1 | subroutine interpolateH2H2(wn,temp,pres,abcoef,firstcall,ind) |
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2 | |
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3 | !================================================================== |
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4 | ! |
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5 | ! Purpose |
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6 | ! ------- |
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7 | ! Calculates the H2-H2 CIA opacity, using a lookup table from |
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8 | ! HITRAN (2011) |
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9 | ! |
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10 | ! Authors |
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11 | ! ------- |
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12 | ! R. Wordsworth (2011) |
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13 | ! |
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14 | !================================================================== |
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15 | |
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16 | use datafile_mod, only: datadir |
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17 | |
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18 | implicit none |
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19 | |
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20 | ! input |
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21 | double precision wn ! wavenumber (cm^-1) |
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22 | double precision temp ! temperature (Kelvin) |
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23 | double precision pres ! pressure (Pascals) |
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24 | |
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25 | ! output |
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26 | double precision abcoef ! absorption coefficient (m^-1) |
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27 | |
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28 | integer nS,nT |
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29 | parameter(nS=2428) |
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30 | parameter(nT=10) |
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31 | |
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32 | double precision, parameter :: losch = 2.6867774e19 |
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33 | ! Loschmit's number (molecule cm^-3 at STP) |
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34 | ! converts cm^5 molecule^-2 --> cm^-1 amagat^-2 |
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35 | ! see Richard et al. 2011, JQSRT for details |
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36 | |
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37 | double precision amagat |
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38 | double precision wn_arr(nS) |
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39 | double precision temp_arr(nT) |
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40 | double precision abs_arr(nS,nT) |
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41 | |
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42 | integer k,iT |
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43 | logical firstcall |
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44 | |
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45 | save wn_arr, temp_arr, abs_arr |
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46 | |
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47 | character*100 dt_file |
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48 | integer strlen,ios |
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49 | |
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50 | character(LEN=*), parameter :: fmat1 = "(A20,F10.3,F10.3,I7,F7.1,E10.3,F5.3)" |
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51 | |
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52 | character*20 bleh |
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53 | double precision blah, Ttemp |
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54 | integer nres |
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55 | |
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56 | integer ind |
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57 | |
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58 | if(temp.gt.400)then |
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59 | print*,'Your temperatures are too high for this H2-H2 CIA dataset. If you ' |
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60 | print*,'really want to run simulations with hydrogen at T > 400 K, contact' |
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61 | print*,'Robin Wordsworth [rwordsworth@uchicago.edu].' |
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62 | stop |
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63 | endif |
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64 | |
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65 | amagat = (273.15/temp)*(pres/101325.0) |
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66 | |
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67 | if(firstcall)then ! called by sugas_corrk only |
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68 | print*,'----------------------------------------------------' |
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69 | print*,'Initialising H2-H2 continuum from HITRAN database...' |
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70 | |
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71 | ! 1.1 Open the ASCII files |
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72 | dt_file=TRIM(datadir)//'/continuum_data/H2-H2_norm_2011.cia' |
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73 | |
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74 | open(33,file=dt_file,form='formatted',status='old',iostat=ios) |
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75 | if (ios.ne.0) then ! file not found |
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76 | write(*,*) 'Error from interpolateH2H2' |
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77 | write(*,*) 'Data file ',trim(dt_file),' not found.' |
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78 | write(*,*) 'Check that your path to datagcm:',trim(datadir) |
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79 | write(*,*) 'is correct. You can change it in callphys.def with:' |
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80 | write(*,*) 'datadir = /absolute/path/to/datagcm' |
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81 | write(*,*) 'Also check that the continuum data continuum_data/H2-H2_norm_2011.cia is there.' |
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82 | call abort |
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83 | else |
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84 | |
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85 | do iT=1,nT |
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86 | |
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87 | read(33,fmat1) bleh,blah,blah,nres,Ttemp |
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88 | if(nS.ne.nres)then |
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89 | print*,'Resolution given in file: ',trim(dt_file) |
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90 | print*,'is ',nres,', which does not match nS.' |
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91 | print*,'Please adjust nS value in interpolateH2H2.F90' |
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92 | stop |
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93 | endif |
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94 | temp_arr(iT)=Ttemp |
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95 | |
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96 | do k=1,nS |
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97 | read(33,*) wn_arr(k),abs_arr(k,it) |
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98 | end do |
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99 | |
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100 | end do |
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101 | |
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102 | endif |
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103 | close(33) |
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104 | |
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105 | print*,'interpolateH2H2: At wavenumber ',wn,' cm^-1' |
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106 | print*,' temperature ',temp,' K' |
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107 | print*,' pressure ',pres,' Pa' |
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108 | |
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109 | endif |
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110 | |
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111 | call bilinearbig(nS,nT,wn_arr,temp_arr,abs_arr,wn,temp,abcoef,ind) |
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112 | |
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113 | !print*,'the absorption is ',abcoef,' cm^5 molecule^-2' |
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114 | !print*,'or ',abcoef*losch**2,' cm^-1 amagat^-2' |
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115 | |
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116 | abcoef=abcoef*losch**2*100.0*amagat**2 ! convert to m^-1 |
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117 | |
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118 | !print*,'We have ',amagat,' amagats of H2' |
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119 | !print*,'So the absorption is ',abcoef,' m^-1' |
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120 | |
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121 | ! unlike for Rayleigh scattering, we do not currently weight by the BB function |
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122 | ! however our bands are normally thin, so this is no big deal. |
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123 | |
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124 | return |
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125 | end subroutine interpolateH2H2 |
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