1 |
module physiq_m |
2 |
|
3 |
IMPLICIT none |
4 |
|
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contains |
6 |
|
7 |
SUBROUTINE physiq(lafin, dayvrai, time, paprs, play, pphi, pphis, u, v, t, & |
8 |
qx, omega, d_u, d_v, d_t, d_qx) |
9 |
|
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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. |
16 |
|
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use aaam_bud_m, only: aaam_bud |
18 |
USE abort_gcm_m, ONLY: abort_gcm |
19 |
use ajsec_m, only: ajsec |
20 |
use calltherm_m, only: calltherm |
21 |
USE clesphys, ONLY: cdhmax, cdmmax, ecrit_ins, ksta, ksta_ter, ok_kzmin, & |
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ok_instan |
23 |
USE clesphys2, ONLY: cycle_diurne, conv_emanuel, nbapp_rad, new_oliq, & |
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ok_orodr, ok_orolf |
25 |
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: offline, day_step, iphysiq, 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, qsatl, qsats, thermcep |
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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 |
48 |
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, rlat, rlon |
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USE phyredem_m, ONLY: phyredem |
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USE phyredem0_m, ONLY: phyredem0 |
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USE phystokenc_m, ONLY: phystokenc |
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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 |
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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 |
79 |
|
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REAL, intent(in):: play(:, :) ! (klon, llm) |
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! pression pour le mileu de chaque couche (en Pa) |
82 |
|
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REAL, intent(in):: pphi(:, :) ! (klon, llm) |
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! géopotentiel de chaque couche (référence sol) |
85 |
|
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REAL, intent(in):: pphis(:) ! (klon) géopotentiel du sol |
87 |
|
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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 |
90 |
|
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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) |
93 |
|
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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) |
96 |
|
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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) |
101 |
|
102 |
REAL, intent(out):: d_qx(:, :, :) ! (klon, llm, nqmx) |
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! tendance physique de "qx" (s-1) |
104 |
|
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! Local: |
106 |
|
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LOGICAL:: firstcal = .true. |
108 |
|
109 |
LOGICAL, PARAMETER:: ok_stratus = .FALSE. |
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! Ajouter artificiellement les stratus |
111 |
|
112 |
! pour phystoke avec thermiques |
113 |
REAL fm_therm(klon, llm + 1) |
114 |
REAL entr_therm(klon, llm) |
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real, save:: q2(klon, llm + 1, nbsrf) |
116 |
|
117 |
INTEGER, PARAMETER:: ivap = 1 ! indice de traceur pour vapeur d'eau |
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INTEGER, PARAMETER:: iliq = 2 ! indice de traceur pour eau liquide |
119 |
|
120 |
REAL, save:: t_ancien(klon, llm), q_ancien(klon, llm) |
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LOGICAL, save:: ancien_ok |
122 |
|
123 |
REAL d_t_dyn(klon, llm) ! tendance dynamique pour "t" (K / s) |
124 |
REAL d_q_dyn(klon, llm) ! tendance dynamique pour "q" (kg / kg / s) |
125 |
|
126 |
real da(klon, llm), phi(klon, llm, llm), mp(klon, llm) |
127 |
|
128 |
REAL, save:: swdn0(klon, llm + 1), swdn(klon, llm + 1) |
129 |
REAL, save:: swup0(klon, llm + 1), swup(klon, llm + 1) |
130 |
|
131 |
REAL, save:: lwdn0(klon, llm + 1), lwdn(klon, llm + 1) |
132 |
REAL, save:: lwup0(klon, llm + 1), lwup(klon, llm + 1) |
133 |
|
134 |
! prw: precipitable water |
135 |
real prw(klon) |
136 |
|
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! flwp, fiwp = Liquid Water Path & Ice Water Path (kg / m2) |
138 |
! flwc, fiwc = Liquid Water Content & Ice Water Content (kg / kg) |
139 |
REAL flwp(klon), fiwp(klon) |
140 |
REAL flwc(klon, llm), fiwc(klon, llm) |
141 |
|
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! Variables propres a la physique |
143 |
|
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INTEGER, save:: radpas |
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! Radiative transfer computations are made every "radpas" call to |
146 |
! "physiq". |
147 |
|
148 |
REAL, save:: radsol(klon) ! bilan radiatif au sol calcule par code radiatif |
149 |
|
150 |
REAL, save:: ftsol(klon, nbsrf) ! skin temperature of surface fraction |
151 |
|
152 |
REAL, save:: ftsoil(klon, nsoilmx, nbsrf) |
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! soil temperature of surface fraction |
154 |
|
155 |
REAL, save:: fevap(klon, nbsrf) ! evaporation |
156 |
REAL, save:: fluxlat(klon, nbsrf) |
157 |
|
158 |
REAL, save:: fqsurf(klon, nbsrf) |
159 |
! humidite de l'air au contact de la surface |
160 |
|
161 |
REAL, save:: qsol(klon) |
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! column-density of water in soil, in kg m-2 |
163 |
|
164 |
REAL, save:: fsnow(klon, nbsrf) ! epaisseur neigeuse |
165 |
REAL, save:: falbe(klon, nbsrf) ! albedo visible par type de surface |
166 |
|
167 |
! Param\`etres de l'orographie \`a l'\'echelle sous-maille (OESM) : |
168 |
REAL, save:: zmea(klon) ! orographie moyenne |
169 |
REAL, save:: zstd(klon) ! deviation standard de l'OESM |
170 |
REAL, save:: zsig(klon) ! pente de l'OESM |
171 |
REAL, save:: zgam(klon) ! anisotropie de l'OESM |
172 |
REAL, save:: zthe(klon) ! orientation de l'OESM |
173 |
REAL, save:: zpic(klon) ! Maximum de l'OESM |
174 |
REAL, save:: zval(klon) ! Minimum de l'OESM |
175 |
REAL, save:: rugoro(klon) ! longueur de rugosite de l'OESM |
176 |
REAL zulow(klon), zvlow(klon) |
177 |
INTEGER igwd, itest(klon) |
178 |
|
179 |
REAL, save:: agesno(klon, nbsrf) ! age de la neige |
180 |
REAL, save:: run_off_lic_0(klon) |
181 |
|
182 |
! Variables li\'ees \`a la convection d'Emanuel : |
183 |
REAL, save:: Ma(klon, llm) ! undilute upward mass flux |
184 |
REAL, save:: qcondc(klon, llm) ! in-cld water content from convect |
185 |
REAL, save:: sig1(klon, llm), w01(klon, llm) |
186 |
|
187 |
! Variables pour la couche limite (Alain Lahellec) : |
188 |
REAL cdragh(klon) ! drag coefficient pour T and Q |
189 |
REAL cdragm(klon) ! drag coefficient pour vent |
190 |
|
191 |
! Pour phytrac : |
192 |
REAL ycoefh(klon, llm) ! coef d'echange pour phytrac |
193 |
REAL yu1(klon) ! vents dans la premiere couche U |
194 |
REAL yv1(klon) ! vents dans la premiere couche V |
195 |
|
196 |
REAL, save:: ffonte(klon, nbsrf) |
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! flux thermique utilise pour fondre la neige |
198 |
|
199 |
REAL, save:: fqcalving(klon, nbsrf) |
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! flux d'eau "perdue" par la surface et necessaire pour limiter la |
201 |
! hauteur de neige, en kg / m2 / s |
202 |
|
203 |
REAL zxffonte(klon), zxfqcalving(klon) |
204 |
|
205 |
REAL, save:: pfrac_impa(klon, llm)! Produits des coefs lessivage impaction |
206 |
REAL, save:: pfrac_nucl(klon, llm)! Produits des coefs lessivage nucleation |
207 |
|
208 |
REAL, save:: pfrac_1nucl(klon, llm) |
209 |
! Produits des coefs lessi nucl (alpha = 1) |
210 |
|
211 |
REAL frac_impa(klon, llm) ! fractions d'aerosols lessivees (impaction) |
212 |
REAL frac_nucl(klon, llm) ! idem (nucleation) |
213 |
|
214 |
REAL, save:: rain_fall(klon) |
215 |
! liquid water mass flux (kg / m2 / s), positive down |
216 |
|
217 |
REAL, save:: snow_fall(klon) |
218 |
! solid water mass flux (kg / m2 / s), positive down |
219 |
|
220 |
REAL rain_tiedtke(klon), snow_tiedtke(klon) |
221 |
|
222 |
REAL evap(klon), devap(klon) ! evaporation and its derivative |
223 |
REAL sens(klon), dsens(klon) ! chaleur sensible et sa derivee |
224 |
REAL, save:: dlw(klon) ! derivee infra rouge |
225 |
REAL bils(klon) ! bilan de chaleur au sol |
226 |
REAL, save:: fder(klon) ! Derive de flux (sensible et latente) |
227 |
REAL ve(klon) ! integr. verticale du transport meri. de l'energie |
228 |
REAL vq(klon) ! integr. verticale du transport meri. de l'eau |
229 |
REAL ue(klon) ! integr. verticale du transport zonal de l'energie |
230 |
REAL uq(klon) ! integr. verticale du transport zonal de l'eau |
231 |
|
232 |
REAL, save:: frugs(klon, nbsrf) ! longueur de rugosite |
233 |
REAL zxrugs(klon) ! longueur de rugosite |
234 |
|
235 |
! Conditions aux limites |
236 |
|
237 |
INTEGER julien |
238 |
REAL, save:: pctsrf(klon, nbsrf) ! percentage of surface |
239 |
REAL, save:: albsol(klon) ! albedo du sol total visible |
240 |
REAL, SAVE:: wo(klon, llm) ! column density of ozone in a cell, in kDU |
241 |
|
242 |
real, save:: clwcon(klon, llm), rnebcon(klon, llm) |
243 |
real, save:: clwcon0(klon, llm), rnebcon0(klon, llm) |
244 |
|
245 |
REAL rhcl(klon, llm) ! humiditi relative ciel clair |
246 |
REAL dialiq(klon, llm) ! eau liquide nuageuse |
247 |
REAL diafra(klon, llm) ! fraction nuageuse |
248 |
REAL cldliq(klon, llm) ! eau liquide nuageuse |
249 |
REAL cldfra(klon, llm) ! fraction nuageuse |
250 |
REAL cldtau(klon, llm) ! epaisseur optique |
251 |
REAL cldemi(klon, llm) ! emissivite infrarouge |
252 |
|
253 |
REAL fluxq(klon, llm, nbsrf) ! flux turbulent d'humidite |
254 |
REAL fluxt(klon, llm, nbsrf) ! flux turbulent de chaleur |
255 |
REAL fluxu(klon, llm, nbsrf) ! flux turbulent de vitesse u |
256 |
REAL fluxv(klon, llm, nbsrf) ! flux turbulent de vitesse v |
257 |
|
258 |
REAL zxfluxt(klon, llm) |
259 |
REAL zxfluxq(klon, llm) |
260 |
REAL zxfluxu(klon, llm) |
261 |
REAL zxfluxv(klon, llm) |
262 |
|
263 |
! Le rayonnement n'est pas calcul\'e tous les pas, il faut donc que |
264 |
! les variables soient r\'emanentes. |
265 |
REAL, save:: heat(klon, llm) ! chauffage solaire |
266 |
REAL, save:: heat0(klon, llm) ! chauffage solaire ciel clair |
267 |
REAL, save:: cool(klon, llm) ! refroidissement infrarouge |
268 |
REAL, save:: cool0(klon, llm) ! refroidissement infrarouge ciel clair |
269 |
REAL, save:: topsw(klon), toplw(klon), solsw(klon) |
270 |
REAL, save:: sollw(klon) ! rayonnement infrarouge montant \`a la surface |
271 |
real, save:: sollwdown(klon) ! downward LW flux at surface |
272 |
REAL, save:: topsw0(klon), toplw0(klon), solsw0(klon), sollw0(klon) |
273 |
REAL, save:: albpla(klon) |
274 |
REAL fsollw(klon, nbsrf) ! bilan flux IR pour chaque sous-surface |
275 |
REAL fsolsw(klon, nbsrf) ! flux solaire absorb\'e pour chaque sous-surface |
276 |
|
277 |
REAL conv_q(klon, llm) ! convergence de l'humidite (kg / kg / s) |
278 |
REAL conv_t(klon, llm) ! convergence of temperature (K / s) |
279 |
|
280 |
REAL cldl(klon), cldm(klon), cldh(klon) ! nuages bas, moyen et haut |
281 |
REAL cldt(klon), cldq(klon) ! nuage total, eau liquide integree |
282 |
|
283 |
REAL zxqsurf(klon), zxsnow(klon), zxfluxlat(klon) |
284 |
|
285 |
REAL dist, mu0(klon), fract(klon) |
286 |
real longi |
287 |
REAL z_avant(klon), z_apres(klon), z_factor(klon) |
288 |
REAL zb |
289 |
REAL zx_t, zx_qs, zcor |
290 |
real zqsat(klon, llm) |
291 |
INTEGER i, k, iq, nsrf |
292 |
REAL, PARAMETER:: t_coup = 234. |
293 |
REAL zphi(klon, llm) |
294 |
|
295 |
! cf. Anne Mathieu, variables pour la couche limite atmosphérique (hbtm) |
296 |
|
297 |
REAL, SAVE:: pblh(klon, nbsrf) ! Hauteur de couche limite |
298 |
REAL, SAVE:: plcl(klon, nbsrf) ! Niveau de condensation de la CLA |
299 |
REAL, SAVE:: capCL(klon, nbsrf) ! CAPE de couche limite |
300 |
REAL, SAVE:: oliqCL(klon, nbsrf) ! eau_liqu integree de couche limite |
301 |
REAL, SAVE:: cteiCL(klon, nbsrf) ! cloud top instab. crit. couche limite |
302 |
REAL, SAVE:: pblt(klon, nbsrf) ! T a la Hauteur de couche limite |
303 |
REAL, SAVE:: therm(klon, nbsrf) |
304 |
REAL, SAVE:: trmb1(klon, nbsrf) ! deep_cape |
305 |
REAL, SAVE:: trmb2(klon, nbsrf) ! inhibition |
306 |
REAL, SAVE:: trmb3(klon, nbsrf) ! Point Omega |
307 |
! Grandeurs de sorties |
308 |
REAL s_pblh(klon), s_lcl(klon), s_capCL(klon) |
309 |
REAL s_oliqCL(klon), s_cteiCL(klon), s_pblt(klon) |
310 |
REAL s_therm(klon), s_trmb1(klon), s_trmb2(klon) |
311 |
REAL s_trmb3(klon) |
312 |
|
313 |
! Variables pour la convection de K. Emanuel : |
314 |
|
315 |
REAL upwd(klon, llm) ! saturated updraft mass flux |
316 |
REAL dnwd(klon, llm) ! saturated downdraft mass flux |
317 |
REAL dnwd0(klon, llm) ! unsaturated downdraft mass flux |
318 |
REAL, save:: cape(klon) |
319 |
|
320 |
INTEGER iflagctrl(klon) ! flag fonctionnement de convect |
321 |
|
322 |
! Variables du changement |
323 |
|
324 |
! con: convection |
325 |
! lsc: large scale condensation |
326 |
! ajs: ajustement sec |
327 |
! eva: \'evaporation de l'eau liquide nuageuse |
328 |
! vdf: vertical diffusion in boundary layer |
329 |
REAL d_t_con(klon, llm), d_q_con(klon, llm) |
330 |
REAL, save:: d_u_con(klon, llm), d_v_con(klon, llm) |
331 |
REAL d_t_lsc(klon, llm), d_q_lsc(klon, llm), d_ql_lsc(klon, llm) |
332 |
REAL d_t_ajs(klon, llm), d_q_ajs(klon, llm) |
333 |
REAL d_u_ajs(klon, llm), d_v_ajs(klon, llm) |
334 |
REAL rneb(klon, llm) |
335 |
|
336 |
REAL mfu(klon, llm), mfd(klon, llm) |
337 |
REAL pen_u(klon, llm), pen_d(klon, llm) |
338 |
REAL pde_u(klon, llm), pde_d(klon, llm) |
339 |
INTEGER kcbot(klon), kctop(klon), kdtop(klon) |
340 |
REAL pmflxr(klon, llm + 1), pmflxs(klon, llm + 1) |
341 |
REAL prfl(klon, llm + 1), psfl(klon, llm + 1) |
342 |
|
343 |
INTEGER, save:: ibas_con(klon), itop_con(klon) |
344 |
real ema_pct(klon) ! Emanuel pressure at cloud top, in Pa |
345 |
|
346 |
REAL, save:: rain_con(klon) |
347 |
real rain_lsc(klon) |
348 |
REAL, save:: snow_con(klon) ! neige (mm / s) |
349 |
real snow_lsc(klon) |
350 |
REAL d_ts(klon, nbsrf) |
351 |
|
352 |
REAL d_u_vdf(klon, llm), d_v_vdf(klon, llm) |
353 |
REAL d_t_vdf(klon, llm), d_q_vdf(klon, llm) |
354 |
|
355 |
REAL d_u_oro(klon, llm), d_v_oro(klon, llm) |
356 |
REAL d_t_oro(klon, llm) |
357 |
REAL d_u_lif(klon, llm), d_v_lif(klon, llm) |
358 |
REAL d_t_lif(klon, llm) |
359 |
|
360 |
REAL, save:: ratqs(klon, llm) |
361 |
real ratqss(klon, llm), ratqsc(klon, llm) |
362 |
real:: ratqsbas = 0.01, ratqshaut = 0.3 |
363 |
|
364 |
! Parametres lies au nouveau schema de nuages (SB, PDF) |
365 |
real:: fact_cldcon = 0.375 |
366 |
real:: facttemps = 1.e-4 |
367 |
logical:: ok_newmicro = .true. |
368 |
real facteur |
369 |
|
370 |
integer:: iflag_cldcon = 1 |
371 |
logical ptconv(klon, llm) |
372 |
|
373 |
! Variables pour effectuer les appels en s\'erie : |
374 |
|
375 |
REAL t_seri(klon, llm), q_seri(klon, llm) |
376 |
REAL ql_seri(klon, llm) |
377 |
REAL u_seri(klon, llm), v_seri(klon, llm) |
378 |
REAL tr_seri(klon, llm, nqmx - 2) |
379 |
|
380 |
REAL zx_rh(klon, llm) |
381 |
|
382 |
REAL zustrdr(klon), zvstrdr(klon) |
383 |
REAL zustrli(klon), zvstrli(klon) |
384 |
REAL zustrph(klon), zvstrph(klon) |
385 |
REAL aam, torsfc |
386 |
|
387 |
REAL ve_lay(klon, llm) ! transport meri. de l'energie a chaque niveau vert. |
388 |
REAL vq_lay(klon, llm) ! transport meri. de l'eau a chaque niveau vert. |
389 |
REAL ue_lay(klon, llm) ! transport zonal de l'energie a chaque niveau vert. |
390 |
REAL uq_lay(klon, llm) ! transport zonal de l'eau a chaque niveau vert. |
391 |
|
392 |
real date0 |
393 |
REAL ztsol(klon) |
394 |
|
395 |
REAL d_t_ec(klon, llm) |
396 |
! tendance due \`a la conversion Ec en énergie thermique |
397 |
|
398 |
REAL ZRCPD |
399 |
|
400 |
REAL, save:: t2m(klon, nbsrf), q2m(klon, nbsrf) |
401 |
! temperature and humidity at 2 m |
402 |
|
403 |
REAL, save:: u10m(klon, nbsrf), v10m(klon, nbsrf) ! vents a 10 m |
404 |
REAL zt2m(klon), zq2m(klon) ! temp., hum. 2 m moyenne s/ 1 maille |
405 |
REAL zu10m(klon), zv10m(klon) ! vents a 10 m moyennes s/1 maille |
406 |
|
407 |
! Aerosol effects: |
408 |
|
409 |
REAL sulfate(klon, llm) ! SO4 aerosol concentration (micro g / m3) |
410 |
|
411 |
REAL, save:: sulfate_pi(klon, llm) |
412 |
! SO4 aerosol concentration, in \mu g / m3, pre-industrial value |
413 |
|
414 |
REAL cldtaupi(klon, llm) |
415 |
! cloud optical thickness for pre-industrial aerosols |
416 |
|
417 |
REAL re(klon, llm) ! Cloud droplet effective radius |
418 |
REAL fl(klon, llm) ! denominator of re |
419 |
|
420 |
! Aerosol optical properties |
421 |
REAL, save:: tau_ae(klon, llm, 2), piz_ae(klon, llm, 2) |
422 |
REAL, save:: cg_ae(klon, llm, 2) |
423 |
|
424 |
REAL, save:: topswad(klon), solswad(klon) ! aerosol direct effect |
425 |
REAL, save:: topswai(klon), solswai(klon) ! aerosol indirect effect |
426 |
|
427 |
LOGICAL:: ok_ade = .false. ! apply aerosol direct effect |
428 |
LOGICAL:: ok_aie = .false. ! apply aerosol indirect effect |
429 |
|
430 |
REAL:: bl95_b0 = 2., bl95_b1 = 0.2 |
431 |
! Parameters in equation (D) of Boucher and Lohmann (1995, Tellus |
432 |
! B). They link cloud droplet number concentration to aerosol mass |
433 |
! concentration. |
434 |
|
435 |
real zmasse(klon, llm) |
436 |
! (column-density of mass of air in a cell, in kg m-2) |
437 |
|
438 |
integer, save:: ncid_startphy |
439 |
|
440 |
namelist /physiq_nml/ fact_cldcon, facttemps, ok_newmicro, iflag_cldcon, & |
441 |
ratqsbas, ratqshaut, ok_ade, ok_aie, bl95_b0, bl95_b1, & |
442 |
iflag_thermals, nsplit_thermals |
443 |
|
444 |
!---------------------------------------------------------------- |
445 |
|
446 |
IF (nqmx < 2) CALL abort_gcm('physiq', & |
447 |
'eaux vapeur et liquide sont indispensables') |
448 |
|
449 |
test_firstcal: IF (firstcal) THEN |
450 |
! initialiser |
451 |
u10m = 0. |
452 |
v10m = 0. |
453 |
t2m = 0. |
454 |
q2m = 0. |
455 |
ffonte = 0. |
456 |
fqcalving = 0. |
457 |
piz_ae = 0. |
458 |
tau_ae = 0. |
459 |
cg_ae = 0. |
460 |
rain_con = 0. |
461 |
snow_con = 0. |
462 |
topswai = 0. |
463 |
topswad = 0. |
464 |
solswai = 0. |
465 |
solswad = 0. |
466 |
|
467 |
d_u_con = 0. |
468 |
d_v_con = 0. |
469 |
rnebcon0 = 0. |
470 |
clwcon0 = 0. |
471 |
rnebcon = 0. |
472 |
clwcon = 0. |
473 |
|
474 |
pblh =0. ! Hauteur de couche limite |
475 |
plcl =0. ! Niveau de condensation de la CLA |
476 |
capCL =0. ! CAPE de couche limite |
477 |
oliqCL =0. ! eau_liqu integree de couche limite |
478 |
cteiCL =0. ! cloud top instab. crit. couche limite |
479 |
pblt =0. ! T a la Hauteur de couche limite |
480 |
therm =0. |
481 |
trmb1 =0. ! deep_cape |
482 |
trmb2 =0. ! inhibition |
483 |
trmb3 =0. ! Point Omega |
484 |
|
485 |
iflag_thermals = 0 |
486 |
nsplit_thermals = 1 |
487 |
print *, "Enter namelist 'physiq_nml'." |
488 |
read(unit=*, nml=physiq_nml) |
489 |
write(unit_nml, nml=physiq_nml) |
490 |
|
491 |
call conf_phys |
492 |
|
493 |
! Initialiser les compteurs: |
494 |
|
495 |
frugs = 0. |
496 |
CALL phyetat0(pctsrf, ftsol, ftsoil, fqsurf, qsol, fsnow, falbe, & |
497 |
fevap, rain_fall, snow_fall, solsw, sollw, dlw, radsol, frugs, & |
498 |
agesno, zmea, zstd, zsig, zgam, zthe, zpic, zval, t_ancien, & |
499 |
q_ancien, ancien_ok, rnebcon, ratqs, clwcon, run_off_lic_0, sig1, & |
500 |
w01, ncid_startphy) |
501 |
|
502 |
! ATTENTION : il faudra a terme relire q2 dans l'etat initial |
503 |
q2 = 1e-8 |
504 |
|
505 |
radpas = lmt_pas / nbapp_rad |
506 |
print *, "radpas = ", radpas |
507 |
|
508 |
! Initialisation pour le sch\'ema de convection d'Emanuel : |
509 |
IF (conv_emanuel) THEN |
510 |
ibas_con = 1 |
511 |
itop_con = 1 |
512 |
ENDIF |
513 |
|
514 |
IF (ok_orodr) THEN |
515 |
rugoro = MAX(1e-5, zstd * zsig / 2) |
516 |
CALL SUGWD(paprs, play) |
517 |
else |
518 |
rugoro = 0. |
519 |
ENDIF |
520 |
|
521 |
ecrit_ins = NINT(ecrit_ins / dtphys) |
522 |
|
523 |
! Initialisation des sorties |
524 |
|
525 |
call ini_histins(dtphys) |
526 |
CALL ymds2ju(annee_ref, 1, day_ref, 0., date0) |
527 |
! Positionner date0 pour initialisation de ORCHIDEE |
528 |
print *, 'physiq date0: ', date0 |
529 |
CALL phyredem0 |
530 |
ENDIF test_firstcal |
531 |
|
532 |
! We will modify variables *_seri and we will not touch variables |
533 |
! u, v, t, qx: |
534 |
t_seri = t |
535 |
u_seri = u |
536 |
v_seri = v |
537 |
q_seri = qx(:, :, ivap) |
538 |
ql_seri = qx(:, :, iliq) |
539 |
tr_seri = qx(:, :, 3:nqmx) |
540 |
|
541 |
ztsol = sum(ftsol * pctsrf, dim = 2) |
542 |
|
543 |
! Diagnostic de la tendance dynamique : |
544 |
IF (ancien_ok) THEN |
545 |
DO k = 1, llm |
546 |
DO i = 1, klon |
547 |
d_t_dyn(i, k) = (t_seri(i, k) - t_ancien(i, k)) / dtphys |
548 |
d_q_dyn(i, k) = (q_seri(i, k) - q_ancien(i, k)) / dtphys |
549 |
ENDDO |
550 |
ENDDO |
551 |
ELSE |
552 |
DO k = 1, llm |
553 |
DO i = 1, klon |
554 |
d_t_dyn(i, k) = 0. |
555 |
d_q_dyn(i, k) = 0. |
556 |
ENDDO |
557 |
ENDDO |
558 |
ancien_ok = .TRUE. |
559 |
ENDIF |
560 |
|
561 |
! Ajouter le geopotentiel du sol: |
562 |
DO k = 1, llm |
563 |
DO i = 1, klon |
564 |
zphi(i, k) = pphi(i, k) + pphis(i) |
565 |
ENDDO |
566 |
ENDDO |
567 |
|
568 |
! Check temperatures: |
569 |
CALL hgardfou(t_seri, ftsol) |
570 |
|
571 |
call increment_itap |
572 |
julien = MOD(dayvrai, 360) |
573 |
if (julien == 0) julien = 360 |
574 |
|
575 |
forall (k = 1: llm) zmasse(:, k) = (paprs(:, k) - paprs(:, k + 1)) / rg |
576 |
|
577 |
! Prescrire l'ozone : |
578 |
wo = ozonecm(REAL(julien), paprs) |
579 |
|
580 |
! \'Evaporation de l'eau liquide nuageuse : |
581 |
DO k = 1, llm |
582 |
DO i = 1, klon |
583 |
zb = MAX(0., ql_seri(i, k)) |
584 |
t_seri(i, k) = t_seri(i, k) & |
585 |
- zb * RLVTT / RCPD / (1. + RVTMP2 * q_seri(i, k)) |
586 |
q_seri(i, k) = q_seri(i, k) + zb |
587 |
ENDDO |
588 |
ENDDO |
589 |
ql_seri = 0. |
590 |
|
591 |
frugs = MAX(frugs, 0.000015) |
592 |
zxrugs = sum(frugs * pctsrf, dim = 2) |
593 |
|
594 |
! Calculs n\'ecessaires au calcul de l'albedo dans l'interface avec |
595 |
! la surface. |
596 |
|
597 |
CALL orbite(REAL(julien), longi, dist) |
598 |
IF (cycle_diurne) THEN |
599 |
CALL zenang(longi, time, dtphys * radpas, mu0, fract) |
600 |
ELSE |
601 |
mu0 = - 999.999 |
602 |
ENDIF |
603 |
|
604 |
! Calcul de l'abedo moyen par maille |
605 |
albsol = sum(falbe * pctsrf, dim = 2) |
606 |
|
607 |
! R\'epartition sous maille des flux longwave et shortwave |
608 |
! R\'epartition du longwave par sous-surface lin\'earis\'ee |
609 |
|
610 |
forall (nsrf = 1: nbsrf) |
611 |
fsollw(:, nsrf) = sollw + 4. * RSIGMA * ztsol**3 & |
612 |
* (ztsol - ftsol(:, nsrf)) |
613 |
fsolsw(:, nsrf) = solsw * (1. - falbe(:, nsrf)) / (1. - albsol) |
614 |
END forall |
615 |
|
616 |
fder = dlw |
617 |
|
618 |
! Couche limite: |
619 |
|
620 |
CALL clmain(dtphys, pctsrf, t_seri, q_seri, u_seri, v_seri, julien, mu0, & |
621 |
ftsol, cdmmax, cdhmax, ksta, ksta_ter, ok_kzmin, ftsoil, qsol, & |
622 |
paprs, play, fsnow, fqsurf, fevap, falbe, fluxlat, rain_fall, & |
623 |
snow_fall, fsolsw, fsollw, fder, rlat, frugs, agesno, rugoro, & |
624 |
d_t_vdf, d_q_vdf, d_u_vdf, d_v_vdf, d_ts, fluxt, fluxq, fluxu, & |
625 |
fluxv, cdragh, cdragm, q2, dsens, devap, ycoefh, yu1, yv1, t2m, q2m, & |
626 |
u10m, v10m, pblh, capCL, oliqCL, cteiCL, pblT, therm, trmb1, trmb2, & |
627 |
trmb3, plcl, fqcalving, ffonte, run_off_lic_0) |
628 |
|
629 |
! Incr\'ementation des flux |
630 |
|
631 |
zxfluxt = 0. |
632 |
zxfluxq = 0. |
633 |
zxfluxu = 0. |
634 |
zxfluxv = 0. |
635 |
DO nsrf = 1, nbsrf |
636 |
DO k = 1, llm |
637 |
DO i = 1, klon |
638 |
zxfluxt(i, k) = zxfluxt(i, k) + fluxt(i, k, nsrf) * pctsrf(i, nsrf) |
639 |
zxfluxq(i, k) = zxfluxq(i, k) + fluxq(i, k, nsrf) * pctsrf(i, nsrf) |
640 |
zxfluxu(i, k) = zxfluxu(i, k) + fluxu(i, k, nsrf) * pctsrf(i, nsrf) |
641 |
zxfluxv(i, k) = zxfluxv(i, k) + fluxv(i, k, nsrf) * pctsrf(i, nsrf) |
642 |
END DO |
643 |
END DO |
644 |
END DO |
645 |
DO i = 1, klon |
646 |
sens(i) = - zxfluxt(i, 1) ! flux de chaleur sensible au sol |
647 |
evap(i) = - zxfluxq(i, 1) ! flux d'\'evaporation au sol |
648 |
fder(i) = dlw(i) + dsens(i) + devap(i) |
649 |
ENDDO |
650 |
|
651 |
DO k = 1, llm |
652 |
DO i = 1, klon |
653 |
t_seri(i, k) = t_seri(i, k) + d_t_vdf(i, k) |
654 |
q_seri(i, k) = q_seri(i, k) + d_q_vdf(i, k) |
655 |
u_seri(i, k) = u_seri(i, k) + d_u_vdf(i, k) |
656 |
v_seri(i, k) = v_seri(i, k) + d_v_vdf(i, k) |
657 |
ENDDO |
658 |
ENDDO |
659 |
|
660 |
! Update surface temperature: |
661 |
|
662 |
DO i = 1, klon |
663 |
zxfluxlat(i) = 0. |
664 |
|
665 |
zt2m(i) = 0. |
666 |
zq2m(i) = 0. |
667 |
zu10m(i) = 0. |
668 |
zv10m(i) = 0. |
669 |
zxffonte(i) = 0. |
670 |
zxfqcalving(i) = 0. |
671 |
|
672 |
s_pblh(i) = 0. |
673 |
s_lcl(i) = 0. |
674 |
s_capCL(i) = 0. |
675 |
s_oliqCL(i) = 0. |
676 |
s_cteiCL(i) = 0. |
677 |
s_pblT(i) = 0. |
678 |
s_therm(i) = 0. |
679 |
s_trmb1(i) = 0. |
680 |
s_trmb2(i) = 0. |
681 |
s_trmb3(i) = 0. |
682 |
ENDDO |
683 |
|
684 |
call assert(abs(sum(pctsrf, dim = 2) - 1.) <= EPSFRA, 'physiq: pctsrf') |
685 |
|
686 |
ftsol = ftsol + d_ts |
687 |
ztsol = sum(ftsol * pctsrf, dim = 2) |
688 |
DO nsrf = 1, nbsrf |
689 |
DO i = 1, klon |
690 |
zxfluxlat(i) = zxfluxlat(i) + fluxlat(i, nsrf) * pctsrf(i, nsrf) |
691 |
|
692 |
zt2m(i) = zt2m(i) + t2m(i, nsrf) * pctsrf(i, nsrf) |
693 |
zq2m(i) = zq2m(i) + q2m(i, nsrf) * pctsrf(i, nsrf) |
694 |
zu10m(i) = zu10m(i) + u10m(i, nsrf) * pctsrf(i, nsrf) |
695 |
zv10m(i) = zv10m(i) + v10m(i, nsrf) * pctsrf(i, nsrf) |
696 |
zxffonte(i) = zxffonte(i) + ffonte(i, nsrf) * pctsrf(i, nsrf) |
697 |
zxfqcalving(i) = zxfqcalving(i) + & |
698 |
fqcalving(i, nsrf) * pctsrf(i, nsrf) |
699 |
s_pblh(i) = s_pblh(i) + pblh(i, nsrf) * pctsrf(i, nsrf) |
700 |
s_lcl(i) = s_lcl(i) + plcl(i, nsrf) * pctsrf(i, nsrf) |
701 |
s_capCL(i) = s_capCL(i) + capCL(i, nsrf) * pctsrf(i, nsrf) |
702 |
s_oliqCL(i) = s_oliqCL(i) + oliqCL(i, nsrf) * pctsrf(i, nsrf) |
703 |
s_cteiCL(i) = s_cteiCL(i) + cteiCL(i, nsrf) * pctsrf(i, nsrf) |
704 |
s_pblT(i) = s_pblT(i) + pblT(i, nsrf) * pctsrf(i, nsrf) |
705 |
s_therm(i) = s_therm(i) + therm(i, nsrf) * pctsrf(i, nsrf) |
706 |
s_trmb1(i) = s_trmb1(i) + trmb1(i, nsrf) * pctsrf(i, nsrf) |
707 |
s_trmb2(i) = s_trmb2(i) + trmb2(i, nsrf) * pctsrf(i, nsrf) |
708 |
s_trmb3(i) = s_trmb3(i) + trmb3(i, nsrf) * pctsrf(i, nsrf) |
709 |
ENDDO |
710 |
ENDDO |
711 |
|
712 |
! Si une sous-fraction n'existe pas, elle prend la valeur moyenne : |
713 |
DO nsrf = 1, nbsrf |
714 |
DO i = 1, klon |
715 |
IF (pctsrf(i, nsrf) < epsfra) then |
716 |
ftsol(i, nsrf) = ztsol(i) |
717 |
t2m(i, nsrf) = zt2m(i) |
718 |
q2m(i, nsrf) = zq2m(i) |
719 |
u10m(i, nsrf) = zu10m(i) |
720 |
v10m(i, nsrf) = zv10m(i) |
721 |
ffonte(i, nsrf) = zxffonte(i) |
722 |
fqcalving(i, nsrf) = zxfqcalving(i) |
723 |
pblh(i, nsrf) = s_pblh(i) |
724 |
plcl(i, nsrf) = s_lcl(i) |
725 |
capCL(i, nsrf) = s_capCL(i) |
726 |
oliqCL(i, nsrf) = s_oliqCL(i) |
727 |
cteiCL(i, nsrf) = s_cteiCL(i) |
728 |
pblT(i, nsrf) = s_pblT(i) |
729 |
therm(i, nsrf) = s_therm(i) |
730 |
trmb1(i, nsrf) = s_trmb1(i) |
731 |
trmb2(i, nsrf) = s_trmb2(i) |
732 |
trmb3(i, nsrf) = s_trmb3(i) |
733 |
end IF |
734 |
ENDDO |
735 |
ENDDO |
736 |
|
737 |
! Calculer la dérive du flux infrarouge |
738 |
|
739 |
DO i = 1, klon |
740 |
dlw(i) = - 4. * RSIGMA * ztsol(i)**3 |
741 |
ENDDO |
742 |
|
743 |
! Appeler la convection |
744 |
|
745 |
if (conv_emanuel) then |
746 |
CALL concvl(paprs, play, t_seri, q_seri, u_seri, v_seri, sig1, w01, & |
747 |
d_t_con, d_q_con, d_u_con, d_v_con, rain_con, ibas_con, itop_con, & |
748 |
upwd, dnwd, dnwd0, Ma, cape, iflagctrl, qcondc, pmflxr, da, phi, mp) |
749 |
snow_con = 0. |
750 |
clwcon0 = qcondc |
751 |
mfu = upwd + dnwd |
752 |
|
753 |
IF (thermcep) THEN |
754 |
zqsat = MIN(0.5, r2es * FOEEW(t_seri, rtt >= t_seri) / play) |
755 |
zqsat = zqsat / (1. - retv * zqsat) |
756 |
ELSE |
757 |
zqsat = merge(qsats(t_seri), qsatl(t_seri), t_seri < t_coup) / play |
758 |
ENDIF |
759 |
|
760 |
! Properties of convective clouds |
761 |
clwcon0 = fact_cldcon * clwcon0 |
762 |
call clouds_gno(klon, llm, q_seri, zqsat, clwcon0, ptconv, ratqsc, & |
763 |
rnebcon0) |
764 |
|
765 |
forall (i = 1:klon) ema_pct(i) = paprs(i, itop_con(i) + 1) |
766 |
mfd = 0. |
767 |
pen_u = 0. |
768 |
pen_d = 0. |
769 |
pde_d = 0. |
770 |
pde_u = 0. |
771 |
else |
772 |
conv_q = d_q_dyn + d_q_vdf / dtphys |
773 |
conv_t = d_t_dyn + d_t_vdf / dtphys |
774 |
z_avant = sum((q_seri + ql_seri) * zmasse, dim=2) |
775 |
CALL conflx(dtphys, paprs, play, t_seri(:, llm:1:- 1), & |
776 |
q_seri(:, llm:1:- 1), conv_t, conv_q, zxfluxq(:, 1), omega, & |
777 |
d_t_con, d_q_con, rain_con, snow_con, mfu(:, llm:1:- 1), & |
778 |
mfd(:, llm:1:- 1), pen_u, pde_u, pen_d, pde_d, kcbot, kctop, & |
779 |
kdtop, pmflxr, pmflxs) |
780 |
WHERE (rain_con < 0.) rain_con = 0. |
781 |
WHERE (snow_con < 0.) snow_con = 0. |
782 |
ibas_con = llm + 1 - kcbot |
783 |
itop_con = llm + 1 - kctop |
784 |
END if |
785 |
|
786 |
DO k = 1, llm |
787 |
DO i = 1, klon |
788 |
t_seri(i, k) = t_seri(i, k) + d_t_con(i, k) |
789 |
q_seri(i, k) = q_seri(i, k) + d_q_con(i, k) |
790 |
u_seri(i, k) = u_seri(i, k) + d_u_con(i, k) |
791 |
v_seri(i, k) = v_seri(i, k) + d_v_con(i, k) |
792 |
ENDDO |
793 |
ENDDO |
794 |
|
795 |
IF (.not. conv_emanuel) THEN |
796 |
z_apres = sum((q_seri + ql_seri) * zmasse, dim=2) |
797 |
z_factor = (z_avant - (rain_con + snow_con) * dtphys) / z_apres |
798 |
DO k = 1, llm |
799 |
DO i = 1, klon |
800 |
IF (z_factor(i) > 1. + 1E-8 .OR. z_factor(i) < 1. - 1E-8) THEN |
801 |
q_seri(i, k) = q_seri(i, k) * z_factor(i) |
802 |
ENDIF |
803 |
ENDDO |
804 |
ENDDO |
805 |
ENDIF |
806 |
|
807 |
! Convection s\`eche (thermiques ou ajustement) |
808 |
|
809 |
d_t_ajs = 0. |
810 |
d_u_ajs = 0. |
811 |
d_v_ajs = 0. |
812 |
d_q_ajs = 0. |
813 |
fm_therm = 0. |
814 |
entr_therm = 0. |
815 |
|
816 |
if (iflag_thermals == 0) then |
817 |
! Ajustement sec |
818 |
CALL ajsec(paprs, play, t_seri, q_seri, d_t_ajs, d_q_ajs) |
819 |
t_seri = t_seri + d_t_ajs |
820 |
q_seri = q_seri + d_q_ajs |
821 |
else |
822 |
call calltherm(dtphys, play, paprs, pphi, u_seri, v_seri, t_seri, & |
823 |
q_seri, d_u_ajs, d_v_ajs, d_t_ajs, d_q_ajs, fm_therm, entr_therm) |
824 |
endif |
825 |
|
826 |
! Caclul des ratqs |
827 |
|
828 |
! ratqs convectifs \`a l'ancienne en fonction de (q(z = 0) - q) / q |
829 |
! on \'ecrase le tableau ratqsc calcul\'e par clouds_gno |
830 |
if (iflag_cldcon == 1) then |
831 |
do k = 1, llm |
832 |
do i = 1, klon |
833 |
if(ptconv(i, k)) then |
834 |
ratqsc(i, k) = ratqsbas + fact_cldcon & |
835 |
* (q_seri(i, 1) - q_seri(i, k)) / q_seri(i, k) |
836 |
else |
837 |
ratqsc(i, k) = 0. |
838 |
endif |
839 |
enddo |
840 |
enddo |
841 |
endif |
842 |
|
843 |
! ratqs stables |
844 |
do k = 1, llm |
845 |
do i = 1, klon |
846 |
ratqss(i, k) = ratqsbas + (ratqshaut - ratqsbas) & |
847 |
* min((paprs(i, 1) - play(i, k)) / (paprs(i, 1) - 3e4), 1.) |
848 |
enddo |
849 |
enddo |
850 |
|
851 |
! ratqs final |
852 |
if (iflag_cldcon == 1 .or. iflag_cldcon == 2) then |
853 |
! les ratqs sont une conbinaison de ratqss et ratqsc |
854 |
! ratqs final |
855 |
! 1e4 (en gros 3 heures), en dur pour le moment, est le temps de |
856 |
! relaxation des ratqs |
857 |
ratqs = max(ratqs * exp(- dtphys * facttemps), ratqss) |
858 |
ratqs = max(ratqs, ratqsc) |
859 |
else |
860 |
! on ne prend que le ratqs stable pour fisrtilp |
861 |
ratqs = ratqss |
862 |
endif |
863 |
|
864 |
CALL fisrtilp(dtphys, paprs, play, t_seri, q_seri, ptconv, ratqs, & |
865 |
d_t_lsc, d_q_lsc, d_ql_lsc, rneb, cldliq, rain_lsc, snow_lsc, & |
866 |
pfrac_impa, pfrac_nucl, pfrac_1nucl, frac_impa, frac_nucl, prfl, & |
867 |
psfl, rhcl) |
868 |
|
869 |
WHERE (rain_lsc < 0) rain_lsc = 0. |
870 |
WHERE (snow_lsc < 0) snow_lsc = 0. |
871 |
DO k = 1, llm |
872 |
DO i = 1, klon |
873 |
t_seri(i, k) = t_seri(i, k) + d_t_lsc(i, k) |
874 |
q_seri(i, k) = q_seri(i, k) + d_q_lsc(i, k) |
875 |
ql_seri(i, k) = ql_seri(i, k) + d_ql_lsc(i, k) |
876 |
cldfra(i, k) = rneb(i, k) |
877 |
IF (.NOT.new_oliq) cldliq(i, k) = ql_seri(i, k) |
878 |
ENDDO |
879 |
ENDDO |
880 |
|
881 |
! PRESCRIPTION DES NUAGES POUR LE RAYONNEMENT |
882 |
|
883 |
! 1. NUAGES CONVECTIFS |
884 |
|
885 |
IF (iflag_cldcon <= - 1) THEN |
886 |
! seulement pour Tiedtke |
887 |
snow_tiedtke = 0. |
888 |
if (iflag_cldcon == - 1) then |
889 |
rain_tiedtke = rain_con |
890 |
else |
891 |
rain_tiedtke = 0. |
892 |
do k = 1, llm |
893 |
do i = 1, klon |
894 |
if (d_q_con(i, k) < 0.) then |
895 |
rain_tiedtke(i) = rain_tiedtke(i) - d_q_con(i, k) / dtphys & |
896 |
* zmasse(i, k) |
897 |
endif |
898 |
enddo |
899 |
enddo |
900 |
endif |
901 |
|
902 |
! Nuages diagnostiques pour Tiedtke |
903 |
CALL diagcld1(paprs, play, rain_tiedtke, snow_tiedtke, ibas_con, & |
904 |
itop_con, diafra, dialiq) |
905 |
DO k = 1, llm |
906 |
DO i = 1, klon |
907 |
IF (diafra(i, k) > cldfra(i, k)) THEN |
908 |
cldliq(i, k) = dialiq(i, k) |
909 |
cldfra(i, k) = diafra(i, k) |
910 |
ENDIF |
911 |
ENDDO |
912 |
ENDDO |
913 |
ELSE IF (iflag_cldcon == 3) THEN |
914 |
! On prend pour les nuages convectifs le maximum du calcul de |
915 |
! la convection et du calcul du pas de temps pr\'ec\'edent diminu\'e |
916 |
! d'un facteur facttemps. |
917 |
facteur = dtphys * facttemps |
918 |
do k = 1, llm |
919 |
do i = 1, klon |
920 |
rnebcon(i, k) = rnebcon(i, k) * facteur |
921 |
if (rnebcon0(i, k) * clwcon0(i, k) & |
922 |
> rnebcon(i, k) * clwcon(i, k)) then |
923 |
rnebcon(i, k) = rnebcon0(i, k) |
924 |
clwcon(i, k) = clwcon0(i, k) |
925 |
endif |
926 |
enddo |
927 |
enddo |
928 |
|
929 |
! On prend la somme des fractions nuageuses et des contenus en eau |
930 |
cldfra = min(max(cldfra, rnebcon), 1.) |
931 |
cldliq = cldliq + rnebcon * clwcon |
932 |
ENDIF |
933 |
|
934 |
! 2. Nuages stratiformes |
935 |
|
936 |
IF (ok_stratus) THEN |
937 |
CALL diagcld2(paprs, play, t_seri, q_seri, diafra, dialiq) |
938 |
DO k = 1, llm |
939 |
DO i = 1, klon |
940 |
IF (diafra(i, k) > cldfra(i, k)) THEN |
941 |
cldliq(i, k) = dialiq(i, k) |
942 |
cldfra(i, k) = diafra(i, k) |
943 |
ENDIF |
944 |
ENDDO |
945 |
ENDDO |
946 |
ENDIF |
947 |
|
948 |
! Precipitation totale |
949 |
DO i = 1, klon |
950 |
rain_fall(i) = rain_con(i) + rain_lsc(i) |
951 |
snow_fall(i) = snow_con(i) + snow_lsc(i) |
952 |
ENDDO |
953 |
|
954 |
! Humidit\'e relative pour diagnostic : |
955 |
DO k = 1, llm |
956 |
DO i = 1, klon |
957 |
zx_t = t_seri(i, k) |
958 |
IF (thermcep) THEN |
959 |
zx_qs = r2es * FOEEW(zx_t, rtt >= zx_t) / play(i, k) |
960 |
zx_qs = MIN(0.5, zx_qs) |
961 |
zcor = 1. / (1. - retv * zx_qs) |
962 |
zx_qs = zx_qs * zcor |
963 |
ELSE |
964 |
IF (zx_t < t_coup) THEN |
965 |
zx_qs = qsats(zx_t) / play(i, k) |
966 |
ELSE |
967 |
zx_qs = qsatl(zx_t) / play(i, k) |
968 |
ENDIF |
969 |
ENDIF |
970 |
zx_rh(i, k) = q_seri(i, k) / zx_qs |
971 |
zqsat(i, k) = zx_qs |
972 |
ENDDO |
973 |
ENDDO |
974 |
|
975 |
! Introduce the aerosol direct and first indirect radiative forcings: |
976 |
tau_ae = 0. |
977 |
piz_ae = 0. |
978 |
cg_ae = 0. |
979 |
|
980 |
! Param\`etres optiques des nuages et quelques param\`etres pour |
981 |
! diagnostics : |
982 |
if (ok_newmicro) then |
983 |
CALL newmicro(paprs, play, t_seri, cldliq, cldfra, cldtau, cldemi, & |
984 |
cldh, cldl, cldm, cldt, cldq, flwp, fiwp, flwc, fiwc, ok_aie, & |
985 |
sulfate, sulfate_pi, bl95_b0, bl95_b1, cldtaupi, re, fl) |
986 |
else |
987 |
CALL nuage(paprs, play, t_seri, cldliq, cldfra, cldtau, cldemi, cldh, & |
988 |
cldl, cldm, cldt, cldq, ok_aie, sulfate, sulfate_pi, bl95_b0, & |
989 |
bl95_b1, cldtaupi, re, fl) |
990 |
endif |
991 |
|
992 |
IF (MOD(itap - 1, radpas) == 0) THEN |
993 |
! Appeler le rayonnement mais calculer tout d'abord l'albedo du sol. |
994 |
! Calcul de l'abedo moyen par maille |
995 |
albsol = sum(falbe * pctsrf, dim = 2) |
996 |
|
997 |
! Rayonnement (compatible Arpege-IFS) : |
998 |
CALL radlwsw(dist, mu0, fract, paprs, play, ztsol, albsol, t_seri, & |
999 |
q_seri, wo, cldfra, cldemi, cldtau, heat, heat0, cool, cool0, & |
1000 |
radsol, albpla, topsw, toplw, solsw, sollw, sollwdown, topsw0, & |
1001 |
toplw0, solsw0, sollw0, lwdn0, lwdn, lwup0, lwup, swdn0, swdn, & |
1002 |
swup0, swup, ok_ade, ok_aie, tau_ae, piz_ae, cg_ae, topswad, & |
1003 |
solswad, cldtaupi, topswai, solswai) |
1004 |
ENDIF |
1005 |
|
1006 |
! Ajouter la tendance des rayonnements (tous les pas) |
1007 |
|
1008 |
DO k = 1, llm |
1009 |
DO i = 1, klon |
1010 |
t_seri(i, k) = t_seri(i, k) + (heat(i, k) - cool(i, k)) * dtphys & |
1011 |
/ 86400. |
1012 |
ENDDO |
1013 |
ENDDO |
1014 |
|
1015 |
! Calculer l'hydrologie de la surface |
1016 |
DO i = 1, klon |
1017 |
zxqsurf(i) = 0. |
1018 |
zxsnow(i) = 0. |
1019 |
ENDDO |
1020 |
DO nsrf = 1, nbsrf |
1021 |
DO i = 1, klon |
1022 |
zxqsurf(i) = zxqsurf(i) + fqsurf(i, nsrf) * pctsrf(i, nsrf) |
1023 |
zxsnow(i) = zxsnow(i) + fsnow(i, nsrf) * pctsrf(i, nsrf) |
1024 |
ENDDO |
1025 |
ENDDO |
1026 |
|
1027 |
! Calculer le bilan du sol et la d\'erive de temp\'erature (couplage) |
1028 |
|
1029 |
DO i = 1, klon |
1030 |
bils(i) = radsol(i) - sens(i) + zxfluxlat(i) |
1031 |
ENDDO |
1032 |
|
1033 |
! Param\'etrisation de l'orographie \`a l'\'echelle sous-maille : |
1034 |
|
1035 |
IF (ok_orodr) THEN |
1036 |
! S\'election des points pour lesquels le sch\'ema est actif : |
1037 |
igwd = 0 |
1038 |
DO i = 1, klon |
1039 |
itest(i) = 0 |
1040 |
IF (zpic(i) - zmea(i) > 100. .AND. zstd(i) > 10.) THEN |
1041 |
itest(i) = 1 |
1042 |
igwd = igwd + 1 |
1043 |
ENDIF |
1044 |
ENDDO |
1045 |
|
1046 |
CALL drag_noro(klon, llm, dtphys, paprs, play, zmea, zstd, zsig, zgam, & |
1047 |
zthe, zpic, zval, itest, t_seri, u_seri, v_seri, zulow, zvlow, & |
1048 |
zustrdr, zvstrdr, d_t_oro, d_u_oro, d_v_oro) |
1049 |
|
1050 |
! ajout des tendances |
1051 |
DO k = 1, llm |
1052 |
DO i = 1, klon |
1053 |
t_seri(i, k) = t_seri(i, k) + d_t_oro(i, k) |
1054 |
u_seri(i, k) = u_seri(i, k) + d_u_oro(i, k) |
1055 |
v_seri(i, k) = v_seri(i, k) + d_v_oro(i, k) |
1056 |
ENDDO |
1057 |
ENDDO |
1058 |
ENDIF |
1059 |
|
1060 |
IF (ok_orolf) THEN |
1061 |
! S\'election des points pour lesquels le sch\'ema est actif : |
1062 |
igwd = 0 |
1063 |
DO i = 1, klon |
1064 |
itest(i) = 0 |
1065 |
IF (zpic(i) - zmea(i) > 100.) THEN |
1066 |
itest(i) = 1 |
1067 |
igwd = igwd + 1 |
1068 |
ENDIF |
1069 |
ENDDO |
1070 |
|
1071 |
CALL lift_noro(klon, llm, dtphys, paprs, play, rlat, zmea, zstd, zpic, & |
1072 |
itest, t_seri, u_seri, v_seri, zulow, zvlow, zustrli, zvstrli, & |
1073 |
d_t_lif, d_u_lif, d_v_lif) |
1074 |
|
1075 |
! Ajout des tendances : |
1076 |
DO k = 1, llm |
1077 |
DO i = 1, klon |
1078 |
t_seri(i, k) = t_seri(i, k) + d_t_lif(i, k) |
1079 |
u_seri(i, k) = u_seri(i, k) + d_u_lif(i, k) |
1080 |
v_seri(i, k) = v_seri(i, k) + d_v_lif(i, k) |
1081 |
ENDDO |
1082 |
ENDDO |
1083 |
ENDIF |
1084 |
|
1085 |
! Stress n\'ecessaires : toute la physique |
1086 |
|
1087 |
DO i = 1, klon |
1088 |
zustrph(i) = 0. |
1089 |
zvstrph(i) = 0. |
1090 |
ENDDO |
1091 |
DO k = 1, llm |
1092 |
DO i = 1, klon |
1093 |
zustrph(i) = zustrph(i) + (u_seri(i, k) - u(i, k)) / dtphys & |
1094 |
* zmasse(i, k) |
1095 |
zvstrph(i) = zvstrph(i) + (v_seri(i, k) - v(i, k)) / dtphys & |
1096 |
* zmasse(i, k) |
1097 |
ENDDO |
1098 |
ENDDO |
1099 |
|
1100 |
CALL aaam_bud(rg, romega, rlat, rlon, pphis, zustrdr, zustrli, zustrph, & |
1101 |
zvstrdr, zvstrli, zvstrph, paprs, u, v, aam, torsfc) |
1102 |
|
1103 |
! Calcul des tendances traceurs |
1104 |
call phytrac(julien, time, firstcal, lafin, dtphys, t, paprs, play, mfu, & |
1105 |
mfd, pde_u, pen_d, ycoefh, fm_therm, entr_therm, yu1, yv1, ftsol, & |
1106 |
pctsrf, frac_impa, frac_nucl, da, phi, mp, upwd, dnwd, tr_seri, & |
1107 |
zmasse, ncid_startphy) |
1108 |
|
1109 |
IF (offline) call phystokenc(dtphys, t, mfu, mfd, pen_u, pde_u, pen_d, & |
1110 |
pde_d, fm_therm, entr_therm, ycoefh, yu1, yv1, ftsol, pctsrf, & |
1111 |
frac_impa, frac_nucl, pphis, airephy, dtphys) |
1112 |
|
1113 |
! Calculer le transport de l'eau et de l'energie (diagnostique) |
1114 |
CALL transp(paprs, t_seri, q_seri, u_seri, v_seri, zphi, ve, vq, ue, uq) |
1115 |
|
1116 |
! diag. bilKP |
1117 |
|
1118 |
CALL transp_lay(paprs, t_seri, q_seri, u_seri, v_seri, zphi, & |
1119 |
ve_lay, vq_lay, ue_lay, uq_lay) |
1120 |
|
1121 |
! Accumuler les variables a stocker dans les fichiers histoire: |
1122 |
|
1123 |
! conversion Ec en énergie thermique |
1124 |
DO k = 1, llm |
1125 |
DO i = 1, klon |
1126 |
ZRCPD = RCPD * (1. + RVTMP2 * q_seri(i, k)) |
1127 |
d_t_ec(i, k) = 0.5 / ZRCPD & |
1128 |
* (u(i, k)**2 + v(i, k)**2 - u_seri(i, k)**2 - v_seri(i, k)**2) |
1129 |
t_seri(i, k) = t_seri(i, k) + d_t_ec(i, k) |
1130 |
d_t_ec(i, k) = d_t_ec(i, k) / dtphys |
1131 |
END DO |
1132 |
END DO |
1133 |
|
1134 |
! SORTIES |
1135 |
|
1136 |
! prw = eau precipitable |
1137 |
DO i = 1, klon |
1138 |
prw(i) = 0. |
1139 |
DO k = 1, llm |
1140 |
prw(i) = prw(i) + q_seri(i, k) * zmasse(i, k) |
1141 |
ENDDO |
1142 |
ENDDO |
1143 |
|
1144 |
! Convertir les incrementations en tendances |
1145 |
|
1146 |
DO k = 1, llm |
1147 |
DO i = 1, klon |
1148 |
d_u(i, k) = (u_seri(i, k) - u(i, k)) / dtphys |
1149 |
d_v(i, k) = (v_seri(i, k) - v(i, k)) / dtphys |
1150 |
d_t(i, k) = (t_seri(i, k) - t(i, k)) / dtphys |
1151 |
d_qx(i, k, ivap) = (q_seri(i, k) - qx(i, k, ivap)) / dtphys |
1152 |
d_qx(i, k, iliq) = (ql_seri(i, k) - qx(i, k, iliq)) / dtphys |
1153 |
ENDDO |
1154 |
ENDDO |
1155 |
|
1156 |
DO iq = 3, nqmx |
1157 |
DO k = 1, llm |
1158 |
DO i = 1, klon |
1159 |
d_qx(i, k, iq) = (tr_seri(i, k, iq - 2) - qx(i, k, iq)) / dtphys |
1160 |
ENDDO |
1161 |
ENDDO |
1162 |
ENDDO |
1163 |
|
1164 |
! Sauvegarder les valeurs de t et q a la fin de la physique: |
1165 |
DO k = 1, llm |
1166 |
DO i = 1, klon |
1167 |
t_ancien(i, k) = t_seri(i, k) |
1168 |
q_ancien(i, k) = q_seri(i, k) |
1169 |
ENDDO |
1170 |
ENDDO |
1171 |
|
1172 |
CALL histwrite_phy("phis", pphis) |
1173 |
CALL histwrite_phy("aire", airephy) |
1174 |
CALL histwrite_phy("psol", paprs(:, 1)) |
1175 |
CALL histwrite_phy("precip", rain_fall + snow_fall) |
1176 |
CALL histwrite_phy("plul", rain_lsc + snow_lsc) |
1177 |
CALL histwrite_phy("pluc", rain_con + snow_con) |
1178 |
CALL histwrite_phy("tsol", ztsol) |
1179 |
CALL histwrite_phy("t2m", zt2m) |
1180 |
CALL histwrite_phy("q2m", zq2m) |
1181 |
CALL histwrite_phy("u10m", zu10m) |
1182 |
CALL histwrite_phy("v10m", zv10m) |
1183 |
CALL histwrite_phy("snow", snow_fall) |
1184 |
CALL histwrite_phy("cdrm", cdragm) |
1185 |
CALL histwrite_phy("cdrh", cdragh) |
1186 |
CALL histwrite_phy("topl", toplw) |
1187 |
CALL histwrite_phy("evap", evap) |
1188 |
CALL histwrite_phy("sols", solsw) |
1189 |
CALL histwrite_phy("soll", sollw) |
1190 |
CALL histwrite_phy("solldown", sollwdown) |
1191 |
CALL histwrite_phy("bils", bils) |
1192 |
CALL histwrite_phy("sens", - sens) |
1193 |
CALL histwrite_phy("fder", fder) |
1194 |
CALL histwrite_phy("dtsvdfo", d_ts(:, is_oce)) |
1195 |
CALL histwrite_phy("dtsvdft", d_ts(:, is_ter)) |
1196 |
CALL histwrite_phy("dtsvdfg", d_ts(:, is_lic)) |
1197 |
CALL histwrite_phy("dtsvdfi", d_ts(:, is_sic)) |
1198 |
|
1199 |
DO nsrf = 1, nbsrf |
1200 |
CALL histwrite_phy("pourc_"//clnsurf(nsrf), pctsrf(:, nsrf) * 100.) |
1201 |
CALL histwrite_phy("fract_"//clnsurf(nsrf), pctsrf(:, nsrf)) |
1202 |
CALL histwrite_phy("sens_"//clnsurf(nsrf), fluxt(:, 1, nsrf)) |
1203 |
CALL histwrite_phy("lat_"//clnsurf(nsrf), fluxlat(:, nsrf)) |
1204 |
CALL histwrite_phy("tsol_"//clnsurf(nsrf), ftsol(:, nsrf)) |
1205 |
CALL histwrite_phy("taux_"//clnsurf(nsrf), fluxu(:, 1, nsrf)) |
1206 |
CALL histwrite_phy("tauy_"//clnsurf(nsrf), fluxv(:, 1, nsrf)) |
1207 |
CALL histwrite_phy("rugs_"//clnsurf(nsrf), frugs(:, nsrf)) |
1208 |
CALL histwrite_phy("albe_"//clnsurf(nsrf), falbe(:, nsrf)) |
1209 |
END DO |
1210 |
|
1211 |
CALL histwrite_phy("albs", albsol) |
1212 |
CALL histwrite_phy("rugs", zxrugs) |
1213 |
CALL histwrite_phy("s_pblh", s_pblh) |
1214 |
CALL histwrite_phy("s_pblt", s_pblt) |
1215 |
CALL histwrite_phy("s_lcl", s_lcl) |
1216 |
CALL histwrite_phy("s_capCL", s_capCL) |
1217 |
CALL histwrite_phy("s_oliqCL", s_oliqCL) |
1218 |
CALL histwrite_phy("s_cteiCL", s_cteiCL) |
1219 |
CALL histwrite_phy("s_therm", s_therm) |
1220 |
CALL histwrite_phy("s_trmb1", s_trmb1) |
1221 |
CALL histwrite_phy("s_trmb2", s_trmb2) |
1222 |
CALL histwrite_phy("s_trmb3", s_trmb3) |
1223 |
if (conv_emanuel) CALL histwrite_phy("ptop", ema_pct) |
1224 |
CALL histwrite_phy("temp", t_seri) |
1225 |
CALL histwrite_phy("vitu", u_seri) |
1226 |
CALL histwrite_phy("vitv", v_seri) |
1227 |
CALL histwrite_phy("geop", zphi) |
1228 |
CALL histwrite_phy("pres", play) |
1229 |
CALL histwrite_phy("dtvdf", d_t_vdf) |
1230 |
CALL histwrite_phy("dqvdf", d_q_vdf) |
1231 |
CALL histwrite_phy("rhum", zx_rh) |
1232 |
|
1233 |
if (ok_instan) call histsync(nid_ins) |
1234 |
|
1235 |
IF (lafin) then |
1236 |
call NF95_CLOSE(ncid_startphy) |
1237 |
CALL phyredem(pctsrf, ftsol, ftsoil, fqsurf, qsol, & |
1238 |
fsnow, falbe, fevap, rain_fall, snow_fall, solsw, sollw, dlw, & |
1239 |
radsol, frugs, agesno, zmea, zstd, zsig, zgam, zthe, zpic, zval, & |
1240 |
t_ancien, q_ancien, rnebcon, ratqs, clwcon, run_off_lic_0, sig1, & |
1241 |
w01) |
1242 |
end IF |
1243 |
|
1244 |
firstcal = .FALSE. |
1245 |
|
1246 |
END SUBROUTINE physiq |
1247 |
|
1248 |
end module physiq_m |