| 1 | module cpdet_mod |
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| 2 | |
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| 3 | implicit none |
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| 4 | |
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| 5 | ! ADAPTATION OF GCM TO CP(T) |
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| 6 | !====================================================================== |
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| 7 | ! S. Lebonnois, 10/2010 |
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| 8 | ! |
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| 9 | ! Cp must be computed using cpdet(t) to be valid |
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| 10 | ! |
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| 11 | ! The Exner function is still pk = RCPD*(play/pref)**RKAPPA |
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| 12 | ! (RCPD=cpp, RKAPPA=kappa) |
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| 13 | ! |
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| 14 | ! One goes from T to teta (potential temperature) using t2tpot(t,teta,pk) |
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| 15 | ! One goes from teta to T using tpot2t(teta,t,pk) |
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| 16 | ! |
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| 17 | !====================================================================== |
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| 18 | |
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| 19 | contains |
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| 20 | |
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| 21 | SUBROUTINE ini_cpdet |
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| 22 | |
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| 23 | USE control_mod, ONLY: planet_type |
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| 24 | USE comconst_mod, ONLY: nu_venus,t0_venus |
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| 25 | IMPLICIT none |
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| 26 | !====================================================================== |
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| 27 | ! Initialization of nu_venus and t0_venus |
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| 28 | !====================================================================== |
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| 29 | |
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| 30 | if (planet_type.eq."venus") then |
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| 31 | nu_venus=0.35 |
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| 32 | t0_venus=460. |
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| 33 | else |
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| 34 | nu_venus=0. |
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| 35 | t0_venus=0. |
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| 36 | endif |
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| 37 | |
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| 38 | return |
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| 39 | end subroutine ini_cpdet |
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| 40 | |
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| 41 | !====================================================================== |
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| 42 | !====================================================================== |
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| 43 | |
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| 44 | FUNCTION cpdet(t) |
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| 45 | |
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| 46 | USE control_mod, ONLY: planet_type |
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| 47 | USE comconst_mod, ONLY: cpp,t0_venus,nu_venus |
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| 48 | IMPLICIT none |
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| 49 | |
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| 50 | ! for cpp, nu_venus and t0_venus: |
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| 51 | |
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| 52 | real,intent(in) :: t |
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| 53 | real cpdet |
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| 54 | |
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| 55 | if (planet_type.eq."venus") then |
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| 56 | cpdet = cpp*(t/t0_venus)**nu_venus |
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| 57 | else |
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| 58 | cpdet = cpp |
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| 59 | endif |
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| 60 | |
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| 61 | return |
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| 62 | end function cpdet |
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| 63 | |
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| 64 | !====================================================================== |
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| 65 | !====================================================================== |
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| 66 | |
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| 67 | SUBROUTINE t2tpot(npoints, yt, yteta, ypk) |
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| 68 | !====================================================================== |
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| 69 | ! Arguments: |
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| 70 | ! |
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| 71 | ! yt --------input-R- Temperature |
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| 72 | ! yteta-------output-R- Temperature potentielle |
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| 73 | ! ypk --------input-R- Fonction d'Exner: RCPD*(pplay/pref)**RKAPPA |
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| 74 | ! |
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| 75 | !====================================================================== |
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| 76 | |
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| 77 | USE control_mod, ONLY: planet_type |
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| 78 | USE comconst_mod, ONLY: cpp,t0_venus,nu_venus |
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| 79 | |
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| 80 | IMPLICIT NONE |
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| 81 | |
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| 82 | integer,intent(in) :: npoints |
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| 83 | REAL,intent(in) :: yt(npoints), ypk(npoints) |
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| 84 | REAL,intent(out) :: yteta(npoints) |
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| 85 | |
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| 86 | !---------------------- |
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| 87 | ! ATMOSPHERE PROFONDE |
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| 88 | real ypklim,ypklim2,mmm0 |
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| 89 | real ratio_mod(npoints) |
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| 90 | integer k |
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| 91 | ! theta_mod = theta * ratio_mod => ratio_mod = mmm0/mmm(p) |
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| 92 | |
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| 93 | ypklim = cpp*( 6e6/9.2e6)**0.1914 |
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| 94 | ypklim2 = cpp*(8.9e6/9.2e6)**0.1914 |
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| 95 | mmm0 = 43.44 |
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| 96 | |
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| 97 | DO k = 1, npoints |
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| 98 | ratio_mod(k) = 1. |
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| 99 | ! ATM PROFONDE DESACTIVEE ! |
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| 100 | if ( (1 .EQ. 0) .AND.(ypk(k).gt.ypklim)) then |
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| 101 | ratio_mod(k) = mmm0 / & |
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| 102 | & (mmm0+0.56*(log(ypklim/cpp)-log(ypk(k)/cpp)) & |
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| 103 | & /(log(ypklim/cpp)-log(ypklim2/cpp))) |
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| 104 | ratio_mod(k) = max(ratio_mod(k),mmm0/(mmm0+0.56)) |
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| 105 | endif |
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| 106 | ENDDO |
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| 107 | !---------------------- |
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| 108 | |
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| 109 | if (planet_type.eq."venus") then |
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| 110 | yteta = yt**nu_venus & |
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| 111 | & - nu_venus * t0_venus**nu_venus * log(ypk/cpp) |
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| 112 | yteta = yteta**(1./nu_venus) |
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| 113 | !---------------------- |
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| 114 | ! ATMOSPHERE PROFONDE |
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| 115 | yteta = yteta*ratio_mod |
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| 116 | !---------------------- |
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| 117 | |
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| 118 | else |
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| 119 | yteta = yt * cpp/ypk |
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| 120 | endif |
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| 121 | |
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| 122 | return |
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| 123 | end subroutine t2tpot |
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| 124 | |
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| 125 | !====================================================================== |
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| 126 | !====================================================================== |
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| 127 | |
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| 128 | SUBROUTINE tpot2t(npoints,yteta, yt, ypk) |
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| 129 | !====================================================================== |
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| 130 | ! Arguments: |
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| 131 | ! |
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| 132 | ! yteta--------input-R- Temperature potentielle |
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| 133 | ! yt -------output-R- Temperature |
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| 134 | ! ypk --------input-R- Fonction d'Exner: RCPD*(pplay/pref)**RKAPPA |
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| 135 | ! |
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| 136 | !====================================================================== |
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| 137 | |
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| 138 | USE control_mod, ONLY: planet_type |
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| 139 | USE comconst_mod, ONLY: cpp,nu_venus,t0_venus |
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| 140 | |
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| 141 | IMPLICIT NONE |
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| 142 | |
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| 143 | integer,intent(in) :: npoints |
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| 144 | REAL,intent(in) :: yteta(npoints), ypk(npoints) |
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| 145 | REAL,intent(out) :: yt(npoints) |
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| 146 | |
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| 147 | !---------------------- |
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| 148 | ! ATMOSPHERE PROFONDE |
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| 149 | real ypklim,ypklim2,mmm0 |
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| 150 | real ratio_mod(npoints) |
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| 151 | integer k |
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| 152 | ! theta_mod = theta * ratio_mod => ratio_mod = mmm0/mmm(p) |
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| 153 | |
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| 154 | ypklim = cpp*( 6e6/9.2e6)**0.1914 |
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| 155 | ypklim2 = cpp*(8.9e6/9.2e6)**0.1914 |
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| 156 | mmm0 = 43.44 |
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| 157 | |
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| 158 | DO k = 1, npoints |
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| 159 | ratio_mod(k) = 1. |
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| 160 | ! ATM PROFONDE DESACTIVEE ! |
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| 161 | if ( (1 .EQ. 0) .AND.(ypk(k).gt.ypklim)) then |
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| 162 | ratio_mod(k) = mmm0 / & |
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| 163 | & (mmm0+0.56*(log(ypklim/cpp)-log(ypk(k)/cpp)) & |
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| 164 | & /(log(ypklim/cpp)-log(ypklim2/cpp))) |
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| 165 | ratio_mod(k) = max(ratio_mod(k),mmm0/(mmm0+0.56)) |
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| 166 | endif |
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| 167 | ENDDO |
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| 168 | !---------------------- |
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| 169 | |
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| 170 | if (planet_type.eq."venus") then |
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| 171 | |
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| 172 | !---------------------- |
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| 173 | ! ATMOSPHERE PROFONDE |
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| 174 | !---------------------- |
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| 175 | yt = (yteta/ratio_mod)**nu_venus & |
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| 176 | !---------------------- |
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| 177 | & + nu_venus * t0_venus**nu_venus * log(ypk/cpp) |
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| 178 | yt = yt**(1./nu_venus) |
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| 179 | else |
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| 180 | yt = yteta * ypk/cpp |
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| 181 | endif |
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| 182 | |
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| 183 | return |
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| 184 | end subroutine tpot2t |
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| 185 | |
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| 186 | !====================================================================== |
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| 187 | !====================================================================== |
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| 188 | ! Routines pour les calculs paralleles |
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| 189 | !====================================================================== |
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| 190 | #ifdef CPP_PARA |
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| 191 | !====================================================================== |
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| 192 | |
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| 193 | SUBROUTINE t2tpot_p(nlon,nlev, yt, yteta, ypk) |
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| 194 | ! Parallel version of t2tpot, for an arbitrary number of columns |
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| 195 | USE control_mod, only : planet_type |
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| 196 | USE parallel_lmdz, only : OMP_CHUNK |
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| 197 | USE comconst_mod, ONLY: cpp,nu_venus,t0_venus |
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| 198 | |
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| 199 | IMPLICIT none |
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| 200 | |
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| 201 | integer,intent(in) :: nlon,nlev |
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| 202 | real,intent(in) :: yt(nlon,nlev) |
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| 203 | real,intent(out) :: yteta(nlon,nlev) |
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| 204 | real,intent(in) :: ypk(nlon,nlev) |
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| 205 | ! local variable: |
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| 206 | integer :: l |
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| 207 | |
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| 208 | !---------------------- |
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| 209 | ! ATMOSPHERE PROFONDE |
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| 210 | real ypklim,ypklim2,mmm0 |
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| 211 | real ratio_mod(nlon,nlev) |
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| 212 | integer k |
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| 213 | ! theta_mod = theta * ratio_mod => ratio_mod = mmm0/mmm(p) |
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| 214 | |
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| 215 | ypklim = cpp*( 6e6/9.2e6)**0.1914 |
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| 216 | ypklim2 = cpp*(8.9e6/9.2e6)**0.1914 |
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| 217 | mmm0 = 43.44 |
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| 218 | |
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| 219 | DO k = 1, nlon |
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| 220 | DO l = 1, nlev |
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| 221 | ratio_mod(k,l) = 1. |
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| 222 | ! ATM PROFONDE DESACTIVEE ! |
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| 223 | if ( (1 .EQ. 0) .AND.(ypk(k,l).gt.ypklim)) then |
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| 224 | ratio_mod(k,l) = mmm0 / & |
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| 225 | & (mmm0+0.56*(log(ypklim/cpp)-log(ypk(k,l)/cpp)) & |
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| 226 | & /(log(ypklim/cpp)-log(ypklim2/cpp))) |
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| 227 | ratio_mod(k,l) = max(ratio_mod(k,l),mmm0/(mmm0+0.56)) |
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| 228 | endif |
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| 229 | ENDDO |
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| 230 | ENDDO |
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| 231 | !---------------------- |
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| 232 | |
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| 233 | if (planet_type.eq."venus") then |
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| 234 | !$OMP DO SCHEDULE(STATIC,OMP_CHUNK) |
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| 235 | do l=1,nlev |
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| 236 | yteta(:,l)=yt(:,l)**nu_venus & |
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| 237 | & -nu_venus*t0_venus**nu_venus* & |
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| 238 | & log(ypk(:,l)/cpp) |
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| 239 | yteta(:,l)=yteta(:,l)**(1./nu_venus) |
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| 240 | !---------------------- |
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| 241 | ! ATMOSPHERE PROFONDE |
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| 242 | yteta(:,l)=yteta(:,l)*ratio_mod(:,l) |
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| 243 | !---------------------- |
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| 244 | enddo |
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| 245 | !$OMP END DO |
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| 246 | else |
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| 247 | !$OMP DO SCHEDULE(STATIC,OMP_CHUNK) |
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| 248 | do l=1,nlev |
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| 249 | yteta(:,l)=yt(:,l)*cpp/ypk(:,l) |
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| 250 | enddo |
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| 251 | !$OMP END DO |
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| 252 | endif ! of if (planet_type.eq."venus") |
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| 253 | |
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| 254 | end subroutine t2tpot_p |
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| 255 | |
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| 256 | !====================================================================== |
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| 257 | !====================================================================== |
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| 258 | |
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| 259 | SUBROUTINE t2tpot_glo_p(yt, yteta, ypk) |
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| 260 | ! Parallel version of t2tpot, over the full dynamics (scalar) grid |
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| 261 | ! (more efficient than multiple calls to t2tpot_p() with slices of data) |
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| 262 | USE parallel_lmdz, only : jj_begin,jj_end,OMP_CHUNK |
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| 263 | USE control_mod, only : planet_type |
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| 264 | USE comconst_mod, ONLY: cpp,nu_venus,t0_venus |
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| 265 | |
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| 266 | IMPLICIT none |
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| 267 | ! for iip1, jjp1 and llm |
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| 268 | #include "dimensions.h" |
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| 269 | #include "paramet.h" |
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| 270 | |
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| 271 | real,intent(in) :: yt(iip1,jjp1,llm) |
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| 272 | real,intent(out) :: yteta(iip1,jjp1,llm) |
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| 273 | real,intent(in) :: ypk(iip1,jjp1,llm) |
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| 274 | ! local variable: |
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| 275 | integer :: j,l |
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| 276 | integer :: jjb,jje |
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| 277 | |
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| 278 | !---------------------- |
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| 279 | ! ATMOSPHERE PROFONDE |
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| 280 | real ypklim,ypklim2,mmm0 |
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| 281 | real ratio_mod(iip1,jjp1,llm) |
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| 282 | integer i |
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| 283 | ! theta_mod = theta * ratio_mod => ratio_mod = mmm0/mmm(p) |
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| 284 | |
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| 285 | ypklim = cpp*( 6e6/9.2e6)**0.1914 |
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| 286 | ypklim2 = cpp*(8.9e6/9.2e6)**0.1914 |
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| 287 | mmm0 = 43.44 |
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| 288 | |
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| 289 | DO i = 1, iip1 |
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| 290 | DO j = 1, jjp1 |
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| 291 | DO l = 1, llm |
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| 292 | ratio_mod(i,j,l) = 1. |
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| 293 | ! ATM PROFONDE DESACTIVEE ! |
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| 294 | if ( (1 .EQ. 0) .AND.(ypk(i,j,l).gt.ypklim)) then |
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| 295 | ratio_mod(i,j,l) = mmm0 / & |
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| 296 | & (mmm0+0.56*(log(ypklim/cpp)-log(ypk(i,j,l)/cpp)) & |
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| 297 | & /(log(ypklim/cpp)-log(ypklim2/cpp))) |
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| 298 | ratio_mod(i,j,l) = max(ratio_mod(i,j,l),mmm0/(mmm0+0.56)) |
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| 299 | endif |
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| 300 | ENDDO |
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| 301 | ENDDO |
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| 302 | ENDDO |
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| 303 | !---------------------- |
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| 304 | |
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| 305 | jjb=jj_begin |
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| 306 | jje=jj_end |
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| 307 | |
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| 308 | if (planet_type.eq."venus") then |
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| 309 | !$OMP DO SCHEDULE(STATIC,OMP_CHUNK) |
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| 310 | do l=1,llm |
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| 311 | yteta(:,jjb:jje,l)=yt(:,jjb:jje,l)**nu_venus & |
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| 312 | & -nu_venus*t0_venus**nu_venus* & |
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| 313 | & log(ypk(:,jjb:jje,l)/cpp) |
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| 314 | yteta(:,jjb:jje,l)=yteta(:,jjb:jje,l)**(1./nu_venus) |
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| 315 | !---------------------- |
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| 316 | ! ATMOSPHERE PROFONDE |
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| 317 | yteta(:,jjb:jje,l)=yteta(:,jjb:jje,l)*ratio_mod(:,jjb:jje,l) |
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| 318 | !---------------------- |
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| 319 | enddo |
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| 320 | !$OMP END DO |
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| 321 | else |
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| 322 | !$OMP DO SCHEDULE(STATIC,OMP_CHUNK) |
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| 323 | do l=1,llm |
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| 324 | yteta(:,jjb:jje,l)=yt(:,jjb:jje,l)*cpp/ypk(:,jjb:jje,l) |
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| 325 | enddo |
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| 326 | !$OMP END DO |
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| 327 | endif ! of if (planet_type.eq."venus") |
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| 328 | |
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| 329 | end subroutine t2tpot_glo_p |
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| 330 | |
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| 331 | !====================================================================== |
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| 332 | !====================================================================== |
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| 333 | |
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| 334 | SUBROUTINE tpot2t_p(nlon,nlev,yteta,yt,ypk) |
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| 335 | ! Parallel version of tpot2t, for an arbitrary number of columns |
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| 336 | USE control_mod, only : planet_type |
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| 337 | USE parallel_lmdz, only : OMP_CHUNK |
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| 338 | USE comconst_mod, ONLY: cpp,nu_venus,t0_venus |
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| 339 | |
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| 340 | IMPLICIT none |
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| 341 | |
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| 342 | integer,intent(in) :: nlon,nlev |
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| 343 | real,intent(out) :: yt(nlon,nlev) |
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| 344 | real,intent(in) :: yteta(nlon,nlev) |
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| 345 | real,intent(in) :: ypk(nlon,nlev) |
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| 346 | |
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| 347 | ! local variable: |
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| 348 | integer :: l |
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| 349 | |
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| 350 | !---------------------- |
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| 351 | ! ATMOSPHERE PROFONDE |
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| 352 | real ypklim,ypklim2,mmm0 |
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| 353 | real ratio_mod(nlon,nlev) |
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| 354 | integer k |
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| 355 | ! theta_mod = theta * ratio_mod => ratio_mod = mmm0/mmm(p) |
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| 356 | |
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| 357 | ypklim = cpp*( 6e6/9.2e6)**0.1914 |
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| 358 | ypklim2 = cpp*(8.9e6/9.2e6)**0.1914 |
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| 359 | mmm0 = 43.44 |
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| 360 | |
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| 361 | DO k = 1, nlon |
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| 362 | DO l = 1, nlev |
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| 363 | ratio_mod(k,l) = 1. |
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| 364 | ! ATM PROFONDE DESACTIVEE ! |
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| 365 | if ( (1 .EQ. 0) .AND.(ypk(k,l).gt.ypklim)) then |
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| 366 | ratio_mod(k,l) = mmm0 / & |
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| 367 | & (mmm0+0.56*(log(ypklim/cpp)-log(ypk(k,l)/cpp)) & |
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| 368 | & /(log(ypklim/cpp)-log(ypklim2/cpp))) |
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| 369 | ratio_mod(k,l) = max(ratio_mod(k,l),mmm0/(mmm0+0.56)) |
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| 370 | endif |
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| 371 | ENDDO |
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| 372 | ENDDO |
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| 373 | !---------------------- |
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| 374 | |
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| 375 | if (planet_type.eq."venus") then |
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| 376 | !$OMP DO SCHEDULE(STATIC,OMP_CHUNK) |
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| 377 | do l=1,nlev |
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| 378 | !---------------------- |
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| 379 | ! ATMOSPHERE PROFONDE |
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| 380 | yt(:,l)=(yteta(:,l)/ratio_mod(:,l))**nu_venus & |
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| 381 | !---------------------- |
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| 382 | & +nu_venus*t0_venus**nu_venus* & |
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| 383 | & log(ypk(:,l)/cpp) |
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| 384 | yt(:,l)=yt(:,l)**(1./nu_venus) |
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| 385 | enddo |
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| 386 | !$OMP END DO |
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| 387 | else |
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| 388 | !$OMP DO SCHEDULE(STATIC,OMP_CHUNK) |
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| 389 | do l=1,nlev |
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| 390 | yt(:,l)=yteta(:,l)*ypk(:,l)/cpp |
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| 391 | enddo |
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| 392 | !$OMP END DO |
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| 393 | endif ! of if (planet_type.eq."venus") |
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| 394 | end subroutine tpot2t_p |
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| 395 | |
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| 396 | !====================================================================== |
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| 397 | !====================================================================== |
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| 398 | |
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| 399 | SUBROUTINE tpot2t_glo_p(yteta,yt,ypk) |
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| 400 | ! Parallel version of tpot2t, over the full dynamics (scalar) grid |
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| 401 | ! (more efficient than multiple calls to tpot2t_p() with slices of data) |
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| 402 | USE parallel_lmdz, only : jj_begin,jj_end,OMP_CHUNK |
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| 403 | USE control_mod, only : planet_type |
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| 404 | USE comconst_mod, ONLY: cpp,nu_venus,t0_venus |
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| 405 | |
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| 406 | IMPLICIT none |
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| 407 | ! for iip1, jjp1 and llm |
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| 408 | #include "dimensions.h" |
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| 409 | #include "paramet.h" |
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| 410 | |
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| 411 | real,intent(out) :: yt(iip1,jjp1,llm) |
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| 412 | real,intent(in) :: yteta(iip1,jjp1,llm) |
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| 413 | real,intent(in) :: ypk(iip1,jjp1,llm) |
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| 414 | ! local variable: |
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| 415 | integer :: j,l |
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| 416 | integer :: jjb,jje |
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| 417 | |
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| 418 | !---------------------- |
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| 419 | ! ATMOSPHERE PROFONDE |
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| 420 | real ypklim,ypklim2,mmm0 |
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| 421 | real ratio_mod(iip1,jjp1,llm) |
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| 422 | integer i |
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| 423 | ! theta_mod = theta * ratio_mod => ratio_mod = mmm0/mmm(p) |
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| 424 | |
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| 425 | ypklim = cpp*( 6e6/9.2e6)**0.1914 |
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| 426 | ypklim2 = cpp*(8.9e6/9.2e6)**0.1914 |
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| 427 | mmm0 = 43.44 |
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| 428 | |
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| 429 | DO i = 1, iip1 |
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| 430 | DO j = 1, jjp1 |
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| 431 | DO l = 1, llm |
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| 432 | ratio_mod(i,j,l) = 1. |
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| 433 | ! ATM PROFONDE DESACTIVEE ! |
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| 434 | if ( (1 .EQ. 0) .AND.(ypk(i,j,l).gt.ypklim)) then |
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| 435 | ratio_mod(i,j,l) = mmm0 / & |
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| 436 | & (mmm0+0.56*(log(ypklim/cpp)-log(ypk(i,j,l)/cpp)) & |
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| 437 | & /(log(ypklim/cpp)-log(ypklim2/cpp))) |
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| 438 | ratio_mod(i,j,l) = max(ratio_mod(i,j,l),mmm0/(mmm0+0.56)) |
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| 439 | endif |
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| 440 | ENDDO |
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| 441 | ENDDO |
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| 442 | ENDDO |
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| 443 | !---------------------- |
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| 444 | |
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| 445 | jjb=jj_begin |
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| 446 | jje=jj_end |
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| 447 | |
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| 448 | if (planet_type.eq."venus") then |
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| 449 | !$OMP DO SCHEDULE(STATIC,OMP_CHUNK) |
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| 450 | do l=1,llm |
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| 451 | !---------------------- |
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| 452 | ! ATMOSPHERE PROFONDE |
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| 453 | yt(:,jjb:jje,l)= & |
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| 454 | & (yteta(:,jjb:jje,l)/ratio_mod(:,jjb:jje,l))**nu_venus & |
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| 455 | !---------------------- |
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| 456 | & +nu_venus*t0_venus**nu_venus* & |
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| 457 | & log(ypk(:,jjb:jje,l)/cpp) |
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| 458 | yt(:,jjb:jje,l)=yt(:,jjb:jje,l)**(1./nu_venus) |
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| 459 | enddo |
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| 460 | !$OMP END DO |
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| 461 | else |
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| 462 | !$OMP DO SCHEDULE(STATIC,OMP_CHUNK) |
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| 463 | do l=1,llm |
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| 464 | yt(:,jjb:jje,l)=yteta(:,jjb:jje,l)*ypk(:,jjb:jje,l)/cpp |
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| 465 | enddo |
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| 466 | !$OMP END DO |
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| 467 | endif ! of if (planet_type.eq."venus") |
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| 468 | end subroutine tpot2t_glo_p |
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| 469 | |
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| 470 | !====================================================================== |
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| 471 | #endif |
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| 472 | !====================================================================== |
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| 473 | ! Fin routines specifiques parallele |
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| 474 | !====================================================================== |
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| 475 | !====================================================================== |
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| 476 | ! |
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| 477 | ! ATTENTION |
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| 478 | ! |
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| 479 | ! Si un jour on a besoin, il faudra coder les routines |
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| 480 | ! dt2dtpot / dtpto2dt |
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| 481 | ! |
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| 482 | !====================================================================== |
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| 483 | !====================================================================== |
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| 484 | end module cpdet_mod |
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