! ! $Id: fluxstokenc.F 1299 2010-01-20 14:27:21Z musat $ ! SUBROUTINE fluxstokenc(pbaru,pbarv,masse,teta,phi,phis, . time_step,itau ) #ifdef CPP_EARTH ! This routine is designed to work for Earth and with ioipsl USE IOIPSL c c Auteur : F. Hourdin c c ccc .. Modif. P. Le Van ( 20/12/97 ) ... c IMPLICIT NONE c #include "dimensions.h" #include "paramet.h" #include "comconst.h" #include "comvert.h" #include "comgeom.h" #include "tracstoke.h" #include "temps.h" #include "iniprint.h" REAL time_step,t_wrt, t_ops REAL pbaru(ip1jmp1,llm),pbarv(ip1jm,llm) REAL masse(ip1jmp1,llm),teta(ip1jmp1,llm),phi(ip1jmp1,llm) REAL phis(ip1jmp1) REAL pbaruc(ip1jmp1,llm),pbarvc(ip1jm,llm) REAL massem(ip1jmp1,llm),tetac(ip1jmp1,llm),phic(ip1jmp1,llm) REAL pbarug(ip1jmp1,llm),pbarvg(iip1,jjm,llm),wg(ip1jmp1,llm) REAL pbarvst(iip1,jjp1,llm),zistdyn real dtcum INTEGER iadvtr,ndex(1) integer nscal real tst(1),ist(1),istp(1) INTEGER ij,l,irec,i,j,itau INTEGER, SAVE :: fluxid, fluxvid,fluxdid SAVE iadvtr, massem,pbaruc,pbarvc,irec SAVE phic,tetac logical first save first data first/.true./ DATA iadvtr/0/ c AC initialisations pbarug(:,:) = 0. pbarvg(:,:,:) = 0. wg(:,:) = 0. if(first) then CALL initfluxsto( 'fluxstoke', . time_step,istdyn* time_step,istdyn* time_step, . fluxid,fluxvid,fluxdid) ndex(1) = 0 call histwrite(fluxid, 'phis', 1, phis, iip1*jjp1, ndex) call histwrite(fluxid, 'aire', 1, aire, iip1*jjp1, ndex) ndex(1) = 0 nscal = 1 tst(1) = time_step call histwrite(fluxdid, 'dtvr', 1, tst, nscal, ndex) ist(1)=istdyn call histwrite(fluxdid, 'istdyn', 1, ist, nscal, ndex) istp(1)= istphy call histwrite(fluxdid, 'istphy', 1, istp, nscal, ndex) first = .false. endif IF(iadvtr.EQ.0) THEN CALL initial0(ijp1llm,phic) CALL initial0(ijp1llm,tetac) CALL initial0(ijp1llm,pbaruc) CALL initial0(ijmllm,pbarvc) ENDIF c accumulation des flux de masse horizontaux DO l=1,llm DO ij = 1,ip1jmp1 pbaruc(ij,l) = pbaruc(ij,l) + pbaru(ij,l) tetac(ij,l) = tetac(ij,l) + teta(ij,l) phic(ij,l) = phic(ij,l) + phi(ij,l) ENDDO DO ij = 1,ip1jm pbarvc(ij,l) = pbarvc(ij,l) + pbarv(ij,l) ENDDO ENDDO c selection de la masse instantannee des mailles avant le transport. IF(iadvtr.EQ.0) THEN CALL SCOPY(ip1jmp1*llm,masse,1,massem,1) ENDIF iadvtr = iadvtr+1 c Test pour savoir si on advecte a ce pas de temps IF ( iadvtr.EQ.istdyn ) THEN c normalisation DO l=1,llm DO ij = 1,ip1jmp1 pbaruc(ij,l) = pbaruc(ij,l)/REAL(istdyn) tetac(ij,l) = tetac(ij,l)/REAL(istdyn) phic(ij,l) = phic(ij,l)/REAL(istdyn) ENDDO DO ij = 1,ip1jm pbarvc(ij,l) = pbarvc(ij,l)/REAL(istdyn) ENDDO ENDDO c traitement des flux de masse avant advection. c 1. calcul de w c 2. groupement des mailles pres du pole. CALL groupe( massem, pbaruc,pbarvc, pbarug,pbarvg,wg ) do l=1,llm do j=1,jjm do i=1,iip1 pbarvst(i,j,l)=pbarvg(i,j,l) enddo enddo do i=1,iip1 pbarvst(i,jjp1,l)=0. enddo enddo iadvtr=0 Print*,'ITAU auqel on stoke les fluxmasses',itau call histwrite(fluxid, 'masse', itau, massem, . iip1*jjp1*llm, ndex) call histwrite(fluxid, 'pbaru', itau, pbarug, . iip1*jjp1*llm, ndex) call histwrite(fluxvid, 'pbarv', itau, pbarvg, . iip1*jjm*llm, ndex) call histwrite(fluxid, 'w' ,itau, wg, . iip1*jjp1*llm, ndex) call histwrite(fluxid, 'teta' ,itau, tetac, . iip1*jjp1*llm, ndex) call histwrite(fluxid, 'phi' ,itau, phic, . iip1*jjp1*llm, ndex) C ENDIF ! if iadvtr.EQ.istdyn #else write(lunout,*) & 'fluxstokenc: Needs Earth physics (and ioipsl) to function' #endif ! of #ifdef CPP_EARTH RETURN END