'' m'')') r1sa |
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94 | |
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95 | ! ----------------------------------------------------------------- |
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96 | |
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97 | ! * 4. DEFINE RADIATION CONSTANTS. |
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98 | ! --------------------------- |
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99 | |
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100 | ! z.x.li RSIGMA=2. * RPI**5 * RKBOL**4 /(15.* RCLUM**2 * RHPLA**3) |
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101 | rsigma = 2.*rpi**5*(rkbol/rhpla)**3*rkbol/rclum/rclum/15. |
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102 | ! IM init. dans conf_phys.F90 RI0=1365. |
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103 | WRITE (UNIT=6, FMT='('' *** Radiation ***'')') |
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104 | WRITE (UNIT=6, FMT='('' Stefan-Bol. = '',E13.7,'' W m-2 K-4'' & |
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105 | & & |
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106 | & )') rsigma |
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107 | ! IM init. dans conf_phys.F90 WRITE(UNIT=6,FMT='('' Solar const. = |
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108 | ! '',E13.7,'' W m-2'')') |
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109 | ! IM init. dans conf_phys.F90 S RI0 |
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110 | |
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111 | ! ----------------------------------------------------------------- |
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112 | |
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113 | ! * 5. DEFINE THERMODYNAMIC CONSTANTS, GAS PHASE. |
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114 | ! ------------------------------------------ |
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115 | |
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116 | r = rnavo*rkbol |
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117 | rmd = 28.9644 |
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118 | rmo3 = 47.9942 |
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119 | rmco2 = 44.011 |
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120 | rmc = 12.0107 |
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121 | rmv = 18.0153 |
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122 | rd = 1000.*r/rmd |
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123 | rv = 1000.*r/rmv |
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124 | rcpd = 3.5*rd |
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125 | rcvd = rcpd - rd |
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126 | rcpv = 4.*rv |
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127 | rcvv = rcpv - rv |
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128 | rkappa = rd/rcpd |
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129 | retv = rv/rd - 1. |
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130 | WRITE (UNIT=6, FMT='('' *** Thermodynamic, gas ***'')') |
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131 | WRITE (UNIT=6, FMT='('' Perfect gas = '',e13.7)') r |
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132 | WRITE (UNIT=6, FMT='('' Dry air mass = '',e13.7)') rmd |
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133 | WRITE (UNIT=6, FMT='('' Ozone mass = '',e13.7)') rmo3 |
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134 | WRITE (UNIT=6, FMT='('' CO2 mass = '',e13.7)') rmco2 |
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135 | WRITE (UNIT=6, FMT='('' CO2 mass = '',e13.7)') rmc |
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136 | WRITE (UNIT=6, FMT='('' Vapour mass = '',e13.7)') rmv |
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137 | WRITE (UNIT=6, FMT='('' Dry air cst. = '',e13.7)') rd |
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138 | WRITE (UNIT=6, FMT='('' Vapour cst. = '',e13.7)') rv |
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139 | WRITE (UNIT=6, FMT='('' Cpd = '',e13.7)') rcpd |
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140 | WRITE (UNIT=6, FMT='('' Cvd = '',e13.7)') rcvd |
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141 | WRITE (UNIT=6, FMT='('' Cpv = '',e13.7)') rcpv |
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142 | WRITE (UNIT=6, FMT='('' Cvv = '',e13.7)') rcvv |
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143 | WRITE (UNIT=6, FMT='('' Rd/Cpd = '',e13.7)') rkappa |
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144 | WRITE (UNIT=6, FMT='('' Rv/Rd-1 = '',e13.7)') retv |
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145 | |
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146 | ! ---------------------------------------------------------------- |
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147 | |
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148 | ! * 6. DEFINE THERMODYNAMIC CONSTANTS, LIQUID PHASE. |
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149 | ! --------------------------------------------- |
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150 | |
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151 | rcw = rcpv |
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152 | WRITE (UNIT=6, FMT='('' *** Thermodynamic, liquid ***'')') |
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153 | WRITE (UNIT=6, FMT='('' Cw = '',E13.7)') rcw |
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154 | |
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155 | ! ---------------------------------------------------------------- |
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156 | |
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157 | ! * 7. DEFINE THERMODYNAMIC CONSTANTS, SOLID PHASE. |
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158 | ! -------------------------------------------- |
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159 | |
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160 | rcs = rcpv |
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161 | WRITE (UNIT=6, FMT='('' *** thermodynamic, solid ***'')') |
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162 | WRITE (UNIT=6, FMT='('' Cs = '',E13.7)') rcs |
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163 | |
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164 | ! ---------------------------------------------------------------- |
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165 | |
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166 | ! * 8. DEFINE THERMODYNAMIC CONSTANTS, TRANSITION OF PHASE. |
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167 | ! ---------------------------------------------------- |
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168 | |
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169 | rtt = 273.16 |
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170 | rlvtt = 2.5008E+6 |
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171 | rlstt = 2.8345E+6 |
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172 | rlmlt = rlstt - rlvtt |
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173 | ratm = 100000. |
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174 | WRITE (UNIT=6, FMT='('' *** Thermodynamic, trans. ***'')') |
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175 | WRITE (UNIT=6, FMT='('' Fusion point = '',E13.7)') rtt |
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176 | WRITE (UNIT=6, FMT='('' RLvTt = '',E13.7)') rlvtt |
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177 | WRITE (UNIT=6, FMT='('' RLsTt = '',E13.7)') rlstt |
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178 | WRITE (UNIT=6, FMT='('' RLMlt = '',E13.7)') rlmlt |
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179 | WRITE (UNIT=6, FMT='('' Normal press. = '',E13.7)') ratm |
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180 | WRITE (UNIT=6, FMT='('' Latent heat : '')') |
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181 | |
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182 | ! ---------------------------------------------------------------- |
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183 | |
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184 | ! * 9. SATURATED VAPOUR PRESSURE. |
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185 | ! -------------------------- |
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186 | |
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187 | restt = 611.14 |
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188 | rgamw = (rcw-rcpv)/rv |
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189 | rbetw = rlvtt/rv + rgamw*rtt |
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190 | ralpw = log(restt) + rbetw/rtt + rgamw*log(rtt) |
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191 | rgams = (rcs-rcpv)/rv |
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192 | rbets = rlstt/rv + rgams*rtt |
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193 | ralps = log(restt) + rbets/rtt + rgams*log(rtt) |
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194 | rgamd = rgams - rgamw |
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195 | rbetd = rbets - rbetw |
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196 | ralpd = ralps - ralpw |
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197 | |
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198 | ! ------------------------------------------------------------------ |
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199 | |
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200 | ! * 10. CONSTANTS FOR THERMODYNAMICAL FUNCTIONS. |
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201 | ! ---------------------------------------- |
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202 | |
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203 | rvtmp2 = rcpv/rcpd - 1. |
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204 | rhoh2o = ratm/100. |
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205 | r2es = restt*rd/rv |
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206 | r3les = 17.269 |
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207 | r3ies = 21.875 |
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208 | r4les = 35.86 |
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209 | r4ies = 7.66 |
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210 | r5les = r3les*(rtt-r4les) |
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211 | r5ies = r3ies*(rtt-r4ies) |
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212 | |
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213 | ! ------------------------------------------------------------------ |
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214 | |
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215 | ! * 10. CONSTANTS FOR METHANE OXIDATION AND PHOTOLYSIS. |
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216 | ! ----------------------------------------------- |
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217 | |
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218 | CALL SUMETHOX() |
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219 | |
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220 | RETURN |
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221 | END SUBROUTINE suphel |
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