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module physiq_m |
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|
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IMPLICIT none |
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|
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contains |
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|
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SUBROUTINE physiq(lafin, rdayvrai, time, dtphys, paprs, play, pphi, pphis, & |
8 |
u, v, t, qx, omega, d_u, d_v, d_t, d_qx, d_ps, dudyn, PVteta) |
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|
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! From phylmd/physiq.F, version 1.22 2006/02/20 09:38:28 (SVN revision 678) |
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! Author: Z.X. Li (LMD/CNRS) 1993 |
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|
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! This is the main procedure for the "physics" part of the program. |
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|
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use abort_gcm_m, only: abort_gcm |
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USE calendar, only: ymds2ju |
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use clesphys, only: ecrit_hf, ecrit_ins, ecrit_mth, cdmmax, cdhmax, & |
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co2_ppm, ecrit_reg, ecrit_tra, ksta, ksta_ter, ok_kzmin |
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use clesphys2, only: iflag_con, ok_orolf, ok_orodr, nbapp_rad, & |
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cycle_diurne, new_oliq, soil_model |
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use clmain_m, only: clmain |
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use comgeomphy |
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use concvl_m, only: concvl |
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use conf_gcm_m, only: raz_date, offline |
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use conf_phys_m, only: conf_phys |
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use ctherm |
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use dimens_m, only: jjm, iim, llm, nqmx |
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use dimphy, only: klon, nbtr |
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use dimsoil, only: nsoilmx |
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use fcttre, only: thermcep, foeew, qsats, qsatl |
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use hgardfou_m, only: hgardfou |
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USE histcom, only: histsync |
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USE histwrite_m, only: histwrite |
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use indicesol, only: nbsrf, is_ter, is_lic, is_sic, is_oce, clnsurf, epsfra |
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use ini_histhf_m, only: ini_histhf |
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use ini_histday_m, only: ini_histday |
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use ini_histins_m, only: ini_histins |
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use iniprint, only: prt_level |
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use oasis_m |
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use orbite_m, only: orbite, zenang |
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use ozonecm_m, only: ozonecm |
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use phyetat0_m, only: phyetat0, rlat, rlon |
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use phyredem_m, only: phyredem |
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use phystokenc_m, only: phystokenc |
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use phytrac_m, only: phytrac |
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use qcheck_m, only: qcheck |
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use radepsi |
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use radopt |
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use SUPHEC_M, only: rcpd, rtt, rlvtt, rg, ra, rsigma, retv, romega |
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use temps, only: itau_phy, day_ref, annee_ref |
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use yoethf_m |
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|
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! Variables argument: |
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|
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REAL, intent(in):: rdayvrai |
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! (elapsed time since January 1st 0h of the starting year, in days) |
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|
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REAL, intent(in):: time ! heure de la journée en fraction de jour |
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REAL, intent(in):: dtphys ! pas d'integration pour la physique (seconde) |
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logical, intent(in):: lafin ! dernier passage |
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|
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REAL, intent(in):: paprs(klon, llm+1) |
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! (pression pour chaque inter-couche, en Pa) |
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|
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REAL, intent(in):: play(klon, llm) |
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! (input pression pour le mileu de chaque couche (en Pa)) |
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|
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REAL, intent(in):: pphi(klon, llm) |
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! (input geopotentiel de chaque couche (g z) (reference sol)) |
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|
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REAL pphis(klon) ! input geopotentiel du sol |
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|
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REAL, intent(in):: u(klon, llm) |
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! vitesse dans la direction X (de O a E) en m/s |
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|
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REAL, intent(in):: v(klon, llm) ! vitesse Y (de S a N) en m/s |
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REAL t(klon, llm) ! input temperature (K) |
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|
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REAL, intent(in):: qx(klon, llm, nqmx) |
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! (humidité spécifique et fractions massiques des autres traceurs) |
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|
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REAL omega(klon, llm) ! input vitesse verticale en Pa/s |
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REAL, intent(out):: d_u(klon, llm) ! tendance physique de "u" (m/s/s) |
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REAL, intent(out):: d_v(klon, llm) ! tendance physique de "v" (m/s/s) |
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REAL, intent(out):: d_t(klon, llm) ! tendance physique de "t" (K/s) |
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REAL d_qx(klon, llm, nqmx) ! output tendance physique de "qx" (kg/kg/s) |
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REAL d_ps(klon) ! output tendance physique de la pression au sol |
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|
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LOGICAL:: firstcal = .true. |
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|
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INTEGER nbteta |
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PARAMETER(nbteta=3) |
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|
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REAL PVteta(klon, nbteta) |
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! (output vorticite potentielle a des thetas constantes) |
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|
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LOGICAL ok_cvl ! pour activer le nouveau driver pour convection KE |
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PARAMETER (ok_cvl=.TRUE.) |
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LOGICAL ok_gust ! pour activer l'effet des gust sur flux surface |
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PARAMETER (ok_gust=.FALSE.) |
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|
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LOGICAL check ! Verifier la conservation du modele en eau |
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PARAMETER (check=.FALSE.) |
104 |
|
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LOGICAL, PARAMETER:: ok_stratus=.FALSE. |
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! Ajouter artificiellement les stratus |
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|
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! Parametres lies au coupleur OASIS: |
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INTEGER, SAVE :: npas, nexca |
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logical rnpb |
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parameter(rnpb=.true.) |
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|
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character(len=6), save:: ocean |
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! (type de modèle océan à utiliser: "force" ou "slab" mais pas "couple") |
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|
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logical ok_ocean |
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SAVE ok_ocean |
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|
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! "slab" ocean |
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REAL, save:: tslab(klon) ! temperature of ocean slab |
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REAL, save:: seaice(klon) ! glace de mer (kg/m2) |
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REAL fluxo(klon) ! flux turbulents ocean-glace de mer |
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REAL fluxg(klon) ! flux turbulents ocean-atmosphere |
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|
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! Modele thermique du sol, a activer pour le cycle diurne: |
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logical, save:: ok_veget |
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LOGICAL, save:: ok_journe ! sortir le fichier journalier |
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|
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LOGICAL ok_mensuel ! sortir le fichier mensuel |
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|
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LOGICAL ok_instan ! sortir le fichier instantane |
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save ok_instan |
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|
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LOGICAL ok_region ! sortir le fichier regional |
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PARAMETER (ok_region=.FALSE.) |
136 |
|
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! pour phsystoke avec thermiques |
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REAL fm_therm(klon, llm+1) |
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REAL entr_therm(klon, llm) |
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real, save:: q2(klon, llm+1, nbsrf) |
141 |
|
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INTEGER ivap ! indice de traceurs pour vapeur d'eau |
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PARAMETER (ivap=1) |
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INTEGER iliq ! indice de traceurs pour eau liquide |
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PARAMETER (iliq=2) |
146 |
|
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REAL, save:: t_ancien(klon, llm), q_ancien(klon, llm) |
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LOGICAL, save:: ancien_ok |
149 |
|
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REAL d_t_dyn(klon, llm) ! tendance dynamique pour "t" (K/s) |
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REAL d_q_dyn(klon, llm) ! tendance dynamique pour "q" (kg/kg/s) |
152 |
|
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real da(klon, llm), phi(klon, llm, llm), mp(klon, llm) |
154 |
|
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!IM Amip2 PV a theta constante |
156 |
|
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CHARACTER(LEN=3) ctetaSTD(nbteta) |
158 |
DATA ctetaSTD/'350', '380', '405'/ |
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REAL rtetaSTD(nbteta) |
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DATA rtetaSTD/350., 380., 405./ |
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|
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!MI Amip2 PV a theta constante |
163 |
|
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INTEGER klevp1 |
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PARAMETER(klevp1=llm+1) |
166 |
|
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REAL swdn0(klon, klevp1), swdn(klon, klevp1) |
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REAL swup0(klon, klevp1), swup(klon, klevp1) |
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SAVE swdn0, swdn, swup0, swup |
170 |
|
171 |
REAL lwdn0(klon, klevp1), lwdn(klon, klevp1) |
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REAL lwup0(klon, klevp1), lwup(klon, klevp1) |
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SAVE lwdn0, lwdn, lwup0, lwup |
174 |
|
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!IM Amip2 |
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! variables a une pression donnee |
177 |
|
178 |
integer nlevSTD |
179 |
PARAMETER(nlevSTD=17) |
180 |
real rlevSTD(nlevSTD) |
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DATA rlevSTD/100000., 92500., 85000., 70000., & |
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60000., 50000., 40000., 30000., 25000., 20000., & |
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15000., 10000., 7000., 5000., 3000., 2000., 1000./ |
184 |
CHARACTER(LEN=4) clevSTD(nlevSTD) |
185 |
DATA clevSTD/'1000', '925 ', '850 ', '700 ', '600 ', & |
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'500 ', '400 ', '300 ', '250 ', '200 ', '150 ', '100 ', & |
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'70 ', '50 ', '30 ', '20 ', '10 '/ |
188 |
|
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! prw: precipitable water |
190 |
real prw(klon) |
191 |
|
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! flwp, fiwp = Liquid Water Path & Ice Water Path (kg/m2) |
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! flwc, fiwc = Liquid Water Content & Ice Water Content (kg/kg) |
194 |
REAL flwp(klon), fiwp(klon) |
195 |
REAL flwc(klon, llm), fiwc(klon, llm) |
196 |
|
197 |
INTEGER kmax, lmax |
198 |
PARAMETER(kmax=8, lmax=8) |
199 |
INTEGER kmaxm1, lmaxm1 |
200 |
PARAMETER(kmaxm1=kmax-1, lmaxm1=lmax-1) |
201 |
|
202 |
REAL zx_tau(kmaxm1), zx_pc(lmaxm1) |
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DATA zx_tau/0.0, 0.3, 1.3, 3.6, 9.4, 23., 60./ |
204 |
DATA zx_pc/50., 180., 310., 440., 560., 680., 800./ |
205 |
|
206 |
! cldtopres pression au sommet des nuages |
207 |
REAL cldtopres(lmaxm1) |
208 |
DATA cldtopres/50., 180., 310., 440., 560., 680., 800./ |
209 |
|
210 |
! taulev: numero du niveau de tau dans les sorties ISCCP |
211 |
CHARACTER(LEN=4) taulev(kmaxm1) |
212 |
|
213 |
DATA taulev/'tau0', 'tau1', 'tau2', 'tau3', 'tau4', 'tau5', 'tau6'/ |
214 |
CHARACTER(LEN=3) pclev(lmaxm1) |
215 |
DATA pclev/'pc1', 'pc2', 'pc3', 'pc4', 'pc5', 'pc6', 'pc7'/ |
216 |
|
217 |
CHARACTER(LEN=28) cnameisccp(lmaxm1, kmaxm1) |
218 |
DATA cnameisccp/'pc< 50hPa, tau< 0.3', 'pc= 50-180hPa, tau< 0.3', & |
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'pc= 180-310hPa, tau< 0.3', 'pc= 310-440hPa, tau< 0.3', & |
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'pc= 440-560hPa, tau< 0.3', 'pc= 560-680hPa, tau< 0.3', & |
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'pc= 680-800hPa, tau< 0.3', 'pc< 50hPa, tau= 0.3-1.3', & |
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'pc= 50-180hPa, tau= 0.3-1.3', 'pc= 180-310hPa, tau= 0.3-1.3', & |
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'pc= 310-440hPa, tau= 0.3-1.3', 'pc= 440-560hPa, tau= 0.3-1.3', & |
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'pc= 560-680hPa, tau= 0.3-1.3', 'pc= 680-800hPa, tau= 0.3-1.3', & |
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'pc< 50hPa, tau= 1.3-3.6', 'pc= 50-180hPa, tau= 1.3-3.6', & |
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'pc= 180-310hPa, tau= 1.3-3.6', 'pc= 310-440hPa, tau= 1.3-3.6', & |
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'pc= 440-560hPa, tau= 1.3-3.6', 'pc= 560-680hPa, tau= 1.3-3.6', & |
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'pc= 680-800hPa, tau= 1.3-3.6', 'pc< 50hPa, tau= 3.6-9.4', & |
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'pc= 50-180hPa, tau= 3.6-9.4', 'pc= 180-310hPa, tau= 3.6-9.4', & |
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'pc= 310-440hPa, tau= 3.6-9.4', 'pc= 440-560hPa, tau= 3.6-9.4', & |
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'pc= 560-680hPa, tau= 3.6-9.4', 'pc= 680-800hPa, tau= 3.6-9.4', & |
232 |
'pc< 50hPa, tau= 9.4-23', 'pc= 50-180hPa, tau= 9.4-23', & |
233 |
'pc= 180-310hPa, tau= 9.4-23', 'pc= 310-440hPa, tau= 9.4-23', & |
234 |
'pc= 440-560hPa, tau= 9.4-23', 'pc= 560-680hPa, tau= 9.4-23', & |
235 |
'pc= 680-800hPa, tau= 9.4-23', 'pc< 50hPa, tau= 23-60', & |
236 |
'pc= 50-180hPa, tau= 23-60', 'pc= 180-310hPa, tau= 23-60', & |
237 |
'pc= 310-440hPa, tau= 23-60', 'pc= 440-560hPa, tau= 23-60', & |
238 |
'pc= 560-680hPa, tau= 23-60', 'pc= 680-800hPa, tau= 23-60', & |
239 |
'pc< 50hPa, tau> 60.', 'pc= 50-180hPa, tau> 60.', & |
240 |
'pc= 180-310hPa, tau> 60.', 'pc= 310-440hPa, tau> 60.', & |
241 |
'pc= 440-560hPa, tau> 60.', 'pc= 560-680hPa, tau> 60.', & |
242 |
'pc= 680-800hPa, tau> 60.'/ |
243 |
|
244 |
!IM ISCCP simulator v3.4 |
245 |
|
246 |
integer nid_hf, nid_hf3d |
247 |
save nid_hf, nid_hf3d |
248 |
|
249 |
! Variables propres a la physique |
250 |
|
251 |
INTEGER, save:: radpas |
252 |
! (Radiative transfer computations are made every "radpas" call to |
253 |
! "physiq".) |
254 |
|
255 |
REAL radsol(klon) |
256 |
SAVE radsol ! bilan radiatif au sol calcule par code radiatif |
257 |
|
258 |
INTEGER, SAVE:: itap ! number of calls to "physiq" |
259 |
|
260 |
REAL, save:: ftsol(klon, nbsrf) ! skin temperature of surface fraction |
261 |
|
262 |
REAL, save:: ftsoil(klon, nsoilmx, nbsrf) |
263 |
! soil temperature of surface fraction |
264 |
|
265 |
REAL fevap(klon, nbsrf) |
266 |
SAVE fevap ! evaporation |
267 |
REAL fluxlat(klon, nbsrf) |
268 |
SAVE fluxlat |
269 |
|
270 |
REAL fqsurf(klon, nbsrf) |
271 |
SAVE fqsurf ! humidite de l'air au contact de la surface |
272 |
|
273 |
REAL, save:: qsol(klon) ! hauteur d'eau dans le sol |
274 |
|
275 |
REAL fsnow(klon, nbsrf) |
276 |
SAVE fsnow ! epaisseur neigeuse |
277 |
|
278 |
REAL falbe(klon, nbsrf) |
279 |
SAVE falbe ! albedo par type de surface |
280 |
REAL falblw(klon, nbsrf) |
281 |
SAVE falblw ! albedo par type de surface |
282 |
|
283 |
! Paramètres de l'orographie à l'échelle sous-maille (OESM) : |
284 |
REAL, save:: zmea(klon) ! orographie moyenne |
285 |
REAL, save:: zstd(klon) ! deviation standard de l'OESM |
286 |
REAL, save:: zsig(klon) ! pente de l'OESM |
287 |
REAL, save:: zgam(klon) ! anisotropie de l'OESM |
288 |
REAL, save:: zthe(klon) ! orientation de l'OESM |
289 |
REAL, save:: zpic(klon) ! Maximum de l'OESM |
290 |
REAL, save:: zval(klon) ! Minimum de l'OESM |
291 |
REAL, save:: rugoro(klon) ! longueur de rugosite de l'OESM |
292 |
|
293 |
REAL zulow(klon), zvlow(klon) |
294 |
|
295 |
INTEGER igwd, idx(klon), itest(klon) |
296 |
|
297 |
REAL agesno(klon, nbsrf) |
298 |
SAVE agesno ! age de la neige |
299 |
|
300 |
REAL run_off_lic_0(klon) |
301 |
SAVE run_off_lic_0 |
302 |
!KE43 |
303 |
! Variables liees a la convection de K. Emanuel (sb): |
304 |
|
305 |
REAL bas, top ! cloud base and top levels |
306 |
SAVE bas |
307 |
SAVE top |
308 |
|
309 |
REAL Ma(klon, llm) ! undilute upward mass flux |
310 |
SAVE Ma |
311 |
REAL qcondc(klon, llm) ! in-cld water content from convect |
312 |
SAVE qcondc |
313 |
REAL ema_work1(klon, llm), ema_work2(klon, llm) |
314 |
SAVE ema_work1, ema_work2 |
315 |
|
316 |
REAL wd(klon) ! sb |
317 |
SAVE wd ! sb |
318 |
|
319 |
! Variables locales pour la couche limite (al1): |
320 |
|
321 |
! Variables locales: |
322 |
|
323 |
REAL cdragh(klon) ! drag coefficient pour T and Q |
324 |
REAL cdragm(klon) ! drag coefficient pour vent |
325 |
|
326 |
!AA Pour phytrac |
327 |
REAL ycoefh(klon, llm) ! coef d'echange pour phytrac |
328 |
REAL yu1(klon) ! vents dans la premiere couche U |
329 |
REAL yv1(klon) ! vents dans la premiere couche V |
330 |
REAL ffonte(klon, nbsrf) !Flux thermique utilise pour fondre la neige |
331 |
REAL fqcalving(klon, nbsrf) !Flux d'eau "perdue" par la surface |
332 |
! !et necessaire pour limiter la |
333 |
! !hauteur de neige, en kg/m2/s |
334 |
REAL zxffonte(klon), zxfqcalving(klon) |
335 |
|
336 |
REAL pfrac_impa(klon, llm)! Produits des coefs lessivage impaction |
337 |
save pfrac_impa |
338 |
REAL pfrac_nucl(klon, llm)! Produits des coefs lessivage nucleation |
339 |
save pfrac_nucl |
340 |
REAL pfrac_1nucl(klon, llm)! Produits des coefs lessi nucl (alpha = 1) |
341 |
save pfrac_1nucl |
342 |
REAL frac_impa(klon, llm) ! fractions d'aerosols lessivees (impaction) |
343 |
REAL frac_nucl(klon, llm) ! idem (nucleation) |
344 |
|
345 |
!AA |
346 |
REAL rain_fall(klon) ! pluie |
347 |
REAL snow_fall(klon) ! neige |
348 |
save snow_fall, rain_fall |
349 |
!IM cf FH pour Tiedtke 080604 |
350 |
REAL rain_tiedtke(klon), snow_tiedtke(klon) |
351 |
|
352 |
REAL evap(klon), devap(klon) ! evaporation et sa derivee |
353 |
REAL sens(klon), dsens(klon) ! chaleur sensible et sa derivee |
354 |
REAL dlw(klon) ! derivee infra rouge |
355 |
SAVE dlw |
356 |
REAL bils(klon) ! bilan de chaleur au sol |
357 |
REAL fder(klon) ! Derive de flux (sensible et latente) |
358 |
save fder |
359 |
REAL ve(klon) ! integr. verticale du transport meri. de l'energie |
360 |
REAL vq(klon) ! integr. verticale du transport meri. de l'eau |
361 |
REAL ue(klon) ! integr. verticale du transport zonal de l'energie |
362 |
REAL uq(klon) ! integr. verticale du transport zonal de l'eau |
363 |
|
364 |
REAL frugs(klon, nbsrf) ! longueur de rugosite |
365 |
save frugs |
366 |
REAL zxrugs(klon) ! longueur de rugosite |
367 |
|
368 |
! Conditions aux limites |
369 |
|
370 |
INTEGER julien |
371 |
|
372 |
INTEGER, SAVE:: lmt_pas ! number of time steps of "physics" per day |
373 |
REAL pctsrf(klon, nbsrf) |
374 |
!IM |
375 |
REAL pctsrf_new(klon, nbsrf) !pourcentage surfaces issus d'ORCHIDEE |
376 |
|
377 |
SAVE pctsrf ! sous-fraction du sol |
378 |
REAL albsol(klon) |
379 |
SAVE albsol ! albedo du sol total |
380 |
REAL albsollw(klon) |
381 |
SAVE albsollw ! albedo du sol total |
382 |
|
383 |
REAL, SAVE:: wo(klon, llm) ! column density of ozone in a cell, in kDU |
384 |
|
385 |
! Declaration des procedures appelees |
386 |
|
387 |
EXTERNAL alboc ! calculer l'albedo sur ocean |
388 |
EXTERNAL ajsec ! ajustement sec |
389 |
!KE43 |
390 |
EXTERNAL conema3 ! convect4.3 |
391 |
EXTERNAL fisrtilp ! schema de condensation a grande echelle (pluie) |
392 |
EXTERNAL nuage ! calculer les proprietes radiatives |
393 |
EXTERNAL radlwsw ! rayonnements solaire et infrarouge |
394 |
EXTERNAL transp ! transport total de l'eau et de l'energie |
395 |
|
396 |
! Variables locales |
397 |
|
398 |
real clwcon(klon, llm), rnebcon(klon, llm) |
399 |
real clwcon0(klon, llm), rnebcon0(klon, llm) |
400 |
|
401 |
save rnebcon, clwcon |
402 |
|
403 |
REAL rhcl(klon, llm) ! humiditi relative ciel clair |
404 |
REAL dialiq(klon, llm) ! eau liquide nuageuse |
405 |
REAL diafra(klon, llm) ! fraction nuageuse |
406 |
REAL cldliq(klon, llm) ! eau liquide nuageuse |
407 |
REAL cldfra(klon, llm) ! fraction nuageuse |
408 |
REAL cldtau(klon, llm) ! epaisseur optique |
409 |
REAL cldemi(klon, llm) ! emissivite infrarouge |
410 |
|
411 |
REAL fluxq(klon, llm, nbsrf) ! flux turbulent d'humidite |
412 |
REAL fluxt(klon, llm, nbsrf) ! flux turbulent de chaleur |
413 |
REAL fluxu(klon, llm, nbsrf) ! flux turbulent de vitesse u |
414 |
REAL fluxv(klon, llm, nbsrf) ! flux turbulent de vitesse v |
415 |
|
416 |
REAL zxfluxt(klon, llm) |
417 |
REAL zxfluxq(klon, llm) |
418 |
REAL zxfluxu(klon, llm) |
419 |
REAL zxfluxv(klon, llm) |
420 |
|
421 |
REAL heat(klon, llm) ! chauffage solaire |
422 |
REAL heat0(klon, llm) ! chauffage solaire ciel clair |
423 |
REAL cool(klon, llm) ! refroidissement infrarouge |
424 |
REAL cool0(klon, llm) ! refroidissement infrarouge ciel clair |
425 |
REAL topsw(klon), toplw(klon), solsw(klon), sollw(klon) |
426 |
real sollwdown(klon) ! downward LW flux at surface |
427 |
REAL topsw0(klon), toplw0(klon), solsw0(klon), sollw0(klon) |
428 |
REAL albpla(klon) |
429 |
REAL fsollw(klon, nbsrf) ! bilan flux IR pour chaque sous surface |
430 |
REAL fsolsw(klon, nbsrf) ! flux solaire absorb. pour chaque sous surface |
431 |
! Le rayonnement n'est pas calcule tous les pas, il faut donc |
432 |
! sauvegarder les sorties du rayonnement |
433 |
SAVE heat, cool, albpla, topsw, toplw, solsw, sollw, sollwdown |
434 |
SAVE topsw0, toplw0, solsw0, sollw0, heat0, cool0 |
435 |
|
436 |
INTEGER itaprad |
437 |
SAVE itaprad |
438 |
|
439 |
REAL conv_q(klon, llm) ! convergence de l'humidite (kg/kg/s) |
440 |
REAL conv_t(klon, llm) ! convergence of temperature (K/s) |
441 |
|
442 |
REAL cldl(klon), cldm(klon), cldh(klon) !nuages bas, moyen et haut |
443 |
REAL cldt(klon), cldq(klon) !nuage total, eau liquide integree |
444 |
|
445 |
REAL zxtsol(klon), zxqsurf(klon), zxsnow(klon), zxfluxlat(klon) |
446 |
|
447 |
REAL dist, rmu0(klon), fract(klon) |
448 |
REAL zdtime ! pas de temps du rayonnement (s) |
449 |
real zlongi |
450 |
|
451 |
REAL z_avant(klon), z_apres(klon), z_factor(klon) |
452 |
LOGICAL zx_ajustq |
453 |
|
454 |
REAL za, zb |
455 |
REAL zx_t, zx_qs, zdelta, zcor, zlvdcp, zlsdcp |
456 |
real zqsat(klon, llm) |
457 |
INTEGER i, k, iq, nsrf |
458 |
REAL t_coup |
459 |
PARAMETER (t_coup=234.0) |
460 |
|
461 |
REAL zphi(klon, llm) |
462 |
|
463 |
!IM cf. AM Variables locales pour la CLA (hbtm2) |
464 |
|
465 |
REAL, SAVE:: pblh(klon, nbsrf) ! Hauteur de couche limite |
466 |
REAL, SAVE:: plcl(klon, nbsrf) ! Niveau de condensation de la CLA |
467 |
REAL, SAVE:: capCL(klon, nbsrf) ! CAPE de couche limite |
468 |
REAL, SAVE:: oliqCL(klon, nbsrf) ! eau_liqu integree de couche limite |
469 |
REAL, SAVE:: cteiCL(klon, nbsrf) ! cloud top instab. crit. couche limite |
470 |
REAL, SAVE:: pblt(klon, nbsrf) ! T a la Hauteur de couche limite |
471 |
REAL, SAVE:: therm(klon, nbsrf) |
472 |
REAL, SAVE:: trmb1(klon, nbsrf) ! deep_cape |
473 |
REAL, SAVE:: trmb2(klon, nbsrf) ! inhibition |
474 |
REAL, SAVE:: trmb3(klon, nbsrf) ! Point Omega |
475 |
! Grdeurs de sorties |
476 |
REAL s_pblh(klon), s_lcl(klon), s_capCL(klon) |
477 |
REAL s_oliqCL(klon), s_cteiCL(klon), s_pblt(klon) |
478 |
REAL s_therm(klon), s_trmb1(klon), s_trmb2(klon) |
479 |
REAL s_trmb3(klon) |
480 |
|
481 |
! Variables locales pour la convection de K. Emanuel (sb): |
482 |
|
483 |
REAL upwd(klon, llm) ! saturated updraft mass flux |
484 |
REAL dnwd(klon, llm) ! saturated downdraft mass flux |
485 |
REAL dnwd0(klon, llm) ! unsaturated downdraft mass flux |
486 |
REAL tvp(klon, llm) ! virtual temp of lifted parcel |
487 |
REAL cape(klon) ! CAPE |
488 |
SAVE cape |
489 |
|
490 |
REAL pbase(klon) ! cloud base pressure |
491 |
SAVE pbase |
492 |
REAL bbase(klon) ! cloud base buoyancy |
493 |
SAVE bbase |
494 |
REAL rflag(klon) ! flag fonctionnement de convect |
495 |
INTEGER iflagctrl(klon) ! flag fonctionnement de convect |
496 |
! -- convect43: |
497 |
INTEGER ntra ! nb traceurs pour convect4.3 |
498 |
REAL dtvpdt1(klon, llm), dtvpdq1(klon, llm) |
499 |
REAL dplcldt(klon), dplcldr(klon) |
500 |
|
501 |
! Variables du changement |
502 |
|
503 |
! con: convection |
504 |
! lsc: condensation a grande echelle (Large-Scale-Condensation) |
505 |
! ajs: ajustement sec |
506 |
! eva: evaporation de l'eau liquide nuageuse |
507 |
! vdf: couche limite (Vertical DiFfusion) |
508 |
REAL d_t_con(klon, llm), d_q_con(klon, llm) |
509 |
REAL d_u_con(klon, llm), d_v_con(klon, llm) |
510 |
REAL d_t_lsc(klon, llm), d_q_lsc(klon, llm), d_ql_lsc(klon, llm) |
511 |
REAL d_t_ajs(klon, llm), d_q_ajs(klon, llm) |
512 |
REAL d_u_ajs(klon, llm), d_v_ajs(klon, llm) |
513 |
REAL rneb(klon, llm) |
514 |
|
515 |
REAL pmfu(klon, llm), pmfd(klon, llm) |
516 |
REAL pen_u(klon, llm), pen_d(klon, llm) |
517 |
REAL pde_u(klon, llm), pde_d(klon, llm) |
518 |
INTEGER kcbot(klon), kctop(klon), kdtop(klon) |
519 |
REAL pmflxr(klon, llm+1), pmflxs(klon, llm+1) |
520 |
REAL prfl(klon, llm+1), psfl(klon, llm+1) |
521 |
|
522 |
INTEGER ibas_con(klon), itop_con(klon) |
523 |
|
524 |
SAVE ibas_con, itop_con |
525 |
|
526 |
REAL rain_con(klon), rain_lsc(klon) |
527 |
REAL snow_con(klon), snow_lsc(klon) |
528 |
REAL d_ts(klon, nbsrf) |
529 |
|
530 |
REAL d_u_vdf(klon, llm), d_v_vdf(klon, llm) |
531 |
REAL d_t_vdf(klon, llm), d_q_vdf(klon, llm) |
532 |
|
533 |
REAL d_u_oro(klon, llm), d_v_oro(klon, llm) |
534 |
REAL d_t_oro(klon, llm) |
535 |
REAL d_u_lif(klon, llm), d_v_lif(klon, llm) |
536 |
REAL d_t_lif(klon, llm) |
537 |
|
538 |
REAL ratqs(klon, llm), ratqss(klon, llm), ratqsc(klon, llm) |
539 |
real ratqsbas, ratqshaut |
540 |
save ratqsbas, ratqshaut, ratqs |
541 |
|
542 |
! Parametres lies au nouveau schema de nuages (SB, PDF) |
543 |
real, save:: fact_cldcon |
544 |
real, save:: facttemps |
545 |
logical ok_newmicro |
546 |
save ok_newmicro |
547 |
real facteur |
548 |
|
549 |
integer iflag_cldcon |
550 |
save iflag_cldcon |
551 |
|
552 |
logical ptconv(klon, llm) |
553 |
|
554 |
! Variables locales pour effectuer les appels en série |
555 |
|
556 |
REAL t_seri(klon, llm), q_seri(klon, llm) |
557 |
REAL ql_seri(klon, llm), qs_seri(klon, llm) |
558 |
REAL u_seri(klon, llm), v_seri(klon, llm) |
559 |
|
560 |
REAL tr_seri(klon, llm, nbtr) |
561 |
REAL d_tr(klon, llm, nbtr) |
562 |
|
563 |
REAL zx_rh(klon, llm) |
564 |
|
565 |
REAL zustrdr(klon), zvstrdr(klon) |
566 |
REAL zustrli(klon), zvstrli(klon) |
567 |
REAL zustrph(klon), zvstrph(klon) |
568 |
REAL aam, torsfc |
569 |
|
570 |
REAL dudyn(iim+1, jjm + 1, llm) |
571 |
|
572 |
REAL zx_tmp_fi2d(klon) ! variable temporaire grille physique |
573 |
REAL zx_tmp_2d(iim, jjm + 1), zx_tmp_3d(iim, jjm + 1, llm) |
574 |
|
575 |
INTEGER, SAVE:: nid_day, nid_ins |
576 |
|
577 |
REAL ve_lay(klon, llm) ! transport meri. de l'energie a chaque niveau vert. |
578 |
REAL vq_lay(klon, llm) ! transport meri. de l'eau a chaque niveau vert. |
579 |
REAL ue_lay(klon, llm) ! transport zonal de l'energie a chaque niveau vert. |
580 |
REAL uq_lay(klon, llm) ! transport zonal de l'eau a chaque niveau vert. |
581 |
|
582 |
REAL zsto |
583 |
|
584 |
character(len=20) modname |
585 |
character(len=80) abort_message |
586 |
logical ok_sync |
587 |
real date0 |
588 |
|
589 |
! Variables liees au bilan d'energie et d'enthalpi |
590 |
REAL ztsol(klon) |
591 |
REAL d_h_vcol, d_qt, d_qw, d_ql, d_qs, d_ec |
592 |
REAL d_h_vcol_phy |
593 |
REAL fs_bound, fq_bound |
594 |
SAVE d_h_vcol_phy |
595 |
REAL zero_v(klon) |
596 |
CHARACTER(LEN=15) ztit |
597 |
INTEGER ip_ebil ! PRINT level for energy conserv. diag. |
598 |
SAVE ip_ebil |
599 |
DATA ip_ebil/0/ |
600 |
INTEGER, SAVE:: if_ebil ! level for energy conservation diagnostics |
601 |
!+jld ec_conser |
602 |
REAL d_t_ec(klon, llm) ! tendance du a la conersion Ec -> E thermique |
603 |
REAL ZRCPD |
604 |
!-jld ec_conser |
605 |
!IM: t2m, q2m, u10m, v10m |
606 |
REAL t2m(klon, nbsrf), q2m(klon, nbsrf) ! temperature and humidity at 2 m |
607 |
REAL u10m(klon, nbsrf), v10m(klon, nbsrf) !vents a 10m |
608 |
REAL zt2m(klon), zq2m(klon) !temp., hum. 2m moyenne s/ 1 maille |
609 |
REAL zu10m(klon), zv10m(klon) !vents a 10m moyennes s/1 maille |
610 |
!jq Aerosol effects (Johannes Quaas, 27/11/2003) |
611 |
REAL sulfate(klon, llm) ! SO4 aerosol concentration [ug/m3] |
612 |
|
613 |
REAL, save:: sulfate_pi(klon, llm) |
614 |
! (SO4 aerosol concentration, in ug/m3, pre-industrial value) |
615 |
|
616 |
REAL cldtaupi(klon, llm) |
617 |
! (Cloud optical thickness for pre-industrial (pi) aerosols) |
618 |
|
619 |
REAL re(klon, llm) ! Cloud droplet effective radius |
620 |
REAL fl(klon, llm) ! denominator of re |
621 |
|
622 |
! Aerosol optical properties |
623 |
REAL tau_ae(klon, llm, 2), piz_ae(klon, llm, 2) |
624 |
REAL cg_ae(klon, llm, 2) |
625 |
|
626 |
REAL topswad(klon), solswad(klon) ! Aerosol direct effect. |
627 |
! ok_ade=True -ADE=topswad-topsw |
628 |
|
629 |
REAL topswai(klon), solswai(klon) ! Aerosol indirect effect. |
630 |
! ok_aie=True -> |
631 |
! ok_ade=True -AIE=topswai-topswad |
632 |
! ok_ade=F -AIE=topswai-topsw |
633 |
|
634 |
REAL aerindex(klon) ! POLDER aerosol index |
635 |
|
636 |
! Parameters |
637 |
LOGICAL ok_ade, ok_aie ! Apply aerosol (in)direct effects or not |
638 |
REAL bl95_b0, bl95_b1 ! Parameter in Boucher and Lohmann (1995) |
639 |
|
640 |
SAVE ok_ade, ok_aie, bl95_b0, bl95_b1 |
641 |
SAVE u10m |
642 |
SAVE v10m |
643 |
SAVE t2m |
644 |
SAVE q2m |
645 |
SAVE ffonte |
646 |
SAVE fqcalving |
647 |
SAVE piz_ae |
648 |
SAVE tau_ae |
649 |
SAVE cg_ae |
650 |
SAVE rain_con |
651 |
SAVE snow_con |
652 |
SAVE topswai |
653 |
SAVE topswad |
654 |
SAVE solswai |
655 |
SAVE solswad |
656 |
SAVE d_u_con |
657 |
SAVE d_v_con |
658 |
SAVE rnebcon0 |
659 |
SAVE clwcon0 |
660 |
|
661 |
real zmasse(klon, llm) |
662 |
! (column-density of mass of air in a cell, in kg m-2) |
663 |
|
664 |
real, parameter:: dobson_u = 2.1415e-05 ! Dobson unit, in kg m-2 |
665 |
|
666 |
!---------------------------------------------------------------- |
667 |
|
668 |
modname = 'physiq' |
669 |
IF (if_ebil >= 1) THEN |
670 |
DO i=1, klon |
671 |
zero_v(i)=0. |
672 |
END DO |
673 |
END IF |
674 |
ok_sync=.TRUE. |
675 |
IF (nqmx < 2) THEN |
676 |
abort_message = 'eaux vapeur et liquide sont indispensables' |
677 |
CALL abort_gcm(modname, abort_message, 1) |
678 |
ENDIF |
679 |
|
680 |
test_firstcal: IF (firstcal) THEN |
681 |
! initialiser |
682 |
u10m=0. |
683 |
v10m=0. |
684 |
t2m=0. |
685 |
q2m=0. |
686 |
ffonte=0. |
687 |
fqcalving=0. |
688 |
piz_ae=0. |
689 |
tau_ae=0. |
690 |
cg_ae=0. |
691 |
rain_con(:)=0. |
692 |
snow_con(:)=0. |
693 |
bl95_b0=0. |
694 |
bl95_b1=0. |
695 |
topswai(:)=0. |
696 |
topswad(:)=0. |
697 |
solswai(:)=0. |
698 |
solswad(:)=0. |
699 |
|
700 |
d_u_con = 0.0 |
701 |
d_v_con = 0.0 |
702 |
rnebcon0 = 0.0 |
703 |
clwcon0 = 0.0 |
704 |
rnebcon = 0.0 |
705 |
clwcon = 0.0 |
706 |
|
707 |
pblh =0. ! Hauteur de couche limite |
708 |
plcl =0. ! Niveau de condensation de la CLA |
709 |
capCL =0. ! CAPE de couche limite |
710 |
oliqCL =0. ! eau_liqu integree de couche limite |
711 |
cteiCL =0. ! cloud top instab. crit. couche limite |
712 |
pblt =0. ! T a la Hauteur de couche limite |
713 |
therm =0. |
714 |
trmb1 =0. ! deep_cape |
715 |
trmb2 =0. ! inhibition |
716 |
trmb3 =0. ! Point Omega |
717 |
|
718 |
IF (if_ebil >= 1) d_h_vcol_phy=0. |
719 |
|
720 |
! appel a la lecture du run.def physique |
721 |
|
722 |
call conf_phys(ocean, ok_veget, ok_journe, ok_mensuel, & |
723 |
ok_instan, fact_cldcon, facttemps, ok_newmicro, & |
724 |
iflag_cldcon, ratqsbas, ratqshaut, if_ebil, & |
725 |
ok_ade, ok_aie, & |
726 |
bl95_b0, bl95_b1, & |
727 |
iflag_thermals, nsplit_thermals) |
728 |
|
729 |
! Initialiser les compteurs: |
730 |
|
731 |
frugs = 0. |
732 |
itap = 0 |
733 |
itaprad = 0 |
734 |
CALL phyetat0("startphy.nc", pctsrf, ftsol, ftsoil, ocean, tslab, & |
735 |
seaice, fqsurf, qsol, fsnow, falbe, falblw, fevap, rain_fall, & |
736 |
snow_fall, solsw, sollwdown, dlw, radsol, frugs, agesno, zmea, & |
737 |
zstd, zsig, zgam, zthe, zpic, zval, t_ancien, q_ancien, & |
738 |
ancien_ok, rnebcon, ratqs, clwcon, run_off_lic_0) |
739 |
|
740 |
! ATTENTION : il faudra a terme relire q2 dans l'etat initial |
741 |
q2=1.e-8 |
742 |
|
743 |
radpas = NINT(86400. / dtphys / nbapp_rad) |
744 |
|
745 |
! on remet le calendrier a zero |
746 |
IF (raz_date) itau_phy = 0 |
747 |
|
748 |
PRINT *, 'cycle_diurne = ', cycle_diurne |
749 |
|
750 |
IF(ocean.NE.'force ') THEN |
751 |
ok_ocean=.TRUE. |
752 |
ENDIF |
753 |
|
754 |
CALL printflag(radpas, ok_ocean, ok_oasis, ok_journe, ok_instan, & |
755 |
ok_region) |
756 |
|
757 |
IF (dtphys*REAL(radpas).GT.21600..AND.cycle_diurne) THEN |
758 |
print *,'Nbre d appels au rayonnement insuffisant' |
759 |
print *,"Au minimum 4 appels par jour si cycle diurne" |
760 |
abort_message='Nbre d appels au rayonnement insuffisant' |
761 |
call abort_gcm(modname, abort_message, 1) |
762 |
ENDIF |
763 |
print *,"Clef pour la convection, iflag_con=", iflag_con |
764 |
print *,"Clef pour le driver de la convection, ok_cvl=", & |
765 |
ok_cvl |
766 |
|
767 |
! Initialisation pour la convection de K.E. (sb): |
768 |
IF (iflag_con >= 3) THEN |
769 |
|
770 |
print *,"*** Convection de Kerry Emanuel 4.3 " |
771 |
|
772 |
!IM15/11/02 rajout initialisation ibas_con, itop_con cf. SB =>BEG |
773 |
DO i = 1, klon |
774 |
ibas_con(i) = 1 |
775 |
itop_con(i) = 1 |
776 |
ENDDO |
777 |
!IM15/11/02 rajout initialisation ibas_con, itop_con cf. SB =>END |
778 |
|
779 |
ENDIF |
780 |
|
781 |
IF (ok_orodr) THEN |
782 |
rugoro = MAX(1e-5, zstd * zsig / 2) |
783 |
CALL SUGWD(klon, llm, paprs, play) |
784 |
else |
785 |
rugoro = 0. |
786 |
ENDIF |
787 |
|
788 |
lmt_pas = NINT(86400. / dtphys) ! tous les jours |
789 |
print *, 'Number of time steps of "physics" per day: ', lmt_pas |
790 |
|
791 |
ecrit_ins = NINT(ecrit_ins/dtphys) |
792 |
ecrit_hf = NINT(ecrit_hf/dtphys) |
793 |
ecrit_mth = NINT(ecrit_mth/dtphys) |
794 |
ecrit_tra = NINT(86400.*ecrit_tra/dtphys) |
795 |
ecrit_reg = NINT(ecrit_reg/dtphys) |
796 |
|
797 |
! Initialiser le couplage si necessaire |
798 |
|
799 |
npas = 0 |
800 |
nexca = 0 |
801 |
|
802 |
print *,'AVANT HIST IFLAG_CON=', iflag_con |
803 |
|
804 |
! Initialisation des sorties |
805 |
|
806 |
call ini_histhf(dtphys, nid_hf, nid_hf3d) |
807 |
call ini_histday(dtphys, ok_journe, nid_day, nqmx) |
808 |
call ini_histins(dtphys, ok_instan, nid_ins) |
809 |
CALL ymds2ju(annee_ref, 1, int(day_ref), 0., date0) |
810 |
!XXXPB Positionner date0 pour initialisation de ORCHIDEE |
811 |
WRITE(*, *) 'physiq date0 : ', date0 |
812 |
ENDIF test_firstcal |
813 |
|
814 |
! Mettre a zero des variables de sortie (pour securite) |
815 |
|
816 |
DO i = 1, klon |
817 |
d_ps(i) = 0.0 |
818 |
ENDDO |
819 |
DO iq = 1, nqmx |
820 |
DO k = 1, llm |
821 |
DO i = 1, klon |
822 |
d_qx(i, k, iq) = 0.0 |
823 |
ENDDO |
824 |
ENDDO |
825 |
ENDDO |
826 |
da=0. |
827 |
mp=0. |
828 |
phi=0. |
829 |
|
830 |
! Ne pas affecter les valeurs entrees de u, v, h, et q |
831 |
|
832 |
DO k = 1, llm |
833 |
DO i = 1, klon |
834 |
t_seri(i, k) = t(i, k) |
835 |
u_seri(i, k) = u(i, k) |
836 |
v_seri(i, k) = v(i, k) |
837 |
q_seri(i, k) = qx(i, k, ivap) |
838 |
ql_seri(i, k) = qx(i, k, iliq) |
839 |
qs_seri(i, k) = 0. |
840 |
ENDDO |
841 |
ENDDO |
842 |
IF (nqmx >= 3) THEN |
843 |
tr_seri(:, :, :nqmx-2) = qx(:, :, 3:nqmx) |
844 |
ELSE |
845 |
tr_seri(:, :, 1) = 0. |
846 |
ENDIF |
847 |
|
848 |
DO i = 1, klon |
849 |
ztsol(i) = 0. |
850 |
ENDDO |
851 |
DO nsrf = 1, nbsrf |
852 |
DO i = 1, klon |
853 |
ztsol(i) = ztsol(i) + ftsol(i, nsrf)*pctsrf(i, nsrf) |
854 |
ENDDO |
855 |
ENDDO |
856 |
|
857 |
IF (if_ebil >= 1) THEN |
858 |
ztit='after dynamic' |
859 |
CALL diagetpq(airephy, ztit, ip_ebil, 1, 1, dtphys, t_seri, q_seri, & |
860 |
ql_seri, qs_seri, u_seri, v_seri, paprs, d_h_vcol, d_qt, d_qw, & |
861 |
d_ql, d_qs, d_ec) |
862 |
! Comme les tendances de la physique sont ajoute dans la dynamique, |
863 |
! on devrait avoir que la variation d'entalpie par la dynamique |
864 |
! est egale a la variation de la physique au pas de temps precedent. |
865 |
! Donc la somme de ces 2 variations devrait etre nulle. |
866 |
call diagphy(airephy, ztit, ip_ebil, zero_v, zero_v, zero_v, zero_v, & |
867 |
zero_v, zero_v, zero_v, zero_v, ztsol, d_h_vcol+d_h_vcol_phy, & |
868 |
d_qt, 0., fs_bound, fq_bound) |
869 |
END IF |
870 |
|
871 |
! Diagnostiquer la tendance dynamique |
872 |
IF (ancien_ok) THEN |
873 |
DO k = 1, llm |
874 |
DO i = 1, klon |
875 |
d_t_dyn(i, k) = (t_seri(i, k) - t_ancien(i, k)) / dtphys |
876 |
d_q_dyn(i, k) = (q_seri(i, k) - q_ancien(i, k)) / dtphys |
877 |
ENDDO |
878 |
ENDDO |
879 |
ELSE |
880 |
DO k = 1, llm |
881 |
DO i = 1, klon |
882 |
d_t_dyn(i, k) = 0.0 |
883 |
d_q_dyn(i, k) = 0.0 |
884 |
ENDDO |
885 |
ENDDO |
886 |
ancien_ok = .TRUE. |
887 |
ENDIF |
888 |
|
889 |
! Ajouter le geopotentiel du sol: |
890 |
DO k = 1, llm |
891 |
DO i = 1, klon |
892 |
zphi(i, k) = pphi(i, k) + pphis(i) |
893 |
ENDDO |
894 |
ENDDO |
895 |
|
896 |
! Check temperatures: |
897 |
CALL hgardfou(t_seri, ftsol) |
898 |
|
899 |
! Incrementer le compteur de la physique |
900 |
itap = itap + 1 |
901 |
julien = MOD(NINT(rdayvrai), 360) |
902 |
if (julien == 0) julien = 360 |
903 |
|
904 |
forall (k = 1: llm) zmasse(:, k) = (paprs(:, k)-paprs(:, k+1)) / rg |
905 |
|
906 |
! Mettre en action les conditions aux limites (albedo, sst, etc.). |
907 |
|
908 |
! Prescrire l'ozone et calculer l'albedo sur l'ocean. |
909 |
if (nqmx >= 5) then |
910 |
wo = qx(:, :, 5) * zmasse / dobson_u / 1e3 |
911 |
else IF (MOD(itap - 1, lmt_pas) == 0) THEN |
912 |
wo = ozonecm(REAL(julien), paprs) |
913 |
ENDIF |
914 |
|
915 |
! Re-evaporer l'eau liquide nuageuse |
916 |
|
917 |
DO k = 1, llm ! re-evaporation de l'eau liquide nuageuse |
918 |
DO i = 1, klon |
919 |
zlvdcp=RLVTT/RCPD/(1.0+RVTMP2*q_seri(i, k)) |
920 |
zlsdcp=RLVTT/RCPD/(1.0+RVTMP2*q_seri(i, k)) |
921 |
zdelta = MAX(0., SIGN(1., RTT-t_seri(i, k))) |
922 |
zb = MAX(0.0, ql_seri(i, k)) |
923 |
za = - MAX(0.0, ql_seri(i, k)) & |
924 |
* (zlvdcp*(1.-zdelta)+zlsdcp*zdelta) |
925 |
t_seri(i, k) = t_seri(i, k) + za |
926 |
q_seri(i, k) = q_seri(i, k) + zb |
927 |
ql_seri(i, k) = 0.0 |
928 |
ENDDO |
929 |
ENDDO |
930 |
|
931 |
IF (if_ebil >= 2) THEN |
932 |
ztit='after reevap' |
933 |
CALL diagetpq(airephy, ztit, ip_ebil, 2, 1, dtphys, t_seri, q_seri, & |
934 |
ql_seri, qs_seri, u_seri, v_seri, paprs, d_h_vcol, d_qt, d_qw, & |
935 |
d_ql, d_qs, d_ec) |
936 |
call diagphy(airephy, ztit, ip_ebil, zero_v, zero_v, zero_v, zero_v, & |
937 |
zero_v, zero_v, zero_v, zero_v, ztsol, d_h_vcol, d_qt, d_ec, & |
938 |
fs_bound, fq_bound) |
939 |
|
940 |
END IF |
941 |
|
942 |
! Appeler la diffusion verticale (programme de couche limite) |
943 |
|
944 |
DO i = 1, klon |
945 |
zxrugs(i) = 0.0 |
946 |
ENDDO |
947 |
DO nsrf = 1, nbsrf |
948 |
DO i = 1, klon |
949 |
frugs(i, nsrf) = MAX(frugs(i, nsrf), 0.000015) |
950 |
ENDDO |
951 |
ENDDO |
952 |
DO nsrf = 1, nbsrf |
953 |
DO i = 1, klon |
954 |
zxrugs(i) = zxrugs(i) + frugs(i, nsrf)*pctsrf(i, nsrf) |
955 |
ENDDO |
956 |
ENDDO |
957 |
|
958 |
! calculs necessaires au calcul de l'albedo dans l'interface |
959 |
|
960 |
CALL orbite(REAL(julien), zlongi, dist) |
961 |
IF (cycle_diurne) THEN |
962 |
zdtime = dtphys * REAL(radpas) |
963 |
CALL zenang(zlongi, time, zdtime, rmu0, fract) |
964 |
ELSE |
965 |
rmu0 = -999.999 |
966 |
ENDIF |
967 |
|
968 |
! Calcul de l'abedo moyen par maille |
969 |
albsol(:)=0. |
970 |
albsollw(:)=0. |
971 |
DO nsrf = 1, nbsrf |
972 |
DO i = 1, klon |
973 |
albsol(i) = albsol(i) + falbe(i, nsrf) * pctsrf(i, nsrf) |
974 |
albsollw(i) = albsollw(i) + falblw(i, nsrf) * pctsrf(i, nsrf) |
975 |
ENDDO |
976 |
ENDDO |
977 |
|
978 |
! Repartition sous maille des flux LW et SW |
979 |
! Repartition du longwave par sous-surface linearisee |
980 |
|
981 |
DO nsrf = 1, nbsrf |
982 |
DO i = 1, klon |
983 |
fsollw(i, nsrf) = sollw(i) & |
984 |
+ 4.0*RSIGMA*ztsol(i)**3 * (ztsol(i)-ftsol(i, nsrf)) |
985 |
fsolsw(i, nsrf) = solsw(i)*(1.-falbe(i, nsrf))/(1.-albsol(i)) |
986 |
ENDDO |
987 |
ENDDO |
988 |
|
989 |
fder = dlw |
990 |
|
991 |
! Couche limite: |
992 |
|
993 |
CALL clmain(dtphys, itap, date0, pctsrf, pctsrf_new, t_seri, q_seri, & |
994 |
u_seri, v_seri, julien, rmu0, co2_ppm, ok_veget, ocean, npas, nexca, & |
995 |
ftsol, soil_model, cdmmax, cdhmax, ksta, ksta_ter, ok_kzmin, ftsoil, & |
996 |
qsol, paprs, play, fsnow, fqsurf, fevap, falbe, falblw, fluxlat, & |
997 |
rain_fall, snow_fall, fsolsw, fsollw, sollwdown, fder, rlon, rlat, & |
998 |
cuphy, cvphy, frugs, firstcal, lafin, agesno, rugoro, d_t_vdf, & |
999 |
d_q_vdf, d_u_vdf, d_v_vdf, d_ts, fluxt, fluxq, fluxu, fluxv, cdragh, & |
1000 |
cdragm, q2, dsens, devap, ycoefh, yu1, yv1, t2m, q2m, u10m, v10m, & |
1001 |
pblh, capCL, oliqCL, cteiCL, pblT, therm, trmb1, trmb2, trmb3, plcl, & |
1002 |
fqcalving, ffonte, run_off_lic_0, fluxo, fluxg, tslab, seaice) |
1003 |
|
1004 |
! Incrémentation des flux |
1005 |
|
1006 |
zxfluxt=0. |
1007 |
zxfluxq=0. |
1008 |
zxfluxu=0. |
1009 |
zxfluxv=0. |
1010 |
DO nsrf = 1, nbsrf |
1011 |
DO k = 1, llm |
1012 |
DO i = 1, klon |
1013 |
zxfluxt(i, k) = zxfluxt(i, k) + & |
1014 |
fluxt(i, k, nsrf) * pctsrf(i, nsrf) |
1015 |
zxfluxq(i, k) = zxfluxq(i, k) + & |
1016 |
fluxq(i, k, nsrf) * pctsrf(i, nsrf) |
1017 |
zxfluxu(i, k) = zxfluxu(i, k) + & |
1018 |
fluxu(i, k, nsrf) * pctsrf(i, nsrf) |
1019 |
zxfluxv(i, k) = zxfluxv(i, k) + & |
1020 |
fluxv(i, k, nsrf) * pctsrf(i, nsrf) |
1021 |
END DO |
1022 |
END DO |
1023 |
END DO |
1024 |
DO i = 1, klon |
1025 |
sens(i) = - zxfluxt(i, 1) ! flux de chaleur sensible au sol |
1026 |
evap(i) = - zxfluxq(i, 1) ! flux d'evaporation au sol |
1027 |
fder(i) = dlw(i) + dsens(i) + devap(i) |
1028 |
ENDDO |
1029 |
|
1030 |
DO k = 1, llm |
1031 |
DO i = 1, klon |
1032 |
t_seri(i, k) = t_seri(i, k) + d_t_vdf(i, k) |
1033 |
q_seri(i, k) = q_seri(i, k) + d_q_vdf(i, k) |
1034 |
u_seri(i, k) = u_seri(i, k) + d_u_vdf(i, k) |
1035 |
v_seri(i, k) = v_seri(i, k) + d_v_vdf(i, k) |
1036 |
ENDDO |
1037 |
ENDDO |
1038 |
|
1039 |
IF (if_ebil >= 2) THEN |
1040 |
ztit='after clmain' |
1041 |
CALL diagetpq(airephy, ztit, ip_ebil, 2, 2, dtphys, t_seri, q_seri, & |
1042 |
ql_seri, qs_seri, u_seri, v_seri, paprs, d_h_vcol, d_qt, d_qw, & |
1043 |
d_ql, d_qs, d_ec) |
1044 |
call diagphy(airephy, ztit, ip_ebil, zero_v, zero_v, zero_v, zero_v, & |
1045 |
sens, evap, zero_v, zero_v, ztsol, d_h_vcol, d_qt, d_ec, & |
1046 |
fs_bound, fq_bound) |
1047 |
END IF |
1048 |
|
1049 |
! Update surface temperature: |
1050 |
|
1051 |
DO i = 1, klon |
1052 |
zxtsol(i) = 0.0 |
1053 |
zxfluxlat(i) = 0.0 |
1054 |
|
1055 |
zt2m(i) = 0.0 |
1056 |
zq2m(i) = 0.0 |
1057 |
zu10m(i) = 0.0 |
1058 |
zv10m(i) = 0.0 |
1059 |
zxffonte(i) = 0.0 |
1060 |
zxfqcalving(i) = 0.0 |
1061 |
|
1062 |
s_pblh(i) = 0.0 |
1063 |
s_lcl(i) = 0.0 |
1064 |
s_capCL(i) = 0.0 |
1065 |
s_oliqCL(i) = 0.0 |
1066 |
s_cteiCL(i) = 0.0 |
1067 |
s_pblT(i) = 0.0 |
1068 |
s_therm(i) = 0.0 |
1069 |
s_trmb1(i) = 0.0 |
1070 |
s_trmb2(i) = 0.0 |
1071 |
s_trmb3(i) = 0.0 |
1072 |
|
1073 |
IF (abs(pctsrf(i, is_ter) + pctsrf(i, is_lic) + & |
1074 |
pctsrf(i, is_oce) + pctsrf(i, is_sic) - 1.) .GT. EPSFRA) & |
1075 |
THEN |
1076 |
WRITE(*, *) 'physiq : pb sous surface au point ', i, & |
1077 |
pctsrf(i, 1 : nbsrf) |
1078 |
ENDIF |
1079 |
ENDDO |
1080 |
DO nsrf = 1, nbsrf |
1081 |
DO i = 1, klon |
1082 |
ftsol(i, nsrf) = ftsol(i, nsrf) + d_ts(i, nsrf) |
1083 |
zxtsol(i) = zxtsol(i) + ftsol(i, nsrf)*pctsrf(i, nsrf) |
1084 |
zxfluxlat(i) = zxfluxlat(i) + fluxlat(i, nsrf)*pctsrf(i, nsrf) |
1085 |
|
1086 |
zt2m(i) = zt2m(i) + t2m(i, nsrf)*pctsrf(i, nsrf) |
1087 |
zq2m(i) = zq2m(i) + q2m(i, nsrf)*pctsrf(i, nsrf) |
1088 |
zu10m(i) = zu10m(i) + u10m(i, nsrf)*pctsrf(i, nsrf) |
1089 |
zv10m(i) = zv10m(i) + v10m(i, nsrf)*pctsrf(i, nsrf) |
1090 |
zxffonte(i) = zxffonte(i) + ffonte(i, nsrf)*pctsrf(i, nsrf) |
1091 |
zxfqcalving(i) = zxfqcalving(i) + & |
1092 |
fqcalving(i, nsrf)*pctsrf(i, nsrf) |
1093 |
s_pblh(i) = s_pblh(i) + pblh(i, nsrf)*pctsrf(i, nsrf) |
1094 |
s_lcl(i) = s_lcl(i) + plcl(i, nsrf)*pctsrf(i, nsrf) |
1095 |
s_capCL(i) = s_capCL(i) + capCL(i, nsrf) *pctsrf(i, nsrf) |
1096 |
s_oliqCL(i) = s_oliqCL(i) + oliqCL(i, nsrf) *pctsrf(i, nsrf) |
1097 |
s_cteiCL(i) = s_cteiCL(i) + cteiCL(i, nsrf) *pctsrf(i, nsrf) |
1098 |
s_pblT(i) = s_pblT(i) + pblT(i, nsrf) *pctsrf(i, nsrf) |
1099 |
s_therm(i) = s_therm(i) + therm(i, nsrf) *pctsrf(i, nsrf) |
1100 |
s_trmb1(i) = s_trmb1(i) + trmb1(i, nsrf) *pctsrf(i, nsrf) |
1101 |
s_trmb2(i) = s_trmb2(i) + trmb2(i, nsrf) *pctsrf(i, nsrf) |
1102 |
s_trmb3(i) = s_trmb3(i) + trmb3(i, nsrf) *pctsrf(i, nsrf) |
1103 |
ENDDO |
1104 |
ENDDO |
1105 |
|
1106 |
! Si une sous-fraction n'existe pas, elle prend la temp. moyenne |
1107 |
|
1108 |
DO nsrf = 1, nbsrf |
1109 |
DO i = 1, klon |
1110 |
IF (pctsrf(i, nsrf) < epsfra) ftsol(i, nsrf) = zxtsol(i) |
1111 |
|
1112 |
IF (pctsrf(i, nsrf) < epsfra) t2m(i, nsrf) = zt2m(i) |
1113 |
IF (pctsrf(i, nsrf) < epsfra) q2m(i, nsrf) = zq2m(i) |
1114 |
IF (pctsrf(i, nsrf) < epsfra) u10m(i, nsrf) = zu10m(i) |
1115 |
IF (pctsrf(i, nsrf) < epsfra) v10m(i, nsrf) = zv10m(i) |
1116 |
IF (pctsrf(i, nsrf) < epsfra) ffonte(i, nsrf) = zxffonte(i) |
1117 |
IF (pctsrf(i, nsrf) < epsfra) & |
1118 |
fqcalving(i, nsrf) = zxfqcalving(i) |
1119 |
IF (pctsrf(i, nsrf) < epsfra) pblh(i, nsrf)=s_pblh(i) |
1120 |
IF (pctsrf(i, nsrf) < epsfra) plcl(i, nsrf)=s_lcl(i) |
1121 |
IF (pctsrf(i, nsrf) < epsfra) capCL(i, nsrf)=s_capCL(i) |
1122 |
IF (pctsrf(i, nsrf) < epsfra) oliqCL(i, nsrf)=s_oliqCL(i) |
1123 |
IF (pctsrf(i, nsrf) < epsfra) cteiCL(i, nsrf)=s_cteiCL(i) |
1124 |
IF (pctsrf(i, nsrf) < epsfra) pblT(i, nsrf)=s_pblT(i) |
1125 |
IF (pctsrf(i, nsrf) < epsfra) therm(i, nsrf)=s_therm(i) |
1126 |
IF (pctsrf(i, nsrf) < epsfra) trmb1(i, nsrf)=s_trmb1(i) |
1127 |
IF (pctsrf(i, nsrf) < epsfra) trmb2(i, nsrf)=s_trmb2(i) |
1128 |
IF (pctsrf(i, nsrf) < epsfra) trmb3(i, nsrf)=s_trmb3(i) |
1129 |
ENDDO |
1130 |
ENDDO |
1131 |
|
1132 |
! Calculer la derive du flux infrarouge |
1133 |
|
1134 |
DO i = 1, klon |
1135 |
dlw(i) = - 4.0*RSIGMA*zxtsol(i)**3 |
1136 |
ENDDO |
1137 |
|
1138 |
! Appeler la convection (au choix) |
1139 |
|
1140 |
DO k = 1, llm |
1141 |
DO i = 1, klon |
1142 |
conv_q(i, k) = d_q_dyn(i, k) & |
1143 |
+ d_q_vdf(i, k)/dtphys |
1144 |
conv_t(i, k) = d_t_dyn(i, k) & |
1145 |
+ d_t_vdf(i, k)/dtphys |
1146 |
ENDDO |
1147 |
ENDDO |
1148 |
IF (check) THEN |
1149 |
za = qcheck(klon, llm, paprs, q_seri, ql_seri, airephy) |
1150 |
print *, "avantcon=", za |
1151 |
ENDIF |
1152 |
zx_ajustq = .FALSE. |
1153 |
IF (iflag_con == 2) zx_ajustq=.TRUE. |
1154 |
IF (zx_ajustq) THEN |
1155 |
DO i = 1, klon |
1156 |
z_avant(i) = 0.0 |
1157 |
ENDDO |
1158 |
DO k = 1, llm |
1159 |
DO i = 1, klon |
1160 |
z_avant(i) = z_avant(i) + (q_seri(i, k)+ql_seri(i, k)) & |
1161 |
*zmasse(i, k) |
1162 |
ENDDO |
1163 |
ENDDO |
1164 |
ENDIF |
1165 |
IF (iflag_con == 1) THEN |
1166 |
stop 'reactiver le call conlmd dans physiq.F' |
1167 |
ELSE IF (iflag_con == 2) THEN |
1168 |
CALL conflx(dtphys, paprs, play, t_seri, q_seri, & |
1169 |
conv_t, conv_q, zxfluxq(1, 1), omega, & |
1170 |
d_t_con, d_q_con, rain_con, snow_con, & |
1171 |
pmfu, pmfd, pen_u, pde_u, pen_d, pde_d, & |
1172 |
kcbot, kctop, kdtop, pmflxr, pmflxs) |
1173 |
WHERE (rain_con < 0.) rain_con = 0. |
1174 |
WHERE (snow_con < 0.) snow_con = 0. |
1175 |
DO i = 1, klon |
1176 |
ibas_con(i) = llm+1 - kcbot(i) |
1177 |
itop_con(i) = llm+1 - kctop(i) |
1178 |
ENDDO |
1179 |
ELSE IF (iflag_con >= 3) THEN |
1180 |
! nb of tracers for the KE convection: |
1181 |
! MAF la partie traceurs est faite dans phytrac |
1182 |
! on met ntra=1 pour limiter les appels mais on peut |
1183 |
! supprimer les calculs / ftra. |
1184 |
ntra = 1 |
1185 |
! Schema de convection modularise et vectorise: |
1186 |
! (driver commun aux versions 3 et 4) |
1187 |
|
1188 |
IF (ok_cvl) THEN ! new driver for convectL |
1189 |
CALL concvl(iflag_con, dtphys, paprs, play, t_seri, q_seri, & |
1190 |
u_seri, v_seri, tr_seri, ntra, ema_work1, ema_work2, d_t_con, & |
1191 |
d_q_con, d_u_con, d_v_con, d_tr, rain_con, snow_con, ibas_con, & |
1192 |
itop_con, upwd, dnwd, dnwd0, Ma, cape, tvp, iflagctrl, pbase, & |
1193 |
bbase, dtvpdt1, dtvpdq1, dplcldt, dplcldr, qcondc, wd, pmflxr, & |
1194 |
pmflxs, da, phi, mp) |
1195 |
|
1196 |
clwcon0=qcondc |
1197 |
pmfu=upwd+dnwd |
1198 |
ELSE |
1199 |
! MAF conema3 ne contient pas les traceurs |
1200 |
CALL conema3 (dtphys, paprs, play, t_seri, q_seri, & |
1201 |
u_seri, v_seri, tr_seri, ntra, & |
1202 |
ema_work1, ema_work2, & |
1203 |
d_t_con, d_q_con, d_u_con, d_v_con, d_tr, & |
1204 |
rain_con, snow_con, ibas_con, itop_con, & |
1205 |
upwd, dnwd, dnwd0, bas, top, & |
1206 |
Ma, cape, tvp, rflag, & |
1207 |
pbase & |
1208 |
, bbase, dtvpdt1, dtvpdq1, dplcldt, dplcldr & |
1209 |
, clwcon0) |
1210 |
ENDIF ! ok_cvl |
1211 |
|
1212 |
IF (.NOT. ok_gust) THEN |
1213 |
do i = 1, klon |
1214 |
wd(i)=0.0 |
1215 |
enddo |
1216 |
ENDIF |
1217 |
|
1218 |
! Calcul des proprietes des nuages convectifs |
1219 |
|
1220 |
DO k = 1, llm |
1221 |
DO i = 1, klon |
1222 |
zx_t = t_seri(i, k) |
1223 |
IF (thermcep) THEN |
1224 |
zdelta = MAX(0., SIGN(1., rtt-zx_t)) |
1225 |
zx_qs = r2es * FOEEW(zx_t, zdelta)/play(i, k) |
1226 |
zx_qs = MIN(0.5, zx_qs) |
1227 |
zcor = 1./(1.-retv*zx_qs) |
1228 |
zx_qs = zx_qs*zcor |
1229 |
ELSE |
1230 |
IF (zx_t < t_coup) THEN |
1231 |
zx_qs = qsats(zx_t)/play(i, k) |
1232 |
ELSE |
1233 |
zx_qs = qsatl(zx_t)/play(i, k) |
1234 |
ENDIF |
1235 |
ENDIF |
1236 |
zqsat(i, k)=zx_qs |
1237 |
ENDDO |
1238 |
ENDDO |
1239 |
|
1240 |
! calcul des proprietes des nuages convectifs |
1241 |
clwcon0=fact_cldcon*clwcon0 |
1242 |
call clouds_gno & |
1243 |
(klon, llm, q_seri, zqsat, clwcon0, ptconv, ratqsc, rnebcon0) |
1244 |
ELSE |
1245 |
print *, "iflag_con non-prevu", iflag_con |
1246 |
stop 1 |
1247 |
ENDIF |
1248 |
|
1249 |
DO k = 1, llm |
1250 |
DO i = 1, klon |
1251 |
t_seri(i, k) = t_seri(i, k) + d_t_con(i, k) |
1252 |
q_seri(i, k) = q_seri(i, k) + d_q_con(i, k) |
1253 |
u_seri(i, k) = u_seri(i, k) + d_u_con(i, k) |
1254 |
v_seri(i, k) = v_seri(i, k) + d_v_con(i, k) |
1255 |
ENDDO |
1256 |
ENDDO |
1257 |
|
1258 |
IF (if_ebil >= 2) THEN |
1259 |
ztit='after convect' |
1260 |
CALL diagetpq(airephy, ztit, ip_ebil, 2, 2, dtphys, t_seri, q_seri, & |
1261 |
ql_seri, qs_seri, u_seri, v_seri, paprs, d_h_vcol, d_qt, d_qw, & |
1262 |
d_ql, d_qs, d_ec) |
1263 |
call diagphy(airephy, ztit, ip_ebil, zero_v, zero_v, zero_v, zero_v, & |
1264 |
zero_v, zero_v, rain_con, snow_con, ztsol, d_h_vcol, d_qt, d_ec, & |
1265 |
fs_bound, fq_bound) |
1266 |
END IF |
1267 |
|
1268 |
IF (check) THEN |
1269 |
za = qcheck(klon, llm, paprs, q_seri, ql_seri, airephy) |
1270 |
print *,"aprescon=", za |
1271 |
zx_t = 0.0 |
1272 |
za = 0.0 |
1273 |
DO i = 1, klon |
1274 |
za = za + airephy(i)/REAL(klon) |
1275 |
zx_t = zx_t + (rain_con(i)+ & |
1276 |
snow_con(i))*airephy(i)/REAL(klon) |
1277 |
ENDDO |
1278 |
zx_t = zx_t/za*dtphys |
1279 |
print *,"Precip=", zx_t |
1280 |
ENDIF |
1281 |
IF (zx_ajustq) THEN |
1282 |
DO i = 1, klon |
1283 |
z_apres(i) = 0.0 |
1284 |
ENDDO |
1285 |
DO k = 1, llm |
1286 |
DO i = 1, klon |
1287 |
z_apres(i) = z_apres(i) + (q_seri(i, k)+ql_seri(i, k)) & |
1288 |
*zmasse(i, k) |
1289 |
ENDDO |
1290 |
ENDDO |
1291 |
DO i = 1, klon |
1292 |
z_factor(i) = (z_avant(i)-(rain_con(i)+snow_con(i))*dtphys) & |
1293 |
/z_apres(i) |
1294 |
ENDDO |
1295 |
DO k = 1, llm |
1296 |
DO i = 1, klon |
1297 |
IF (z_factor(i).GT.(1.0+1.0E-08) .OR. & |
1298 |
z_factor(i) < (1.0-1.0E-08)) THEN |
1299 |
q_seri(i, k) = q_seri(i, k) * z_factor(i) |
1300 |
ENDIF |
1301 |
ENDDO |
1302 |
ENDDO |
1303 |
ENDIF |
1304 |
zx_ajustq=.FALSE. |
1305 |
|
1306 |
! Convection seche (thermiques ou ajustement) |
1307 |
|
1308 |
d_t_ajs=0. |
1309 |
d_u_ajs=0. |
1310 |
d_v_ajs=0. |
1311 |
d_q_ajs=0. |
1312 |
fm_therm=0. |
1313 |
entr_therm=0. |
1314 |
|
1315 |
if (iflag_thermals == 0) then |
1316 |
! Ajustement sec |
1317 |
CALL ajsec(paprs, play, t_seri, q_seri, d_t_ajs, d_q_ajs) |
1318 |
t_seri = t_seri + d_t_ajs |
1319 |
q_seri = q_seri + d_q_ajs |
1320 |
else |
1321 |
! Thermiques |
1322 |
call calltherm(dtphys, play, paprs, pphi, u_seri, v_seri, t_seri, & |
1323 |
q_seri, d_u_ajs, d_v_ajs, d_t_ajs, d_q_ajs, fm_therm, entr_therm) |
1324 |
endif |
1325 |
|
1326 |
IF (if_ebil >= 2) THEN |
1327 |
ztit='after dry_adjust' |
1328 |
CALL diagetpq(airephy, ztit, ip_ebil, 2, 2, dtphys, t_seri, q_seri, & |
1329 |
ql_seri, qs_seri, u_seri, v_seri, paprs, d_h_vcol, d_qt, d_qw, & |
1330 |
d_ql, d_qs, d_ec) |
1331 |
END IF |
1332 |
|
1333 |
! Caclul des ratqs |
1334 |
|
1335 |
! ratqs convectifs a l'ancienne en fonction de q(z=0)-q / q |
1336 |
! on ecrase le tableau ratqsc calcule par clouds_gno |
1337 |
if (iflag_cldcon == 1) then |
1338 |
do k=1, llm |
1339 |
do i=1, klon |
1340 |
if(ptconv(i, k)) then |
1341 |
ratqsc(i, k)=ratqsbas & |
1342 |
+fact_cldcon*(q_seri(i, 1)-q_seri(i, k))/q_seri(i, k) |
1343 |
else |
1344 |
ratqsc(i, k)=0. |
1345 |
endif |
1346 |
enddo |
1347 |
enddo |
1348 |
endif |
1349 |
|
1350 |
! ratqs stables |
1351 |
do k=1, llm |
1352 |
do i=1, klon |
1353 |
ratqss(i, k)=ratqsbas+(ratqshaut-ratqsbas)* & |
1354 |
min((paprs(i, 1)-play(i, k))/(paprs(i, 1)-30000.), 1.) |
1355 |
enddo |
1356 |
enddo |
1357 |
|
1358 |
! ratqs final |
1359 |
if (iflag_cldcon == 1 .or.iflag_cldcon == 2) then |
1360 |
! les ratqs sont une conbinaison de ratqss et ratqsc |
1361 |
! ratqs final |
1362 |
! 1e4 (en gros 3 heures), en dur pour le moment, est le temps de |
1363 |
! relaxation des ratqs |
1364 |
facteur=exp(-dtphys*facttemps) |
1365 |
ratqs=max(ratqs*facteur, ratqss) |
1366 |
ratqs=max(ratqs, ratqsc) |
1367 |
else |
1368 |
! on ne prend que le ratqs stable pour fisrtilp |
1369 |
ratqs=ratqss |
1370 |
endif |
1371 |
|
1372 |
! Appeler le processus de condensation a grande echelle |
1373 |
! et le processus de precipitation |
1374 |
CALL fisrtilp(dtphys, paprs, play, & |
1375 |
t_seri, q_seri, ptconv, ratqs, & |
1376 |
d_t_lsc, d_q_lsc, d_ql_lsc, rneb, cldliq, & |
1377 |
rain_lsc, snow_lsc, & |
1378 |
pfrac_impa, pfrac_nucl, pfrac_1nucl, & |
1379 |
frac_impa, frac_nucl, & |
1380 |
prfl, psfl, rhcl) |
1381 |
|
1382 |
WHERE (rain_lsc < 0) rain_lsc = 0. |
1383 |
WHERE (snow_lsc < 0) snow_lsc = 0. |
1384 |
DO k = 1, llm |
1385 |
DO i = 1, klon |
1386 |
t_seri(i, k) = t_seri(i, k) + d_t_lsc(i, k) |
1387 |
q_seri(i, k) = q_seri(i, k) + d_q_lsc(i, k) |
1388 |
ql_seri(i, k) = ql_seri(i, k) + d_ql_lsc(i, k) |
1389 |
cldfra(i, k) = rneb(i, k) |
1390 |
IF (.NOT.new_oliq) cldliq(i, k) = ql_seri(i, k) |
1391 |
ENDDO |
1392 |
ENDDO |
1393 |
IF (check) THEN |
1394 |
za = qcheck(klon, llm, paprs, q_seri, ql_seri, airephy) |
1395 |
print *,"apresilp=", za |
1396 |
zx_t = 0.0 |
1397 |
za = 0.0 |
1398 |
DO i = 1, klon |
1399 |
za = za + airephy(i)/REAL(klon) |
1400 |
zx_t = zx_t + (rain_lsc(i) & |
1401 |
+ snow_lsc(i))*airephy(i)/REAL(klon) |
1402 |
ENDDO |
1403 |
zx_t = zx_t/za*dtphys |
1404 |
print *,"Precip=", zx_t |
1405 |
ENDIF |
1406 |
|
1407 |
IF (if_ebil >= 2) THEN |
1408 |
ztit='after fisrt' |
1409 |
CALL diagetpq(airephy, ztit, ip_ebil, 2, 2, dtphys, t_seri, q_seri, & |
1410 |
ql_seri, qs_seri, u_seri, v_seri, paprs, d_h_vcol, d_qt, d_qw, & |
1411 |
d_ql, d_qs, d_ec) |
1412 |
call diagphy(airephy, ztit, ip_ebil, zero_v, zero_v, zero_v, zero_v, & |
1413 |
zero_v, zero_v, rain_lsc, snow_lsc, ztsol, d_h_vcol, d_qt, d_ec, & |
1414 |
fs_bound, fq_bound) |
1415 |
END IF |
1416 |
|
1417 |
! PRESCRIPTION DES NUAGES POUR LE RAYONNEMENT |
1418 |
|
1419 |
! 1. NUAGES CONVECTIFS |
1420 |
|
1421 |
IF (iflag_cldcon.le.-1) THEN ! seulement pour Tiedtke |
1422 |
snow_tiedtke=0. |
1423 |
if (iflag_cldcon == -1) then |
1424 |
rain_tiedtke=rain_con |
1425 |
else |
1426 |
rain_tiedtke=0. |
1427 |
do k=1, llm |
1428 |
do i=1, klon |
1429 |
if (d_q_con(i, k) < 0.) then |
1430 |
rain_tiedtke(i)=rain_tiedtke(i)-d_q_con(i, k)/dtphys & |
1431 |
*zmasse(i, k) |
1432 |
endif |
1433 |
enddo |
1434 |
enddo |
1435 |
endif |
1436 |
|
1437 |
! Nuages diagnostiques pour Tiedtke |
1438 |
CALL diagcld1(paprs, play, & |
1439 |
rain_tiedtke, snow_tiedtke, ibas_con, itop_con, & |
1440 |
diafra, dialiq) |
1441 |
DO k = 1, llm |
1442 |
DO i = 1, klon |
1443 |
IF (diafra(i, k).GT.cldfra(i, k)) THEN |
1444 |
cldliq(i, k) = dialiq(i, k) |
1445 |
cldfra(i, k) = diafra(i, k) |
1446 |
ENDIF |
1447 |
ENDDO |
1448 |
ENDDO |
1449 |
ELSE IF (iflag_cldcon == 3) THEN |
1450 |
! On prend pour les nuages convectifs le max du calcul de la |
1451 |
! convection et du calcul du pas de temps précédent diminué d'un facteur |
1452 |
! facttemps |
1453 |
facteur = dtphys *facttemps |
1454 |
do k=1, llm |
1455 |
do i=1, klon |
1456 |
rnebcon(i, k)=rnebcon(i, k)*facteur |
1457 |
if (rnebcon0(i, k)*clwcon0(i, k).gt.rnebcon(i, k)*clwcon(i, k)) & |
1458 |
then |
1459 |
rnebcon(i, k)=rnebcon0(i, k) |
1460 |
clwcon(i, k)=clwcon0(i, k) |
1461 |
endif |
1462 |
enddo |
1463 |
enddo |
1464 |
|
1465 |
! On prend la somme des fractions nuageuses et des contenus en eau |
1466 |
cldfra=min(max(cldfra, rnebcon), 1.) |
1467 |
cldliq=cldliq+rnebcon*clwcon |
1468 |
ENDIF |
1469 |
|
1470 |
! 2. NUAGES STARTIFORMES |
1471 |
|
1472 |
IF (ok_stratus) THEN |
1473 |
CALL diagcld2(paprs, play, t_seri, q_seri, diafra, dialiq) |
1474 |
DO k = 1, llm |
1475 |
DO i = 1, klon |
1476 |
IF (diafra(i, k).GT.cldfra(i, k)) THEN |
1477 |
cldliq(i, k) = dialiq(i, k) |
1478 |
cldfra(i, k) = diafra(i, k) |
1479 |
ENDIF |
1480 |
ENDDO |
1481 |
ENDDO |
1482 |
ENDIF |
1483 |
|
1484 |
! Precipitation totale |
1485 |
|
1486 |
DO i = 1, klon |
1487 |
rain_fall(i) = rain_con(i) + rain_lsc(i) |
1488 |
snow_fall(i) = snow_con(i) + snow_lsc(i) |
1489 |
ENDDO |
1490 |
|
1491 |
IF (if_ebil >= 2) THEN |
1492 |
ztit="after diagcld" |
1493 |
CALL diagetpq(airephy, ztit, ip_ebil, 2, 2, dtphys, t_seri, q_seri, & |
1494 |
ql_seri, qs_seri, u_seri, v_seri, paprs, d_h_vcol, d_qt, d_qw, & |
1495 |
d_ql, d_qs, d_ec) |
1496 |
END IF |
1497 |
|
1498 |
! Calculer l'humidite relative pour diagnostique |
1499 |
|
1500 |
DO k = 1, llm |
1501 |
DO i = 1, klon |
1502 |
zx_t = t_seri(i, k) |
1503 |
IF (thermcep) THEN |
1504 |
zdelta = MAX(0., SIGN(1., rtt-zx_t)) |
1505 |
zx_qs = r2es * FOEEW(zx_t, zdelta)/play(i, k) |
1506 |
zx_qs = MIN(0.5, zx_qs) |
1507 |
zcor = 1./(1.-retv*zx_qs) |
1508 |
zx_qs = zx_qs*zcor |
1509 |
ELSE |
1510 |
IF (zx_t < t_coup) THEN |
1511 |
zx_qs = qsats(zx_t)/play(i, k) |
1512 |
ELSE |
1513 |
zx_qs = qsatl(zx_t)/play(i, k) |
1514 |
ENDIF |
1515 |
ENDIF |
1516 |
zx_rh(i, k) = q_seri(i, k)/zx_qs |
1517 |
zqsat(i, k)=zx_qs |
1518 |
ENDDO |
1519 |
ENDDO |
1520 |
!jq - introduce the aerosol direct and first indirect radiative forcings |
1521 |
!jq - Johannes Quaas, 27/11/2003 (quaas@lmd.jussieu.fr) |
1522 |
IF (ok_ade.OR.ok_aie) THEN |
1523 |
! Get sulfate aerosol distribution |
1524 |
CALL readsulfate(rdayvrai, firstcal, sulfate) |
1525 |
CALL readsulfate_preind(rdayvrai, firstcal, sulfate_pi) |
1526 |
|
1527 |
! Calculate aerosol optical properties (Olivier Boucher) |
1528 |
CALL aeropt(play, paprs, t_seri, sulfate, rhcl, & |
1529 |
tau_ae, piz_ae, cg_ae, aerindex) |
1530 |
ELSE |
1531 |
tau_ae=0.0 |
1532 |
piz_ae=0.0 |
1533 |
cg_ae=0.0 |
1534 |
ENDIF |
1535 |
|
1536 |
! Calculer les parametres optiques des nuages et quelques |
1537 |
! parametres pour diagnostiques: |
1538 |
|
1539 |
if (ok_newmicro) then |
1540 |
CALL newmicro (paprs, play, ok_newmicro, & |
1541 |
t_seri, cldliq, cldfra, cldtau, cldemi, & |
1542 |
cldh, cldl, cldm, cldt, cldq, & |
1543 |
flwp, fiwp, flwc, fiwc, & |
1544 |
ok_aie, & |
1545 |
sulfate, sulfate_pi, & |
1546 |
bl95_b0, bl95_b1, & |
1547 |
cldtaupi, re, fl) |
1548 |
else |
1549 |
CALL nuage (paprs, play, & |
1550 |
t_seri, cldliq, cldfra, cldtau, cldemi, & |
1551 |
cldh, cldl, cldm, cldt, cldq, & |
1552 |
ok_aie, & |
1553 |
sulfate, sulfate_pi, & |
1554 |
bl95_b0, bl95_b1, & |
1555 |
cldtaupi, re, fl) |
1556 |
|
1557 |
endif |
1558 |
|
1559 |
! Appeler le rayonnement mais calculer tout d'abord l'albedo du sol. |
1560 |
|
1561 |
IF (MOD(itaprad, radpas) == 0) THEN |
1562 |
DO i = 1, klon |
1563 |
albsol(i) = falbe(i, is_oce) * pctsrf(i, is_oce) & |
1564 |
+ falbe(i, is_lic) * pctsrf(i, is_lic) & |
1565 |
+ falbe(i, is_ter) * pctsrf(i, is_ter) & |
1566 |
+ falbe(i, is_sic) * pctsrf(i, is_sic) |
1567 |
albsollw(i) = falblw(i, is_oce) * pctsrf(i, is_oce) & |
1568 |
+ falblw(i, is_lic) * pctsrf(i, is_lic) & |
1569 |
+ falblw(i, is_ter) * pctsrf(i, is_ter) & |
1570 |
+ falblw(i, is_sic) * pctsrf(i, is_sic) |
1571 |
ENDDO |
1572 |
! nouveau rayonnement (compatible Arpege-IFS): |
1573 |
CALL radlwsw(dist, rmu0, fract, paprs, play, zxtsol, albsol, & |
1574 |
albsollw, t_seri, q_seri, wo, cldfra, cldemi, cldtau, heat, & |
1575 |
heat0, cool, cool0, radsol, albpla, topsw, toplw, solsw, sollw, & |
1576 |
sollwdown, topsw0, toplw0, solsw0, sollw0, lwdn0, lwdn, lwup0, & |
1577 |
lwup, swdn0, swdn, swup0, swup, ok_ade, ok_aie, tau_ae, piz_ae, & |
1578 |
cg_ae, topswad, solswad, cldtaupi, topswai, solswai) |
1579 |
itaprad = 0 |
1580 |
ENDIF |
1581 |
itaprad = itaprad + 1 |
1582 |
|
1583 |
! Ajouter la tendance des rayonnements (tous les pas) |
1584 |
|
1585 |
DO k = 1, llm |
1586 |
DO i = 1, klon |
1587 |
t_seri(i, k) = t_seri(i, k) & |
1588 |
+ (heat(i, k)-cool(i, k)) * dtphys/86400. |
1589 |
ENDDO |
1590 |
ENDDO |
1591 |
|
1592 |
IF (if_ebil >= 2) THEN |
1593 |
ztit='after rad' |
1594 |
CALL diagetpq(airephy, ztit, ip_ebil, 2, 2, dtphys, t_seri, q_seri, & |
1595 |
ql_seri, qs_seri, u_seri, v_seri, paprs, d_h_vcol, d_qt, d_qw, & |
1596 |
d_ql, d_qs, d_ec) |
1597 |
call diagphy(airephy, ztit, ip_ebil, topsw, toplw, solsw, sollw, & |
1598 |
zero_v, zero_v, zero_v, zero_v, ztsol, d_h_vcol, d_qt, d_ec, & |
1599 |
fs_bound, fq_bound) |
1600 |
END IF |
1601 |
|
1602 |
! Calculer l'hydrologie de la surface |
1603 |
DO i = 1, klon |
1604 |
zxqsurf(i) = 0.0 |
1605 |
zxsnow(i) = 0.0 |
1606 |
ENDDO |
1607 |
DO nsrf = 1, nbsrf |
1608 |
DO i = 1, klon |
1609 |
zxqsurf(i) = zxqsurf(i) + fqsurf(i, nsrf)*pctsrf(i, nsrf) |
1610 |
zxsnow(i) = zxsnow(i) + fsnow(i, nsrf)*pctsrf(i, nsrf) |
1611 |
ENDDO |
1612 |
ENDDO |
1613 |
|
1614 |
! Calculer le bilan du sol et la derive de temperature (couplage) |
1615 |
|
1616 |
DO i = 1, klon |
1617 |
bils(i) = radsol(i) - sens(i) + zxfluxlat(i) |
1618 |
ENDDO |
1619 |
|
1620 |
!mod deb lott(jan95) |
1621 |
! Appeler le programme de parametrisation de l'orographie |
1622 |
! a l'echelle sous-maille: |
1623 |
|
1624 |
IF (ok_orodr) THEN |
1625 |
! selection des points pour lesquels le shema est actif: |
1626 |
igwd=0 |
1627 |
DO i=1, klon |
1628 |
itest(i)=0 |
1629 |
IF (((zpic(i)-zmea(i)).GT.100.).AND.(zstd(i).GT.10.0)) THEN |
1630 |
itest(i)=1 |
1631 |
igwd=igwd+1 |
1632 |
idx(igwd)=i |
1633 |
ENDIF |
1634 |
ENDDO |
1635 |
|
1636 |
CALL drag_noro(klon, llm, dtphys, paprs, play, & |
1637 |
zmea, zstd, zsig, zgam, zthe, zpic, zval, & |
1638 |
igwd, idx, itest, & |
1639 |
t_seri, u_seri, v_seri, & |
1640 |
zulow, zvlow, zustrdr, zvstrdr, & |
1641 |
d_t_oro, d_u_oro, d_v_oro) |
1642 |
|
1643 |
! ajout des tendances |
1644 |
DO k = 1, llm |
1645 |
DO i = 1, klon |
1646 |
t_seri(i, k) = t_seri(i, k) + d_t_oro(i, k) |
1647 |
u_seri(i, k) = u_seri(i, k) + d_u_oro(i, k) |
1648 |
v_seri(i, k) = v_seri(i, k) + d_v_oro(i, k) |
1649 |
ENDDO |
1650 |
ENDDO |
1651 |
ENDIF |
1652 |
|
1653 |
IF (ok_orolf) THEN |
1654 |
! selection des points pour lesquels le shema est actif: |
1655 |
igwd=0 |
1656 |
DO i=1, klon |
1657 |
itest(i)=0 |
1658 |
IF ((zpic(i)-zmea(i)).GT.100.) THEN |
1659 |
itest(i)=1 |
1660 |
igwd=igwd+1 |
1661 |
idx(igwd)=i |
1662 |
ENDIF |
1663 |
ENDDO |
1664 |
|
1665 |
CALL lift_noro(klon, llm, dtphys, paprs, play, rlat, zmea, zstd, zpic, & |
1666 |
itest, t_seri, u_seri, v_seri, zulow, zvlow, zustrli, zvstrli, & |
1667 |
d_t_lif, d_u_lif, d_v_lif) |
1668 |
|
1669 |
! ajout des tendances |
1670 |
DO k = 1, llm |
1671 |
DO i = 1, klon |
1672 |
t_seri(i, k) = t_seri(i, k) + d_t_lif(i, k) |
1673 |
u_seri(i, k) = u_seri(i, k) + d_u_lif(i, k) |
1674 |
v_seri(i, k) = v_seri(i, k) + d_v_lif(i, k) |
1675 |
ENDDO |
1676 |
ENDDO |
1677 |
ENDIF |
1678 |
|
1679 |
! STRESS NECESSAIRES: TOUTE LA PHYSIQUE |
1680 |
|
1681 |
DO i = 1, klon |
1682 |
zustrph(i)=0. |
1683 |
zvstrph(i)=0. |
1684 |
ENDDO |
1685 |
DO k = 1, llm |
1686 |
DO i = 1, klon |
1687 |
zustrph(i)=zustrph(i)+(u_seri(i, k)-u(i, k))/dtphys* zmasse(i, k) |
1688 |
zvstrph(i)=zvstrph(i)+(v_seri(i, k)-v(i, k))/dtphys* zmasse(i, k) |
1689 |
ENDDO |
1690 |
ENDDO |
1691 |
|
1692 |
!IM calcul composantes axiales du moment angulaire et couple des montagnes |
1693 |
|
1694 |
CALL aaam_bud(27, klon, llm, time, ra, rg, romega, rlat, rlon, pphis, & |
1695 |
zustrdr, zustrli, zustrph, zvstrdr, zvstrli, zvstrph, paprs, u, v, & |
1696 |
aam, torsfc) |
1697 |
|
1698 |
IF (if_ebil >= 2) THEN |
1699 |
ztit='after orography' |
1700 |
CALL diagetpq(airephy, ztit, ip_ebil, 2, 2, dtphys, t_seri, q_seri, & |
1701 |
ql_seri, qs_seri, u_seri, v_seri, paprs, d_h_vcol, d_qt, d_qw, & |
1702 |
d_ql, d_qs, d_ec) |
1703 |
END IF |
1704 |
|
1705 |
! Calcul des tendances traceurs |
1706 |
call phytrac(rnpb, itap, lmt_pas, julien, time, firstcal, lafin, & |
1707 |
nqmx-2, dtphys, u, t, paprs, play, pmfu, pmfd, pen_u, pde_u, & |
1708 |
pen_d, pde_d, ycoefh, fm_therm, entr_therm, yu1, yv1, ftsol, pctsrf, & |
1709 |
frac_impa, frac_nucl, pphis, albsol, rhcl, cldfra, rneb, & |
1710 |
diafra, cldliq, pmflxr, pmflxs, prfl, psfl, da, phi, mp, upwd, dnwd, & |
1711 |
tr_seri, zmasse) |
1712 |
|
1713 |
IF (offline) THEN |
1714 |
call phystokenc(dtphys, rlon, rlat, t, pmfu, pmfd, pen_u, pde_u, & |
1715 |
pen_d, pde_d, fm_therm, entr_therm, ycoefh, yu1, yv1, ftsol, & |
1716 |
pctsrf, frac_impa, frac_nucl, pphis, airephy, dtphys, itap) |
1717 |
ENDIF |
1718 |
|
1719 |
! Calculer le transport de l'eau et de l'energie (diagnostique) |
1720 |
CALL transp(paprs, zxtsol, t_seri, q_seri, u_seri, v_seri, zphi, ve, vq, & |
1721 |
ue, uq) |
1722 |
|
1723 |
! diag. bilKP |
1724 |
|
1725 |
CALL transp_lay (paprs, zxtsol, t_seri, q_seri, u_seri, v_seri, zphi, & |
1726 |
ve_lay, vq_lay, ue_lay, uq_lay) |
1727 |
|
1728 |
! Accumuler les variables a stocker dans les fichiers histoire: |
1729 |
|
1730 |
!+jld ec_conser |
1731 |
DO k = 1, llm |
1732 |
DO i = 1, klon |
1733 |
ZRCPD = RCPD*(1.0+RVTMP2*q_seri(i, k)) |
1734 |
d_t_ec(i, k)=0.5/ZRCPD & |
1735 |
*(u(i, k)**2+v(i, k)**2-u_seri(i, k)**2-v_seri(i, k)**2) |
1736 |
t_seri(i, k)=t_seri(i, k)+d_t_ec(i, k) |
1737 |
d_t_ec(i, k) = d_t_ec(i, k)/dtphys |
1738 |
END DO |
1739 |
END DO |
1740 |
!-jld ec_conser |
1741 |
IF (if_ebil >= 1) THEN |
1742 |
ztit='after physic' |
1743 |
CALL diagetpq(airephy, ztit, ip_ebil, 1, 1, dtphys, t_seri, q_seri, & |
1744 |
ql_seri, qs_seri, u_seri, v_seri, paprs, d_h_vcol, d_qt, d_qw, & |
1745 |
d_ql, d_qs, d_ec) |
1746 |
! Comme les tendances de la physique sont ajoute dans la dynamique, |
1747 |
! on devrait avoir que la variation d'entalpie par la dynamique |
1748 |
! est egale a la variation de la physique au pas de temps precedent. |
1749 |
! Donc la somme de ces 2 variations devrait etre nulle. |
1750 |
call diagphy(airephy, ztit, ip_ebil, topsw, toplw, solsw, sollw, sens, & |
1751 |
evap, rain_fall, snow_fall, ztsol, d_h_vcol, d_qt, d_ec, & |
1752 |
fs_bound, fq_bound) |
1753 |
|
1754 |
d_h_vcol_phy=d_h_vcol |
1755 |
|
1756 |
END IF |
1757 |
|
1758 |
! SORTIES |
1759 |
|
1760 |
!cc prw = eau precipitable |
1761 |
DO i = 1, klon |
1762 |
prw(i) = 0. |
1763 |
DO k = 1, llm |
1764 |
prw(i) = prw(i) + q_seri(i, k)*zmasse(i, k) |
1765 |
ENDDO |
1766 |
ENDDO |
1767 |
|
1768 |
! Convertir les incrementations en tendances |
1769 |
|
1770 |
DO k = 1, llm |
1771 |
DO i = 1, klon |
1772 |
d_u(i, k) = (u_seri(i, k) - u(i, k)) / dtphys |
1773 |
d_v(i, k) = (v_seri(i, k) - v(i, k)) / dtphys |
1774 |
d_t(i, k) = (t_seri(i, k) - t(i, k)) / dtphys |
1775 |
d_qx(i, k, ivap) = (q_seri(i, k) - qx(i, k, ivap)) / dtphys |
1776 |
d_qx(i, k, iliq) = (ql_seri(i, k) - qx(i, k, iliq)) / dtphys |
1777 |
ENDDO |
1778 |
ENDDO |
1779 |
|
1780 |
IF (nqmx >= 3) THEN |
1781 |
DO iq = 3, nqmx |
1782 |
DO k = 1, llm |
1783 |
DO i = 1, klon |
1784 |
d_qx(i, k, iq) = (tr_seri(i, k, iq-2) - qx(i, k, iq)) / dtphys |
1785 |
ENDDO |
1786 |
ENDDO |
1787 |
ENDDO |
1788 |
ENDIF |
1789 |
|
1790 |
! Sauvegarder les valeurs de t et q a la fin de la physique: |
1791 |
DO k = 1, llm |
1792 |
DO i = 1, klon |
1793 |
t_ancien(i, k) = t_seri(i, k) |
1794 |
q_ancien(i, k) = q_seri(i, k) |
1795 |
ENDDO |
1796 |
ENDDO |
1797 |
|
1798 |
! Ecriture des sorties |
1799 |
call write_histhf |
1800 |
call write_histday |
1801 |
call write_histins |
1802 |
|
1803 |
! Si c'est la fin, il faut conserver l'etat de redemarrage |
1804 |
IF (lafin) THEN |
1805 |
itau_phy = itau_phy + itap |
1806 |
CALL phyredem("restartphy.nc", rlat, rlon, pctsrf, ftsol, ftsoil, & |
1807 |
tslab, seaice, fqsurf, qsol, fsnow, falbe, falblw, fevap, & |
1808 |
rain_fall, snow_fall, solsw, sollwdown, dlw, radsol, frugs, & |
1809 |
agesno, zmea, zstd, zsig, zgam, zthe, zpic, zval, t_ancien, & |
1810 |
q_ancien, rnebcon, ratqs, clwcon, run_off_lic_0) |
1811 |
ENDIF |
1812 |
|
1813 |
firstcal = .FALSE. |
1814 |
|
1815 |
contains |
1816 |
|
1817 |
subroutine write_histday |
1818 |
|
1819 |
use gr_phy_write_3d_m, only: gr_phy_write_3d |
1820 |
integer itau_w ! pas de temps ecriture |
1821 |
|
1822 |
!------------------------------------------------ |
1823 |
|
1824 |
if (ok_journe) THEN |
1825 |
itau_w = itau_phy + itap |
1826 |
if (nqmx <= 4) then |
1827 |
call histwrite(nid_day, "Sigma_O3_Royer", itau_w, & |
1828 |
gr_phy_write_3d(wo) * 1e3) |
1829 |
! (convert "wo" from kDU to DU) |
1830 |
end if |
1831 |
if (ok_sync) then |
1832 |
call histsync(nid_day) |
1833 |
endif |
1834 |
ENDIF |
1835 |
|
1836 |
End subroutine write_histday |
1837 |
|
1838 |
!**************************** |
1839 |
|
1840 |
subroutine write_histhf |
1841 |
|
1842 |
! From phylmd/write_histhf.h, version 1.5 2005/05/25 13:10:09 |
1843 |
|
1844 |
!------------------------------------------------ |
1845 |
|
1846 |
call write_histhf3d |
1847 |
|
1848 |
IF (ok_sync) THEN |
1849 |
call histsync(nid_hf) |
1850 |
ENDIF |
1851 |
|
1852 |
end subroutine write_histhf |
1853 |
|
1854 |
!*************************************************************** |
1855 |
|
1856 |
subroutine write_histins |
1857 |
|
1858 |
! From phylmd/write_histins.h, version 1.2 2005/05/25 13:10:09 |
1859 |
|
1860 |
real zout |
1861 |
integer itau_w ! pas de temps ecriture |
1862 |
|
1863 |
!-------------------------------------------------- |
1864 |
|
1865 |
IF (ok_instan) THEN |
1866 |
! Champs 2D: |
1867 |
|
1868 |
zsto = dtphys * ecrit_ins |
1869 |
zout = dtphys * ecrit_ins |
1870 |
itau_w = itau_phy + itap |
1871 |
|
1872 |
i = NINT(zout/zsto) |
1873 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), pphis, zx_tmp_2d) |
1874 |
CALL histwrite(nid_ins, "phis", itau_w, zx_tmp_2d) |
1875 |
|
1876 |
i = NINT(zout/zsto) |
1877 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), airephy, zx_tmp_2d) |
1878 |
CALL histwrite(nid_ins, "aire", itau_w, zx_tmp_2d) |
1879 |
|
1880 |
DO i = 1, klon |
1881 |
zx_tmp_fi2d(i) = paprs(i, 1) |
1882 |
ENDDO |
1883 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
1884 |
CALL histwrite(nid_ins, "psol", itau_w, zx_tmp_2d) |
1885 |
|
1886 |
DO i = 1, klon |
1887 |
zx_tmp_fi2d(i) = rain_fall(i) + snow_fall(i) |
1888 |
ENDDO |
1889 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
1890 |
CALL histwrite(nid_ins, "precip", itau_w, zx_tmp_2d) |
1891 |
|
1892 |
DO i = 1, klon |
1893 |
zx_tmp_fi2d(i) = rain_lsc(i) + snow_lsc(i) |
1894 |
ENDDO |
1895 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
1896 |
CALL histwrite(nid_ins, "plul", itau_w, zx_tmp_2d) |
1897 |
|
1898 |
DO i = 1, klon |
1899 |
zx_tmp_fi2d(i) = rain_con(i) + snow_con(i) |
1900 |
ENDDO |
1901 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
1902 |
CALL histwrite(nid_ins, "pluc", itau_w, zx_tmp_2d) |
1903 |
|
1904 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zxtsol, zx_tmp_2d) |
1905 |
CALL histwrite(nid_ins, "tsol", itau_w, zx_tmp_2d) |
1906 |
!ccIM |
1907 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zt2m, zx_tmp_2d) |
1908 |
CALL histwrite(nid_ins, "t2m", itau_w, zx_tmp_2d) |
1909 |
|
1910 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zq2m, zx_tmp_2d) |
1911 |
CALL histwrite(nid_ins, "q2m", itau_w, zx_tmp_2d) |
1912 |
|
1913 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zu10m, zx_tmp_2d) |
1914 |
CALL histwrite(nid_ins, "u10m", itau_w, zx_tmp_2d) |
1915 |
|
1916 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zv10m, zx_tmp_2d) |
1917 |
CALL histwrite(nid_ins, "v10m", itau_w, zx_tmp_2d) |
1918 |
|
1919 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), snow_fall, zx_tmp_2d) |
1920 |
CALL histwrite(nid_ins, "snow", itau_w, zx_tmp_2d) |
1921 |
|
1922 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), cdragm, zx_tmp_2d) |
1923 |
CALL histwrite(nid_ins, "cdrm", itau_w, zx_tmp_2d) |
1924 |
|
1925 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), cdragh, zx_tmp_2d) |
1926 |
CALL histwrite(nid_ins, "cdrh", itau_w, zx_tmp_2d) |
1927 |
|
1928 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), toplw, zx_tmp_2d) |
1929 |
CALL histwrite(nid_ins, "topl", itau_w, zx_tmp_2d) |
1930 |
|
1931 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), evap, zx_tmp_2d) |
1932 |
CALL histwrite(nid_ins, "evap", itau_w, zx_tmp_2d) |
1933 |
|
1934 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), solsw, zx_tmp_2d) |
1935 |
CALL histwrite(nid_ins, "sols", itau_w, zx_tmp_2d) |
1936 |
|
1937 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), sollw, zx_tmp_2d) |
1938 |
CALL histwrite(nid_ins, "soll", itau_w, zx_tmp_2d) |
1939 |
|
1940 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), sollwdown, zx_tmp_2d) |
1941 |
CALL histwrite(nid_ins, "solldown", itau_w, zx_tmp_2d) |
1942 |
|
1943 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), bils, zx_tmp_2d) |
1944 |
CALL histwrite(nid_ins, "bils", itau_w, zx_tmp_2d) |
1945 |
|
1946 |
zx_tmp_fi2d(1:klon)=-1*sens(1:klon) |
1947 |
! CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), sens, zx_tmp_2d) |
1948 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
1949 |
CALL histwrite(nid_ins, "sens", itau_w, zx_tmp_2d) |
1950 |
|
1951 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), fder, zx_tmp_2d) |
1952 |
CALL histwrite(nid_ins, "fder", itau_w, zx_tmp_2d) |
1953 |
|
1954 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), d_ts(1, is_oce), zx_tmp_2d) |
1955 |
CALL histwrite(nid_ins, "dtsvdfo", itau_w, zx_tmp_2d) |
1956 |
|
1957 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), d_ts(1, is_ter), zx_tmp_2d) |
1958 |
CALL histwrite(nid_ins, "dtsvdft", itau_w, zx_tmp_2d) |
1959 |
|
1960 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), d_ts(1, is_lic), zx_tmp_2d) |
1961 |
CALL histwrite(nid_ins, "dtsvdfg", itau_w, zx_tmp_2d) |
1962 |
|
1963 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), d_ts(1, is_sic), zx_tmp_2d) |
1964 |
CALL histwrite(nid_ins, "dtsvdfi", itau_w, zx_tmp_2d) |
1965 |
|
1966 |
DO nsrf = 1, nbsrf |
1967 |
!XXX |
1968 |
zx_tmp_fi2d(1 : klon) = pctsrf(1 : klon, nsrf)*100. |
1969 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
1970 |
CALL histwrite(nid_ins, "pourc_"//clnsurf(nsrf), itau_w, & |
1971 |
zx_tmp_2d) |
1972 |
|
1973 |
zx_tmp_fi2d(1 : klon) = pctsrf(1 : klon, nsrf) |
1974 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
1975 |
CALL histwrite(nid_ins, "fract_"//clnsurf(nsrf), itau_w, & |
1976 |
zx_tmp_2d) |
1977 |
|
1978 |
zx_tmp_fi2d(1 : klon) = fluxt(1 : klon, 1, nsrf) |
1979 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
1980 |
CALL histwrite(nid_ins, "sens_"//clnsurf(nsrf), itau_w, & |
1981 |
zx_tmp_2d) |
1982 |
|
1983 |
zx_tmp_fi2d(1 : klon) = fluxlat(1 : klon, nsrf) |
1984 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
1985 |
CALL histwrite(nid_ins, "lat_"//clnsurf(nsrf), itau_w, & |
1986 |
zx_tmp_2d) |
1987 |
|
1988 |
zx_tmp_fi2d(1 : klon) = ftsol(1 : klon, nsrf) |
1989 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
1990 |
CALL histwrite(nid_ins, "tsol_"//clnsurf(nsrf), itau_w, & |
1991 |
zx_tmp_2d) |
1992 |
|
1993 |
zx_tmp_fi2d(1 : klon) = fluxu(1 : klon, 1, nsrf) |
1994 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
1995 |
CALL histwrite(nid_ins, "taux_"//clnsurf(nsrf), itau_w, & |
1996 |
zx_tmp_2d) |
1997 |
|
1998 |
zx_tmp_fi2d(1 : klon) = fluxv(1 : klon, 1, nsrf) |
1999 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
2000 |
CALL histwrite(nid_ins, "tauy_"//clnsurf(nsrf), itau_w, & |
2001 |
zx_tmp_2d) |
2002 |
|
2003 |
zx_tmp_fi2d(1 : klon) = frugs(1 : klon, nsrf) |
2004 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
2005 |
CALL histwrite(nid_ins, "rugs_"//clnsurf(nsrf), itau_w, & |
2006 |
zx_tmp_2d) |
2007 |
|
2008 |
zx_tmp_fi2d(1 : klon) = falbe(1 : klon, nsrf) |
2009 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zx_tmp_fi2d, zx_tmp_2d) |
2010 |
CALL histwrite(nid_ins, "albe_"//clnsurf(nsrf), itau_w, & |
2011 |
zx_tmp_2d) |
2012 |
|
2013 |
END DO |
2014 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), albsol, zx_tmp_2d) |
2015 |
CALL histwrite(nid_ins, "albs", itau_w, zx_tmp_2d) |
2016 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), albsollw, zx_tmp_2d) |
2017 |
CALL histwrite(nid_ins, "albslw", itau_w, zx_tmp_2d) |
2018 |
|
2019 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), zxrugs, zx_tmp_2d) |
2020 |
CALL histwrite(nid_ins, "rugs", itau_w, zx_tmp_2d) |
2021 |
|
2022 |
!IM cf. AM 081204 BEG |
2023 |
|
2024 |
!HBTM2 |
2025 |
|
2026 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), s_pblh, zx_tmp_2d) |
2027 |
CALL histwrite(nid_ins, "s_pblh", itau_w, zx_tmp_2d) |
2028 |
|
2029 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), s_pblt, zx_tmp_2d) |
2030 |
CALL histwrite(nid_ins, "s_pblt", itau_w, zx_tmp_2d) |
2031 |
|
2032 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), s_lcl, zx_tmp_2d) |
2033 |
CALL histwrite(nid_ins, "s_lcl", itau_w, zx_tmp_2d) |
2034 |
|
2035 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), s_capCL, zx_tmp_2d) |
2036 |
CALL histwrite(nid_ins, "s_capCL", itau_w, zx_tmp_2d) |
2037 |
|
2038 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), s_oliqCL, zx_tmp_2d) |
2039 |
CALL histwrite(nid_ins, "s_oliqCL", itau_w, zx_tmp_2d) |
2040 |
|
2041 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), s_cteiCL, zx_tmp_2d) |
2042 |
CALL histwrite(nid_ins, "s_cteiCL", itau_w, zx_tmp_2d) |
2043 |
|
2044 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), s_therm, zx_tmp_2d) |
2045 |
CALL histwrite(nid_ins, "s_therm", itau_w, zx_tmp_2d) |
2046 |
|
2047 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), s_trmb1, zx_tmp_2d) |
2048 |
CALL histwrite(nid_ins, "s_trmb1", itau_w, zx_tmp_2d) |
2049 |
|
2050 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), s_trmb2, zx_tmp_2d) |
2051 |
CALL histwrite(nid_ins, "s_trmb2", itau_w, zx_tmp_2d) |
2052 |
|
2053 |
CALL gr_fi_ecrit(1, klon, iim, (jjm + 1), s_trmb3, zx_tmp_2d) |
2054 |
CALL histwrite(nid_ins, "s_trmb3", itau_w, zx_tmp_2d) |
2055 |
|
2056 |
!IM cf. AM 081204 END |
2057 |
|
2058 |
! Champs 3D: |
2059 |
|
2060 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), t_seri, zx_tmp_3d) |
2061 |
CALL histwrite(nid_ins, "temp", itau_w, zx_tmp_3d) |
2062 |
|
2063 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), u_seri, zx_tmp_3d) |
2064 |
CALL histwrite(nid_ins, "vitu", itau_w, zx_tmp_3d) |
2065 |
|
2066 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), v_seri, zx_tmp_3d) |
2067 |
CALL histwrite(nid_ins, "vitv", itau_w, zx_tmp_3d) |
2068 |
|
2069 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), zphi, zx_tmp_3d) |
2070 |
CALL histwrite(nid_ins, "geop", itau_w, zx_tmp_3d) |
2071 |
|
2072 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), play, zx_tmp_3d) |
2073 |
CALL histwrite(nid_ins, "pres", itau_w, zx_tmp_3d) |
2074 |
|
2075 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), d_t_vdf, zx_tmp_3d) |
2076 |
CALL histwrite(nid_ins, "dtvdf", itau_w, zx_tmp_3d) |
2077 |
|
2078 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), d_q_vdf, zx_tmp_3d) |
2079 |
CALL histwrite(nid_ins, "dqvdf", itau_w, zx_tmp_3d) |
2080 |
|
2081 |
if (ok_sync) then |
2082 |
call histsync(nid_ins) |
2083 |
endif |
2084 |
ENDIF |
2085 |
|
2086 |
end subroutine write_histins |
2087 |
|
2088 |
!**************************************************** |
2089 |
|
2090 |
subroutine write_histhf3d |
2091 |
|
2092 |
! From phylmd/write_histhf3d.h, version 1.2 2005/05/25 13:10:09 |
2093 |
|
2094 |
integer itau_w ! pas de temps ecriture |
2095 |
|
2096 |
!------------------------------------------------------- |
2097 |
|
2098 |
itau_w = itau_phy + itap |
2099 |
|
2100 |
! Champs 3D: |
2101 |
|
2102 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), t_seri, zx_tmp_3d) |
2103 |
CALL histwrite(nid_hf3d, "temp", itau_w, zx_tmp_3d) |
2104 |
|
2105 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), qx(1, 1, ivap), zx_tmp_3d) |
2106 |
CALL histwrite(nid_hf3d, "ovap", itau_w, zx_tmp_3d) |
2107 |
|
2108 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), u_seri, zx_tmp_3d) |
2109 |
CALL histwrite(nid_hf3d, "vitu", itau_w, zx_tmp_3d) |
2110 |
|
2111 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), v_seri, zx_tmp_3d) |
2112 |
CALL histwrite(nid_hf3d, "vitv", itau_w, zx_tmp_3d) |
2113 |
|
2114 |
if (nbtr >= 3) then |
2115 |
CALL gr_fi_ecrit(llm, klon, iim, (jjm + 1), tr_seri(1, 1, 3), & |
2116 |
zx_tmp_3d) |
2117 |
CALL histwrite(nid_hf3d, "O3", itau_w, zx_tmp_3d) |
2118 |
end if |
2119 |
|
2120 |
if (ok_sync) then |
2121 |
call histsync(nid_hf3d) |
2122 |
endif |
2123 |
|
2124 |
end subroutine write_histhf3d |
2125 |
|
2126 |
END SUBROUTINE physiq |
2127 |
|
2128 |
end module physiq_m |