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module pbl_surface_m |
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|
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IMPLICIT NONE |
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|
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contains |
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|
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SUBROUTINE pbl_surface(pctsrf, t, q, u, v, julien, mu0, ftsol, cdmmax, & |
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cdhmax, ftsoil, qsol, paprs, play, fsnow, fqsurf, falbe, fluxlat, & |
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rain_fall, snow_fall, frugs, agesno, rugoro, d_t, d_q, d_u, d_v, & |
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flux_t, flux_q, flux_u, flux_v, cdragh, cdragm, q2, dflux_t, dflux_q, & |
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coefh, t2m, q2m, u10m_srf, v10m_srf, pblh, capcl, oliqcl, cteicl, pblt, & |
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therm, plcl, fqcalving, ffonte, run_off_lic_0, albsol, sollw, solsw, & |
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tsol) |
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|
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! From phylmd/clmain.F, version 1.6, 2005/11/16 14:47:19 |
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! Author: Z. X. Li (LMD/CNRS) |
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! Date: Aug. 18th, 1993 |
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! Objet : interface de couche limite (diffusion verticale) |
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|
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! Tout ce qui a trait aux traceurs est dans "phytrac". Le calcul |
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! de la couche limite pour les traceurs se fait avec "cltrac" et |
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! ne tient pas compte de la diff\'erentiation des sous-fractions |
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! de sol. |
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|
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use cdrag_m, only: cdrag |
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use clqh_m, only: clqh |
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use clvent_m, only: clvent |
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use coef_diff_turb_m, only: coef_diff_turb |
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USE conf_gcm_m, ONLY: lmt_pas |
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USE conf_phys_m, ONLY: iflag_pbl |
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USE dimphy, ONLY: klev, klon |
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USE dimsoil, ONLY: nsoilmx |
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use hbtm_m, only: hbtm |
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USE histwrite_phy_m, ONLY: histwrite_phy |
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USE indicesol, ONLY: epsfra, is_lic, is_oce, is_sic, is_ter, nbsrf |
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USE interfoce_lim_m, ONLY: interfoce_lim |
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use phyetat0_m, only: masque |
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use stdlevvar_m, only: stdlevvar |
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USE suphec_m, ONLY: rd, rg, rsigma |
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use time_phylmdz, only: itap |
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|
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REAL, INTENT(inout):: pctsrf(:, :) ! (klon, nbsrf) |
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! pourcentages de surface de chaque maille |
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|
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REAL, INTENT(IN):: t(klon, klev) ! temperature (K) |
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REAL, INTENT(IN):: q(klon, klev) ! vapeur d'eau (kg / kg) |
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REAL, INTENT(IN):: u(klon, klev), v(klon, klev) ! vitesse |
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INTEGER, INTENT(IN):: julien ! jour de l'annee en cours |
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REAL, intent(in):: mu0(klon) ! cosinus de l'angle solaire zenithal |
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|
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REAL, INTENT(INout):: ftsol(:, :) ! (klon, nbsrf) |
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! skin temperature of surface fraction, in K |
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|
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REAL, INTENT(IN):: cdmmax, cdhmax ! seuils cdrm, cdrh |
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|
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REAL, INTENT(inout):: ftsoil(klon, nsoilmx, nbsrf) |
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! soil temperature of surface fraction |
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|
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REAL, INTENT(inout):: qsol(:) ! (klon) |
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! column-density of water in soil, in kg m-2 |
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|
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REAL, INTENT(IN):: paprs(klon, klev + 1) ! pression a intercouche (Pa) |
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REAL, INTENT(IN):: play(klon, klev) ! pression au milieu de couche (Pa) |
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|
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REAL, INTENT(inout):: fsnow(:, :) ! (klon, nbsrf) |
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! column-density of mass of snow at the surface, in kg m-2 |
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|
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REAL, INTENT(inout):: fqsurf(klon, nbsrf) |
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REAL, intent(inout):: falbe(klon, nbsrf) |
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|
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REAL, intent(out):: fluxlat(:, :) ! (klon, nbsrf) |
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! flux de chaleur latente, en W m-2 |
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|
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REAL, intent(in):: rain_fall(klon) |
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! liquid water mass flux (kg / m2 / s), positive down |
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|
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REAL, intent(in):: snow_fall(klon) |
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! solid water mass flux (kg / m2 / s), positive down |
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|
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REAL, intent(inout):: frugs(klon, nbsrf) ! longueur de rugosit\'e (en m) |
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real, intent(inout):: agesno(:, :) ! (klon, nbsrf) |
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REAL, INTENT(IN):: rugoro(klon) |
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|
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REAL, intent(out):: d_t(:, :), d_q(:, :) ! (klon, klev) |
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! changement pour t et q |
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|
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REAL, intent(out):: d_u(klon, klev), d_v(klon, klev) |
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! changement pour "u" et "v" |
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|
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REAL, intent(out):: flux_t(klon, nbsrf) |
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! flux de chaleur sensible (c_p T) (W / m2) (orientation positive |
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! vers le bas) à la surface |
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|
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REAL, intent(out):: flux_q(klon, nbsrf) |
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! flux de vapeur d'eau (kg / m2 / s) à la surface |
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|
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REAL, intent(out):: flux_u(:, :), flux_v(:, :) ! (klon, nbsrf) |
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! tension du vent (flux turbulent de vent) à la surface, en Pa |
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|
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REAL, INTENT(out):: cdragh(klon), cdragm(klon) |
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real q2(klon, klev + 1, nbsrf) |
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|
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! Ocean slab: |
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REAL, INTENT(out):: dflux_t(klon) ! derive du flux sensible |
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REAL, INTENT(out):: dflux_q(klon) ! derive du flux latent |
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|
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REAL, intent(out):: coefh(:, 2:) ! (klon, 2:klev) |
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! Pour pouvoir extraire les coefficients d'\'echange, le champ |
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! "coefh" a \'et\'e cr\'e\'e. Nous avons moyenn\'e les valeurs de |
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! ce champ sur les quatre sous-surfaces du mod\`ele. |
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|
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REAL, INTENT(inout):: t2m(klon, nbsrf), q2m(klon, nbsrf) |
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|
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REAL, INTENT(inout):: u10m_srf(:, :), v10m_srf(:, :) ! (klon, nbsrf) |
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! composantes du vent \`a 10m sans spirale d'Ekman |
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|
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! Ionela Musat. Cf. Anne Mathieu : planetary boundary layer, hbtm. |
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! Comme les autres diagnostics on cumule dans physiq ce qui permet |
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! de sortir les grandeurs par sous-surface. |
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REAL pblh(klon, nbsrf) ! height of planetary boundary layer |
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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, INTENT(inout):: pblt(klon, nbsrf) ! T au nveau HCL |
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REAL therm(klon, nbsrf) |
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REAL plcl(klon, nbsrf) |
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|
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REAL, intent(out):: fqcalving(klon, nbsrf) |
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! flux d'eau "perdue" par la surface et necessaire pour limiter la |
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! hauteur de neige, en kg / m2 / s |
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|
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real ffonte(klon, nbsrf) ! flux thermique utilise pour fondre la neige |
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REAL, intent(inout):: run_off_lic_0(:) ! (klon) |
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|
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REAL, intent(out):: albsol(:) ! (klon) |
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! albedo du sol total, visible, moyen par maille |
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|
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REAL, intent(in):: sollw(:) ! (klon) |
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! surface net downward longwave flux, in W m-2 |
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|
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REAL, intent(in):: solsw(:) ! (klon) |
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! surface net downward shortwave flux, in W m-2 |
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|
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REAL, intent(in):: tsol(:) ! (klon) |
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|
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! Local: |
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|
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REAL d_ts(klon, nbsrf) ! variation of ftsol |
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REAL fsollw(klon, nbsrf) ! bilan flux IR pour chaque sous-surface |
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REAL fsolsw(klon, nbsrf) ! flux solaire absorb\'e pour chaque sous-surface |
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|
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! la nouvelle repartition des surfaces sortie de l'interface |
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REAL, save:: pctsrf_new_oce(klon) |
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REAL, save:: pctsrf_new_sic(klon) |
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|
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REAL y_fqcalving(klon), y_ffonte(klon) |
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real y_run_off_lic_0(klon), y_run_off_lic(klon) |
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REAL run_off_lic(klon) ! ruissellement total |
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REAL rugmer(klon) |
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REAL ytsoil(klon, nsoilmx) |
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REAL yts(klon), ypctsrf(klon), yz0_new(klon) |
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real yrugos(klon) ! longueur de rugosite (en m) |
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REAL yalb(klon) |
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REAL snow(klon) ! column-density of mass of snow at the surface, in kg m-2 |
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real yqsurf(klon), yagesno(klon) |
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real yqsol(klon) ! column-density of water in soil, in kg m-2 |
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REAL yrain_fall(klon) ! liquid water mass flux (kg / m2 / s), positive down |
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REAL ysnow_fall(klon) ! solid water mass flux (kg / m2 / s), positive down |
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REAL yrugm(klon), radsol(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), y_flux_q(klon) |
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REAL y_flux_u(klon), y_flux_v(klon) |
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REAL y_dflux_t(klon), y_dflux_q(klon) |
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REAL ycoefh(klon, 2:klev), ycoefm(klon, 2:klev) |
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real ycdragh(klon), ycdragm(klon) |
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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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REAL yq2(klon, klev + 1) |
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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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|
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REAL pctsrf_pot(klon, nbsrf) |
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! "pourcentage potentiel" pour tenir compte des \'eventuelles |
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! apparitions ou disparitions de la glace de mer |
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|
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REAL yt2m(klon), yq2m(klon), wind10m(klon) |
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REAL ustar(klon) |
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|
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REAL yt10m(klon), yq10m(klon) |
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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 u1(klon), v1(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 zgeo1(klon) |
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REAL rugo1(klon) |
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REAL zgeop(klon, klev) |
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|
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!------------------------------------------------------------ |
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|
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albsol = sum(falbe * pctsrf, dim = 2) |
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|
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! R\'epartition sous maille des flux longwave et shortwave |
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! R\'epartition du longwave par sous-surface lin\'earis\'ee |
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|
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forall (nsrf = 1:nbsrf) |
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fsollw(:, nsrf) = sollw + 4. * RSIGMA * tsol**3 & |
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* (tsol - ftsol(:, nsrf)) |
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fsolsw(:, nsrf) = solsw * (1. - falbe(:, nsrf)) / (1. - albsol) |
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END forall |
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|
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ytherm = 0. |
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|
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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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|
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! Initialization: |
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rugmer = 0. |
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cdragh = 0. |
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cdragm = 0. |
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dflux_t = 0. |
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dflux_q = 0. |
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yrugos = 0. |
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ypaprs = 0. |
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ypplay = 0. |
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ydelp = 0. |
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yrugoro = 0. |
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d_ts = 0. |
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flux_t = 0. |
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flux_q = 0. |
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flux_u = 0. |
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flux_v = 0. |
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fluxlat = 0. |
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d_t = 0. |
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d_q = 0. |
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d_u = 0. |
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d_v = 0. |
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coefh = 0. |
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fqcalving = 0. |
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run_off_lic = 0. |
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|
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! Initialisation des "pourcentages potentiels". On consid\`ere ici qu'on |
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! peut avoir potentiellement de la glace sur tout le domaine oc\'eanique |
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! (\`a affiner). |
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|
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pctsrf_pot(:, is_ter) = pctsrf(:, is_ter) |
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pctsrf_pot(:, is_lic) = pctsrf(:, is_lic) |
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pctsrf_pot(:, is_oce) = 1. - masque |
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pctsrf_pot(:, is_sic) = 1. - masque |
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|
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! Tester si c'est le moment de lire le fichier: |
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if (mod(itap - 1, lmt_pas) == 0) then |
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CALL interfoce_lim(julien, pctsrf_new_oce, pctsrf_new_sic) |
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endif |
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|
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! Boucler sur toutes les sous-fractions du sol: |
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|
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loop_surface: DO nsrf = 1, nbsrf |
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! Define ni and knon: |
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|
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ni = 0 |
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knon = 0 |
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|
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DO i = 1, klon |
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! Pour d\'eterminer le domaine \`a traiter, on utilise les surfaces |
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! "potentielles" |
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IF (pctsrf_pot(i, nsrf) > epsfra) THEN |
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knon = knon + 1 |
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ni(knon) = i |
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END IF |
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END DO |
| 285 |
|
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if_knon: IF (knon /= 0) then |
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ypctsrf(:knon) = pctsrf(ni(:knon), nsrf) |
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yts(:knon) = ftsol(ni(:knon), nsrf) |
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snow(:knon) = fsnow(ni(:knon), nsrf) |
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yqsurf(:knon) = fqsurf(ni(:knon), nsrf) |
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yalb(:knon) = falbe(ni(:knon), nsrf) |
| 292 |
yrain_fall(:knon) = rain_fall(ni(:knon)) |
| 293 |
ysnow_fall(:knon) = snow_fall(ni(:knon)) |
| 294 |
yagesno(:knon) = agesno(ni(:knon), nsrf) |
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yrugos(:knon) = frugs(ni(:knon), nsrf) |
| 296 |
yrugoro(:knon) = rugoro(ni(:knon)) |
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radsol(:knon) = fsolsw(ni(:knon), nsrf) + fsollw(ni(:knon), nsrf) |
| 298 |
ypaprs(:knon, klev + 1) = paprs(ni(:knon), klev + 1) |
| 299 |
y_run_off_lic_0(:knon) = run_off_lic_0(ni(:knon)) |
| 300 |
|
| 301 |
! For continent, copy soil water content |
| 302 |
IF (nsrf == is_ter) yqsol(:knon) = qsol(ni(:knon)) |
| 303 |
|
| 304 |
ytsoil(:knon, :) = ftsoil(ni(:knon), :, nsrf) |
| 305 |
|
| 306 |
DO k = 1, klev |
| 307 |
DO j = 1, knon |
| 308 |
i = ni(j) |
| 309 |
ypaprs(j, k) = paprs(i, k) |
| 310 |
ypplay(j, k) = play(i, k) |
| 311 |
ydelp(j, k) = delp(i, k) |
| 312 |
yu(j, k) = u(i, k) |
| 313 |
yv(j, k) = v(i, k) |
| 314 |
yt(j, k) = t(i, k) |
| 315 |
yq(j, k) = q(i, k) |
| 316 |
END DO |
| 317 |
END DO |
| 318 |
|
| 319 |
! Calculer les géopotentiels de chaque couche: |
| 320 |
|
| 321 |
zgeop(:knon, 1) = RD * yt(:knon, 1) / (0.5 * (ypaprs(:knon, 1) & |
| 322 |
+ ypplay(:knon, 1))) * (ypaprs(:knon, 1) - ypplay(:knon, 1)) |
| 323 |
|
| 324 |
DO k = 2, klev |
| 325 |
zgeop(:knon, k) = zgeop(:knon, k - 1) + RD * 0.5 & |
| 326 |
* (yt(:knon, k - 1) + yt(:knon, k)) / ypaprs(:knon, k) & |
| 327 |
* (ypplay(:knon, k - 1) - ypplay(:knon, k)) |
| 328 |
ENDDO |
| 329 |
|
| 330 |
CALL cdrag(nsrf, sqrt(yu(:knon, 1)**2 + yv(:knon, 1)**2), & |
| 331 |
yt(:knon, 1), yq(:knon, 1), zgeop(:knon, 1), ypaprs(:knon, 1), & |
| 332 |
yts(:knon), yqsurf(:knon), yrugos(:knon), ycdragm(:knon), & |
| 333 |
ycdragh(:knon)) |
| 334 |
|
| 335 |
IF (iflag_pbl == 1) THEN |
| 336 |
ycdragm(:knon) = max(ycdragm(:knon), 0.) |
| 337 |
ycdragh(:knon) = max(ycdragh(:knon), 0.) |
| 338 |
end IF |
| 339 |
|
| 340 |
! on met un seuil pour ycdragm et ycdragh |
| 341 |
IF (nsrf == is_oce) THEN |
| 342 |
ycdragm(:knon) = min(ycdragm(:knon), cdmmax) |
| 343 |
ycdragh(:knon) = min(ycdragh(:knon), cdhmax) |
| 344 |
END IF |
| 345 |
|
| 346 |
IF (iflag_pbl >= 6) yq2(:knon, :) = q2(ni(:knon), :, nsrf) |
| 347 |
call coef_diff_turb(nsrf, ni(:knon), ypaprs(:knon, :), & |
| 348 |
ypplay(:knon, :), yu(:knon, :), yv(:knon, :), yq(:knon, :), & |
| 349 |
yt(:knon, :), yts(:knon), ycdragm(:knon), zgeop(:knon, :), & |
| 350 |
ycoefm(:knon, :), ycoefh(:knon, :), yq2(:knon, :)) |
| 351 |
|
| 352 |
CALL clvent(yu(:knon, 1), yv(:knon, 1), ycoefm(:knon, :), & |
| 353 |
ycdragm(:knon), yt(:knon, :), yu(:knon, :), ypaprs(:knon, :), & |
| 354 |
ypplay(:knon, :), ydelp(:knon, :), y_d_u(:knon, :), & |
| 355 |
y_flux_u(:knon)) |
| 356 |
CALL clvent(yu(:knon, 1), yv(:knon, 1), ycoefm(:knon, :), & |
| 357 |
ycdragm(:knon), yt(:knon, :), yv(:knon, :), ypaprs(:knon, :), & |
| 358 |
ypplay(:knon, :), ydelp(:knon, :), y_d_v(:knon, :), & |
| 359 |
y_flux_v(:knon)) |
| 360 |
|
| 361 |
CALL clqh(julien, nsrf, ni(:knon), ytsoil(:knon, :), yqsol(:knon), & |
| 362 |
mu0(ni(:knon)), yrugos(:knon), yrugoro(:knon), yu(:knon, 1), & |
| 363 |
yv(:knon, 1), ycoefh(:knon, :), ycdragh(:knon), yt(:knon, :), & |
| 364 |
yq(:knon, :), yts(:knon), ypaprs(:knon, :), ypplay(:knon, :), & |
| 365 |
ydelp(:knon, :), radsol(:knon), yalb(:knon), snow(:knon), & |
| 366 |
yqsurf(:knon), yrain_fall(:knon), ysnow_fall(:knon), & |
| 367 |
yfluxlat(:knon), pctsrf_new_sic(ni(:knon)), yagesno(:knon), & |
| 368 |
y_d_t(:knon, :), y_d_q(:knon, :), y_d_ts(:knon), & |
| 369 |
yz0_new(:knon), y_flux_t(:knon), y_flux_q(:knon), & |
| 370 |
y_dflux_t(:knon), y_dflux_q(:knon), y_fqcalving(:knon), & |
| 371 |
y_ffonte(:knon), y_run_off_lic_0(:knon), y_run_off_lic(:knon)) |
| 372 |
|
| 373 |
! calculer la longueur de rugosite sur ocean |
| 374 |
|
| 375 |
yrugm = 0. |
| 376 |
|
| 377 |
IF (nsrf == is_oce) THEN |
| 378 |
DO j = 1, knon |
| 379 |
yrugm(j) = 0.018 * ycdragm(j) * (yu(j, 1)**2 + yv(j, 1)**2) & |
| 380 |
/ rg + 0.11 * 14E-6 & |
| 381 |
/ sqrt(ycdragm(j) * (yu(j, 1)**2 + yv(j, 1)**2)) |
| 382 |
yrugm(j) = max(1.5E-05, yrugm(j)) |
| 383 |
END DO |
| 384 |
END IF |
| 385 |
|
| 386 |
DO k = 1, klev |
| 387 |
DO j = 1, knon |
| 388 |
i = ni(j) |
| 389 |
y_d_t(j, k) = y_d_t(j, k) * ypctsrf(j) |
| 390 |
y_d_q(j, k) = y_d_q(j, k) * ypctsrf(j) |
| 391 |
y_d_u(j, k) = y_d_u(j, k) * ypctsrf(j) |
| 392 |
y_d_v(j, k) = y_d_v(j, k) * ypctsrf(j) |
| 393 |
END DO |
| 394 |
END DO |
| 395 |
|
| 396 |
flux_t(ni(:knon), nsrf) = y_flux_t(:knon) |
| 397 |
flux_q(ni(:knon), nsrf) = y_flux_q(:knon) |
| 398 |
flux_u(ni(:knon), nsrf) = y_flux_u(:knon) |
| 399 |
flux_v(ni(:knon), nsrf) = y_flux_v(:knon) |
| 400 |
|
| 401 |
falbe(:, nsrf) = 0. |
| 402 |
fsnow(:, nsrf) = 0. |
| 403 |
fqsurf(:, nsrf) = 0. |
| 404 |
frugs(:, nsrf) = 0. |
| 405 |
DO j = 1, knon |
| 406 |
i = ni(j) |
| 407 |
d_ts(i, nsrf) = y_d_ts(j) |
| 408 |
falbe(i, nsrf) = yalb(j) |
| 409 |
fsnow(i, nsrf) = snow(j) |
| 410 |
fqsurf(i, nsrf) = yqsurf(j) |
| 411 |
frugs(i, nsrf) = yz0_new(j) |
| 412 |
fluxlat(i, nsrf) = yfluxlat(j) |
| 413 |
IF (nsrf == is_oce) THEN |
| 414 |
rugmer(i) = yrugm(j) |
| 415 |
frugs(i, nsrf) = yrugm(j) |
| 416 |
END IF |
| 417 |
agesno(i, nsrf) = yagesno(j) |
| 418 |
fqcalving(i, nsrf) = y_fqcalving(j) |
| 419 |
ffonte(i, nsrf) = y_ffonte(j) |
| 420 |
cdragh(i) = cdragh(i) + ycdragh(j) * ypctsrf(j) |
| 421 |
cdragm(i) = cdragm(i) + ycdragm(j) * ypctsrf(j) |
| 422 |
dflux_t(i) = dflux_t(i) + y_dflux_t(j) * ypctsrf(j) |
| 423 |
dflux_q(i) = dflux_q(i) + y_dflux_q(j) * ypctsrf(j) |
| 424 |
END DO |
| 425 |
IF (nsrf == is_ter) THEN |
| 426 |
qsol(ni(:knon)) = yqsol(:knon) |
| 427 |
else IF (nsrf == is_lic) THEN |
| 428 |
DO j = 1, knon |
| 429 |
i = ni(j) |
| 430 |
run_off_lic_0(i) = y_run_off_lic_0(j) |
| 431 |
run_off_lic(i) = y_run_off_lic(j) |
| 432 |
END DO |
| 433 |
END IF |
| 434 |
|
| 435 |
ftsoil(:, :, nsrf) = 0. |
| 436 |
ftsoil(ni(:knon), :, nsrf) = ytsoil(:knon, :) |
| 437 |
|
| 438 |
DO j = 1, knon |
| 439 |
i = ni(j) |
| 440 |
DO k = 1, klev |
| 441 |
d_t(i, k) = d_t(i, k) + y_d_t(j, k) |
| 442 |
d_q(i, k) = d_q(i, k) + y_d_q(j, k) |
| 443 |
d_u(i, k) = d_u(i, k) + y_d_u(j, k) |
| 444 |
d_v(i, k) = d_v(i, k) + y_d_v(j, k) |
| 445 |
END DO |
| 446 |
END DO |
| 447 |
|
| 448 |
forall (k = 2:klev) coefh(ni(:knon), k) & |
| 449 |
= coefh(ni(:knon), k) + ycoefh(:knon, k) * ypctsrf(:knon) |
| 450 |
|
| 451 |
! diagnostic t, q a 2m et u, v a 10m |
| 452 |
|
| 453 |
DO j = 1, knon |
| 454 |
i = ni(j) |
| 455 |
u1(j) = yu(j, 1) + y_d_u(j, 1) |
| 456 |
v1(j) = yv(j, 1) + y_d_v(j, 1) |
| 457 |
tair1(j) = yt(j, 1) + y_d_t(j, 1) |
| 458 |
qair1(j) = yq(j, 1) + y_d_q(j, 1) |
| 459 |
zgeo1(j) = rd * tair1(j) / (0.5 * (ypaprs(j, 1) + ypplay(j, & |
| 460 |
1))) * (ypaprs(j, 1)-ypplay(j, 1)) |
| 461 |
tairsol(j) = yts(j) + y_d_ts(j) |
| 462 |
rugo1(j) = yrugos(j) |
| 463 |
IF (nsrf == is_oce) THEN |
| 464 |
rugo1(j) = frugs(i, nsrf) |
| 465 |
END IF |
| 466 |
psfce(j) = ypaprs(j, 1) |
| 467 |
patm(j) = ypplay(j, 1) |
| 468 |
END DO |
| 469 |
|
| 470 |
CALL stdlevvar(nsrf, u1(:knon), v1(:knon), tair1(:knon), qair1, & |
| 471 |
zgeo1, tairsol, yqsurf(:knon), rugo1, psfce, patm, yt2m, yq2m, & |
| 472 |
yt10m, yq10m, wind10m(:knon), ustar(:knon)) |
| 473 |
|
| 474 |
DO j = 1, knon |
| 475 |
i = ni(j) |
| 476 |
t2m(i, nsrf) = yt2m(j) |
| 477 |
q2m(i, nsrf) = yq2m(j) |
| 478 |
|
| 479 |
u10m_srf(i, nsrf) = (wind10m(j) * u1(j)) & |
| 480 |
/ sqrt(u1(j)**2 + v1(j)**2) |
| 481 |
v10m_srf(i, nsrf) = (wind10m(j) * v1(j)) & |
| 482 |
/ sqrt(u1(j)**2 + v1(j)**2) |
| 483 |
END DO |
| 484 |
|
| 485 |
CALL hbtm(ypaprs, ypplay, yt2m, yq2m, ustar(:knon), y_flux_t(:knon), & |
| 486 |
y_flux_q(:knon), yu(:knon, :), yv(:knon, :), yt(:knon, :), & |
| 487 |
yq(:knon, :), ypblh(:knon), ycapcl, yoliqcl, ycteicl, ypblt, & |
| 488 |
ytherm, ylcl) |
| 489 |
|
| 490 |
DO j = 1, knon |
| 491 |
i = ni(j) |
| 492 |
pblh(i, nsrf) = ypblh(j) |
| 493 |
plcl(i, nsrf) = ylcl(j) |
| 494 |
capcl(i, nsrf) = ycapcl(j) |
| 495 |
oliqcl(i, nsrf) = yoliqcl(j) |
| 496 |
cteicl(i, nsrf) = ycteicl(j) |
| 497 |
pblt(i, nsrf) = ypblt(j) |
| 498 |
therm(i, nsrf) = ytherm(j) |
| 499 |
END DO |
| 500 |
|
| 501 |
IF (iflag_pbl >= 6) q2(ni(:knon), :, nsrf) = yq2(:knon, :) |
| 502 |
else |
| 503 |
fsnow(:, nsrf) = 0. |
| 504 |
end IF if_knon |
| 505 |
END DO loop_surface |
| 506 |
|
| 507 |
! On utilise les nouvelles surfaces |
| 508 |
frugs(:, is_oce) = rugmer |
| 509 |
pctsrf(:, is_oce) = pctsrf_new_oce |
| 510 |
pctsrf(:, is_sic) = pctsrf_new_sic |
| 511 |
|
| 512 |
CALL histwrite_phy("run_off_lic", run_off_lic) |
| 513 |
ftsol = ftsol + d_ts ! update surface temperature |
| 514 |
CALL histwrite_phy("dtsvdfo", d_ts(:, is_oce)) |
| 515 |
CALL histwrite_phy("dtsvdft", d_ts(:, is_ter)) |
| 516 |
CALL histwrite_phy("dtsvdfg", d_ts(:, is_lic)) |
| 517 |
CALL histwrite_phy("dtsvdfi", d_ts(:, is_sic)) |
| 518 |
|
| 519 |
END SUBROUTINE pbl_surface |
| 520 |
|
| 521 |
end module pbl_surface_m |
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