1 | ! |
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2 | ! $Id: acama_gwd_rando_m.F90 3977 2021-08-25 17:24:20Z nfevrier $ |
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3 | ! |
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4 | module ACAMA_GWD_rando_m |
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5 | |
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6 | implicit none |
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7 | |
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8 | contains |
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9 | |
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10 | SUBROUTINE ACAMA_GWD_rando(DTIME, pp, plat, tt, uu, vv, rot, & |
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11 | zustr, zvstr, d_u, d_v,east_gwstress,west_gwstress) |
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12 | |
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13 | ! Parametrization of the momentum flux deposition due to a discrete |
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14 | ! number of gravity waves. |
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15 | ! Author: F. Lott, A. de la Camara |
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16 | ! July, 24th, 2014 |
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17 | ! Gaussian distribution of the source, source is vorticity squared |
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18 | ! Reference: de la Camara and Lott (GRL, 2015, vol 42, 2071-2078 ) |
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19 | ! Lott et al (JAS, 2010, vol 67, page 157-170) |
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20 | ! Lott et al (JAS, 2012, vol 69, page 2134-2151) |
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21 | |
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22 | ! ONLINE: |
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23 | use dimphy, only: klon, klev |
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24 | use assert_m, only: assert |
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25 | USE ioipsl_getin_p_mod, ONLY : getin_p |
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26 | USE vertical_layers_mod, ONLY : presnivs |
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27 | |
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28 | include "YOMCST.h" |
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29 | include "clesphys.h" |
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30 | ! OFFLINE: |
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31 | ! include "dimensions.h" |
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32 | ! include "dimphy.h" |
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33 | !END DIFFERENCE |
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34 | include "YOEGWD.h" |
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35 | |
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36 | ! 0. DECLARATIONS: |
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37 | |
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38 | ! 0.1 INPUTS |
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39 | REAL, intent(in)::DTIME ! Time step of the Physics |
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40 | REAL, intent(in):: PP(:, :) ! (KLON, KLEV) Pressure at full levels |
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41 | REAL, intent(in):: ROT(:,:) ! Relative vorticity |
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42 | REAL, intent(in):: TT(:, :) ! (KLON, KLEV) Temp at full levels |
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43 | REAL, intent(in):: UU(:, :) ! (KLON, KLEV) Zonal wind at full levels |
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44 | REAL, intent(in):: VV(:, :) ! (KLON, KLEV) Merid wind at full levels |
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45 | REAL, intent(in):: PLAT(:) ! (KLON) LATITUDE |
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46 | |
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47 | ! 0.2 OUTPUTS |
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48 | REAL, intent(out):: zustr(:), zvstr(:) ! (KLON) Surface Stresses |
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49 | |
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50 | REAL, intent(inout):: d_u(:, :), d_v(:, :) |
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51 | REAL, intent(inout):: east_gwstress(:, :) ! Profile of eastward stress |
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52 | REAL, intent(inout):: west_gwstress(:, :) ! Profile of westward stress |
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53 | ! (KLON, KLEV) tendencies on winds |
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54 | |
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55 | ! O.3 INTERNAL ARRAYS |
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56 | REAL BVLOW(klon) ! LOW LEVEL BV FREQUENCY |
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57 | REAL ROTBA(KLON),CORIO(KLON) ! BAROTROPIC REL. VORTICITY AND PLANETARY |
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58 | REAL UZ(KLON, KLEV + 1) |
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59 | |
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60 | INTEGER II, JJ, LL |
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61 | |
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62 | ! 0.3.0 TIME SCALE OF THE LIFE CYCLE OF THE WAVES PARAMETERIZED |
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63 | |
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64 | REAL DELTAT |
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65 | |
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66 | ! 0.3.1 GRAVITY-WAVES SPECIFICATIONS |
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67 | |
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68 | INTEGER, PARAMETER:: NK = 2, NP = 2, NO = 2, NW = NK * NP * NO |
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69 | INTEGER JK, JP, JO, JW |
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70 | INTEGER, PARAMETER:: NA = 5 !number of realizations to get the phase speed |
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71 | REAL KMIN, KMAX ! Min and Max horizontal wavenumbers |
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72 | REAL CMIN, CMAX ! Min and Max absolute ph. vel. |
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73 | REAL CPHA ! absolute PHASE VELOCITY frequency |
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74 | REAL ZK(NW, KLON) ! Horizontal wavenumber amplitude |
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75 | REAL ZP(NW, KLON) ! Horizontal wavenumber angle |
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76 | REAL ZO(NW, KLON) ! Absolute frequency ! |
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77 | |
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78 | ! Waves Intr. freq. at the 1/2 lev surrounding the full level |
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79 | REAL ZOM(NW, KLON), ZOP(NW, KLON) |
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80 | |
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81 | ! Wave EP-fluxes at the 2 semi levels surrounding the full level |
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82 | REAL WWM(NW, KLON), WWP(NW, KLON) |
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83 | |
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84 | REAL RUW0(NW, KLON) ! Fluxes at launching level |
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85 | |
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86 | REAL RUWP(NW, KLON), RVWP(NW, KLON) |
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87 | ! Fluxes X and Y for each waves at 1/2 Levels |
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88 | |
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89 | INTEGER LAUNCH, LTROP ! Launching altitude and tropo altitude |
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90 | |
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91 | REAL XLAUNCH ! Controle the launching altitude |
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92 | REAL XTROP ! SORT of Tropopause altitude |
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93 | REAL RUW(KLON, KLEV + 1) ! Flux x at semi levels |
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94 | REAL RVW(KLON, KLEV + 1) ! Flux y at semi levels |
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95 | |
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96 | REAL PRMAX ! Maximum value of PREC, and for which our linear formula |
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97 | ! for GWs parameterisation apply |
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98 | |
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99 | ! 0.3.2 PARAMETERS OF WAVES DISSIPATIONS |
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100 | |
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101 | REAL RDISS, ZOISEC ! COEFF DE DISSIPATION, SECURITY FOR INTRINSIC FREQ |
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102 | REAL CORSEC ! SECURITY FOR INTRINSIC CORIOLIS |
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103 | REAL RUWFRT,SATFRT |
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104 | |
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105 | ! 0.3.3 BACKGROUND FLOW AT 1/2 LEVELS AND VERTICAL COORDINATE |
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106 | |
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107 | REAL H0 ! Characteristic Height of the atmosphere |
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108 | REAL DZ ! Characteristic depth of the source! |
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109 | REAL PR, TR ! Reference Pressure and Temperature |
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110 | |
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111 | REAL ZH(KLON, KLEV + 1) ! Log-pressure altitude |
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112 | |
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113 | REAL UH(KLON, KLEV + 1), VH(KLON, KLEV + 1) ! Winds at 1/2 levels |
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114 | REAL PH(KLON, KLEV + 1) ! Pressure at 1/2 levels |
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115 | REAL PSEC ! Security to avoid division by 0 pressure |
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116 | REAL PHM1(KLON, KLEV + 1) ! 1/Press at 1/2 levels |
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117 | REAL BV(KLON, KLEV + 1) ! Brunt Vaisala freq. (BVF) at 1/2 levels |
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118 | REAL BVSEC ! Security to avoid negative BVF |
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119 | |
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120 | REAL, DIMENSION(klev+1) ::HREF |
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121 | LOGICAL, SAVE :: gwd_reproductibilite_mpiomp=.true. |
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122 | LOGICAL, SAVE :: firstcall = .TRUE. |
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123 | !$OMP THREADPRIVATE(firstcall,gwd_reproductibilite_mpiomp) |
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124 | |
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125 | CHARACTER (LEN=20) :: modname='acama_gwd_rando_m' |
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126 | CHARACTER (LEN=80) :: abort_message |
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127 | |
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128 | |
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129 | |
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130 | IF (firstcall) THEN |
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131 | ! Cle introduite pour resoudre un probleme de non reproductibilite |
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132 | ! Le but est de pouvoir tester de revenir a la version precedenete |
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133 | ! A eliminer rapidement |
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134 | CALL getin_p('gwd_reproductibilite_mpiomp',gwd_reproductibilite_mpiomp) |
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135 | IF (NW+4*(NA-1)+NA>=KLEV) THEN |
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136 | abort_message = 'NW+3*NA>=KLEV Probleme pour generation des ondes' |
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137 | CALL abort_physic (modname,abort_message,1) |
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138 | ENDIF |
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139 | firstcall=.false. |
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140 | ! CALL iophys_ini(dtime) |
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141 | ENDIF |
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142 | |
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143 | !----------------------------------------------------------------- |
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144 | |
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145 | ! 1. INITIALISATIONS |
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146 | |
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147 | ! 1.1 Basic parameter |
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148 | |
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149 | ! Are provided from elsewhere (latent heat of vaporization, dry |
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150 | ! gaz constant for air, gravity constant, heat capacity of dry air |
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151 | ! at constant pressure, earth rotation rate, pi). |
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152 | |
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153 | ! 1.2 Tuning parameters of V14 |
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154 | |
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155 | ! Values for linear in rot (recommended): |
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156 | ! RUWFRT=0.005 ! As RUWMAX but for frontal waves |
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157 | ! SATFRT=1.00 ! As SAT but for frontal waves |
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158 | ! Values when rot^2 is used |
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159 | ! RUWFRT=0.02 ! As RUWMAX but for frontal waves |
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160 | ! SATFRT=1.00 ! As SAT but for frontal waves |
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161 | ! CMAX = 30. ! Characteristic phase speed |
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162 | ! Values when rot^2*EXP(-pi*sqrt(J)) is used |
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163 | ! RUWFRT=2.5 ! As RUWMAX but for frontal waves ~ N0*F0/4*DZ |
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164 | ! SATFRT=0.60 ! As SAT but for frontal waves |
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165 | RUWFRT=gwd_front_ruwmax |
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166 | SATFRT=gwd_front_sat |
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167 | CMAX = 50. ! Characteristic phase speed |
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168 | ! Phase speed test |
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169 | ! RUWFRT=0.01 |
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170 | ! CMAX = 50. ! Characteristic phase speed (TEST) |
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171 | ! Values when rot^2 and exp(-m^2*dz^2) are used |
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172 | ! RUWFRT=0.03 ! As RUWMAX but for frontal waves |
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173 | ! SATFRT=1.00 ! As SAT but for frontal waves |
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174 | ! CRUCIAL PARAMETERS FOR THE WIND FILTERING |
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175 | XLAUNCH=0.95 ! Parameter that control launching altitude |
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176 | RDISS = 0.5 ! Diffusion parameter |
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177 | |
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178 | ! maximum of rain for which our theory applies (in kg/m^2/s) |
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179 | |
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180 | DZ = 1000. ! Characteristic depth of the source |
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181 | XTROP=0.2 ! Parameter that control tropopause altitude |
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182 | DELTAT=24.*3600. ! Time scale of the waves (first introduced in 9b) |
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183 | ! DELTAT=DTIME ! No AR-1 Accumulation, OR OFFLINE |
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184 | |
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185 | KMIN = 2.E-5 |
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186 | ! minimum horizontal wavenumber (inverse of the subgrid scale resolution) |
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187 | |
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188 | KMAX = 1.E-3 ! Max horizontal wavenumber |
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189 | CMIN = 1. ! Min phase velocity |
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190 | |
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191 | TR = 240. ! Reference Temperature |
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192 | PR = 101300. ! Reference pressure |
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193 | H0 = RD * TR / RG ! Characteristic vertical scale height |
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194 | |
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195 | BVSEC = 5.E-3 ! Security to avoid negative BVF |
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196 | PSEC = 1.E-6 ! Security to avoid division by 0 pressure |
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197 | ZOISEC = 1.E-6 ! Security FOR 0 INTRINSIC FREQ |
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198 | CORSEC = ROMEGA*2.*SIN(2.*RPI/180.)! Security for CORIO |
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199 | |
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200 | ! ONLINE |
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201 | call assert(klon == (/size(pp, 1), size(tt, 1), size(uu, 1), & |
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202 | size(vv, 1), size(rot,1), size(zustr), size(zvstr), size(d_u, 1), & |
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203 | size(d_v, 1), & |
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204 | size(east_gwstress,1), size(west_gwstress,1) /), & |
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205 | "ACAMA_GWD_RANDO klon") |
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206 | call assert(klev == (/size(pp, 2), size(tt, 2), size(uu, 2), & |
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207 | size(vv, 2), size(d_u, 2), size(d_v, 2), & |
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208 | size(east_gwstress,2), size(west_gwstress,2) /), & |
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209 | "ACAMA_GWD_RANDO klev") |
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210 | ! END ONLINE |
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211 | |
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212 | IF(DELTAT < DTIME)THEN |
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213 | ! PRINT *, 'flott_gwd_rando: deltat < dtime!' |
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214 | ! STOP 1 |
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215 | abort_message=' deltat < dtime! ' |
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216 | CALL abort_physic(modname,abort_message,1) |
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217 | ENDIF |
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218 | |
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219 | IF (KLEV < NW) THEN |
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220 | ! PRINT *, 'flott_gwd_rando: you will have problem with random numbers' |
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221 | ! STOP 1 |
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222 | abort_message=' you will have problem with random numbers' |
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223 | CALL abort_physic(modname,abort_message,1) |
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224 | ENDIF |
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225 | |
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226 | ! 2. EVALUATION OF THE BACKGROUND FLOW AT SEMI-LEVELS |
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227 | |
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228 | ! Pressure and Inv of pressure |
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229 | DO LL = 2, KLEV |
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230 | PH(:, LL) = EXP((LOG(PP(:, LL)) + LOG(PP(:, LL - 1))) / 2.) |
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231 | PHM1(:, LL) = 1. / PH(:, LL) |
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232 | end DO |
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233 | |
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234 | PH(:, KLEV + 1) = 0. |
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235 | PHM1(:, KLEV + 1) = 1. / PSEC |
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236 | PH(:, 1) = 2. * PP(:, 1) - PH(:, 2) |
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237 | |
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238 | ! Launching altitude |
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239 | |
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240 | IF (gwd_reproductibilite_mpiomp) THEN |
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241 | ! Reprend la formule qui calcule PH en fonction de PP=play |
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242 | DO LL = 2, KLEV |
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243 | HREF(LL) = EXP((LOG(presnivs(LL)) + LOG(presnivs(LL - 1))) / 2.) |
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244 | end DO |
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245 | HREF(KLEV + 1) = 0. |
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246 | HREF(1) = 2. * presnivs(1) - HREF(2) |
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247 | ELSE |
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248 | HREF(1:KLEV)=PH(KLON/2,1:KLEV) |
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249 | ENDIF |
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250 | |
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251 | LAUNCH=0 |
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252 | LTROP =0 |
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253 | DO LL = 1, KLEV |
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254 | IF (HREF(LL) / HREF(1) > XLAUNCH) LAUNCH = LL |
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255 | ENDDO |
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256 | DO LL = 1, KLEV |
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257 | IF (HREF(LL) / HREF(1) > XTROP) LTROP = LL |
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258 | ENDDO |
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259 | !LAUNCH=22 ; LTROP=33 |
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260 | ! print*,'LAUNCH=',LAUNCH,'LTROP=',LTROP |
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261 | |
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262 | |
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263 | ! PRINT *,'LAUNCH IN ACAMARA:',LAUNCH |
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264 | |
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265 | ! Log pressure vert. coordinate |
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266 | DO LL = 1, KLEV + 1 |
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267 | ZH(:, LL) = H0 * LOG(PR / (PH(:, LL) + PSEC)) |
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268 | end DO |
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269 | |
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270 | ! BV frequency |
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271 | DO LL = 2, KLEV |
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272 | ! BVSEC: BV Frequency (UH USED IS AS A TEMPORARY ARRAY DOWN TO WINDS) |
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273 | UH(:, LL) = 0.5 * (TT(:, LL) + TT(:, LL - 1)) & |
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274 | * RD**2 / RCPD / H0**2 + (TT(:, LL) & |
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275 | - TT(:, LL - 1)) / (ZH(:, LL) - ZH(:, LL - 1)) * RD / H0 |
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276 | end DO |
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277 | BVLOW = 0.5 * (TT(:, LTROP )+ TT(:, LAUNCH)) & |
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278 | * RD**2 / RCPD / H0**2 + (TT(:, LTROP ) & |
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279 | - TT(:, LAUNCH))/(ZH(:, LTROP )- ZH(:, LAUNCH)) * RD / H0 |
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280 | |
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281 | UH(:, 1) = UH(:, 2) |
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282 | UH(:, KLEV + 1) = UH(:, KLEV) |
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283 | BV(:, 1) = UH(:, 2) |
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284 | BV(:, KLEV + 1) = UH(:, KLEV) |
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285 | ! SMOOTHING THE BV HELPS |
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286 | DO LL = 2, KLEV |
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287 | BV(:, LL)=(UH(:, LL+1)+2.*UH(:, LL)+UH(:, LL-1))/4. |
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288 | end DO |
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289 | |
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290 | BV=MAX(SQRT(MAX(BV, 0.)), BVSEC) |
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291 | BVLOW=MAX(SQRT(MAX(BVLOW, 0.)), BVSEC) |
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292 | |
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293 | ! WINDS |
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294 | DO LL = 2, KLEV |
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295 | UH(:, LL) = 0.5 * (UU(:, LL) + UU(:, LL - 1)) ! Zonal wind |
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296 | VH(:, LL) = 0.5 * (VV(:, LL) + VV(:, LL - 1)) ! Meridional wind |
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297 | UZ(:, LL) = ABS((SQRT(UU(:, LL)**2+VV(:, LL)**2) & |
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298 | - SQRT(UU(:,LL-1)**2+VV(:, LL-1)**2)) & |
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299 | /(ZH(:, LL)-ZH(:, LL-1)) ) |
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300 | end DO |
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301 | UH(:, 1) = 0. |
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302 | VH(:, 1) = 0. |
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303 | UH(:, KLEV + 1) = UU(:, KLEV) |
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304 | VH(:, KLEV + 1) = VV(:, KLEV) |
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305 | |
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306 | UZ(:, 1) = UZ(:, 2) |
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307 | UZ(:, KLEV + 1) = UZ(:, KLEV) |
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308 | UZ(:, :) = MAX(UZ(:,:), PSEC) |
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309 | |
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310 | ! BAROTROPIC VORTICITY AND INTEGRATED CORIOLIS PARAMETER |
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311 | |
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312 | CORIO(:) = MAX(ROMEGA*2.*ABS(SIN(PLAT(:)*RPI/180.)),CORSEC) |
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313 | ROTBA(:)=0. |
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314 | DO LL = 1,KLEV-1 |
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315 | !ROTBA(:) = ROTBA(:) + (ROT(:,LL)+ROT(:,LL+1))/2./RG*(PP(:,LL)-PP(:,LL+1)) |
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316 | ! Introducing the complete formula (exp of Richardson number): |
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317 | ROTBA(:) = ROTBA(:) + & |
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318 | !((ROT(:,LL)+ROT(:,LL+1))/2.)**2 & |
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319 | (CORIO(:)*TANH(ABS(ROT(:,LL)+ROT(:,LL+1))/2./CORIO(:)))**2 & |
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320 | /RG*(PP(:,LL)-PP(:,LL+1)) & |
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321 | * EXP(-RPI*BV(:,LL+1)/UZ(:,LL+1)) & |
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322 | ! * DZ*BV(:,LL+1)/4./ABS(CORIO(:)) |
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323 | * DZ*BV(:,LL+1)/4./1.E-4 ! Changes after 1991 |
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324 | !ARRET |
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325 | ENDDO |
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326 | ! PRINT *,'MAX ROTBA:',MAXVAL(ROTBA) |
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327 | ! ROTBA(:)=(1.*ROTBA(:) & ! Testing zone |
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328 | ! +0.15*CORIO(:)**2 & |
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329 | ! /(COS(PLAT(:)*RPI/180.)+0.02) & |
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330 | ! )*DZ*0.01/0.0001/4. ! & ! Testing zone |
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331 | ! MODIF GWD4 AFTER 1985 |
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332 | ! *(1.25+SIN(PLAT(:)*RPI/180.))/(1.05+SIN(PLAT(:)*RPI/180.))/1.25 |
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333 | ! *1./(COS(PLAT(:)*RPI/180.)+0.02) |
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334 | ! CORIO(:) = MAX(ROMEGA*2.*ABS(SIN(PLAT(:)*RPI/180.)),ZOISEC)/RG*PP(:,1) |
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335 | |
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336 | ! 3 WAVES CHARACTERISTICS CHOSEN RANDOMLY AT THE LAUNCH ALTITUDE |
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337 | |
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338 | ! The mod functions of weird arguments are used to produce the |
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339 | ! waves characteristics in an almost stochastic way |
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340 | |
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341 | JW = 0 |
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342 | DO JW = 1, NW |
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343 | ! Angle |
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344 | DO II = 1, KLON |
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345 | ! Angle (0 or PI so far) |
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346 | ! ZP(JW, II) = (SIGN(1., 0.5 - MOD(TT(II, JW) * 10., 1.)) + 1.) & |
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347 | ! * RPI / 2. |
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348 | ! Angle between 0 and pi |
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349 | ZP(JW, II) = MOD(TT(II, JW) * 10., 1.) * RPI |
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350 | ! TEST WITH POSITIVE WAVES ONLY (Part I/II) |
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351 | ! ZP(JW, II) = 0. |
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352 | ! Horizontal wavenumber amplitude |
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353 | ZK(JW, II) = KMIN + (KMAX - KMIN) * MOD(TT(II, JW) * 100., 1.) |
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354 | ! Horizontal phase speed |
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355 | CPHA = 0. |
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356 | DO JJ = 1, NA |
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357 | CPHA = CPHA + & |
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358 | CMAX*2.*(MOD(TT(II, JW+4*(JJ-1)+JJ)**2, 1.)-0.5)*SQRT(3.)/SQRT(NA*1.) |
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359 | END DO |
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360 | IF (CPHA.LT.0.) THEN |
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361 | CPHA = -1.*CPHA |
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362 | ZP(JW,II) = ZP(JW,II) + RPI |
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363 | ! TEST WITH POSITIVE WAVES ONLY (Part II/II) |
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364 | ! ZP(JW, II) = 0. |
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365 | ENDIF |
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366 | CPHA = CPHA + CMIN !we dont allow |c|<1m/s |
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367 | ! Absolute frequency is imposed |
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368 | ZO(JW, II) = CPHA * ZK(JW, II) |
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369 | ! Intrinsic frequency is imposed |
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370 | ZO(JW, II) = ZO(JW, II) & |
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371 | + ZK(JW, II) * COS(ZP(JW, II)) * UH(II, LAUNCH) & |
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372 | + ZK(JW, II) * SIN(ZP(JW, II)) * VH(II, LAUNCH) |
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373 | ! Momentum flux at launch lev |
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374 | ! LAUNCHED RANDOM WAVES WITH LOG-NORMAL AMPLITUDE |
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375 | ! RIGHT IN THE SH (GWD4 after 1990) |
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376 | RUW0(JW, II) = 0. |
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377 | DO JJ = 1, NA |
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378 | RUW0(JW, II) = RUW0(JW,II) + & |
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379 | 2.*(MOD(TT(II, JW+4*(JJ-1)+JJ)**2, 1.)-0.5)*SQRT(3.)/SQRT(NA*1.) |
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380 | END DO |
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381 | RUW0(JW, II) = RUWFRT & |
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382 | * EXP(RUW0(JW,II))/1250. & ! 2 mpa at south pole |
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383 | *((1.05+SIN(PLAT(II)*RPI/180.))/(1.01+SIN(PLAT(II)*RPI/180.))-2.05/2.01) |
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384 | ! RUW0(JW, II) = RUWFRT |
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385 | ENDDO |
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386 | end DO |
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387 | |
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388 | ! 4. COMPUTE THE FLUXES |
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389 | |
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390 | ! 4.0 |
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391 | |
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392 | ! 4.1 Vertical velocity at launching altitude to ensure |
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393 | ! the correct value to the imposed fluxes. |
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394 | |
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395 | DO JW = 1, NW |
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396 | |
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397 | ! Evaluate intrinsic frequency at launching altitude: |
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398 | ZOP(JW, :) = ZO(JW, :) & |
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399 | - ZK(JW, :) * COS(ZP(JW, :)) * UH(:, LAUNCH) & |
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400 | - ZK(JW, :) * SIN(ZP(JW, :)) * VH(:, LAUNCH) |
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401 | |
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402 | ! VERSION WITH FRONTAL SOURCES |
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403 | |
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404 | ! Momentum flux at launch level imposed by vorticity sources |
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405 | |
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406 | ! tanh limitation for values above CORIO (inertial instability). |
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407 | ! WWP(JW, :) = RUW0(JW, :) & |
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408 | WWP(JW, :) = RUWFRT & |
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409 | ! * (CORIO(:)*TANH(ROTBA(:)/CORIO(:)))**2 & |
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410 | ! * ABS((CORIO(:)*TANH(ROTBA(:)/CORIO(:)))*CORIO(:)) & |
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411 | ! CONSTANT FLUX |
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412 | ! * (CORIO(:)*CORIO(:)) & |
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413 | ! MODERATION BY THE DEPTH OF THE SOURCE (DZ HERE) |
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414 | ! *EXP(-BVLOW(:)**2/MAX(ABS(ZOP(JW, :)),ZOISEC)**2 & |
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415 | ! *ZK(JW, :)**2*DZ**2) & |
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416 | ! COMPLETE FORMULA: |
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417 | !* CORIO(:)**2*TANH(ROTBA(:)/CORIO(:)**2) & |
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418 | * ROTBA(:) & |
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419 | ! RESTORE DIMENSION OF A FLUX |
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420 | ! *RD*TR/PR |
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421 | ! *1. + RUW0(JW, :) |
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422 | *1. |
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423 | |
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424 | ! Factor related to the characteristics of the waves: NONE |
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425 | |
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426 | ! Moderation by the depth of the source (dz here): NONE |
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427 | |
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428 | ! Put the stress in the right direction: |
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429 | |
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430 | RUWP(JW, :) = SIGN(1., ZOP(JW, :))*COS(ZP(JW, :)) * WWP(JW, :) |
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431 | RVWP(JW, :) = SIGN(1., ZOP(JW, :))*SIN(ZP(JW, :)) * WWP(JW, :) |
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432 | |
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433 | end DO |
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434 | |
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435 | ! 4.2 Uniform values below the launching altitude |
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436 | |
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437 | DO LL = 1, LAUNCH |
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438 | RUW(:, LL) = 0 |
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439 | RVW(:, LL) = 0 |
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440 | DO JW = 1, NW |
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441 | RUW(:, LL) = RUW(:, LL) + RUWP(JW, :) |
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442 | RVW(:, LL) = RVW(:, LL) + RVWP(JW, :) |
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443 | end DO |
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444 | end DO |
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445 | |
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446 | ! 4.3 Loop over altitudes, with passage from one level to the next |
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447 | ! done by i) conserving the EP flux, ii) dissipating a little, |
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448 | ! iii) testing critical levels, and vi) testing the breaking. |
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449 | |
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450 | DO LL = LAUNCH, KLEV - 1 |
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451 | ! Warning: all the physics is here (passage from one level |
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452 | ! to the next) |
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453 | DO JW = 1, NW |
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454 | ZOM(JW, :) = ZOP(JW, :) |
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455 | WWM(JW, :) = WWP(JW, :) |
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456 | ! Intrinsic Frequency |
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457 | ZOP(JW, :) = ZO(JW, :) - ZK(JW, :) * COS(ZP(JW, :)) * UH(:, LL + 1) & |
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458 | - ZK(JW, :) * SIN(ZP(JW, :)) * VH(:, LL + 1) |
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459 | |
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460 | ! No breaking (Eq.6) |
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461 | ! Dissipation (Eq. 8) |
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462 | WWP(JW, :) = WWM(JW, :) * EXP(- 4. * RDISS * PR / (PH(:, LL + 1) & |
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463 | + PH(:, LL)) * ((BV(:, LL + 1) + BV(:, LL)) / 2.)**3 & |
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464 | / MAX(ABS(ZOP(JW, :) + ZOM(JW, :)) / 2., ZOISEC)**4 & |
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465 | * ZK(JW, :)**3 * (ZH(:, LL + 1) - ZH(:, LL))) |
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466 | |
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467 | ! Critical levels (forced to zero if intrinsic frequency changes sign) |
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468 | ! Saturation (Eq. 12) |
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469 | WWP(JW, :) = min(WWP(JW, :), MAX(0., & |
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470 | SIGN(1., ZOP(JW, :) * ZOM(JW, :))) * ABS(ZOP(JW, :))**3 & |
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471 | ! / BV(:, LL + 1) * EXP(- ZH(:, LL + 1) / H0) * SATFRT**2 * KMIN**2 & |
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472 | / BV(:, LL + 1) * EXP(- ZH(:, LL + 1) / H0) * KMIN**2 & |
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473 | ! *(SATFRT*(2.5+1.5*TANH((ZH(:,LL+1)/H0-8.)/2.)))**2 & |
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474 | *SATFRT**2 & |
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475 | / ZK(JW, :)**4) |
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476 | end DO |
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477 | |
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478 | ! Evaluate EP-flux from Eq. 7 and give the right orientation to |
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479 | ! the stress |
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480 | |
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481 | DO JW = 1, NW |
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482 | RUWP(JW, :) = SIGN(1., ZOP(JW, :))*COS(ZP(JW, :)) * WWP(JW, :) |
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483 | RVWP(JW, :) = SIGN(1., ZOP(JW, :))*SIN(ZP(JW, :)) * WWP(JW, :) |
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484 | end DO |
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485 | |
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486 | RUW(:, LL + 1) = 0. |
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487 | RVW(:, LL + 1) = 0. |
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488 | |
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489 | DO JW = 1, NW |
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490 | RUW(:, LL + 1) = RUW(:, LL + 1) + RUWP(JW, :) |
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491 | RVW(:, LL + 1) = RVW(:, LL + 1) + RVWP(JW, :) |
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492 | EAST_GWSTRESS(:, LL)=EAST_GWSTRESS(:, LL)+MAX(0.,RUWP(JW,:))/FLOAT(NW) |
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493 | WEST_GWSTRESS(:, LL)=WEST_GWSTRESS(:, LL)+MIN(0.,RUWP(JW,:))/FLOAT(NW) |
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494 | end DO |
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495 | end DO |
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496 | |
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497 | ! 5 CALCUL DES TENDANCES: |
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498 | |
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499 | ! 5.1 Rectification des flux au sommet et dans les basses couches |
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500 | |
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501 | RUW(:, KLEV + 1) = 0. |
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502 | RVW(:, KLEV + 1) = 0. |
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503 | RUW(:, 1) = RUW(:, LAUNCH) |
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504 | RVW(:, 1) = RVW(:, LAUNCH) |
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505 | DO LL = 1, LAUNCH |
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506 | RUW(:, LL) = RUW(:, LAUNCH+1) |
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507 | RVW(:, LL) = RVW(:, LAUNCH+1) |
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508 | EAST_GWSTRESS(:, LL)=EAST_GWSTRESS(:, LAUNCH) |
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509 | WEST_GWSTRESS(:, LL)=WEST_GWSTRESS(:, LAUNCH) |
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510 | end DO |
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511 | |
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512 | ! AR-1 RECURSIVE FORMULA (13) IN VERSION 4 |
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513 | DO LL = 1, KLEV |
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514 | D_U(:, LL) = (1.-DTIME/DELTAT) * D_U(:, LL) + DTIME/DELTAT/REAL(NW) * & |
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515 | RG * (RUW(:, LL + 1) - RUW(:, LL)) & |
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516 | / (PH(:, LL + 1) - PH(:, LL)) * DTIME |
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517 | ! NO AR1 FOR MERIDIONAL TENDENCIES |
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518 | ! D_V(:, LL) = (1.-DTIME/DELTAT) * D_V(:, LL) + DTIME/DELTAT/REAL(NW) * & |
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519 | D_V(:, LL) = 1./REAL(NW) * & |
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520 | RG * (RVW(:, LL + 1) - RVW(:, LL)) & |
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521 | / (PH(:, LL + 1) - PH(:, LL)) * DTIME |
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522 | ENDDO |
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523 | |
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524 | ! Cosmetic: evaluation of the cumulated stress |
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525 | ZUSTR = 0. |
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526 | ZVSTR = 0. |
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527 | DO LL = 1, KLEV |
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528 | ZUSTR = ZUSTR + D_U(:, LL) / RG * (PH(:, LL + 1) - PH(:, LL))/DTIME |
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529 | ! ZVSTR = ZVSTR + D_V(:, LL) / RG * (PH(:, LL + 1) - PH(:, LL))/DTIME |
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530 | ENDDO |
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531 | ! COSMETICS TO VISUALIZE ROTBA |
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532 | ZVSTR = ROTBA |
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533 | |
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534 | END SUBROUTINE ACAMA_GWD_RANDO |
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535 | |
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536 | end module ACAMA_GWD_rando_m |
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