1 | subroutine read_dust_scenario(ngrid,nlayer,zday,pplev,tauref) |
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2 | |
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3 | ! Reading of the dust scenario file |
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4 | |
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5 | use netcdf |
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6 | use geometry_mod, only: latitude, longitude ! in radians |
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7 | use datafile_mod, only: datadir |
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8 | implicit none |
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9 | |
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10 | include "callkeys.h" |
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11 | |
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12 | integer, intent(in) :: ngrid,nlayer |
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13 | real, intent(in) :: zday ! date in martian days |
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14 | real, dimension(ngrid,nlayer+1), intent(in) :: pplev |
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15 | real, dimension(ngrid), intent(out) :: tauref |
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16 | |
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17 | ! Local variables |
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18 | |
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19 | real :: realday |
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20 | integer nid,nvarid,ierr |
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21 | integer ltloop,lsloop,iloop,jloop,varloop,ig |
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22 | real, dimension(2) :: taubuf |
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23 | real tau1(4),tau |
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24 | real alt(4) |
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25 | integer latp(4),lonp(4) |
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26 | integer yinf,ysup,xinf,xsup,tinf,tsup |
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27 | real latinf,latsup,loninf,lonsup |
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28 | real latintmp,lonintmp,latdeg,londeg |
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29 | real colat,dlat,dlon,colattmp |
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30 | logical, save :: firstcall=.true. |
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31 | logical :: timeflag |
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32 | real,save :: radeg,pi |
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33 | integer :: timedim,londim,latdim |
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34 | real, dimension(:), allocatable, save :: lat,lon,time |
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35 | real, dimension(:,:,:), allocatable, save :: tautes |
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36 | integer, save :: timelen,lonlen,latlen |
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37 | character(len=33),save :: filename |
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38 | |
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39 | realday=mod(zday,669.) |
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40 | |
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41 | ! AS: firstcall OK absolute |
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42 | if (firstcall) then |
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43 | firstcall=.false. |
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44 | |
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45 | pi=acos(-1.) |
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46 | radeg=180/pi |
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47 | |
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48 | ! assimilated dust file: (NB: iaervar is a common in "callkeys.h") |
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49 | ! iaervar=4 means read dust_tes.nc file |
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50 | ! iaervar=6 means read dust_cold.nc file |
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51 | ! iaervar=7 means read dust_warm.nc file |
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52 | ! iaervar=8 means read dust_clim.nc file |
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53 | ! iaervar=24 means read dust_MY24.nc file |
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54 | ! iaervar=25 means read dust_MY25.nc file |
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55 | ! iaervar=26 means read dust_MY26.nc file, etc. |
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56 | if (iaervar.eq.4) then |
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57 | ! NB: 4: old TES assimilated MY24 dust scenarios (at 700Pa ref pressure!) |
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58 | filename="dust_tes.nc" |
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59 | else if (iaervar.eq.6) then |
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60 | filename="dust_cold.nc" |
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61 | else if (iaervar.eq.7) then |
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62 | filename="dust_warm.nc" |
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63 | else if (iaervar.eq.8) then |
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64 | filename="dust_clim.nc" |
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65 | else if (iaervar.eq.24) then |
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66 | filename="dust_MY24.nc" |
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67 | else if (iaervar.eq.25) then |
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68 | filename="dust_MY25.nc" |
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69 | else if (iaervar.eq.26) then |
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70 | filename="dust_MY26.nc" |
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71 | else if (iaervar.eq.27) then |
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72 | filename="dust_MY27.nc" |
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73 | else if (iaervar.eq.28) then |
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74 | filename="dust_MY28.nc" |
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75 | else if (iaervar.eq.29) then |
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76 | filename="dust_MY29.nc" |
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77 | else if (iaervar.eq.30) then |
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78 | filename="dust_MY30.nc" |
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79 | else if (iaervar.eq.31) then |
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80 | filename="dust_MY31.nc" |
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81 | else if (iaervar.eq.32) then |
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82 | filename="dust_MY32.nc" |
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83 | else if (iaervar.eq.33) then |
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84 | filename="dust_MY33.nc" |
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85 | else if (iaervar.eq.34) then |
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86 | filename="dust_MY34.nc" |
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87 | ! 124,125,126: old TES assimilated dust scenarios (at 700Pa ref pressure!) |
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88 | else if (iaervar.eq.124) then |
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89 | filename="dust_tes_MY24.nc" |
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90 | else if (iaervar.eq.125) then |
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91 | filename="dust_tes_MY25.nc" |
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92 | else if (iaervar.eq.126) then |
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93 | filename="dust_tes_MY26.nc" |
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94 | endif |
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95 | |
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96 | ierr=nf90_open(trim(datadir)//"/"//trim(filename),NF90_NOWRITE,nid) |
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97 | IF (ierr.NE.nf90_noerr) THEN |
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98 | write(*,*)'Problem opening ',trim(filename),' (in phymars/read_dust_scenario.F90)' |
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99 | write(*,*)'It should be in :',trim(datadir),'/' |
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100 | write(*,*)'1) You can change this directory address in callfis.def with' |
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101 | write(*,*)' datadir=/path/to/datafiles' |
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102 | write(*,*)'2) If necessary, dust*.nc (and other datafiles)' |
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103 | write(*,*)' can be obtained online on:' |
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104 | write(*,*)' http://www.lmd.jussieu.fr/~lmdz/planets/mars/datadir' |
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105 | CALL ABORT |
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106 | ENDIF |
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107 | |
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108 | ierr=nf90_inq_dimid(nid,"Time",timedim) |
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109 | if (ierr.ne.nf90_noerr) then |
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110 | ! 'Time' dimension not found, look for 'time' |
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111 | ierr=nf90_inq_dimid(nid,"time",timedim) |
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112 | if (ierr.ne.nf90_noerr) then |
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113 | write(*,*)"Error: read_dust_scenario <time> not found" |
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114 | endif |
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115 | endif |
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116 | ierr=nf90_inquire_dimension(nid,timedim,len=timelen) |
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117 | ierr=nf90_inq_dimid(nid,"latitude",latdim) |
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118 | ierr=nf90_inquire_dimension(nid,latdim,len=latlen) |
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119 | ierr=nf90_inq_dimid(nid,"longitude",londim) |
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120 | ierr=nf90_inquire_dimension(nid,londim,len=lonlen) |
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121 | |
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122 | |
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123 | if (.not.allocated(tautes)) allocate(tautes(lonlen,latlen,timelen)) |
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124 | if (.not.allocated(lat)) allocate(lat(latlen), lon(lonlen), time(timelen)) |
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125 | |
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126 | ! "dustop" if loading visible extinction opacity |
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127 | ! "cdod" if loading IR absorption opacity |
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128 | ierr=nf90_inq_varid(nid,"dustop",nvarid) |
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129 | if (ierr.eq.nf90_noerr) then |
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130 | ierr=nf90_get_var(nid,nvarid,tautes) |
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131 | IF (ierr .NE. nf90_noerr) THEN |
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132 | PRINT*, "Error: read_dust_scenario <dustop> not found" |
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133 | write(*,*)trim(nf90_strerror(ierr)) |
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134 | stop |
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135 | ENDIF |
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136 | else |
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137 | ! did not find "dustop" , look for "cdod" |
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138 | ierr=nf90_inq_varid(nid,"cdod",nvarid) |
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139 | ierr=nf90_get_var(nid,nvarid,tautes) |
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140 | IF (ierr .NE. nf90_noerr) THEN |
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141 | PRINT*, "Error: read_dust_scenario <cdod> not found" |
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142 | write(*,*)trim(nf90_strerror(ierr)) |
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143 | stop |
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144 | ENDIF |
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145 | ! and multiply by 2*1.3=2.6 to convert from IR absorption |
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146 | ! to visible extinction opacity |
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147 | tautes(:,:,:)=2.6*tautes(:,:,:) |
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148 | endif |
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149 | |
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150 | ierr=nf90_inq_varid(nid,"Time",nvarid) |
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151 | ierr=nf90_get_var(nid,nvarid,time) |
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152 | IF (ierr .NE. nf90_noerr) THEN |
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153 | PRINT*, "Error: read_dust_scenario <Time> not found" |
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154 | write(*,*)trim(nf90_strerror(ierr)) |
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155 | stop |
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156 | ENDIF |
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157 | |
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158 | ierr=nf90_inq_varid(nid,"latitude",nvarid) |
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159 | ierr=nf90_get_var(nid,nvarid,lat) |
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160 | IF (ierr .NE. nf90_noerr) THEN |
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161 | PRINT*, "Error: read_dust_scenario <latitude> not found" |
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162 | write(*,*)trim(nf90_strerror(ierr)) |
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163 | stop |
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164 | ENDIF |
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165 | |
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166 | ierr=nf90_inq_varid(nid,"longitude",nvarid) |
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167 | ierr=nf90_get_var(nid,nvarid,lon) |
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168 | IF (ierr .NE. nf90_noerr) THEN |
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169 | PRINT*, "Error: read_dust_scenario <longitude> not found" |
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170 | write(*,*)trim(nf90_strerror(ierr)) |
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171 | stop |
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172 | ENDIF |
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173 | |
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174 | ierr=nf90_close(nid) |
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175 | |
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176 | endif ! of if (firstcall) |
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177 | |
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178 | do ig=1,ngrid |
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179 | |
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180 | ! Find the four nearest points, arranged as follows: |
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181 | ! 1 2 |
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182 | ! 3 4 |
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183 | |
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184 | latdeg=latitude(ig)*radeg ! latitude, in degrees |
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185 | londeg=longitude(ig)*radeg ! longitude, in degrees east |
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186 | colat=90-latdeg ! colatitude, in degrees |
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187 | |
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188 | ! Ehouarn: rounding effects and/or specific compiler issues |
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189 | ! sometime cause londeg to be sligthly below -180 ... |
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190 | if (londeg.lt.-180) then |
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191 | ! check if it is by a large amount |
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192 | if ((londeg+180).lt.-1.e-3) then |
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193 | write(*,*) 'reattesassim: error!!' |
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194 | write(*,*) ' ig=',ig,' londeg=',londeg |
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195 | stop |
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196 | else |
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197 | londeg=-180 |
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198 | endif |
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199 | endif |
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200 | |
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201 | ! Find encompassing latitudes |
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202 | if (colat<(90-lat(1))) then ! between north pole and lat(1) |
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203 | ysup=1 |
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204 | yinf=1 |
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205 | else if (colat>=90-(lat(latlen))) then ! between south pole and lat(laten) |
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206 | ysup=latlen |
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207 | yinf=latlen |
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208 | else ! general case |
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209 | do iloop=2,latlen |
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210 | if(colat<(90-lat(iloop))) then |
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211 | ysup=iloop-1 |
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212 | yinf=iloop |
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213 | exit |
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214 | endif |
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215 | enddo |
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216 | endif |
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217 | |
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218 | latinf=lat(yinf) |
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219 | latsup=lat(ysup) |
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220 | |
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221 | |
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222 | ! Find encompassing longitudes |
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223 | ! Note: in input file, lon(1)=-180. |
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224 | if (londeg>lon(lonlen)) then |
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225 | xsup=1 |
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226 | xinf=lonlen |
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227 | loninf=lon(xsup) |
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228 | lonsup=180.0 ! since lon(1)=-180.0 |
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229 | else |
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230 | do iloop=2,lonlen |
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231 | if(londeg<lon(iloop)) then |
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232 | xsup=iloop |
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233 | xinf=iloop-1 |
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234 | exit |
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235 | endif |
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236 | enddo |
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237 | loninf=lon(xinf) |
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238 | lonsup=lon(xsup) |
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239 | endif |
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240 | |
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241 | if ((xsup.gt.lonlen).OR.(yinf.gt.latlen).OR.(xinf.lt.1)& |
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242 | .OR.(ysup.lt.1)) then |
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243 | write (*,*) "read_dust_scenario: SYSTEM ERROR on x or y in ts_gcm" |
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244 | write (*,*) "xinf: ",xinf |
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245 | write (*,*) "xsup: ",xsup |
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246 | write (*,*) "yinf: ",yinf |
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247 | write (*,*) "ysup: ",ysup |
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248 | stop |
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249 | endif |
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250 | |
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251 | ! loninf=lon(xinf) |
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252 | ! lonsup=lon(xsup) |
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253 | ! latinf=lat(yinf) |
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254 | ! latsup=lat(ysup) |
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255 | |
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256 | ! The four neighbouring points are arranged as follows: |
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257 | ! 1 2 |
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258 | ! 3 4 |
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259 | |
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260 | latp(1)=ysup |
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261 | latp(2)=ysup |
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262 | latp(3)=yinf |
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263 | latp(4)=yinf |
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264 | |
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265 | lonp(1)=xinf |
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266 | lonp(2)=xsup |
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267 | lonp(3)=xinf |
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268 | lonp(4)=xsup |
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269 | |
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270 | ! Linear interpolation on time, for all four neighbouring points |
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271 | |
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272 | if ((realday<time(1)).or.(realday>time(timelen))) then |
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273 | tinf=timelen |
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274 | tsup=1 |
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275 | timeflag=.true. |
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276 | else |
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277 | timeflag=.false. |
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278 | do iloop=2,timelen |
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279 | if (realday<=time(iloop)) then |
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280 | tinf=iloop-1 |
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281 | tsup=iloop |
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282 | exit |
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283 | endif |
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284 | enddo |
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285 | endif |
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286 | |
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287 | ! Bilinear interpolation on the four nearest points |
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288 | |
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289 | if ((colat<(90-lat(1))).OR.(colat>(90-lat(latlen))).OR.(latsup==latinf)) then |
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290 | dlat=0 |
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291 | else |
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292 | dlat=((90-latinf)-colat)/((90-latinf)-(90-latsup)) |
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293 | endif |
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294 | |
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295 | if (lonsup==loninf) then |
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296 | dlon=0 |
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297 | else |
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298 | dlon=(londeg-loninf)/(lonsup-loninf) |
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299 | endif |
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300 | |
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301 | do iloop=1,4 |
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302 | taubuf(1)=tautes(lonp(iloop),latp(iloop),tinf) |
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303 | taubuf(2)=tautes(lonp(iloop),latp(iloop),tsup) |
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304 | if (timeflag) then |
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305 | if (realday>time(timelen)) then |
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306 | tau1(iloop)=taubuf(1)+(taubuf(2)-taubuf(1))*(realday-time(tinf))/(time(tsup)+(669-time(tinf))) |
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307 | else |
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308 | tau1(iloop)=taubuf(1)+(taubuf(2)-taubuf(1))*realday/(time(tsup)+(669-time(tinf))) |
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309 | endif |
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310 | else |
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311 | tau1(iloop)=taubuf(1)+(taubuf(2)-taubuf(1))*(realday-time(tinf))/(time(tsup)-time(tinf)) |
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312 | endif |
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313 | if (tau1(iloop)<0) then |
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314 | write (*,*) "read_dust_scenario: SYSTEM ERROR on tau" |
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315 | write (*,*) "utime ",realday |
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316 | write (*,*) "time(tinf) ",time(tinf) |
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317 | write (*,*) "time(tsup) ",time(tsup) |
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318 | write (*,*) "tau1 ",taubuf(1) |
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319 | write (*,*) "tau2 ",taubuf(2) |
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320 | write (*,*) "tau ",tau1(iloop) |
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321 | stop |
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322 | endif |
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323 | enddo |
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324 | |
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325 | if ((dlat>1).OR.(dlon>1) .OR. (dlat<0) .OR. (dlon<0)) then |
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326 | write (*,*) "read_dust_scenario: SYSTEM ERROR on dlat or dlon in ts_gcm" |
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327 | write (*,*) "dlat: ",dlat |
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328 | write (*,*) "lat: ",latdeg |
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329 | write (*,*) "dlon: ",dlon |
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330 | write (*,*) "lon: ",londeg |
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331 | stop |
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332 | endif |
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333 | |
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334 | tau= dlat*(dlon*(tau1(2)+tau1(3)-tau1(1)-tau1(4))+tau1(1)-tau1(3)) +dlon*(tau1(4)-tau1(3))+tau1(3) |
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335 | |
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336 | tauref(ig)=tau |
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337 | ! |
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338 | enddo ! of ig=1,ngrid |
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339 | |
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340 | if (filename(1:8)=="dust_tes") then |
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341 | ! when using old TES files, correction for: |
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342 | ! - the reference pressure was 700Pa (unlike 610Pa now) |
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343 | ! - the 1.3 conversion factor from IR absorbtion opacity to |
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344 | ! IR extinction opacity |
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345 | tauref(:)=tauref(:)*1.3*(610./700.) |
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346 | endif |
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347 | |
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348 | if (swrtype.eq.1) then ! Fouquart (NB: swrtype is set in callkeys.h) |
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349 | ! when using old radiative transfer (like in MCD 4.x) |
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350 | ! needed to decrease opacity (*0.825) to compensate overestimation of |
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351 | ! heating rates |
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352 | tauref(:)=tauref(:)*0.825/1.3 |
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353 | endif |
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354 | |
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355 | end |
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