1 | |
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2 | subroutine interpolateH2H2(wn,temp,pres,abcoef,firstcall,ind) |
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3 | |
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4 | !================================================================== |
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5 | ! |
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6 | ! Purpose |
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7 | ! ------- |
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8 | ! Calculates the H2-H2 CIA opacity, using a lookup table from |
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9 | ! HITRAN (2011 or later) |
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10 | ! |
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11 | ! Authors |
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12 | ! ------- |
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13 | ! R. Wordsworth (2011) |
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14 | ! |
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15 | ! + J.Vatant d'Ollone (2019) |
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16 | ! - Enable updated HITRAN file (Karman2019,Fletcher2018) |
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17 | ! (2018 one should be default for giant planets) |
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18 | !================================================================== |
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19 | |
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20 | use callkeys_mod, only: versH2H2cia, strictboundcia, H2orthopara_mixture |
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21 | use datafile_mod, only: datadir |
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22 | use mod_phys_lmdz_para, only : is_master |
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23 | |
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24 | implicit none |
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25 | |
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26 | ! input |
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27 | double precision wn ! wavenumber (cm^-1) |
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28 | double precision temp ! temperature (Kelvin) |
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29 | double precision pres ! pressure (Pascals) |
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30 | |
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31 | ! output |
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32 | double precision abcoef ! absorption coefficient (m^-1) |
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33 | |
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34 | integer nS,nT |
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35 | parameter(nT=10) |
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36 | |
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37 | double precision, parameter :: losch = 2.6867774e19 |
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38 | ! Loschmit's number (molecule cm^-3 at STP) |
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39 | ! converts cm^5 molecule^-2 --> cm^-1 amagat^-2 |
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40 | ! see Richard et al. 2011, JQSRT for details |
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41 | |
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42 | double precision amagat |
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43 | double precision temp_arr(nT) |
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44 | |
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45 | double precision, dimension(:), allocatable :: wn_arr |
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46 | double precision, dimension(:,:), allocatable :: abs_arr |
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47 | |
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48 | integer k,iT |
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49 | logical firstcall |
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50 | |
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51 | save nS, wn_arr, temp_arr, abs_arr !read by master |
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52 | |
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53 | character*100 dt_file |
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54 | integer ios |
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55 | |
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56 | character(LEN=*), parameter :: fmat11 = "(A20,F10.3,F10.3,I7,F7.1,E10.3,F5.3)" |
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57 | character(LEN=*), parameter :: fmat18 = "(A12,A3,A5,F10.6,F10.4,I7,F7.3,E10.3,F5.3)" |
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58 | |
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59 | character*20 bleh |
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60 | double precision blah, Ttemp, ztemp |
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61 | integer nres |
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62 | |
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63 | integer ind |
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64 | |
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65 | ztemp=temp |
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66 | if ((H2orthopara_mixture .eq. "hot")) then |
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67 | if (ztemp .gt. 7000.) then |
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68 | if (strictboundcia) then |
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69 | if (is_master) then |
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70 | print*,'Your temperatures are too high for this H2-H2 CIA dataset (>7000K, Hot Jupiter case)' |
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71 | endif !is_master |
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72 | stop |
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73 | else |
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74 | !if (is_master) then |
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75 | ! print*,'Your temperatures are too high for this H2-H2 CIA dataset (Hot Jupiter case)' |
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76 | ! print*,'you have chosen strictboundcia = ', strictboundcia |
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77 | ! print*,'*********************************************************' |
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78 | ! print*,' we allow model to continue but with temp = 7000 ' |
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79 | ! print*,' ... for H2-H2 CIA dataset ... ' |
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80 | ! print*,' ... we assume we know what you are doing ... ' |
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81 | ! print*,'*********************************************************' |
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82 | !endif !is_master |
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83 | ztemp = 7000. |
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84 | endif !strictboundcia |
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85 | endif !(temp .gt. 7000.) |
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86 | else ! if not "hot" |
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87 | if(ztemp.gt.400)then |
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88 | if (strictboundcia) then |
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89 | if (is_master) then |
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90 | print*,'Your temperatures are too high for this H2-H2 CIA dataset. If you ' |
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91 | print*,'really want to run simulations with hydrogen at T > 400 K, contact' |
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92 | print*,'Robin Wordsworth [rwordsworth@uchicago.edu].' |
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93 | endif !is_master |
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94 | stop |
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95 | else |
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96 | !if (is_master) then |
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97 | ! print*,'Your temperatures are too high for this H2-H2 CIA dataset' |
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98 | ! print*,'you have chosen strictboundcia = ', strictboundcia |
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99 | ! print*,'*********************************************************' |
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100 | ! print*,' we allow model to continue but with temp = 400 ' |
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101 | ! print*,' ... for H2-H2 CIA dataset ... ' |
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102 | ! print*,' ... we assume we know what you are doing ... ' |
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103 | ! print*,'*********************************************************' |
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104 | !endif !is_master |
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105 | ztemp = 400 |
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106 | endif !of strictboundcia |
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107 | elseif(ztemp.lt.40)then |
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108 | if (strictboundcia) then |
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109 | if (is_master) then |
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110 | print*,'Your temperatures are too low for this H2-H2 CIA dataset. If you ' |
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111 | print*,'really want to run simulations with hydrogen at T < 40 K, contact' |
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112 | print*,'Robin Wordsworth [rwordsworth@uchicago.edu].' |
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113 | endif ! is_master |
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114 | stop |
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115 | else |
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116 | !if (is_master) then |
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117 | ! print*,'Your temperatures are too low for this H2-H2 CIA dataset' |
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118 | ! print*,'you have chosen strictboundcia = ', strictboundcia |
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119 | ! print*,'*********************************************************' |
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120 | ! print*,' we allow model to continue but with temp = 40 ' |
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121 | ! print*,' ... for H2-H2 CIA dataset ... ' |
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122 | ! print*,' ... we assume we know what you are doing ... ' |
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123 | ! print*,'*********************************************************' |
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124 | !endif !is_master |
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125 | ztemp = 40 |
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126 | endif !of strictboundcia |
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127 | endif ! of (temp .gt. 400) |
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128 | endif ! of ((H2orthopara_mixture .eq. "hot").and. (temp .gt. 3000.)) |
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129 | amagat = (273.15/temp)*(pres/101325.0) |
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130 | |
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131 | if(firstcall)then ! called by sugas_corrk only |
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132 | if (is_master) print*,'----------------------------------------------------' |
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133 | if (is_master) print*,'Initialising H2-H2 continuum from HITRAN database...' |
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134 | |
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135 | ! 1.1 Open the ASCII files and set nS according to version |
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136 | ! Only two possible versions for now : 2011 or 2018 (sanity check in inifis_mod) |
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137 | if (versH2H2cia.eq.2011) then |
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138 | nS = 2428 |
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139 | if (H2orthopara_mixture.eq."normal") then |
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140 | dt_file=TRIM(datadir)//'/continuum_data/H2-H2_norm_2011.cia' |
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141 | else if (H2orthopara_mixture.eq."equilibrium") then |
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142 | dt_file=TRIM(datadir)//'/continuum_data/H2-H2_eq_2011.cia' |
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143 | else if (H2orthopara_mixture.eq."hot") then |
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144 | dt_file=TRIM(datadir)//'/continuum_data/H2-H2_2011_extended.cia' |
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145 | ns = 800 |
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146 | endif |
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147 | else if (versH2H2cia.eq.2018) then |
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148 | nS = 9600 |
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149 | if (H2orthopara_mixture.eq."normal") then |
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150 | dt_file=TRIM(datadir)//'/continuum_data/H2-H2_norm_2018.cia' |
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151 | else if (H2orthopara_mixture.eq."equilibrium") then |
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152 | dt_file=TRIM(datadir)//'/continuum_data/H2-H2_eq_2018.cia' |
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153 | endif |
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154 | endif |
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155 | |
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156 | if(.not.allocated(wn_arr)) allocate(wn_arr(nS)) |
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157 | if(.not.allocated(abs_arr)) allocate(abs_arr(nS,nT)) |
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158 | |
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159 | !$OMP MASTER |
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160 | open(33,file=dt_file,form='formatted',status='old',iostat=ios) |
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161 | if (ios.ne.0) then ! file not found |
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162 | if (is_master) then |
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163 | write(*,*) 'Error from interpolateH2H2' |
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164 | write(*,*) 'Data file ',trim(dt_file),' not found.' |
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165 | write(*,*) 'Check that your path to datagcm:',trim(datadir) |
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166 | write(*,*) 'is correct. You can change it in callphys.def with:' |
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167 | write(*,*) 'datadir = /absolute/path/to/datagcm' |
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168 | write(*,*) 'Also check that the continuum data is there.' |
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169 | endif |
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170 | call abort |
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171 | else |
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172 | |
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173 | if(versH2H2cia.eq.2011) then |
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174 | if (is_master) then |
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175 | write(*,*) '... You are using H2-H2 CIA from 2011 but you should use more recent data available on HITRAN !' |
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176 | write(*,*) '... (Especially if you are running a giant planet atmosphere)' |
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177 | write(*,*) '... Just find out the H2-H2 CIA from 2018, put it in your datadir and have a look at interpolateH2H2.F90 ! .' |
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178 | endif |
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179 | endif |
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180 | |
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181 | do iT=1,nT |
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182 | |
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183 | ! Only two possibles values for now : 2011 or 2018 (sanity check in inifis_mod) |
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184 | if(versH2H2cia.eq.2011) then |
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185 | read(33,fmat11) bleh,blah,blah,nres,Ttemp |
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186 | else if (versH2H2cia.eq.2018) then |
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187 | read(33,fmat18) bleh,bleh,bleh,blah,blah,nres,Ttemp |
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188 | endif |
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189 | |
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190 | if(nS.ne.nres)then |
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191 | if (is_master) then |
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192 | print*,'Resolution given in file: ',trim(dt_file) |
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193 | print*,'is ',nres,', which does not match nS.' |
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194 | print*,'Please adjust nS value in interpolateH2H2.F90' |
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195 | endif |
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196 | stop |
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197 | endif |
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198 | temp_arr(iT)=Ttemp |
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199 | |
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200 | do k=1,nS |
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201 | read(33,*) wn_arr(k),abs_arr(k,it) |
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202 | end do |
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203 | |
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204 | end do |
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205 | |
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206 | endif |
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207 | close(33) |
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208 | !$OMP END MASTER |
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209 | !$OMP BARRIER |
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210 | |
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211 | if (is_master) then |
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212 | print*,'interpolateH2H2: At wavenumber ',wn,' cm^-1' |
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213 | print*,' temperature ',temp,' K' |
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214 | print*,' pressure ',pres,' Pa' |
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215 | endif |
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216 | endif |
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217 | |
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218 | |
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219 | |
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220 | call bilinearbig(nS,nT,wn_arr,temp_arr,abs_arr,wn,ztemp,abcoef,ind) |
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221 | |
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222 | !print*,'the absorption is ',abcoef,' cm^5 molecule^-2' |
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223 | !print*,'or ',abcoef*losch**2,' cm^-1 amagat^-2' |
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224 | |
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225 | abcoef=abcoef*losch**2*100.0*amagat**2 ! convert to m^-1 |
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226 | |
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227 | !print*,'We have ',amagat,' amagats of H2' |
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228 | !print*,'So the absorption is ',abcoef,' m^-1' |
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229 | |
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230 | ! unlike for Rayleigh scattering, we do not currently weight by the BB function |
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231 | ! however our bands are normally thin, so this is no big deal. |
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232 | |
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233 | return |
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234 | end subroutine interpolateH2H2 |
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