1 |
module clmain_m |
2 |
|
3 |
IMPLICIT NONE |
4 |
|
5 |
contains |
6 |
|
7 |
SUBROUTINE clmain(dtime, pctsrf, t, q, u, v, jour, rmu0, ftsol, cdmmax, & |
8 |
cdhmax, ksta, ksta_ter, ok_kzmin, ftsoil, qsol, paprs, pplay, snow, & |
9 |
qsurf, evap, falbe, fluxlat, rain_fall, snow_f, solsw, sollw, fder, & |
10 |
rlat, rugos, agesno, rugoro, d_t, d_q, d_u, d_v, d_ts, flux_t, flux_q, & |
11 |
flux_u, flux_v, cdragh, cdragm, q2, dflux_t, dflux_q, ycoefh, zu1, & |
12 |
zv1, t2m, q2m, u10m, v10m, pblh, capcl, oliqcl, cteicl, pblt, therm, & |
13 |
trmb1, trmb2, trmb3, plcl, fqcalving, ffonte, run_off_lic_0) |
14 |
|
15 |
! From phylmd/clmain.F, version 1.6, 2005/11/16 14:47:19 |
16 |
! Author: Z. X. Li (LMD/CNRS), date: 1993/08/18 |
17 |
! Objet : interface de couche limite (diffusion verticale) |
18 |
|
19 |
! Tout ce qui a trait aux traceurs est dans "phytrac". Le calcul |
20 |
! de la couche limite pour les traceurs se fait avec "cltrac" et |
21 |
! ne tient pas compte de la diff\'erentiation des sous-fractions |
22 |
! de sol. |
23 |
|
24 |
! Pour pouvoir extraire les coefficients d'\'echanges et le vent |
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! dans la premi\`ere couche, trois champs ont \'et\'e cr\'e\'es : "ycoefh", |
26 |
! "zu1" et "zv1". Nous avons moyenn\'e les valeurs de ces trois |
27 |
! champs sur les quatre sous-surfaces du mod\`ele. |
28 |
|
29 |
use clqh_m, only: clqh |
30 |
use clvent_m, only: clvent |
31 |
use coefkz_m, only: coefkz |
32 |
use coefkzmin_m, only: coefkzmin |
33 |
USE conf_gcm_m, ONLY: prt_level, lmt_pas |
34 |
USE conf_phys_m, ONLY: iflag_pbl |
35 |
USE dimphy, ONLY: klev, klon, zmasq |
36 |
USE dimsoil, ONLY: nsoilmx |
37 |
use hbtm_m, only: hbtm |
38 |
USE indicesol, ONLY: epsfra, is_lic, is_oce, is_sic, is_ter, nbsrf |
39 |
USE interfoce_lim_m, ONLY: interfoce_lim |
40 |
use stdlevvar_m, only: stdlevvar |
41 |
USE suphec_m, ONLY: rd, rg, rkappa |
42 |
use time_phylmdz, only: itap |
43 |
use ustarhb_m, only: ustarhb |
44 |
use vdif_kcay_m, only: vdif_kcay |
45 |
use yamada4_m, only: yamada4 |
46 |
|
47 |
REAL, INTENT(IN):: dtime ! interval du temps (secondes) |
48 |
|
49 |
REAL, INTENT(inout):: pctsrf(klon, nbsrf) |
50 |
! tableau des pourcentages de surface de chaque maille |
51 |
|
52 |
REAL, INTENT(IN):: t(klon, klev) ! temperature (K) |
53 |
REAL, INTENT(IN):: q(klon, klev) ! vapeur d'eau (kg/kg) |
54 |
REAL, INTENT(IN):: u(klon, klev), v(klon, klev) ! vitesse |
55 |
INTEGER, INTENT(IN):: jour ! jour de l'annee en cours |
56 |
REAL, intent(in):: rmu0(klon) ! cosinus de l'angle solaire zenithal |
57 |
REAL, INTENT(IN):: ftsol(klon, nbsrf) ! temp\'erature du sol (en K) |
58 |
REAL, INTENT(IN):: cdmmax, cdhmax ! seuils cdrm, cdrh |
59 |
REAL, INTENT(IN):: ksta, ksta_ter |
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LOGICAL, INTENT(IN):: ok_kzmin |
61 |
|
62 |
REAL, INTENT(inout):: ftsoil(klon, nsoilmx, nbsrf) |
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! soil temperature of surface fraction |
64 |
|
65 |
REAL, INTENT(inout):: qsol(klon) |
66 |
! column-density of water in soil, in kg m-2 |
67 |
|
68 |
REAL, INTENT(IN):: paprs(klon, klev+1) ! pression a intercouche (Pa) |
69 |
REAL, INTENT(IN):: pplay(klon, klev) ! pression au milieu de couche (Pa) |
70 |
REAL, INTENT(inout):: snow(klon, nbsrf) |
71 |
REAL qsurf(klon, nbsrf) |
72 |
REAL evap(klon, nbsrf) |
73 |
REAL, intent(inout):: falbe(klon, nbsrf) |
74 |
|
75 |
REAL fluxlat(klon, nbsrf) |
76 |
|
77 |
REAL, intent(in):: rain_fall(klon) |
78 |
! liquid water mass flux (kg/m2/s), positive down |
79 |
|
80 |
REAL, intent(in):: snow_f(klon) |
81 |
! solid water mass flux (kg/m2/s), positive down |
82 |
|
83 |
REAL, INTENT(IN):: solsw(klon, nbsrf), sollw(klon, nbsrf) |
84 |
REAL, intent(in):: fder(klon) |
85 |
REAL, INTENT(IN):: rlat(klon) ! latitude en degr\'es |
86 |
|
87 |
REAL, intent(inout):: rugos(klon, nbsrf) ! longueur de rugosit\'e (en m) |
88 |
|
89 |
real agesno(klon, nbsrf) |
90 |
REAL, INTENT(IN):: rugoro(klon) |
91 |
|
92 |
REAL d_t(klon, klev), d_q(klon, klev) |
93 |
! d_t------output-R- le changement pour "t" |
94 |
! d_q------output-R- le changement pour "q" |
95 |
|
96 |
REAL, intent(out):: d_u(klon, klev), d_v(klon, klev) |
97 |
! changement pour "u" et "v" |
98 |
|
99 |
REAL, intent(out):: d_ts(klon, nbsrf) ! le changement pour ftsol |
100 |
|
101 |
REAL, intent(out):: flux_t(klon, nbsrf) |
102 |
! flux de chaleur sensible (Cp T) (W/m2) (orientation positive vers |
103 |
! le bas) à la surface |
104 |
|
105 |
REAL, intent(out):: flux_q(klon, nbsrf) |
106 |
! flux de vapeur d'eau (kg/m2/s) à la surface |
107 |
|
108 |
REAL, intent(out):: flux_u(klon, nbsrf), flux_v(klon, nbsrf) |
109 |
! tension du vent à la surface, en Pa |
110 |
|
111 |
REAL, INTENT(out):: cdragh(klon), cdragm(klon) |
112 |
real q2(klon, klev+1, nbsrf) |
113 |
|
114 |
REAL, INTENT(out):: dflux_t(klon), dflux_q(klon) |
115 |
! dflux_t derive du flux sensible |
116 |
! dflux_q derive du flux latent |
117 |
! IM "slab" ocean |
118 |
|
119 |
REAL, intent(out):: ycoefh(klon, klev) |
120 |
REAL, intent(out):: zu1(klon) |
121 |
REAL zv1(klon) |
122 |
REAL t2m(klon, nbsrf), q2m(klon, nbsrf) |
123 |
REAL u10m(klon, nbsrf), v10m(klon, nbsrf) |
124 |
|
125 |
! Ionela Musat cf. Anne Mathieu : planetary boundary layer, hbtm |
126 |
! (Comme les autres diagnostics on cumule dans physiq ce qui |
127 |
! permet de sortir les grandeurs par sous-surface) |
128 |
REAL pblh(klon, nbsrf) ! height of planetary boundary layer |
129 |
REAL capcl(klon, nbsrf) |
130 |
REAL oliqcl(klon, nbsrf) |
131 |
REAL cteicl(klon, nbsrf) |
132 |
REAL pblt(klon, nbsrf) |
133 |
! pblT------- T au nveau HCL |
134 |
REAL therm(klon, nbsrf) |
135 |
REAL trmb1(klon, nbsrf) |
136 |
! trmb1-------deep_cape |
137 |
REAL trmb2(klon, nbsrf) |
138 |
! trmb2--------inhibition |
139 |
REAL trmb3(klon, nbsrf) |
140 |
! trmb3-------Point Omega |
141 |
REAL plcl(klon, nbsrf) |
142 |
REAL fqcalving(klon, nbsrf), ffonte(klon, nbsrf) |
143 |
! ffonte----Flux thermique utilise pour fondre la neige |
144 |
! fqcalving-Flux d'eau "perdue" par la surface et necessaire pour limiter la |
145 |
! hauteur de neige, en kg/m2/s |
146 |
REAL run_off_lic_0(klon) |
147 |
|
148 |
! Local: |
149 |
|
150 |
LOGICAL:: firstcal = .true. |
151 |
|
152 |
! la nouvelle repartition des surfaces sortie de l'interface |
153 |
REAL, save:: pctsrf_new_oce(klon) |
154 |
REAL, save:: pctsrf_new_sic(klon) |
155 |
|
156 |
REAL y_fqcalving(klon), y_ffonte(klon) |
157 |
real y_run_off_lic_0(klon) |
158 |
REAL rugmer(klon) |
159 |
REAL ytsoil(klon, nsoilmx) |
160 |
REAL yts(klon), yrugos(klon), ypct(klon), yz0_new(klon) |
161 |
REAL yalb(klon) |
162 |
REAL yu1(klon), yv1(klon) |
163 |
! on rajoute en output yu1 et yv1 qui sont les vents dans |
164 |
! la premiere couche |
165 |
REAL ysnow(klon), yqsurf(klon), yagesno(klon) |
166 |
|
167 |
real yqsol(klon) |
168 |
! column-density of water in soil, in kg m-2 |
169 |
|
170 |
REAL yrain_f(klon) |
171 |
! liquid water mass flux (kg/m2/s), positive down |
172 |
|
173 |
REAL ysnow_f(klon) |
174 |
! solid water mass flux (kg/m2/s), positive down |
175 |
|
176 |
REAL yfder(klon) |
177 |
REAL yrugm(klon), yrads(klon), yrugoro(klon) |
178 |
|
179 |
REAL yfluxlat(klon) |
180 |
|
181 |
REAL y_d_ts(klon) |
182 |
REAL y_d_t(klon, klev), y_d_q(klon, klev) |
183 |
REAL y_d_u(klon, klev), y_d_v(klon, klev) |
184 |
REAL y_flux_t(klon), y_flux_q(klon) |
185 |
REAL y_flux_u(klon), y_flux_v(klon) |
186 |
REAL y_dflux_t(klon), y_dflux_q(klon) |
187 |
REAL coefh(klon, klev), coefm(klon, klev) |
188 |
REAL yu(klon, klev), yv(klon, klev) |
189 |
REAL yt(klon, klev), yq(klon, klev) |
190 |
REAL ypaprs(klon, klev+1), ypplay(klon, klev), ydelp(klon, klev) |
191 |
|
192 |
REAL ycoefm0(klon, klev), ycoefh0(klon, klev) |
193 |
|
194 |
REAL yzlay(klon, klev), yzlev(klon, klev+1), yteta(klon, klev) |
195 |
REAL ykmm(klon, klev+1), ykmn(klon, klev+1) |
196 |
REAL ykmq(klon, klev+1) |
197 |
REAL yq2(klon, klev+1) |
198 |
REAL q2diag(klon, klev+1) |
199 |
|
200 |
REAL u1lay(klon), v1lay(klon) |
201 |
REAL delp(klon, klev) |
202 |
INTEGER i, k, nsrf |
203 |
|
204 |
INTEGER ni(klon), knon, j |
205 |
|
206 |
REAL pctsrf_pot(klon, nbsrf) |
207 |
! "pourcentage potentiel" pour tenir compte des \'eventuelles |
208 |
! apparitions ou disparitions de la glace de mer |
209 |
|
210 |
REAL zx_alf1, zx_alf2 ! valeur ambiante par extrapolation |
211 |
|
212 |
REAL yt2m(klon), yq2m(klon), yu10m(klon) |
213 |
REAL yustar(klon) |
214 |
|
215 |
REAL yt10m(klon), yq10m(klon) |
216 |
REAL ypblh(klon) |
217 |
REAL ylcl(klon) |
218 |
REAL ycapcl(klon) |
219 |
REAL yoliqcl(klon) |
220 |
REAL ycteicl(klon) |
221 |
REAL ypblt(klon) |
222 |
REAL ytherm(klon) |
223 |
REAL ytrmb1(klon) |
224 |
REAL ytrmb2(klon) |
225 |
REAL ytrmb3(klon) |
226 |
REAL uzon(klon), vmer(klon) |
227 |
REAL tair1(klon), qair1(klon), tairsol(klon) |
228 |
REAL psfce(klon), patm(klon) |
229 |
|
230 |
REAL qairsol(klon), zgeo1(klon) |
231 |
REAL rugo1(klon) |
232 |
|
233 |
! utiliser un jeu de fonctions simples |
234 |
LOGICAL zxli |
235 |
PARAMETER (zxli=.FALSE.) |
236 |
|
237 |
!------------------------------------------------------------ |
238 |
|
239 |
ytherm = 0. |
240 |
|
241 |
DO k = 1, klev ! epaisseur de couche |
242 |
DO i = 1, klon |
243 |
delp(i, k) = paprs(i, k) - paprs(i, k+1) |
244 |
END DO |
245 |
END DO |
246 |
DO i = 1, klon ! vent de la premiere couche |
247 |
zx_alf1 = 1.0 |
248 |
zx_alf2 = 1.0 - zx_alf1 |
249 |
u1lay(i) = u(i, 1)*zx_alf1 + u(i, 2)*zx_alf2 |
250 |
v1lay(i) = v(i, 1)*zx_alf1 + v(i, 2)*zx_alf2 |
251 |
END DO |
252 |
|
253 |
! Initialization: |
254 |
rugmer = 0. |
255 |
cdragh = 0. |
256 |
cdragm = 0. |
257 |
dflux_t = 0. |
258 |
dflux_q = 0. |
259 |
zu1 = 0. |
260 |
zv1 = 0. |
261 |
ypct = 0. |
262 |
yts = 0. |
263 |
ysnow = 0. |
264 |
yqsurf = 0. |
265 |
yrain_f = 0. |
266 |
ysnow_f = 0. |
267 |
yfder = 0. |
268 |
yrugos = 0. |
269 |
yu1 = 0. |
270 |
yv1 = 0. |
271 |
yrads = 0. |
272 |
ypaprs = 0. |
273 |
ypplay = 0. |
274 |
ydelp = 0. |
275 |
yu = 0. |
276 |
yv = 0. |
277 |
yt = 0. |
278 |
yq = 0. |
279 |
y_dflux_t = 0. |
280 |
y_dflux_q = 0. |
281 |
yrugoro = 0. |
282 |
d_ts = 0. |
283 |
yfluxlat = 0. |
284 |
flux_t = 0. |
285 |
flux_q = 0. |
286 |
flux_u = 0. |
287 |
flux_v = 0. |
288 |
d_t = 0. |
289 |
d_q = 0. |
290 |
d_u = 0. |
291 |
d_v = 0. |
292 |
ycoefh = 0. |
293 |
|
294 |
! Initialisation des "pourcentages potentiels". On consid\`ere ici qu'on |
295 |
! peut avoir potentiellement de la glace sur tout le domaine oc\'eanique |
296 |
! (\`a affiner) |
297 |
|
298 |
pctsrf_pot(:, is_ter) = pctsrf(:, is_ter) |
299 |
pctsrf_pot(:, is_lic) = pctsrf(:, is_lic) |
300 |
pctsrf_pot(:, is_oce) = 1. - zmasq |
301 |
pctsrf_pot(:, is_sic) = 1. - zmasq |
302 |
|
303 |
! Tester si c'est le moment de lire le fichier: |
304 |
if (mod(itap - 1, lmt_pas) == 0) then |
305 |
CALL interfoce_lim(jour, pctsrf_new_oce, pctsrf_new_sic) |
306 |
endif |
307 |
|
308 |
! Boucler sur toutes les sous-fractions du sol: |
309 |
|
310 |
loop_surface: DO nsrf = 1, nbsrf |
311 |
! Chercher les indices : |
312 |
ni = 0 |
313 |
knon = 0 |
314 |
DO i = 1, klon |
315 |
! Pour d\'eterminer le domaine \`a traiter, on utilise les surfaces |
316 |
! "potentielles" |
317 |
IF (pctsrf_pot(i, nsrf) > epsfra) THEN |
318 |
knon = knon + 1 |
319 |
ni(knon) = i |
320 |
END IF |
321 |
END DO |
322 |
|
323 |
if_knon: IF (knon /= 0) then |
324 |
DO j = 1, knon |
325 |
i = ni(j) |
326 |
ypct(j) = pctsrf(i, nsrf) |
327 |
yts(j) = ftsol(i, nsrf) |
328 |
ysnow(j) = snow(i, nsrf) |
329 |
yqsurf(j) = qsurf(i, nsrf) |
330 |
yalb(j) = falbe(i, nsrf) |
331 |
yrain_f(j) = rain_fall(i) |
332 |
ysnow_f(j) = snow_f(i) |
333 |
yagesno(j) = agesno(i, nsrf) |
334 |
yfder(j) = fder(i) |
335 |
yrugos(j) = rugos(i, nsrf) |
336 |
yrugoro(j) = rugoro(i) |
337 |
yu1(j) = u1lay(i) |
338 |
yv1(j) = v1lay(i) |
339 |
yrads(j) = solsw(i, nsrf) + sollw(i, nsrf) |
340 |
ypaprs(j, klev+1) = paprs(i, klev+1) |
341 |
y_run_off_lic_0(j) = run_off_lic_0(i) |
342 |
END DO |
343 |
|
344 |
! For continent, copy soil water content |
345 |
IF (nsrf == is_ter) THEN |
346 |
yqsol(:knon) = qsol(ni(:knon)) |
347 |
ELSE |
348 |
yqsol = 0. |
349 |
END IF |
350 |
|
351 |
ytsoil(:knon, :) = ftsoil(ni(:knon), :, nsrf) |
352 |
|
353 |
DO k = 1, klev |
354 |
DO j = 1, knon |
355 |
i = ni(j) |
356 |
ypaprs(j, k) = paprs(i, k) |
357 |
ypplay(j, k) = pplay(i, k) |
358 |
ydelp(j, k) = delp(i, k) |
359 |
yu(j, k) = u(i, k) |
360 |
yv(j, k) = v(i, k) |
361 |
yt(j, k) = t(i, k) |
362 |
yq(j, k) = q(i, k) |
363 |
END DO |
364 |
END DO |
365 |
|
366 |
! calculer Cdrag et les coefficients d'echange |
367 |
CALL coefkz(nsrf, ypaprs, ypplay, ksta, ksta_ter, yts, yrugos, yu, & |
368 |
yv, yt, yq, yqsurf, coefm(:knon, :), coefh(:knon, :)) |
369 |
IF (iflag_pbl == 1) THEN |
370 |
CALL coefkz2(nsrf, knon, ypaprs, ypplay, yt, ycoefm0, ycoefh0) |
371 |
coefm(:knon, :) = max(coefm(:knon, :), ycoefm0(:knon, :)) |
372 |
coefh(:knon, :) = max(coefh(:knon, :), ycoefh0(:knon, :)) |
373 |
END IF |
374 |
|
375 |
! on met un seuil pour coefm et coefh |
376 |
IF (nsrf == is_oce) THEN |
377 |
coefm(:knon, 1) = min(coefm(:knon, 1), cdmmax) |
378 |
coefh(:knon, 1) = min(coefh(:knon, 1), cdhmax) |
379 |
END IF |
380 |
|
381 |
IF (ok_kzmin) THEN |
382 |
! Calcul d'une diffusion minimale pour les conditions tres stables |
383 |
CALL coefkzmin(knon, ypaprs, ypplay, yu, yv, yt, yq, & |
384 |
coefm(:knon, 1), ycoefm0, ycoefh0) |
385 |
coefm(:knon, :) = max(coefm(:knon, :), ycoefm0(:knon, :)) |
386 |
coefh(:knon, :) = max(coefh(:knon, :), ycoefh0(:knon, :)) |
387 |
END IF |
388 |
|
389 |
IF (iflag_pbl >= 3) THEN |
390 |
! Mellor et Yamada adapt\'e \`a Mars, Richard Fournier et |
391 |
! Fr\'ed\'eric Hourdin |
392 |
yzlay(:knon, 1) = rd * yt(:knon, 1) / (0.5 * (ypaprs(:knon, 1) & |
393 |
+ ypplay(:knon, 1))) & |
394 |
* (ypaprs(:knon, 1) - ypplay(:knon, 1)) / rg |
395 |
DO k = 2, klev |
396 |
yzlay(1:knon, k) = yzlay(1:knon, k-1) & |
397 |
+ rd * 0.5 * (yt(1:knon, k-1) + yt(1:knon, k)) & |
398 |
/ ypaprs(1:knon, k) & |
399 |
* (ypplay(1:knon, k-1) - ypplay(1:knon, k)) / rg |
400 |
END DO |
401 |
DO k = 1, klev |
402 |
yteta(1:knon, k) = yt(1:knon, k)*(ypaprs(1:knon, 1) & |
403 |
/ ypplay(1:knon, k))**rkappa * (1.+0.61*yq(1:knon, k)) |
404 |
END DO |
405 |
yzlev(1:knon, 1) = 0. |
406 |
yzlev(:knon, klev+1) = 2. * yzlay(:knon, klev) & |
407 |
- yzlay(:knon, klev - 1) |
408 |
DO k = 2, klev |
409 |
yzlev(1:knon, k) = 0.5*(yzlay(1:knon, k)+yzlay(1:knon, k-1)) |
410 |
END DO |
411 |
DO k = 1, klev + 1 |
412 |
DO j = 1, knon |
413 |
i = ni(j) |
414 |
yq2(j, k) = q2(i, k, nsrf) |
415 |
END DO |
416 |
END DO |
417 |
|
418 |
CALL ustarhb(knon, yu, yv, coefm(:knon, 1), yustar) |
419 |
IF (prt_level > 9) PRINT *, 'USTAR = ', yustar |
420 |
|
421 |
! iflag_pbl peut \^etre utilis\'e comme longueur de m\'elange |
422 |
|
423 |
IF (iflag_pbl >= 11) THEN |
424 |
CALL vdif_kcay(knon, dtime, rg, ypaprs, yzlev, yzlay, yu, yv, & |
425 |
yteta, coefm(:knon, 1), yq2, q2diag, ykmm, ykmn, yustar, & |
426 |
iflag_pbl) |
427 |
ELSE |
428 |
CALL yamada4(knon, dtime, rg, yzlev, yzlay, yu, yv, yteta, & |
429 |
coefm(:knon, 1), yq2, ykmm, ykmn, ykmq, yustar, iflag_pbl) |
430 |
END IF |
431 |
|
432 |
coefm(:knon, 2:) = ykmm(:knon, 2:klev) |
433 |
coefh(:knon, 2:) = ykmn(:knon, 2:klev) |
434 |
END IF |
435 |
|
436 |
! calculer la diffusion des vitesses "u" et "v" |
437 |
CALL clvent(knon, dtime, yu1, yv1, coefm(:knon, :), yt, yu, ypaprs, & |
438 |
ypplay, ydelp, y_d_u, y_flux_u(:knon)) |
439 |
CALL clvent(knon, dtime, yu1, yv1, coefm(:knon, :), yt, yv, ypaprs, & |
440 |
ypplay, ydelp, y_d_v, y_flux_v(:knon)) |
441 |
|
442 |
! calculer la diffusion de "q" et de "h" |
443 |
CALL clqh(dtime, jour, firstcal, rlat, nsrf, ni(:knon), & |
444 |
ytsoil(:knon, :), yqsol, rmu0, yrugos, yrugoro, yu1, yv1, & |
445 |
coefh(:knon, :), yt, yq, yts(:knon), ypaprs, ypplay, ydelp, & |
446 |
yrads, yalb(:knon), ysnow, yqsurf, yrain_f, ysnow_f, yfder, & |
447 |
yfluxlat, pctsrf_new_sic, yagesno(:knon), y_d_t, y_d_q, & |
448 |
y_d_ts(:knon), yz0_new, y_flux_t(:knon), y_flux_q(:knon), & |
449 |
y_dflux_t, y_dflux_q, y_fqcalving, y_ffonte, y_run_off_lic_0) |
450 |
|
451 |
! calculer la longueur de rugosite sur ocean |
452 |
yrugm = 0. |
453 |
IF (nsrf == is_oce) THEN |
454 |
DO j = 1, knon |
455 |
yrugm(j) = 0.018*coefm(j, 1)*(yu1(j)**2+yv1(j)**2)/rg + & |
456 |
0.11*14E-6/sqrt(coefm(j, 1)*(yu1(j)**2+yv1(j)**2)) |
457 |
yrugm(j) = max(1.5E-05, yrugm(j)) |
458 |
END DO |
459 |
END IF |
460 |
DO j = 1, knon |
461 |
y_dflux_t(j) = y_dflux_t(j)*ypct(j) |
462 |
y_dflux_q(j) = y_dflux_q(j)*ypct(j) |
463 |
yu1(j) = yu1(j)*ypct(j) |
464 |
yv1(j) = yv1(j)*ypct(j) |
465 |
END DO |
466 |
|
467 |
DO k = 1, klev |
468 |
DO j = 1, knon |
469 |
i = ni(j) |
470 |
coefh(j, k) = coefh(j, k)*ypct(j) |
471 |
coefm(j, k) = coefm(j, k)*ypct(j) |
472 |
y_d_t(j, k) = y_d_t(j, k)*ypct(j) |
473 |
y_d_q(j, k) = y_d_q(j, k)*ypct(j) |
474 |
y_d_u(j, k) = y_d_u(j, k)*ypct(j) |
475 |
y_d_v(j, k) = y_d_v(j, k)*ypct(j) |
476 |
END DO |
477 |
END DO |
478 |
|
479 |
DO j = 1, knon |
480 |
i = ni(j) |
481 |
flux_t(i, nsrf) = y_flux_t(j) |
482 |
flux_q(i, nsrf) = y_flux_q(j) |
483 |
flux_u(i, nsrf) = y_flux_u(j) |
484 |
flux_v(i, nsrf) = y_flux_v(j) |
485 |
END DO |
486 |
|
487 |
evap(:, nsrf) = -flux_q(:, nsrf) |
488 |
|
489 |
falbe(:, nsrf) = 0. |
490 |
snow(:, nsrf) = 0. |
491 |
qsurf(:, nsrf) = 0. |
492 |
rugos(:, nsrf) = 0. |
493 |
fluxlat(:, nsrf) = 0. |
494 |
DO j = 1, knon |
495 |
i = ni(j) |
496 |
d_ts(i, nsrf) = y_d_ts(j) |
497 |
falbe(i, nsrf) = yalb(j) |
498 |
snow(i, nsrf) = ysnow(j) |
499 |
qsurf(i, nsrf) = yqsurf(j) |
500 |
rugos(i, nsrf) = yz0_new(j) |
501 |
fluxlat(i, nsrf) = yfluxlat(j) |
502 |
IF (nsrf == is_oce) THEN |
503 |
rugmer(i) = yrugm(j) |
504 |
rugos(i, nsrf) = yrugm(j) |
505 |
END IF |
506 |
agesno(i, nsrf) = yagesno(j) |
507 |
fqcalving(i, nsrf) = y_fqcalving(j) |
508 |
ffonte(i, nsrf) = y_ffonte(j) |
509 |
cdragh(i) = cdragh(i) + coefh(j, 1) |
510 |
cdragm(i) = cdragm(i) + coefm(j, 1) |
511 |
dflux_t(i) = dflux_t(i) + y_dflux_t(j) |
512 |
dflux_q(i) = dflux_q(i) + y_dflux_q(j) |
513 |
zu1(i) = zu1(i) + yu1(j) |
514 |
zv1(i) = zv1(i) + yv1(j) |
515 |
END DO |
516 |
IF (nsrf == is_ter) THEN |
517 |
qsol(ni(:knon)) = yqsol(:knon) |
518 |
else IF (nsrf == is_lic) THEN |
519 |
DO j = 1, knon |
520 |
i = ni(j) |
521 |
run_off_lic_0(i) = y_run_off_lic_0(j) |
522 |
END DO |
523 |
END IF |
524 |
|
525 |
ftsoil(:, :, nsrf) = 0. |
526 |
ftsoil(ni(:knon), :, nsrf) = ytsoil(:knon, :) |
527 |
|
528 |
DO j = 1, knon |
529 |
i = ni(j) |
530 |
DO k = 1, klev |
531 |
d_t(i, k) = d_t(i, k) + y_d_t(j, k) |
532 |
d_q(i, k) = d_q(i, k) + y_d_q(j, k) |
533 |
d_u(i, k) = d_u(i, k) + y_d_u(j, k) |
534 |
d_v(i, k) = d_v(i, k) + y_d_v(j, k) |
535 |
ycoefh(i, k) = ycoefh(i, k) + coefh(j, k) |
536 |
END DO |
537 |
END DO |
538 |
|
539 |
! diagnostic t, q a 2m et u, v a 10m |
540 |
|
541 |
DO j = 1, knon |
542 |
i = ni(j) |
543 |
uzon(j) = yu(j, 1) + y_d_u(j, 1) |
544 |
vmer(j) = yv(j, 1) + y_d_v(j, 1) |
545 |
tair1(j) = yt(j, 1) + y_d_t(j, 1) |
546 |
qair1(j) = yq(j, 1) + y_d_q(j, 1) |
547 |
zgeo1(j) = rd*tair1(j)/(0.5*(ypaprs(j, 1)+ypplay(j, & |
548 |
1)))*(ypaprs(j, 1)-ypplay(j, 1)) |
549 |
tairsol(j) = yts(j) + y_d_ts(j) |
550 |
rugo1(j) = yrugos(j) |
551 |
IF (nsrf == is_oce) THEN |
552 |
rugo1(j) = rugos(i, nsrf) |
553 |
END IF |
554 |
psfce(j) = ypaprs(j, 1) |
555 |
patm(j) = ypplay(j, 1) |
556 |
|
557 |
qairsol(j) = yqsurf(j) |
558 |
END DO |
559 |
|
560 |
CALL stdlevvar(klon, knon, nsrf, zxli, uzon, vmer, tair1, qair1, & |
561 |
zgeo1, tairsol, qairsol, rugo1, psfce, patm, yt2m, yq2m, & |
562 |
yt10m, yq10m, yu10m, yustar) |
563 |
|
564 |
DO j = 1, knon |
565 |
i = ni(j) |
566 |
t2m(i, nsrf) = yt2m(j) |
567 |
q2m(i, nsrf) = yq2m(j) |
568 |
|
569 |
! u10m, v10m : composantes du vent a 10m sans spirale de Ekman |
570 |
u10m(i, nsrf) = (yu10m(j)*uzon(j))/sqrt(uzon(j)**2+vmer(j)**2) |
571 |
v10m(i, nsrf) = (yu10m(j)*vmer(j))/sqrt(uzon(j)**2+vmer(j)**2) |
572 |
END DO |
573 |
|
574 |
CALL hbtm(ypaprs, ypplay, yt2m, yq2m, yustar, y_flux_t(:knon), & |
575 |
y_flux_q(:knon), yu, yv, yt, yq, ypblh(:knon), ycapcl, & |
576 |
yoliqcl, ycteicl, ypblt, ytherm, ytrmb1, ytrmb2, ytrmb3, ylcl) |
577 |
|
578 |
DO j = 1, knon |
579 |
i = ni(j) |
580 |
pblh(i, nsrf) = ypblh(j) |
581 |
plcl(i, nsrf) = ylcl(j) |
582 |
capcl(i, nsrf) = ycapcl(j) |
583 |
oliqcl(i, nsrf) = yoliqcl(j) |
584 |
cteicl(i, nsrf) = ycteicl(j) |
585 |
pblt(i, nsrf) = ypblt(j) |
586 |
therm(i, nsrf) = ytherm(j) |
587 |
trmb1(i, nsrf) = ytrmb1(j) |
588 |
trmb2(i, nsrf) = ytrmb2(j) |
589 |
trmb3(i, nsrf) = ytrmb3(j) |
590 |
END DO |
591 |
|
592 |
DO j = 1, knon |
593 |
DO k = 1, klev + 1 |
594 |
i = ni(j) |
595 |
q2(i, k, nsrf) = yq2(j, k) |
596 |
END DO |
597 |
END DO |
598 |
end IF if_knon |
599 |
END DO loop_surface |
600 |
|
601 |
! On utilise les nouvelles surfaces |
602 |
rugos(:, is_oce) = rugmer |
603 |
pctsrf(:, is_oce) = pctsrf_new_oce |
604 |
pctsrf(:, is_sic) = pctsrf_new_sic |
605 |
|
606 |
firstcal = .false. |
607 |
|
608 |
END SUBROUTINE clmain |
609 |
|
610 |
end module clmain_m |