! ! $Id: calfis.F 1676 2012-11-08 20:03:30Z oboucher $ ! C C SUBROUTINE calfis(lafin, $ jD_cur, jH_cur, $ pucov, $ pvcov, $ pteta, $ pq, $ pmasse, $ pps, $ pp, $ ppk, $ pphis, $ pphi, $ pducov, $ pdvcov, $ pdteta, $ pdq, $ flxw, $ clesphy0, $ pdufi, $ pdvfi, $ pdhfi, $ pdqfi, $ pdpsfi) c c Auteur : P. Le Van, F. Hourdin c ......... USE infotrac USE control_mod IMPLICIT NONE c======================================================================= c c 1. rearrangement des tableaux et transformation c variables dynamiques > variables physiques c 2. calcul des termes physiques c 3. retransformation des tendances physiques en tendances dynamiques c c remarques: c ---------- c c - les vents sont donnes dans la physique par leurs composantes c naturelles. c - la variable thermodynamique de la physique est une variable c intensive : T c pour la dynamique on prend T * ( preff / p(l) ) **kappa c - les deux seules variables dependant de la geometrie necessaires c pour la physique sont la latitude pour le rayonnement et c l'aire de la maille quand on veut integrer une grandeur c horizontalement. c - les points de la physique sont les points scalaires de la c la dynamique; numerotation: c 1 pour le pole nord c (jjm-1)*iim pour l'interieur du domaine c ngridmx pour le pole sud c ---> ngridmx=2+(jjm-1)*iim c c Input : c ------- c pucov covariant zonal velocity c pvcov covariant meridional velocity c pteta potential temperature c pps surface pressure c pmasse masse d'air dans chaque maille c pts surface temperature (K) c callrad clef d'appel au rayonnement c c Output : c -------- c pdufi tendency for the natural zonal velocity (ms-1) c pdvfi tendency for the natural meridional velocity c pdhfi tendency for the potential temperature c pdtsfi tendency for the surface temperature c c pdtrad radiative tendencies \ both input c pfluxrad radiative fluxes / and output c c======================================================================= c c----------------------------------------------------------------------- c c 0. Declarations : c ------------------ #include "dimensions.h" #include "paramet.h" #include "temps.h" INTEGER ngridmx PARAMETER( ngridmx = 2+(jjm-1)*iim - 1/jjm ) #include "comconst.h" #include "comvert.h" #include "comgeom2.h" #include "iniprint.h" c Arguments : c ----------- LOGICAL lafin REAL pvcov(iip1,jjm,llm) REAL pucov(iip1,jjp1,llm) REAL pteta(iip1,jjp1,llm) REAL pmasse(iip1,jjp1,llm) REAL pq(iip1,jjp1,llm,nqtot) REAL pphis(iip1,jjp1) REAL pphi(iip1,jjp1,llm) c REAL pdvcov(iip1,jjm,llm) REAL pducov(iip1,jjp1,llm) REAL pdteta(iip1,jjp1,llm) REAL pdq(iip1,jjp1,llm,nqtot) c REAL pps(iip1,jjp1) REAL pp(iip1,jjp1,llmp1) REAL ppk(iip1,jjp1,llm) c REAL pdvfi(iip1,jjm,llm) REAL pdufi(iip1,jjp1,llm) REAL pdhfi(iip1,jjp1,llm) REAL pdqfi(iip1,jjp1,llm,nqtot) REAL pdpsfi(iip1,jjp1) INTEGER longcles PARAMETER ( longcles = 20 ) REAL clesphy0( longcles ) c Local variables : c ----------------- INTEGER i,j,l,ig0,ig,iq,iiq REAL zpsrf(ngridmx) REAL zplev(ngridmx,llm+1),zplay(ngridmx,llm) REAL zphi(ngridmx,llm),zphis(ngridmx) c REAL zufi(ngridmx,llm), zvfi(ngridmx,llm) REAL ztfi(ngridmx,llm),zqfi(ngridmx,llm,nqtot) c REAL pcvgu(ngridmx,llm), pcvgv(ngridmx,llm) REAL pcvgt(ngridmx,llm), pcvgq(ngridmx,llm,2) c REAL zdufi(ngridmx,llm),zdvfi(ngridmx,llm) REAL zdtfi(ngridmx,llm),zdqfi(ngridmx,llm,nqtot) REAL zdpsrf(ngridmx) c REAL zdufic(ngridmx,llm),zdvfic(ngridmx,llm) REAL zdtfic(ngridmx,llm),zdqfic(ngridmx,llm,nqtot) REAL jH_cur_split,zdt_split LOGICAL debut_split,lafin_split INTEGER isplit REAL zsin(iim),zcos(iim),z1(iim) REAL zsinbis(iim),zcosbis(iim),z1bis(iim) REAL unskap, pksurcp c cIM diagnostique PVteta, Amip2 INTEGER ntetaSTD PARAMETER(ntetaSTD=3) REAL rtetaSTD(ntetaSTD) DATA rtetaSTD/350., 380., 405./ ! Earth-specific values, beware !! REAL PVteta(ngridmx,ntetaSTD) c REAL flxw(iip1,jjp1,llm) ! Flux de masse verticale sur la grille dynamique REAL flxwfi(ngridmx,llm) ! Flux de masse verticale sur la grille physiq c REAL SSUM LOGICAL firstcal, debut DATA firstcal/.true./ SAVE firstcal,debut ! REAL rdayvrai REAL, intent(in):: jD_cur, jH_cur LOGICAL tracerdyn c c----------------------------------------------------------------------- c c 1. Initialisations : c -------------------- c c IF ( firstcal ) THEN debut = .TRUE. IF (ngridmx.NE.2+(jjm-1)*iim) THEN write(lunout,*) 'STOP dans calfis' write(lunout,*) & 'La dimension ngridmx doit etre egale a 2 + (jjm-1)*iim' write(lunout,*) ' ngridmx jjm iim ' write(lunout,*) ngridmx,jjm,iim STOP ENDIF ELSE debut = .FALSE. ENDIF ! of IF (firstcal) c c c----------------------------------------------------------------------- c 40. transformation des variables dynamiques en variables physiques: c --------------------------------------------------------------- c 41. pressions au sol (en Pascals) c ---------------------------------- zpsrf(1) = pps(1,1) ig0 = 2 DO j = 2,jjm CALL SCOPY( iim,pps(1,j),1,zpsrf(ig0), 1 ) ig0 = ig0+iim ENDDO zpsrf(ngridmx) = pps(1,jjp1) c 42. pression intercouches : c c ----------------------------------------------------------------- c .... zplev definis aux (llm +1) interfaces des couches .... c .... zplay definis aux ( llm ) milieux des couches .... c ----------------------------------------------------------------- c ... Exner = cp * ( p(l) / preff ) ** kappa .... c unskap = 1./ kappa c DO l = 1, llmp1 zplev( 1,l ) = pp(1,1,l) ig0 = 2 DO j = 2, jjm DO i =1, iim zplev( ig0,l ) = pp(i,j,l) ig0 = ig0 +1 ENDDO ENDDO zplev( ngridmx,l ) = pp(1,jjp1,l) ENDDO c c c 43. temperature naturelle (en K) et pressions milieux couches . c --------------------------------------------------------------- DO l=1,llm pksurcp = ppk(1,1,l) / cpp zplay(1,l) = preff * pksurcp ** unskap ztfi(1,l) = pteta(1,1,l) * pksurcp pcvgt(1,l) = pdteta(1,1,l) * pksurcp / pmasse(1,1,l) ig0 = 2 DO j = 2, jjm DO i = 1, iim pksurcp = ppk(i,j,l) / cpp zplay(ig0,l) = preff * pksurcp ** unskap ztfi(ig0,l) = pteta(i,j,l) * pksurcp pcvgt(ig0,l) = pdteta(i,j,l) * pksurcp / pmasse(i,j,l) ig0 = ig0 + 1 ENDDO ENDDO pksurcp = ppk(1,jjp1,l) / cpp zplay(ig0,l) = preff * pksurcp ** unskap ztfi (ig0,l) = pteta(1,jjp1,l) * pksurcp pcvgt(ig0,l) = pdteta(1,jjp1,l) * pksurcp/ pmasse(1,jjp1,l) ENDDO c 43.bis traceurs c --------------- c DO iq=1,nqtot iiq=niadv(iq) DO l=1,llm zqfi(1,l,iq) = pq(1,1,l,iiq) ig0 = 2 DO j=2,jjm DO i = 1, iim zqfi(ig0,l,iq) = pq(i,j,l,iiq) ig0 = ig0 + 1 ENDDO ENDDO zqfi(ig0,l,iq) = pq(1,jjp1,l,iiq) ENDDO ENDDO c convergence dynamique pour les traceurs "EAU" ! Earth-specific treatment of first 2 tracers (water) if (planet_type=="earth") then DO iq=1,2 DO l=1,llm pcvgq(1,l,iq)= pdq(1,1,l,iq) / pmasse(1,1,l) ig0 = 2 DO j=2,jjm DO i = 1, iim pcvgq(ig0,l,iq) = pdq(i,j,l,iq) / pmasse(i,j,l) ig0 = ig0 + 1 ENDDO ENDDO pcvgq(ig0,l,iq)= pdq(1,jjp1,l,iq) / pmasse(1,jjp1,l) ENDDO ENDDO endif ! of if (planet_type=="earth") c Geopotentiel calcule par rapport a la surface locale: c ----------------------------------------------------- CALL gr_dyn_fi(llm,iip1,jjp1,ngridmx,pphi,zphi) CALL gr_dyn_fi(1,iip1,jjp1,ngridmx,pphis,zphis) DO l=1,llm DO ig=1,ngridmx zphi(ig,l)=zphi(ig,l)-zphis(ig) ENDDO ENDDO c .... Calcul de la vitesse verticale ( en Pa*m*s ou Kg/s ) .... c JG : ancien calcule de omega utilise dans physiq.F. Maintenant le flux c de masse est calclue dans advtrac.F c DO l=1,llm c pvervel(1,l)=pw(1,1,l) * g /apoln c ig0=2 c DO j=2,jjm c DO i = 1, iim c pvervel(ig0,l) = pw(i,j,l) * g * unsaire(i,j) c ig0 = ig0 + 1 c ENDDO c ENDDO c pvervel(ig0,l)=pw(1,jjp1,l) * g /apols c ENDDO c c 45. champ u: c ------------ DO 50 l=1,llm DO 25 j=2,jjm ig0 = 1+(j-2)*iim zufi(ig0+1,l)= 0.5 * $ ( pucov(iim,j,l)/cu(iim,j) + pucov(1,j,l)/cu(1,j) ) pcvgu(ig0+1,l)= 0.5 * $ ( pducov(iim,j,l)/cu(iim,j) + pducov(1,j,l)/cu(1,j) ) DO 10 i=2,iim zufi(ig0+i,l)= 0.5 * $ ( pucov(i-1,j,l)/cu(i-1,j) + pucov(i,j,l)/cu(i,j) ) pcvgu(ig0+i,l)= 0.5 * $ ( pducov(i-1,j,l)/cu(i-1,j) + pducov(i,j,l)/cu(i,j) ) 10 CONTINUE 25 CONTINUE 50 CONTINUE c 46.champ v: c ----------- DO l=1,llm DO j=2,jjm ig0=1+(j-2)*iim DO i=1,iim zvfi(ig0+i,l)= 0.5 * $ ( pvcov(i,j-1,l)/cv(i,j-1) + pvcov(i,j,l)/cv(i,j) ) pcvgv(ig0+i,l)= 0.5 * $ ( pdvcov(i,j-1,l)/cv(i,j-1) + pdvcov(i,j,l)/cv(i,j) ) ENDDO ENDDO ENDDO c 47. champs de vents aux pole nord c ------------------------------ c U = 1 / pi * integrale [ v * cos(long) * d long ] c V = 1 / pi * integrale [ v * sin(long) * d long ] DO l=1,llm z1(1) =(rlonu(1)-rlonu(iim)+2.*pi)*pvcov(1,1,l)/cv(1,1) z1bis(1)=(rlonu(1)-rlonu(iim)+2.*pi)*pdvcov(1,1,l)/cv(1,1) DO i=2,iim z1(i) =(rlonu(i)-rlonu(i-1))*pvcov(i,1,l)/cv(i,1) z1bis(i)=(rlonu(i)-rlonu(i-1))*pdvcov(i,1,l)/cv(i,1) ENDDO DO i=1,iim zcos(i) = COS(rlonv(i))*z1(i) zcosbis(i)= COS(rlonv(i))*z1bis(i) zsin(i) = SIN(rlonv(i))*z1(i) zsinbis(i)= SIN(rlonv(i))*z1bis(i) ENDDO zufi(1,l) = SSUM(iim,zcos,1)/pi pcvgu(1,l) = SSUM(iim,zcosbis,1)/pi zvfi(1,l) = SSUM(iim,zsin,1)/pi pcvgv(1,l) = SSUM(iim,zsinbis,1)/pi ENDDO c 48. champs de vents aux pole sud: c --------------------------------- c U = 1 / pi * integrale [ v * cos(long) * d long ] c V = 1 / pi * integrale [ v * sin(long) * d long ] DO l=1,llm z1(1) =(rlonu(1)-rlonu(iim)+2.*pi)*pvcov(1,jjm,l)/cv(1,jjm) z1bis(1)=(rlonu(1)-rlonu(iim)+2.*pi)*pdvcov(1,jjm,l)/cv(1,jjm) DO i=2,iim z1(i) =(rlonu(i)-rlonu(i-1))*pvcov(i,jjm,l)/cv(i,jjm) z1bis(i)=(rlonu(i)-rlonu(i-1))*pdvcov(i,jjm,l)/cv(i,jjm) ENDDO DO i=1,iim zcos(i) = COS(rlonv(i))*z1(i) zcosbis(i) = COS(rlonv(i))*z1bis(i) zsin(i) = SIN(rlonv(i))*z1(i) zsinbis(i) = SIN(rlonv(i))*z1bis(i) ENDDO zufi(ngridmx,l) = SSUM(iim,zcos,1)/pi pcvgu(ngridmx,l) = SSUM(iim,zcosbis,1)/pi zvfi(ngridmx,l) = SSUM(iim,zsin,1)/pi pcvgv(ngridmx,l) = SSUM(iim,zsinbis,1)/pi ENDDO c if (planet_type=="earth") then #ifdef CPP_PHYS ! PVtheta calls tetalevel, which is in the physics cIM calcul PV a teta=350, 380, 405K CALL PVtheta(ngridmx,llm,pucov,pvcov,pteta, $ ztfi,zplay,zplev, $ ntetaSTD,rtetaSTD,PVteta) #endif endif c c On change de grille, dynamique vers physiq, pour le flux de masse verticale CALL gr_dyn_fi(llm,iip1,jjp1,ngridmx,flxw,flxwfi) c----------------------------------------------------------------------- c Appel de la physique: c --------------------- ! write(lunout,*) 'PHYSIQUE AVEC NSPLIT_PHYS=',nsplit_phys zdt_split=dtphys/nsplit_phys zdufic(:,:)=0. zdvfic(:,:)=0. zdtfic(:,:)=0. zdqfic(:,:,:)=0. #ifdef CPP_PHYS do isplit=1,nsplit_phys jH_cur_split=jH_cur+(isplit-1) * dtvr / (daysec *nsplit_phys) debut_split=debut.and.isplit==1 lafin_split=lafin.and.isplit==nsplit_phys if (planet_type=="earth") then CALL physiq (ngridmx, . llm, . debut_split, . lafin_split, . jD_cur, . jH_cur_split, . zdt_split, . zplev, . zplay, . zphi, . zphis, . presnivs, . clesphy0, . zufi, . zvfi, . ztfi, . zqfi, . flxwfi, . zdufi, . zdvfi, . zdtfi, . zdqfi, . zdpsrf, cIM diagnostique PVteta, Amip2 . pducov, . PVteta) else if ( planet_type=="generic" ) then CALL physiq (ngridmx, !! ngrid . llm, !! nlayer . nqtot, !! nq . tname, !! tracer names from dynamical core (given in infotrac) . debut_split, !! firstcall . lafin_split, !! lastcall . jD_cur, !! pday. see leapfrog . jH_cur_split, !! ptime "fraction of day" . zdt_split, !! ptimestep . zplev, !! pplev . zplay, !! pplay . zphi, !! pphi . zufi, !! pu . zvfi, !! pv . ztfi, !! pt . zqfi, !! pq . flxwfi, !! pw !! or 0. anyway this is for diagnostic. not used in physiq. . zdufi, !! pdu . zdvfi, !! pdv . zdtfi, !! pdt . zdqfi, !! pdq . zdpsrf, !! pdpsrf . tracerdyn) !! tracerdyn <-- utilite ??? endif ! of if (planet_type=="earth") zufi(:,:)=zufi(:,:)+zdufi(:,:)*zdt_split zvfi(:,:)=zvfi(:,:)+zdvfi(:,:)*zdt_split ztfi(:,:)=ztfi(:,:)+zdtfi(:,:)*zdt_split zqfi(:,:,:)=zqfi(:,:,:)+zdqfi(:,:,:)*zdt_split zdufic(:,:)=zdufic(:,:)+zdufi(:,:) zdvfic(:,:)=zdvfic(:,:)+zdvfi(:,:) zdtfic(:,:)=zdtfic(:,:)+zdtfi(:,:) zdqfic(:,:,:)=zdqfic(:,:,:)+zdqfi(:,:,:) enddo ! of do isplit=1,nsplit_phys #endif ! of #ifdef CPP_PHYS zdufi(:,:)=zdufic(:,:)/nsplit_phys zdvfi(:,:)=zdvfic(:,:)/nsplit_phys zdtfi(:,:)=zdtfic(:,:)/nsplit_phys zdqfi(:,:,:)=zdqfic(:,:,:)/nsplit_phys 500 CONTINUE c----------------------------------------------------------------------- c transformation des tendances physiques en tendances dynamiques: c --------------------------------------------------------------- c tendance sur la pression : c ----------------------------------- CALL gr_fi_dyn(1,ngridmx,iip1,jjp1,zdpsrf,pdpsfi) c c 62. enthalpie potentielle c --------------------- DO l=1,llm DO i=1,iip1 pdhfi(i,1,l) = cpp * zdtfi(1,l) / ppk(i, 1 ,l) pdhfi(i,jjp1,l) = cpp * zdtfi(ngridmx,l)/ ppk(i,jjp1,l) ENDDO DO j=2,jjm ig0=1+(j-2)*iim DO i=1,iim pdhfi(i,j,l) = cpp * zdtfi(ig0+i,l) / ppk(i,j,l) ENDDO pdhfi(iip1,j,l) = pdhfi(1,j,l) ENDDO ENDDO c 62. humidite specifique c --------------------- ! Ehouarn: removed this useless bit: was overwritten at step 63 anyways ! DO iq=1,nqtot ! DO l=1,llm ! DO i=1,iip1 ! pdqfi(i,1,l,iq) = zdqfi(1,l,iq) ! pdqfi(i,jjp1,l,iq) = zdqfi(ngridmx,l,iq) ! ENDDO ! DO j=2,jjm ! ig0=1+(j-2)*iim ! DO i=1,iim ! pdqfi(i,j,l,iq) = zdqfi(ig0+i,l,iq) ! ENDDO ! pdqfi(iip1,j,l,iq) = pdqfi(1,j,l,iq) ! ENDDO ! ENDDO ! ENDDO c 63. traceurs c ------------ C initialisation des tendances pdqfi(:,:,:,:)=0. C DO iq=1,nqtot iiq=niadv(iq) DO l=1,llm DO i=1,iip1 pdqfi(i,1,l,iiq) = zdqfi(1,l,iq) pdqfi(i,jjp1,l,iiq) = zdqfi(ngridmx,l,iq) ENDDO DO j=2,jjm ig0=1+(j-2)*iim DO i=1,iim pdqfi(i,j,l,iiq) = zdqfi(ig0+i,l,iq) ENDDO pdqfi(iip1,j,l,iiq) = pdqfi(1,j,l,iq) ENDDO ENDDO ENDDO c 65. champ u: c ------------ DO l=1,llm DO i=1,iip1 pdufi(i,1,l) = 0. pdufi(i,jjp1,l) = 0. ENDDO DO j=2,jjm ig0=1+(j-2)*iim DO i=1,iim-1 pdufi(i,j,l)= $ 0.5*(zdufi(ig0+i,l)+zdufi(ig0+i+1,l))*cu(i,j) ENDDO pdufi(iim,j,l)= $ 0.5*(zdufi(ig0+1,l)+zdufi(ig0+iim,l))*cu(iim,j) pdufi(iip1,j,l)=pdufi(1,j,l) ENDDO ENDDO c 67. champ v: c ------------ DO l=1,llm DO j=2,jjm-1 ig0=1+(j-2)*iim DO i=1,iim pdvfi(i,j,l)= $ 0.5*(zdvfi(ig0+i,l)+zdvfi(ig0+i+iim,l))*cv(i,j) ENDDO pdvfi(iip1,j,l) = pdvfi(1,j,l) ENDDO ENDDO c 68. champ v pres des poles: c --------------------------- c v = U * cos(long) + V * SIN(long) DO l=1,llm DO i=1,iim pdvfi(i,1,l)= $ zdufi(1,l)*COS(rlonv(i))+zdvfi(1,l)*SIN(rlonv(i)) pdvfi(i,jjm,l)=zdufi(ngridmx,l)*COS(rlonv(i)) $ +zdvfi(ngridmx,l)*SIN(rlonv(i)) pdvfi(i,1,l)= $ 0.5*(pdvfi(i,1,l)+zdvfi(i+1,l))*cv(i,1) pdvfi(i,jjm,l)= $ 0.5*(pdvfi(i,jjm,l)+zdvfi(ngridmx-iip1+i,l))*cv(i,jjm) ENDDO pdvfi(iip1,1,l) = pdvfi(1,1,l) pdvfi(iip1,jjm,l)= pdvfi(1,jjm,l) ENDDO c----------------------------------------------------------------------- 700 CONTINUE firstcal = .FALSE. RETURN END