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SUBROUTINE clmain(dtime, itap, date0, pctsrf, pctsrf_new, t, q, u, v,& |
module clmain_m |
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jour, rmu0, co2_ppm, ok_veget, ocean, npas, nexca, ts,& |
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soil_model, cdmmax, cdhmax, ksta, ksta_ter, ok_kzmin, ftsoil,& |
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qsol, paprs, pplay, snow, qsurf, evap, albe, alblw, fluxlat,& |
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rain_f, snow_f, solsw, sollw, sollwdown, fder, rlon, rlat, cufi,& |
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cvfi, rugos, debut, lafin, agesno, rugoro, d_t, d_q, d_u, d_v,& |
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d_ts, flux_t, flux_q, flux_u, flux_v, cdragh, cdragm, q2,& |
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dflux_t, dflux_q, zcoefh, zu1, zv1, t2m, q2m, u10m, v10m, pblh,& |
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capcl, oliqcl, cteicl, pblt, therm, trmb1, trmb2, trmb3, plcl,& |
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fqcalving, ffonte, run_off_lic_0, flux_o, flux_g, tslab, seaice) |
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! From phylmd/clmain.F, v 1.6 2005/11/16 14:47:19 |
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!AA Tout ce qui a trait au traceurs est dans phytrac maintenant |
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!AA pour l'instant le calcul de la couche limite pour les traceurs |
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!AA se fait avec cltrac et ne tient pas compte de la differentiation |
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!AA des sous-fraction de sol. |
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!AA Pour pouvoir extraire les coefficient d'echanges et le vent |
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!AA dans la premiere couche, 3 champs supplementaires ont ete crees |
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!AA zcoefh, zu1 et zv1. Pour l'instant nous avons moyenne les valeurs |
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!AA de ces trois champs sur les 4 subsurfaces du modele. Dans l'avenir |
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!AA si les informations des subsurfaces doivent etre prises en compte |
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!AA il faudra sortir ces memes champs en leur ajoutant une dimension, |
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!AA c'est a dire nbsrf (nbre de subsurface). |
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! Auteur(s) Z.X. Li (LMD/CNRS) date: 19930818 |
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! Objet: interface de "couche limite" (diffusion verticale) |
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! Arguments: |
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! dtime----input-R- interval du temps (secondes) |
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! itap-----input-I- numero du pas de temps |
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! date0----input-R- jour initial |
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! t--------input-R- temperature (K) |
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! q--------input-R- vapeur d'eau (kg/kg) |
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! u--------input-R- vitesse u |
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! v--------input-R- vitesse v |
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! ts-------input-R- temperature du sol (en Kelvin) |
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! paprs----input-R- pression a intercouche (Pa) |
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! pplay----input-R- pression au milieu de couche (Pa) |
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! radsol---input-R- flux radiatif net (positif vers le sol) en W/m**2 |
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! rlat-----input-R- latitude en degree |
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! rugos----input-R- longeur de rugosite (en m) |
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! cufi-----input-R- resolution des mailles en x (m) |
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! cvfi-----input-R- resolution des mailles en y (m) |
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! d_t------output-R- le changement pour "t" |
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! d_q------output-R- le changement pour "q" |
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! d_u------output-R- le changement pour "u" |
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! d_v------output-R- le changement pour "v" |
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! d_ts-----output-R- le changement pour "ts" |
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! flux_t---output-R- flux de chaleur sensible (CpT) J/m**2/s (W/m**2) |
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! (orientation positive vers le bas) |
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! flux_q---output-R- flux de vapeur d'eau (kg/m**2/s) |
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! flux_u---output-R- tension du vent X: (kg m/s)/(m**2 s) ou Pascal |
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! flux_v---output-R- tension du vent Y: (kg m/s)/(m**2 s) ou Pascal |
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! dflux_t derive du flux sensible |
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! dflux_q derive du flux latent |
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!IM "slab" ocean |
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! flux_g---output-R- flux glace (pour OCEAN='slab ') |
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! flux_o---output-R- flux ocean (pour OCEAN='slab ') |
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! tslab-in/output-R temperature du slab ocean (en Kelvin) ! uniqmnt pour slab |
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! seaice---output-R- glace de mer (kg/m2) (pour OCEAN='slab ') |
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!cc |
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! ffonte----Flux thermique utilise pour fondre la neige |
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! fqcalving-Flux d'eau "perdue" par la surface et necessaire pour limiter la |
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! hauteur de neige, en kg/m2/s |
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!AA on rajoute en output yu1 et yv1 qui sont les vents dans |
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!AA la premiere couche |
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!AA ces 4 variables sont maintenant traites dans phytrac |
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! itr--------input-I- nombre de traceurs |
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! tr---------input-R- q. de traceurs |
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! flux_surf--input-R- flux de traceurs a la surface |
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! d_tr-------output-R tendance de traceurs |
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!IM cf. AM : PBL |
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! trmb1-------deep_cape |
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! trmb2--------inhibition |
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! trmb3-------Point Omega |
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! Cape(klon)-------Cape du thermique |
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! EauLiq(klon)-------Eau liqu integr du thermique |
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! ctei(klon)-------Critere d'instab d'entrainmt des nuages de CL |
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! lcl------- Niveau de condensation |
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! pblh------- HCL |
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! pblT------- T au nveau HCL |
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!$$$ PB ajout pour soil |
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USE histcom, ONLY : histbeg_totreg, histdef, histend, histsync |
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use histwrite_m, only: histwrite |
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use calendar, ONLY : ymds2ju |
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USE dimens_m, ONLY : iim, jjm |
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USE indicesol, ONLY : epsfra, is_lic, is_oce, is_sic, is_ter, nbsrf |
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USE dimphy, ONLY : klev, klon, zmasq |
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USE dimsoil, ONLY : nsoilmx |
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USE temps, ONLY : annee_ref, itau_phy |
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USE dynetat0_m, ONLY : day_ini |
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USE iniprint, ONLY : prt_level |
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USE yomcst, ONLY : rd, rg, rkappa |
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USE conf_phys_m, ONLY : iflag_pbl |
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USE gath_cpl, ONLY : gath2cpl |
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use hbtm_m, only: hbtm |
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IMPLICIT NONE |
IMPLICIT NONE |
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REAL, INTENT (IN) :: dtime |
contains |
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REAL date0 |
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INTEGER, INTENT (IN) :: itap |
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REAL t(klon, klev), q(klon, klev) |
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REAL u(klon, klev), v(klon, klev) |
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REAL, INTENT (IN) :: paprs(klon, klev+1) |
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REAL, INTENT (IN) :: pplay(klon, klev) |
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REAL, INTENT (IN) :: rlon(klon), rlat(klon) |
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REAL cufi(klon), cvfi(klon) |
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REAL d_t(klon, klev), d_q(klon, klev) |
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REAL d_u(klon, klev), d_v(klon, klev) |
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REAL flux_t(klon, klev, nbsrf), flux_q(klon, klev, nbsrf) |
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REAL dflux_t(klon), dflux_q(klon) |
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!IM "slab" ocean |
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REAL flux_o(klon), flux_g(klon) |
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REAL y_flux_o(klon), y_flux_g(klon) |
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REAL tslab(klon), ytslab(klon) |
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REAL seaice(klon), y_seaice(klon) |
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REAL y_fqcalving(klon), y_ffonte(klon) |
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REAL fqcalving(klon, nbsrf), ffonte(klon, nbsrf) |
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REAL run_off_lic_0(klon), y_run_off_lic_0(klon) |
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REAL flux_u(klon, klev, nbsrf), flux_v(klon, klev, nbsrf) |
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REAL rugmer(klon), agesno(klon, nbsrf) |
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REAL, INTENT (IN) :: rugoro(klon) |
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REAL cdragh(klon), cdragm(klon) |
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! jour de l'annee en cours |
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INTEGER jour |
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REAL rmu0(klon) ! cosinus de l'angle solaire zenithal |
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! taux CO2 atmosphere |
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REAL co2_ppm |
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LOGICAL, INTENT (IN) :: debut |
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LOGICAL, INTENT (IN) :: lafin |
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LOGICAL ok_veget |
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CHARACTER (len=*), INTENT (IN) :: ocean |
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INTEGER npas, nexca |
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REAL pctsrf(klon, nbsrf) |
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REAL ts(klon, nbsrf) |
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REAL d_ts(klon, nbsrf) |
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REAL snow(klon, nbsrf) |
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REAL qsurf(klon, nbsrf) |
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REAL evap(klon, nbsrf) |
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REAL albe(klon, nbsrf) |
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REAL alblw(klon, nbsrf) |
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REAL fluxlat(klon, nbsrf) |
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REAL rain_f(klon), snow_f(klon) |
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REAL fder(klon) |
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REAL sollw(klon, nbsrf), solsw(klon, nbsrf), sollwdown(klon) |
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REAL rugos(klon, nbsrf) |
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! la nouvelle repartition des surfaces sortie de l'interface |
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REAL pctsrf_new(klon, nbsrf) |
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REAL zcoefh(klon, klev) |
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REAL zu1(klon) |
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REAL zv1(klon) |
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!$$$ PB ajout pour soil |
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LOGICAL, INTENT (IN) :: soil_model |
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!IM ajout seuils cdrm, cdrh |
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REAL cdmmax, cdhmax |
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REAL ksta, ksta_ter |
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LOGICAL ok_kzmin |
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REAL ftsoil(klon, nsoilmx, nbsrf) |
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REAL ytsoil(klon, nsoilmx) |
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REAL qsol(klon) |
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EXTERNAL clqh, clvent, coefkz, calbeta, cltrac |
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REAL yts(klon), yrugos(klon), ypct(klon), yz0_new(klon) |
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REAL yalb(klon) |
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REAL yalblw(klon) |
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REAL yu1(klon), yv1(klon) |
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REAL ysnow(klon), yqsurf(klon), yagesno(klon), yqsol(klon) |
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REAL yrain_f(klon), ysnow_f(klon) |
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REAL ysollw(klon), ysolsw(klon), ysollwdown(klon) |
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REAL yfder(klon), ytaux(klon), ytauy(klon) |
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REAL yrugm(klon), yrads(klon), yrugoro(klon) |
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REAL yfluxlat(klon) |
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REAL y_d_ts(klon) |
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REAL y_d_t(klon, klev), y_d_q(klon, klev) |
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REAL y_d_u(klon, klev), y_d_v(klon, klev) |
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REAL y_flux_t(klon, klev), y_flux_q(klon, klev) |
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REAL y_flux_u(klon, klev), y_flux_v(klon, klev) |
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REAL y_dflux_t(klon), y_dflux_q(klon) |
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REAL ycoefh(klon, klev), ycoefm(klon, klev) |
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REAL yu(klon, klev), yv(klon, klev) |
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REAL yt(klon, klev), yq(klon, klev) |
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REAL ypaprs(klon, klev+1), ypplay(klon, klev), ydelp(klon, klev) |
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LOGICAL ok_nonloc |
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PARAMETER (ok_nonloc=.FALSE.) |
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REAL ycoefm0(klon, klev), ycoefh0(klon, klev) |
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!IM 081204 hcl_Anne ? BEG |
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REAL yzlay(klon, klev), yzlev(klon, klev+1), yteta(klon, klev) |
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REAL ykmm(klon, klev+1), ykmn(klon, klev+1) |
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REAL ykmq(klon, klev+1) |
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REAL yq2(klon, klev+1), q2(klon, klev+1, nbsrf) |
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REAL q2diag(klon, klev+1) |
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!IM 081204 hcl_Anne ? END |
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REAL u1lay(klon), v1lay(klon) |
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REAL delp(klon, klev) |
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INTEGER i, k, nsrf |
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INTEGER ni(klon), knon, j |
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! Introduction d'une variable "pourcentage potentiel" pour tenir compte |
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! des eventuelles apparitions et/ou disparitions de la glace de mer |
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REAL pctsrf_pot(klon, nbsrf) |
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REAL zx_alf1, zx_alf2 !valeur ambiante par extrapola. |
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! maf pour sorties IOISPL en cas de debugagage |
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CHARACTER (80) cldebug |
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SAVE cldebug |
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CHARACTER (8) cl_surf(nbsrf) |
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SAVE cl_surf |
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INTEGER nhoridbg, nidbg |
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SAVE nhoridbg, nidbg |
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INTEGER ndexbg(iim*(jjm+1)) |
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REAL zx_lon(iim, jjm+1), zx_lat(iim, jjm+1), zjulian |
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REAL tabindx(klon) |
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REAL debugtab(iim, jjm+1) |
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LOGICAL first_appel |
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SAVE first_appel |
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DATA first_appel/ .TRUE./ |
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LOGICAL :: debugindex = .FALSE. |
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INTEGER idayref |
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REAL t2m(klon, nbsrf), q2m(klon, nbsrf) |
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REAL u10m(klon, nbsrf), v10m(klon, nbsrf) |
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REAL yt2m(klon), yq2m(klon), yu10m(klon) |
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REAL yustar(klon) |
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! -- LOOP |
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REAL yu10mx(klon) |
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REAL yu10my(klon) |
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REAL ywindsp(klon) |
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! -- LOOP |
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REAL yt10m(klon), yq10m(klon) |
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!IM cf. AM : pbl, hbtm (Comme les autres diagnostics on cumule ds |
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! physiq ce qui permet de sortir les grdeurs par sous surface) |
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REAL pblh(klon, nbsrf) |
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REAL plcl(klon, nbsrf) |
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REAL capcl(klon, nbsrf) |
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REAL oliqcl(klon, nbsrf) |
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REAL cteicl(klon, nbsrf) |
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REAL pblt(klon, nbsrf) |
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REAL therm(klon, nbsrf) |
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REAL trmb1(klon, nbsrf) |
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REAL trmb2(klon, nbsrf) |
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REAL trmb3(klon, nbsrf) |
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REAL ypblh(klon) |
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REAL ylcl(klon) |
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REAL ycapcl(klon) |
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REAL yoliqcl(klon) |
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REAL ycteicl(klon) |
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REAL ypblt(klon) |
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REAL ytherm(klon) |
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REAL ytrmb1(klon) |
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REAL ytrmb2(klon) |
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REAL ytrmb3(klon) |
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REAL y_cd_h(klon), y_cd_m(klon) |
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REAL uzon(klon), vmer(klon) |
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REAL tair1(klon), qair1(klon), tairsol(klon) |
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REAL psfce(klon), patm(klon) |
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REAL qairsol(klon), zgeo1(klon) |
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REAL rugo1(klon) |
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! utiliser un jeu de fonctions simples |
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LOGICAL zxli |
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PARAMETER (zxli=.FALSE.) |
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REAL zt, zqs, zdelta, zcor |
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REAL t_coup |
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PARAMETER (t_coup=273.15) |
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CHARACTER (len=20) :: modname = 'clmain' |
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!------------------------------------------------------------ |
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! initialisation Anne |
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ytherm = 0. |
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IF (debugindex .AND. first_appel) THEN |
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first_appel = .FALSE. |
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! initialisation sorties netcdf |
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idayref = day_ini |
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CALL ymds2ju(annee_ref, 1, idayref, 0.0, zjulian) |
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CALL gr_fi_ecrit(1, klon, iim, jjm+1, rlon, zx_lon) |
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DO i = 1, iim |
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zx_lon(i, 1) = rlon(i+1) |
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zx_lon(i, jjm+1) = rlon(i+1) |
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END DO |
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CALL gr_fi_ecrit(1, klon, iim, jjm+1, rlat, zx_lat) |
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cldebug = 'sous_index' |
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CALL histbeg_totreg(cldebug, zx_lon(:, 1), zx_lat(1, :), 1, & |
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iim, 1, jjm+1, itau_phy, zjulian, dtime, nhoridbg, nidbg) |
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! no vertical axis |
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cl_surf(1) = 'ter' |
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cl_surf(2) = 'lic' |
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cl_surf(3) = 'oce' |
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cl_surf(4) = 'sic' |
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DO nsrf = 1, nbsrf |
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CALL histdef(nidbg, cl_surf(nsrf), cl_surf(nsrf), '-', iim, jjm+1, & |
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nhoridbg, 1, 1, 1, -99, 'inst', dtime, dtime) |
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END DO |
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CALL histend(nidbg) |
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CALL histsync(nidbg) |
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END IF |
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DO k = 1, klev ! epaisseur de couche |
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DO i = 1, klon |
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delp(i, k) = paprs(i, k) - paprs(i, k+1) |
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END DO |
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END DO |
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DO i = 1, klon ! vent de la premiere couche |
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zx_alf1 = 1.0 |
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zx_alf2 = 1.0 - zx_alf1 |
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u1lay(i) = u(i, 1)*zx_alf1 + u(i, 2)*zx_alf2 |
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v1lay(i) = v(i, 1)*zx_alf1 + v(i, 2)*zx_alf2 |
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END DO |
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! initialisation: |
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DO i = 1, klon |
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rugmer(i) = 0.0 |
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cdragh(i) = 0.0 |
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cdragm(i) = 0.0 |
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dflux_t(i) = 0.0 |
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dflux_q(i) = 0.0 |
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zu1(i) = 0.0 |
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zv1(i) = 0.0 |
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END DO |
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ypct = 0.0 |
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yts = 0.0 |
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ysnow = 0.0 |
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yqsurf = 0.0 |
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yalb = 0.0 |
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yalblw = 0.0 |
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yrain_f = 0.0 |
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ysnow_f = 0.0 |
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yfder = 0.0 |
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ytaux = 0.0 |
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ytauy = 0.0 |
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ysolsw = 0.0 |
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ysollw = 0.0 |
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ysollwdown = 0.0 |
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yrugos = 0.0 |
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yu1 = 0.0 |
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yv1 = 0.0 |
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yrads = 0.0 |
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ypaprs = 0.0 |
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ypplay = 0.0 |
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ydelp = 0.0 |
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yu = 0.0 |
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yv = 0.0 |
|
|
yt = 0.0 |
|
|
yq = 0.0 |
|
|
pctsrf_new = 0.0 |
|
|
y_flux_u = 0.0 |
|
|
y_flux_v = 0.0 |
|
|
!$$ PB |
|
|
y_dflux_t = 0.0 |
|
|
y_dflux_q = 0.0 |
|
|
ytsoil = 999999. |
|
|
yrugoro = 0. |
|
|
! -- LOOP |
|
|
yu10mx = 0.0 |
|
|
yu10my = 0.0 |
|
|
ywindsp = 0.0 |
|
|
! -- LOOP |
|
|
DO nsrf = 1, nbsrf |
|
|
DO i = 1, klon |
|
|
d_ts(i, nsrf) = 0.0 |
|
|
END DO |
|
|
END DO |
|
|
!§§§ PB |
|
|
yfluxlat = 0. |
|
|
flux_t = 0. |
|
|
flux_q = 0. |
|
|
flux_u = 0. |
|
|
flux_v = 0. |
|
|
DO k = 1, klev |
|
|
DO i = 1, klon |
|
|
d_t(i, k) = 0.0 |
|
|
d_q(i, k) = 0.0 |
|
|
!$$$ flux_t(i, k) = 0.0 |
|
|
!$$$ flux_q(i, k) = 0.0 |
|
|
d_u(i, k) = 0.0 |
|
|
d_v(i, k) = 0.0 |
|
|
!$$$ flux_u(i, k) = 0.0 |
|
|
!$$$ flux_v(i, k) = 0.0 |
|
|
zcoefh(i, k) = 0.0 |
|
|
END DO |
|
|
END DO |
|
|
!AA IF (itr.GE.1) THEN |
|
|
!AA DO it = 1, itr |
|
|
!AA DO k = 1, klev |
|
|
!AA DO i = 1, klon |
|
|
!AA d_tr(i, k, it) = 0.0 |
|
|
!AA ENDDO |
|
|
!AA ENDDO |
|
|
!AA ENDDO |
|
|
!AA ENDIF |
|
|
|
|
|
|
|
|
! Boucler sur toutes les sous-fractions du sol: |
|
|
|
|
|
! Initialisation des "pourcentages potentiels". On considere ici qu'on |
|
|
! peut avoir potentiellementdela glace sur tout le domaine oceanique |
|
|
! (a affiner) |
|
|
|
|
|
pctsrf_pot = pctsrf |
|
|
pctsrf_pot(:, is_oce) = 1. - zmasq |
|
|
pctsrf_pot(:, is_sic) = 1. - zmasq |
|
|
|
|
|
DO nsrf = 1, nbsrf |
|
|
! chercher les indices: |
|
|
ni = 0 |
|
|
knon = 0 |
|
|
DO i = 1, klon |
|
|
! pour determiner le domaine a traiter on utilise les surfaces |
|
|
! "potentielles" |
|
|
IF (pctsrf_pot(i, nsrf) > epsfra) THEN |
|
|
knon = knon + 1 |
|
|
ni(knon) = i |
|
|
END IF |
|
|
END DO |
|
|
|
|
|
! variables pour avoir une sortie IOIPSL des INDEX |
|
|
IF (debugindex) THEN |
|
|
tabindx = 0. |
|
|
DO i = 1, knon |
|
|
tabindx(i) = real(i) |
|
|
END DO |
|
|
debugtab = 0. |
|
|
ndexbg = 0 |
|
|
CALL gath2cpl(tabindx, debugtab, klon, knon, iim, jjm, ni) |
|
|
CALL histwrite(nidbg, cl_surf(nsrf), itap, debugtab) |
|
|
END IF |
|
|
|
|
|
IF (knon==0) CYCLE |
|
|
|
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
ypct(j) = pctsrf(i, nsrf) |
|
|
yts(j) = ts(i, nsrf) |
|
|
ytslab(i) = tslab(i) |
|
|
ysnow(j) = snow(i, nsrf) |
|
|
yqsurf(j) = qsurf(i, nsrf) |
|
|
yalb(j) = albe(i, nsrf) |
|
|
yalblw(j) = alblw(i, nsrf) |
|
|
yrain_f(j) = rain_f(i) |
|
|
ysnow_f(j) = snow_f(i) |
|
|
yagesno(j) = agesno(i, nsrf) |
|
|
yfder(j) = fder(i) |
|
|
ytaux(j) = flux_u(i, 1, nsrf) |
|
|
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) |
|
|
yu10mx(j) = u10m(i, nsrf) |
|
|
yu10my(j) = v10m(i, nsrf) |
|
|
ywindsp(j) = sqrt(yu10mx(j)*yu10mx(j)+yu10my(j)*yu10my(j)) |
|
|
END DO |
|
|
|
|
|
! IF bucket model for continent, copy soil water content |
|
|
IF (nsrf==is_ter .AND. .NOT. ok_veget) THEN |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
yqsol(j) = qsol(i) |
|
|
END DO |
|
|
ELSE |
|
|
yqsol = 0. |
|
|
END IF |
|
|
!$$$ 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) |
|
|
END DO |
|
|
END DO |
|
|
|
|
|
! calculer Cdrag et les coefficients d'echange |
|
|
CALL coefkz(nsrf, knon, ypaprs, ypplay, ksta, ksta_ter, yts,& |
|
|
yrugos, yu, yv, yt, yq, yqsurf, ycoefm, ycoefh) |
|
|
!IM 081204 BEG |
|
|
!CR test |
|
|
IF (iflag_pbl==1) THEN |
|
|
!IM 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)) |
|
|
END DO |
|
|
END DO |
|
|
END IF |
|
|
|
|
|
!IM cf JLD : on seuille ycoefm et ycoefh |
|
|
IF (nsrf==is_oce) THEN |
|
|
DO j = 1, knon |
|
|
! ycoefm(j, 1)=min(ycoefm(j, 1), 1.1E-3) |
|
|
ycoefm(j, 1) = min(ycoefm(j, 1), cdmmax) |
|
|
! ycoefh(j, 1)=min(ycoefh(j, 1), 1.1E-3) |
|
|
ycoefh(j, 1) = min(ycoefh(j, 1), cdhmax) |
|
|
END DO |
|
|
END IF |
|
|
|
|
|
|
|
|
!IM: 261103 |
|
|
IF (ok_kzmin) THEN |
|
|
!IM cf FH: 201103 BEG |
|
|
! Calcul d'une diffusion minimale pour les conditions tres stables. |
|
|
CALL coefkzmin(knon, ypaprs, ypplay, yu, yv, yt, yq, ycoefm, ycoefm0, & |
|
|
ycoefh0) |
|
|
! call dump2d(iim, jjm-1, ycoefm(2:klon-1, 2), 'KZ ') |
|
|
! call dump2d(iim, jjm-1, ycoefm0(2:klon-1, 2), 'KZMIN ') |
|
|
|
|
|
IF (1==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)) |
|
|
END DO |
|
|
END DO |
|
|
END IF |
|
|
!IM cf FH: 201103 END |
|
|
!IM: 261103 |
|
|
END IF !ok_kzmin |
|
|
|
|
|
IF (iflag_pbl>=3) THEN |
|
|
|
|
|
!ccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
! MELLOR ET YAMADA adapte a Mars Richard Fournier et Frederic Hourdin |
|
|
!ccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
|
|
|
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 |
|
|
END DO |
|
|
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)) |
|
|
END DO |
|
|
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)) |
|
|
END DO |
|
|
DO k = 1, klev + 1 |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
yq2(j, k) = q2(i, k, nsrf) |
|
|
END DO |
|
|
END DO |
|
|
|
|
|
|
|
|
! Bug introduit volontairement pour converger avec les resultats |
|
|
! du papier sur les thermiques. |
|
|
IF (1==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) |
|
|
END IF |
|
|
CALL ustarhb(knon, yu, yv, y_cd_m, yustar) |
|
|
|
|
|
IF (prt_level>9) THEN |
|
|
PRINT *, 'USTAR = ', yustar |
|
|
END IF |
|
|
|
|
|
! iflag_pbl peut etre utilise comme longuer de melange |
|
|
|
|
|
IF (iflag_pbl>=11) THEN |
|
|
CALL vdif_kcay(knon, dtime, rg, rd, ypaprs, yt, yzlev, yzlay, yu, yv, yteta, & |
|
|
y_cd_m, yq2, q2diag, ykmm, ykmn, yustar, iflag_pbl) |
|
|
ELSE |
|
|
CALL yamada4(knon, dtime, rg, rd, ypaprs, yt, yzlev, yzlay, yu, yv, yteta, & |
|
|
y_cd_m, yq2, ykmm, ykmn, ykmq, yustar, iflag_pbl) |
|
|
END IF |
|
|
|
|
|
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) |
|
|
|
|
|
|
|
|
END IF |
|
|
|
|
|
!ccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
! calculer la diffusion des vitesses "u" et "v" |
|
|
!ccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc |
|
|
|
|
|
CALL clvent(knon, dtime, yu1, yv1, ycoefm, yt, yu, ypaprs, ypplay, & |
|
|
ydelp, y_d_u, y_flux_u) |
|
|
CALL clvent(knon, dtime, yu1, yv1, ycoefm, yt, yv, ypaprs, ypplay, & |
|
|
ydelp, y_d_v, y_flux_v) |
|
|
|
|
|
! pour le couplage |
|
|
ytaux = y_flux_u(:, 1) |
|
|
ytauy = y_flux_v(:, 1) |
|
|
|
|
|
! FH modif sur le cdrag temperature |
|
|
!$$$PB : déplace dans clcdrag |
|
|
!$$$ do i=1, knon |
|
|
!$$$ ycoefh(i, 1)=ycoefm(i, 1)*0.8 |
|
|
!$$$ enddo |
|
|
|
|
|
! calculer la diffusion de "q" et de "h" |
|
|
CALL clqh(dtime, itap, date0, jour, debut, lafin, rlon, rlat,& |
|
|
cufi, cvfi, knon, nsrf, ni, pctsrf, soil_model, ytsoil,& |
|
|
yqsol, ok_veget, ocean, npas, nexca, rmu0, co2_ppm, yrugos,& |
|
|
yrugoro, yu1, yv1, ycoefh, yt, yq, yts, ypaprs, ypplay,& |
|
|
ydelp, yrads, yalb, yalblw, ysnow, yqsurf, yrain_f, ysnow_f, & |
|
|
yfder, ytaux, ytauy, ywindsp, ysollw, ysollwdown, ysolsw,& |
|
|
yfluxlat, pctsrf_new, yagesno, y_d_t, y_d_q, y_d_ts,& |
|
|
yz0_new, y_flux_t, y_flux_q, y_dflux_t, y_dflux_q,& |
|
|
y_fqcalving, y_ffonte, y_run_off_lic_0, y_flux_o, y_flux_g,& |
|
|
ytslab, y_seaice) |
|
|
|
|
|
! calculer la longueur de rugosite sur ocean |
|
|
yrugm = 0. |
|
|
IF (nsrf==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)) |
|
|
END DO |
|
|
END IF |
|
|
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) |
|
|
END DO |
|
|
|
|
|
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) |
|
|
!§§§ 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) |
|
|
!$$$ PB y_flux_t(j, k) = y_flux_t(j, k) * ypct(j) |
|
|
!$$$ 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) |
|
|
!$$$ PB y_flux_u(j, k) = y_flux_u(j, k) * ypct(j) |
|
|
!$$$ PB y_flux_v(j, k) = y_flux_v(j, k) * ypct(j) |
|
|
END DO |
|
|
END DO |
|
|
|
|
|
|
|
|
evap(:, nsrf) = -flux_q(:, 1, nsrf) |
|
|
|
|
|
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) |
|
|
!$$$ pb rugmer(i) = yrugm(j) |
|
|
IF (nsrf==is_oce) THEN |
|
|
rugmer(i) = yrugm(j) |
|
|
rugos(i, nsrf) = yrugm(j) |
|
|
END IF |
|
|
!IM cf JLD ?? |
|
|
agesno(i, nsrf) = yagesno(j) |
|
|
fqcalving(i, nsrf) = y_fqcalving(j) |
|
|
ffonte(i, nsrf) = y_ffonte(j) |
|
|
cdragh(i) = cdragh(i) + ycoefh(j, 1) |
|
|
cdragm(i) = cdragm(i) + ycoefm(j, 1) |
|
|
dflux_t(i) = dflux_t(i) + y_dflux_t(j) |
|
|
dflux_q(i) = dflux_q(i) + y_dflux_q(j) |
|
|
zu1(i) = zu1(i) + yu1(j) |
|
|
zv1(i) = zv1(i) + yv1(j) |
|
|
END DO |
|
|
IF (nsrf==is_ter) THEN |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
qsol(i) = yqsol(j) |
|
|
END DO |
|
|
END IF |
|
|
IF (nsrf==is_lic) THEN |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
run_off_lic_0(i) = y_run_off_lic_0(j) |
|
|
END DO |
|
|
END IF |
|
|
!$$$ 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 |
|
|
|
|
|
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) |
|
|
!$$$ PB flux_t(i, k) = flux_t(i, k) + y_flux_t(j, k) |
|
|
!$$$ 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) |
|
|
!$$$ PB flux_u(i, k) = flux_u(i, k) + y_flux_u(j, k) |
|
|
!$$$ flux_v(i, k) = flux_v(i, k) + y_flux_v(j, k) |
|
|
zcoefh(i, k) = zcoefh(i, k) + ycoefh(j, k) |
|
|
END DO |
|
|
END DO |
|
|
|
|
|
|
|
|
!cc diagnostic t, q a 2m et u, v a 10m |
|
|
|
|
|
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==is_oce) THEN |
|
|
rugo1(j) = rugos(i, nsrf) |
|
|
END IF |
|
|
psfce(j) = ypaprs(j, 1) |
|
|
patm(j) = ypplay(j, 1) |
|
|
|
|
|
qairsol(j) = yqsurf(j) |
|
|
END DO |
|
|
|
|
|
CALL stdlevvar(klon, knon, nsrf, zxli, uzon, vmer, tair1, qair1, zgeo1, & |
|
|
tairsol, qairsol, rugo1, psfce, patm, yt2m, yq2m, yt10m, yq10m, & |
|
|
yu10m, yustar) |
|
|
!IM 081204 END |
|
|
|
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
t2m(i, nsrf) = yt2m(j) |
|
|
q2m(i, nsrf) = yq2m(j) |
|
|
|
|
|
! 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) |
|
|
|
|
|
END DO |
|
|
|
|
|
DO i = 1, knon |
|
|
y_cd_h(i) = ycoefh(i, 1) |
|
|
y_cd_m(i) = ycoefm(i, 1) |
|
|
END DO |
|
|
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) |
|
|
|
|
|
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) |
|
|
END DO |
|
|
|
|
|
|
|
|
DO j = 1, knon |
|
|
DO k = 1, klev + 1 |
|
|
i = ni(j) |
|
|
q2(i, k, nsrf) = yq2(j, k) |
|
|
END DO |
|
|
END DO |
|
|
!IM "slab" ocean |
|
|
IF (nsrf==is_oce) THEN |
|
|
DO j = 1, knon |
|
|
! on projette sur la grille globale |
|
|
i = ni(j) |
|
|
IF (pctsrf_new(i, is_oce)>epsfra) THEN |
|
|
flux_o(i) = y_flux_o(j) |
|
|
ELSE |
|
|
flux_o(i) = 0. |
|
|
END IF |
|
|
END DO |
|
|
END IF |
|
|
|
|
|
IF (nsrf==is_sic) THEN |
|
|
DO j = 1, knon |
|
|
i = ni(j) |
|
|
!IM 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)>epsfra) THEN |
|
|
flux_g(i) = y_flux_g(j) |
|
|
ELSE |
|
|
flux_g(i) = 0. |
|
|
END IF |
|
|
END DO |
|
|
|
|
|
END IF |
|
|
!nsrf.EQ.is_sic |
|
|
IF (ocean=='slab ') THEN |
|
|
IF (nsrf==is_oce) THEN |
|
|
tslab(1:klon) = ytslab(1:klon) |
|
|
seaice(1:klon) = y_seaice(1:klon) |
|
|
!nsrf |
|
|
END IF |
|
|
!OCEAN |
|
|
END IF |
|
|
END DO |
|
| 6 |
|
|
| 7 |
! On utilise les nouvelles surfaces |
SUBROUTINE clmain(dtime, itap, pctsrf, pctsrf_new, t, q, u, v, jour, rmu0, & |
| 8 |
! A rajouter: conservation de l'albedo |
co2_ppm, ts, cdmmax, cdhmax, ksta, ksta_ter, ok_kzmin, ftsoil, qsol, & |
| 9 |
|
paprs, pplay, snow, qsurf, evap, albe, alblw, fluxlat, rain_fall, & |
| 10 |
|
snow_f, solsw, sollw, fder, rlat, rugos, debut, agesno, rugoro, d_t, & |
| 11 |
|
d_q, d_u, d_v, d_ts, flux_t, flux_q, flux_u, flux_v, cdragh, cdragm, & |
| 12 |
|
q2, dflux_t, dflux_q, ycoefh, zu1, zv1, t2m, q2m, u10m, v10m, pblh, & |
| 13 |
|
capcl, oliqcl, cteicl, pblt, therm, trmb1, trmb2, trmb3, plcl, & |
| 14 |
|
fqcalving, ffonte, run_off_lic_0, flux_o, flux_g, tslab) |
| 15 |
|
|
| 16 |
|
! From phylmd/clmain.F, version 1.6, 2005/11/16 14:47:19 |
| 17 |
|
! Author: Z. X. Li (LMD/CNRS), date: 1993/08/18 |
| 18 |
|
! Objet : interface de couche limite (diffusion verticale) |
| 19 |
|
|
| 20 |
|
! Tout ce qui a trait aux traceurs est dans "phytrac". Le calcul |
| 21 |
|
! de la couche limite pour les traceurs se fait avec "cltrac" et |
| 22 |
|
! ne tient pas compte de la différentiation des sous-fractions de |
| 23 |
|
! sol. |
| 24 |
|
|
| 25 |
|
! Pour pouvoir extraire les coefficients d'échanges et le vent |
| 26 |
|
! dans la première couche, trois champs ont été créés : "ycoefh", |
| 27 |
|
! "zu1" et "zv1". Nous avons moyenné les valeurs de ces trois |
| 28 |
|
! champs sur les quatre sous-surfaces du modèle. |
| 29 |
|
|
| 30 |
|
use clqh_m, only: clqh |
| 31 |
|
use clvent_m, only: clvent |
| 32 |
|
use coefkz_m, only: coefkz |
| 33 |
|
use coefkzmin_m, only: coefkzmin |
| 34 |
|
USE conf_gcm_m, ONLY: prt_level |
| 35 |
|
USE conf_phys_m, ONLY: iflag_pbl |
| 36 |
|
USE dimens_m, ONLY: iim, jjm |
| 37 |
|
USE dimphy, ONLY: klev, klon, zmasq |
| 38 |
|
USE dimsoil, ONLY: nsoilmx |
| 39 |
|
use hbtm_m, only: hbtm |
| 40 |
|
USE indicesol, ONLY: epsfra, is_lic, is_oce, is_sic, is_ter, nbsrf |
| 41 |
|
USE suphec_m, ONLY: rd, rg, rkappa |
| 42 |
|
use ustarhb_m, only: ustarhb |
| 43 |
|
use vdif_kcay_m, only: vdif_kcay |
| 44 |
|
use yamada4_m, only: yamada4 |
| 45 |
|
|
| 46 |
|
REAL, INTENT(IN):: dtime ! interval du temps (secondes) |
| 47 |
|
INTEGER, INTENT(IN):: itap ! numero du pas de temps |
| 48 |
|
REAL, INTENT(inout):: pctsrf(klon, nbsrf) |
| 49 |
|
|
| 50 |
|
! la nouvelle repartition des surfaces sortie de l'interface |
| 51 |
|
REAL, INTENT(out):: pctsrf_new(klon, nbsrf) |
| 52 |
|
|
| 53 |
|
REAL, INTENT(IN):: t(klon, klev) ! temperature (K) |
| 54 |
|
REAL, INTENT(IN):: q(klon, klev) ! vapeur d'eau (kg/kg) |
| 55 |
|
REAL, INTENT(IN):: u(klon, klev), v(klon, klev) ! vitesse |
| 56 |
|
INTEGER, INTENT(IN):: jour ! jour de l'annee en cours |
| 57 |
|
REAL, intent(in):: rmu0(klon) ! cosinus de l'angle solaire zenithal |
| 58 |
|
REAL, intent(in):: co2_ppm ! taux CO2 atmosphere |
| 59 |
|
REAL, INTENT(IN):: ts(klon, nbsrf) ! input-R- temperature du sol (en Kelvin) |
| 60 |
|
REAL, INTENT(IN):: cdmmax, cdhmax ! seuils cdrm, cdrh |
| 61 |
|
REAL, INTENT(IN):: ksta, ksta_ter |
| 62 |
|
LOGICAL, INTENT(IN):: ok_kzmin |
| 63 |
|
REAL ftsoil(klon, nsoilmx, nbsrf) |
| 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 snow(klon, nbsrf) |
| 71 |
|
REAL qsurf(klon, nbsrf) |
| 72 |
|
REAL evap(klon, nbsrf) |
| 73 |
|
REAL albe(klon, nbsrf) |
| 74 |
|
REAL alblw(klon, nbsrf) |
| 75 |
|
|
| 76 |
|
REAL fluxlat(klon, nbsrf) |
| 77 |
|
|
| 78 |
|
REAL, intent(in):: rain_fall(klon) |
| 79 |
|
! liquid water mass flux (kg/m2/s), positive down |
| 80 |
|
|
| 81 |
|
REAL, intent(in):: snow_f(klon) |
| 82 |
|
! solid water mass flux (kg/m2/s), positive down |
| 83 |
|
|
| 84 |
|
REAL, INTENT(IN):: solsw(klon, nbsrf), sollw(klon, nbsrf) |
| 85 |
|
REAL fder(klon) |
| 86 |
|
REAL, INTENT(IN):: rlat(klon) ! latitude en degrés |
| 87 |
|
|
| 88 |
|
REAL rugos(klon, nbsrf) |
| 89 |
|
! rugos----input-R- longeur de rugosite (en m) |
| 90 |
|
|
| 91 |
|
LOGICAL, INTENT(IN):: debut |
| 92 |
|
real agesno(klon, nbsrf) |
| 93 |
|
REAL, INTENT(IN):: rugoro(klon) |
| 94 |
|
|
| 95 |
|
REAL d_t(klon, klev), d_q(klon, klev) |
| 96 |
|
! d_t------output-R- le changement pour "t" |
| 97 |
|
! d_q------output-R- le changement pour "q" |
| 98 |
|
|
| 99 |
|
REAL, intent(out):: d_u(klon, klev), d_v(klon, klev) |
| 100 |
|
! changement pour "u" et "v" |
| 101 |
|
|
| 102 |
|
REAL d_ts(klon, nbsrf) |
| 103 |
|
! d_ts-----output-R- le changement pour "ts" |
| 104 |
|
|
| 105 |
|
REAL flux_t(klon, klev, nbsrf), flux_q(klon, klev, nbsrf) |
| 106 |
|
! flux_t---output-R- flux de chaleur sensible (CpT) J/m**2/s (W/m**2) |
| 107 |
|
! (orientation positive vers le bas) |
| 108 |
|
! flux_q---output-R- flux de vapeur d'eau (kg/m**2/s) |
| 109 |
|
|
| 110 |
|
REAL flux_u(klon, klev, nbsrf), flux_v(klon, klev, nbsrf) |
| 111 |
|
! flux_u---output-R- tension du vent X: (kg m/s)/(m**2 s) ou Pascal |
| 112 |
|
! flux_v---output-R- tension du vent Y: (kg m/s)/(m**2 s) ou Pascal |
| 113 |
|
|
| 114 |
|
REAL, INTENT(out):: cdragh(klon), cdragm(klon) |
| 115 |
|
real q2(klon, klev+1, nbsrf) |
| 116 |
|
|
| 117 |
|
REAL, INTENT(out):: dflux_t(klon), dflux_q(klon) |
| 118 |
|
! dflux_t derive du flux sensible |
| 119 |
|
! dflux_q derive du flux latent |
| 120 |
|
!IM "slab" ocean |
| 121 |
|
|
| 122 |
|
REAL, intent(out):: ycoefh(klon, klev) |
| 123 |
|
REAL, intent(out):: zu1(klon) |
| 124 |
|
REAL zv1(klon) |
| 125 |
|
REAL t2m(klon, nbsrf), q2m(klon, nbsrf) |
| 126 |
|
REAL u10m(klon, nbsrf), v10m(klon, nbsrf) |
| 127 |
|
|
| 128 |
|
!IM cf. AM : pbl, hbtm (Comme les autres diagnostics on cumule ds |
| 129 |
|
! physiq ce qui permet de sortir les grdeurs par sous surface) |
| 130 |
|
REAL pblh(klon, nbsrf) |
| 131 |
|
! pblh------- HCL |
| 132 |
|
REAL capcl(klon, nbsrf) |
| 133 |
|
REAL oliqcl(klon, nbsrf) |
| 134 |
|
REAL cteicl(klon, nbsrf) |
| 135 |
|
REAL pblt(klon, nbsrf) |
| 136 |
|
! pblT------- T au nveau HCL |
| 137 |
|
REAL therm(klon, nbsrf) |
| 138 |
|
REAL trmb1(klon, nbsrf) |
| 139 |
|
! trmb1-------deep_cape |
| 140 |
|
REAL trmb2(klon, nbsrf) |
| 141 |
|
! trmb2--------inhibition |
| 142 |
|
REAL trmb3(klon, nbsrf) |
| 143 |
|
! trmb3-------Point Omega |
| 144 |
|
REAL plcl(klon, nbsrf) |
| 145 |
|
REAL fqcalving(klon, nbsrf), ffonte(klon, nbsrf) |
| 146 |
|
! ffonte----Flux thermique utilise pour fondre la neige |
| 147 |
|
! fqcalving-Flux d'eau "perdue" par la surface et necessaire pour limiter la |
| 148 |
|
! hauteur de neige, en kg/m2/s |
| 149 |
|
REAL run_off_lic_0(klon) |
| 150 |
|
|
| 151 |
|
REAL flux_o(klon), flux_g(klon) |
| 152 |
|
!IM "slab" ocean |
| 153 |
|
! flux_g---output-R- flux glace (pour OCEAN='slab ') |
| 154 |
|
! flux_o---output-R- flux ocean (pour OCEAN='slab ') |
| 155 |
|
|
| 156 |
|
REAL tslab(klon) |
| 157 |
|
! tslab-in/output-R temperature du slab ocean (en Kelvin) |
| 158 |
|
! uniqmnt pour slab |
| 159 |
|
|
| 160 |
|
! Local: |
| 161 |
|
|
| 162 |
|
REAL y_flux_o(klon), y_flux_g(klon) |
| 163 |
|
real ytslab(klon) |
| 164 |
|
REAL y_fqcalving(klon), y_ffonte(klon) |
| 165 |
|
real y_run_off_lic_0(klon) |
| 166 |
|
|
| 167 |
|
REAL rugmer(klon) |
| 168 |
|
|
| 169 |
|
REAL ytsoil(klon, nsoilmx) |
| 170 |
|
|
| 171 |
|
REAL yts(klon), yrugos(klon), ypct(klon), yz0_new(klon) |
| 172 |
|
REAL yalb(klon) |
| 173 |
|
REAL yalblw(klon) |
| 174 |
|
REAL yu1(klon), yv1(klon) |
| 175 |
|
! on rajoute en output yu1 et yv1 qui sont les vents dans |
| 176 |
|
! la premiere couche |
| 177 |
|
REAL ysnow(klon), yqsurf(klon), yagesno(klon) |
| 178 |
|
|
| 179 |
|
real yqsol(klon) |
| 180 |
|
! column-density of water in soil, in kg m-2 |
| 181 |
|
|
| 182 |
|
REAL yrain_f(klon) |
| 183 |
|
! liquid water mass flux (kg/m2/s), positive down |
| 184 |
|
|
| 185 |
|
REAL ysnow_f(klon) |
| 186 |
|
! solid water mass flux (kg/m2/s), positive down |
| 187 |
|
|
| 188 |
|
REAL ysollw(klon), ysolsw(klon) |
| 189 |
|
REAL yfder(klon) |
| 190 |
|
REAL yrugm(klon), yrads(klon), yrugoro(klon) |
| 191 |
|
|
| 192 |
|
REAL yfluxlat(klon) |
| 193 |
|
|
| 194 |
|
REAL y_d_ts(klon) |
| 195 |
|
REAL y_d_t(klon, klev), y_d_q(klon, klev) |
| 196 |
|
REAL y_d_u(klon, klev), y_d_v(klon, klev) |
| 197 |
|
REAL y_flux_t(klon, klev), y_flux_q(klon, klev) |
| 198 |
|
REAL y_flux_u(klon, klev), y_flux_v(klon, klev) |
| 199 |
|
REAL y_dflux_t(klon), y_dflux_q(klon) |
| 200 |
|
REAL coefh(klon, klev), coefm(klon, klev) |
| 201 |
|
REAL yu(klon, klev), yv(klon, klev) |
| 202 |
|
REAL yt(klon, klev), yq(klon, klev) |
| 203 |
|
REAL ypaprs(klon, klev+1), ypplay(klon, klev), ydelp(klon, klev) |
| 204 |
|
|
| 205 |
|
REAL ycoefm0(klon, klev), ycoefh0(klon, klev) |
| 206 |
|
|
| 207 |
|
REAL yzlay(klon, klev), yzlev(klon, klev+1), yteta(klon, klev) |
| 208 |
|
REAL ykmm(klon, klev+1), ykmn(klon, klev+1) |
| 209 |
|
REAL ykmq(klon, klev+1) |
| 210 |
|
REAL yq2(klon, klev+1) |
| 211 |
|
REAL q2diag(klon, klev+1) |
| 212 |
|
|
| 213 |
|
REAL u1lay(klon), v1lay(klon) |
| 214 |
|
REAL delp(klon, klev) |
| 215 |
|
INTEGER i, k, nsrf |
| 216 |
|
|
| 217 |
|
INTEGER ni(klon), knon, j |
| 218 |
|
|
| 219 |
|
REAL pctsrf_pot(klon, nbsrf) |
| 220 |
|
! "pourcentage potentiel" pour tenir compte des éventuelles |
| 221 |
|
! apparitions ou disparitions de la glace de mer |
| 222 |
|
|
| 223 |
|
REAL zx_alf1, zx_alf2 !valeur ambiante par extrapola. |
| 224 |
|
|
| 225 |
|
REAL yt2m(klon), yq2m(klon), yu10m(klon) |
| 226 |
|
REAL yustar(klon) |
| 227 |
|
! -- LOOP |
| 228 |
|
REAL yu10mx(klon) |
| 229 |
|
REAL yu10my(klon) |
| 230 |
|
REAL ywindsp(klon) |
| 231 |
|
! -- LOOP |
| 232 |
|
|
| 233 |
|
REAL yt10m(klon), yq10m(klon) |
| 234 |
|
REAL ypblh(klon) |
| 235 |
|
REAL ylcl(klon) |
| 236 |
|
REAL ycapcl(klon) |
| 237 |
|
REAL yoliqcl(klon) |
| 238 |
|
REAL ycteicl(klon) |
| 239 |
|
REAL ypblt(klon) |
| 240 |
|
REAL ytherm(klon) |
| 241 |
|
REAL ytrmb1(klon) |
| 242 |
|
REAL ytrmb2(klon) |
| 243 |
|
REAL ytrmb3(klon) |
| 244 |
|
REAL uzon(klon), vmer(klon) |
| 245 |
|
REAL tair1(klon), qair1(klon), tairsol(klon) |
| 246 |
|
REAL psfce(klon), patm(klon) |
| 247 |
|
|
| 248 |
|
REAL qairsol(klon), zgeo1(klon) |
| 249 |
|
REAL rugo1(klon) |
| 250 |
|
|
| 251 |
|
! utiliser un jeu de fonctions simples |
| 252 |
|
LOGICAL zxli |
| 253 |
|
PARAMETER (zxli=.FALSE.) |
| 254 |
|
|
| 255 |
|
!------------------------------------------------------------ |
| 256 |
|
|
| 257 |
|
ytherm = 0. |
| 258 |
|
|
| 259 |
|
DO k = 1, klev ! epaisseur de couche |
| 260 |
|
DO i = 1, klon |
| 261 |
|
delp(i, k) = paprs(i, k) - paprs(i, k+1) |
| 262 |
|
END DO |
| 263 |
|
END DO |
| 264 |
|
DO i = 1, klon ! vent de la premiere couche |
| 265 |
|
zx_alf1 = 1.0 |
| 266 |
|
zx_alf2 = 1.0 - zx_alf1 |
| 267 |
|
u1lay(i) = u(i, 1)*zx_alf1 + u(i, 2)*zx_alf2 |
| 268 |
|
v1lay(i) = v(i, 1)*zx_alf1 + v(i, 2)*zx_alf2 |
| 269 |
|
END DO |
| 270 |
|
|
| 271 |
|
! Initialization: |
| 272 |
|
rugmer = 0. |
| 273 |
|
cdragh = 0. |
| 274 |
|
cdragm = 0. |
| 275 |
|
dflux_t = 0. |
| 276 |
|
dflux_q = 0. |
| 277 |
|
zu1 = 0. |
| 278 |
|
zv1 = 0. |
| 279 |
|
ypct = 0. |
| 280 |
|
yts = 0. |
| 281 |
|
ysnow = 0. |
| 282 |
|
yqsurf = 0. |
| 283 |
|
yalb = 0. |
| 284 |
|
yalblw = 0. |
| 285 |
|
yrain_f = 0. |
| 286 |
|
ysnow_f = 0. |
| 287 |
|
yfder = 0. |
| 288 |
|
ysolsw = 0. |
| 289 |
|
ysollw = 0. |
| 290 |
|
yrugos = 0. |
| 291 |
|
yu1 = 0. |
| 292 |
|
yv1 = 0. |
| 293 |
|
yrads = 0. |
| 294 |
|
ypaprs = 0. |
| 295 |
|
ypplay = 0. |
| 296 |
|
ydelp = 0. |
| 297 |
|
yu = 0. |
| 298 |
|
yv = 0. |
| 299 |
|
yt = 0. |
| 300 |
|
yq = 0. |
| 301 |
|
pctsrf_new = 0. |
| 302 |
|
y_flux_u = 0. |
| 303 |
|
y_flux_v = 0. |
| 304 |
|
y_dflux_t = 0. |
| 305 |
|
y_dflux_q = 0. |
| 306 |
|
ytsoil = 999999. |
| 307 |
|
yrugoro = 0. |
| 308 |
|
! -- LOOP |
| 309 |
|
yu10mx = 0. |
| 310 |
|
yu10my = 0. |
| 311 |
|
ywindsp = 0. |
| 312 |
|
! -- LOOP |
| 313 |
|
d_ts = 0. |
| 314 |
|
yfluxlat = 0. |
| 315 |
|
flux_t = 0. |
| 316 |
|
flux_q = 0. |
| 317 |
|
flux_u = 0. |
| 318 |
|
flux_v = 0. |
| 319 |
|
d_t = 0. |
| 320 |
|
d_q = 0. |
| 321 |
|
d_u = 0. |
| 322 |
|
d_v = 0. |
| 323 |
|
ycoefh = 0. |
| 324 |
|
|
| 325 |
|
! Initialisation des "pourcentages potentiels". On considère ici qu'on |
| 326 |
|
! peut avoir potentiellement de la glace sur tout le domaine océanique |
| 327 |
|
! (à affiner) |
| 328 |
|
|
| 329 |
|
pctsrf_pot = pctsrf |
| 330 |
|
pctsrf_pot(:, is_oce) = 1. - zmasq |
| 331 |
|
pctsrf_pot(:, is_sic) = 1. - zmasq |
| 332 |
|
|
| 333 |
|
! Boucler sur toutes les sous-fractions du sol: |
| 334 |
|
|
| 335 |
|
loop_surface: DO nsrf = 1, nbsrf |
| 336 |
|
! Chercher les indices : |
| 337 |
|
ni = 0 |
| 338 |
|
knon = 0 |
| 339 |
|
DO i = 1, klon |
| 340 |
|
! Pour déterminer le domaine à traiter, on utilise les surfaces |
| 341 |
|
! "potentielles" |
| 342 |
|
IF (pctsrf_pot(i, nsrf) > epsfra) THEN |
| 343 |
|
knon = knon + 1 |
| 344 |
|
ni(knon) = i |
| 345 |
|
END IF |
| 346 |
|
END DO |
| 347 |
|
|
| 348 |
|
if_knon: IF (knon /= 0) then |
| 349 |
|
DO j = 1, knon |
| 350 |
|
i = ni(j) |
| 351 |
|
ypct(j) = pctsrf(i, nsrf) |
| 352 |
|
yts(j) = ts(i, nsrf) |
| 353 |
|
ytslab(i) = tslab(i) |
| 354 |
|
ysnow(j) = snow(i, nsrf) |
| 355 |
|
yqsurf(j) = qsurf(i, nsrf) |
| 356 |
|
yalb(j) = albe(i, nsrf) |
| 357 |
|
yalblw(j) = alblw(i, nsrf) |
| 358 |
|
yrain_f(j) = rain_fall(i) |
| 359 |
|
ysnow_f(j) = snow_f(i) |
| 360 |
|
yagesno(j) = agesno(i, nsrf) |
| 361 |
|
yfder(j) = fder(i) |
| 362 |
|
ysolsw(j) = solsw(i, nsrf) |
| 363 |
|
ysollw(j) = sollw(i, nsrf) |
| 364 |
|
yrugos(j) = rugos(i, nsrf) |
| 365 |
|
yrugoro(j) = rugoro(i) |
| 366 |
|
yu1(j) = u1lay(i) |
| 367 |
|
yv1(j) = v1lay(i) |
| 368 |
|
yrads(j) = ysolsw(j) + ysollw(j) |
| 369 |
|
ypaprs(j, klev+1) = paprs(i, klev+1) |
| 370 |
|
y_run_off_lic_0(j) = run_off_lic_0(i) |
| 371 |
|
yu10mx(j) = u10m(i, nsrf) |
| 372 |
|
yu10my(j) = v10m(i, nsrf) |
| 373 |
|
ywindsp(j) = sqrt(yu10mx(j)*yu10mx(j)+yu10my(j)*yu10my(j)) |
| 374 |
|
END DO |
| 375 |
|
|
| 376 |
|
! For continent, copy soil water content |
| 377 |
|
IF (nsrf == is_ter) THEN |
| 378 |
|
yqsol(:knon) = qsol(ni(:knon)) |
| 379 |
|
ELSE |
| 380 |
|
yqsol = 0. |
| 381 |
|
END IF |
| 382 |
|
|
| 383 |
|
DO k = 1, nsoilmx |
| 384 |
|
DO j = 1, knon |
| 385 |
|
i = ni(j) |
| 386 |
|
ytsoil(j, k) = ftsoil(i, k, nsrf) |
| 387 |
|
END DO |
| 388 |
|
END DO |
| 389 |
|
|
| 390 |
|
DO k = 1, klev |
| 391 |
|
DO j = 1, knon |
| 392 |
|
i = ni(j) |
| 393 |
|
ypaprs(j, k) = paprs(i, k) |
| 394 |
|
ypplay(j, k) = pplay(i, k) |
| 395 |
|
ydelp(j, k) = delp(i, k) |
| 396 |
|
yu(j, k) = u(i, k) |
| 397 |
|
yv(j, k) = v(i, k) |
| 398 |
|
yt(j, k) = t(i, k) |
| 399 |
|
yq(j, k) = q(i, k) |
| 400 |
|
END DO |
| 401 |
|
END DO |
| 402 |
|
|
| 403 |
|
! calculer Cdrag et les coefficients d'echange |
| 404 |
|
CALL coefkz(nsrf, knon, ypaprs, ypplay, ksta, ksta_ter, yts, yrugos, & |
| 405 |
|
yu, yv, yt, yq, yqsurf, coefm(:knon, :), coefh(:knon, :)) |
| 406 |
|
IF (iflag_pbl == 1) THEN |
| 407 |
|
CALL coefkz2(nsrf, knon, ypaprs, ypplay, yt, ycoefm0, ycoefh0) |
| 408 |
|
coefm(:knon, :) = max(coefm(:knon, :), ycoefm0(:knon, :)) |
| 409 |
|
coefh(:knon, :) = max(coefh(:knon, :), ycoefh0(:knon, :)) |
| 410 |
|
END IF |
| 411 |
|
|
| 412 |
|
! on met un seuil pour coefm et coefh |
| 413 |
|
IF (nsrf == is_oce) THEN |
| 414 |
|
coefm(:knon, 1) = min(coefm(:knon, 1), cdmmax) |
| 415 |
|
coefh(:knon, 1) = min(coefh(:knon, 1), cdhmax) |
| 416 |
|
END IF |
| 417 |
|
|
| 418 |
|
IF (ok_kzmin) THEN |
| 419 |
|
! Calcul d'une diffusion minimale pour les conditions tres stables |
| 420 |
|
CALL coefkzmin(knon, ypaprs, ypplay, yu, yv, yt, yq, & |
| 421 |
|
coefm(:knon, 1), ycoefm0, ycoefh0) |
| 422 |
|
coefm(:knon, :) = max(coefm(:knon, :), ycoefm0(:knon, :)) |
| 423 |
|
coefh(:knon, :) = max(coefh(:knon, :), ycoefh0(:knon, :)) |
| 424 |
|
END IF |
| 425 |
|
|
| 426 |
|
IF (iflag_pbl >= 3) THEN |
| 427 |
|
! Mellor et Yamada adapté à Mars, Richard Fournier et |
| 428 |
|
! Frédéric Hourdin |
| 429 |
|
yzlay(:knon, 1) = rd * yt(:knon, 1) / (0.5 * (ypaprs(:knon, 1) & |
| 430 |
|
+ ypplay(:knon, 1))) & |
| 431 |
|
* (ypaprs(:knon, 1) - ypplay(:knon, 1)) / rg |
| 432 |
|
DO k = 2, klev |
| 433 |
|
yzlay(1:knon, k) = yzlay(1:knon, k-1) & |
| 434 |
|
+ rd * 0.5 * (yt(1:knon, k-1) + yt(1:knon, k)) & |
| 435 |
|
/ ypaprs(1:knon, k) & |
| 436 |
|
* (ypplay(1:knon, k-1) - ypplay(1:knon, k)) / rg |
| 437 |
|
END DO |
| 438 |
|
DO k = 1, klev |
| 439 |
|
yteta(1:knon, k) = yt(1:knon, k)*(ypaprs(1:knon, 1) & |
| 440 |
|
/ ypplay(1:knon, k))**rkappa * (1.+0.61*yq(1:knon, k)) |
| 441 |
|
END DO |
| 442 |
|
yzlev(1:knon, 1) = 0. |
| 443 |
|
yzlev(:knon, klev+1) = 2. * yzlay(:knon, klev) & |
| 444 |
|
- yzlay(:knon, klev - 1) |
| 445 |
|
DO k = 2, klev |
| 446 |
|
yzlev(1:knon, k) = 0.5*(yzlay(1:knon, k)+yzlay(1:knon, k-1)) |
| 447 |
|
END DO |
| 448 |
|
DO k = 1, klev + 1 |
| 449 |
|
DO j = 1, knon |
| 450 |
|
i = ni(j) |
| 451 |
|
yq2(j, k) = q2(i, k, nsrf) |
| 452 |
|
END DO |
| 453 |
|
END DO |
| 454 |
|
|
| 455 |
|
CALL ustarhb(knon, yu, yv, coefm(:knon, 1), yustar) |
| 456 |
|
IF (prt_level > 9) PRINT *, 'USTAR = ', yustar |
| 457 |
|
|
| 458 |
|
! iflag_pbl peut être utilisé comme longueur de mélange |
| 459 |
|
|
| 460 |
|
IF (iflag_pbl >= 11) THEN |
| 461 |
|
CALL vdif_kcay(knon, dtime, rg, rd, ypaprs, yt, yzlev, yzlay, & |
| 462 |
|
yu, yv, yteta, coefm(:knon, 1), yq2, q2diag, ykmm, ykmn, & |
| 463 |
|
yustar, iflag_pbl) |
| 464 |
|
ELSE |
| 465 |
|
CALL yamada4(knon, dtime, rg, yzlev, yzlay, yu, yv, yteta, & |
| 466 |
|
coefm(:knon, 1), yq2, ykmm, ykmn, ykmq, yustar, iflag_pbl) |
| 467 |
|
END IF |
| 468 |
|
|
| 469 |
|
coefm(:knon, 2:) = ykmm(:knon, 2:klev) |
| 470 |
|
coefh(:knon, 2:) = ykmn(:knon, 2:klev) |
| 471 |
|
END IF |
| 472 |
|
|
| 473 |
|
! calculer la diffusion des vitesses "u" et "v" |
| 474 |
|
CALL clvent(knon, dtime, yu1, yv1, coefm(:knon, :), yt, yu, ypaprs, & |
| 475 |
|
ypplay, ydelp, y_d_u, y_flux_u) |
| 476 |
|
CALL clvent(knon, dtime, yu1, yv1, coefm(:knon, :), yt, yv, ypaprs, & |
| 477 |
|
ypplay, ydelp, y_d_v, y_flux_v) |
| 478 |
|
|
| 479 |
|
! calculer la diffusion de "q" et de "h" |
| 480 |
|
CALL clqh(dtime, itap, jour, debut, rlat, knon, nsrf, ni, pctsrf, & |
| 481 |
|
ytsoil, yqsol, rmu0, co2_ppm, yrugos, yrugoro, & |
| 482 |
|
yu1, yv1, coefh(:knon, :), yt, yq, yts, ypaprs, ypplay, ydelp, & |
| 483 |
|
yrads, yalb, yalblw, ysnow, yqsurf, yrain_f, ysnow_f, yfder, & |
| 484 |
|
ysolsw, yfluxlat, pctsrf_new, yagesno, y_d_t, y_d_q, y_d_ts, & |
| 485 |
|
yz0_new, y_flux_t, y_flux_q, y_dflux_t, y_dflux_q, & |
| 486 |
|
y_fqcalving, y_ffonte, y_run_off_lic_0, y_flux_o, y_flux_g) |
| 487 |
|
|
| 488 |
|
! calculer la longueur de rugosite sur ocean |
| 489 |
|
yrugm = 0. |
| 490 |
|
IF (nsrf == is_oce) THEN |
| 491 |
|
DO j = 1, knon |
| 492 |
|
yrugm(j) = 0.018*coefm(j, 1)*(yu1(j)**2+yv1(j)**2)/rg + & |
| 493 |
|
0.11*14E-6/sqrt(coefm(j, 1)*(yu1(j)**2+yv1(j)**2)) |
| 494 |
|
yrugm(j) = max(1.5E-05, yrugm(j)) |
| 495 |
|
END DO |
| 496 |
|
END IF |
| 497 |
|
DO j = 1, knon |
| 498 |
|
y_dflux_t(j) = y_dflux_t(j)*ypct(j) |
| 499 |
|
y_dflux_q(j) = y_dflux_q(j)*ypct(j) |
| 500 |
|
yu1(j) = yu1(j)*ypct(j) |
| 501 |
|
yv1(j) = yv1(j)*ypct(j) |
| 502 |
|
END DO |
| 503 |
|
|
| 504 |
|
DO k = 1, klev |
| 505 |
|
DO j = 1, knon |
| 506 |
|
i = ni(j) |
| 507 |
|
coefh(j, k) = coefh(j, k)*ypct(j) |
| 508 |
|
coefm(j, k) = coefm(j, k)*ypct(j) |
| 509 |
|
y_d_t(j, k) = y_d_t(j, k)*ypct(j) |
| 510 |
|
y_d_q(j, k) = y_d_q(j, k)*ypct(j) |
| 511 |
|
flux_t(i, k, nsrf) = y_flux_t(j, k) |
| 512 |
|
flux_q(i, k, nsrf) = y_flux_q(j, k) |
| 513 |
|
flux_u(i, k, nsrf) = y_flux_u(j, k) |
| 514 |
|
flux_v(i, k, nsrf) = y_flux_v(j, k) |
| 515 |
|
y_d_u(j, k) = y_d_u(j, k)*ypct(j) |
| 516 |
|
y_d_v(j, k) = y_d_v(j, k)*ypct(j) |
| 517 |
|
END DO |
| 518 |
|
END DO |
| 519 |
|
|
| 520 |
|
evap(:, nsrf) = -flux_q(:, 1, nsrf) |
| 521 |
|
|
| 522 |
|
albe(:, nsrf) = 0. |
| 523 |
|
alblw(:, nsrf) = 0. |
| 524 |
|
snow(:, nsrf) = 0. |
| 525 |
|
qsurf(:, nsrf) = 0. |
| 526 |
|
rugos(:, nsrf) = 0. |
| 527 |
|
fluxlat(:, nsrf) = 0. |
| 528 |
|
DO j = 1, knon |
| 529 |
|
i = ni(j) |
| 530 |
|
d_ts(i, nsrf) = y_d_ts(j) |
| 531 |
|
albe(i, nsrf) = yalb(j) |
| 532 |
|
alblw(i, nsrf) = yalblw(j) |
| 533 |
|
snow(i, nsrf) = ysnow(j) |
| 534 |
|
qsurf(i, nsrf) = yqsurf(j) |
| 535 |
|
rugos(i, nsrf) = yz0_new(j) |
| 536 |
|
fluxlat(i, nsrf) = yfluxlat(j) |
| 537 |
|
IF (nsrf == is_oce) THEN |
| 538 |
|
rugmer(i) = yrugm(j) |
| 539 |
|
rugos(i, nsrf) = yrugm(j) |
| 540 |
|
END IF |
| 541 |
|
agesno(i, nsrf) = yagesno(j) |
| 542 |
|
fqcalving(i, nsrf) = y_fqcalving(j) |
| 543 |
|
ffonte(i, nsrf) = y_ffonte(j) |
| 544 |
|
cdragh(i) = cdragh(i) + coefh(j, 1) |
| 545 |
|
cdragm(i) = cdragm(i) + coefm(j, 1) |
| 546 |
|
dflux_t(i) = dflux_t(i) + y_dflux_t(j) |
| 547 |
|
dflux_q(i) = dflux_q(i) + y_dflux_q(j) |
| 548 |
|
zu1(i) = zu1(i) + yu1(j) |
| 549 |
|
zv1(i) = zv1(i) + yv1(j) |
| 550 |
|
END DO |
| 551 |
|
IF (nsrf == is_ter) THEN |
| 552 |
|
qsol(ni(:knon)) = yqsol(:knon) |
| 553 |
|
else IF (nsrf == is_lic) THEN |
| 554 |
|
DO j = 1, knon |
| 555 |
|
i = ni(j) |
| 556 |
|
run_off_lic_0(i) = y_run_off_lic_0(j) |
| 557 |
|
END DO |
| 558 |
|
END IF |
| 559 |
|
!$$$ PB ajout pour soil |
| 560 |
|
ftsoil(:, :, nsrf) = 0. |
| 561 |
|
DO k = 1, nsoilmx |
| 562 |
|
DO j = 1, knon |
| 563 |
|
i = ni(j) |
| 564 |
|
ftsoil(i, k, nsrf) = ytsoil(j, k) |
| 565 |
|
END DO |
| 566 |
|
END DO |
| 567 |
|
|
| 568 |
|
DO j = 1, knon |
| 569 |
|
i = ni(j) |
| 570 |
|
DO k = 1, klev |
| 571 |
|
d_t(i, k) = d_t(i, k) + y_d_t(j, k) |
| 572 |
|
d_q(i, k) = d_q(i, k) + y_d_q(j, k) |
| 573 |
|
d_u(i, k) = d_u(i, k) + y_d_u(j, k) |
| 574 |
|
d_v(i, k) = d_v(i, k) + y_d_v(j, k) |
| 575 |
|
ycoefh(i, k) = ycoefh(i, k) + coefh(j, k) |
| 576 |
|
END DO |
| 577 |
|
END DO |
| 578 |
|
|
| 579 |
|
! diagnostic t, q a 2m et u, v a 10m |
| 580 |
|
|
| 581 |
|
DO j = 1, knon |
| 582 |
|
i = ni(j) |
| 583 |
|
uzon(j) = yu(j, 1) + y_d_u(j, 1) |
| 584 |
|
vmer(j) = yv(j, 1) + y_d_v(j, 1) |
| 585 |
|
tair1(j) = yt(j, 1) + y_d_t(j, 1) |
| 586 |
|
qair1(j) = yq(j, 1) + y_d_q(j, 1) |
| 587 |
|
zgeo1(j) = rd*tair1(j)/(0.5*(ypaprs(j, 1)+ypplay(j, & |
| 588 |
|
1)))*(ypaprs(j, 1)-ypplay(j, 1)) |
| 589 |
|
tairsol(j) = yts(j) + y_d_ts(j) |
| 590 |
|
rugo1(j) = yrugos(j) |
| 591 |
|
IF (nsrf == is_oce) THEN |
| 592 |
|
rugo1(j) = rugos(i, nsrf) |
| 593 |
|
END IF |
| 594 |
|
psfce(j) = ypaprs(j, 1) |
| 595 |
|
patm(j) = ypplay(j, 1) |
| 596 |
|
|
| 597 |
|
qairsol(j) = yqsurf(j) |
| 598 |
|
END DO |
| 599 |
|
|
| 600 |
|
CALL stdlevvar(klon, knon, nsrf, zxli, uzon, vmer, tair1, qair1, & |
| 601 |
|
zgeo1, tairsol, qairsol, rugo1, psfce, patm, yt2m, yq2m, & |
| 602 |
|
yt10m, yq10m, yu10m, yustar) |
| 603 |
|
|
| 604 |
|
DO j = 1, knon |
| 605 |
|
i = ni(j) |
| 606 |
|
t2m(i, nsrf) = yt2m(j) |
| 607 |
|
q2m(i, nsrf) = yq2m(j) |
| 608 |
|
|
| 609 |
|
! u10m, v10m : composantes du vent a 10m sans spirale de Ekman |
| 610 |
|
u10m(i, nsrf) = (yu10m(j)*uzon(j))/sqrt(uzon(j)**2+vmer(j)**2) |
| 611 |
|
v10m(i, nsrf) = (yu10m(j)*vmer(j))/sqrt(uzon(j)**2+vmer(j)**2) |
| 612 |
|
|
| 613 |
|
END DO |
| 614 |
|
|
| 615 |
|
CALL hbtm(knon, ypaprs, ypplay, yt2m, yt10m, yq2m, yq10m, yustar, & |
| 616 |
|
y_flux_t, y_flux_q, yu, yv, yt, yq, ypblh, ycapcl, yoliqcl, & |
| 617 |
|
ycteicl, ypblt, ytherm, ytrmb1, ytrmb2, ytrmb3, ylcl) |
| 618 |
|
|
| 619 |
|
DO j = 1, knon |
| 620 |
|
i = ni(j) |
| 621 |
|
pblh(i, nsrf) = ypblh(j) |
| 622 |
|
plcl(i, nsrf) = ylcl(j) |
| 623 |
|
capcl(i, nsrf) = ycapcl(j) |
| 624 |
|
oliqcl(i, nsrf) = yoliqcl(j) |
| 625 |
|
cteicl(i, nsrf) = ycteicl(j) |
| 626 |
|
pblt(i, nsrf) = ypblt(j) |
| 627 |
|
therm(i, nsrf) = ytherm(j) |
| 628 |
|
trmb1(i, nsrf) = ytrmb1(j) |
| 629 |
|
trmb2(i, nsrf) = ytrmb2(j) |
| 630 |
|
trmb3(i, nsrf) = ytrmb3(j) |
| 631 |
|
END DO |
| 632 |
|
|
| 633 |
|
DO j = 1, knon |
| 634 |
|
DO k = 1, klev + 1 |
| 635 |
|
i = ni(j) |
| 636 |
|
q2(i, k, nsrf) = yq2(j, k) |
| 637 |
|
END DO |
| 638 |
|
END DO |
| 639 |
|
!IM "slab" ocean |
| 640 |
|
IF (nsrf == is_oce) THEN |
| 641 |
|
DO j = 1, knon |
| 642 |
|
! on projette sur la grille globale |
| 643 |
|
i = ni(j) |
| 644 |
|
IF (pctsrf_new(i, is_oce)>epsfra) THEN |
| 645 |
|
flux_o(i) = y_flux_o(j) |
| 646 |
|
ELSE |
| 647 |
|
flux_o(i) = 0. |
| 648 |
|
END IF |
| 649 |
|
END DO |
| 650 |
|
END IF |
| 651 |
|
|
| 652 |
|
IF (nsrf == is_sic) THEN |
| 653 |
|
DO j = 1, knon |
| 654 |
|
i = ni(j) |
| 655 |
|
! On pondère lorsque l'on fait le bilan au sol : |
| 656 |
|
IF (pctsrf_new(i, is_sic)>epsfra) THEN |
| 657 |
|
flux_g(i) = y_flux_g(j) |
| 658 |
|
ELSE |
| 659 |
|
flux_g(i) = 0. |
| 660 |
|
END IF |
| 661 |
|
END DO |
| 662 |
|
|
| 663 |
|
END IF |
| 664 |
|
end IF if_knon |
| 665 |
|
END DO loop_surface |
| 666 |
|
|
| 667 |
rugos(:, is_oce) = rugmer |
! On utilise les nouvelles surfaces |
|
pctsrf = pctsrf_new |
|
| 668 |
|
|
| 669 |
END SUBROUTINE clmain |
rugos(:, is_oce) = rugmer |
| 670 |
|
pctsrf = pctsrf_new |
| 671 |
|
|
| 672 |
|
END SUBROUTINE clmain |
| 673 |
|
|
| 674 |
|
end module clmain_m |
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