1 |
SUBROUTINE clmain(dtime,itap,date0,pctsrf,pctsrf_new, |
module clmain_m |
2 |
. t,q,u,v, |
|
3 |
. jour, rmu0, co2_ppm, |
IMPLICIT NONE |
4 |
. ok_veget, ocean, npas, nexca, ts, |
|
5 |
. soil_model,cdmmax, cdhmax, |
contains |
6 |
. ksta, ksta_ter, ok_kzmin, ftsoil,qsol, |
|
7 |
. paprs,pplay,snow,qsurf,evap,albe,alblw, |
SUBROUTINE clmain(dtime, pctsrf, t, q, u, v, julien, mu0, ftsol, cdmmax, & |
8 |
. fluxlat, |
cdhmax, ksta, ksta_ter, ok_kzmin, ftsoil, qsol, paprs, pplay, fsnow, & |
9 |
. rain_f, snow_f, solsw, sollw, sollwdown, fder, |
qsurf, evap, falbe, fluxlat, rain_fall, snow_f, fsolsw, fsollw, frugs, & |
10 |
. rlon, rlat, cufi, cvfi, rugos, |
agesno, rugoro, d_t, d_q, d_u, d_v, d_ts, flux_t, flux_q, flux_u, & |
11 |
. debut, lafin, agesno,rugoro, |
flux_v, cdragh, cdragm, q2, dflux_t, dflux_q, ycoefh, t2m, q2m, & |
12 |
. d_t,d_q,d_u,d_v,d_ts, |
u10m_srf, v10m_srf, pblh, capcl, oliqcl, cteicl, pblt, therm, trmb1, & |
13 |
. flux_t,flux_q,flux_u,flux_v,cdragh,cdragm, |
trmb2, trmb3, plcl, fqcalving, ffonte, run_off_lic_0) |
14 |
. q2, |
|
15 |
. dflux_t,dflux_q, |
! From phylmd/clmain.F, version 1.6, 2005/11/16 14:47:19 |
16 |
. zcoefh,zu1,zv1, t2m, q2m, u10m, v10m, |
! Author: Z. X. Li (LMD/CNRS), date: 1993/08/18 |
17 |
cIM cf. AM : pbl |
! Objet : interface de couche limite (diffusion verticale) |
18 |
. pblh,capCL,oliqCL,cteiCL,pblT, |
|
19 |
. therm,trmb1,trmb2,trmb3,plcl, |
! Tout ce qui a trait aux traceurs est dans "phytrac". Le calcul |
20 |
. fqcalving,ffonte, run_off_lic_0, |
! de la couche limite pour les traceurs se fait avec "cltrac" et |
21 |
cIM "slab" ocean |
! ne tient pas compte de la diff\'erentiation des sous-fractions |
22 |
. flux_o, flux_g, tslab, seaice) |
! de sol. |
23 |
|
|
24 |
! |
use clqh_m, only: clqh |
25 |
! $Header: /home/cvsroot/LMDZ4/libf/phylmd/clmain.F,v 1.6 2005/11/16 14:47:19 lmdzadmin Exp $ |
use clvent_m, only: clvent |
26 |
! |
use coefkz_m, only: coefkz |
27 |
c |
use coefkzmin_m, only: coefkzmin |
28 |
c |
USE conf_gcm_m, ONLY: lmt_pas |
29 |
cAA REM: |
USE conf_phys_m, ONLY: iflag_pbl |
30 |
cAA----- |
USE dimphy, ONLY: klev, klon, zmasq |
31 |
cAA Tout ce qui a trait au traceurs est dans phytrac maintenant |
USE dimsoil, ONLY: nsoilmx |
32 |
cAA pour l'instant le calcul de la couche limite pour les traceurs |
use hbtm_m, only: hbtm |
33 |
cAA se fait avec cltrac et ne tient pas compte de la differentiation |
USE indicesol, ONLY: epsfra, is_lic, is_oce, is_sic, is_ter, nbsrf |
34 |
cAA des sous-fraction de sol. |
USE interfoce_lim_m, ONLY: interfoce_lim |
35 |
cAA REM bis : |
use stdlevvar_m, only: stdlevvar |
36 |
cAA---------- |
USE suphec_m, ONLY: rd, rg, rkappa |
37 |
cAA Pour pouvoir extraire les coefficient d'echanges et le vent |
use time_phylmdz, only: itap |
38 |
cAA dans la premiere couche, 3 champs supplementaires ont ete crees |
use ustarhb_m, only: ustarhb |
39 |
cAA zcoefh,zu1 et zv1. Pour l'instant nous avons moyenne les valeurs |
use vdif_kcay_m, only: vdif_kcay |
40 |
cAA de ces trois champs sur les 4 subsurfaces du modele. Dans l'avenir |
use yamada4_m, only: yamada4 |
41 |
cAA si les informations des subsurfaces doivent etre prises en compte |
|
42 |
cAA il faudra sortir ces memes champs en leur ajoutant une dimension, |
REAL, INTENT(IN):: dtime ! interval du temps (secondes) |
43 |
cAA c'est a dire nbsrf (nbre de subsurface). |
|
44 |
USE ioipsl |
REAL, INTENT(inout):: pctsrf(klon, nbsrf) |
45 |
USE interface_surf |
! tableau des pourcentages de surface de chaque maille |
46 |
use dimens_m |
|
47 |
use indicesol |
REAL, INTENT(IN):: t(klon, klev) ! temperature (K) |
48 |
use dimphy |
REAL, INTENT(IN):: q(klon, klev) ! vapeur d'eau (kg / kg) |
49 |
use dimsoil |
REAL, INTENT(IN):: u(klon, klev), v(klon, klev) ! vitesse |
50 |
use temps |
INTEGER, INTENT(IN):: julien ! jour de l'annee en cours |
51 |
use iniprint |
REAL, intent(in):: mu0(klon) ! cosinus de l'angle solaire zenithal |
52 |
use YOMCST |
REAL, INTENT(IN):: ftsol(:, :) ! (klon, nbsrf) temp\'erature du sol (en K) |
53 |
use yoethf |
REAL, INTENT(IN):: cdmmax, cdhmax ! seuils cdrm, cdrh |
54 |
use fcttre |
REAL, INTENT(IN):: ksta, ksta_ter |
55 |
use conf_phys_m |
LOGICAL, INTENT(IN):: ok_kzmin |
56 |
use gath_cpl, only: gath2cpl |
|
57 |
IMPLICIT none |
REAL, INTENT(inout):: ftsoil(klon, nsoilmx, nbsrf) |
58 |
c====================================================================== |
! soil temperature of surface fraction |
59 |
c Auteur(s) Z.X. Li (LMD/CNRS) date: 19930818 |
|
60 |
c Objet: interface de "couche limite" (diffusion verticale) |
REAL, INTENT(inout):: qsol(:) ! (klon) |
61 |
c Arguments: |
! column-density of water in soil, in kg m-2 |
62 |
c dtime----input-R- interval du temps (secondes) |
|
63 |
c itap-----input-I- numero du pas de temps |
REAL, INTENT(IN):: paprs(klon, klev + 1) ! pression a intercouche (Pa) |
64 |
c date0----input-R- jour initial |
REAL, INTENT(IN):: pplay(klon, klev) ! pression au milieu de couche (Pa) |
65 |
c t--------input-R- temperature (K) |
REAL, INTENT(inout):: fsnow(:, :) ! (klon, nbsrf) \'epaisseur neigeuse |
66 |
c q--------input-R- vapeur d'eau (kg/kg) |
REAL qsurf(klon, nbsrf) |
67 |
c u--------input-R- vitesse u |
REAL evap(klon, nbsrf) |
68 |
c v--------input-R- vitesse v |
REAL, intent(inout):: falbe(klon, nbsrf) |
69 |
c ts-------input-R- temperature du sol (en Kelvin) |
REAL, intent(out):: fluxlat(:, :) ! (klon, nbsrf) |
70 |
c paprs----input-R- pression a intercouche (Pa) |
|
71 |
c pplay----input-R- pression au milieu de couche (Pa) |
REAL, intent(in):: rain_fall(klon) |
72 |
c radsol---input-R- flux radiatif net (positif vers le sol) en W/m**2 |
! liquid water mass flux (kg / m2 / s), positive down |
73 |
c rlat-----input-R- latitude en degree |
|
74 |
c rugos----input-R- longeur de rugosite (en m) |
REAL, intent(in):: snow_f(klon) |
75 |
c cufi-----input-R- resolution des mailles en x (m) |
! solid water mass flux (kg / m2 / s), positive down |
76 |
c cvfi-----input-R- resolution des mailles en y (m) |
|
77 |
c |
REAL, INTENT(IN):: fsolsw(klon, nbsrf), fsollw(klon, nbsrf) |
78 |
c d_t------output-R- le changement pour "t" |
REAL, intent(inout):: frugs(klon, nbsrf) ! longueur de rugosit\'e (en m) |
79 |
c d_q------output-R- le changement pour "q" |
real agesno(klon, nbsrf) |
80 |
c d_u------output-R- le changement pour "u" |
REAL, INTENT(IN):: rugoro(klon) |
81 |
c d_v------output-R- le changement pour "v" |
|
82 |
c d_ts-----output-R- le changement pour "ts" |
REAL d_t(klon, klev), d_q(klon, klev) |
83 |
c flux_t---output-R- flux de chaleur sensible (CpT) J/m**2/s (W/m**2) |
! d_t------output-R- le changement pour "t" |
84 |
c (orientation positive vers le bas) |
! d_q------output-R- le changement pour "q" |
85 |
c flux_q---output-R- flux de vapeur d'eau (kg/m**2/s) |
|
86 |
c flux_u---output-R- tension du vent X: (kg m/s)/(m**2 s) ou Pascal |
REAL, intent(out):: d_u(klon, klev), d_v(klon, klev) |
87 |
c flux_v---output-R- tension du vent Y: (kg m/s)/(m**2 s) ou Pascal |
! changement pour "u" et "v" |
88 |
c dflux_t derive du flux sensible |
|
89 |
c dflux_q derive du flux latent |
REAL, intent(out):: d_ts(:, :) ! (klon, nbsrf) variation of ftsol |
90 |
cIM "slab" ocean |
|
91 |
c flux_g---output-R- flux glace (pour OCEAN='slab ') |
REAL, intent(out):: flux_t(klon, nbsrf) |
92 |
c flux_o---output-R- flux ocean (pour OCEAN='slab ') |
! flux de chaleur sensible (Cp T) (W / m2) (orientation positive vers |
93 |
c tslab-in/output-R temperature du slab ocean (en Kelvin) ! uniqmnt pour slab |
! le bas) Ã la surface |
94 |
c seaice---output-R- glace de mer (kg/m2) (pour OCEAN='slab ') |
|
95 |
ccc |
REAL, intent(out):: flux_q(klon, nbsrf) |
96 |
c ffonte----Flux thermique utilise pour fondre la neige |
! flux de vapeur d'eau (kg / m2 / s) Ã la surface |
97 |
c fqcalving-Flux d'eau "perdue" par la surface et necessaire pour limiter la |
|
98 |
c hauteur de neige, en kg/m2/s |
REAL, intent(out):: flux_u(klon, nbsrf), flux_v(klon, nbsrf) |
99 |
cAA on rajoute en output yu1 et yv1 qui sont les vents dans |
! tension du vent à la surface, en Pa |
100 |
cAA la premiere couche |
|
101 |
cAA ces 4 variables sont maintenant traites dans phytrac |
REAL, INTENT(out):: cdragh(klon), cdragm(klon) |
102 |
c itr--------input-I- nombre de traceurs |
real q2(klon, klev + 1, nbsrf) |
103 |
c tr---------input-R- q. de traceurs |
|
104 |
c flux_surf--input-R- flux de traceurs a la surface |
REAL, INTENT(out):: dflux_t(klon), dflux_q(klon) |
105 |
c d_tr-------output-R tendance de traceurs |
! dflux_t derive du flux sensible |
106 |
cIM cf. AM : PBL |
! dflux_q derive du flux latent |
107 |
c trmb1-------deep_cape |
! IM "slab" ocean |
108 |
c trmb2--------inhibition |
|
109 |
c trmb3-------Point Omega |
REAL, intent(out):: ycoefh(klon, klev) |
110 |
c Cape(klon)-------Cape du thermique |
! Pour pouvoir extraire les coefficients d'\'echange, le champ |
111 |
c EauLiq(klon)-------Eau liqu integr du thermique |
! "ycoefh" a \'et\'e cr\'e\'e. Nous avons moyenn\'e les valeurs de |
112 |
c ctei(klon)-------Critere d'instab d'entrainmt des nuages de CL |
! ce champ sur les quatre sous-surfaces du mod\`ele. |
113 |
c lcl------- Niveau de condensation |
|
114 |
c pblh------- HCL |
REAL, INTENT(inout):: t2m(klon, nbsrf), q2m(klon, nbsrf) |
115 |
c pblT------- T au nveau HCL |
|
116 |
c====================================================================== |
REAL, INTENT(inout):: u10m_srf(:, :), v10m_srf(:, :) ! (klon, nbsrf) |
117 |
c$$$ PB ajout pour soil |
! composantes du vent \`a 10m sans spirale d'Ekman |
118 |
c |
|
119 |
REAL, intent(in):: dtime |
! Ionela Musat. Cf. Anne Mathieu : planetary boundary layer, hbtm. |
120 |
real date0 |
! Comme les autres diagnostics on cumule dans physiq ce qui permet |
121 |
integer, intent(in):: itap |
! de sortir les grandeurs par sous-surface. |
122 |
REAL t(klon,klev), q(klon,klev) |
REAL pblh(klon, nbsrf) ! height of planetary boundary layer |
123 |
REAL u(klon,klev), v(klon,klev) |
REAL capcl(klon, nbsrf) |
124 |
cIM 230604 BAD REAL radsol(klon) ??? |
REAL oliqcl(klon, nbsrf) |
125 |
REAL, intent(in):: paprs(klon,klev+1) |
REAL cteicl(klon, nbsrf) |
126 |
real, intent(in):: pplay(klon,klev) |
REAL, INTENT(inout):: pblt(klon, nbsrf) ! T au nveau HCL |
127 |
REAL, intent(in):: rlon(klon), rlat(klon) |
REAL therm(klon, nbsrf) |
128 |
real cufi(klon), cvfi(klon) |
REAL trmb1(klon, nbsrf) |
129 |
REAL d_t(klon, klev), d_q(klon, klev) |
! trmb1-------deep_cape |
130 |
REAL d_u(klon, klev), d_v(klon, klev) |
REAL trmb2(klon, nbsrf) |
131 |
REAL flux_t(klon,klev, nbsrf), flux_q(klon,klev, nbsrf) |
! trmb2--------inhibition |
132 |
REAL dflux_t(klon), dflux_q(klon) |
REAL trmb3(klon, nbsrf) |
133 |
cIM "slab" ocean |
! trmb3-------Point Omega |
134 |
REAL flux_o(klon), flux_g(klon) |
REAL plcl(klon, nbsrf) |
135 |
REAL y_flux_o(klon), y_flux_g(klon) |
REAL fqcalving(klon, nbsrf), ffonte(klon, nbsrf) |
136 |
REAL tslab(klon), ytslab(klon) |
! ffonte----Flux thermique utilise pour fondre la neige |
137 |
REAL seaice(klon), y_seaice(klon) |
! fqcalving-Flux d'eau "perdue" par la surface et necessaire pour limiter la |
138 |
cIM cf JLD |
! hauteur de neige, en kg / m2 / s |
139 |
REAL y_fqcalving(klon), y_ffonte(klon) |
REAL run_off_lic_0(klon) |
140 |
REAL fqcalving(klon,nbsrf), ffonte(klon,nbsrf) |
|
141 |
REAL run_off_lic_0(klon), y_run_off_lic_0(klon) |
! Local: |
142 |
|
|
143 |
REAL flux_u(klon,klev, nbsrf), flux_v(klon,klev, nbsrf) |
LOGICAL:: firstcal = .true. |
144 |
REAL rugmer(klon), agesno(klon,nbsrf) |
|
145 |
real, intent(in):: rugoro(klon) |
! la nouvelle repartition des surfaces sortie de l'interface |
146 |
REAL cdragh(klon), cdragm(klon) |
REAL, save:: pctsrf_new_oce(klon) |
147 |
integer jour ! jour de l'annee en cours |
REAL, save:: pctsrf_new_sic(klon) |
148 |
real rmu0(klon) ! cosinus de l'angle solaire zenithal |
|
149 |
REAL co2_ppm ! taux CO2 atmosphere |
REAL y_fqcalving(klon), y_ffonte(klon) |
150 |
LOGICAL, intent(in):: debut |
real y_run_off_lic_0(klon) |
151 |
logical, intent(in):: lafin |
REAL rugmer(klon) |
152 |
logical ok_veget |
REAL ytsoil(klon, nsoilmx) |
153 |
character(len=*), intent(IN):: ocean |
REAL yts(klon), yrugos(klon), ypct(klon), yz0_new(klon) |
154 |
integer npas, nexca |
REAL yalb(klon) |
155 |
c |
REAL snow(klon), yqsurf(klon), yagesno(klon) |
156 |
REAL pctsrf(klon,nbsrf) |
real yqsol(klon) ! column-density of water in soil, in kg m-2 |
157 |
REAL ts(klon,nbsrf) |
REAL yrain_f(klon) ! liquid water mass flux (kg / m2 / s), positive down |
158 |
REAL d_ts(klon,nbsrf) |
REAL ysnow_f(klon) ! solid water mass flux (kg / m2 / s), positive down |
159 |
REAL snow(klon,nbsrf) |
REAL yrugm(klon), yrads(klon), yrugoro(klon) |
160 |
REAL qsurf(klon,nbsrf) |
REAL yfluxlat(klon) |
161 |
REAL evap(klon,nbsrf) |
REAL y_d_ts(klon) |
162 |
REAL albe(klon,nbsrf) |
REAL y_d_t(klon, klev), y_d_q(klon, klev) |
163 |
REAL alblw(klon,nbsrf) |
REAL y_d_u(klon, klev), y_d_v(klon, klev) |
164 |
c$$$ PB |
REAL y_flux_t(klon), y_flux_q(klon) |
165 |
REAL fluxlat(klon,nbsrf) |
REAL y_flux_u(klon), y_flux_v(klon) |
166 |
C |
REAL y_dflux_t(klon), y_dflux_q(klon) |
167 |
real rain_f(klon), snow_f(klon) |
REAL coefh(klon, klev), coefm(klon, klev) |
168 |
REAL fder(klon) |
REAL yu(klon, klev), yv(klon, klev) |
169 |
cIM cf. JLD REAL sollw(klon), solsw(klon), sollwdown(klon) |
REAL yt(klon, klev), yq(klon, klev) |
170 |
REAL sollw(klon,nbsrf), solsw(klon,nbsrf), sollwdown(klon) |
REAL ypaprs(klon, klev + 1), ypplay(klon, klev), ydelp(klon, klev) |
171 |
REAL rugos(klon,nbsrf) |
|
172 |
C la nouvelle repartition des surfaces sortie de l'interface |
REAL ycoefm0(klon, klev), ycoefh0(klon, klev) |
173 |
REAL pctsrf_new(klon,nbsrf) |
|
174 |
cAA |
REAL yzlay(klon, klev), zlev(klon, klev + 1), yteta(klon, klev) |
175 |
REAL zcoefh(klon,klev) |
REAL ykmm(klon, klev + 1), ykmn(klon, klev + 1) |
176 |
REAL zu1(klon) |
REAL ykmq(klon, klev + 1) |
177 |
REAL zv1(klon) |
REAL yq2(klon, klev + 1) |
178 |
cAA |
REAL q2diag(klon, klev + 1) |
179 |
c$$$ PB ajout pour soil |
|
180 |
LOGICAL, intent(in):: soil_model |
REAL delp(klon, klev) |
181 |
cIM ajout seuils cdrm, cdrh |
INTEGER i, k, nsrf |
182 |
REAL cdmmax, cdhmax |
|
183 |
cIM: 261103 |
INTEGER ni(klon), knon, j |
184 |
REAL ksta, ksta_ter |
|
185 |
LOGICAL ok_kzmin |
REAL pctsrf_pot(klon, nbsrf) |
186 |
cIM: 261103 |
! "pourcentage potentiel" pour tenir compte des \'eventuelles |
187 |
REAL ftsoil(klon,nsoilmx,nbsrf) |
! apparitions ou disparitions de la glace de mer |
188 |
REAL ytsoil(klon,nsoilmx) |
|
189 |
REAL qsol(klon) |
REAL yt2m(klon), yq2m(klon), wind10m(klon) |
190 |
c====================================================================== |
REAL ustar(klon) |
191 |
EXTERNAL clqh, clvent, coefkz, calbeta, cltrac |
|
192 |
c====================================================================== |
REAL yt10m(klon), yq10m(klon) |
193 |
REAL yts(klon), yrugos(klon), ypct(klon), yz0_new(klon) |
REAL ypblh(klon) |
194 |
REAL yalb(klon) |
REAL ylcl(klon) |
195 |
REAL yalblw(klon) |
REAL ycapcl(klon) |
196 |
REAL yu1(klon), yv1(klon) |
REAL yoliqcl(klon) |
197 |
real ysnow(klon), yqsurf(klon), yagesno(klon), yqsol(klon) |
REAL ycteicl(klon) |
198 |
real yrain_f(klon), ysnow_f(klon) |
REAL ypblt(klon) |
199 |
real ysollw(klon), ysolsw(klon), ysollwdown(klon) |
REAL ytherm(klon) |
200 |
real yfder(klon), ytaux(klon), ytauy(klon) |
REAL ytrmb1(klon) |
201 |
REAL yrugm(klon), yrads(klon),yrugoro(klon) |
REAL ytrmb2(klon) |
202 |
c$$$ PB |
REAL ytrmb3(klon) |
203 |
REAL yfluxlat(klon) |
REAL u1(klon), v1(klon) |
204 |
C |
REAL tair1(klon), qair1(klon), tairsol(klon) |
205 |
REAL y_d_ts(klon) |
REAL psfce(klon), patm(klon) |
206 |
REAL y_d_t(klon, klev), y_d_q(klon, klev) |
|
207 |
REAL y_d_u(klon, klev), y_d_v(klon, klev) |
REAL qairsol(klon), zgeo1(klon) |
208 |
REAL y_flux_t(klon,klev), y_flux_q(klon,klev) |
REAL rugo1(klon) |
209 |
REAL y_flux_u(klon,klev), y_flux_v(klon,klev) |
|
210 |
REAL y_dflux_t(klon), y_dflux_q(klon) |
!------------------------------------------------------------ |
211 |
REAL ycoefh(klon,klev), ycoefm(klon,klev) |
|
212 |
REAL yu(klon,klev), yv(klon,klev) |
ytherm = 0. |
213 |
REAL yt(klon,klev), yq(klon,klev) |
|
214 |
REAL ypaprs(klon,klev+1), ypplay(klon,klev), ydelp(klon,klev) |
DO k = 1, klev ! epaisseur de couche |
215 |
c |
DO i = 1, klon |
216 |
LOGICAL ok_nonloc |
delp(i, k) = paprs(i, k) - paprs(i, k + 1) |
217 |
PARAMETER (ok_nonloc=.FALSE.) |
END DO |
218 |
REAL ycoefm0(klon,klev), ycoefh0(klon,klev) |
END DO |
219 |
|
|
220 |
cIM 081204 hcl_Anne ? BEG |
! Initialization: |
221 |
real yzlay(klon,klev),yzlev(klon,klev+1),yteta(klon,klev) |
rugmer = 0. |
222 |
real ykmm(klon,klev+1),ykmn(klon,klev+1) |
cdragh = 0. |
223 |
real ykmq(klon,klev+1) |
cdragm = 0. |
224 |
real yq2(klon,klev+1),q2(klon,klev+1,nbsrf) |
dflux_t = 0. |
225 |
real q2diag(klon,klev+1) |
dflux_q = 0. |
226 |
cIM 081204 real yustar(klon),y_cd_m(klon),y_cd_h(klon) |
ypct = 0. |
227 |
cIM 081204 hcl_Anne ? END |
yqsurf = 0. |
228 |
c |
yrain_f = 0. |
229 |
REAL u1lay(klon), v1lay(klon) |
ysnow_f = 0. |
230 |
REAL delp(klon,klev) |
yrugos = 0. |
231 |
INTEGER i, k, nsrf |
ypaprs = 0. |
232 |
cAA INTEGER it |
ypplay = 0. |
233 |
INTEGER ni(klon), knon, j |
ydelp = 0. |
234 |
c Introduction d'une variable "pourcentage potentiel" pour tenir compte |
yu = 0. |
235 |
c des eventuelles apparitions et/ou disparitions de la glace de mer |
yv = 0. |
236 |
REAL pctsrf_pot(klon,nbsrf) |
yt = 0. |
237 |
|
yq = 0. |
238 |
c====================================================================== |
y_dflux_t = 0. |
239 |
REAL zx_alf1, zx_alf2 !valeur ambiante par extrapola. |
y_dflux_q = 0. |
240 |
c====================================================================== |
yrugoro = 0. |
241 |
c |
d_ts = 0. |
242 |
c maf pour sorties IOISPL en cas de debugagage |
flux_t = 0. |
243 |
c |
flux_q = 0. |
244 |
CHARACTER*80 cldebug |
flux_u = 0. |
245 |
SAVE cldebug |
flux_v = 0. |
246 |
CHARACTER*8 cl_surf(nbsrf) |
fluxlat = 0. |
247 |
SAVE cl_surf |
d_t = 0. |
248 |
INTEGER nhoridbg, nidbg |
d_q = 0. |
249 |
SAVE nhoridbg, nidbg |
d_u = 0. |
250 |
INTEGER ndexbg(iim*(jjm+1)) |
d_v = 0. |
251 |
REAL zx_lon(iim,jjm+1), zx_lat(iim,jjm+1), zjulian |
ycoefh = 0. |
252 |
REAL tabindx(klon) |
|
253 |
REAL debugtab(iim,jjm+1) |
! Initialisation des "pourcentages potentiels". On consid\`ere ici qu'on |
254 |
LOGICAL first_appel |
! peut avoir potentiellement de la glace sur tout le domaine oc\'eanique |
255 |
SAVE first_appel |
! (\`a affiner) |
256 |
DATA first_appel/.true./ |
|
257 |
LOGICAL:: debugindex = .false. |
pctsrf_pot(:, is_ter) = pctsrf(:, is_ter) |
258 |
integer idayref |
pctsrf_pot(:, is_lic) = pctsrf(:, is_lic) |
259 |
REAL t2m(klon,nbsrf), q2m(klon,nbsrf) |
pctsrf_pot(:, is_oce) = 1. - zmasq |
260 |
REAL u10m(klon,nbsrf), v10m(klon,nbsrf) |
pctsrf_pot(:, is_sic) = 1. - zmasq |
261 |
c |
|
262 |
REAL yt2m(klon), yq2m(klon), yu10m(klon) |
! Tester si c'est le moment de lire le fichier: |
263 |
REAL yustar(klon) |
if (mod(itap - 1, lmt_pas) == 0) then |
264 |
c -- LOOP |
CALL interfoce_lim(julien, pctsrf_new_oce, pctsrf_new_sic) |
265 |
REAL yu10mx(klon) |
endif |
266 |
REAL yu10my(klon) |
|
267 |
REAL ywindsp(klon) |
! Boucler sur toutes les sous-fractions du sol: |
268 |
c -- LOOP |
|
269 |
c |
loop_surface: DO nsrf = 1, nbsrf |
270 |
REAL yt10m(klon), yq10m(klon) |
! Chercher les indices : |
271 |
cIM cf. AM : pbl, hbtm2 (Comme les autres diagnostics on cumule ds physic ce qui |
ni = 0 |
272 |
c permet de sortir les grdeurs par sous surface) |
knon = 0 |
273 |
REAL pblh(klon,nbsrf) |
DO i = 1, klon |
274 |
REAL plcl(klon,nbsrf) |
! Pour d\'eterminer le domaine \`a traiter, on utilise les surfaces |
275 |
REAL capCL(klon,nbsrf) |
! "potentielles" |
276 |
REAL oliqCL(klon,nbsrf) |
IF (pctsrf_pot(i, nsrf) > epsfra) THEN |
277 |
REAL cteiCL(klon,nbsrf) |
knon = knon + 1 |
278 |
REAL pblT(klon,nbsrf) |
ni(knon) = i |
279 |
REAL therm(klon,nbsrf) |
END IF |
280 |
REAL trmb1(klon,nbsrf) |
END DO |
281 |
REAL trmb2(klon,nbsrf) |
|
282 |
REAL trmb3(klon,nbsrf) |
if_knon: IF (knon /= 0) then |
283 |
REAL ypblh(klon) |
DO j = 1, knon |
284 |
REAL ylcl(klon) |
i = ni(j) |
285 |
REAL ycapCL(klon) |
ypct(j) = pctsrf(i, nsrf) |
286 |
REAL yoliqCL(klon) |
yts(j) = ftsol(i, nsrf) |
287 |
REAL ycteiCL(klon) |
snow(j) = fsnow(i, nsrf) |
288 |
REAL ypblT(klon) |
yqsurf(j) = qsurf(i, nsrf) |
289 |
REAL ytherm(klon) |
yalb(j) = falbe(i, nsrf) |
290 |
REAL ytrmb1(klon) |
yrain_f(j) = rain_fall(i) |
291 |
REAL ytrmb2(klon) |
ysnow_f(j) = snow_f(i) |
292 |
REAL ytrmb3(klon) |
yagesno(j) = agesno(i, nsrf) |
293 |
REAL y_cd_h(klon), y_cd_m(klon) |
yrugos(j) = frugs(i, nsrf) |
294 |
c REAL ygamt(klon,2:klev) ! contre-gradient pour temperature |
yrugoro(j) = rugoro(i) |
295 |
c REAL ygamq(klon,2:klev) ! contre-gradient pour humidite |
yrads(j) = fsolsw(i, nsrf) + fsollw(i, nsrf) |
296 |
REAL uzon(klon), vmer(klon) |
ypaprs(j, klev + 1) = paprs(i, klev + 1) |
297 |
REAL tair1(klon), qair1(klon), tairsol(klon) |
y_run_off_lic_0(j) = run_off_lic_0(i) |
|
REAL psfce(klon), patm(klon) |
|
|
c |
|
|
REAL qairsol(klon), zgeo1(klon) |
|
|
REAL rugo1(klon) |
|
|
c |
|
|
LOGICAL zxli ! utiliser un jeu de fonctions simples |
|
|
PARAMETER (zxli=.FALSE.) |
|
|
c |
|
|
REAL zt, zqs, zdelta, zcor |
|
|
REAL t_coup |
|
|
PARAMETER(t_coup=273.15) |
|
|
C |
|
|
character (len = 20) :: modname = 'clmain' |
|
|
LOGICAL check |
|
|
PARAMETER (check=.false.) |
|
|
|
|
|
|
|
|
c initialisation Anne |
|
|
ytherm(:) = 0. |
|
|
C |
|
|
if (check) THEN |
|
|
write(*,*) modname,' klon=',klon |
|
|
CC call flush(6) |
|
|
endif |
|
|
IF (debugindex .and. first_appel) THEN |
|
|
first_appel=.false. |
|
|
! |
|
|
! initialisation sorties netcdf |
|
|
! |
|
|
idayref = day_ini |
|
|
CALL ymds2ju(annee_ref, 1, idayref, 0.0, zjulian) |
|
|
CALL gr_fi_ecrit(1,klon,iim,jjm+1,rlon,zx_lon) |
|
|
DO i = 1, iim |
|
|
zx_lon(i,1) = rlon(i+1) |
|
|
zx_lon(i,jjm+1) = rlon(i+1) |
|
|
ENDDO |
|
|
CALL gr_fi_ecrit(1,klon,iim,jjm+1,rlat,zx_lat) |
|
|
cldebug='sous_index' |
|
|
CALL histbeg_totreg(cldebug, iim,zx_lon(:,1),jjm+1, |
|
|
$ zx_lat(1,:),1,iim,1,jjm |
|
|
$ +1, itau_phy,zjulian,dtime,nhoridbg,nidbg) |
|
|
! no vertical axis |
|
|
cl_surf(1)='ter' |
|
|
cl_surf(2)='lic' |
|
|
cl_surf(3)='oce' |
|
|
cl_surf(4)='sic' |
|
|
DO nsrf=1,nbsrf |
|
|
CALL histdef(nidbg, cl_surf(nsrf),cl_surf(nsrf), "-",iim, |
|
|
$ jjm+1,nhoridbg, 1, 1, 1, -99, 32, "inst", dtime,dtime) |
|
298 |
END DO |
END DO |
299 |
CALL histend(nidbg) |
|
300 |
CALL histsync(nidbg) |
! For continent, copy soil water content |
301 |
ENDIF |
IF (nsrf == is_ter) yqsol(:knon) = qsol(ni(:knon)) |
302 |
|
|
303 |
|
ytsoil(:knon, :) = ftsoil(ni(:knon), :, nsrf) |
304 |
|
|
305 |
|
DO k = 1, klev |
306 |
|
DO j = 1, knon |
307 |
|
i = ni(j) |
308 |
|
ypaprs(j, k) = paprs(i, k) |
309 |
|
ypplay(j, k) = pplay(i, k) |
310 |
|
ydelp(j, k) = delp(i, k) |
311 |
|
yu(j, k) = u(i, k) |
312 |
|
yv(j, k) = v(i, k) |
313 |
|
yt(j, k) = t(i, k) |
314 |
|
yq(j, k) = q(i, k) |
315 |
|
END DO |
316 |
|
END DO |
317 |
|
|
318 |
|
! calculer Cdrag et les coefficients d'echange |
319 |
|
CALL coefkz(nsrf, ypaprs, ypplay, ksta, ksta_ter, yts(:knon), & |
320 |
|
yrugos, yu, yv, yt, yq, yqsurf(:knon), coefm(:knon, :), & |
321 |
|
coefh(:knon, :)) |
322 |
|
|
323 |
DO k = 1, klev ! epaisseur de couche |
IF (iflag_pbl == 1) THEN |
324 |
DO i = 1, klon |
CALL coefkz2(nsrf, knon, ypaprs, ypplay, yt, ycoefm0, ycoefh0) |
325 |
delp(i,k) = paprs(i,k)-paprs(i,k+1) |
coefm(:knon, :) = max(coefm(:knon, :), ycoefm0(:knon, :)) |
326 |
ENDDO |
coefh(:knon, :) = max(coefh(:knon, :), ycoefh0(:knon, :)) |
327 |
ENDDO |
END IF |
328 |
DO i = 1, klon ! vent de la premiere couche |
|
329 |
zx_alf1 = 1.0 |
! on met un seuil pour coefm et coefh |
330 |
zx_alf2 = 1.0 - zx_alf1 |
IF (nsrf == is_oce) THEN |
331 |
u1lay(i) = u(i,1)*zx_alf1 + u(i,2)*zx_alf2 |
coefm(:knon, 1) = min(coefm(:knon, 1), cdmmax) |
332 |
v1lay(i) = v(i,1)*zx_alf1 + v(i,2)*zx_alf2 |
coefh(:knon, 1) = min(coefh(:knon, 1), cdhmax) |
333 |
ENDDO |
END IF |
334 |
c |
|
335 |
c initialisation: |
IF (ok_kzmin) THEN |
336 |
c |
! Calcul d'une diffusion minimale pour les conditions tres stables |
337 |
DO i = 1, klon |
CALL coefkzmin(knon, ypaprs, ypplay, yu, yv, yt, yq, & |
338 |
rugmer(i) = 0.0 |
coefm(:knon, 1), ycoefm0, ycoefh0) |
339 |
cdragh(i) = 0.0 |
coefm(:knon, :) = max(coefm(:knon, :), ycoefm0(:knon, :)) |
340 |
cdragm(i) = 0.0 |
coefh(:knon, :) = max(coefh(:knon, :), ycoefh0(:knon, :)) |
341 |
dflux_t(i) = 0.0 |
END IF |
342 |
dflux_q(i) = 0.0 |
|
343 |
zu1(i) = 0.0 |
IF (iflag_pbl >= 3) THEN |
344 |
zv1(i) = 0.0 |
! Mellor et Yamada adapt\'e \`a Mars, Richard Fournier et |
345 |
ENDDO |
! Fr\'ed\'eric Hourdin |
346 |
ypct = 0.0 |
yzlay(:knon, 1) = rd * yt(:knon, 1) / (0.5 * (ypaprs(:knon, 1) & |
347 |
yts = 0.0 |
+ ypplay(:knon, 1))) & |
348 |
ysnow = 0.0 |
* (ypaprs(:knon, 1) - ypplay(:knon, 1)) / rg |
349 |
yqsurf = 0.0 |
|
350 |
yalb = 0.0 |
DO k = 2, klev |
351 |
yalblw = 0.0 |
yzlay(:knon, k) = yzlay(:knon, k-1) & |
352 |
yrain_f = 0.0 |
+ rd * 0.5 * (yt(1:knon, k-1) + yt(1:knon, k)) & |
353 |
ysnow_f = 0.0 |
/ ypaprs(1:knon, k) & |
354 |
yfder = 0.0 |
* (ypplay(1:knon, k-1) - ypplay(1:knon, k)) / rg |
355 |
ytaux = 0.0 |
END DO |
356 |
ytauy = 0.0 |
|
357 |
ysolsw = 0.0 |
DO k = 1, klev |
358 |
ysollw = 0.0 |
yteta(1:knon, k) = yt(1:knon, k) * (ypaprs(1:knon, 1) & |
359 |
ysollwdown = 0.0 |
/ ypplay(1:knon, k))**rkappa * (1. + 0.61 * yq(1:knon, k)) |
360 |
yrugos = 0.0 |
END DO |
361 |
yu1 = 0.0 |
|
362 |
yv1 = 0.0 |
zlev(:knon, 1) = 0. |
363 |
yrads = 0.0 |
zlev(:knon, klev + 1) = 2. * yzlay(:knon, klev) & |
364 |
ypaprs = 0.0 |
- yzlay(:knon, klev - 1) |
365 |
ypplay = 0.0 |
|
366 |
ydelp = 0.0 |
DO k = 2, klev |
367 |
yu = 0.0 |
zlev(:knon, k) = 0.5 * (yzlay(:knon, k) + yzlay(:knon, k-1)) |
368 |
yv = 0.0 |
END DO |
369 |
yt = 0.0 |
|
370 |
yq = 0.0 |
DO k = 1, klev + 1 |
371 |
pctsrf_new = 0.0 |
DO j = 1, knon |
372 |
y_flux_u = 0.0 |
i = ni(j) |
373 |
y_flux_v = 0.0 |
yq2(j, k) = q2(i, k, nsrf) |
374 |
C$$ PB |
END DO |
375 |
y_dflux_t = 0.0 |
END DO |
376 |
y_dflux_q = 0.0 |
|
377 |
ytsoil = 999999. |
ustar(:knon) = ustarhb(yu(:knon, 1), yv(:knon, 1), coefm(:knon, 1)) |
378 |
yrugoro = 0. |
|
379 |
c -- LOOP |
! iflag_pbl peut \^etre utilis\'e comme longueur de m\'elange |
380 |
yu10mx = 0.0 |
|
381 |
yu10my = 0.0 |
IF (iflag_pbl >= 11) THEN |
382 |
ywindsp = 0.0 |
CALL vdif_kcay(knon, dtime, rg, zlev, yzlay, yu, yv, yteta, & |
383 |
c -- LOOP |
coefm(:knon, 1), yq2, q2diag, ykmm, ykmn, ustar(:knon), & |
384 |
DO nsrf = 1, nbsrf |
iflag_pbl) |
385 |
DO i = 1, klon |
ELSE |
386 |
d_ts(i,nsrf) = 0.0 |
CALL yamada4(dtime, rg, zlev(:knon, :), yzlay(:knon, :), & |
387 |
ENDDO |
yu(:knon, :), yv(:knon, :), yteta(:knon, :), & |
388 |
END DO |
coefm(:knon, 1), yq2(:knon, :), ykmm(:knon, :), & |
389 |
C§§§ PB |
ykmn(:knon, :), ykmq(:knon, :), ustar(:knon), iflag_pbl) |
390 |
yfluxlat=0. |
END IF |
391 |
flux_t = 0. |
|
392 |
flux_q = 0. |
coefm(:knon, 2:) = ykmm(:knon, 2:klev) |
393 |
flux_u = 0. |
coefh(:knon, 2:) = ykmn(:knon, 2:klev) |
394 |
flux_v = 0. |
END IF |
395 |
DO k = 1, klev |
|
396 |
DO i = 1, klon |
! calculer la diffusion des vitesses "u" et "v" |
397 |
d_t(i,k) = 0.0 |
CALL clvent(knon, dtime, yu(:knon, 1), yv(:knon, 1), & |
398 |
d_q(i,k) = 0.0 |
coefm(:knon, :), yt, yu, ypaprs, ypplay, ydelp, y_d_u, & |
399 |
c$$$ flux_t(i,k) = 0.0 |
y_flux_u(:knon)) |
400 |
c$$$ flux_q(i,k) = 0.0 |
CALL clvent(knon, dtime, yu(:knon, 1), yv(:knon, 1), & |
401 |
d_u(i,k) = 0.0 |
coefm(:knon, :), yt, yv, ypaprs, ypplay, ydelp, y_d_v, & |
402 |
d_v(i,k) = 0.0 |
y_flux_v(:knon)) |
403 |
c$$$ flux_u(i,k) = 0.0 |
|
404 |
c$$$ flux_v(i,k) = 0.0 |
! calculer la diffusion de "q" et de "h" |
405 |
zcoefh(i,k) = 0.0 |
CALL clqh(dtime, julien, firstcal, nsrf, ni(:knon), & |
406 |
ENDDO |
ytsoil(:knon, :), yqsol(:knon), mu0, yrugos, yrugoro, & |
407 |
ENDDO |
yu(:knon, 1), yv(:knon, 1), coefh(:knon, :), yt, yq, & |
408 |
cAA IF (itr.GE.1) THEN |
yts(:knon), ypaprs, ypplay, ydelp, yrads(:knon), yalb(:knon), & |
409 |
cAA DO it = 1, itr |
snow(:knon), yqsurf, yrain_f, ysnow_f, yfluxlat(:knon), & |
410 |
cAA DO k = 1, klev |
pctsrf_new_sic, yagesno(:knon), y_d_t, y_d_q, y_d_ts(:knon), & |
411 |
cAA DO i = 1, klon |
yz0_new, y_flux_t(:knon), y_flux_q(:knon), y_dflux_t(:knon), & |
412 |
cAA d_tr(i,k,it) = 0.0 |
y_dflux_q(:knon), y_fqcalving, y_ffonte, y_run_off_lic_0) |
413 |
cAA ENDDO |
|
414 |
cAA ENDDO |
! calculer la longueur de rugosite sur ocean |
415 |
cAA ENDDO |
yrugm = 0. |
416 |
cAA ENDIF |
IF (nsrf == is_oce) THEN |
417 |
|
DO j = 1, knon |
418 |
c |
yrugm(j) = 0.018 * coefm(j, 1) * (yu(j, 1)**2 + yv(j, 1)**2) & |
419 |
c Boucler sur toutes les sous-fractions du sol: |
/ rg + 0.11 * 14E-6 & |
420 |
c |
/ sqrt(coefm(j, 1) * (yu(j, 1)**2 + yv(j, 1)**2)) |
421 |
C Initialisation des "pourcentages potentiels". On considere ici qu'on |
yrugm(j) = max(1.5E-05, yrugm(j)) |
422 |
C peut avoir potentiellementdela glace sur tout le domaine oceanique |
END DO |
423 |
C (a affiner) |
END IF |
424 |
|
DO j = 1, knon |
425 |
pctsrf_pot = pctsrf |
y_dflux_t(j) = y_dflux_t(j) * ypct(j) |
426 |
pctsrf_pot(:,is_oce) = 1. - zmasq(:) |
y_dflux_q(j) = y_dflux_q(j) * ypct(j) |
427 |
pctsrf_pot(:,is_sic) = 1. - zmasq(:) |
END DO |
428 |
|
|
429 |
DO nsrf = 1, nbsrf |
DO k = 1, klev |
430 |
|
DO j = 1, knon |
431 |
c chercher les indices: |
i = ni(j) |
432 |
DO j = 1, klon |
coefh(j, k) = coefh(j, k) * ypct(j) |
433 |
ni(j) = 0 |
coefm(j, k) = coefm(j, k) * ypct(j) |
434 |
ENDDO |
y_d_t(j, k) = y_d_t(j, k) * ypct(j) |
435 |
knon = 0 |
y_d_q(j, k) = y_d_q(j, k) * ypct(j) |
436 |
DO i = 1, klon |
y_d_u(j, k) = y_d_u(j, k) * ypct(j) |
437 |
|
y_d_v(j, k) = y_d_v(j, k) * ypct(j) |
438 |
C pour determiner le domaine a traiter on utilise les surfaces "potentielles" |
END DO |
439 |
C |
END DO |
440 |
IF (pctsrf_pot(i,nsrf).GT.epsfra) THEN |
|
441 |
knon = knon + 1 |
flux_t(ni(:knon), nsrf) = y_flux_t(:knon) |
442 |
ni(knon) = i |
flux_q(ni(:knon), nsrf) = y_flux_q(:knon) |
443 |
ENDIF |
flux_u(ni(:knon), nsrf) = y_flux_u(:knon) |
444 |
ENDDO |
flux_v(ni(:knon), nsrf) = y_flux_v(:knon) |
445 |
c |
|
446 |
if (check) THEN |
evap(:, nsrf) = -flux_q(:, nsrf) |
447 |
write(*,*)'CLMAIN, nsrf, knon =',nsrf, knon |
|
448 |
CC call flush(6) |
falbe(:, nsrf) = 0. |
449 |
endif |
fsnow(:, nsrf) = 0. |
450 |
c |
qsurf(:, nsrf) = 0. |
451 |
c variables pour avoir une sortie IOIPSL des INDEX |
frugs(:, nsrf) = 0. |
452 |
c |
DO j = 1, knon |
453 |
IF (debugindex) THEN |
i = ni(j) |
454 |
tabindx(:)=0. |
d_ts(i, nsrf) = y_d_ts(j) |
455 |
c tabindx(1:knon)=(/FLOAT(i),i=1:knon/) |
falbe(i, nsrf) = yalb(j) |
456 |
DO i=1,knon |
fsnow(i, nsrf) = snow(j) |
457 |
tabindx(1:knon)=FLOAT(i) |
qsurf(i, nsrf) = yqsurf(j) |
458 |
END DO |
frugs(i, nsrf) = yz0_new(j) |
459 |
debugtab(:,:)=0. |
fluxlat(i, nsrf) = yfluxlat(j) |
460 |
ndexbg(:)=0 |
IF (nsrf == is_oce) THEN |
461 |
CALL gath2cpl(tabindx,debugtab,klon,knon,iim,jjm,ni) |
rugmer(i) = yrugm(j) |
462 |
CALL histwrite(nidbg,cl_surf(nsrf),itap,debugtab,iim*(jjm+1) |
frugs(i, nsrf) = yrugm(j) |
463 |
$ ,ndexbg) |
END IF |
464 |
ENDIF |
agesno(i, nsrf) = yagesno(j) |
465 |
IF (knon.EQ.0) cycle |
fqcalving(i, nsrf) = y_fqcalving(j) |
466 |
DO j = 1, knon |
ffonte(i, nsrf) = y_ffonte(j) |
467 |
i = ni(j) |
cdragh(i) = cdragh(i) + coefh(j, 1) |
468 |
ypct(j) = pctsrf(i,nsrf) |
cdragm(i) = cdragm(i) + coefm(j, 1) |
469 |
yts(j) = ts(i,nsrf) |
dflux_t(i) = dflux_t(i) + y_dflux_t(j) |
470 |
cIM "slab" ocean |
dflux_q(i) = dflux_q(i) + y_dflux_q(j) |
471 |
c PRINT *, 'tslab = ', i, tslab(i) |
END DO |
472 |
ytslab(i) = tslab(i) |
IF (nsrf == is_ter) THEN |
473 |
c |
qsol(ni(:knon)) = yqsol(:knon) |
474 |
ysnow(j) = snow(i,nsrf) |
else IF (nsrf == is_lic) THEN |
475 |
yqsurf(j) = qsurf(i,nsrf) |
DO j = 1, knon |
476 |
yalb(j) = albe(i,nsrf) |
i = ni(j) |
477 |
yalblw(j) = alblw(i,nsrf) |
run_off_lic_0(i) = y_run_off_lic_0(j) |
478 |
yrain_f(j) = rain_f(i) |
END DO |
479 |
ysnow_f(j) = snow_f(i) |
END IF |
480 |
yagesno(j) = agesno(i,nsrf) |
|
481 |
yfder(j) = fder(i) |
ftsoil(:, :, nsrf) = 0. |
482 |
ytaux(j) = flux_u(i,1,nsrf) |
ftsoil(ni(:knon), :, nsrf) = ytsoil(:knon, :) |
483 |
ytauy(j) = flux_v(i,1,nsrf) |
|
|
ysolsw(j) = solsw(i,nsrf) |
|
|
ysollw(j) = sollw(i,nsrf) |
|
|
ysollwdown(j) = sollwdown(i) |
|
|
yrugos(j) = rugos(i,nsrf) |
|
|
yrugoro(j) = rugoro(i) |
|
|
yu1(j) = u1lay(i) |
|
|
yv1(j) = v1lay(i) |
|
|
yrads(j) = ysolsw(j)+ ysollw(j) |
|
|
ypaprs(j,klev+1) = paprs(i,klev+1) |
|
|
y_run_off_lic_0(j) = run_off_lic_0(i) |
|
|
c -- LOOP |
|
|
yu10mx(j) = u10m(i,nsrf) |
|
|
yu10my(j) = v10m(i,nsrf) |
|
|
ywindsp(j) = SQRT(yu10mx(j)*yu10mx(j) + yu10my(j)*yu10my(j) ) |
|
|
c -- LOOP |
|
|
END DO |
|
|
C |
|
|
C IF bucket model for continent, copy soil water content |
|
|
IF ( nsrf .eq. is_ter .and. .not. ok_veget ) THEN |
|
484 |
DO j = 1, knon |
DO j = 1, knon |
485 |
i = ni(j) |
i = ni(j) |
486 |
yqsol(j) = qsol(i) |
DO k = 1, klev |
487 |
|
d_t(i, k) = d_t(i, k) + y_d_t(j, k) |
488 |
|
d_q(i, k) = d_q(i, k) + y_d_q(j, k) |
489 |
|
d_u(i, k) = d_u(i, k) + y_d_u(j, k) |
490 |
|
d_v(i, k) = d_v(i, k) + y_d_v(j, k) |
491 |
|
ycoefh(i, k) = ycoefh(i, k) + coefh(j, k) |
492 |
|
END DO |
493 |
END DO |
END DO |
|
ELSE |
|
|
yqsol(:)=0. |
|
|
ENDIF |
|
|
c$$$ PB ajour pour soil |
|
|
DO k = 1, nsoilmx |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
ytsoil(j,k) = ftsoil(i,k,nsrf) |
|
|
END DO |
|
|
END DO |
|
|
DO k = 1, klev |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
ypaprs(j,k) = paprs(i,k) |
|
|
ypplay(j,k) = pplay(i,k) |
|
|
ydelp(j,k) = delp(i,k) |
|
|
yu(j,k) = u(i,k) |
|
|
yv(j,k) = v(i,k) |
|
|
yt(j,k) = t(i,k) |
|
|
yq(j,k) = q(i,k) |
|
|
ENDDO |
|
|
ENDDO |
|
|
c |
|
|
c |
|
|
c calculer Cdrag et les coefficients d'echange |
|
|
CALL coefkz(nsrf, knon, ypaprs, ypplay, |
|
|
cIM 261103 |
|
|
. ksta, ksta_ter, |
|
|
cIM 261103 |
|
|
. yts, yrugos, yu, yv, yt, yq, |
|
|
. yqsurf, |
|
|
. ycoefm, ycoefh) |
|
|
cIM 081204 BEG |
|
|
cCR test |
|
|
if (iflag_pbl.eq.1) then |
|
|
cIM 081204 END |
|
|
CALL coefkz2(nsrf, knon, ypaprs, ypplay,yt, |
|
|
. ycoefm0, ycoefh0) |
|
|
DO k = 1, klev |
|
|
DO i = 1, knon |
|
|
ycoefm(i,k) = MAX(ycoefm(i,k),ycoefm0(i,k)) |
|
|
ycoefh(i,k) = MAX(ycoefh(i,k),ycoefh0(i,k)) |
|
|
ENDDO |
|
|
ENDDO |
|
|
endif |
|
|
c |
|
|
cIM cf JLD : on seuille ycoefm et ycoefh |
|
|
if (nsrf.eq.is_oce) then |
|
|
do j=1,knon |
|
|
c ycoefm(j,1)=min(ycoefm(j,1),1.1E-3) |
|
|
ycoefm(j,1)=min(ycoefm(j,1),cdmmax) |
|
|
c ycoefh(j,1)=min(ycoefh(j,1),1.1E-3) |
|
|
ycoefh(j,1)=min(ycoefh(j,1),cdhmax) |
|
|
enddo |
|
|
endif |
|
|
|
|
|
c |
|
|
cIM: 261103 |
|
|
if (ok_kzmin) THEN |
|
|
cIM cf FH: 201103 BEG |
|
|
c Calcul d'une diffusion minimale pour les conditions tres stables. |
|
|
call coefkzmin(knon,ypaprs,ypplay,yu,yv,yt,yq,ycoefm |
|
|
. ,ycoefm0,ycoefh0) |
|
|
c call dump2d(iim,jjm-1,ycoefm(2:klon-1,2), 'KZ ') |
|
|
c call dump2d(iim,jjm-1,ycoefm0(2:klon-1,2),'KZMIN ') |
|
|
|
|
|
if ( 1.eq.1 ) then |
|
|
DO k = 1, klev |
|
|
DO i = 1, knon |
|
|
ycoefm(i,k) = MAX(ycoefm(i,k),ycoefm0(i,k)) |
|
|
ycoefh(i,k) = MAX(ycoefh(i,k),ycoefh0(i,k)) |
|
|
ENDDO |
|
|
ENDDO |
|
|
endif |
|
|
cIM cf FH: 201103 END |
|
|
endif !ok_kzmin |
|
|
cIM: 261103 |
|
|
|
|
|
|
|
|
IF (iflag_pbl.ge.3) then |
|
|
|
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
c MELLOR ET YAMADA adapte a Mars Richard Fournier et Frederic Hourdin |
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
|
|
|
yzlay(1:knon,1)= |
|
|
. RD*yt(1:knon,1)/(0.5*(ypaprs(1:knon,1)+ypplay(1:knon,1))) |
|
|
. *(ypaprs(1:knon,1)-ypplay(1:knon,1))/RG |
|
|
do k=2,klev |
|
|
yzlay(1:knon,k)= |
|
|
. yzlay(1:knon,k-1)+RD*0.5*(yt(1:knon,k-1)+yt(1:knon,k)) |
|
|
. /ypaprs(1:knon,k)*(ypplay(1:knon,k-1)-ypplay(1:knon,k))/RG |
|
|
enddo |
|
|
do k=1,klev |
|
|
yteta(1:knon,k)= |
|
|
. yt(1:knon,k)*(ypaprs(1:knon,1)/ypplay(1:knon,k))**rkappa |
|
|
. *(1.+0.61*yq(1:knon,k)) |
|
|
enddo |
|
|
yzlev(1:knon,1)=0. |
|
|
yzlev(1:knon,klev+1)=2.*yzlay(1:knon,klev)-yzlay(1:knon,klev-1) |
|
|
do k=2,klev |
|
|
yzlev(1:knon,k)=0.5*(yzlay(1:knon,k)+yzlay(1:knon,k-1)) |
|
|
enddo |
|
|
DO k = 1, klev+1 |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
yq2(j,k)=q2(i,k,nsrf) |
|
|
enddo |
|
|
enddo |
|
|
|
|
|
|
|
|
c Bug introduit volontairement pour converger avec les resultats |
|
|
c du papier sur les thermiques. |
|
|
if (1.eq.1) then |
|
|
y_cd_m(1:knon) = ycoefm(1:knon,1) |
|
|
y_cd_h(1:knon) = ycoefh(1:knon,1) |
|
|
else |
|
|
y_cd_h(1:knon) = ycoefm(1:knon,1) |
|
|
y_cd_m(1:knon) = ycoefh(1:knon,1) |
|
|
endif |
|
|
call ustarhb(knon,yu,yv,y_cd_m, yustar) |
|
|
|
|
|
if (prt_level > 9) THEN |
|
|
print *,'USTAR = ',yustar |
|
|
ENDIF |
|
|
|
|
|
c iflag_pbl peut etre utilise comme longuer de melange |
|
|
|
|
|
if (iflag_pbl.ge.11) then |
|
|
call vdif_kcay(knon,dtime,rg,rd,ypaprs,yt |
|
|
s ,yzlev,yzlay,yu,yv,yteta |
|
|
s ,y_cd_m,yq2,q2diag,ykmm,ykmn,yustar, |
|
|
s iflag_pbl) |
|
|
else |
|
|
call yamada4(knon,dtime,rg,rd,ypaprs,yt |
|
|
s ,yzlev,yzlay,yu,yv,yteta |
|
|
s ,y_cd_m,yq2,ykmm,ykmn,ykmq,yustar, |
|
|
s iflag_pbl) |
|
|
endif |
|
|
|
|
|
ycoefm(1:knon,1)=y_cd_m(1:knon) |
|
|
ycoefh(1:knon,1)=y_cd_h(1:knon) |
|
|
ycoefm(1:knon,2:klev)=ykmm(1:knon,2:klev) |
|
|
ycoefh(1:knon,2:klev)=ykmn(1:knon,2:klev) |
|
|
|
|
|
|
|
|
ENDIF |
|
|
|
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
c calculer la diffusion des vitesses "u" et "v" |
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
|
|
|
CALL clvent(knon,dtime,yu1,yv1,ycoefm,yt,yu,ypaprs,ypplay,ydelp, |
|
|
s y_d_u,y_flux_u) |
|
|
CALL clvent(knon,dtime,yu1,yv1,ycoefm,yt,yv,ypaprs,ypplay,ydelp, |
|
|
s y_d_v,y_flux_v) |
|
|
|
|
|
c pour le couplage |
|
|
ytaux = y_flux_u(:,1) |
|
|
ytauy = y_flux_v(:,1) |
|
|
|
|
|
c FH modif sur le cdrag temperature |
|
|
c$$$PB : déplace dans clcdrag |
|
|
c$$$ do i=1,knon |
|
|
c$$$ ycoefh(i,1)=ycoefm(i,1)*0.8 |
|
|
c$$$ enddo |
|
|
|
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
c calculer la diffusion de "q" et de "h" |
|
|
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
CALL clqh(dtime, itap, date0,jour, debut,lafin, |
|
|
e rlon, rlat, cufi, cvfi, |
|
|
e knon, nsrf, ni, pctsrf, |
|
|
e soil_model, ytsoil,yqsol, |
|
|
e ok_veget, ocean, npas, nexca, |
|
|
e rmu0, co2_ppm, yrugos, yrugoro, |
|
|
e yu1, yv1, ycoefh, |
|
|
e yt,yq,yts,ypaprs,ypplay, |
|
|
e ydelp,yrads,yalb, yalblw, ysnow, yqsurf, |
|
|
e yrain_f, ysnow_f, yfder, ytaux, ytauy, |
|
|
c -- LOOP |
|
|
e ywindsp, |
|
|
c -- LOOP |
|
|
c$$$ e ysollw, ysolsw, |
|
|
e ysollw, ysollwdown, ysolsw,yfluxlat, |
|
|
s pctsrf_new, yagesno, |
|
|
s y_d_t, y_d_q, y_d_ts, yz0_new, |
|
|
s y_flux_t, y_flux_q, y_dflux_t, y_dflux_q, |
|
|
s y_fqcalving,y_ffonte,y_run_off_lic_0, |
|
|
cIM "slab" ocean |
|
|
s y_flux_o, y_flux_g, ytslab, y_seaice) |
|
|
c |
|
|
c calculer la longueur de rugosite sur ocean |
|
|
yrugm=0. |
|
|
IF (nsrf.EQ.is_oce) THEN |
|
|
DO j = 1, knon |
|
|
yrugm(j) = 0.018*ycoefm(j,1) * (yu1(j)**2+yv1(j)**2)/RG |
|
|
$ + 0.11*14e-6 / sqrt(ycoefm(j,1) * (yu1(j)**2+yv1(j)**2)) |
|
|
yrugm(j) = MAX(1.5e-05,yrugm(j)) |
|
|
ENDDO |
|
|
ENDIF |
|
|
DO j = 1, knon |
|
|
y_dflux_t(j) = y_dflux_t(j) * ypct(j) |
|
|
y_dflux_q(j) = y_dflux_q(j) * ypct(j) |
|
|
yu1(j) = yu1(j) * ypct(j) |
|
|
yv1(j) = yv1(j) * ypct(j) |
|
|
ENDDO |
|
|
c |
|
|
DO k = 1, klev |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
ycoefh(j,k) = ycoefh(j,k) * ypct(j) |
|
|
ycoefm(j,k) = ycoefm(j,k) * ypct(j) |
|
|
y_d_t(j,k) = y_d_t(j,k) * ypct(j) |
|
|
y_d_q(j,k) = y_d_q(j,k) * ypct(j) |
|
|
C§§§ PB |
|
|
flux_t(i,k,nsrf) = y_flux_t(j,k) |
|
|
flux_q(i,k,nsrf) = y_flux_q(j,k) |
|
|
flux_u(i,k,nsrf) = y_flux_u(j,k) |
|
|
flux_v(i,k,nsrf) = y_flux_v(j,k) |
|
|
c$$$ PB y_flux_t(j,k) = y_flux_t(j,k) * ypct(j) |
|
|
c$$$ PB y_flux_q(j,k) = y_flux_q(j,k) * ypct(j) |
|
|
y_d_u(j,k) = y_d_u(j,k) * ypct(j) |
|
|
y_d_v(j,k) = y_d_v(j,k) * ypct(j) |
|
|
c$$$ PB y_flux_u(j,k) = y_flux_u(j,k) * ypct(j) |
|
|
c$$$ PB y_flux_v(j,k) = y_flux_v(j,k) * ypct(j) |
|
|
ENDDO |
|
|
ENDDO |
|
|
|
|
|
|
|
|
evap(:,nsrf) = - flux_q(:,1,nsrf) |
|
|
c |
|
|
albe(:, nsrf) = 0. |
|
|
alblw(:, nsrf) = 0. |
|
|
snow(:, nsrf) = 0. |
|
|
qsurf(:, nsrf) = 0. |
|
|
rugos(:, nsrf) = 0. |
|
|
fluxlat(:,nsrf) = 0. |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
d_ts(i,nsrf) = y_d_ts(j) |
|
|
albe(i,nsrf) = yalb(j) |
|
|
alblw(i,nsrf) = yalblw(j) |
|
|
snow(i,nsrf) = ysnow(j) |
|
|
qsurf(i,nsrf) = yqsurf(j) |
|
|
rugos(i,nsrf) = yz0_new(j) |
|
|
fluxlat(i,nsrf) = yfluxlat(j) |
|
|
c$$$ pb rugmer(i) = yrugm(j) |
|
|
IF (nsrf .EQ. is_oce) then |
|
|
rugmer(i) = yrugm(j) |
|
|
rugos(i,nsrf) = yrugm(j) |
|
|
endif |
|
|
cIM cf JLD ?? |
|
|
agesno(i,nsrf) = yagesno(j) |
|
|
fqcalving(i,nsrf) = y_fqcalving(j) |
|
|
ffonte(i,nsrf) = y_ffonte(j) |
|
|
cdragh(i) = cdragh(i) + ycoefh(j,1) |
|
|
cdragm(i) = cdragm(i) + ycoefm(j,1) |
|
|
dflux_t(i) = dflux_t(i) + y_dflux_t(j) |
|
|
dflux_q(i) = dflux_q(i) + y_dflux_q(j) |
|
|
zu1(i) = zu1(i) + yu1(j) |
|
|
zv1(i) = zv1(i) + yv1(j) |
|
|
END DO |
|
|
IF ( nsrf .eq. is_ter ) THEN |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
qsol(i) = yqsol(j) |
|
|
END DO |
|
|
END IF |
|
|
IF ( nsrf .eq. is_lic ) THEN |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
run_off_lic_0(i) = y_run_off_lic_0(j) |
|
|
END DO |
|
|
END IF |
|
|
c$$$ PB ajout pour soil |
|
|
ftsoil(:,:,nsrf) = 0. |
|
|
DO k = 1, nsoilmx |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
ftsoil(i, k, nsrf) = ytsoil(j,k) |
|
|
END DO |
|
|
END DO |
|
|
c |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
DO k = 1, klev |
|
|
d_t(i,k) = d_t(i,k) + y_d_t(j,k) |
|
|
d_q(i,k) = d_q(i,k) + y_d_q(j,k) |
|
|
c$$$ PB flux_t(i,k) = flux_t(i,k) + y_flux_t(j,k) |
|
|
c$$$ flux_q(i,k) = flux_q(i,k) + y_flux_q(j,k) |
|
|
d_u(i,k) = d_u(i,k) + y_d_u(j,k) |
|
|
d_v(i,k) = d_v(i,k) + y_d_v(j,k) |
|
|
c$$$ PB flux_u(i,k) = flux_u(i,k) + y_flux_u(j,k) |
|
|
c$$$ flux_v(i,k) = flux_v(i,k) + y_flux_v(j,k) |
|
|
zcoefh(i,k) = zcoefh(i,k) + ycoefh(j,k) |
|
|
ENDDO |
|
|
ENDDO |
|
|
c |
|
|
c |
|
|
ccc diagnostic t,q a 2m et u, v a 10m |
|
|
c |
|
|
DO j=1, knon |
|
|
i = ni(j) |
|
|
uzon(j) = yu(j,1) + y_d_u(j,1) |
|
|
vmer(j) = yv(j,1) + y_d_v(j,1) |
|
|
tair1(j) = yt(j,1) + y_d_t(j,1) |
|
|
qair1(j) = yq(j,1) + y_d_q(j,1) |
|
|
zgeo1(j) = RD * tair1(j) / (0.5*(ypaprs(j,1)+ypplay(j,1))) |
|
|
& * (ypaprs(j,1)-ypplay(j,1)) |
|
|
tairsol(j) = yts(j) + y_d_ts(j) |
|
|
rugo1(j) = yrugos(j) |
|
|
IF(nsrf.EQ.is_oce) THEN |
|
|
rugo1(j) = rugos(i,nsrf) |
|
|
ENDIF |
|
|
psfce(j)=ypaprs(j,1) |
|
|
patm(j)=ypplay(j,1) |
|
|
c |
|
|
qairsol(j) = yqsurf(j) |
|
|
ENDDO |
|
|
c |
|
|
CALL stdlevvar(klon, knon, nsrf, zxli, |
|
|
& uzon, vmer, tair1, qair1, zgeo1, |
|
|
& tairsol, qairsol, rugo1, psfce, patm, |
|
|
cIM & yt2m, yq2m, yu10m) |
|
|
& yt2m, yq2m, yt10m, yq10m, yu10m, yustar) |
|
|
cIM 081204 END |
|
|
c |
|
|
c |
|
|
DO j=1, knon |
|
|
i = ni(j) |
|
|
t2m(i,nsrf)=yt2m(j) |
|
|
|
|
|
c |
|
|
q2m(i,nsrf)=yq2m(j) |
|
|
c |
|
|
c u10m, v10m : composantes du vent a 10m sans spirale de Ekman |
|
|
u10m(i,nsrf)=(yu10m(j) * uzon(j))/sqrt(uzon(j)**2+vmer(j)**2) |
|
|
v10m(i,nsrf)=(yu10m(j) * vmer(j))/sqrt(uzon(j)**2+vmer(j)**2) |
|
|
c |
|
|
ENDDO |
|
|
c |
|
|
cIM cf AM : pbl, HBTM |
|
|
DO i = 1, knon |
|
|
y_cd_h(i) = ycoefh(i,1) |
|
|
y_cd_m(i) = ycoefm(i,1) |
|
|
ENDDO |
|
|
c print*,'appel hbtm2' |
|
|
CALL HBTM(knon, ypaprs, ypplay, |
|
|
. yt2m,yt10m,yq2m,yq10m,yustar, |
|
|
. y_flux_t,y_flux_q,yu,yv,yt,yq, |
|
|
. ypblh,ycapCL,yoliqCL,ycteiCL,ypblT, |
|
|
. ytherm,ytrmb1,ytrmb2,ytrmb3,ylcl) |
|
|
c print*,'fin hbtm2' |
|
|
c |
|
|
DO j=1, knon |
|
|
i = ni(j) |
|
|
pblh(i,nsrf) = ypblh(j) |
|
|
plcl(i,nsrf) = ylcl(j) |
|
|
capCL(i,nsrf) = ycapCL(j) |
|
|
oliqCL(i,nsrf) = yoliqCL(j) |
|
|
cteiCL(i,nsrf) = ycteiCL(j) |
|
|
pblT(i,nsrf) = ypblT(j) |
|
|
therm(i,nsrf) = ytherm(j) |
|
|
trmb1(i,nsrf) = ytrmb1(j) |
|
|
trmb2(i,nsrf) = ytrmb2(j) |
|
|
trmb3(i,nsrf) = ytrmb3(j) |
|
|
ENDDO |
|
|
c |
|
|
|
|
|
do j=1,knon |
|
|
do k=1,klev+1 |
|
|
i=ni(j) |
|
|
q2(i,k,nsrf)=yq2(j,k) |
|
|
enddo |
|
|
enddo |
|
|
cIM "slab" ocean |
|
|
IF (nsrf.EQ.is_oce) THEN |
|
|
DO j = 1, knon |
|
|
c on projette sur la grille globale |
|
|
i = ni(j) |
|
|
IF(pctsrf_new(i,is_oce).GT.epsfra) THEN |
|
|
flux_o(i) = y_flux_o(j) |
|
|
ELSE |
|
|
flux_o(i) = 0. |
|
|
ENDIF |
|
|
ENDDO |
|
|
ENDIF |
|
|
c |
|
|
IF (nsrf.EQ.is_sic) THEN |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
cIM 230604 on pondere lorsque l'on fait le bilan au sol : flux_g(i) = y_flux_g(j)*ypct(j) |
|
|
IF(pctsrf_new(i,is_sic).GT.epsfra) THEN |
|
|
flux_g(i) = y_flux_g(j) |
|
|
ELSE |
|
|
flux_g(i) = 0. |
|
|
ENDIF |
|
|
ENDDO |
|
|
ENDIF !nsrf.EQ.is_sic |
|
|
c |
|
|
IF(OCEAN.EQ.'slab ') THEN |
|
|
IF(nsrf.EQ.is_oce) then |
|
|
tslab(1:klon) = ytslab(1:klon) |
|
|
seaice(1:klon) = y_seaice(1:klon) |
|
|
ENDIF !nsrf |
|
|
ENDIF !OCEAN |
|
|
end do |
|
|
C |
|
|
C On utilise les nouvelles surfaces |
|
|
C A rajouter: conservation de l'albedo |
|
|
C |
|
|
rugos(:,is_oce) = rugmer |
|
|
pctsrf = pctsrf_new |
|
494 |
|
|
495 |
RETURN |
! diagnostic t, q a 2m et u, v a 10m |
496 |
END |
|
497 |
|
DO j = 1, knon |
498 |
|
i = ni(j) |
499 |
|
u1(j) = yu(j, 1) + y_d_u(j, 1) |
500 |
|
v1(j) = yv(j, 1) + y_d_v(j, 1) |
501 |
|
tair1(j) = yt(j, 1) + y_d_t(j, 1) |
502 |
|
qair1(j) = yq(j, 1) + y_d_q(j, 1) |
503 |
|
zgeo1(j) = rd * tair1(j) / (0.5 * (ypaprs(j, 1) + ypplay(j, & |
504 |
|
1))) * (ypaprs(j, 1)-ypplay(j, 1)) |
505 |
|
tairsol(j) = yts(j) + y_d_ts(j) |
506 |
|
rugo1(j) = yrugos(j) |
507 |
|
IF (nsrf == is_oce) THEN |
508 |
|
rugo1(j) = frugs(i, nsrf) |
509 |
|
END IF |
510 |
|
psfce(j) = ypaprs(j, 1) |
511 |
|
patm(j) = ypplay(j, 1) |
512 |
|
|
513 |
|
qairsol(j) = yqsurf(j) |
514 |
|
END DO |
515 |
|
|
516 |
|
CALL stdlevvar(klon, knon, nsrf, u1(:knon), v1(:knon), tair1(:knon), & |
517 |
|
qair1, zgeo1, tairsol, qairsol, rugo1, psfce, patm, yt2m, & |
518 |
|
yq2m, yt10m, yq10m, wind10m(:knon), ustar) |
519 |
|
|
520 |
|
DO j = 1, knon |
521 |
|
i = ni(j) |
522 |
|
t2m(i, nsrf) = yt2m(j) |
523 |
|
q2m(i, nsrf) = yq2m(j) |
524 |
|
|
525 |
|
u10m_srf(i, nsrf) = (wind10m(j) * u1(j)) & |
526 |
|
/ sqrt(u1(j)**2 + v1(j)**2) |
527 |
|
v10m_srf(i, nsrf) = (wind10m(j) * v1(j)) & |
528 |
|
/ sqrt(u1(j)**2 + v1(j)**2) |
529 |
|
END DO |
530 |
|
|
531 |
|
CALL hbtm(ypaprs, ypplay, yt2m, yq2m, ustar(:knon), y_flux_t(:knon), & |
532 |
|
y_flux_q(:knon), yu, yv, yt, yq, ypblh(:knon), ycapcl, & |
533 |
|
yoliqcl, ycteicl, ypblt, ytherm, ytrmb1, ytrmb2, ytrmb3, ylcl) |
534 |
|
|
535 |
|
DO j = 1, knon |
536 |
|
i = ni(j) |
537 |
|
pblh(i, nsrf) = ypblh(j) |
538 |
|
plcl(i, nsrf) = ylcl(j) |
539 |
|
capcl(i, nsrf) = ycapcl(j) |
540 |
|
oliqcl(i, nsrf) = yoliqcl(j) |
541 |
|
cteicl(i, nsrf) = ycteicl(j) |
542 |
|
pblt(i, nsrf) = ypblt(j) |
543 |
|
therm(i, nsrf) = ytherm(j) |
544 |
|
trmb1(i, nsrf) = ytrmb1(j) |
545 |
|
trmb2(i, nsrf) = ytrmb2(j) |
546 |
|
trmb3(i, nsrf) = ytrmb3(j) |
547 |
|
END DO |
548 |
|
|
549 |
|
DO j = 1, knon |
550 |
|
DO k = 1, klev + 1 |
551 |
|
i = ni(j) |
552 |
|
q2(i, k, nsrf) = yq2(j, k) |
553 |
|
END DO |
554 |
|
END DO |
555 |
|
else |
556 |
|
fsnow(:, nsrf) = 0. |
557 |
|
end IF if_knon |
558 |
|
END DO loop_surface |
559 |
|
|
560 |
|
! On utilise les nouvelles surfaces |
561 |
|
frugs(:, is_oce) = rugmer |
562 |
|
pctsrf(:, is_oce) = pctsrf_new_oce |
563 |
|
pctsrf(:, is_sic) = pctsrf_new_sic |
564 |
|
|
565 |
|
firstcal = .false. |
566 |
|
|
567 |
|
END SUBROUTINE clmain |
568 |
|
|
569 |
|
end module clmain_m |