! ! $Id: calfis.F 1407 2010-07-07 10:31:52Z fairhead $ ! C C SUBROUTINE calfis(lafin, $ jD_cur, jH_cur, $ pucov, $ pvcov, $ pteta, $ pq, $ pmasse, $ pps, $ pp, $ ppk, $ pphis, $ pphi, $ pducov, $ pdvcov, $ pdteta, $ pdq, $ flxw, $ pdufi, $ pdvfi, $ pdhfi, $ pdqfi, $ pdpsfi) c c Auteur : P. Le Van, F. Hourdin c ......... USE infotrac, ONLY: nqtot, niadv, tname USE control_mod, ONLY: planet_type, nsplit_phys USE write_field USE cpdet_mod, only: t2tpot,tpot2t #ifdef CPP_PHYS USE callphysiq_mod, ONLY: call_physiq #endif ! used only for zonal averages USE moyzon_mod USE comvert_mod, ONLY: presnivs,preff USE comconst_mod, ONLY: daysec,dtvr,dtphys,kappa,cpp,g,rad,pi USE logic_mod, ONLY: moyzon_ch,moyzon_mu 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 (K/s) 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" INTEGER ngridmx PARAMETER( ngridmx = 2+(jjm-1)*iim - 1/jjm ) include "comgeom2.h" include "iniprint.h" c Arguments : c ----------- LOGICAL,INTENT(IN) :: lafin ! .true. for the very last call to physics REAL,INTENT(IN) :: jD_cur, jH_cur REAL,INTENT(IN) :: pvcov(iip1,jjm,llm) ! covariant meridional velocity REAL,INTENT(IN) :: pucov(iip1,jjp1,llm) ! covariant zonal velocity REAL,INTENT(IN) :: pteta(iip1,jjp1,llm) ! potential temperature REAL,INTENT(IN) :: pmasse(iip1,jjp1,llm) ! mass in each cell ! not used REAL,INTENT(IN) :: pq(iip1,jjp1,llm,nqtot) ! tracers REAL,INTENT(IN) :: pphis(iip1,jjp1) ! surface geopotential REAL,INTENT(IN) :: pphi(iip1,jjp1,llm) ! geopotential REAL,INTENT(IN) :: pdvcov(iip1,jjm,llm) ! dynamical tendency on vcov REAL,INTENT(IN) :: pducov(iip1,jjp1,llm) ! dynamical tendency on ucov REAL,INTENT(IN) :: pdteta(iip1,jjp1,llm) ! dynamical tendency on teta ! commentaire SL: pdq ne sert que pour le calcul de pcvgq, ! qui lui meme ne sert a rien dans la routine telle qu'elle est ! ecrite, et que j'ai donc commente.... REAL,INTENT(IN) :: pdq(iip1,jjp1,llm,nqtot) ! dynamical tendency on tracers ! NB: pdq is only used to compute pcvgq which is in fact not used... REAL,INTENT(IN) :: pps(iip1,jjp1) ! surface pressure (Pa) REAL,INTENT(IN) :: pp(iip1,jjp1,llmp1) ! pressure at mesh interfaces (Pa) REAL,INTENT(IN) :: ppk(iip1,jjp1,llm) ! Exner at mid-layer REAL,INTENT(IN) :: flxw(iip1,jjp1,llm) ! Vertical mass flux on lower mesh interfaces (kg/s) (on llm because flxw(:,:,llm+1)=0) ! tendencies (in */s) from the physics REAL,INTENT(OUT) :: pdvfi(iip1,jjm,llm) ! tendency on covariant meridional wind REAL,INTENT(OUT) :: pdufi(iip1,jjp1,llm) ! tendency on covariant zonal wind REAL,INTENT(OUT) :: pdhfi(iip1,jjp1,llm) ! tendency on potential temperature (K/s) REAL,INTENT(OUT) :: pdqfi(iip1,jjp1,llm,nqtot) ! tendency on tracers REAL,INTENT(OUT) :: pdpsfi(iip1,jjp1) ! tendency on surface pressure (Pa/s) #ifndef CPP_PARA 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) REAL zrot(iip1,jjm,llm) ! AdlC May 2014 REAL zufi(ngridmx,llm), zvfi(ngridmx,llm) REAL zrfi(ngridmx,llm) ! relative wind vorticity REAL ztfi(ngridmx,llm),zqfi(ngridmx,llm,nqtot) ! ADAPTATION GCM POUR CP(T) REAL zteta(ngridmx,llm) REAL zpk(ngridmx,llm) ! RQ SL 13/10/10: ! Ces calculs ne servent pas. ! Si necessaire, decommenter ces variables et les calculs... ! REAL pcvgu(ngridmx,llm), pcvgv(ngridmx,llm) ! REAL pcvgt(ngridmx,llm), pcvgq(ngridmx,llm,2) REAL zdufi(ngridmx,llm),zdvfi(ngridmx,llm) REAL zdtfi(ngridmx,llm),zdqfi(ngridmx,llm,nqtot) REAL zdpsrf(ngridmx) 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 save unskap REAL flxwfi(ngridmx,llm) ! Flux de masse verticale sur la grille physiq REAL SSUM LOGICAL,SAVE :: firstcal=.true., debut=.true. ! REAL rdayvrai LOGICAL tracerdyn ! for generic/mars physics call ; possibly to get rid of ! For Titan only right now: ! to allow for 2D computation of microphys and chemistry LOGICAL,save :: flag_moyzon REAL,allocatable,save :: tmpvar(:,:) REAL,allocatable,save :: tmpvarp1(:,:) REAL,allocatable,save :: tmpvarbar(:) REAL,allocatable,save :: tmpvarbarp1(:) real :: zz1,zz2 c----------------------------------------------------------------------- c 1. Initialisations : 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 unskap = 1./ kappa flag_moyzon = .false. if(moyzon_ch.or.moyzon_mu) then flag_moyzon = .true. allocate(tmpvar(iip1,llm)) allocate(tmpvarp1(iip1,llmp1)) allocate(tmpvarbar(llm)) allocate(tmpvarbarp1(llmp1)) endif if (flag_moyzon) call moyzon_init(ngridmx,llm,nqtot) c---------------------------------------------- c moyennes globales pour le profil de pression if(planet_type.eq."titan".or.planet_type.eq."venus") then ALLOCATE(plevmoy(llm+1)) ALLOCATE(playmoy(llm)) ALLOCATE(tmoy(llm)) ALLOCATE(tetamoy(llm)) ALLOCATE(pkmoy(llm)) ALLOCATE(phimoy(0:llm)) ALLOCATE(zlevmoy(llm+1)) ALLOCATE(zlaymoy(llm)) plevmoy=0. do l=1,llmp1 do i=1,iip1 do j=1,jjp1 plevmoy(l)=plevmoy(l)+pp(i,j,l)/(iip1*jjp1) enddo enddo enddo tetamoy=0. pkmoy=0. phimoy=0. do i=1,iip1 do j=1,jjp1 phimoy(0)=phimoy(0)+pphis(i,j)/(iip1*jjp1) enddo enddo do l=1,llm do i=1,iip1 do j=1,jjp1 tetamoy(l)=tetamoy(l)+pteta(i,j,l)/(iip1*jjp1) pkmoy(l)=pkmoy(l)+ppk(i,j,l)/(iip1*jjp1) phimoy(l)=phimoy(l)+pphi(i,j,l)/(iip1*jjp1) enddo enddo enddo playmoy(:) = preff * (pkmoy(:)/cpp) ** unskap call tpot2t(llm,tetamoy,tmoy,pkmoy) c SI ON TIENT COMPTE DE LA VARIATION DE G AVEC L'ALTITUDE: zlaymoy(1:llm) = g*rad*rad/(g*rad-phimoy(1:llm))-rad zlevmoy(1) = phimoy(0)/g DO l=2,llm zz1=(playmoy(l-1)+plevmoy(l))/(playmoy(l-1)-plevmoy(l)) zz2=(plevmoy(l) +playmoy(l))/(plevmoy(l) -playmoy(l)) zlevmoy(l)=(zz1*zlaymoy(l-1)+zz2*zlaymoy(l))/(zz1+zz2) ENDDO zlevmoy(llmp1)=zlaymoy(llm)+(zlaymoy(llm)-zlevmoy(llm)) c------------------- c + lat index allocate(klat(ngridmx)) klat=0 klat(1) = 1 ig0 = 2 DO j = 2,jjm do i=0,iim-1 klat(ig0+i) = j enddo ig0 = ig0+iim ENDDO klat(ngridmx) = jjp1 endif ! planet_type=titan c---------------------------------------------- ELSE debut = .FALSE. ENDIF ! of IF (firstcal) 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 et fonction d'Exner: 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 .... ! ADAPTATION GCM POUR CP(T) DO l = 1, llm zpk( 1,l ) = ppk(1,1,l) zteta( 1,l ) = pteta(1,1,l) zplev( 1,l ) = pp(1,1,l) ig0 = 2 DO j = 2, jjm DO i =1, iim zpk( ig0,l ) = ppk(i,j,l) zteta( ig0,l ) = pteta(i,j,l) zplev( ig0,l ) = pp(i,j,l) ig0 = ig0 +1 ENDDO ENDDO zpk( ngridmx,l ) = ppk(1,jjp1,l) zteta( ngridmx,l ) = pteta(1,jjp1,l) zplev( ngridmx,l ) = pp(1,jjp1,l) ENDDO zplev( 1,llmp1 ) = pp(1,1,llmp1) ig0 = 2 DO j = 2, jjm DO i =1, iim zplev( ig0,llmp1 ) = pp(i,j,llmp1) ig0 = ig0 +1 ENDDO ENDDO zplev( ngridmx,llmp1 ) = pp(1,jjp1,llmp1) if (flag_moyzon) then tmpvarp1(:,:) = pp(:,1,:) call moyzon(llmp1,tmpvarp1,tmpvarbarp1) zplevbar(1,:) = tmpvarbarp1 tmpvar(:,:) = ppk(:,1,:) call moyzon(llm,tmpvar,tmpvarbar) zpkbar(1,:) = tmpvarbar tmpvar(:,:) = pteta(:,1,:) call moyzon(llm,tmpvar,tmpvarbar) ztetabar(1,:) = tmpvarbar call tpot2t(llm,ztetabar(1,:),ztfibar(1,:),zpkbar(1,:)) ig0 = 2 do j = 2, jjm tmpvarp1(:,:) = pp(:,j,:) call moyzon(llmp1,tmpvarp1,tmpvarbarp1) zplevbar(ig0,:) = tmpvarbarp1 tmpvar(:,:) = ppk(:,j,:) call moyzon(llm,tmpvar,tmpvarbar) zpkbar(ig0,:) = tmpvarbar tmpvar(:,:) = pteta(:,j,:) call moyzon(llm,tmpvar,tmpvarbar) ztetabar(ig0,:) = tmpvarbar call tpot2t(llm,ztetabar(ig0,:),ztfibar(ig0,:),zpkbar(ig0,:)) ig0 = ig0+1 do i=2,iim zplevbar(ig0,:) = zplevbar(ig0-1,:) zpkbar(ig0,:) = zpkbar(ig0-1,:) ztetabar(ig0,:) = ztetabar(ig0-1,:) ztfibar(ig0,:) = ztfibar(ig0-1,:) ig0 = ig0+1 enddo enddo tmpvarp1(:,:) = pp(:,jjp1,:) call moyzon(llmp1,tmpvarp1,tmpvarbarp1) zplevbar(ngridmx,:) = tmpvarbarp1 tmpvar(:,:) = ppk(:,jjp1,:) call moyzon(llm,tmpvar,tmpvarbar) zpkbar(ngridmx,:) = tmpvarbar tmpvar(:,:) = pteta(:,jjp1,:) call moyzon(llm,tmpvar,tmpvarbar) ztetabar(ngridmx,:) = tmpvarbar call tpot2t(llm,ztetabar(ngridmx,:), . ztfibar(ngridmx,:),zpkbar(ngridmx,:)) endif c 43. temperature naturelle (en K) et pressions milieux couches . c --------------------------------------------------------------- ! ADAPTATION GCM POUR CP(T) call tpot2t(ngridmx*llm,zteta,ztfi,zpk) DO l=1,llm pksurcp = ppk(1,1,l) / cpp zplay(1,l) = preff * pksurcp ** unskap ! 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 ! 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 ! pcvgt(ig0,l) = pdteta(1,jjp1,l) * pksurcp/ pmasse(1,jjp1,l) ENDDO if (flag_moyzon) then zplaybar(:,:) = preff * (zpkbar(:,:)/cpp)**unskap endif c 43.bis traceurs (tous intensifs) c --------------- DO iq=1,nqtot DO l=1,llm zqfi(1,l,iq) = pq(1,1,l,iq) ig0 = 2 DO j=2,jjm DO i = 1, iim zqfi(ig0,l,iq) = pq(i,j,l,iq) ig0 = ig0 + 1 ENDDO ENDDO zqfi(ig0,l,iq) = pq(1,jjp1,l,iq) ENDDO ENDDO ! boucle sur traceurs if (flag_moyzon) then DO iq=1,nqtot ! RQ: REVOIR A QUOI CA SERT... ET VERIFIER... ! iiq=niadv(iq) ! en fait, iiq=iq... ! FIN RQ tmpvar(:,:) = pq(:,1,:,iq) call moyzon(llm,tmpvar,tmpvarbar) zqfibar(1,:,iq) = tmpvarbar ig0 = 2 do j = 2, jjm tmpvar(:,:) = pq(:,j,:,iq) call moyzon(llm,tmpvar,tmpvarbar) zqfibar(ig0,:,iq) = tmpvarbar ig0 = ig0+1 do i=2,iim zqfibar(ig0,:,iq) = zqfibar(ig0-1,:,iq) ig0 = ig0+1 enddo enddo tmpvar(:,:) = pq(:,jjp1,:,iq) call moyzon(llm,tmpvar,tmpvarbar) zqfibar(ngridmx,:,iq) = tmpvarbar ENDDO ! of DO iq=1,nqtot endif ! DEBUG ! do ig0=1,ngridmx ! write(*,'(6(e13.5,1x))') zqfibar(ig0,1,10),zqfi(ig0,1,10), ! . zqfibar(ig0,llm/2,10),zqfi(ig0,llm/2,10), ! . zqfibar(ig0,llm,10),zqfi(ig0,llm,10) ! enddo ! stop !----------------- ! RQ SL 13/10/10: ! Ces calculs ne servent pas. ! Si necessaire, decommenter ces variables et les calculs... ! ! 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 if (flag_moyzon) then tmpvar(:,1) = pphis(:,1) call moyzon(1,tmpvar(:,1),tmpvarbar(1)) zphisbar(1) = tmpvarbar(1) tmpvar(:,:) = pphi(:,1,:) call moyzon(llm,tmpvar,tmpvarbar) zphibar(1,:) = tmpvarbar ig0 = 2 do j = 2, jjm tmpvar(:,1) = pphis(:,j) call moyzon(1,tmpvar(:,1),tmpvarbar(1)) zphisbar(ig0) = tmpvarbar(1) tmpvar(:,:) = pphi(:,j,:) call moyzon(llm,tmpvar,tmpvarbar) zphibar(ig0,:) = tmpvarbar ig0 = ig0+1 do i=2,iim zphisbar(ig0) = zphisbar(ig0-1) zphibar(ig0,:) = zphibar(ig0-1,:) ig0 = ig0+1 enddo enddo tmpvar(:,1) = pphis(:,jjp1) call moyzon(1,tmpvar(:,1),tmpvarbar(1)) zphisbar(ngridmx) = tmpvarbar(1) tmpvar(:,:) = pphi(:,jjp1,:) call moyzon(llm,tmpvar,tmpvarbar) zphibar(ngridmx,:) = tmpvarbar endif 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 Alvaro de la Camara (May 2014) C 46.1 Calcul de la vorticite et passage sur la grille physique C -------------------------------------------------------------- DO l=1,llm do i=1,iim do j=1,jjm zrot(i,j,l) = (pvcov(i+1,j,l) - pvcov(i,j,l) $ + pucov(i,j+1,l) - pucov(i,j,l)) $ / (cu(i,j)+cu(i,j+1)) $ / (cv(i+1,j)+cv(i,j)) *4 enddo enddo ENDDO 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) ) c pcvgv(ig0+i,l)= 0.5 * c $ ( pdvcov(i,j-1,l)/cv(i,j-1) + pdvcov(i,j,l)/cv(i,j) ) ENDDO zrfi(ig0 + 1,l)= 0.25 *(zrot(iim,j-1,l)+zrot(iim,j,l) & +zrot(1,j-1,l)+zrot(1,j,l)) DO i=2,iim zrfi(ig0 + i,l)= 0.25 *(zrot(i-1,j-1,l)+zrot(i-1,j,l) $ +zrot(i,j-1,l)+zrot(i,j,l)) ! AdlC MAY 2014 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 zrfi(1, l) = 0. 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 zrfi(ngridmx, l) = 0. ENDDO 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 --------------------- ! Appel de la physique: pose probleme quand on tourne ! SANS physique, car physiq.F est dans le repertoire phy[]... ! Il faut une cle CPP_PHYS ! Le fait que les arguments de physiq soient differents selon les planetes ! ne pose pas de probleme a priori. ! 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 CALL call_physiq(ngridmx,llm,nqtot,tname, & debut_split,lafin_split, & jD_cur,jH_cur_split,zdt_split, & zplev,zplay, & zpk,zphi,zphis, & presnivs, & zufi,zvfi,zrfi,ztfi,zqfi, & flxwfi,pducov, & zdufi,zdvfi,zdtfi,zdqfi,zdpsrf, & tracerdyn) ! if (planet_type.eq."earth") then ! CALL physiq (ngridmx, ! . llm, ! . debut_split, ! . lafin_split, ! . jD_cur, ! . jH_cur_split, ! . zdt_split, ! . zplev, ! . zplay, ! . zphi, ! . zphis, ! . presnivs, ! . zufi, ! . zvfi, ! . ztfi, ! . zqfi, ! . flxwfi, ! . zdufi, ! . zdvfi, ! . zdtfi, ! . zdqfi, ! . zdpsrf, ! . pducov) ! ! 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 ??? ! ! else if ( planet_type=="mars" ) then ! ! CALL physiq (ngridmx, ! ngrid ! . llm, ! nlayer ! . nqtot, ! nq ! . debut_split, ! firstcall ! . lafin_split, ! lastcall ! . jD_cur, ! pday ! . jH_cur_split, ! ptime ! . zdt_split, ! ptimestep ! . zplev, ! pplev ! . zplay, ! pplay ! . zphi, ! pphi ! . zufi, ! pu ! . zvfi, ! pv ! . ztfi, ! pt ! . zqfi, ! pq ! . flxwfi, ! pw ! . zdufi, ! pdu ! . zdvfi, ! pdv ! . zdtfi, ! pdt ! . zdqfi, ! pdq ! . zdpsrf, ! pdpsrf ! . tracerdyn) ! tracerdyn (somewhat obsolete) ! ! else if ((planet_type=="titan").or.(planet_type=="venus")) then ! ! CALL physiq (ngridmx, ! . llm, ! . nqtot, ! . debut_split, ! . lafin_split, ! . jD_cur, ! . jH_cur_split, ! . zdt_split, ! . zplev, ! . zplay, ! . zpk, ! . zphi, ! . zphis, ! . presnivs, ! . zufi, ! . zvfi, ! . ztfi, ! . zqfi, ! . flxwfi, ! . zdufi, ! . zdvfi, ! . zdtfi, ! . zdqfi, ! . zdpsrf) ! ! else ! unknown "planet_type" ! ! write(lunout,*) "calfis_p: error, unknown planet_type: ", ! & trim(planet_type) ! stop ! ! endif ! planet_type 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 ! ATTENTION... if (flag_moyzon.and.(nsplit_phys.ne.1)) then print*,"WARNING ! flag_moyzon + nsplit_phys" print*,"zqfibar n'est pas implemente au cours des iterations" print*,"Donc a revoir..." stop endif #endif ! #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 --------------------- ! ADAPTATION GCM POUR CP(T) call t2tpot(ngridmx*llm,ztfi,zteta,zpk) DO i=1,iip1 pdhfi(i,1,:) = (zteta(1,:) - pteta(i,1,:))/dtphys pdhfi(i,jjp1,:) = (zteta(ngridmx,:) - pteta(i,jjp1,:))/dtphys ENDDO DO j=2,jjm ig0=1+(j-2)*iim DO i=1,iim pdhfi(i,j,:) = (zteta(ig0+i,:) - pteta(i,j,:))/dtphys ENDDO pdhfi(iip1,j,:) = pdhfi(1,j,:) 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 (tous en intensifs) 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. #endif ! of #ifndef CPP_PARA END