1 | SUBROUTINE calcratqs(klon,klev,prt_level,lunout, & |
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2 | iflag_ratqs,iflag_con,iflag_cld_th,pdtphys, & |
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3 | ratqsbas,ratqshaut,ratqsp0,ratqsdp, & |
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4 | tau_ratqs,fact_cldcon,wake_s, wake_deltaq, & |
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5 | ptconv,ptconvth,clwcon0th, rnebcon0th, & |
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6 | paprs,pplay,t_seri,q_seri, & |
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7 | qtc_cv, sigt_cv, zqsat, & |
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8 | tke,tke_dissip,lmix,wprime, & |
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9 | t2m,q2m,fm_therm,cell_area,& |
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10 | ratqs,ratqsc,ratqs_inter) |
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11 | |
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12 | |
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13 | USE indice_sol_mod |
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14 | USE phys_state_var_mod, ONLY: pctsrf |
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15 | USE calcratqs_multi_mod, ONLY: calcratqs_inter, calcratqs_oro, calcratqs_hetero, calcratqs_tke |
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16 | |
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17 | implicit none |
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18 | |
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19 | !======================================================================== |
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20 | ! Computation of ratqs, the width of the subrid scale water distribution |
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21 | ! (normalized by the mean value) |
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22 | ! Various options controled by flags iflag_con and iflag_ratqs |
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23 | ! F Hourdin 2012/12/06 |
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24 | !======================================================================== |
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25 | |
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26 | ! Declarations |
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27 | |
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28 | ! Input |
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29 | integer,intent(in) :: klon,klev,prt_level,lunout |
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30 | integer,intent(in) :: iflag_con,iflag_cld_th,iflag_ratqs |
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31 | real,intent(in) :: pdtphys,ratqsbas,ratqshaut,fact_cldcon,tau_ratqs |
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32 | real,intent(in) :: ratqsp0, ratqsdp |
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33 | real, dimension(klon,klev+1),intent(in) :: paprs,tke,tke_dissip,lmix,wprime |
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34 | real, dimension(klon,klev),intent(in) :: pplay,t_seri,q_seri,zqsat,fm_therm, qtc_cv, sigt_cv |
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35 | logical, dimension(klon,klev),intent(in) :: ptconv |
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36 | real, dimension(klon,klev),intent(in) :: rnebcon0th,clwcon0th |
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37 | real, dimension(klon,klev),intent(in) :: wake_deltaq,wake_s |
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38 | real, dimension(klon,nbsrf),intent(in) :: t2m,q2m |
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39 | real, dimension(klon), intent(in) :: cell_area |
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40 | ! Output |
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41 | real, dimension(klon,klev),intent(inout) :: ratqs,ratqsc,ratqs_inter |
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42 | |
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43 | logical, dimension(klon,klev),intent(inout) :: ptconvth |
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44 | |
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45 | ! local |
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46 | integer i,k |
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47 | real, dimension(klon,klev) :: ratqss |
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48 | real facteur,zfratqs1,zfratqs2 |
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49 | real, dimension(klon,klev) :: ratqs_hetero,ratqs_oro,ratqs_tke |
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50 | real resol,resolmax,fact |
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51 | |
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52 | !------------------------------------------------------------------------- |
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53 | ! Caclul des ratqs |
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54 | !------------------------------------------------------------------------- |
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55 | |
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56 | ! print*,'calcul des ratqs' |
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57 | ! ratqs convectifs a l'ancienne en fonction de q(z=0)-q / q |
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58 | ! ---------------- |
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59 | ! on ecrase le tableau ratqsc calcule par clouds_gno |
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60 | if (iflag_cld_th.eq.1) then |
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61 | do k=1,klev |
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62 | do i=1,klon |
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63 | if(ptconv(i,k)) then |
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64 | ratqsc(i,k)=ratqsbas & |
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65 | +fact_cldcon*(q_seri(i,1)-q_seri(i,k))/q_seri(i,k) |
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66 | else |
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67 | ratqsc(i,k)=0. |
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68 | endif |
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69 | enddo |
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70 | enddo |
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71 | |
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72 | !----------------------------------------------------------------------- |
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73 | ! par nversion de la fonction log normale |
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74 | !----------------------------------------------------------------------- |
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75 | else if (iflag_cld_th.eq.4) then |
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76 | ptconvth(:,:)=.false. |
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77 | ratqsc(:,:)=0. |
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78 | if(prt_level.ge.9) print*,'avant clouds_gno thermique' |
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79 | call clouds_gno & |
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80 | (klon,klev,q_seri,zqsat,clwcon0th,ptconvth,ratqsc,rnebcon0th) |
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81 | if(prt_level.ge.9) print*,' CLOUDS_GNO OK' |
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82 | |
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83 | endif |
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84 | |
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85 | ! ratqs stables |
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86 | ! ------------- |
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87 | |
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88 | if (iflag_ratqs.eq.0) then |
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89 | |
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90 | ! Le cas iflag_ratqs=0 correspond a la version IPCC 2005 du modele. |
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91 | do k=1,klev |
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92 | do i=1, klon |
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93 | ratqss(i,k)=ratqsbas+(ratqshaut-ratqsbas)* & |
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94 | min((paprs(i,1)-pplay(i,k))/(paprs(i,1)-30000.),1.) |
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95 | enddo |
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96 | enddo |
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97 | |
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98 | ! Pour iflag_ratqs=1 ou 2, le ratqs est constant au dessus de |
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99 | ! 300 hPa (ratqshaut), varie lineariement en fonction de la pression |
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100 | ! entre 600 et 300 hPa et est soit constant (ratqsbas) pour iflag_ratqs=1 |
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101 | ! soit lineaire (entre 0 a la surface et ratqsbas) pour iflag_ratqs=2 |
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102 | ! Il s'agit de differents tests dans la phase de reglage du modele |
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103 | ! avec thermiques. |
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104 | |
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105 | else if (iflag_ratqs.eq.1) then |
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106 | |
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107 | do k=1,klev |
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108 | do i=1, klon |
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109 | if (pplay(i,k).ge.60000.) then |
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110 | ratqss(i,k)=ratqsbas |
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111 | else if ((pplay(i,k).ge.30000.).and.(pplay(i,k).lt.60000.)) then |
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112 | ratqss(i,k)=ratqsbas+(ratqshaut-ratqsbas)*(60000.-pplay(i,k))/(60000.-30000.) |
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113 | else |
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114 | ratqss(i,k)=ratqshaut |
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115 | endif |
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116 | enddo |
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117 | enddo |
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118 | |
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119 | else if (iflag_ratqs.eq.2) then |
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120 | |
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121 | do k=1,klev |
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122 | do i=1, klon |
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123 | if (pplay(i,k).ge.60000.) then |
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124 | ratqss(i,k)=ratqsbas*(paprs(i,1)-pplay(i,k))/(paprs(i,1)-60000.) |
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125 | else if ((pplay(i,k).ge.30000.).and.(pplay(i,k).lt.60000.)) then |
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126 | ratqss(i,k)=ratqsbas+(ratqshaut-ratqsbas)*(60000.-pplay(i,k))/(60000.-30000.) |
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127 | else |
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128 | ratqss(i,k)=ratqshaut |
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129 | endif |
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130 | enddo |
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131 | enddo |
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132 | |
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133 | else if (iflag_ratqs==3) then |
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134 | do k=1,klev |
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135 | ratqss(:,k)=ratqsbas+(ratqshaut-ratqsbas) & |
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136 | *min( ((paprs(:,1)-pplay(:,k))/70000.)**2 , 1. ) |
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137 | enddo |
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138 | |
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139 | else if (iflag_ratqs==4) then |
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140 | do k=1,klev |
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141 | ratqss(:,k)=ratqsbas+0.5*(ratqshaut-ratqsbas) & |
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142 | ! *( tanh( (50000.-pplay(:,k))/20000.) + 1.) |
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143 | *( tanh( (ratqsp0-pplay(:,k))/ratqsdp) + 1.) |
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144 | enddo |
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145 | |
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146 | |
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147 | else if (iflag_ratqs==5) then |
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148 | ! Dependency of ratqs on model resolution |
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149 | ! Audran, Meryl, Lea, Gwendal and Etienne |
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150 | ! April 2023 |
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151 | resolmax=sqrt(maxval(cell_area)) |
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152 | do k=1,klev |
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153 | do i=1,klon |
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154 | resol=sqrt(cell_area(i)) |
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155 | fact=sqrt(resol/resolmax) |
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156 | ratqss(i,k)=ratqsbas*fact+0.5*(ratqshaut-ratqsbas)*fact & |
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157 | *( tanh( (ratqsp0-pplay(i,k))/ratqsdp) + 1.) |
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158 | enddo |
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159 | enddo |
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160 | |
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161 | |
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162 | else if (iflag_ratqs .GT. 9) then |
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163 | |
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164 | ! interactive ratqs calculations that depend on cold pools, orography, surface heterogeneity and small-scale turbulence |
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165 | ! This should help getting a more realistic ratqs in the low and mid troposphere |
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166 | ! We however need a "background" ratqs to account for subgrid distribution of qt (or qt/qs) |
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167 | ! in the high troposphere |
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168 | |
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169 | ! background ratqs and initialisations |
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170 | do k=1,klev |
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171 | do i=1,klon |
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172 | ratqss(i,k)=ratqsbas+0.5*(ratqshaut-ratqsbas) & |
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173 | *( tanh( (ratqsp0-pplay(i,k))/ratqsdp) + 1.) |
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174 | ratqss(i,k)=max(ratqss(i,k),0.0) |
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175 | |
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176 | ratqs_hetero(i,k)=0. |
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177 | ratqs_oro(i,k)=0. |
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178 | ratqs_tke(i,k)=0. |
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179 | ratqs_inter(i,k)=0 |
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180 | enddo |
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181 | enddo |
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182 | |
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183 | if (iflag_ratqs .EQ. 10) then |
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184 | ! interactive ratqs in presence of cold pools |
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185 | call calcratqs_inter(klon,klev,iflag_ratqs,pdtphys,ratqsbas,wake_deltaq,wake_s,q_seri,qtc_cv, sigt_cv,ratqs_inter) |
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186 | do k=1,klev |
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187 | do i=1,klon |
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188 | ratqs_inter(i,k)=ratqs_inter(i,k)-0.5*ratqs_inter(i,k)*(tanh((ratqsp0-pplay(i,k))/ratqsdp)+1.) |
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189 | enddo |
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190 | enddo |
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191 | ratqss=ratqss+ratqs_inter |
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192 | else if (iflag_ratqs .EQ. 11) then |
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193 | ! interactive ratqs with several sources |
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194 | call calcratqs_inter(klon,klev,iflag_ratqs,pdtphys,ratqsbas,wake_deltaq,wake_s,q_seri,qtc_cv, sigt_cv,ratqs_inter) |
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195 | ratqss=ratqss+ratqs_inter |
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196 | else if (iflag_ratqs .EQ. 12) then |
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197 | ! contribution of surface heterogeneities to ratqs |
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198 | call calcratqs_hetero(klon,klev,t2m,q2m,t_seri,q_seri,pplay,paprs,ratqs_hetero) |
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199 | ratqss=ratqss+ratqs_hetero |
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200 | else if (iflag_ratqs .EQ. 13) then |
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201 | ! contribution of ubgrid orography to ratqs |
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202 | call calcratqs_oro(klon,klev,zqsat,t_seri,pplay,paprs,ratqs_oro) |
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203 | ratqss=ratqss+ratqs_oro |
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204 | else if (iflag_ratqs .EQ. 14) then |
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205 | ! effect of subgrid-scale TKE on ratqs (in development) |
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206 | call calcratqs_tke(klon,klev,pdtphys,t_seri,q_seri,zqsat,pplay,paprs,tke,tke_dissip,lmix,wprime,ratqs_tke) |
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207 | ratqss=ratqss+ratqs_tke |
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208 | endif |
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209 | |
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210 | |
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211 | endif |
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212 | |
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213 | |
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214 | ! ratqs final |
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215 | ! ----------- |
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216 | |
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217 | if (iflag_cld_th.eq.1 .or.iflag_cld_th.eq.2.or.iflag_cld_th.eq.4) then |
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218 | |
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219 | ! On ajoute une constante au ratqsc*2 pour tenir compte de |
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220 | ! fluctuations turbulentes de petite echelle |
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221 | |
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222 | do k=1,klev |
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223 | do i=1,klon |
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224 | if ((fm_therm(i,k).gt.1.e-10)) then |
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225 | ratqsc(i,k)=sqrt(ratqsc(i,k)**2+0.05**2) |
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226 | endif |
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227 | enddo |
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228 | enddo |
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229 | |
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230 | ! les ratqs sont une combinaison de ratqss et ratqsc |
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231 | if(prt_level.ge.9) write(lunout,*)'PHYLMD NOUVEAU TAU_RATQS ',tau_ratqs |
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232 | |
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233 | if (tau_ratqs>1.e-10) then |
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234 | facteur=exp(-pdtphys/tau_ratqs) |
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235 | else |
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236 | facteur=0. |
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237 | endif |
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238 | ratqs(:,:)=ratqsc(:,:)*(1.-facteur)+ratqs(:,:)*facteur |
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239 | !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! |
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240 | ! FH 22/09/2009 |
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241 | ! La ligne ci-dessous faisait osciller le modele et donnait une solution |
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242 | ! assymptotique bidon et dépendant fortement du pas de temps. |
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243 | ! ratqs(:,:)=sqrt(ratqs(:,:)**2+ratqss(:,:)**2) |
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244 | !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! |
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245 | ratqs(:,:)=max(ratqs(:,:),ratqss(:,:)) |
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246 | else if (iflag_cld_th<=6) then |
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247 | ! on ne prend que le ratqs stable pour fisrtilp |
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248 | ratqs(:,:)=ratqss(:,:) |
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249 | else |
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250 | zfratqs1=exp(-pdtphys/10800.) |
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251 | zfratqs2=exp(-pdtphys/10800.) |
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252 | do k=1,klev |
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253 | do i=1,klon |
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254 | if (ratqsc(i,k).gt.1.e-10) then |
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255 | ratqs(i,k)=ratqs(i,k)*zfratqs2+(iflag_cld_th/100.)*ratqsc(i,k)*(1.-zfratqs2) |
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256 | endif |
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257 | ratqs(i,k)=min(ratqs(i,k)*zfratqs1+ratqss(i,k)*(1.-zfratqs1),0.5) |
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258 | enddo |
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259 | enddo |
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260 | endif |
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261 | |
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262 | |
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263 | return |
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264 | end |
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