| 1 |
SUBROUTINE clmain(dtime,itap,date0,pctsrf,pctsrf_new, |
module clmain_m |
| 2 |
. t,q,u,v, |
|
| 3 |
. jour, rmu0, co2_ppm, |
IMPLICIT NONE |
| 4 |
. ok_veget, ocean, npas, nexca, ts, |
|
| 5 |
. soil_model,cdmmax, cdhmax, |
contains |
| 6 |
. ksta, ksta_ter, ok_kzmin, ftsoil,qsol, |
|
| 7 |
. paprs,pplay,snow,qsurf,evap,albe,alblw, |
SUBROUTINE clmain(dtime, pctsrf, t, q, u, v, jour, rmu0, ts, cdmmax, & |
| 8 |
. fluxlat, |
cdhmax, ksta, ksta_ter, ok_kzmin, ftsoil, qsol, paprs, pplay, snow, & |
| 9 |
. rain_f, snow_f, solsw, sollw, sollwdown, fder, |
qsurf, evap, falbe, fluxlat, rain_fall, snow_f, solsw, sollw, fder, & |
| 10 |
. rlon, rlat, cufi, cvfi, rugos, |
rlat, rugos, agesno, rugoro, d_t, d_q, d_u, d_v, d_ts, flux_t, flux_q, & |
| 11 |
. debut, lafin, agesno,rugoro, |
flux_u, flux_v, cdragh, cdragm, q2, dflux_t, dflux_q, ycoefh, zu1, & |
| 12 |
. d_t,d_q,d_u,d_v,d_ts, |
zv1, t2m, q2m, u10m, v10m, pblh, capcl, oliqcl, cteicl, pblt, therm, & |
| 13 |
. flux_t,flux_q,flux_u,flux_v,cdragh,cdragm, |
trmb1, trmb2, trmb3, plcl, fqcalving, ffonte, run_off_lic_0) |
| 14 |
. q2, |
|
| 15 |
. dflux_t,dflux_q, |
! From phylmd/clmain.F, version 1.6, 2005/11/16 14:47:19 |
| 16 |
. zcoefh,zu1,zv1, t2m, q2m, u10m, v10m, |
! Author: Z. X. Li (LMD/CNRS), date: 1993/08/18 |
| 17 |
cIM cf. AM : pbl |
! Objet : interface de couche limite (diffusion verticale) |
| 18 |
. pblh,capCL,oliqCL,cteiCL,pblT, |
|
| 19 |
. therm,trmb1,trmb2,trmb3,plcl, |
! Tout ce qui a trait aux traceurs est dans "phytrac". Le calcul |
| 20 |
. fqcalving,ffonte, run_off_lic_0, |
! de la couche limite pour les traceurs se fait avec "cltrac" et |
| 21 |
cIM "slab" ocean |
! ne tient pas compte de la diff\'erentiation des sous-fractions |
| 22 |
. flux_o, flux_g, tslab, seaice) |
! de sol. |
| 23 |
|
|
| 24 |
! |
! Pour pouvoir extraire les coefficients d'\'echanges et le vent |
| 25 |
! $Header: /home/cvsroot/LMDZ4/libf/phylmd/clmain.F,v 1.6 2005/11/16 14:47:19 lmdzadmin Exp $ |
! dans la premi\`ere couche, trois champs ont \'et\'e cr\'e\'es : "ycoefh", |
| 26 |
! |
! "zu1" et "zv1". Nous avons moyenn\'e les valeurs de ces trois |
| 27 |
c |
! champs sur les quatre sous-surfaces du mod\`ele. |
| 28 |
c |
|
| 29 |
cAA REM: |
use clqh_m, only: clqh |
| 30 |
cAA----- |
use clvent_m, only: clvent |
| 31 |
cAA Tout ce qui a trait au traceurs est dans phytrac maintenant |
use coefkz_m, only: coefkz |
| 32 |
cAA pour l'instant le calcul de la couche limite pour les traceurs |
use coefkzmin_m, only: coefkzmin |
| 33 |
cAA se fait avec cltrac et ne tient pas compte de la differentiation |
USE conf_gcm_m, ONLY: prt_level, lmt_pas |
| 34 |
cAA des sous-fraction de sol. |
USE conf_phys_m, ONLY: iflag_pbl |
| 35 |
cAA REM bis : |
USE dimphy, ONLY: klev, klon, zmasq |
| 36 |
cAA---------- |
USE dimsoil, ONLY: nsoilmx |
| 37 |
cAA Pour pouvoir extraire les coefficient d'echanges et le vent |
use hbtm_m, only: hbtm |
| 38 |
cAA dans la premiere couche, 3 champs supplementaires ont ete crees |
USE indicesol, ONLY: epsfra, is_lic, is_oce, is_sic, is_ter, nbsrf |
| 39 |
cAA zcoefh,zu1 et zv1. Pour l'instant nous avons moyenne les valeurs |
USE interfoce_lim_m, ONLY: interfoce_lim |
| 40 |
cAA de ces trois champs sur les 4 subsurfaces du modele. Dans l'avenir |
use stdlevvar_m, only: stdlevvar |
| 41 |
cAA si les informations des subsurfaces doivent etre prises en compte |
USE suphec_m, ONLY: rd, rg, rkappa |
| 42 |
cAA il faudra sortir ces memes champs en leur ajoutant une dimension, |
use time_phylmdz, only: itap |
| 43 |
cAA c'est a dire nbsrf (nbre de subsurface). |
use ustarhb_m, only: ustarhb |
| 44 |
USE ioipsl |
use vdif_kcay_m, only: vdif_kcay |
| 45 |
USE interface_surf |
use yamada4_m, only: yamada4 |
| 46 |
use dimens_m |
|
| 47 |
use indicesol |
REAL, INTENT(IN):: dtime ! interval du temps (secondes) |
| 48 |
use dimphy |
|
| 49 |
use dimsoil |
REAL, INTENT(inout):: pctsrf(klon, nbsrf) |
| 50 |
use temps |
! tableau des pourcentages de surface de chaque maille |
| 51 |
use iniprint |
|
| 52 |
use YOMCST |
REAL, INTENT(IN):: t(klon, klev) ! temperature (K) |
| 53 |
use yoethf |
REAL, INTENT(IN):: q(klon, klev) ! vapeur d'eau (kg/kg) |
| 54 |
use fcttre |
REAL, INTENT(IN):: u(klon, klev), v(klon, klev) ! vitesse |
| 55 |
use conf_phys_m |
INTEGER, INTENT(IN):: jour ! jour de l'annee en cours |
| 56 |
use gath_cpl, only: gath2cpl |
REAL, intent(in):: rmu0(klon) ! cosinus de l'angle solaire zenithal |
| 57 |
IMPLICIT none |
REAL, INTENT(IN):: ts(klon, nbsrf) ! temperature du sol (en Kelvin) |
| 58 |
c====================================================================== |
REAL, INTENT(IN):: cdmmax, cdhmax ! seuils cdrm, cdrh |
| 59 |
c Auteur(s) Z.X. Li (LMD/CNRS) date: 19930818 |
REAL, INTENT(IN):: ksta, ksta_ter |
| 60 |
c Objet: interface de "couche limite" (diffusion verticale) |
LOGICAL, INTENT(IN):: ok_kzmin |
| 61 |
c Arguments: |
|
| 62 |
c dtime----input-R- interval du temps (secondes) |
REAL, INTENT(inout):: ftsoil(klon, nsoilmx, nbsrf) |
| 63 |
c itap-----input-I- numero du pas de temps |
! soil temperature of surface fraction |
| 64 |
c date0----input-R- jour initial |
|
| 65 |
c t--------input-R- temperature (K) |
REAL, INTENT(inout):: qsol(klon) |
| 66 |
c q--------input-R- vapeur d'eau (kg/kg) |
! column-density of water in soil, in kg m-2 |
| 67 |
c u--------input-R- vitesse u |
|
| 68 |
c v--------input-R- vitesse v |
REAL, INTENT(IN):: paprs(klon, klev+1) ! pression a intercouche (Pa) |
| 69 |
c ts-------input-R- temperature du sol (en Kelvin) |
REAL, INTENT(IN):: pplay(klon, klev) ! pression au milieu de couche (Pa) |
| 70 |
c paprs----input-R- pression a intercouche (Pa) |
REAL, INTENT(inout):: snow(klon, nbsrf) |
| 71 |
c pplay----input-R- pression au milieu de couche (Pa) |
REAL qsurf(klon, nbsrf) |
| 72 |
c radsol---input-R- flux radiatif net (positif vers le sol) en W/m**2 |
REAL evap(klon, nbsrf) |
| 73 |
c rlat-----input-R- latitude en degree |
REAL, intent(inout):: falbe(klon, nbsrf) |
| 74 |
c rugos----input-R- longeur de rugosite (en m) |
|
| 75 |
c cufi-----input-R- resolution des mailles en x (m) |
REAL fluxlat(klon, nbsrf) |
| 76 |
c cvfi-----input-R- resolution des mailles en y (m) |
|
| 77 |
c |
REAL, intent(in):: rain_fall(klon) |
| 78 |
c d_t------output-R- le changement pour "t" |
! liquid water mass flux (kg/m2/s), positive down |
| 79 |
c d_q------output-R- le changement pour "q" |
|
| 80 |
c d_u------output-R- le changement pour "u" |
REAL, intent(in):: snow_f(klon) |
| 81 |
c d_v------output-R- le changement pour "v" |
! solid water mass flux (kg/m2/s), positive down |
| 82 |
c d_ts-----output-R- le changement pour "ts" |
|
| 83 |
c flux_t---output-R- flux de chaleur sensible (CpT) J/m**2/s (W/m**2) |
REAL, INTENT(IN):: solsw(klon, nbsrf), sollw(klon, nbsrf) |
| 84 |
c (orientation positive vers le bas) |
REAL, intent(in):: fder(klon) |
| 85 |
c flux_q---output-R- flux de vapeur d'eau (kg/m**2/s) |
REAL, INTENT(IN):: rlat(klon) ! latitude en degr\'es |
| 86 |
c flux_u---output-R- tension du vent X: (kg m/s)/(m**2 s) ou Pascal |
|
| 87 |
c flux_v---output-R- tension du vent Y: (kg m/s)/(m**2 s) ou Pascal |
REAL, intent(inout):: rugos(klon, nbsrf) ! longueur de rugosit\'e (en m) |
| 88 |
c dflux_t derive du flux sensible |
|
| 89 |
c dflux_q derive du flux latent |
real agesno(klon, nbsrf) |
| 90 |
cIM "slab" ocean |
REAL, INTENT(IN):: rugoro(klon) |
| 91 |
c flux_g---output-R- flux glace (pour OCEAN='slab ') |
|
| 92 |
c flux_o---output-R- flux ocean (pour OCEAN='slab ') |
REAL d_t(klon, klev), d_q(klon, klev) |
| 93 |
c tslab-in/output-R temperature du slab ocean (en Kelvin) ! uniqmnt pour slab |
! d_t------output-R- le changement pour "t" |
| 94 |
c seaice---output-R- glace de mer (kg/m2) (pour OCEAN='slab ') |
! d_q------output-R- le changement pour "q" |
| 95 |
ccc |
|
| 96 |
c ffonte----Flux thermique utilise pour fondre la neige |
REAL, intent(out):: d_u(klon, klev), d_v(klon, klev) |
| 97 |
c fqcalving-Flux d'eau "perdue" par la surface et necessaire pour limiter la |
! changement pour "u" et "v" |
| 98 |
c hauteur de neige, en kg/m2/s |
|
| 99 |
cAA on rajoute en output yu1 et yv1 qui sont les vents dans |
REAL, intent(out):: d_ts(klon, nbsrf) ! le changement pour "ts" |
| 100 |
cAA la premiere couche |
|
| 101 |
cAA ces 4 variables sont maintenant traites dans phytrac |
REAL, intent(out):: flux_t(klon, nbsrf) |
| 102 |
c itr--------input-I- nombre de traceurs |
! flux de chaleur sensible (Cp T) (W/m2) (orientation positive vers |
| 103 |
c tr---------input-R- q. de traceurs |
! le bas) Ã la surface |
| 104 |
c flux_surf--input-R- flux de traceurs a la surface |
|
| 105 |
c d_tr-------output-R tendance de traceurs |
REAL, intent(out):: flux_q(klon, nbsrf) |
| 106 |
cIM cf. AM : PBL |
! flux de vapeur d'eau (kg/m2/s) Ã la surface |
| 107 |
c trmb1-------deep_cape |
|
| 108 |
c trmb2--------inhibition |
REAL, intent(out):: flux_u(klon, nbsrf), flux_v(klon, nbsrf) |
| 109 |
c trmb3-------Point Omega |
! tension du vent à la surface, en Pa |
| 110 |
c Cape(klon)-------Cape du thermique |
|
| 111 |
c EauLiq(klon)-------Eau liqu integr du thermique |
REAL, INTENT(out):: cdragh(klon), cdragm(klon) |
| 112 |
c ctei(klon)-------Critere d'instab d'entrainmt des nuages de CL |
real q2(klon, klev+1, nbsrf) |
| 113 |
c lcl------- Niveau de condensation |
|
| 114 |
c pblh------- HCL |
REAL, INTENT(out):: dflux_t(klon), dflux_q(klon) |
| 115 |
c pblT------- T au nveau HCL |
! dflux_t derive du flux sensible |
| 116 |
c====================================================================== |
! dflux_q derive du flux latent |
| 117 |
c$$$ PB ajout pour soil |
! IM "slab" ocean |
| 118 |
c |
|
| 119 |
REAL dtime |
REAL, intent(out):: ycoefh(klon, klev) |
| 120 |
real date0 |
REAL, intent(out):: zu1(klon) |
| 121 |
integer, intent(in):: itap |
REAL zv1(klon) |
| 122 |
REAL t(klon,klev), q(klon,klev) |
REAL t2m(klon, nbsrf), q2m(klon, nbsrf) |
| 123 |
REAL u(klon,klev), v(klon,klev) |
REAL u10m(klon, nbsrf), v10m(klon, nbsrf) |
| 124 |
cIM 230604 BAD REAL radsol(klon) ??? |
|
| 125 |
REAL, intent(in):: paprs(klon,klev+1) |
! Ionela Musat cf. Anne Mathieu : planetary boundary layer, hbtm |
| 126 |
real, intent(in):: pplay(klon,klev) |
! (Comme les autres diagnostics on cumule dans physiq ce qui |
| 127 |
REAL, intent(in):: rlon(klon), rlat(klon) |
! permet de sortir les grandeurs par sous-surface) |
| 128 |
real cufi(klon), cvfi(klon) |
REAL pblh(klon, nbsrf) ! height of planetary boundary layer |
| 129 |
REAL d_t(klon, klev), d_q(klon, klev) |
REAL capcl(klon, nbsrf) |
| 130 |
REAL d_u(klon, klev), d_v(klon, klev) |
REAL oliqcl(klon, nbsrf) |
| 131 |
REAL flux_t(klon,klev, nbsrf), flux_q(klon,klev, nbsrf) |
REAL cteicl(klon, nbsrf) |
| 132 |
REAL dflux_t(klon), dflux_q(klon) |
REAL pblt(klon, nbsrf) |
| 133 |
cIM "slab" ocean |
! pblT------- T au nveau HCL |
| 134 |
REAL flux_o(klon), flux_g(klon) |
REAL therm(klon, nbsrf) |
| 135 |
REAL y_flux_o(klon), y_flux_g(klon) |
REAL trmb1(klon, nbsrf) |
| 136 |
REAL tslab(klon), ytslab(klon) |
! trmb1-------deep_cape |
| 137 |
REAL seaice(klon), y_seaice(klon) |
REAL trmb2(klon, nbsrf) |
| 138 |
cIM cf JLD |
! trmb2--------inhibition |
| 139 |
REAL y_fqcalving(klon), y_ffonte(klon) |
REAL trmb3(klon, nbsrf) |
| 140 |
REAL fqcalving(klon,nbsrf), ffonte(klon,nbsrf) |
! trmb3-------Point Omega |
| 141 |
REAL run_off_lic_0(klon), y_run_off_lic_0(klon) |
REAL plcl(klon, nbsrf) |
| 142 |
|
REAL fqcalving(klon, nbsrf), ffonte(klon, nbsrf) |
| 143 |
REAL flux_u(klon,klev, nbsrf), flux_v(klon,klev, nbsrf) |
! ffonte----Flux thermique utilise pour fondre la neige |
| 144 |
REAL rugmer(klon), agesno(klon,nbsrf),rugoro(klon) |
! fqcalving-Flux d'eau "perdue" par la surface et necessaire pour limiter la |
| 145 |
REAL cdragh(klon), cdragm(klon) |
! hauteur de neige, en kg/m2/s |
| 146 |
integer jour ! jour de l'annee en cours |
REAL run_off_lic_0(klon) |
| 147 |
real rmu0(klon) ! cosinus de l'angle solaire zenithal |
|
| 148 |
REAL co2_ppm ! taux CO2 atmosphere |
! Local: |
| 149 |
LOGICAL, intent(in):: debut |
|
| 150 |
logical, intent(in):: lafin |
LOGICAL:: firstcal = .true. |
| 151 |
logical ok_veget |
|
| 152 |
character*6 ocean |
! la nouvelle repartition des surfaces sortie de l'interface |
| 153 |
integer npas, nexca |
REAL, save:: pctsrf_new_oce(klon) |
| 154 |
c |
REAL, save:: pctsrf_new_sic(klon) |
| 155 |
REAL pctsrf(klon,nbsrf) |
|
| 156 |
REAL ts(klon,nbsrf) |
REAL y_fqcalving(klon), y_ffonte(klon) |
| 157 |
REAL d_ts(klon,nbsrf) |
real y_run_off_lic_0(klon) |
| 158 |
REAL snow(klon,nbsrf) |
|
| 159 |
REAL qsurf(klon,nbsrf) |
REAL rugmer(klon) |
| 160 |
REAL evap(klon,nbsrf) |
|
| 161 |
REAL albe(klon,nbsrf) |
REAL ytsoil(klon, nsoilmx) |
| 162 |
REAL alblw(klon,nbsrf) |
|
| 163 |
c$$$ PB |
REAL yts(klon), yrugos(klon), ypct(klon), yz0_new(klon) |
| 164 |
REAL fluxlat(klon,nbsrf) |
REAL yalb(klon) |
| 165 |
C |
REAL yu1(klon), yv1(klon) |
| 166 |
real rain_f(klon), snow_f(klon) |
! on rajoute en output yu1 et yv1 qui sont les vents dans |
| 167 |
REAL fder(klon) |
! la premiere couche |
| 168 |
cIM cf. JLD REAL sollw(klon), solsw(klon), sollwdown(klon) |
REAL ysnow(klon), yqsurf(klon), yagesno(klon) |
| 169 |
REAL sollw(klon,nbsrf), solsw(klon,nbsrf), sollwdown(klon) |
|
| 170 |
REAL rugos(klon,nbsrf) |
real yqsol(klon) |
| 171 |
C la nouvelle repartition des surfaces sortie de l'interface |
! column-density of water in soil, in kg m-2 |
| 172 |
REAL pctsrf_new(klon,nbsrf) |
|
| 173 |
cAA |
REAL yrain_f(klon) |
| 174 |
REAL zcoefh(klon,klev) |
! liquid water mass flux (kg/m2/s), positive down |
| 175 |
REAL zu1(klon) |
|
| 176 |
REAL zv1(klon) |
REAL ysnow_f(klon) |
| 177 |
cAA |
! solid water mass flux (kg/m2/s), positive down |
| 178 |
c$$$ PB ajout pour soil |
|
| 179 |
LOGICAL soil_model |
REAL yfder(klon) |
| 180 |
cIM ajout seuils cdrm, cdrh |
REAL yrugm(klon), yrads(klon), yrugoro(klon) |
| 181 |
REAL cdmmax, cdhmax |
|
| 182 |
cIM: 261103 |
REAL yfluxlat(klon) |
| 183 |
REAL ksta, ksta_ter |
|
| 184 |
LOGICAL ok_kzmin |
REAL y_d_ts(klon) |
| 185 |
cIM: 261103 |
REAL y_d_t(klon, klev), y_d_q(klon, klev) |
| 186 |
REAL ftsoil(klon,nsoilmx,nbsrf) |
REAL y_d_u(klon, klev), y_d_v(klon, klev) |
| 187 |
REAL ytsoil(klon,nsoilmx) |
REAL y_flux_t(klon), y_flux_q(klon) |
| 188 |
REAL qsol(klon) |
REAL y_flux_u(klon), y_flux_v(klon) |
| 189 |
c====================================================================== |
REAL y_dflux_t(klon), y_dflux_q(klon) |
| 190 |
EXTERNAL clqh, clvent, coefkz, calbeta, cltrac |
REAL coefh(klon, klev), coefm(klon, klev) |
| 191 |
c====================================================================== |
REAL yu(klon, klev), yv(klon, klev) |
| 192 |
REAL yts(klon), yrugos(klon), ypct(klon), yz0_new(klon) |
REAL yt(klon, klev), yq(klon, klev) |
| 193 |
REAL yalb(klon) |
REAL ypaprs(klon, klev+1), ypplay(klon, klev), ydelp(klon, klev) |
| 194 |
REAL yalblw(klon) |
|
| 195 |
REAL yu1(klon), yv1(klon) |
REAL ycoefm0(klon, klev), ycoefh0(klon, klev) |
| 196 |
real ysnow(klon), yqsurf(klon), yagesno(klon), yqsol(klon) |
|
| 197 |
real yrain_f(klon), ysnow_f(klon) |
REAL yzlay(klon, klev), yzlev(klon, klev+1), yteta(klon, klev) |
| 198 |
real ysollw(klon), ysolsw(klon), ysollwdown(klon) |
REAL ykmm(klon, klev+1), ykmn(klon, klev+1) |
| 199 |
real yfder(klon), ytaux(klon), ytauy(klon) |
REAL ykmq(klon, klev+1) |
| 200 |
REAL yrugm(klon), yrads(klon),yrugoro(klon) |
REAL yq2(klon, klev+1) |
| 201 |
c$$$ PB |
REAL q2diag(klon, klev+1) |
| 202 |
REAL yfluxlat(klon) |
|
| 203 |
C |
REAL u1lay(klon), v1lay(klon) |
| 204 |
REAL y_d_ts(klon) |
REAL delp(klon, klev) |
| 205 |
REAL y_d_t(klon, klev), y_d_q(klon, klev) |
INTEGER i, k, nsrf |
| 206 |
REAL y_d_u(klon, klev), y_d_v(klon, klev) |
|
| 207 |
REAL y_flux_t(klon,klev), y_flux_q(klon,klev) |
INTEGER ni(klon), knon, j |
| 208 |
REAL y_flux_u(klon,klev), y_flux_v(klon,klev) |
|
| 209 |
REAL y_dflux_t(klon), y_dflux_q(klon) |
REAL pctsrf_pot(klon, nbsrf) |
| 210 |
REAL ycoefh(klon,klev), ycoefm(klon,klev) |
! "pourcentage potentiel" pour tenir compte des \'eventuelles |
| 211 |
REAL yu(klon,klev), yv(klon,klev) |
! apparitions ou disparitions de la glace de mer |
| 212 |
REAL yt(klon,klev), yq(klon,klev) |
|
| 213 |
REAL ypaprs(klon,klev+1), ypplay(klon,klev), ydelp(klon,klev) |
REAL zx_alf1, zx_alf2 ! valeur ambiante par extrapolation |
| 214 |
c |
|
| 215 |
LOGICAL ok_nonloc |
REAL yt2m(klon), yq2m(klon), yu10m(klon) |
| 216 |
PARAMETER (ok_nonloc=.FALSE.) |
REAL yustar(klon) |
| 217 |
REAL ycoefm0(klon,klev), ycoefh0(klon,klev) |
|
| 218 |
|
REAL yt10m(klon), yq10m(klon) |
| 219 |
cIM 081204 hcl_Anne ? BEG |
REAL ypblh(klon) |
| 220 |
real yzlay(klon,klev),yzlev(klon,klev+1),yteta(klon,klev) |
REAL ylcl(klon) |
| 221 |
real ykmm(klon,klev+1),ykmn(klon,klev+1) |
REAL ycapcl(klon) |
| 222 |
real ykmq(klon,klev+1) |
REAL yoliqcl(klon) |
| 223 |
real yq2(klon,klev+1),q2(klon,klev+1,nbsrf) |
REAL ycteicl(klon) |
| 224 |
real q2diag(klon,klev+1) |
REAL ypblt(klon) |
| 225 |
cIM 081204 real yustar(klon),y_cd_m(klon),y_cd_h(klon) |
REAL ytherm(klon) |
| 226 |
cIM 081204 hcl_Anne ? END |
REAL ytrmb1(klon) |
| 227 |
c |
REAL ytrmb2(klon) |
| 228 |
REAL u1lay(klon), v1lay(klon) |
REAL ytrmb3(klon) |
| 229 |
REAL delp(klon,klev) |
REAL uzon(klon), vmer(klon) |
| 230 |
INTEGER i, k, nsrf |
REAL tair1(klon), qair1(klon), tairsol(klon) |
| 231 |
cAA INTEGER it |
REAL psfce(klon), patm(klon) |
| 232 |
INTEGER ni(klon), knon, j |
|
| 233 |
c Introduction d'une variable "pourcentage potentiel" pour tenir compte |
REAL qairsol(klon), zgeo1(klon) |
| 234 |
c des eventuelles apparitions et/ou disparitions de la glace de mer |
REAL rugo1(klon) |
| 235 |
REAL pctsrf_pot(klon,nbsrf) |
|
| 236 |
|
! utiliser un jeu de fonctions simples |
| 237 |
c====================================================================== |
LOGICAL zxli |
| 238 |
REAL zx_alf1, zx_alf2 !valeur ambiante par extrapola. |
PARAMETER (zxli=.FALSE.) |
| 239 |
c====================================================================== |
|
| 240 |
c |
!------------------------------------------------------------ |
| 241 |
c maf pour sorties IOISPL en cas de debugagage |
|
| 242 |
c |
ytherm = 0. |
| 243 |
CHARACTER*80 cldebug |
|
| 244 |
SAVE cldebug |
DO k = 1, klev ! epaisseur de couche |
| 245 |
CHARACTER*8 cl_surf(nbsrf) |
DO i = 1, klon |
| 246 |
SAVE cl_surf |
delp(i, k) = paprs(i, k) - paprs(i, k+1) |
| 247 |
INTEGER nhoridbg, nidbg |
END DO |
| 248 |
SAVE nhoridbg, nidbg |
END DO |
| 249 |
INTEGER ndexbg(iim*(jjm+1)) |
DO i = 1, klon ! vent de la premiere couche |
| 250 |
REAL zx_lon(iim,jjm+1), zx_lat(iim,jjm+1), zjulian |
zx_alf1 = 1.0 |
| 251 |
REAL tabindx(klon) |
zx_alf2 = 1.0 - zx_alf1 |
| 252 |
REAL debugtab(iim,jjm+1) |
u1lay(i) = u(i, 1)*zx_alf1 + u(i, 2)*zx_alf2 |
| 253 |
LOGICAL first_appel |
v1lay(i) = v(i, 1)*zx_alf1 + v(i, 2)*zx_alf2 |
| 254 |
SAVE first_appel |
END DO |
| 255 |
DATA first_appel/.true./ |
|
| 256 |
LOGICAL debugindex |
! Initialization: |
| 257 |
SAVE debugindex |
rugmer = 0. |
| 258 |
DATA debugindex/.false./ |
cdragh = 0. |
| 259 |
integer idayref |
cdragm = 0. |
| 260 |
REAL t2m(klon,nbsrf), q2m(klon,nbsrf) |
dflux_t = 0. |
| 261 |
REAL u10m(klon,nbsrf), v10m(klon,nbsrf) |
dflux_q = 0. |
| 262 |
c |
zu1 = 0. |
| 263 |
REAL yt2m(klon), yq2m(klon), yu10m(klon) |
zv1 = 0. |
| 264 |
REAL yustar(klon) |
ypct = 0. |
| 265 |
c -- LOOP |
yts = 0. |
| 266 |
REAL yu10mx(klon) |
ysnow = 0. |
| 267 |
REAL yu10my(klon) |
yqsurf = 0. |
| 268 |
REAL ywindsp(klon) |
yrain_f = 0. |
| 269 |
c -- LOOP |
ysnow_f = 0. |
| 270 |
c |
yfder = 0. |
| 271 |
REAL yt10m(klon), yq10m(klon) |
yrugos = 0. |
| 272 |
cIM cf. AM : pbl, hbtm2 (Comme les autres diagnostics on cumule ds physic ce qui |
yu1 = 0. |
| 273 |
c permet de sortir les grdeurs par sous surface) |
yv1 = 0. |
| 274 |
REAL pblh(klon,nbsrf) |
yrads = 0. |
| 275 |
REAL plcl(klon,nbsrf) |
ypaprs = 0. |
| 276 |
REAL capCL(klon,nbsrf) |
ypplay = 0. |
| 277 |
REAL oliqCL(klon,nbsrf) |
ydelp = 0. |
| 278 |
REAL cteiCL(klon,nbsrf) |
yu = 0. |
| 279 |
REAL pblT(klon,nbsrf) |
yv = 0. |
| 280 |
REAL therm(klon,nbsrf) |
yt = 0. |
| 281 |
REAL trmb1(klon,nbsrf) |
yq = 0. |
| 282 |
REAL trmb2(klon,nbsrf) |
y_dflux_t = 0. |
| 283 |
REAL trmb3(klon,nbsrf) |
y_dflux_q = 0. |
| 284 |
REAL ypblh(klon) |
ytsoil = 999999. |
| 285 |
REAL ylcl(klon) |
yrugoro = 0. |
| 286 |
REAL ycapCL(klon) |
d_ts = 0. |
| 287 |
REAL yoliqCL(klon) |
yfluxlat = 0. |
| 288 |
REAL ycteiCL(klon) |
flux_t = 0. |
| 289 |
REAL ypblT(klon) |
flux_q = 0. |
| 290 |
REAL ytherm(klon) |
flux_u = 0. |
| 291 |
REAL ytrmb1(klon) |
flux_v = 0. |
| 292 |
REAL ytrmb2(klon) |
d_t = 0. |
| 293 |
REAL ytrmb3(klon) |
d_q = 0. |
| 294 |
REAL y_cd_h(klon), y_cd_m(klon) |
d_u = 0. |
| 295 |
c REAL ygamt(klon,2:klev) ! contre-gradient pour temperature |
d_v = 0. |
| 296 |
c REAL ygamq(klon,2:klev) ! contre-gradient pour humidite |
ycoefh = 0. |
| 297 |
REAL uzon(klon), vmer(klon) |
|
| 298 |
REAL tair1(klon), qair1(klon), tairsol(klon) |
! Initialisation des "pourcentages potentiels". On consid\`ere ici qu'on |
| 299 |
REAL psfce(klon), patm(klon) |
! peut avoir potentiellement de la glace sur tout le domaine oc\'eanique |
| 300 |
c |
! (\`a affiner) |
| 301 |
REAL qairsol(klon), zgeo1(klon) |
|
| 302 |
REAL rugo1(klon) |
pctsrf_pot(:, is_ter) = pctsrf(:, is_ter) |
| 303 |
c |
pctsrf_pot(:, is_lic) = pctsrf(:, is_lic) |
| 304 |
LOGICAL zxli ! utiliser un jeu de fonctions simples |
pctsrf_pot(:, is_oce) = 1. - zmasq |
| 305 |
PARAMETER (zxli=.FALSE.) |
pctsrf_pot(:, is_sic) = 1. - zmasq |
| 306 |
c |
|
| 307 |
REAL zt, zqs, zdelta, zcor |
! Tester si c'est le moment de lire le fichier: |
| 308 |
REAL t_coup |
if (mod(itap - 1, lmt_pas) == 0) then |
| 309 |
PARAMETER(t_coup=273.15) |
CALL interfoce_lim(jour, pctsrf_new_oce, pctsrf_new_sic) |
| 310 |
C |
endif |
| 311 |
character (len = 20) :: modname = 'clmain' |
|
| 312 |
LOGICAL check |
! Boucler sur toutes les sous-fractions du sol: |
| 313 |
PARAMETER (check=.false.) |
|
| 314 |
|
loop_surface: DO nsrf = 1, nbsrf |
| 315 |
|
! Chercher les indices : |
| 316 |
c initialisation Anne |
ni = 0 |
| 317 |
ytherm(:) = 0. |
knon = 0 |
| 318 |
C |
DO i = 1, klon |
| 319 |
if (check) THEN |
! Pour d\'eterminer le domaine \`a traiter, on utilise les surfaces |
| 320 |
write(*,*) modname,' klon=',klon |
! "potentielles" |
| 321 |
CC call flush(6) |
IF (pctsrf_pot(i, nsrf) > epsfra) THEN |
| 322 |
endif |
knon = knon + 1 |
| 323 |
IF (debugindex .and. first_appel) THEN |
ni(knon) = i |
| 324 |
first_appel=.false. |
END IF |
| 325 |
! |
END DO |
| 326 |
! initialisation sorties netcdf |
|
| 327 |
! |
if_knon: IF (knon /= 0) then |
| 328 |
idayref = day_ini |
DO j = 1, knon |
| 329 |
CALL ymds2ju(annee_ref, 1, idayref, 0.0, zjulian) |
i = ni(j) |
| 330 |
CALL gr_fi_ecrit(1,klon,iim,jjm+1,rlon,zx_lon) |
ypct(j) = pctsrf(i, nsrf) |
| 331 |
DO i = 1, iim |
yts(j) = ts(i, nsrf) |
| 332 |
zx_lon(i,1) = rlon(i+1) |
ysnow(j) = snow(i, nsrf) |
| 333 |
zx_lon(i,jjm+1) = rlon(i+1) |
yqsurf(j) = qsurf(i, nsrf) |
| 334 |
ENDDO |
yalb(j) = falbe(i, nsrf) |
| 335 |
CALL gr_fi_ecrit(1,klon,iim,jjm+1,rlat,zx_lat) |
yrain_f(j) = rain_fall(i) |
| 336 |
cldebug='sous_index' |
ysnow_f(j) = snow_f(i) |
| 337 |
CALL histbeg_totreg(cldebug, iim,zx_lon(:,1),jjm+1, |
yagesno(j) = agesno(i, nsrf) |
| 338 |
$ zx_lat(1,:),1,iim,1,jjm |
yfder(j) = fder(i) |
| 339 |
$ +1, itau_phy,zjulian,dtime,nhoridbg,nidbg) |
yrugos(j) = rugos(i, nsrf) |
| 340 |
! no vertical axis |
yrugoro(j) = rugoro(i) |
| 341 |
cl_surf(1)='ter' |
yu1(j) = u1lay(i) |
| 342 |
cl_surf(2)='lic' |
yv1(j) = v1lay(i) |
| 343 |
cl_surf(3)='oce' |
yrads(j) = solsw(i, nsrf) + sollw(i, nsrf) |
| 344 |
cl_surf(4)='sic' |
ypaprs(j, klev+1) = paprs(i, klev+1) |
| 345 |
DO nsrf=1,nbsrf |
y_run_off_lic_0(j) = run_off_lic_0(i) |
| 346 |
CALL histdef(nidbg, cl_surf(nsrf),cl_surf(nsrf), "-",iim, |
END DO |
| 347 |
$ jjm+1,nhoridbg, 1, 1, 1, -99, 32, "inst", dtime,dtime) |
|
| 348 |
END DO |
! For continent, copy soil water content |
| 349 |
CALL histend(nidbg) |
IF (nsrf == is_ter) THEN |
| 350 |
CALL histsync(nidbg) |
yqsol(:knon) = qsol(ni(:knon)) |
| 351 |
ENDIF |
ELSE |
| 352 |
|
yqsol = 0. |
| 353 |
DO k = 1, klev ! epaisseur de couche |
END IF |
| 354 |
DO i = 1, klon |
|
| 355 |
delp(i,k) = paprs(i,k)-paprs(i,k+1) |
DO k = 1, nsoilmx |
| 356 |
ENDDO |
DO j = 1, knon |
| 357 |
ENDDO |
i = ni(j) |
| 358 |
DO i = 1, klon ! vent de la premiere couche |
ytsoil(j, k) = ftsoil(i, k, nsrf) |
| 359 |
zx_alf1 = 1.0 |
END DO |
| 360 |
zx_alf2 = 1.0 - zx_alf1 |
END DO |
| 361 |
u1lay(i) = u(i,1)*zx_alf1 + u(i,2)*zx_alf2 |
|
| 362 |
v1lay(i) = v(i,1)*zx_alf1 + v(i,2)*zx_alf2 |
DO k = 1, klev |
| 363 |
ENDDO |
DO j = 1, knon |
| 364 |
c |
i = ni(j) |
| 365 |
c initialisation: |
ypaprs(j, k) = paprs(i, k) |
| 366 |
c |
ypplay(j, k) = pplay(i, k) |
| 367 |
DO i = 1, klon |
ydelp(j, k) = delp(i, k) |
| 368 |
rugmer(i) = 0.0 |
yu(j, k) = u(i, k) |
| 369 |
cdragh(i) = 0.0 |
yv(j, k) = v(i, k) |
| 370 |
cdragm(i) = 0.0 |
yt(j, k) = t(i, k) |
| 371 |
dflux_t(i) = 0.0 |
yq(j, k) = q(i, k) |
| 372 |
dflux_q(i) = 0.0 |
END DO |
| 373 |
zu1(i) = 0.0 |
END DO |
| 374 |
zv1(i) = 0.0 |
|
| 375 |
ENDDO |
! calculer Cdrag et les coefficients d'echange |
| 376 |
ypct = 0.0 |
CALL coefkz(nsrf, knon, ypaprs, ypplay, ksta, ksta_ter, yts, yrugos, & |
| 377 |
yts = 0.0 |
yu, yv, yt, yq, yqsurf, coefm(:knon, :), coefh(:knon, :)) |
| 378 |
ysnow = 0.0 |
IF (iflag_pbl == 1) THEN |
| 379 |
yqsurf = 0.0 |
CALL coefkz2(nsrf, knon, ypaprs, ypplay, yt, ycoefm0, ycoefh0) |
| 380 |
yalb = 0.0 |
coefm(:knon, :) = max(coefm(:knon, :), ycoefm0(:knon, :)) |
| 381 |
yalblw = 0.0 |
coefh(:knon, :) = max(coefh(:knon, :), ycoefh0(:knon, :)) |
| 382 |
yrain_f = 0.0 |
END IF |
| 383 |
ysnow_f = 0.0 |
|
| 384 |
yfder = 0.0 |
! on met un seuil pour coefm et coefh |
| 385 |
ytaux = 0.0 |
IF (nsrf == is_oce) THEN |
| 386 |
ytauy = 0.0 |
coefm(:knon, 1) = min(coefm(:knon, 1), cdmmax) |
| 387 |
ysolsw = 0.0 |
coefh(:knon, 1) = min(coefh(:knon, 1), cdhmax) |
| 388 |
ysollw = 0.0 |
END IF |
| 389 |
ysollwdown = 0.0 |
|
| 390 |
yrugos = 0.0 |
IF (ok_kzmin) THEN |
| 391 |
yu1 = 0.0 |
! Calcul d'une diffusion minimale pour les conditions tres stables |
| 392 |
yv1 = 0.0 |
CALL coefkzmin(knon, ypaprs, ypplay, yu, yv, yt, yq, & |
| 393 |
yrads = 0.0 |
coefm(:knon, 1), ycoefm0, ycoefh0) |
| 394 |
ypaprs = 0.0 |
coefm(:knon, :) = max(coefm(:knon, :), ycoefm0(:knon, :)) |
| 395 |
ypplay = 0.0 |
coefh(:knon, :) = max(coefh(:knon, :), ycoefh0(:knon, :)) |
| 396 |
ydelp = 0.0 |
END IF |
| 397 |
yu = 0.0 |
|
| 398 |
yv = 0.0 |
IF (iflag_pbl >= 3) THEN |
| 399 |
yt = 0.0 |
! Mellor et Yamada adapt\'e \`a Mars, Richard Fournier et |
| 400 |
yq = 0.0 |
! Fr\'ed\'eric Hourdin |
| 401 |
pctsrf_new = 0.0 |
yzlay(:knon, 1) = rd * yt(:knon, 1) / (0.5 * (ypaprs(:knon, 1) & |
| 402 |
y_flux_u = 0.0 |
+ ypplay(:knon, 1))) & |
| 403 |
y_flux_v = 0.0 |
* (ypaprs(:knon, 1) - ypplay(:knon, 1)) / rg |
| 404 |
C$$ PB |
DO k = 2, klev |
| 405 |
y_dflux_t = 0.0 |
yzlay(1:knon, k) = yzlay(1:knon, k-1) & |
| 406 |
y_dflux_q = 0.0 |
+ rd * 0.5 * (yt(1:knon, k-1) + yt(1:knon, k)) & |
| 407 |
ytsoil = 999999. |
/ ypaprs(1:knon, k) & |
| 408 |
yrugoro = 0. |
* (ypplay(1:knon, k-1) - ypplay(1:knon, k)) / rg |
| 409 |
c -- LOOP |
END DO |
| 410 |
yu10mx = 0.0 |
DO k = 1, klev |
| 411 |
yu10my = 0.0 |
yteta(1:knon, k) = yt(1:knon, k)*(ypaprs(1:knon, 1) & |
| 412 |
ywindsp = 0.0 |
/ ypplay(1:knon, k))**rkappa * (1.+0.61*yq(1:knon, k)) |
| 413 |
c -- LOOP |
END DO |
| 414 |
DO nsrf = 1, nbsrf |
yzlev(1:knon, 1) = 0. |
| 415 |
DO i = 1, klon |
yzlev(:knon, klev+1) = 2. * yzlay(:knon, klev) & |
| 416 |
d_ts(i,nsrf) = 0.0 |
- yzlay(:knon, klev - 1) |
| 417 |
ENDDO |
DO k = 2, klev |
| 418 |
END DO |
yzlev(1:knon, k) = 0.5*(yzlay(1:knon, k)+yzlay(1:knon, k-1)) |
| 419 |
C§§§ PB |
END DO |
| 420 |
yfluxlat=0. |
DO k = 1, klev + 1 |
| 421 |
flux_t = 0. |
DO j = 1, knon |
| 422 |
flux_q = 0. |
i = ni(j) |
| 423 |
flux_u = 0. |
yq2(j, k) = q2(i, k, nsrf) |
| 424 |
flux_v = 0. |
END DO |
| 425 |
DO k = 1, klev |
END DO |
| 426 |
DO i = 1, klon |
|
| 427 |
d_t(i,k) = 0.0 |
CALL ustarhb(knon, yu, yv, coefm(:knon, 1), yustar) |
| 428 |
d_q(i,k) = 0.0 |
IF (prt_level > 9) PRINT *, 'USTAR = ', yustar |
| 429 |
c$$$ flux_t(i,k) = 0.0 |
|
| 430 |
c$$$ flux_q(i,k) = 0.0 |
! iflag_pbl peut \^etre utilis\'e comme longueur de m\'elange |
| 431 |
d_u(i,k) = 0.0 |
|
| 432 |
d_v(i,k) = 0.0 |
IF (iflag_pbl >= 11) THEN |
| 433 |
c$$$ flux_u(i,k) = 0.0 |
CALL vdif_kcay(knon, dtime, rg, ypaprs, yzlev, yzlay, yu, yv, & |
| 434 |
c$$$ flux_v(i,k) = 0.0 |
yteta, coefm(:knon, 1), yq2, q2diag, ykmm, ykmn, yustar, & |
| 435 |
zcoefh(i,k) = 0.0 |
iflag_pbl) |
| 436 |
ENDDO |
ELSE |
| 437 |
ENDDO |
CALL yamada4(knon, dtime, rg, yzlev, yzlay, yu, yv, yteta, & |
| 438 |
cAA IF (itr.GE.1) THEN |
coefm(:knon, 1), yq2, ykmm, ykmn, ykmq, yustar, iflag_pbl) |
| 439 |
cAA DO it = 1, itr |
END IF |
| 440 |
cAA DO k = 1, klev |
|
| 441 |
cAA DO i = 1, klon |
coefm(:knon, 2:) = ykmm(:knon, 2:klev) |
| 442 |
cAA d_tr(i,k,it) = 0.0 |
coefh(:knon, 2:) = ykmn(:knon, 2:klev) |
| 443 |
cAA ENDDO |
END IF |
| 444 |
cAA ENDDO |
|
| 445 |
cAA ENDDO |
! calculer la diffusion des vitesses "u" et "v" |
| 446 |
cAA ENDIF |
CALL clvent(knon, dtime, yu1, yv1, coefm(:knon, :), yt, yu, ypaprs, & |
| 447 |
|
ypplay, ydelp, y_d_u, y_flux_u(:knon)) |
| 448 |
c |
CALL clvent(knon, dtime, yu1, yv1, coefm(:knon, :), yt, yv, ypaprs, & |
| 449 |
c Boucler sur toutes les sous-fractions du sol: |
ypplay, ydelp, y_d_v, y_flux_v(:knon)) |
| 450 |
c |
|
| 451 |
C Initialisation des "pourcentages potentiels". On considere ici qu'on |
! calculer la diffusion de "q" et de "h" |
| 452 |
C peut avoir potentiellementdela glace sur tout le domaine oceanique |
CALL clqh(dtime, jour, firstcal, rlat, nsrf, ni(:knon), ytsoil, & |
| 453 |
C (a affiner) |
yqsol, rmu0, yrugos, yrugoro, yu1, yv1, coefh(:knon, :), yt, & |
| 454 |
|
yq, yts, ypaprs, ypplay, ydelp, yrads, yalb(:knon), ysnow, & |
| 455 |
pctsrf_pot = pctsrf |
yqsurf, yrain_f, ysnow_f, yfder, yfluxlat, pctsrf_new_sic, & |
| 456 |
pctsrf_pot(:,is_oce) = 1. - zmasq(:) |
yagesno(:knon), y_d_t, y_d_q, y_d_ts(:knon), yz0_new, & |
| 457 |
pctsrf_pot(:,is_sic) = 1. - zmasq(:) |
y_flux_t(:knon), y_flux_q(:knon), y_dflux_t, y_dflux_q, & |
| 458 |
|
y_fqcalving, y_ffonte, y_run_off_lic_0) |
| 459 |
DO 99999 nsrf = 1, nbsrf |
|
| 460 |
|
! calculer la longueur de rugosite sur ocean |
| 461 |
c chercher les indices: |
yrugm = 0. |
| 462 |
DO j = 1, klon |
IF (nsrf == is_oce) THEN |
| 463 |
ni(j) = 0 |
DO j = 1, knon |
| 464 |
ENDDO |
yrugm(j) = 0.018*coefm(j, 1)*(yu1(j)**2+yv1(j)**2)/rg + & |
| 465 |
knon = 0 |
0.11*14E-6/sqrt(coefm(j, 1)*(yu1(j)**2+yv1(j)**2)) |
| 466 |
DO i = 1, klon |
yrugm(j) = max(1.5E-05, yrugm(j)) |
| 467 |
|
END DO |
| 468 |
C pour determiner le domaine a traiter on utilise les surfaces "potentielles" |
END IF |
| 469 |
C |
DO j = 1, knon |
| 470 |
IF (pctsrf_pot(i,nsrf).GT.epsfra) THEN |
y_dflux_t(j) = y_dflux_t(j)*ypct(j) |
| 471 |
knon = knon + 1 |
y_dflux_q(j) = y_dflux_q(j)*ypct(j) |
| 472 |
ni(knon) = i |
yu1(j) = yu1(j)*ypct(j) |
| 473 |
ENDIF |
yv1(j) = yv1(j)*ypct(j) |
| 474 |
ENDDO |
END DO |
| 475 |
c |
|
| 476 |
if (check) THEN |
DO k = 1, klev |
| 477 |
write(*,*)'CLMAIN, nsrf, knon =',nsrf, knon |
DO j = 1, knon |
| 478 |
CC call flush(6) |
i = ni(j) |
| 479 |
endif |
coefh(j, k) = coefh(j, k)*ypct(j) |
| 480 |
c |
coefm(j, k) = coefm(j, k)*ypct(j) |
| 481 |
c variables pour avoir une sortie IOIPSL des INDEX |
y_d_t(j, k) = y_d_t(j, k)*ypct(j) |
| 482 |
c |
y_d_q(j, k) = y_d_q(j, k)*ypct(j) |
| 483 |
IF (debugindex) THEN |
y_d_u(j, k) = y_d_u(j, k)*ypct(j) |
| 484 |
tabindx(:)=0. |
y_d_v(j, k) = y_d_v(j, k)*ypct(j) |
| 485 |
c tabindx(1:knon)=(/FLOAT(i),i=1:knon/) |
END DO |
| 486 |
DO i=1,knon |
END DO |
| 487 |
tabindx(1:knon)=FLOAT(i) |
|
| 488 |
END DO |
DO j = 1, knon |
| 489 |
debugtab(:,:)=0. |
i = ni(j) |
| 490 |
ndexbg(:)=0 |
flux_t(i, nsrf) = y_flux_t(j) |
| 491 |
CALL gath2cpl(tabindx,debugtab,klon,knon,iim,jjm,ni) |
flux_q(i, nsrf) = y_flux_q(j) |
| 492 |
CALL histwrite(nidbg,cl_surf(nsrf),itap,debugtab,iim*(jjm+1) |
flux_u(i, nsrf) = y_flux_u(j) |
| 493 |
$ ,ndexbg) |
flux_v(i, nsrf) = y_flux_v(j) |
| 494 |
ENDIF |
END DO |
| 495 |
IF (knon.EQ.0) GOTO 99999 |
|
| 496 |
DO j = 1, knon |
evap(:, nsrf) = -flux_q(:, nsrf) |
| 497 |
i = ni(j) |
|
| 498 |
ypct(j) = pctsrf(i,nsrf) |
falbe(:, nsrf) = 0. |
| 499 |
yts(j) = ts(i,nsrf) |
snow(:, nsrf) = 0. |
| 500 |
cIM "slab" ocean |
qsurf(:, nsrf) = 0. |
| 501 |
c PRINT *, 'tslab = ', i, tslab(i) |
rugos(:, nsrf) = 0. |
| 502 |
ytslab(i) = tslab(i) |
fluxlat(:, nsrf) = 0. |
| 503 |
c |
DO j = 1, knon |
| 504 |
ysnow(j) = snow(i,nsrf) |
i = ni(j) |
| 505 |
yqsurf(j) = qsurf(i,nsrf) |
d_ts(i, nsrf) = y_d_ts(j) |
| 506 |
yalb(j) = albe(i,nsrf) |
falbe(i, nsrf) = yalb(j) |
| 507 |
yalblw(j) = alblw(i,nsrf) |
snow(i, nsrf) = ysnow(j) |
| 508 |
yrain_f(j) = rain_f(i) |
qsurf(i, nsrf) = yqsurf(j) |
| 509 |
ysnow_f(j) = snow_f(i) |
rugos(i, nsrf) = yz0_new(j) |
| 510 |
yagesno(j) = agesno(i,nsrf) |
fluxlat(i, nsrf) = yfluxlat(j) |
| 511 |
yfder(j) = fder(i) |
IF (nsrf == is_oce) THEN |
| 512 |
ytaux(j) = flux_u(i,1,nsrf) |
rugmer(i) = yrugm(j) |
| 513 |
ytauy(j) = flux_v(i,1,nsrf) |
rugos(i, nsrf) = yrugm(j) |
| 514 |
ysolsw(j) = solsw(i,nsrf) |
END IF |
| 515 |
ysollw(j) = sollw(i,nsrf) |
agesno(i, nsrf) = yagesno(j) |
| 516 |
ysollwdown(j) = sollwdown(i) |
fqcalving(i, nsrf) = y_fqcalving(j) |
| 517 |
yrugos(j) = rugos(i,nsrf) |
ffonte(i, nsrf) = y_ffonte(j) |
| 518 |
yrugoro(j) = rugoro(i) |
cdragh(i) = cdragh(i) + coefh(j, 1) |
| 519 |
yu1(j) = u1lay(i) |
cdragm(i) = cdragm(i) + coefm(j, 1) |
| 520 |
yv1(j) = v1lay(i) |
dflux_t(i) = dflux_t(i) + y_dflux_t(j) |
| 521 |
yrads(j) = ysolsw(j)+ ysollw(j) |
dflux_q(i) = dflux_q(i) + y_dflux_q(j) |
| 522 |
ypaprs(j,klev+1) = paprs(i,klev+1) |
zu1(i) = zu1(i) + yu1(j) |
| 523 |
y_run_off_lic_0(j) = run_off_lic_0(i) |
zv1(i) = zv1(i) + yv1(j) |
| 524 |
c -- LOOP |
END DO |
| 525 |
yu10mx(j) = u10m(i,nsrf) |
IF (nsrf == is_ter) THEN |
| 526 |
yu10my(j) = v10m(i,nsrf) |
qsol(ni(:knon)) = yqsol(:knon) |
| 527 |
ywindsp(j) = SQRT(yu10mx(j)*yu10mx(j) + yu10my(j)*yu10my(j) ) |
else IF (nsrf == is_lic) THEN |
| 528 |
c -- LOOP |
DO j = 1, knon |
| 529 |
END DO |
i = ni(j) |
| 530 |
C |
run_off_lic_0(i) = y_run_off_lic_0(j) |
| 531 |
C IF bucket model for continent, copy soil water content |
END DO |
| 532 |
IF ( nsrf .eq. is_ter .and. .not. ok_veget ) THEN |
END IF |
| 533 |
|
|
| 534 |
|
ftsoil(:, :, nsrf) = 0. |
| 535 |
|
DO k = 1, nsoilmx |
| 536 |
|
DO j = 1, knon |
| 537 |
|
i = ni(j) |
| 538 |
|
ftsoil(i, k, nsrf) = ytsoil(j, k) |
| 539 |
|
END DO |
| 540 |
|
END DO |
| 541 |
|
|
| 542 |
|
DO j = 1, knon |
| 543 |
|
i = ni(j) |
| 544 |
|
DO k = 1, klev |
| 545 |
|
d_t(i, k) = d_t(i, k) + y_d_t(j, k) |
| 546 |
|
d_q(i, k) = d_q(i, k) + y_d_q(j, k) |
| 547 |
|
d_u(i, k) = d_u(i, k) + y_d_u(j, k) |
| 548 |
|
d_v(i, k) = d_v(i, k) + y_d_v(j, k) |
| 549 |
|
ycoefh(i, k) = ycoefh(i, k) + coefh(j, k) |
| 550 |
|
END DO |
| 551 |
|
END DO |
| 552 |
|
|
| 553 |
|
! diagnostic t, q a 2m et u, v a 10m |
| 554 |
|
|
| 555 |
|
DO j = 1, knon |
| 556 |
|
i = ni(j) |
| 557 |
|
uzon(j) = yu(j, 1) + y_d_u(j, 1) |
| 558 |
|
vmer(j) = yv(j, 1) + y_d_v(j, 1) |
| 559 |
|
tair1(j) = yt(j, 1) + y_d_t(j, 1) |
| 560 |
|
qair1(j) = yq(j, 1) + y_d_q(j, 1) |
| 561 |
|
zgeo1(j) = rd*tair1(j)/(0.5*(ypaprs(j, 1)+ypplay(j, & |
| 562 |
|
1)))*(ypaprs(j, 1)-ypplay(j, 1)) |
| 563 |
|
tairsol(j) = yts(j) + y_d_ts(j) |
| 564 |
|
rugo1(j) = yrugos(j) |
| 565 |
|
IF (nsrf == is_oce) THEN |
| 566 |
|
rugo1(j) = rugos(i, nsrf) |
| 567 |
|
END IF |
| 568 |
|
psfce(j) = ypaprs(j, 1) |
| 569 |
|
patm(j) = ypplay(j, 1) |
| 570 |
|
|
| 571 |
|
qairsol(j) = yqsurf(j) |
| 572 |
|
END DO |
| 573 |
|
|
| 574 |
|
CALL stdlevvar(klon, knon, nsrf, zxli, uzon, vmer, tair1, qair1, & |
| 575 |
|
zgeo1, tairsol, qairsol, rugo1, psfce, patm, yt2m, yq2m, & |
| 576 |
|
yt10m, yq10m, yu10m, yustar) |
| 577 |
|
|
| 578 |
DO j = 1, knon |
DO j = 1, knon |
| 579 |
i = ni(j) |
i = ni(j) |
| 580 |
yqsol(j) = qsol(i) |
t2m(i, nsrf) = yt2m(j) |
| 581 |
|
q2m(i, nsrf) = yq2m(j) |
| 582 |
|
|
| 583 |
|
! u10m, v10m : composantes du vent a 10m sans spirale de Ekman |
| 584 |
|
u10m(i, nsrf) = (yu10m(j)*uzon(j))/sqrt(uzon(j)**2+vmer(j)**2) |
| 585 |
|
v10m(i, nsrf) = (yu10m(j)*vmer(j))/sqrt(uzon(j)**2+vmer(j)**2) |
| 586 |
|
|
| 587 |
|
END DO |
| 588 |
|
|
| 589 |
|
CALL hbtm(ypaprs, ypplay, yt2m, yq2m, yustar, y_flux_t(:knon), & |
| 590 |
|
y_flux_q(:knon), yu, yv, yt, yq, ypblh(:knon), ycapcl, & |
| 591 |
|
yoliqcl, ycteicl, ypblt, ytherm, ytrmb1, ytrmb2, ytrmb3, ylcl) |
| 592 |
|
|
| 593 |
|
DO j = 1, knon |
| 594 |
|
i = ni(j) |
| 595 |
|
pblh(i, nsrf) = ypblh(j) |
| 596 |
|
plcl(i, nsrf) = ylcl(j) |
| 597 |
|
capcl(i, nsrf) = ycapcl(j) |
| 598 |
|
oliqcl(i, nsrf) = yoliqcl(j) |
| 599 |
|
cteicl(i, nsrf) = ycteicl(j) |
| 600 |
|
pblt(i, nsrf) = ypblt(j) |
| 601 |
|
therm(i, nsrf) = ytherm(j) |
| 602 |
|
trmb1(i, nsrf) = ytrmb1(j) |
| 603 |
|
trmb2(i, nsrf) = ytrmb2(j) |
| 604 |
|
trmb3(i, nsrf) = ytrmb3(j) |
| 605 |
END DO |
END DO |
|
ELSE |
|
|
yqsol(:)=0. |
|
|
ENDIF |
|
|
c$$$ PB ajour pour soil |
|
|
DO k = 1, nsoilmx |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
ytsoil(j,k) = ftsoil(i,k,nsrf) |
|
|
END DO |
|
|
END DO |
|
|
DO k = 1, klev |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
ypaprs(j,k) = paprs(i,k) |
|
|
ypplay(j,k) = pplay(i,k) |
|
|
ydelp(j,k) = delp(i,k) |
|
|
yu(j,k) = u(i,k) |
|
|
yv(j,k) = v(i,k) |
|
|
yt(j,k) = t(i,k) |
|
|
yq(j,k) = q(i,k) |
|
|
ENDDO |
|
|
ENDDO |
|
|
c |
|
|
c |
|
|
c calculer Cdrag et les coefficients d'echange |
|
|
CALL coefkz(nsrf, knon, ypaprs, ypplay, |
|
|
cIM 261103 |
|
|
. ksta, ksta_ter, |
|
|
cIM 261103 |
|
|
. yts, yrugos, yu, yv, yt, yq, |
|
|
. yqsurf, |
|
|
. ycoefm, ycoefh) |
|
|
cIM 081204 BEG |
|
|
cCR test |
|
|
if (iflag_pbl.eq.1) then |
|
|
cIM 081204 END |
|
|
CALL coefkz2(nsrf, knon, ypaprs, ypplay,yt, |
|
|
. ycoefm0, ycoefh0) |
|
|
DO k = 1, klev |
|
|
DO i = 1, knon |
|
|
ycoefm(i,k) = MAX(ycoefm(i,k),ycoefm0(i,k)) |
|
|
ycoefh(i,k) = MAX(ycoefh(i,k),ycoefh0(i,k)) |
|
|
ENDDO |
|
|
ENDDO |
|
|
endif |
|
|
c |
|
|
cIM cf JLD : on seuille ycoefm et ycoefh |
|
|
if (nsrf.eq.is_oce) then |
|
|
do j=1,knon |
|
|
c ycoefm(j,1)=min(ycoefm(j,1),1.1E-3) |
|
|
ycoefm(j,1)=min(ycoefm(j,1),cdmmax) |
|
|
c ycoefh(j,1)=min(ycoefh(j,1),1.1E-3) |
|
|
ycoefh(j,1)=min(ycoefh(j,1),cdhmax) |
|
|
enddo |
|
|
endif |
|
|
|
|
|
c |
|
|
cIM: 261103 |
|
|
if (ok_kzmin) THEN |
|
|
cIM cf FH: 201103 BEG |
|
|
c Calcul d'une diffusion minimale pour les conditions tres stables. |
|
|
call coefkzmin(knon,ypaprs,ypplay,yu,yv,yt,yq,ycoefm |
|
|
. ,ycoefm0,ycoefh0) |
|
|
c call dump2d(iim,jjm-1,ycoefm(2:klon-1,2), 'KZ ') |
|
|
c call dump2d(iim,jjm-1,ycoefm0(2:klon-1,2),'KZMIN ') |
|
|
|
|
|
if ( 1.eq.1 ) then |
|
|
DO k = 1, klev |
|
|
DO i = 1, knon |
|
|
ycoefm(i,k) = MAX(ycoefm(i,k),ycoefm0(i,k)) |
|
|
ycoefh(i,k) = MAX(ycoefh(i,k),ycoefh0(i,k)) |
|
|
ENDDO |
|
|
ENDDO |
|
|
endif |
|
|
cIM cf FH: 201103 END |
|
|
endif !ok_kzmin |
|
|
cIM: 261103 |
|
|
|
|
|
|
|
|
IF (iflag_pbl.ge.3) then |
|
|
|
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
c MELLOR ET YAMADA adapte a Mars Richard Fournier et Frederic Hourdin |
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
|
|
|
yzlay(1:knon,1)= |
|
|
. RD*yt(1:knon,1)/(0.5*(ypaprs(1:knon,1)+ypplay(1:knon,1))) |
|
|
. *(ypaprs(1:knon,1)-ypplay(1:knon,1))/RG |
|
|
do k=2,klev |
|
|
yzlay(1:knon,k)= |
|
|
. yzlay(1:knon,k-1)+RD*0.5*(yt(1:knon,k-1)+yt(1:knon,k)) |
|
|
. /ypaprs(1:knon,k)*(ypplay(1:knon,k-1)-ypplay(1:knon,k))/RG |
|
|
enddo |
|
|
do k=1,klev |
|
|
yteta(1:knon,k)= |
|
|
. yt(1:knon,k)*(ypaprs(1:knon,1)/ypplay(1:knon,k))**rkappa |
|
|
. *(1.+0.61*yq(1:knon,k)) |
|
|
enddo |
|
|
yzlev(1:knon,1)=0. |
|
|
yzlev(1:knon,klev+1)=2.*yzlay(1:knon,klev)-yzlay(1:knon,klev-1) |
|
|
do k=2,klev |
|
|
yzlev(1:knon,k)=0.5*(yzlay(1:knon,k)+yzlay(1:knon,k-1)) |
|
|
enddo |
|
|
DO k = 1, klev+1 |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
yq2(j,k)=q2(i,k,nsrf) |
|
|
enddo |
|
|
enddo |
|
|
|
|
|
|
|
|
c Bug introduit volontairement pour converger avec les resultats |
|
|
c du papier sur les thermiques. |
|
|
if (1.eq.1) then |
|
|
y_cd_m(1:knon) = ycoefm(1:knon,1) |
|
|
y_cd_h(1:knon) = ycoefh(1:knon,1) |
|
|
else |
|
|
y_cd_h(1:knon) = ycoefm(1:knon,1) |
|
|
y_cd_m(1:knon) = ycoefh(1:knon,1) |
|
|
endif |
|
|
call ustarhb(knon,yu,yv,y_cd_m, yustar) |
|
|
|
|
|
if (prt_level > 9) THEN |
|
|
WRITE(lunout,*)'USTAR = ',yustar |
|
|
ENDIF |
|
|
|
|
|
c iflag_pbl peut etre utilise comme longuer de melange |
|
|
|
|
|
if (iflag_pbl.ge.11) then |
|
|
call vdif_kcay(knon,dtime,rg,rd,ypaprs,yt |
|
|
s ,yzlev,yzlay,yu,yv,yteta |
|
|
s ,y_cd_m,yq2,q2diag,ykmm,ykmn,yustar, |
|
|
s iflag_pbl) |
|
|
else |
|
|
call yamada4(knon,dtime,rg,rd,ypaprs,yt |
|
|
s ,yzlev,yzlay,yu,yv,yteta |
|
|
s ,y_cd_m,yq2,ykmm,ykmn,ykmq,yustar, |
|
|
s iflag_pbl) |
|
|
endif |
|
|
|
|
|
ycoefm(1:knon,1)=y_cd_m(1:knon) |
|
|
ycoefh(1:knon,1)=y_cd_h(1:knon) |
|
|
ycoefm(1:knon,2:klev)=ykmm(1:knon,2:klev) |
|
|
ycoefh(1:knon,2:klev)=ykmn(1:knon,2:klev) |
|
|
|
|
|
|
|
|
ENDIF |
|
|
|
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
c calculer la diffusion des vitesses "u" et "v" |
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
|
|
|
CALL clvent(knon,dtime,yu1,yv1,ycoefm,yt,yu,ypaprs,ypplay,ydelp, |
|
|
s y_d_u,y_flux_u) |
|
|
CALL clvent(knon,dtime,yu1,yv1,ycoefm,yt,yv,ypaprs,ypplay,ydelp, |
|
|
s y_d_v,y_flux_v) |
|
|
|
|
|
c pour le couplage |
|
|
ytaux = y_flux_u(:,1) |
|
|
ytauy = y_flux_v(:,1) |
|
|
|
|
|
c FH modif sur le cdrag temperature |
|
|
c$$$PB : déplace dans clcdrag |
|
|
c$$$ do i=1,knon |
|
|
c$$$ ycoefh(i,1)=ycoefm(i,1)*0.8 |
|
|
c$$$ enddo |
|
|
|
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
c calculer la diffusion de "q" et de "h" |
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
CALL clqh(dtime, itap, date0,jour, debut,lafin, |
|
|
e rlon, rlat, cufi, cvfi, |
|
|
e knon, nsrf, ni, pctsrf, |
|
|
e soil_model, ytsoil,yqsol, |
|
|
e ok_veget, ocean, npas, nexca, |
|
|
e rmu0, co2_ppm, yrugos, yrugoro, |
|
|
e yu1, yv1, ycoefh, |
|
|
e yt,yq,yts,ypaprs,ypplay, |
|
|
e ydelp,yrads,yalb, yalblw, ysnow, yqsurf, |
|
|
e yrain_f, ysnow_f, yfder, ytaux, ytauy, |
|
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c -- LOOP |
|
|
e ywindsp, |
|
|
c -- LOOP |
|
|
c$$$ e ysollw, ysolsw, |
|
|
e ysollw, ysollwdown, ysolsw,yfluxlat, |
|
|
s pctsrf_new, yagesno, |
|
|
s y_d_t, y_d_q, y_d_ts, yz0_new, |
|
|
s y_flux_t, y_flux_q, y_dflux_t, y_dflux_q, |
|
|
s y_fqcalving,y_ffonte,y_run_off_lic_0, |
|
|
cIM "slab" ocean |
|
|
s y_flux_o, y_flux_g, ytslab, y_seaice) |
|
|
c |
|
|
c calculer la longueur de rugosite sur ocean |
|
|
yrugm=0. |
|
|
IF (nsrf.EQ.is_oce) THEN |
|
|
DO j = 1, knon |
|
|
yrugm(j) = 0.018*ycoefm(j,1) * (yu1(j)**2+yv1(j)**2)/RG |
|
|
$ + 0.11*14e-6 / sqrt(ycoefm(j,1) * (yu1(j)**2+yv1(j)**2)) |
|
|
yrugm(j) = MAX(1.5e-05,yrugm(j)) |
|
|
ENDDO |
|
|
ENDIF |
|
|
DO j = 1, knon |
|
|
y_dflux_t(j) = y_dflux_t(j) * ypct(j) |
|
|
y_dflux_q(j) = y_dflux_q(j) * ypct(j) |
|
|
yu1(j) = yu1(j) * ypct(j) |
|
|
yv1(j) = yv1(j) * ypct(j) |
|
|
ENDDO |
|
|
c |
|
|
DO k = 1, klev |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
ycoefh(j,k) = ycoefh(j,k) * ypct(j) |
|
|
ycoefm(j,k) = ycoefm(j,k) * ypct(j) |
|
|
y_d_t(j,k) = y_d_t(j,k) * ypct(j) |
|
|
y_d_q(j,k) = y_d_q(j,k) * ypct(j) |
|
|
C§§§ PB |
|
|
flux_t(i,k,nsrf) = y_flux_t(j,k) |
|
|
flux_q(i,k,nsrf) = y_flux_q(j,k) |
|
|
flux_u(i,k,nsrf) = y_flux_u(j,k) |
|
|
flux_v(i,k,nsrf) = y_flux_v(j,k) |
|
|
c$$$ PB y_flux_t(j,k) = y_flux_t(j,k) * ypct(j) |
|
|
c$$$ PB y_flux_q(j,k) = y_flux_q(j,k) * ypct(j) |
|
|
y_d_u(j,k) = y_d_u(j,k) * ypct(j) |
|
|
y_d_v(j,k) = y_d_v(j,k) * ypct(j) |
|
|
c$$$ PB y_flux_u(j,k) = y_flux_u(j,k) * ypct(j) |
|
|
c$$$ PB y_flux_v(j,k) = y_flux_v(j,k) * ypct(j) |
|
|
ENDDO |
|
|
ENDDO |
|
|
|
|
|
|
|
|
evap(:,nsrf) = - flux_q(:,1,nsrf) |
|
|
c |
|
|
albe(:, nsrf) = 0. |
|
|
alblw(:, nsrf) = 0. |
|
|
snow(:, nsrf) = 0. |
|
|
qsurf(:, nsrf) = 0. |
|
|
rugos(:, nsrf) = 0. |
|
|
fluxlat(:,nsrf) = 0. |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
d_ts(i,nsrf) = y_d_ts(j) |
|
|
albe(i,nsrf) = yalb(j) |
|
|
alblw(i,nsrf) = yalblw(j) |
|
|
snow(i,nsrf) = ysnow(j) |
|
|
qsurf(i,nsrf) = yqsurf(j) |
|
|
rugos(i,nsrf) = yz0_new(j) |
|
|
fluxlat(i,nsrf) = yfluxlat(j) |
|
|
c$$$ pb rugmer(i) = yrugm(j) |
|
|
IF (nsrf .EQ. is_oce) then |
|
|
rugmer(i) = yrugm(j) |
|
|
rugos(i,nsrf) = yrugm(j) |
|
|
endif |
|
|
cIM cf JLD ?? |
|
|
agesno(i,nsrf) = yagesno(j) |
|
|
fqcalving(i,nsrf) = y_fqcalving(j) |
|
|
ffonte(i,nsrf) = y_ffonte(j) |
|
|
cdragh(i) = cdragh(i) + ycoefh(j,1) |
|
|
cdragm(i) = cdragm(i) + ycoefm(j,1) |
|
|
dflux_t(i) = dflux_t(i) + y_dflux_t(j) |
|
|
dflux_q(i) = dflux_q(i) + y_dflux_q(j) |
|
|
zu1(i) = zu1(i) + yu1(j) |
|
|
zv1(i) = zv1(i) + yv1(j) |
|
|
END DO |
|
|
IF ( nsrf .eq. is_ter ) THEN |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
qsol(i) = yqsol(j) |
|
|
END DO |
|
|
END IF |
|
|
IF ( nsrf .eq. is_lic ) THEN |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
run_off_lic_0(i) = y_run_off_lic_0(j) |
|
|
END DO |
|
|
END IF |
|
|
c$$$ PB ajout pour soil |
|
|
ftsoil(:,:,nsrf) = 0. |
|
|
DO k = 1, nsoilmx |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
ftsoil(i, k, nsrf) = ytsoil(j,k) |
|
|
END DO |
|
|
END DO |
|
|
c |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
DO k = 1, klev |
|
|
d_t(i,k) = d_t(i,k) + y_d_t(j,k) |
|
|
d_q(i,k) = d_q(i,k) + y_d_q(j,k) |
|
|
c$$$ PB flux_t(i,k) = flux_t(i,k) + y_flux_t(j,k) |
|
|
c$$$ flux_q(i,k) = flux_q(i,k) + y_flux_q(j,k) |
|
|
d_u(i,k) = d_u(i,k) + y_d_u(j,k) |
|
|
d_v(i,k) = d_v(i,k) + y_d_v(j,k) |
|
|
c$$$ PB flux_u(i,k) = flux_u(i,k) + y_flux_u(j,k) |
|
|
c$$$ flux_v(i,k) = flux_v(i,k) + y_flux_v(j,k) |
|
|
zcoefh(i,k) = zcoefh(i,k) + ycoefh(j,k) |
|
|
ENDDO |
|
|
ENDDO |
|
|
c |
|
|
c |
|
|
ccc diagnostic t,q a 2m et u, v a 10m |
|
|
c |
|
|
DO j=1, knon |
|
|
i = ni(j) |
|
|
uzon(j) = yu(j,1) + y_d_u(j,1) |
|
|
vmer(j) = yv(j,1) + y_d_v(j,1) |
|
|
tair1(j) = yt(j,1) + y_d_t(j,1) |
|
|
qair1(j) = yq(j,1) + y_d_q(j,1) |
|
|
zgeo1(j) = RD * tair1(j) / (0.5*(ypaprs(j,1)+ypplay(j,1))) |
|
|
& * (ypaprs(j,1)-ypplay(j,1)) |
|
|
tairsol(j) = yts(j) + y_d_ts(j) |
|
|
rugo1(j) = yrugos(j) |
|
|
IF(nsrf.EQ.is_oce) THEN |
|
|
rugo1(j) = rugos(i,nsrf) |
|
|
ENDIF |
|
|
psfce(j)=ypaprs(j,1) |
|
|
patm(j)=ypplay(j,1) |
|
|
c |
|
|
qairsol(j) = yqsurf(j) |
|
|
ENDDO |
|
|
c |
|
|
CALL stdlevvar(klon, knon, nsrf, zxli, |
|
|
& uzon, vmer, tair1, qair1, zgeo1, |
|
|
& tairsol, qairsol, rugo1, psfce, patm, |
|
|
cIM & yt2m, yq2m, yu10m) |
|
|
& yt2m, yq2m, yt10m, yq10m, yu10m, yustar) |
|
|
cIM 081204 END |
|
|
c |
|
|
c |
|
|
DO j=1, knon |
|
|
i = ni(j) |
|
|
t2m(i,nsrf)=yt2m(j) |
|
|
|
|
|
c |
|
|
q2m(i,nsrf)=yq2m(j) |
|
|
c |
|
|
c u10m, v10m : composantes du vent a 10m sans spirale de Ekman |
|
|
u10m(i,nsrf)=(yu10m(j) * uzon(j))/sqrt(uzon(j)**2+vmer(j)**2) |
|
|
v10m(i,nsrf)=(yu10m(j) * vmer(j))/sqrt(uzon(j)**2+vmer(j)**2) |
|
|
c |
|
|
ENDDO |
|
|
c |
|
|
cIM cf AM : pbl, HBTM |
|
|
DO i = 1, knon |
|
|
y_cd_h(i) = ycoefh(i,1) |
|
|
y_cd_m(i) = ycoefm(i,1) |
|
|
ENDDO |
|
|
c print*,'appel hbtm2' |
|
|
CALL HBTM(knon, ypaprs, ypplay, |
|
|
. yt2m,yt10m,yq2m,yq10m,yustar, |
|
|
. y_flux_t,y_flux_q,yu,yv,yt,yq, |
|
|
. ypblh,ycapCL,yoliqCL,ycteiCL,ypblT, |
|
|
. ytherm,ytrmb1,ytrmb2,ytrmb3,ylcl) |
|
|
c print*,'fin hbtm2' |
|
|
c |
|
|
DO j=1, knon |
|
|
i = ni(j) |
|
|
pblh(i,nsrf) = ypblh(j) |
|
|
plcl(i,nsrf) = ylcl(j) |
|
|
capCL(i,nsrf) = ycapCL(j) |
|
|
oliqCL(i,nsrf) = yoliqCL(j) |
|
|
cteiCL(i,nsrf) = ycteiCL(j) |
|
|
pblT(i,nsrf) = ypblT(j) |
|
|
therm(i,nsrf) = ytherm(j) |
|
|
trmb1(i,nsrf) = ytrmb1(j) |
|
|
trmb2(i,nsrf) = ytrmb2(j) |
|
|
trmb3(i,nsrf) = ytrmb3(j) |
|
|
ENDDO |
|
|
c |
|
|
|
|
|
do j=1,knon |
|
|
do k=1,klev+1 |
|
|
i=ni(j) |
|
|
q2(i,k,nsrf)=yq2(j,k) |
|
|
enddo |
|
|
enddo |
|
|
cIM "slab" ocean |
|
|
IF(OCEAN.EQ.'slab '.OR.OCEAN.EQ.'force ') THEN |
|
|
IF (nsrf.EQ.is_oce) THEN |
|
|
DO j = 1, knon |
|
|
c on projette sur la grille globale |
|
|
i = ni(j) |
|
|
IF(pctsrf_new(i,is_oce).GT.epsfra) THEN |
|
|
flux_o(i) = y_flux_o(j) |
|
|
ELSE |
|
|
flux_o(i) = 0. |
|
|
ENDIF |
|
|
ENDDO |
|
|
ENDIF |
|
|
c |
|
|
IF (nsrf.EQ.is_sic) THEN |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
cIM 230604 on pondere lorsque l'on fait le bilan au sol : flux_g(i) = y_flux_g(j)*ypct(j) |
|
|
IF(pctsrf_new(i,is_sic).GT.epsfra) THEN |
|
|
flux_g(i) = y_flux_g(j) |
|
|
ELSE |
|
|
flux_g(i) = 0. |
|
|
ENDIF |
|
|
ENDDO |
|
|
ENDIF !nsrf.EQ.is_sic |
|
|
ENDIF !OCEAN |
|
|
c |
|
|
IF(OCEAN.EQ.'slab ') THEN |
|
|
IF(nsrf.EQ.is_oce) then |
|
|
tslab(1:klon) = ytslab(1:klon) |
|
|
seaice(1:klon) = y_seaice(1:klon) |
|
|
ENDIF !nsrf |
|
|
ENDIF !OCEAN |
|
|
99999 CONTINUE |
|
|
C |
|
|
C On utilise les nouvelles surfaces |
|
|
C A rajouter: conservation de l'albedo |
|
|
C |
|
|
rugos(:,is_oce) = rugmer |
|
|
pctsrf = pctsrf_new |
|
| 606 |
|
|
| 607 |
RETURN |
DO j = 1, knon |
| 608 |
END |
DO k = 1, klev + 1 |
| 609 |
|
i = ni(j) |
| 610 |
|
q2(i, k, nsrf) = yq2(j, k) |
| 611 |
|
END DO |
| 612 |
|
END DO |
| 613 |
|
end IF if_knon |
| 614 |
|
END DO loop_surface |
| 615 |
|
|
| 616 |
|
! On utilise les nouvelles surfaces |
| 617 |
|
rugos(:, is_oce) = rugmer |
| 618 |
|
pctsrf(:, is_oce) = pctsrf_new_oce |
| 619 |
|
pctsrf(:, is_sic) = pctsrf_new_sic |
| 620 |
|
|
| 621 |
|
firstcal = .false. |
| 622 |
|
|
| 623 |
|
END SUBROUTINE clmain |
| 624 |
|
|
| 625 |
|
end module clmain_m |
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