1 | ! |
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2 | ! $Header$ |
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3 | ! |
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4 | SUBROUTINE yamada_c(ngrid,timestep,plev,play & |
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5 | & ,pu,pv,pt,d_u,d_v,d_t,cd,q2,km,kn,kq,d_t_diss,ustar & |
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6 | & ,iflag_pbl) |
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7 | USE dimphy, ONLY: klon, klev |
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8 | USE print_control_mod, ONLY: prt_level |
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9 | USE ioipsl_getin_p_mod, ONLY : getin_p |
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10 | |
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11 | USE yomcst_mod_h |
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12 | IMPLICIT NONE |
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13 | |
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14 | ! |
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15 | ! timestep : pas de temps |
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16 | ! g : g |
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17 | ! zlev : altitude a chaque niveau (interface inferieure de la couche |
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18 | ! de meme indice) |
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19 | ! zlay : altitude au centre de chaque couche |
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20 | ! u,v : vitesse au centre de chaque couche |
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21 | ! (en entree : la valeur au debut du pas de temps) |
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22 | ! teta : temperature potentielle au centre de chaque couche |
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23 | ! (en entree : la valeur au debut du pas de temps) |
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24 | ! cd : cdrag |
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25 | ! (en entree : la valeur au debut du pas de temps) |
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26 | ! q2 : $q^2$ au bas de chaque couche |
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27 | ! (en entree : la valeur au debut du pas de temps) |
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28 | ! (en sortie : la valeur a la fin du pas de temps) |
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29 | ! km : diffusivite turbulente de quantite de mouvement (au bas de chaque |
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30 | ! couche) |
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31 | ! (en sortie : la valeur a la fin du pas de temps) |
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32 | ! kn : diffusivite turbulente des scalaires (au bas de chaque couche) |
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33 | ! (en sortie : la valeur a la fin du pas de temps) |
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34 | ! |
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35 | ! iflag_pbl doit valoir entre 6 et 9 |
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36 | ! l=6, on prend systematiquement une longueur d'equilibre |
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37 | ! iflag_pbl=6 : MY 2.0 |
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38 | ! iflag_pbl=7 : MY 2.0.Fournier |
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39 | ! iflag_pbl=8/9 : MY 2.5 |
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40 | ! iflag_pbl=8 with special obsolete treatments for convergence |
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41 | ! with Cmpi5 NPv3.1 simulations |
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42 | ! iflag_pbl=10/11 : New scheme M2 and N2 explicit and dissiptation exact |
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43 | ! iflag_pbl=12 = 11 with vertical diffusion off q2 |
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44 | ! |
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45 | ! 2013/04/01 (FH hourdin@lmd.jussieu.fr) |
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46 | ! Correction for very stable PBLs (iflag_pbl=10 and 11) |
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47 | ! iflag_pbl=8 converges numerically with NPv3.1 |
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48 | ! iflag_pbl=11 -> the model starts with NP from start files created by ce0l |
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49 | ! -> the model can run with longer time-steps. |
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50 | !....................................................................... |
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51 | |
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52 | REAL, DIMENSION(klon,klev) :: d_u,d_v,d_t |
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53 | REAL, DIMENSION(klon,klev) :: pu,pv,pt |
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54 | REAL, DIMENSION(klon,klev) :: d_t_diss |
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55 | |
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56 | REAL timestep |
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57 | real plev(klon,klev+1) |
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58 | real play(klon,klev) |
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59 | real ustar(klon) |
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60 | real kmin,qmin,pblhmin(klon),coriol(klon) |
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61 | REAL zlev(klon,klev+1) |
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62 | REAL zlay(klon,klev) |
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63 | REAL zu(klon,klev) |
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64 | REAL zv(klon,klev) |
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65 | REAL zt(klon,klev) |
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66 | REAL teta(klon,klev) |
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67 | REAL cd(klon) |
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68 | REAL q2(klon,klev+1),qpre |
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69 | REAL unsdz(klon,klev) |
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70 | REAL unsdzdec(klon,klev+1) |
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71 | |
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72 | REAL km(klon,klev) |
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73 | REAL kmpre(klon,klev+1),tmp2 |
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74 | REAL mpre(klon,klev+1) |
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75 | REAL kn(klon,klev) |
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76 | REAL kq(klon,klev) |
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77 | real ff(klon,klev+1),delta(klon,klev+1) |
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78 | real aa(klon,klev+1),aa0,aa1 |
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79 | integer iflag_pbl,ngrid |
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80 | integer nlay,nlev |
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81 | |
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82 | logical first |
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83 | integer ipas |
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84 | save first,ipas |
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85 | !FH/IM data first,ipas/.true.,0/ |
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86 | data first,ipas/.false.,0/ |
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87 | !$OMP THREADPRIVATE( first,ipas) |
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88 | INTEGER, SAVE :: iflag_tke_diff=0 |
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89 | !$OMP THREADPRIVATE(iflag_tke_diff) |
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90 | |
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91 | |
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92 | integer ig,k |
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93 | |
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94 | |
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95 | real ri,zrif,zalpha,zsm,zsn |
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96 | real rif(klon,klev+1),sm(klon,klev+1),alpha(klon,klev) |
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97 | |
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98 | real m2(klon,klev+1),dz(klon,klev+1),zq,n2(klon,klev+1) |
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99 | REAL, DIMENSION(klon,klev+1) :: km2,kn2,sqrtq |
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100 | real dtetadz(klon,klev+1) |
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101 | real m2cstat,mcstat,kmcstat |
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102 | real l(klon,klev+1) |
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103 | real leff(klon,klev+1) |
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104 | real,allocatable,save :: l0(:) |
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105 | !$OMP THREADPRIVATE(l0) |
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106 | real sq(klon),sqz(klon),zz(klon,klev+1) |
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107 | integer iter |
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108 | |
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109 | real ric,rifc,b1,kap |
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110 | save ric,rifc,b1,kap |
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111 | data ric,rifc,b1,kap/0.195,0.191,16.6,0.4/ |
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112 | !$OMP THREADPRIVATE(ric,rifc,b1,kap) |
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113 | real frif,falpha,fsm |
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114 | real fl,zzz,zl0,zq2,zn2 |
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115 | |
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116 | real rino(klon,klev+1),smyam(klon,klev),styam(klon,klev) |
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117 | real lyam(klon,klev),knyam(klon,klev) |
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118 | real w2yam(klon,klev),t2yam(klon,klev) |
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119 | logical,save :: firstcall=.true. |
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120 | !$OMP THREADPRIVATE(firstcall) |
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121 | CHARACTER(len=20),PARAMETER :: modname="yamada_c" |
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122 | REAL, DIMENSION(klon,klev+1) :: fluxu,fluxv,fluxt |
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123 | REAL, DIMENSION(klon,klev+1) :: dddu,dddv,dddt |
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124 | REAL, DIMENSION(klon,klev) :: exner,masse |
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125 | REAL, DIMENSION(klon,klev+1) :: masseb,q2old,q2neg |
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126 | LOGICAL okiophys |
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127 | |
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128 | frif(ri)=0.6588*(ri+0.1776-sqrt(ri*ri-0.3221*ri+0.03156)) |
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129 | falpha(ri)=1.318*(0.2231-ri)/(0.2341-ri) |
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130 | fsm(ri)=1.96*(0.1912-ri)*(0.2341-ri)/((1.-ri)*(0.2231-ri)) |
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131 | fl(zzz,zl0,zq2,zn2)= & |
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132 | & max(min(l0(ig)*kap*zlev(ig,k)/(kap*zlev(ig,k)+l0(ig)) & |
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133 | & ,0.5*sqrt(q2(ig,k))/sqrt(max(n2(ig,k),1.e-10))) ,1.) |
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134 | |
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135 | |
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136 | okiophys=klon==1 |
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137 | if (firstcall) then |
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138 | CALL getin_p('iflag_tke_diff',iflag_tke_diff) |
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139 | allocate(l0(klon)) |
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140 | #define IOPHYS |
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141 | #ifdef IOPHYS |
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142 | ! call iophys_ini(timestep) |
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143 | #endif |
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144 | firstcall=.false. |
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145 | endif |
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146 | |
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147 | IF (ngrid<=0) RETURN ! Bizarre : on n a pas ce probeleme pour coef_diff_turb |
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148 | |
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149 | #ifdef IOPHYS |
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150 | if (okiophys) then |
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151 | call iophys_ecrit('q2i',klev,'q2 debut my','m2/s2',q2(:,1:klev)) |
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152 | call iophys_ecrit('kmi',klev,'Kz debut my','m/s2',km(:,1:klev)) |
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153 | endif |
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154 | #endif |
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155 | |
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156 | nlay=klev |
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157 | nlev=klev+1 |
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158 | |
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159 | |
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160 | !------------------------------------------------------------------------- |
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161 | ! Computation of conservative source terms from the turbulent tendencies |
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162 | !------------------------------------------------------------------------- |
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163 | |
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164 | |
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165 | zalpha=0.5 ! Anciennement 0.5. Essayer de voir pourquoi ? |
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166 | zu(:,:)=pu(:,:)+zalpha*d_u(:,:) |
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167 | zv(:,:)=pv(:,:)+zalpha*d_v(:,:) |
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168 | zt(:,:)=pt(:,:)+zalpha*d_t(:,:) |
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169 | |
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170 | do k=1,klev |
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171 | exner(:,k)=(play(:,k)/plev(:,1))**RKAPPA |
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172 | masse(:,k)=(plev(:,k)-plev(:,k+1))/RG |
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173 | teta(:,k)=zt(:,k)/exner(:,k) |
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174 | enddo |
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175 | |
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176 | ! Atmospheric mass at layer interfaces, where the TKE is computed |
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177 | masseb(:,:)=0. |
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178 | do k=1,klev |
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179 | masseb(:,k)=masseb(:,k)+masse(:,k) |
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180 | masseb(:,k+1)=masseb(:,k+1)+masse(:,k) |
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181 | enddo |
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182 | masseb(:,:)=0.5*masseb(:,:) |
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183 | |
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184 | zlev(:,1)=0. |
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185 | zlay(:,1)=RCPD*teta(:,1)*(1.-exner(:,1)) |
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186 | do k=1,klev-1 |
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187 | zlay(:,k+1)=zlay(:,k)+0.5*RCPD*(teta(:,k)+teta(:,k+1))*(exner(:,k)-exner(:,k+1))/RG |
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188 | zlev(:,k)=0.5*(zlay(:,k)+zlay(:,k+1)) ! PASBO |
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189 | enddo |
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190 | |
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191 | fluxu(:,klev+1)=0. |
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192 | fluxv(:,klev+1)=0. |
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193 | fluxt(:,klev+1)=0. |
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194 | |
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195 | do k=klev,1,-1 |
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196 | fluxu(:,k)=fluxu(:,k+1)+masse(:,k)*d_u(:,k) |
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197 | fluxv(:,k)=fluxv(:,k+1)+masse(:,k)*d_v(:,k) |
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198 | fluxt(:,k)=fluxt(:,k+1)+masse(:,k)*d_t(:,k)/exner(:,k) ! Flux de theta |
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199 | enddo |
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200 | |
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201 | dddu(:,1)=2*zu(:,1)*fluxu(:,1) |
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202 | dddv(:,1)=2*zv(:,1)*fluxv(:,1) |
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203 | dddt(:,1)=(exner(:,1)-1.)*fluxt(:,1) |
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204 | |
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205 | do k=2,klev |
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206 | dddu(:,k)=(zu(:,k)-zu(:,k-1))*fluxu(:,k) |
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207 | dddv(:,k)=(zv(:,k)-zv(:,k-1))*fluxv(:,k) |
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208 | dddt(:,k)=(exner(:,k)-exner(:,k-1))*fluxt(:,k) |
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209 | enddo |
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210 | dddu(:,klev+1)=0. |
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211 | dddv(:,klev+1)=0. |
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212 | dddt(:,klev+1)=0. |
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213 | |
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214 | #ifdef IOPHYS |
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215 | if (okiophys) then |
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216 | call iophys_ecrit('zlay',klev,'Geop','m',zlay) |
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217 | call iophys_ecrit('teta',klev,'teta','K',teta) |
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218 | call iophys_ecrit('temp',klev,'temp','K',zt) |
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219 | call iophys_ecrit('pt',klev,'temp','K',pt) |
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220 | call iophys_ecrit('pu',klev,'u','m/s',pu) |
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221 | call iophys_ecrit('pv',klev,'v','m/s',pv) |
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222 | call iophys_ecrit('d_u',klev,'d_u','m/s2',d_u) |
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223 | call iophys_ecrit('d_v',klev,'d_v','m/s2',d_v) |
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224 | call iophys_ecrit('d_t',klev,'d_t','K/s',d_t) |
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225 | call iophys_ecrit('exner',klev,'exner','',exner) |
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226 | call iophys_ecrit('masse',klev,'masse','',masse) |
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227 | call iophys_ecrit('masseb',klev,'masseb','',masseb) |
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228 | endif |
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229 | #endif |
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230 | |
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231 | |
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232 | |
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233 | ipas=ipas+1 |
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234 | |
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235 | |
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236 | !....................................................................... |
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237 | ! les increments verticaux |
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238 | !....................................................................... |
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239 | ! |
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240 | !!!!!! allerte !!!!!c |
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241 | !!!!!! zlev n'est pas declare a nlev !!!!!c |
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242 | !!!!!! ----> |
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243 | DO ig=1,ngrid |
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244 | zlev(ig,nlev)=zlay(ig,nlay) & |
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245 | & +( zlay(ig,nlay) - zlev(ig,nlev-1) ) |
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246 | ENDDO |
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247 | !!!!!! <---- |
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248 | !!!!!! allerte !!!!!c |
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249 | ! |
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250 | DO k=1,nlay |
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251 | DO ig=1,ngrid |
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252 | unsdz(ig,k)=1.E+0/(zlev(ig,k+1)-zlev(ig,k)) |
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253 | ENDDO |
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254 | ENDDO |
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255 | DO ig=1,ngrid |
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256 | unsdzdec(ig,1)=1.E+0/(zlay(ig,1)-zlev(ig,1)) |
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257 | ENDDO |
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258 | DO k=2,nlay |
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259 | DO ig=1,ngrid |
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260 | unsdzdec(ig,k)=1.E+0/(zlay(ig,k)-zlay(ig,k-1)) |
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261 | ENDDO |
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262 | ENDDO |
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263 | DO ig=1,ngrid |
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264 | unsdzdec(ig,nlay+1)=1.E+0/(zlev(ig,nlay+1)-zlay(ig,nlay)) |
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265 | ENDDO |
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266 | ! |
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267 | !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! |
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268 | ! Computing M^2, N^2, Richardson numbers, stability functions |
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269 | !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! |
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270 | |
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271 | |
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272 | do k=2,klev |
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273 | do ig=1,ngrid |
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274 | dz(ig,k)=zlay(ig,k)-zlay(ig,k-1) |
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275 | m2(ig,k)=((zu(ig,k)-zu(ig,k-1))**2+(zv(ig,k)-zv(ig,k-1))**2)/(dz(ig,k)*dz(ig,k)) |
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276 | dtetadz(ig,k)=(teta(ig,k)-teta(ig,k-1))/dz(ig,k) |
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277 | n2(ig,k)=RG*2.*dtetadz(ig,k)/(teta(ig,k-1)+teta(ig,k)) |
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278 | ! n2(ig,k)=0. |
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279 | ri=n2(ig,k)/max(m2(ig,k),1.e-10) |
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280 | if (ri.lt.ric) then |
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281 | rif(ig,k)=frif(ri) |
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282 | else |
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283 | rif(ig,k)=rifc |
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284 | endif |
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285 | if(rif(ig,k)<0.16) then |
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286 | alpha(ig,k)=falpha(rif(ig,k)) |
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287 | sm(ig,k)=fsm(rif(ig,k)) |
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288 | else |
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289 | alpha(ig,k)=1.12 |
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290 | sm(ig,k)=0.085 |
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291 | endif |
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292 | zz(ig,k)=b1*m2(ig,k)*(1.-rif(ig,k))*sm(ig,k) |
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293 | enddo |
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294 | enddo |
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295 | |
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296 | |
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297 | |
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298 | !==================================================================== |
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299 | ! Computing the mixing length |
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300 | !==================================================================== |
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301 | |
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302 | ! Mise a jour de l0 |
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303 | if (iflag_pbl==8.or.iflag_pbl==10) then |
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304 | |
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305 | !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! |
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306 | ! Iterative computation of l0 |
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307 | ! This version is kept for iflag_pbl only for convergence |
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308 | ! with NPv3.1 Cmip5 simulations |
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309 | !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! |
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310 | |
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311 | do ig=1,ngrid |
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312 | sq(ig)=1.e-10 |
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313 | sqz(ig)=1.e-10 |
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314 | enddo |
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315 | do k=2,klev-1 |
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316 | do ig=1,ngrid |
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317 | zq=sqrt(q2(ig,k)) |
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318 | sqz(ig)=sqz(ig)+zq*zlev(ig,k)*(zlay(ig,k)-zlay(ig,k-1)) |
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319 | sq(ig)=sq(ig)+zq*(zlay(ig,k)-zlay(ig,k-1)) |
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320 | enddo |
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321 | enddo |
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322 | do ig=1,ngrid |
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323 | l0(ig)=0.2*sqz(ig)/sq(ig) |
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324 | enddo |
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325 | do k=2,klev |
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326 | do ig=1,ngrid |
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327 | l(ig,k)=fl(zlev(ig,k),l0(ig),q2(ig,k),n2(ig,k)) |
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328 | enddo |
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329 | enddo |
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330 | ! print*,'L0 cas 8 ou 10 ',l0 |
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331 | |
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332 | else |
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333 | |
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334 | !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! |
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335 | ! In all other case, the assymptotic mixing length l0 is imposed (100m) |
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336 | !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! |
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337 | |
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338 | l0(:)=150. |
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339 | do k=2,klev |
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340 | do ig=1,ngrid |
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341 | l(ig,k)=fl(zlev(ig,k),l0(ig),q2(ig,k),n2(ig,k)) |
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342 | enddo |
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343 | enddo |
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344 | ! print*,'L0 cas autres ',l0 |
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345 | |
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346 | endif |
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347 | |
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348 | |
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349 | #ifdef IOPHYS |
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350 | if (okiophys) then |
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351 | call iophys_ecrit('rif',klev,'Flux Richardson','m',rif(:,1:klev)) |
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352 | call iophys_ecrit('m2',klev,'m2 ','m/s',m2(:,1:klev)) |
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353 | call iophys_ecrit('Km2app',klev,'m2 conserv','m/s',km(:,1:klev)*m2(:,1:klev)) |
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354 | call iophys_ecrit('Km',klev,'Km','m2/s',km(:,1:klev)) |
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355 | endif |
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356 | #endif |
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357 | |
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358 | |
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359 | IF (iflag_pbl<20) then |
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360 | ! For diagnostics only |
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361 | RETURN |
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362 | |
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363 | ELSE |
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364 | |
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365 | ! print*,'OK1' |
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366 | |
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367 | ! Evolution of TKE under source terms K M2 and K N2 |
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368 | leff(:,:)=max(l(:,:),1.) |
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369 | |
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370 | !################################################################## |
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371 | !# IF (iflag_pbl==29) THEN |
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372 | !# STOP'Ne pas utiliser iflag_pbl=29' |
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373 | !# km2(:,:)=km(:,:)*m2(:,:) |
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374 | !# kn2(:,:)=kn2(:,:)*rif(:,:) |
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375 | !# ELSEIF (iflag_pbl==25) THEN |
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376 | ! VERSION AVEC LA TKE EN MILIEU DE COUCHE |
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377 | !# STOP'Ne pas utiliser iflag_pbl=25' |
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378 | !# DO k=1,klev |
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379 | !# km2(:,k)=-0.5*(dddu(:,k)+dddv(:,k)+dddu(:,k+1)+dddv(:,k+1)) & |
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380 | !# & /(masse(:,k)*timestep) |
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381 | !# kn2(:,k)=rcpd*0.5*(dddt(:,k)+dddt(:,k+1))/(masse(:,k)*timestep) |
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382 | !# leff(:,k)=0.5*(leff(:,k)+leff(:,k+1)) |
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383 | !# ENDDO |
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384 | !# km2(:,klev+1)=0. ; kn2(:,klev+1)=0. |
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385 | !# ELSE |
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386 | !################################################################# |
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387 | |
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388 | km2(:,:)=-(dddu(:,:)+dddv(:,:))/(masseb(:,:)*timestep) |
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389 | kn2(:,:)=rcpd*dddt(:,:)/(masseb(:,:)*timestep) |
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390 | ! ENDIF |
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391 | q2neg(:,:)=q2(:,:)+timestep*(km2(:,:)-kn2(:,:)) |
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392 | q2(:,:)=min(max(q2neg(:,:),1.e-10),1.e4) |
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393 | |
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394 | |
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395 | #ifdef IOPHYS |
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396 | if (okiophys) then |
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397 | call iophys_ecrit('km2',klev,'m2 conserv','m/s',km2(:,1:klev)) |
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398 | call iophys_ecrit('kn2',klev,'n2 conserv','m/s',kn2(:,1:klev)) |
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399 | endif |
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400 | #endif |
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401 | |
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402 | ! Dissipation of TKE |
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403 | q2old(:,:)=q2(:,:) |
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404 | q2(:,:)=1./(1./sqrt(q2(:,:))+timestep/(2*leff(:,:)*b1)) |
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405 | q2(:,:)=q2(:,:)*q2(:,:) |
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406 | ! IF (iflag_pbl<=24) THEN |
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407 | DO k=1,klev |
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408 | d_t_diss(:,k)=(masseb(:,k)*(q2neg(:,k)-q2(:,k))+masseb(:,k+1)*(q2neg(:,k+1)-q2(:,k+1)))/(2.*rcpd*masse(:,k)) |
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409 | ENDDO |
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410 | |
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411 | !################################################################### |
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412 | ! ELSE IF (iflag_pbl<=27) THEN |
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413 | ! DO k=1,klev |
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414 | ! d_t_diss(:,k)=(q2neg(:,k)-q2(:,k))/rcpd |
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415 | ! ENDDO |
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416 | ! ENDIF |
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417 | ! print*,'iflag_pbl ',d_t_diss |
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418 | !################################################################### |
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419 | |
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420 | |
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421 | ! Compuation of stability functions |
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422 | ! IF (iflag_pbl/=29) THEN |
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423 | DO k=1,klev |
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424 | DO ig=1,ngrid |
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425 | IF (ABS(km2(ig,k))<=1.e-20) THEN |
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426 | rif(ig,k)=0. |
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427 | ELSE |
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428 | rif(ig,k)=min(kn2(ig,k)/km2(ig,k),rifc) |
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429 | ENDIF |
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430 | IF (rif(ig,k).lt.0.16) THEN |
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431 | alpha(ig,k)=falpha(rif(ig,k)) |
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432 | sm(ig,k)=fsm(rif(ig,k)) |
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433 | else |
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434 | alpha(ig,k)=1.12 |
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435 | sm(ig,k)=0.085 |
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436 | endif |
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437 | ENDDO |
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438 | ENDDO |
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439 | ! ENDIF |
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440 | |
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441 | ! Computation of turbulent diffusivities |
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442 | ! IF (25<=iflag_pbl.and.iflag_pbl<=28) THEN |
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443 | ! DO k=2,klev |
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444 | ! sqrtq(:,k)=sqrt(0.5*(q2(:,k)+q2(:,k-1))) |
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445 | ! ENDDO |
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446 | ! ELSE |
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447 | kq(:,:)=0. |
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448 | DO k=1,klev |
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449 | ! Coefficient au milieu des couches pour diffuser la TKE |
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450 | kq(:,k)=0.5*leff(:,k)*sqrt(q2(:,k))*0.2 |
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451 | ENDDO |
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452 | |
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453 | #ifdef IOPHYS |
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454 | if (okiophys) then |
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455 | call iophys_ecrit('q2b',klev,'KTE inter','m2/s',q2(:,1:klev)) |
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456 | endif |
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457 | #endif |
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458 | |
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459 | IF (iflag_tke_diff==1) THEN |
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460 | CALL vdif_q2(timestep, RG, RD, ngrid, plev, pt, kq, q2) |
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461 | ENDIF |
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462 | |
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463 | km(:,:)=0. |
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464 | kn(:,:)=0. |
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465 | DO k=1,klev |
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466 | km(:,k)=leff(:,k)*sqrt(q2(:,k))*sm(:,k) |
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467 | kn(:,k)=km(:,k)*alpha(:,k) |
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468 | ENDDO |
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469 | |
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470 | |
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471 | #ifdef IOPHYS |
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472 | if (okiophys) then |
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473 | call iophys_ecrit('mixingl',klev,'Mixing length','m',leff(:,1:klev)) |
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474 | call iophys_ecrit('rife',klev,'Flux Richardson','m',rif(:,1:klev)) |
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475 | call iophys_ecrit('q2f',klev,'KTE finale','m2/s',q2(:,1:klev)) |
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476 | call iophys_ecrit('q2neg',klev,'KTE non bornee','m2/s',q2neg(:,1:klev)) |
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477 | call iophys_ecrit('alpha',klev,'alpha','',alpha(:,1:klev)) |
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478 | call iophys_ecrit('sm',klev,'sm','',sm(:,1:klev)) |
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479 | call iophys_ecrit('q2f',klev,'KTE finale','m2/s',q2(:,1:klev)) |
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480 | call iophys_ecrit('kmf',klev,'Kz final','m2/s',km(:,1:klev)) |
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481 | call iophys_ecrit('knf',klev,'Kz final','m2/s',kn(:,1:klev)) |
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482 | call iophys_ecrit('kqf',klev,'Kz final','m2/s',kq(:,1:klev)) |
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483 | endif |
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484 | #endif |
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485 | |
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486 | |
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487 | ENDIF |
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488 | |
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489 | |
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490 | ! print*,'OK2' |
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491 | RETURN |
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492 | END SUBROUTINE yamada_c |
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