1 |
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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|
7 |
SUBROUTINE physiq(lafin, dayvrai, time, paprs, play, pphi, pphis, u, v, t, & |
8 |
qx, omega, d_u, d_v, d_t, d_qx) |
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|
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! From phylmd/physiq.F, version 1.22 2006/02/20 09:38:28 |
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! (subversion revision 678) |
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|
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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 aaam_bud_m, only: aaam_bud |
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USE abort_gcm_m, ONLY: abort_gcm |
19 |
use ajsec_m, only: ajsec |
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use calltherm_m, only: calltherm |
21 |
USE clesphys, ONLY: cdhmax, cdmmax, ecrit_ins, ok_instan |
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USE clesphys2, ONLY: conv_emanuel, nbapp_rad, new_oliq, ok_orodr, ok_orolf |
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USE clmain_m, ONLY: clmain |
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use clouds_gno_m, only: clouds_gno |
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use comconst, only: dtphys |
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USE comgeomphy, ONLY: airephy |
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USE concvl_m, ONLY: concvl |
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USE conf_gcm_m, ONLY: lmt_pas |
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USE conf_phys_m, ONLY: conf_phys |
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use conflx_m, only: conflx |
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USE ctherm, ONLY: iflag_thermals, nsplit_thermals |
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use diagcld2_m, only: diagcld2 |
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USE dimens_m, ONLY: llm, nqmx |
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USE dimphy, ONLY: klon |
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USE dimsoil, ONLY: nsoilmx |
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use drag_noro_m, only: drag_noro |
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use dynetat0_m, only: day_ref, annee_ref |
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USE fcttre, ONLY: foeew |
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use fisrtilp_m, only: fisrtilp |
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USE hgardfou_m, ONLY: hgardfou |
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USE histsync_m, ONLY: histsync |
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USE histwrite_phy_m, ONLY: histwrite_phy |
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USE indicesol, ONLY: clnsurf, epsfra, is_lic, is_oce, is_sic, is_ter, & |
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nbsrf |
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USE ini_histins_m, ONLY: ini_histins, nid_ins |
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use lift_noro_m, only: lift_noro |
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use netcdf95, only: NF95_CLOSE |
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use newmicro_m, only: newmicro |
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use nr_util, only: assert |
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use nuage_m, only: nuage |
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USE orbite_m, ONLY: orbite |
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USE ozonecm_m, ONLY: ozonecm |
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USE phyetat0_m, ONLY: phyetat0 |
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USE phyredem_m, ONLY: phyredem |
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USE phyredem0_m, ONLY: phyredem0 |
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USE phytrac_m, ONLY: phytrac |
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use radlwsw_m, only: radlwsw |
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use yoegwd, only: sugwd |
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USE suphec_m, ONLY: rcpd, retv, rg, rlvtt, romega, rsigma, rtt, rmo3, md |
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use time_phylmdz, only: itap, increment_itap |
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use transp_m, only: transp |
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use transp_lay_m, only: transp_lay |
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use unit_nml_m, only: unit_nml |
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USE ymds2ju_m, ONLY: ymds2ju |
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USE yoethf_m, ONLY: r2es, rvtmp2 |
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use zenang_m, only: zenang |
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|
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logical, intent(in):: lafin ! dernier passage |
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|
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integer, intent(in):: dayvrai |
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! current day number, based at value 1 on January 1st of annee_ref |
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|
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REAL, intent(in):: time ! heure de la journ\'ee en fraction de jour |
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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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! pression pour le mileu de chaque couche (en Pa) |
80 |
|
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REAL, intent(in):: pphi(:, :) ! (klon, llm) |
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! géopotentiel de chaque couche (référence sol) |
83 |
|
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REAL, intent(in):: pphis(:) ! (klon) géopotentiel du sol |
85 |
|
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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 |
88 |
|
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REAL, intent(in):: v(:, :) ! (klon, llm) vitesse Y (de S a N) en m / s |
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REAL, intent(in):: t(:, :) ! (klon, llm) temperature (K) |
91 |
|
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REAL, intent(in):: qx(:, :, :) ! (klon, llm, nqmx) |
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! (humidit\'e sp\'ecifique et fractions massiques des autres traceurs) |
94 |
|
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REAL, intent(in):: omega(:, :) ! (klon, llm) vitesse verticale en Pa / s |
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REAL, intent(out):: d_u(:, :) ! (klon, llm) tendance physique de "u" (m s-2) |
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REAL, intent(out):: d_v(:, :) ! (klon, llm) tendance physique de "v" (m s-2) |
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REAL, intent(out):: d_t(:, :) ! (klon, llm) tendance physique de "t" (K / s) |
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|
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REAL, intent(out):: d_qx(:, :, :) ! (klon, llm, nqmx) |
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! tendance physique de "qx" (s-1) |
102 |
|
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! Local: |
104 |
|
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LOGICAL:: firstcal = .true. |
106 |
|
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LOGICAL, PARAMETER:: ok_stratus = .FALSE. |
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! Ajouter artificiellement les stratus |
109 |
|
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! pour phystoke avec thermiques |
111 |
REAL fm_therm(klon, llm + 1) |
112 |
REAL entr_therm(klon, llm) |
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real, save:: q2(klon, llm + 1, nbsrf) |
114 |
|
115 |
INTEGER, PARAMETER:: ivap = 1 ! indice de traceur pour vapeur d'eau |
116 |
INTEGER, PARAMETER:: iliq = 2 ! indice de traceur pour eau liquide |
117 |
|
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REAL, save:: t_ancien(klon, llm), q_ancien(klon, llm) |
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LOGICAL, save:: ancien_ok |
120 |
|
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REAL d_t_dyn(klon, llm) ! tendance dynamique pour "t" (K / s) |
122 |
REAL d_q_dyn(klon, llm) ! tendance dynamique pour "q" (kg / kg / s) |
123 |
|
124 |
real da(klon, llm), phi(klon, llm, llm), mp(klon, llm) |
125 |
|
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REAL, save:: swdn0(klon, llm + 1), swdn(klon, llm + 1) |
127 |
REAL, save:: swup0(klon, llm + 1), swup(klon, llm + 1) |
128 |
|
129 |
REAL, save:: lwdn0(klon, llm + 1), lwdn(klon, llm + 1) |
130 |
REAL, save:: lwup0(klon, llm + 1), lwup(klon, llm + 1) |
131 |
|
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! prw: precipitable water |
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real prw(klon) |
134 |
|
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! flwp, fiwp = Liquid Water Path & Ice Water Path (kg / m2) |
136 |
! flwc, fiwc = Liquid Water Content & Ice Water Content (kg / kg) |
137 |
REAL flwp(klon), fiwp(klon) |
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REAL flwc(klon, llm), fiwc(klon, llm) |
139 |
|
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! Variables propres a la physique |
141 |
|
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INTEGER, save:: radpas |
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! Radiative transfer computations are made every "radpas" call to |
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! "physiq". |
145 |
|
146 |
REAL, save:: radsol(klon) ! bilan radiatif au sol calcule par code radiatif |
147 |
REAL, save:: ftsol(klon, nbsrf) ! skin temperature of surface fraction |
148 |
|
149 |
REAL, save:: ftsoil(klon, nsoilmx, nbsrf) |
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! soil temperature of surface fraction |
151 |
|
152 |
REAL, save:: fevap(klon, nbsrf) ! evaporation |
153 |
REAL fluxlat(klon, nbsrf) |
154 |
|
155 |
REAL, save:: fqsurf(klon, nbsrf) |
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! humidite de l'air au contact de la surface |
157 |
|
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REAL, save:: qsol(klon) ! column-density of water in soil, in kg m-2 |
159 |
REAL, save:: fsnow(klon, nbsrf) ! \'epaisseur neigeuse |
160 |
REAL, save:: falbe(klon, nbsrf) ! albedo visible par type de surface |
161 |
|
162 |
! Param\`etres de l'orographie \`a l'\'echelle sous-maille (OESM) : |
163 |
REAL, save:: zmea(klon) ! orographie moyenne |
164 |
REAL, save:: zstd(klon) ! deviation standard de l'OESM |
165 |
REAL, save:: zsig(klon) ! pente de l'OESM |
166 |
REAL, save:: zgam(klon) ! anisotropie de l'OESM |
167 |
REAL, save:: zthe(klon) ! orientation de l'OESM |
168 |
REAL, save:: zpic(klon) ! Maximum de l'OESM |
169 |
REAL, save:: zval(klon) ! Minimum de l'OESM |
170 |
REAL, save:: rugoro(klon) ! longueur de rugosite de l'OESM |
171 |
REAL zulow(klon), zvlow(klon) |
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INTEGER ktest(klon) |
173 |
|
174 |
REAL, save:: agesno(klon, nbsrf) ! age de la neige |
175 |
REAL, save:: run_off_lic_0(klon) |
176 |
|
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! Variables li\'ees \`a la convection d'Emanuel : |
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REAL, save:: Ma(klon, llm) ! undilute upward mass flux |
179 |
REAL, save:: qcondc(klon, llm) ! in-cld water content from convect |
180 |
REAL, save:: sig1(klon, llm), w01(klon, llm) |
181 |
|
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! Variables pour la couche limite (Alain Lahellec) : |
183 |
REAL cdragh(klon) ! drag coefficient pour T and Q |
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REAL cdragm(klon) ! drag coefficient pour vent |
185 |
|
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REAL coefh(klon, 2:llm) ! coef d'echange pour phytrac |
187 |
|
188 |
REAL, save:: ffonte(klon, nbsrf) |
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! flux thermique utilise pour fondre la neige |
190 |
|
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REAL, save:: fqcalving(klon, nbsrf) |
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! flux d'eau "perdue" par la surface et necessaire pour limiter la |
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! hauteur de neige, en kg / m2 / s |
194 |
|
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REAL zxffonte(klon), zxfqcalving(klon) |
196 |
|
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REAL, save:: pfrac_impa(klon, llm)! Produits des coefs lessivage impaction |
198 |
REAL, save:: pfrac_nucl(klon, llm)! Produits des coefs lessivage nucleation |
199 |
|
200 |
REAL, save:: pfrac_1nucl(klon, llm) |
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! Produits des coefs lessi nucl (alpha = 1) |
202 |
|
203 |
REAL frac_impa(klon, llm) ! fraction d'a\'erosols lessiv\'es (impaction) |
204 |
REAL frac_nucl(klon, llm) ! idem (nucleation) |
205 |
|
206 |
REAL, save:: rain_fall(klon) |
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! liquid water mass flux (kg / m2 / s), positive down |
208 |
|
209 |
REAL, save:: snow_fall(klon) |
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! solid water mass flux (kg / m2 / s), positive down |
211 |
|
212 |
REAL rain_tiedtke(klon), snow_tiedtke(klon) |
213 |
|
214 |
REAL evap(klon) ! flux d'\'evaporation au sol |
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real devap(klon) ! derivative of the evaporation flux at the surface |
216 |
REAL sens(klon) ! flux de chaleur sensible au sol |
217 |
real dsens(klon) ! derivee du flux de chaleur sensible au sol |
218 |
REAL, save:: dlw(klon) ! derivative of infra-red flux |
219 |
REAL bils(klon) ! bilan de chaleur au sol |
220 |
REAL fder(klon) ! Derive de flux (sensible et latente) |
221 |
REAL ve(klon) ! integr. verticale du transport meri. de l'energie |
222 |
REAL vq(klon) ! integr. verticale du transport meri. de l'eau |
223 |
REAL ue(klon) ! integr. verticale du transport zonal de l'energie |
224 |
REAL uq(klon) ! integr. verticale du transport zonal de l'eau |
225 |
|
226 |
REAL, save:: frugs(klon, nbsrf) ! longueur de rugosite |
227 |
REAL zxrugs(klon) ! longueur de rugosite |
228 |
|
229 |
! Conditions aux limites |
230 |
|
231 |
INTEGER julien |
232 |
REAL, save:: pctsrf(klon, nbsrf) ! percentage of surface |
233 |
REAL, save:: albsol(klon) ! albedo du sol total, visible, moyen par maille |
234 |
REAL, SAVE:: wo(klon, llm) ! column density of ozone in a cell, in kDU |
235 |
real, parameter:: dobson_u = 2.1415e-05 ! Dobson unit, in kg m-2 |
236 |
|
237 |
real, save:: clwcon(klon, llm), rnebcon(klon, llm) |
238 |
real, save:: clwcon0(klon, llm), rnebcon0(klon, llm) |
239 |
|
240 |
REAL rhcl(klon, llm) ! humiditi relative ciel clair |
241 |
REAL dialiq(klon, llm) ! eau liquide nuageuse |
242 |
REAL diafra(klon, llm) ! fraction nuageuse |
243 |
REAL cldliq(klon, llm) ! eau liquide nuageuse |
244 |
REAL cldfra(klon, llm) ! fraction nuageuse |
245 |
REAL cldtau(klon, llm) ! epaisseur optique |
246 |
REAL cldemi(klon, llm) ! emissivite infrarouge |
247 |
|
248 |
REAL flux_q(klon, nbsrf) ! flux turbulent d'humidite à la surface |
249 |
REAL flux_t(klon, nbsrf) ! flux turbulent de chaleur à la surface |
250 |
|
251 |
REAL flux_u(klon, nbsrf), flux_v(klon, nbsrf) |
252 |
! tension du vent (flux turbulent de vent) à la surface, en Pa |
253 |
|
254 |
! Le rayonnement n'est pas calcul\'e tous les pas, il faut donc que |
255 |
! les variables soient r\'emanentes. |
256 |
REAL, save:: heat(klon, llm) ! chauffage solaire |
257 |
REAL, save:: heat0(klon, llm) ! chauffage solaire ciel clair |
258 |
REAL, save:: cool(klon, llm) ! refroidissement infrarouge |
259 |
REAL, save:: cool0(klon, llm) ! refroidissement infrarouge ciel clair |
260 |
REAL, save:: topsw(klon), toplw(klon), solsw(klon) |
261 |
REAL, save:: sollw(klon) ! rayonnement infrarouge montant \`a la surface |
262 |
real, save:: sollwdown(klon) ! downward LW flux at surface |
263 |
REAL, save:: topsw0(klon), toplw0(klon), solsw0(klon), sollw0(klon) |
264 |
REAL, save:: albpla(klon) |
265 |
REAL fsollw(klon, nbsrf) ! bilan flux IR pour chaque sous-surface |
266 |
REAL fsolsw(klon, nbsrf) ! flux solaire absorb\'e pour chaque sous-surface |
267 |
|
268 |
REAL conv_q(klon, llm) ! convergence de l'humidite (kg / kg / s) |
269 |
REAL conv_t(klon, llm) ! convergence of temperature (K / s) |
270 |
|
271 |
REAL cldl(klon), cldm(klon), cldh(klon) ! nuages bas, moyen et haut |
272 |
REAL cldt(klon), cldq(klon) ! nuage total, eau liquide integree |
273 |
|
274 |
REAL zxfluxlat(klon) |
275 |
REAL dist, mu0(klon), fract(klon) |
276 |
real longi |
277 |
REAL z_avant(klon), z_apres(klon), z_factor(klon) |
278 |
REAL zb |
279 |
REAL zx_t, zx_qs, zcor |
280 |
real zqsat(klon, llm) |
281 |
INTEGER i, k, iq, nsrf |
282 |
REAL zphi(klon, llm) |
283 |
|
284 |
! cf. Anne Mathieu, variables pour la couche limite atmosphérique (hbtm) |
285 |
|
286 |
REAL, SAVE:: pblh(klon, nbsrf) ! Hauteur de couche limite |
287 |
REAL, SAVE:: plcl(klon, nbsrf) ! Niveau de condensation de la CLA |
288 |
REAL, SAVE:: capCL(klon, nbsrf) ! CAPE de couche limite |
289 |
REAL, SAVE:: oliqCL(klon, nbsrf) ! eau_liqu integree de couche limite |
290 |
REAL, SAVE:: cteiCL(klon, nbsrf) ! cloud top instab. crit. couche limite |
291 |
REAL, SAVE:: pblt(klon, nbsrf) ! T \`a la hauteur de couche limite |
292 |
REAL, SAVE:: therm(klon, nbsrf) |
293 |
REAL, SAVE:: trmb1(klon, nbsrf) ! deep_cape |
294 |
REAL, SAVE:: trmb2(klon, nbsrf) ! inhibition |
295 |
REAL, SAVE:: trmb3(klon, nbsrf) ! Point Omega |
296 |
! Grandeurs de sorties |
297 |
REAL s_pblh(klon), s_lcl(klon), s_capCL(klon) |
298 |
REAL s_oliqCL(klon), s_cteiCL(klon), s_pblt(klon) |
299 |
REAL s_therm(klon), s_trmb1(klon), s_trmb2(klon) |
300 |
REAL s_trmb3(klon) |
301 |
|
302 |
! Variables pour la convection de K. Emanuel : |
303 |
|
304 |
REAL upwd(klon, llm) ! saturated updraft mass flux |
305 |
REAL dnwd(klon, llm) ! saturated downdraft mass flux |
306 |
REAL, save:: cape(klon) |
307 |
|
308 |
INTEGER iflagctrl(klon) ! flag fonctionnement de convect |
309 |
|
310 |
! Variables du changement |
311 |
|
312 |
! con: convection |
313 |
! lsc: large scale condensation |
314 |
! ajs: ajustement sec |
315 |
! eva: \'evaporation de l'eau liquide nuageuse |
316 |
! vdf: vertical diffusion in boundary layer |
317 |
REAL d_t_con(klon, llm), d_q_con(klon, llm) |
318 |
REAL, save:: d_u_con(klon, llm), d_v_con(klon, llm) |
319 |
REAL d_t_lsc(klon, llm), d_q_lsc(klon, llm), d_ql_lsc(klon, llm) |
320 |
REAL d_t_ajs(klon, llm), d_q_ajs(klon, llm) |
321 |
REAL d_u_ajs(klon, llm), d_v_ajs(klon, llm) |
322 |
REAL rneb(klon, llm) |
323 |
|
324 |
REAL mfu(klon, llm), mfd(klon, llm) |
325 |
REAL pen_u(klon, llm), pen_d(klon, llm) |
326 |
REAL pde_u(klon, llm), pde_d(klon, llm) |
327 |
INTEGER kcbot(klon), kctop(klon), kdtop(klon) |
328 |
REAL pmflxr(klon, llm + 1), pmflxs(klon, llm + 1) |
329 |
REAL prfl(klon, llm + 1), psfl(klon, llm + 1) |
330 |
|
331 |
INTEGER, save:: ibas_con(klon), itop_con(klon) |
332 |
real ema_pct(klon) ! Emanuel pressure at cloud top, in Pa |
333 |
|
334 |
REAL, save:: rain_con(klon) |
335 |
real rain_lsc(klon) |
336 |
REAL, save:: snow_con(klon) ! neige (mm / s) |
337 |
real snow_lsc(klon) |
338 |
REAL d_ts(klon, nbsrf) ! variation of ftsol |
339 |
|
340 |
REAL d_u_vdf(klon, llm), d_v_vdf(klon, llm) |
341 |
REAL d_t_vdf(klon, llm), d_q_vdf(klon, llm) |
342 |
|
343 |
REAL d_u_oro(klon, llm), d_v_oro(klon, llm) |
344 |
REAL d_t_oro(klon, llm) |
345 |
REAL d_u_lif(klon, llm), d_v_lif(klon, llm) |
346 |
REAL d_t_lif(klon, llm) |
347 |
|
348 |
REAL, save:: ratqs(klon, llm) |
349 |
real ratqss(klon, llm), ratqsc(klon, llm) |
350 |
real:: ratqsbas = 0.01, ratqshaut = 0.3 |
351 |
|
352 |
! Parametres lies au nouveau schema de nuages (SB, PDF) |
353 |
real:: fact_cldcon = 0.375 |
354 |
real:: facttemps = 1.e-4 |
355 |
logical:: ok_newmicro = .true. |
356 |
real facteur |
357 |
|
358 |
integer:: iflag_cldcon = 1 |
359 |
logical ptconv(klon, llm) |
360 |
|
361 |
! Variables pour effectuer les appels en s\'erie : |
362 |
|
363 |
REAL t_seri(klon, llm), q_seri(klon, llm) |
364 |
REAL ql_seri(klon, llm) |
365 |
REAL u_seri(klon, llm), v_seri(klon, llm) |
366 |
REAL tr_seri(klon, llm, nqmx - 2) |
367 |
|
368 |
REAL zx_rh(klon, llm) |
369 |
|
370 |
REAL zustrdr(klon), zvstrdr(klon) |
371 |
REAL zustrli(klon), zvstrli(klon) |
372 |
REAL aam, torsfc |
373 |
|
374 |
REAL ve_lay(klon, llm) ! transport meri. de l'energie a chaque niveau vert. |
375 |
REAL vq_lay(klon, llm) ! transport meri. de l'eau a chaque niveau vert. |
376 |
REAL ue_lay(klon, llm) ! transport zonal de l'energie a chaque niveau vert. |
377 |
REAL uq_lay(klon, llm) ! transport zonal de l'eau a chaque niveau vert. |
378 |
|
379 |
real date0 |
380 |
REAL tsol(klon) |
381 |
|
382 |
REAL d_t_ec(klon, llm) |
383 |
! tendance due \`a la conversion d'\'energie cin\'etique en |
384 |
! énergie thermique |
385 |
|
386 |
REAL, save:: t2m(klon, nbsrf), q2m(klon, nbsrf) |
387 |
! temperature and humidity at 2 m |
388 |
|
389 |
REAL, save:: u10m_srf(klon, nbsrf), v10m_srf(klon, nbsrf) |
390 |
! composantes du vent \`a 10 m |
391 |
|
392 |
REAL zt2m(klon), zq2m(klon) ! température, humidité 2 m moyenne sur 1 maille |
393 |
REAL u10m(klon), v10m(klon) ! vent \`a 10 m moyenn\' sur les sous-surfaces |
394 |
|
395 |
! Aerosol effects: |
396 |
|
397 |
REAL, save:: topswad(klon), solswad(klon) ! aerosol direct effect |
398 |
LOGICAL:: ok_ade = .false. ! apply aerosol direct effect |
399 |
|
400 |
REAL:: bl95_b0 = 2., bl95_b1 = 0.2 |
401 |
! Parameters in equation (D) of Boucher and Lohmann (1995, Tellus |
402 |
! B). They link cloud droplet number concentration to aerosol mass |
403 |
! concentration. |
404 |
|
405 |
real zmasse(klon, llm) |
406 |
! (column-density of mass of air in a cell, in kg m-2) |
407 |
|
408 |
integer, save:: ncid_startphy |
409 |
|
410 |
namelist /physiq_nml/ fact_cldcon, facttemps, ok_newmicro, iflag_cldcon, & |
411 |
ratqsbas, ratqshaut, ok_ade, bl95_b0, bl95_b1, iflag_thermals, & |
412 |
nsplit_thermals |
413 |
|
414 |
!---------------------------------------------------------------- |
415 |
|
416 |
IF (nqmx < 2) CALL abort_gcm('physiq', & |
417 |
'eaux vapeur et liquide sont indispensables') |
418 |
|
419 |
test_firstcal: IF (firstcal) THEN |
420 |
! initialiser |
421 |
u10m_srf = 0. |
422 |
v10m_srf = 0. |
423 |
t2m = 0. |
424 |
q2m = 0. |
425 |
ffonte = 0. |
426 |
fqcalving = 0. |
427 |
rain_con = 0. |
428 |
snow_con = 0. |
429 |
d_u_con = 0. |
430 |
d_v_con = 0. |
431 |
rnebcon0 = 0. |
432 |
clwcon0 = 0. |
433 |
rnebcon = 0. |
434 |
clwcon = 0. |
435 |
pblh =0. ! Hauteur de couche limite |
436 |
plcl =0. ! Niveau de condensation de la CLA |
437 |
capCL =0. ! CAPE de couche limite |
438 |
oliqCL =0. ! eau_liqu integree de couche limite |
439 |
cteiCL =0. ! cloud top instab. crit. couche limite |
440 |
pblt =0. |
441 |
therm =0. |
442 |
trmb1 =0. ! deep_cape |
443 |
trmb2 =0. ! inhibition |
444 |
trmb3 =0. ! Point Omega |
445 |
|
446 |
iflag_thermals = 0 |
447 |
nsplit_thermals = 1 |
448 |
print *, "Enter namelist 'physiq_nml'." |
449 |
read(unit=*, nml=physiq_nml) |
450 |
write(unit_nml, nml=physiq_nml) |
451 |
|
452 |
call conf_phys |
453 |
|
454 |
! Initialiser les compteurs: |
455 |
|
456 |
frugs = 0. |
457 |
CALL phyetat0(pctsrf, ftsol, ftsoil, fqsurf, qsol, fsnow, falbe, & |
458 |
fevap, rain_fall, snow_fall, solsw, sollw, dlw, radsol, frugs, & |
459 |
agesno, zmea, zstd, zsig, zgam, zthe, zpic, zval, t_ancien, & |
460 |
q_ancien, ancien_ok, rnebcon, ratqs, clwcon, run_off_lic_0, sig1, & |
461 |
w01, ncid_startphy) |
462 |
|
463 |
! ATTENTION : il faudra a terme relire q2 dans l'etat initial |
464 |
q2 = 1e-8 |
465 |
|
466 |
radpas = lmt_pas / nbapp_rad |
467 |
print *, "radpas = ", radpas |
468 |
|
469 |
! Initialisation pour le sch\'ema de convection d'Emanuel : |
470 |
IF (conv_emanuel) THEN |
471 |
ibas_con = 1 |
472 |
itop_con = 1 |
473 |
ENDIF |
474 |
|
475 |
IF (ok_orodr) THEN |
476 |
rugoro = MAX(1e-5, zstd * zsig / 2) |
477 |
CALL SUGWD(paprs, play) |
478 |
else |
479 |
rugoro = 0. |
480 |
ENDIF |
481 |
|
482 |
ecrit_ins = NINT(ecrit_ins / dtphys) |
483 |
|
484 |
! Initialisation des sorties |
485 |
|
486 |
call ini_histins(dtphys, ok_newmicro) |
487 |
CALL ymds2ju(annee_ref, 1, day_ref, 0., date0) |
488 |
! Positionner date0 pour initialisation de ORCHIDEE |
489 |
print *, 'physiq date0: ', date0 |
490 |
CALL phyredem0 |
491 |
ENDIF test_firstcal |
492 |
|
493 |
! We will modify variables *_seri and we will not touch variables |
494 |
! u, v, t, qx: |
495 |
t_seri = t |
496 |
u_seri = u |
497 |
v_seri = v |
498 |
q_seri = qx(:, :, ivap) |
499 |
ql_seri = qx(:, :, iliq) |
500 |
tr_seri = qx(:, :, 3:nqmx) |
501 |
|
502 |
tsol = sum(ftsol * pctsrf, dim = 2) |
503 |
|
504 |
! Diagnostic de la tendance dynamique : |
505 |
IF (ancien_ok) THEN |
506 |
DO k = 1, llm |
507 |
DO i = 1, klon |
508 |
d_t_dyn(i, k) = (t_seri(i, k) - t_ancien(i, k)) / dtphys |
509 |
d_q_dyn(i, k) = (q_seri(i, k) - q_ancien(i, k)) / dtphys |
510 |
ENDDO |
511 |
ENDDO |
512 |
ELSE |
513 |
DO k = 1, llm |
514 |
DO i = 1, klon |
515 |
d_t_dyn(i, k) = 0. |
516 |
d_q_dyn(i, k) = 0. |
517 |
ENDDO |
518 |
ENDDO |
519 |
ancien_ok = .TRUE. |
520 |
ENDIF |
521 |
|
522 |
! Ajouter le geopotentiel du sol: |
523 |
DO k = 1, llm |
524 |
DO i = 1, klon |
525 |
zphi(i, k) = pphi(i, k) + pphis(i) |
526 |
ENDDO |
527 |
ENDDO |
528 |
|
529 |
! Check temperatures: |
530 |
CALL hgardfou(t_seri, ftsol) |
531 |
|
532 |
call increment_itap |
533 |
julien = MOD(dayvrai, 360) |
534 |
if (julien == 0) julien = 360 |
535 |
|
536 |
forall (k = 1: llm) zmasse(:, k) = (paprs(:, k) - paprs(:, k + 1)) / rg |
537 |
|
538 |
! \'Evaporation de l'eau liquide nuageuse : |
539 |
DO k = 1, llm |
540 |
DO i = 1, klon |
541 |
zb = MAX(0., ql_seri(i, k)) |
542 |
t_seri(i, k) = t_seri(i, k) & |
543 |
- zb * RLVTT / RCPD / (1. + RVTMP2 * q_seri(i, k)) |
544 |
q_seri(i, k) = q_seri(i, k) + zb |
545 |
ENDDO |
546 |
ENDDO |
547 |
ql_seri = 0. |
548 |
|
549 |
frugs = MAX(frugs, 0.000015) |
550 |
zxrugs = sum(frugs * pctsrf, dim = 2) |
551 |
|
552 |
! Calculs n\'ecessaires au calcul de l'albedo dans l'interface avec |
553 |
! la surface. |
554 |
|
555 |
CALL orbite(REAL(julien), longi, dist) |
556 |
CALL zenang(longi, time, dtphys * radpas, mu0, fract) |
557 |
albsol = sum(falbe * pctsrf, dim = 2) |
558 |
|
559 |
! R\'epartition sous maille des flux longwave et shortwave |
560 |
! R\'epartition du longwave par sous-surface lin\'earis\'ee |
561 |
|
562 |
forall (nsrf = 1: nbsrf) |
563 |
fsollw(:, nsrf) = sollw + 4. * RSIGMA * tsol**3 & |
564 |
* (tsol - ftsol(:, nsrf)) |
565 |
fsolsw(:, nsrf) = solsw * (1. - falbe(:, nsrf)) / (1. - albsol) |
566 |
END forall |
567 |
|
568 |
CALL clmain(dtphys, pctsrf, t_seri, q_seri, u_seri, v_seri, julien, mu0, & |
569 |
ftsol, cdmmax, cdhmax, ftsoil, qsol, paprs, play, fsnow, fqsurf, & |
570 |
fevap, falbe, fluxlat, rain_fall, snow_fall, fsolsw, fsollw, frugs, & |
571 |
agesno, rugoro, d_t_vdf, d_q_vdf, d_u_vdf, d_v_vdf, d_ts, flux_t, & |
572 |
flux_q, flux_u, flux_v, cdragh, cdragm, q2, dsens, devap, coefh, t2m, & |
573 |
q2m, u10m_srf, v10m_srf, pblh, capCL, oliqCL, cteiCL, pblT, therm, & |
574 |
trmb1, trmb2, trmb3, plcl, fqcalving, ffonte, run_off_lic_0) |
575 |
|
576 |
! Incr\'ementation des flux |
577 |
|
578 |
sens = - sum(flux_t * pctsrf, dim = 2) |
579 |
evap = - sum(flux_q * pctsrf, dim = 2) |
580 |
fder = dlw + dsens + devap |
581 |
|
582 |
DO k = 1, llm |
583 |
DO i = 1, klon |
584 |
t_seri(i, k) = t_seri(i, k) + d_t_vdf(i, k) |
585 |
q_seri(i, k) = q_seri(i, k) + d_q_vdf(i, k) |
586 |
u_seri(i, k) = u_seri(i, k) + d_u_vdf(i, k) |
587 |
v_seri(i, k) = v_seri(i, k) + d_v_vdf(i, k) |
588 |
ENDDO |
589 |
ENDDO |
590 |
|
591 |
! Update surface temperature: |
592 |
|
593 |
call assert(abs(sum(pctsrf, dim = 2) - 1.) <= EPSFRA, 'physiq: pctsrf') |
594 |
ftsol = ftsol + d_ts |
595 |
tsol = sum(ftsol * pctsrf, dim = 2) |
596 |
zxfluxlat = sum(fluxlat * pctsrf, dim = 2) |
597 |
zt2m = sum(t2m * pctsrf, dim = 2) |
598 |
zq2m = sum(q2m * pctsrf, dim = 2) |
599 |
u10m = sum(u10m_srf * pctsrf, dim = 2) |
600 |
v10m = sum(v10m_srf * pctsrf, dim = 2) |
601 |
zxffonte = sum(ffonte * pctsrf, dim = 2) |
602 |
zxfqcalving = sum(fqcalving * pctsrf, dim = 2) |
603 |
s_pblh = sum(pblh * pctsrf, dim = 2) |
604 |
s_lcl = sum(plcl * pctsrf, dim = 2) |
605 |
s_capCL = sum(capCL * pctsrf, dim = 2) |
606 |
s_oliqCL = sum(oliqCL * pctsrf, dim = 2) |
607 |
s_cteiCL = sum(cteiCL * pctsrf, dim = 2) |
608 |
s_pblT = sum(pblT * pctsrf, dim = 2) |
609 |
s_therm = sum(therm * pctsrf, dim = 2) |
610 |
s_trmb1 = sum(trmb1 * pctsrf, dim = 2) |
611 |
s_trmb2 = sum(trmb2 * pctsrf, dim = 2) |
612 |
s_trmb3 = sum(trmb3 * pctsrf, dim = 2) |
613 |
|
614 |
! Si une sous-fraction n'existe pas, elle prend la valeur moyenne : |
615 |
DO nsrf = 1, nbsrf |
616 |
DO i = 1, klon |
617 |
IF (pctsrf(i, nsrf) < epsfra) then |
618 |
ftsol(i, nsrf) = tsol(i) |
619 |
t2m(i, nsrf) = zt2m(i) |
620 |
q2m(i, nsrf) = zq2m(i) |
621 |
u10m_srf(i, nsrf) = u10m(i) |
622 |
v10m_srf(i, nsrf) = v10m(i) |
623 |
ffonte(i, nsrf) = zxffonte(i) |
624 |
fqcalving(i, nsrf) = zxfqcalving(i) |
625 |
pblh(i, nsrf) = s_pblh(i) |
626 |
plcl(i, nsrf) = s_lcl(i) |
627 |
capCL(i, nsrf) = s_capCL(i) |
628 |
oliqCL(i, nsrf) = s_oliqCL(i) |
629 |
cteiCL(i, nsrf) = s_cteiCL(i) |
630 |
pblT(i, nsrf) = s_pblT(i) |
631 |
therm(i, nsrf) = s_therm(i) |
632 |
trmb1(i, nsrf) = s_trmb1(i) |
633 |
trmb2(i, nsrf) = s_trmb2(i) |
634 |
trmb3(i, nsrf) = s_trmb3(i) |
635 |
end IF |
636 |
ENDDO |
637 |
ENDDO |
638 |
|
639 |
dlw = - 4. * RSIGMA * tsol**3 |
640 |
|
641 |
! Appeler la convection |
642 |
|
643 |
if (conv_emanuel) then |
644 |
CALL concvl(paprs, play, t_seri, q_seri, u_seri, v_seri, sig1, w01, & |
645 |
d_t_con, d_q_con, d_u_con, d_v_con, rain_con, ibas_con, itop_con, & |
646 |
upwd, dnwd, Ma, cape, iflagctrl, qcondc, pmflxr, da, phi, mp) |
647 |
snow_con = 0. |
648 |
clwcon0 = qcondc |
649 |
mfu = upwd + dnwd |
650 |
|
651 |
zqsat = MIN(0.5, r2es * FOEEW(t_seri, rtt >= t_seri) / play) |
652 |
zqsat = zqsat / (1. - retv * zqsat) |
653 |
|
654 |
! Properties of convective clouds |
655 |
clwcon0 = fact_cldcon * clwcon0 |
656 |
call clouds_gno(klon, llm, q_seri, zqsat, clwcon0, ptconv, ratqsc, & |
657 |
rnebcon0) |
658 |
|
659 |
forall (i = 1:klon) ema_pct(i) = paprs(i, itop_con(i) + 1) |
660 |
mfd = 0. |
661 |
pen_u = 0. |
662 |
pen_d = 0. |
663 |
pde_d = 0. |
664 |
pde_u = 0. |
665 |
else |
666 |
conv_q = d_q_dyn + d_q_vdf / dtphys |
667 |
conv_t = d_t_dyn + d_t_vdf / dtphys |
668 |
z_avant = sum((q_seri + ql_seri) * zmasse, dim=2) |
669 |
CALL conflx(dtphys, paprs, play, t_seri(:, llm:1:- 1), & |
670 |
q_seri(:, llm:1:- 1), conv_t, conv_q, - evap, omega, & |
671 |
d_t_con, d_q_con, rain_con, snow_con, mfu(:, llm:1:- 1), & |
672 |
mfd(:, llm:1:- 1), pen_u, pde_u, pen_d, pde_d, kcbot, kctop, & |
673 |
kdtop, pmflxr, pmflxs) |
674 |
WHERE (rain_con < 0.) rain_con = 0. |
675 |
WHERE (snow_con < 0.) snow_con = 0. |
676 |
ibas_con = llm + 1 - kcbot |
677 |
itop_con = llm + 1 - kctop |
678 |
END if |
679 |
|
680 |
DO k = 1, llm |
681 |
DO i = 1, klon |
682 |
t_seri(i, k) = t_seri(i, k) + d_t_con(i, k) |
683 |
q_seri(i, k) = q_seri(i, k) + d_q_con(i, k) |
684 |
u_seri(i, k) = u_seri(i, k) + d_u_con(i, k) |
685 |
v_seri(i, k) = v_seri(i, k) + d_v_con(i, k) |
686 |
ENDDO |
687 |
ENDDO |
688 |
|
689 |
IF (.not. conv_emanuel) THEN |
690 |
z_apres = sum((q_seri + ql_seri) * zmasse, dim=2) |
691 |
z_factor = (z_avant - (rain_con + snow_con) * dtphys) / z_apres |
692 |
DO k = 1, llm |
693 |
DO i = 1, klon |
694 |
IF (z_factor(i) > 1. + 1E-8 .OR. z_factor(i) < 1. - 1E-8) THEN |
695 |
q_seri(i, k) = q_seri(i, k) * z_factor(i) |
696 |
ENDIF |
697 |
ENDDO |
698 |
ENDDO |
699 |
ENDIF |
700 |
|
701 |
! Convection s\`eche (thermiques ou ajustement) |
702 |
|
703 |
d_t_ajs = 0. |
704 |
d_u_ajs = 0. |
705 |
d_v_ajs = 0. |
706 |
d_q_ajs = 0. |
707 |
fm_therm = 0. |
708 |
entr_therm = 0. |
709 |
|
710 |
if (iflag_thermals == 0) then |
711 |
! Ajustement sec |
712 |
CALL ajsec(paprs, play, t_seri, q_seri, d_t_ajs, d_q_ajs) |
713 |
t_seri = t_seri + d_t_ajs |
714 |
q_seri = q_seri + d_q_ajs |
715 |
else |
716 |
call calltherm(dtphys, play, paprs, pphi, u_seri, v_seri, t_seri, & |
717 |
q_seri, d_u_ajs, d_v_ajs, d_t_ajs, d_q_ajs, fm_therm, entr_therm) |
718 |
endif |
719 |
|
720 |
! Caclul des ratqs |
721 |
|
722 |
! ratqs convectifs \`a l'ancienne en fonction de (q(z = 0) - q) / q |
723 |
! on \'ecrase le tableau ratqsc calcul\'e par clouds_gno |
724 |
if (iflag_cldcon == 1) then |
725 |
do k = 1, llm |
726 |
do i = 1, klon |
727 |
if(ptconv(i, k)) then |
728 |
ratqsc(i, k) = ratqsbas + fact_cldcon & |
729 |
* (q_seri(i, 1) - q_seri(i, k)) / q_seri(i, k) |
730 |
else |
731 |
ratqsc(i, k) = 0. |
732 |
endif |
733 |
enddo |
734 |
enddo |
735 |
endif |
736 |
|
737 |
! ratqs stables |
738 |
do k = 1, llm |
739 |
do i = 1, klon |
740 |
ratqss(i, k) = ratqsbas + (ratqshaut - ratqsbas) & |
741 |
* min((paprs(i, 1) - play(i, k)) / (paprs(i, 1) - 3e4), 1.) |
742 |
enddo |
743 |
enddo |
744 |
|
745 |
! ratqs final |
746 |
if (iflag_cldcon == 1 .or. iflag_cldcon == 2) then |
747 |
! les ratqs sont une conbinaison de ratqss et ratqsc |
748 |
! ratqs final |
749 |
! 1e4 (en gros 3 heures), en dur pour le moment, est le temps de |
750 |
! relaxation des ratqs |
751 |
ratqs = max(ratqs * exp(- dtphys * facttemps), ratqss) |
752 |
ratqs = max(ratqs, ratqsc) |
753 |
else |
754 |
! on ne prend que le ratqs stable pour fisrtilp |
755 |
ratqs = ratqss |
756 |
endif |
757 |
|
758 |
CALL fisrtilp(dtphys, paprs, play, t_seri, q_seri, ptconv, ratqs, & |
759 |
d_t_lsc, d_q_lsc, d_ql_lsc, rneb, cldliq, rain_lsc, snow_lsc, & |
760 |
pfrac_impa, pfrac_nucl, pfrac_1nucl, frac_impa, frac_nucl, prfl, & |
761 |
psfl, rhcl) |
762 |
|
763 |
WHERE (rain_lsc < 0) rain_lsc = 0. |
764 |
WHERE (snow_lsc < 0) snow_lsc = 0. |
765 |
DO k = 1, llm |
766 |
DO i = 1, klon |
767 |
t_seri(i, k) = t_seri(i, k) + d_t_lsc(i, k) |
768 |
q_seri(i, k) = q_seri(i, k) + d_q_lsc(i, k) |
769 |
ql_seri(i, k) = ql_seri(i, k) + d_ql_lsc(i, k) |
770 |
cldfra(i, k) = rneb(i, k) |
771 |
IF (.NOT.new_oliq) cldliq(i, k) = ql_seri(i, k) |
772 |
ENDDO |
773 |
ENDDO |
774 |
|
775 |
! PRESCRIPTION DES NUAGES POUR LE RAYONNEMENT |
776 |
|
777 |
! 1. NUAGES CONVECTIFS |
778 |
|
779 |
IF (iflag_cldcon <= - 1) THEN |
780 |
! seulement pour Tiedtke |
781 |
snow_tiedtke = 0. |
782 |
if (iflag_cldcon == - 1) then |
783 |
rain_tiedtke = rain_con |
784 |
else |
785 |
rain_tiedtke = 0. |
786 |
do k = 1, llm |
787 |
do i = 1, klon |
788 |
if (d_q_con(i, k) < 0.) then |
789 |
rain_tiedtke(i) = rain_tiedtke(i) - d_q_con(i, k) / dtphys & |
790 |
* zmasse(i, k) |
791 |
endif |
792 |
enddo |
793 |
enddo |
794 |
endif |
795 |
|
796 |
! Nuages diagnostiques pour Tiedtke |
797 |
CALL diagcld1(paprs, play, rain_tiedtke, snow_tiedtke, ibas_con, & |
798 |
itop_con, diafra, dialiq) |
799 |
DO k = 1, llm |
800 |
DO i = 1, klon |
801 |
IF (diafra(i, k) > cldfra(i, k)) THEN |
802 |
cldliq(i, k) = dialiq(i, k) |
803 |
cldfra(i, k) = diafra(i, k) |
804 |
ENDIF |
805 |
ENDDO |
806 |
ENDDO |
807 |
ELSE IF (iflag_cldcon == 3) THEN |
808 |
! On prend pour les nuages convectifs le maximum du calcul de |
809 |
! la convection et du calcul du pas de temps pr\'ec\'edent diminu\'e |
810 |
! d'un facteur facttemps. |
811 |
facteur = dtphys * facttemps |
812 |
do k = 1, llm |
813 |
do i = 1, klon |
814 |
rnebcon(i, k) = rnebcon(i, k) * facteur |
815 |
if (rnebcon0(i, k) * clwcon0(i, k) & |
816 |
> rnebcon(i, k) * clwcon(i, k)) then |
817 |
rnebcon(i, k) = rnebcon0(i, k) |
818 |
clwcon(i, k) = clwcon0(i, k) |
819 |
endif |
820 |
enddo |
821 |
enddo |
822 |
|
823 |
! On prend la somme des fractions nuageuses et des contenus en eau |
824 |
cldfra = min(max(cldfra, rnebcon), 1.) |
825 |
cldliq = cldliq + rnebcon * clwcon |
826 |
ENDIF |
827 |
|
828 |
! 2. Nuages stratiformes |
829 |
|
830 |
IF (ok_stratus) THEN |
831 |
CALL diagcld2(paprs, play, t_seri, q_seri, diafra, dialiq) |
832 |
DO k = 1, llm |
833 |
DO i = 1, klon |
834 |
IF (diafra(i, k) > cldfra(i, k)) THEN |
835 |
cldliq(i, k) = dialiq(i, k) |
836 |
cldfra(i, k) = diafra(i, k) |
837 |
ENDIF |
838 |
ENDDO |
839 |
ENDDO |
840 |
ENDIF |
841 |
|
842 |
! Precipitation totale |
843 |
DO i = 1, klon |
844 |
rain_fall(i) = rain_con(i) + rain_lsc(i) |
845 |
snow_fall(i) = snow_con(i) + snow_lsc(i) |
846 |
ENDDO |
847 |
|
848 |
! Humidit\'e relative pour diagnostic : |
849 |
DO k = 1, llm |
850 |
DO i = 1, klon |
851 |
zx_t = t_seri(i, k) |
852 |
zx_qs = r2es * FOEEW(zx_t, rtt >= zx_t) / play(i, k) |
853 |
zx_qs = MIN(0.5, zx_qs) |
854 |
zcor = 1. / (1. - retv * zx_qs) |
855 |
zx_qs = zx_qs * zcor |
856 |
zx_rh(i, k) = q_seri(i, k) / zx_qs |
857 |
zqsat(i, k) = zx_qs |
858 |
ENDDO |
859 |
ENDDO |
860 |
|
861 |
! Param\`etres optiques des nuages et quelques param\`etres pour |
862 |
! diagnostics : |
863 |
if (ok_newmicro) then |
864 |
CALL newmicro(paprs, play, t_seri, cldliq, cldfra, cldtau, cldemi, & |
865 |
cldh, cldl, cldm, cldt, cldq, flwp, fiwp, flwc, fiwc) |
866 |
else |
867 |
CALL nuage(paprs, play, t_seri, cldliq, cldfra, cldtau, cldemi, cldh, & |
868 |
cldl, cldm, cldt, cldq) |
869 |
endif |
870 |
|
871 |
IF (MOD(itap - 1, radpas) == 0) THEN |
872 |
wo = ozonecm(REAL(julien), paprs) |
873 |
albsol = sum(falbe * pctsrf, dim = 2) |
874 |
CALL radlwsw(dist, mu0, fract, paprs, play, tsol, albsol, t_seri, & |
875 |
q_seri, wo, cldfra, cldemi, cldtau, heat, heat0, cool, cool0, & |
876 |
radsol, albpla, topsw, toplw, solsw, sollw, sollwdown, topsw0, & |
877 |
toplw0, solsw0, sollw0, lwdn0, lwdn, lwup0, lwup, swdn0, swdn, & |
878 |
swup0, swup, ok_ade, topswad, solswad) |
879 |
ENDIF |
880 |
|
881 |
! Ajouter la tendance des rayonnements (tous les pas) |
882 |
DO k = 1, llm |
883 |
DO i = 1, klon |
884 |
t_seri(i, k) = t_seri(i, k) + (heat(i, k) - cool(i, k)) * dtphys & |
885 |
/ 86400. |
886 |
ENDDO |
887 |
ENDDO |
888 |
|
889 |
! Calculer le bilan du sol et la d\'erive de temp\'erature (couplage) |
890 |
DO i = 1, klon |
891 |
bils(i) = radsol(i) - sens(i) + zxfluxlat(i) |
892 |
ENDDO |
893 |
|
894 |
! Param\'etrisation de l'orographie \`a l'\'echelle sous-maille : |
895 |
|
896 |
IF (ok_orodr) THEN |
897 |
! S\'election des points pour lesquels le sch\'ema est actif : |
898 |
DO i = 1, klon |
899 |
ktest(i) = 0 |
900 |
IF (zpic(i) - zmea(i) > 100. .AND. zstd(i) > 10.) THEN |
901 |
ktest(i) = 1 |
902 |
ENDIF |
903 |
ENDDO |
904 |
|
905 |
CALL drag_noro(dtphys, paprs, play, zmea, zstd, zsig, zgam, zthe, & |
906 |
zpic, zval, ktest, t_seri, u_seri, v_seri, zulow, zvlow, zustrdr, & |
907 |
zvstrdr, d_t_oro, d_u_oro, d_v_oro) |
908 |
|
909 |
! ajout des tendances |
910 |
DO k = 1, llm |
911 |
DO i = 1, klon |
912 |
t_seri(i, k) = t_seri(i, k) + d_t_oro(i, k) |
913 |
u_seri(i, k) = u_seri(i, k) + d_u_oro(i, k) |
914 |
v_seri(i, k) = v_seri(i, k) + d_v_oro(i, k) |
915 |
ENDDO |
916 |
ENDDO |
917 |
ENDIF |
918 |
|
919 |
IF (ok_orolf) THEN |
920 |
! S\'election des points pour lesquels le sch\'ema est actif : |
921 |
DO i = 1, klon |
922 |
ktest(i) = 0 |
923 |
IF (zpic(i) - zmea(i) > 100.) THEN |
924 |
ktest(i) = 1 |
925 |
ENDIF |
926 |
ENDDO |
927 |
|
928 |
CALL lift_noro(dtphys, paprs, play, zmea, zstd, zpic, ktest, t_seri, & |
929 |
u_seri, v_seri, zulow, zvlow, zustrli, zvstrli, d_t_lif, & |
930 |
d_u_lif, d_v_lif) |
931 |
|
932 |
! Ajout des tendances : |
933 |
DO k = 1, llm |
934 |
DO i = 1, klon |
935 |
t_seri(i, k) = t_seri(i, k) + d_t_lif(i, k) |
936 |
u_seri(i, k) = u_seri(i, k) + d_u_lif(i, k) |
937 |
v_seri(i, k) = v_seri(i, k) + d_v_lif(i, k) |
938 |
ENDDO |
939 |
ENDDO |
940 |
ENDIF |
941 |
|
942 |
CALL aaam_bud(rg, romega, pphis, zustrdr, zustrli, & |
943 |
sum((u_seri - u) / dtphys * zmasse, dim = 2), zvstrdr, & |
944 |
zvstrli, sum((v_seri - v) / dtphys * zmasse, dim = 2), paprs, u, v, & |
945 |
aam, torsfc) |
946 |
|
947 |
! Calcul des tendances traceurs |
948 |
call phytrac(julien, time, firstcal, lafin, dtphys, t, paprs, play, mfu, & |
949 |
mfd, pde_u, pen_d, coefh, cdragh, fm_therm, entr_therm, u(:, 1), & |
950 |
v(:, 1), ftsol, pctsrf, frac_impa, frac_nucl, da, phi, mp, upwd, & |
951 |
dnwd, tr_seri, zmasse, ncid_startphy) |
952 |
|
953 |
! Calculer le transport de l'eau et de l'energie (diagnostique) |
954 |
CALL transp(paprs, t_seri, q_seri, u_seri, v_seri, zphi, ve, vq, ue, uq) |
955 |
|
956 |
! diag. bilKP |
957 |
|
958 |
CALL transp_lay(paprs, t_seri, q_seri, u_seri, v_seri, zphi, & |
959 |
ve_lay, vq_lay, ue_lay, uq_lay) |
960 |
|
961 |
! Accumuler les variables a stocker dans les fichiers histoire: |
962 |
|
963 |
! conversion Ec en énergie thermique |
964 |
DO k = 1, llm |
965 |
DO i = 1, klon |
966 |
d_t_ec(i, k) = 0.5 / (RCPD * (1. + RVTMP2 * q_seri(i, k))) & |
967 |
* (u(i, k)**2 + v(i, k)**2 - u_seri(i, k)**2 - v_seri(i, k)**2) |
968 |
t_seri(i, k) = t_seri(i, k) + d_t_ec(i, k) |
969 |
d_t_ec(i, k) = d_t_ec(i, k) / dtphys |
970 |
END DO |
971 |
END DO |
972 |
|
973 |
! SORTIES |
974 |
|
975 |
! prw = eau precipitable |
976 |
DO i = 1, klon |
977 |
prw(i) = 0. |
978 |
DO k = 1, llm |
979 |
prw(i) = prw(i) + q_seri(i, k) * zmasse(i, k) |
980 |
ENDDO |
981 |
ENDDO |
982 |
|
983 |
! Convertir les incrementations en tendances |
984 |
|
985 |
DO k = 1, llm |
986 |
DO i = 1, klon |
987 |
d_u(i, k) = (u_seri(i, k) - u(i, k)) / dtphys |
988 |
d_v(i, k) = (v_seri(i, k) - v(i, k)) / dtphys |
989 |
d_t(i, k) = (t_seri(i, k) - t(i, k)) / dtphys |
990 |
d_qx(i, k, ivap) = (q_seri(i, k) - qx(i, k, ivap)) / dtphys |
991 |
d_qx(i, k, iliq) = (ql_seri(i, k) - qx(i, k, iliq)) / dtphys |
992 |
ENDDO |
993 |
ENDDO |
994 |
|
995 |
DO iq = 3, nqmx |
996 |
DO k = 1, llm |
997 |
DO i = 1, klon |
998 |
d_qx(i, k, iq) = (tr_seri(i, k, iq - 2) - qx(i, k, iq)) / dtphys |
999 |
ENDDO |
1000 |
ENDDO |
1001 |
ENDDO |
1002 |
|
1003 |
! Sauvegarder les valeurs de t et q a la fin de la physique: |
1004 |
DO k = 1, llm |
1005 |
DO i = 1, klon |
1006 |
t_ancien(i, k) = t_seri(i, k) |
1007 |
q_ancien(i, k) = q_seri(i, k) |
1008 |
ENDDO |
1009 |
ENDDO |
1010 |
|
1011 |
CALL histwrite_phy("phis", pphis) |
1012 |
CALL histwrite_phy("aire", airephy) |
1013 |
CALL histwrite_phy("psol", paprs(:, 1)) |
1014 |
CALL histwrite_phy("precip", rain_fall + snow_fall) |
1015 |
CALL histwrite_phy("plul", rain_lsc + snow_lsc) |
1016 |
CALL histwrite_phy("pluc", rain_con + snow_con) |
1017 |
CALL histwrite_phy("tsol", tsol) |
1018 |
CALL histwrite_phy("t2m", zt2m) |
1019 |
CALL histwrite_phy("q2m", zq2m) |
1020 |
CALL histwrite_phy("u10m", u10m) |
1021 |
CALL histwrite_phy("v10m", v10m) |
1022 |
CALL histwrite_phy("snow", snow_fall) |
1023 |
CALL histwrite_phy("cdrm", cdragm) |
1024 |
CALL histwrite_phy("cdrh", cdragh) |
1025 |
CALL histwrite_phy("topl", toplw) |
1026 |
CALL histwrite_phy("evap", evap) |
1027 |
CALL histwrite_phy("sols", solsw) |
1028 |
CALL histwrite_phy("soll", sollw) |
1029 |
CALL histwrite_phy("solldown", sollwdown) |
1030 |
CALL histwrite_phy("bils", bils) |
1031 |
CALL histwrite_phy("sens", - sens) |
1032 |
CALL histwrite_phy("fder", fder) |
1033 |
CALL histwrite_phy("dtsvdfo", d_ts(:, is_oce)) |
1034 |
CALL histwrite_phy("dtsvdft", d_ts(:, is_ter)) |
1035 |
CALL histwrite_phy("dtsvdfg", d_ts(:, is_lic)) |
1036 |
CALL histwrite_phy("dtsvdfi", d_ts(:, is_sic)) |
1037 |
|
1038 |
DO nsrf = 1, nbsrf |
1039 |
CALL histwrite_phy("pourc_"//clnsurf(nsrf), pctsrf(:, nsrf) * 100.) |
1040 |
CALL histwrite_phy("fract_"//clnsurf(nsrf), pctsrf(:, nsrf)) |
1041 |
CALL histwrite_phy("sens_"//clnsurf(nsrf), flux_t(:, nsrf)) |
1042 |
CALL histwrite_phy("lat_"//clnsurf(nsrf), fluxlat(:, nsrf)) |
1043 |
CALL histwrite_phy("tsol_"//clnsurf(nsrf), ftsol(:, nsrf)) |
1044 |
CALL histwrite_phy("taux_"//clnsurf(nsrf), flux_u(:, nsrf)) |
1045 |
CALL histwrite_phy("tauy_"//clnsurf(nsrf), flux_v(:, nsrf)) |
1046 |
CALL histwrite_phy("rugs_"//clnsurf(nsrf), frugs(:, nsrf)) |
1047 |
CALL histwrite_phy("albe_"//clnsurf(nsrf), falbe(:, nsrf)) |
1048 |
CALL histwrite_phy("u10m_"//clnsurf(nsrf), u10m_srf(:, nsrf)) |
1049 |
CALL histwrite_phy("v10m_"//clnsurf(nsrf), v10m_srf(:, nsrf)) |
1050 |
END DO |
1051 |
|
1052 |
CALL histwrite_phy("albs", albsol) |
1053 |
CALL histwrite_phy("tro3", wo * dobson_u * 1e3 / zmasse / rmo3 * md) |
1054 |
CALL histwrite_phy("rugs", zxrugs) |
1055 |
CALL histwrite_phy("s_pblh", s_pblh) |
1056 |
CALL histwrite_phy("s_pblt", s_pblt) |
1057 |
CALL histwrite_phy("s_lcl", s_lcl) |
1058 |
CALL histwrite_phy("s_capCL", s_capCL) |
1059 |
CALL histwrite_phy("s_oliqCL", s_oliqCL) |
1060 |
CALL histwrite_phy("s_cteiCL", s_cteiCL) |
1061 |
CALL histwrite_phy("s_therm", s_therm) |
1062 |
CALL histwrite_phy("s_trmb1", s_trmb1) |
1063 |
CALL histwrite_phy("s_trmb2", s_trmb2) |
1064 |
CALL histwrite_phy("s_trmb3", s_trmb3) |
1065 |
|
1066 |
if (conv_emanuel) then |
1067 |
CALL histwrite_phy("ptop", ema_pct) |
1068 |
CALL histwrite_phy("dnwd0", - mp) |
1069 |
end if |
1070 |
|
1071 |
CALL histwrite_phy("temp", t_seri) |
1072 |
CALL histwrite_phy("vitu", u_seri) |
1073 |
CALL histwrite_phy("vitv", v_seri) |
1074 |
CALL histwrite_phy("geop", zphi) |
1075 |
CALL histwrite_phy("pres", play) |
1076 |
CALL histwrite_phy("dtvdf", d_t_vdf) |
1077 |
CALL histwrite_phy("dqvdf", d_q_vdf) |
1078 |
CALL histwrite_phy("rhum", zx_rh) |
1079 |
CALL histwrite_phy("d_t_ec", d_t_ec) |
1080 |
CALL histwrite_phy("dtsw0", heat0 / 86400.) |
1081 |
CALL histwrite_phy("dtlw0", - cool0 / 86400.) |
1082 |
CALL histwrite_phy("msnow", sum(fsnow * pctsrf, dim = 2)) |
1083 |
call histwrite_phy("qsurf", sum(fqsurf * pctsrf, dim = 2)) |
1084 |
|
1085 |
if (ok_instan) call histsync(nid_ins) |
1086 |
|
1087 |
IF (lafin) then |
1088 |
call NF95_CLOSE(ncid_startphy) |
1089 |
CALL phyredem(pctsrf, ftsol, ftsoil, fqsurf, qsol, & |
1090 |
fsnow, falbe, fevap, rain_fall, snow_fall, solsw, sollw, dlw, & |
1091 |
radsol, frugs, agesno, zmea, zstd, zsig, zgam, zthe, zpic, zval, & |
1092 |
t_ancien, q_ancien, rnebcon, ratqs, clwcon, run_off_lic_0, sig1, & |
1093 |
w01) |
1094 |
end IF |
1095 |
|
1096 |
firstcal = .FALSE. |
1097 |
|
1098 |
END SUBROUTINE physiq |
1099 |
|
1100 |
end module physiq_m |