C======================================================================= SUBROUTINE CERENE( STEPCR ) C----------------------------------------------------------------------- C CEREN(KOV RADIATION FROM) E(LECTRONS) C C CREATION OF CERENKOV PHOTONS ALONG A TRACK OF ELECTRONS C CERENKOV RADIATION IS ONLY CALCULATED FOR LOWEST OBSERVATION LEVEL C THE COORDINATES ON EGS-STACK ARE AT THE END OF STEP EXCEPT E(NP), C WHICH IS AT THE BEGINNING OF STEP C THIS SUBROUTINE IS CALLED FROM ELECTR C ARGUMENT: C STEPCR = STEP LENGTH FOR ELECTRON OR POSITRON (REAL*4) C C AUTHOR : M. ROZANSKA UNIVERSITY OF KRAKOW C S. MARTINEZ UNIVERSITY OF MADRID C F. ARQUEROS UNIVERSITY OF MADRID C CHANGES : D. HECK IK3 FZK KARLSRUHE C R. ATTALLAH UNIVERSITY OF PERPIGNAN C----------------------------------------------------------------------- c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> parameter (xct=1) parameter (yct=2) parameter (zct=3) parameter (ctthet=4) parameter (ctphi=5) parameter (ctdiam=6) parameter (ctfoc=7) c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c IMPLICIT NONE *KEEP,BUFFS. COMMON /BUFFS/ RUNH,RUNE,EVTH,EVTE,DATAB,LH INTEGER MAXBUF,MAXLEN PARAMETER (MAXBUF=39*7) PARAMETER (MAXLEN=12) REAL RUNH(MAXBUF),EVTH(MAXBUF),EVTE(MAXBUF), * RUNE(MAXBUF),DATAB(MAXBUF) INTEGER LH CHARACTER*4 CRUNH,CRUNE,CEVTH,CEVTE EQUIVALENCE (RUNH(1),CRUNH), (RUNE(1),CRUNE) EQUIVALENCE (EVTH(1),CEVTH), (EVTE(1),CEVTE) *KEEP,CONST. COMMON /CONST/ PI,PI2,OB3,TB3,ENEPER DOUBLE PRECISION PI,PI2,OB3,TB3,ENEPER *KEEP,EPCONT. COMMON/EPCONT/ EDEP,RATIO,TSTEP,TUSTEP,USTEP,TVSTEP,VSTEP,IDISC, * IROLD,IRNEW,RHOFAC, EOLD,ENEW,EKE,ELKE,BETA2,GLE, * TSCAT,IAUSFL DOUBLE PRECISION EDEP,RATIO REAL TSTEP,TUSTEP,USTEP,TVSTEP,VSTEP,RHOFAC,EOLD,ENEW, * EKE,ELKE,BETA2,GLE,TSCAT INTEGER IDISC,IROLD,IRNEW,IAUSFL(29) *KEEP,LONGI. COMMON /LONGI/ APLONG,HLONG,PLONG,SPLONG,THSTEP,THSTPI, * NSTEP,LLONGI,FLGFIT DOUBLE PRECISION APLONG(0:1040,9),HLONG(0:1024),PLONG(0:1040,9), * SPLONG(0:1040,9),THSTEP,THSTPI INTEGER NSTEP LOGICAL LLONGI,FLGFIT *KEEP,MAGANG. COMMON /MAGANG/ ARRANG,ARRANR,COSANG,SINANG DOUBLE PRECISION ARRANG,ARRANR,COSANG,SINANG *KEEP,OBSPAR. COMMON /OBSPAR/ OBSLEV,THCKOB,XOFF,YOFF,THETAP,PHIP, * THETPR,PHIPR,NOBSLV DOUBLE PRECISION OBSLEV(10),THCKOB(10),XOFF(10),YOFF(10), * THETAP,THETPR(2),PHIP,PHIPR(2) INTEGER NOBSLV *KEEP,PAM. COMMON /PAM/ PAMA,SIGNUM DOUBLE PRECISION PAMA(6000),SIGNUM(6000) *KEEP,PARPAR. COMMON /PARPAR/ CURPAR,SECPAR,PRMPAR,OUTPAR,C, * E00,E00PN,PTOT0,PTOT0N,THICKH,ITYPE,LEVL DOUBLE PRECISION CURPAR(14),SECPAR(14),PRMPAR(14),OUTPAR(14), * C(50),E00,E00PN,PTOT0,PTOT0N,THICKH INTEGER ITYPE,LEVL *KEEP,RANDPA. COMMON /RANDPA/ FAC,U1,U2,RD,NSEQ,ISEED,KNOR DOUBLE PRECISION FAC,U1,U2 REAL RD(3000) INTEGER ISEED(103,10),NSEQ LOGICAL KNOR *KEEP,RUNPAR. COMMON /RUNPAR/ FIXHEI,THICK0,HILOECM,HILOELB, * STEPFC,NRRUN,NSHOW,PATAPE,MONIIN, * MONIOU,MDEBUG,NUCNUC, * CETAPE, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE, * DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG COMMON /RUNPAC/ DSN,HOST,USER DOUBLE PRECISION FIXHEI,THICK0,HILOECM,HILOELB REAL STEPFC INTEGER NRRUN,NSHOW,PATAPE,MONIIN,MONIOU,MDEBUG,NUCNUC, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE INTEGER CETAPE CHARACTER*79 DSN CHARACTER*20 HOST,USER LOGICAL DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG *KEEP,STACKE. COMMON/STACKE/ E,TIME,X,Y,Z,U,V,W,DNEAR,IQ,IGEN,IR,IOBS,LPCTE,NP DOUBLE PRECISION E(60),TIME(60) REAL X(60),Y(60),Z(60),U(60),V(60),W(60),DNEAR(60) INTEGER IQ(60),IGEN(60),IR(60),IOBS(60),LPCTE(60),NP *KEEP,CEREN1. COMMON /CEREN1/ CERELE,CERHAD,ETADSN,WAVLGL,WAVLGU,CYIELD, * CERSIZ,LCERFI DOUBLE PRECISION CERELE,CERHAD,ETADSN,WAVLGL,WAVLGU,CYIELD REAL CERSIZ LOGICAL LCERFI *KEEP,CEREN2. COMMON /CEREN2/ PHOTCM,XCER,YCER,UEMIS,VEMIS,CARTIM,ZEMIS, * DCERX,DCERY,ACERX,ACERY, * XCMAX,YCMAX,EPSX,EPSY, * DCERXI,DCERYI,FCERX,FCERY, * XSCATT,YSCATT,CERXOS,CERYOS, * NCERX,NCERY,ICERML REAL PHOTCM,XCER,YCER,UEMIS,VEMIS,CARTIM,ZEMIS, * DCERX,DCERY,ACERX,ACERY, * XCMAX,YCMAX,EPSX,EPSY, * DCERXI,DCERYI,FCERX,FCERY, * XSCATT,YSCATT,CERXOS(20),CERYOS(20) INTEGER NCERX,NCERY,ICERML c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> *keep,certel. common /certel/ cormxd,cord,coralp,ctpars,omega, + photn,photnp,phpt,pht,vphot, + vchi,veta,vzeta,vchim,vetam,vzetam, + lambda,mu,nu,nctels,ncph double precision cormxd,cord,coralp,ctpars(20,7),omega(20,3,3), + photn(3),photnp(3),phpt(3),pht,vphot(3), + vchi(3),veta(3),vzeta(3),vchim,vetam,vzetam, + lambda,mu,nu integer nctels,ncph(5) double precision xg,yg,zg,xgp,ygp,zgp,up,vp,wp,xpcut,ypcut,zpcut equivalence (photn(1) ,xg) ,(photn(2) ,yg) ,(photn(3) ,zg) , + (photnp(1),xgp) ,(photnp(2),ygp) ,(photnp(3),zgp), + (phpt(1) ,xpcut),(phpt(2) ,ypcut),(phpt(3) ,zpcut), + (vphot(1) ,up) ,(vphot(2) ,vp) ,(vphot(3) ,wp) character *72 ctfile *keep,graal1. common /graal1/ wavelength ! (nm) real wavelength c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> *KEND. COMMON /ACLOCK/ NCLOCK,JCLOCK DOUBLE PRECISION BETAE,BETAF,BETAI,CTHETA,DBETA,ECR, * ETA1,E1,STHETA,STHETF,STHETI DOUBLE PRECISION RHOF,THICK REAL A,B,CC,COSCR,COSDEL,DVCOR,DXXX,DYYY,FSTEPI, * HTOP,H2,PATHCR,PHICER,PHOTCT,RADINV, * SINCR,SINDEL,SINPSI,SINPS2,STEPCR,UEMIS2,US,VCOR, * VEMIS2,VS,WEMIS,XCER1,XCER2,XEMIS,XXX, * YCER1,YCER2,YEMIS,YYY INTEGER I,ISTC,I1,JCLOCK,LPCT1,NCLOCK,NSTEPC EXTERNAL RHOF,THICK C----------------------------------------------------------------------- C_____IF (NCLOCK.GT.JCLOCK) THEN C______WRITE(MDEBUG,*)'CERENE: NP=',NP,' IR=',IR(NP),' IOBS=',IOBS(NP) C______CALL AUSGB2 C_____ENDIF C----------------------------------------------------------------------- C SKIP PARTICLES OUT OF ZENITH ANGULAR CUT IF ( W(NP) .LT. C(29) ) RETURN C E(NP) IS ENERGY AT BEGIN OF STEP E1 = E(NP) C LOOK WETHER CERENKOV CONDITION IS FULFILLED AT BEGIN OF STEP BETAI = SQRT( 1.D0 - (PAMA(2)*1.D3/E1)**2 ) C REFRACTIVE INDEX PARAMETRISATION: N=1+ETA = ETA1 H2 = -Z(NP) HTOP = H2 + VSTEP * W(NP) ETA1 = 1.D0 + ETADSN * RHOF(DBLE(HTOP)) CTHETA = 1.D0 /( ETA1 * BETAI) STHETI = 1.D0 - CTHETA**2 IF ( STHETI .GT. 0.D0 ) THEN C PARTICLE IS ABOVE ENERGY THRESHOLD IF EMISSION ANGLE IS >0 PHOTCT = CYIELD * STEPCR * STHETI NSTEPC = PHOTCT / CERSIZ + 1 IF ( NSTEPC .LT. 1 ) RETURN FSTEPI = 1. / REAL(NSTEPC) C CALCULATE INCREMENTS AND START VALUES FOR POSITION AND VELOCITY DVCOR = -VSTEP * FSTEPI VCOR = VSTEP - 0.5 * DVCOR DBETA = -2.D0*FSTEPI*EDEP*(PAMA(2)*1.D3)**2 / (E1**3*BETAI) BETAE = BETAI - 0.5D0 * DBETA ELSE C LOOK WETHER CERENKOV CONDITION IS FULFILLED AT END OF STEP, BUT NOT C AT THE BEGINNING. THIS MAY HAPPEN ONLY ABOVE ABOUT 22 KM IF ( HTOP .LT. 22.E5 ) RETURN C ENERGY AT END OF STEP IS ENEW (FROM COMMON EPCONT) BETAF = SQRT( 1.D0 - (PAMA(2)*1.D3/ENEW)**2 ) C REFRACTIVE INDEX PARAMETRISATION: N=1+ETA = ETA1 ETA1 = 1.D0 + ETADSN * RHOF( DBLE(H2) ) CTHETA = 1.D0 /( ETA1 * BETAF) STHETF = 1.D0 - CTHETA**2 C PARTICLE IS BELOW ENERGY THRESHOLD IF EMISSION ANGLE IS 0 IF ( STHETF .LE. 0.D0 ) RETURN PHOTCT = CYIELD * STEPCR * STHETF NSTEPC = PHOTCT / CERSIZ + 1 IF ( NSTEPC .LT. 1 ) RETURN FSTEPI = 1. / REAL(NSTEPC) C CALCULATE INCREMENTS AND START VALUES FOR POSITION AND VELOCITY C LOOP 1000 RUNS FROM BOTTOM TO TOP OF STEP DVCOR = VSTEP * FSTEPI VCOR = -0.5 * DVCOR DBETA = 2.D0*FSTEPI*EDEP*(PAMA(2)*1.D3)**2 / (ENEW**3*BETAF) BETAE = BETAF - 0.5D0 * DBETA ENDIF C LOOP OVER SUBSTEPS DO 1000 ISTC = 1,NSTEPC VCOR = VCOR + DVCOR ZEMIS = H2 + VCOR * W(NP) ETA1 = 1.D0 + ETADSN * RHOF(DBLE(ZEMIS)) C VELOCITY IN THE MIDDLE OF SUBSTEP BETAE = BETAE + DBETA CTHETA = 1.D0 / (ETA1*BETAE) STHETA = 1.D0 - CTHETA**2 C PARTICLE IS AT ENERGY THRESHOLD IF EMISSION ANGLE BECOMES 0 IF ( STHETA .LE. 0.D0 ) RETURN C NUMBER OF EMITTED PHOTONS ON DISTANCE DVCOR PHOTCM = CYIELD * STHETA * STEPCR * FSTEPI STHETA = SQRT(STHETA) C ASSUME EMISSION POINT OF ALL PHOTONS IN THE MIDDLE OF THE STEP XEMIS = X(NP) - VCOR * U(NP) YEMIS = -Y(NP) + VCOR * V(NP) C>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> C GENERATE RANDOM WAVELENGTH FOR SINGLE C-PHOTON. CALL RMMAR( RD,1,3 ) WAVELENGTH = 1. / (1/WAVLGL - + RD(1)/(WAVLGL*WAVLGU/(WAVLGU-WAVLGL))) C>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> C CALCULATE PHOTON DIRECTION IN THE CORSIKA COORDINATE FRAME CALL RMMAR( RD,1,3 ) PHICER = RD(1) * PI2 SINCR = SIN(PHICER) COSCR = COS(PHICER) A = U(NP) B = -V(NP) CC = W(NP) SINPS2 = A**2 + B**2 IF ( SINPS2 .LT. 1.E-10 ) THEN UEMIS = STHETA * COSCR VEMIS = STHETA * SINCR WEMIS = CTHETA * CC ELSE SINPSI = SQRT(SINPS2) US = STHETA * COSCR VS = STHETA * SINCR SINDEL = B * (1./SINPSI) COSDEL = A * (1./SINPSI) UEMIS = CC * COSDEL * US - SINDEL * VS + A * CTHETA VEMIS = CC * SINDEL * US + COSDEL * VS + B * CTHETA WEMIS = -SINPSI * US + CC * CTHETA ENDIF C EMISSION ANGLE WITHIN ZENITH ANGULAR CUT? IF ( WEMIS .LT. C(29) ) GOTO 1000 RADINV = 1.5 - 0.5 * ( UEMIS**2 + VEMIS**2 + WEMIS**2 ) UEMIS2 = UEMIS * RADINV VEMIS2 = VEMIS * RADINV WEMIS = WEMIS * RADINV C CALCULATE DISTANCE FROM SHOWER AXIS AT THE DETECTOR LEVEL PATHCR = ( ZEMIS - OBSLEV(NOBSLV) ) / WEMIS XCER2 = XEMIS + PATHCR * UEMIS2 - XOFF(NOBSLV) YCER2 = YEMIS + PATHCR * VEMIS2 - YOFF(NOBSLV) C ADD THE CERENKOV PHOTONS TO THE LONGITUDINAL DEVELOPMENT IF ( LLONGI ) THEN C IF STARTING POINT BELOW LOWEST LEVEL THEN DON'T CHECK IF ( HLONG(NSTEP) .LE. ZEMIS ) THEN C FIND FIRST THE EQUIVALENT LEVELS LPCT1 = LPCTE(NP) C ZEMIS IS ONLY LITTLE BELOW Z OLD, THEREFORE INCREMENTAL SEARCH C (REMEBER: LPCTE IS AT START OF ELECTRON STEP) DO 6002 I1 = LPCT1,NSTEP IF ( HLONG(I1) .LT. ZEMIS ) GOTO 6003 6002 CONTINUE I1 = NSTEP + 1 6003 CONTINUE DO 4862 I=I1,NSTEP PLONG(I,9) = PLONG(I,9) + PHOTCM 4862 CONTINUE ENDIF ENDIF C TAKE INTO ACCOUNT A ROTATION OF ARRAY RELATIVE TO MAGNETIC NORD XCER = XCER2 * COSANG + YCER2 * SINANG YCER = YCER2 * COSANG - XCER2 * SINANG UEMIS = UEMIS2 * COSANG + VEMIS2 * SINANG VEMIS = VEMIS2 * COSANG - UEMIS2 * SINANG c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> CERELE = CERELE + PHOTCM DO 7001 I=1,ICERML DO 101 NCT=1,NCTELS c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c>> Modification to implement sphere algorithm >>>>>>>>>>>>>>>>>>>>>>>> c>> JCG Wed Sep 21 10:49:14 MET DST 1998 >>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c>>>>> this is the last (simple) check <<<<< C changes to ct frame c XG = XCER - CERXOS(I) - CTPARS(NCT,XCT) c YG = YCER - CERYOS(I) - CTPARS(NCT,YCT) c ZG = 0.0 - CTPARS(NCT,ZCT) c DIST2 = SQRT( XG**2 + YG**2 ) c IF ( DIST2 .LT. (CTPARS(NCT,CTDIAM)/2.) ) GOTO 102 c>> New check >>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> XG = XCER - CERXOS(I) YG = YCER - CERYOS(I) ZG = 0.0 DIST2 = > SQRT((VEMIS*(-CTPARS(NCT,XCT) + XG) - > UEMIS*(-CTPARS(NCT,YCT) + YG))**2 + > (-(SQRT(1 - UEMIS**2 - VEMIS**2)* > (-CTPARS(NCT,XCT) + XG)) + > UEMIS*(-CTPARS(NCT,ZCT) + ZG))**2 + > (SQRT(1 - UEMIS**2 - VEMIS**2)* > (-CTPARS(NCT,YCT) + YG) - > VEMIS*(-CTPARS(NCT,ZCT) + ZG))**2) IF ( DIST2 .LT. (CTPARS(NCT,CTDIAM)/2.) ) GOTO 102 c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> 101 CONTINUE GOTO 7001 C BUNCH FALLS ON A DETECTOR, CALCULATE ARRIVAL TIME (NSEC) 102 CARTIM = ((ETADSN*(THCKOB(NOBSLV)-THICK(DBLE(ZEMIS))) * /WEMIS+PATHCR-VCOR/BETAE)/C(25)+TIME(NP))* 1.E9 c CALL OUTPT2(IQ(NP),I) CALL OUTPT2(NCT,I) c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> call jctime(cartim) c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> GOTO 1000 7001 CONTINUE 1000 CONTINUE c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> RETURN END C======================================================================= SUBROUTINE CERENH( STEPCR,BETACR ) C----------------------------------------------------------------------- C CEREN(KOV RADIATION FROM) H(ADRONS) C C CERENKOV RADIATION FROM HADRONS C CERENKOV RADIATION IS ONLY CALCULATED FOR LOWEST OBSERVATION LEVEL C THIS SUBROUTINE IS CALLED FROM UPDATE C ARGUMENTS: C STEPCR = STEP LENGTH FOR ELECTRON OR POSITRON C BETACR = VELOCITY OF PARTICLE IN UNITS OF SPEED OF LIGHT C C AUTHOR : M. ROZANSKA UNIVERSITY OF KRAKOW C S. MARTINEZ UNIVERSITY OF MADRID C F. ARQUEROS UNIVERSITY OF MADRID C CHANGES : D. HECK IK3 FZK KARLSRUHE C----------------------------------------------------------------------- c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> parameter (xct=1) parameter (yct=2) parameter (zct=3) parameter (ctthet=4) parameter (ctphi=5) parameter (ctdiam=6) parameter (ctfoc=7) c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c IMPLICIT NONE *KEEP,BUFFS. COMMON /BUFFS/ RUNH,RUNE,EVTH,EVTE,DATAB,LH INTEGER MAXBUF,MAXLEN PARAMETER (MAXBUF=39*7) PARAMETER (MAXLEN=12) REAL RUNH(MAXBUF),EVTH(MAXBUF),EVTE(MAXBUF), * RUNE(MAXBUF),DATAB(MAXBUF) INTEGER LH CHARACTER*4 CRUNH,CRUNE,CEVTH,CEVTE EQUIVALENCE (RUNH(1),CRUNH), (RUNE(1),CRUNE) EQUIVALENCE (EVTH(1),CEVTH), (EVTE(1),CEVTE) *KEEP,CONST. COMMON /CONST/ PI,PI2,OB3,TB3,ENEPER DOUBLE PRECISION PI,PI2,OB3,TB3,ENEPER *KEEP,EPCONT. COMMON/EPCONT/ EDEP,RATIO,TSTEP,TUSTEP,USTEP,TVSTEP,VSTEP,IDISC, * IROLD,IRNEW,RHOFAC, EOLD,ENEW,EKE,ELKE,BETA2,GLE, * TSCAT,IAUSFL DOUBLE PRECISION EDEP,RATIO REAL TSTEP,TUSTEP,USTEP,TVSTEP,VSTEP,RHOFAC,EOLD,ENEW, * EKE,ELKE,BETA2,GLE,TSCAT INTEGER IDISC,IROLD,IRNEW,IAUSFL(29) *KEEP,LONGI. COMMON /LONGI/ APLONG,HLONG,PLONG,SPLONG,THSTEP,THSTPI, * NSTEP,LLONGI,FLGFIT DOUBLE PRECISION APLONG(0:1040,9),HLONG(0:1024),PLONG(0:1040,9), * SPLONG(0:1040,9),THSTEP,THSTPI INTEGER NSTEP LOGICAL LLONGI,FLGFIT *KEEP,MAGANG. COMMON /MAGANG/ ARRANG,ARRANR,COSANG,SINANG DOUBLE PRECISION ARRANG,ARRANR,COSANG,SINANG *KEEP,OBSPAR. COMMON /OBSPAR/ OBSLEV,THCKOB,XOFF,YOFF,THETAP,PHIP, * THETPR,PHIPR,NOBSLV DOUBLE PRECISION OBSLEV(10),THCKOB(10),XOFF(10),YOFF(10), * THETAP,THETPR(2),PHIP,PHIPR(2) INTEGER NOBSLV *KEEP,PAM. COMMON /PAM/ PAMA,SIGNUM DOUBLE PRECISION PAMA(6000),SIGNUM(6000) *KEEP,PARPAR. COMMON /PARPAR/ CURPAR,SECPAR,PRMPAR,OUTPAR,C, * E00,E00PN,PTOT0,PTOT0N,THICKH,ITYPE,LEVL DOUBLE PRECISION CURPAR(14),SECPAR(14),PRMPAR(14),OUTPAR(14), * C(50),E00,E00PN,PTOT0,PTOT0N,THICKH INTEGER ITYPE,LEVL *KEEP,PARPAE. DOUBLE PRECISION GAMMA,COSTHE,PHI,H,T,X,Y,CHI,BETA,GCM,ECM EQUIVALENCE (CURPAR(2),GAMMA), (CURPAR(3),COSTHE), * (CURPAR(4), PHI ), (CURPAR(5), H ), * (CURPAR(6), T ), (CURPAR(7), X ), * (CURPAR(8), Y ), (CURPAR(9), CHI ), * (CURPAR(10),BETA), (CURPAR(11),GCM ), * (CURPAR(12),ECM ) *KEEP,RANDPA. COMMON /RANDPA/ FAC,U1,U2,RD,NSEQ,ISEED,KNOR DOUBLE PRECISION FAC,U1,U2 REAL RD(3000) INTEGER ISEED(103,10),NSEQ LOGICAL KNOR *KEEP,RUNPAR. COMMON /RUNPAR/ FIXHEI,THICK0,HILOECM,HILOELB, * STEPFC,NRRUN,NSHOW,PATAPE,MONIIN, * MONIOU,MDEBUG,NUCNUC, * CETAPE, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE, * DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG COMMON /RUNPAC/ DSN,HOST,USER DOUBLE PRECISION FIXHEI,THICK0,HILOECM,HILOELB REAL STEPFC INTEGER NRRUN,NSHOW,PATAPE,MONIIN,MONIOU,MDEBUG,NUCNUC, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE INTEGER CETAPE CHARACTER*79 DSN CHARACTER*20 HOST,USER LOGICAL DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG *KEEP,CEREN1. COMMON /CEREN1/ CERELE,CERHAD,ETADSN,WAVLGL,WAVLGU,CYIELD, * CERSIZ,LCERFI DOUBLE PRECISION CERELE,CERHAD,ETADSN,WAVLGL,WAVLGU,CYIELD REAL CERSIZ LOGICAL LCERFI *KEEP,CEREN2. COMMON /CEREN2/ PHOTCM,XCER,YCER,UEMIS,VEMIS,CARTIM,ZEMIS, * DCERX,DCERY,ACERX,ACERY, * XCMAX,YCMAX,EPSX,EPSY, * DCERXI,DCERYI,FCERX,FCERY, * XSCATT,YSCATT,CERXOS,CERYOS, * NCERX,NCERY,ICERML REAL PHOTCM,XCER,YCER,UEMIS,VEMIS,CARTIM,ZEMIS, * DCERX,DCERY,ACERX,ACERY, * XCMAX,YCMAX,EPSX,EPSY, * DCERXI,DCERYI,FCERX,FCERY, * XSCATT,YSCATT,CERXOS(20),CERYOS(20) INTEGER NCERX,NCERY,ICERML *KEEP,CERHDR. COMMON/CERHDR/ TPART,UPART,VPART,WPART,XPART,YPART,ZPART DOUBLE PRECISION TPART,UPART,VPART,WPART,XPART,YPART,ZPART c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> *keep,certel. common /certel/ cormxd,cord,coralp,ctpars,omega, + photn,photnp,phpt,pht,vphot, + vchi,veta,vzeta,vchim,vetam,vzetam, + lambda,mu,nu,nctels,ncph double precision cormxd,cord,coralp,ctpars(20,7),omega(20,3,3), + photn(3),photnp(3),phpt(3),pht,vphot(3), + vchi(3),veta(3),vzeta(3),vchim,vetam,vzetam, + lambda,mu,nu integer nctels,ncph(5) double precision xg,yg,zg,xgp,ygp,zgp,up,vp,wp,xpcut,ypcut,zpcut equivalence (photn(1) ,xg) ,(photn(2) ,yg) ,(photn(3) ,zg) , + (photnp(1),xgp) ,(photnp(2),ygp) ,(photnp(3),zgp), + (phpt(1) ,xpcut),(phpt(2) ,ypcut),(phpt(3) ,zpcut), + (vphot(1) ,up) ,(vphot(2) ,vp) ,(vphot(3) ,wp) character *72 ctfile *keep,graal1. common /graal1/ wavelength ! (nm) real wavelength c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> *KEND. DOUBLE PRECISION BETACR,CINTEN,CTHETA,ETA,ETA1,HMID,PHOTCT, * RHOF,STEPCR,STHETA,THICK REAL A,B,CC,COSCR,COSDEL,DVCOR,DXXX,DYYY,FSTEPI, * PATHCR,PHICER,RADINV,SINCR,SINDEL,SINPSI,SINPS2, * UEMIS2,US,VEMIS2,VCOR,VS,WEMIS,XCER1,XCER2,XEMIS, * XXX,YCER1,YCER2,YEMIS,YYY INTEGER I,II,ISTC,I1,I2,NSTEPC EXTERNAL RHOF,THICK C----------------------------------------------------------------------- c IF ( DEBUG ) WRITE(MDEBUG,*) 'CERENH: ZPART=',SNGL(ZPART), c * ' STEPCR=',SNGL(STEPCR),' BETACR=',SNGL(BETACR) C SKIP PARTICLE OUT OF ANGULAR ACCEPTANCE RANGE IF ( WPART .LT. C(29) ) RETURN C CERENKOV INTENSITY FACTOR DEPENDS ON CHARGE STATE OF HEAVY IONS CINTEN = CYIELD * ABS(SIGNUM(INT(CURPAR(1)))) C REFRACTIVE INDEX PARAMETRISATION: N=1+ETA HMID = ZPART + 0.5D0 * STEPCR * WPART ETA1 = 1.D0 + ETADSN * RHOF(DBLE(HMID)) CTHETA = 1.D0 / ( ETA1 * BETACR ) STHETA = 1.D0 - CTHETA**2 IF ( STHETA .LE. 0.D0 ) RETURN PHOTCT = CINTEN * STHETA * STEPCR NSTEPC = PHOTCT / CERSIZ + 1 IF ( NSTEPC .LT. 1 ) RETURN FSTEPI = 1. / REAL(NSTEPC) VCOR = -0.5 * STEPCR * FSTEPI DVCOR = -2. * VCOR C CERENKOV RADIATION IS ONLY CALCULATED FOR LOWEST OBSERVATION LEVEL DO 1000 ISTC = 1,NSTEPC VCOR = VCOR + DVCOR ZEMIS = ZPART + VCOR * WPART ETA = ETADSN * RHOF(DBLE(ZEMIS)) ETA1 = 1.D0 + ETA CTHETA = 1.D0 / ( ETA1 * BETACR ) STHETA = 1.D0 - CTHETA**2 IF ( STHETA .LE. 0.D0 ) RETURN C NUMBER OF EMITTED PHOTONS ON DISTANCE STEPCR PHOTCM = CINTEN * STHETA * STEPCR * FSTEPI STHETA = SQRT(STHETA) C ASSUME EMISSION POINT OF ALL PHOTONS IN THE MIDDLE OF THE STEP C HAS TO BE CHECKED IF STEPS ARE NOT TOO LONG XEMIS = XPART - VCOR * UPART YEMIS = YPART - VCOR * VPART C>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> C GENERATE RANDOM WAVELENGTH FOR SINGLE C-PHOTON. CALL RMMAR( RD,1,3 ) WAVELENGTH = 1. / (1/WAVLGL - + RD(1)/(WAVLGL*WAVLGU/(WAVLGU-WAVLGL))) C>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> C CALCULATE PHOTON DIRECTION IN THE OVERALL COORDINATE FRAME CALL RMMAR( RD,1,3 ) PHICER = RD(1) * PI2 SINCR = SIN(PHICER) COSCR = COS(PHICER) A = UPART B = VPART CC = WPART SINPS2 = A**2 + B**2 IF ( SINPS2 .LT. 1.E-10 ) THEN UEMIS = STHETA * COSCR VEMIS = STHETA * SINCR WEMIS = CTHETA * CC ELSE SINPSI = SQRT(SINPS2) US = STHETA * COSCR VS = STHETA * SINCR SINDEL = B * (1./SINPSI) COSDEL = A * (1./SINPSI) UEMIS = CC * COSDEL * US - SINDEL * VS + A * CTHETA VEMIS = CC * SINDEL * US + COSDEL * VS + B * CTHETA WEMIS = -SINPSI * US + CC * CTHETA ENDIF C EMISSION ANGLE WITHIN ZENITH ANGULAR CUT? IF ( WEMIS .LT. C(29) ) GOTO 1000 RADINV = 1.5 - 0.5 * ( UEMIS**2 + VEMIS**2 + WEMIS**2 ) UEMIS2 = UEMIS * RADINV VEMIS2 = VEMIS * RADINV WEMIS = WEMIS * RADINV C CALCULATE DISTANCE FROM SHOWER AXIS AT THE DETECTOR LEVEL PATHCR = ( ZEMIS - OBSLEV(NOBSLV) ) / WEMIS XCER2 = XEMIS + PATHCR * UEMIS2 - XOFF(NOBSLV) YCER2 = YEMIS + PATHCR * VEMIS2 - YOFF(NOBSLV) C ADD THE CERENKOV PHOTONS TO THE LONGITUDINAL DEVELOPMENT IF ( LLONGI ) THEN C IF STARTING POINT BELOW LOWEST LEVEL THEN DON'T CHECK IF ( HLONG(NSTEP) .LE. ZEMIS ) THEN C FIND FIRST THE EQUIVALENT LEVELS I1 = 0 I2 = NSTEP 6001 CONTINUE II = (I1+I2)/2 IF ( HLONG(II) .LT. ZEMIS ) THEN I2 = II ELSE I1 = II ENDIF IF ( I2-I1 .GT. 1 ) GOTO 6001 DO 4862 I=I2,NSTEP PLONG(I,9) = PLONG(I,9) + PHOTCM 4862 CONTINUE ENDIF ENDIF C TAKE INTO ACCOUNT A ROTATION OF ARRAY RELATIVE TO MAGNETIC NORD XCER = XCER2 * COSANG + YCER2 * SINANG YCER = YCER2 * COSANG - XCER2 * SINANG UEMIS = UEMIS2 * COSANG + VEMIS2 * SINANG VEMIS = VEMIS2 * COSANG - UEMIS2 * SINANG c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> CERHAD = CERHAD + PHOTCM DO 7001 I=1,ICERML DO 101 NCT=1,NCTELS c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c>> Modification to implement sphere algorithm >>>>>>>>>>>>>>>>>>>>>>>> c>> JCG Wed Sep 21 10:49:14 MET DST 1998 >>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c>>>>> this is the last (simple) check <<<<< C changes to ct frame c XG = XCER - CERXOS(I) - CTPARS(NCT,XCT) c YG = YCER - CERYOS(I) - CTPARS(NCT,YCT) c ZG = 0.0 - CTPARS(NCT,ZCT) c DIST2 = SQRT( XG**2 + YG**2 ) c IF ( DIST2 .LT. (CTPARS(NCT,CTDIAM)/2.) ) GOTO 102 c>> New check >>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> XG = XCER - CERXOS(I) YG = YCER - CERYOS(I) ZG = 0.0 DIST2 = > SQRT((VEMIS*(-CTPARS(NCT,XCT) + XG) - > UEMIS*(-CTPARS(NCT,YCT) + YG))**2 + > (-(SQRT(1 - UEMIS**2 - VEMIS**2)* > (-CTPARS(NCT,XCT) + XG)) + > UEMIS*(-CTPARS(NCT,ZCT) + ZG))**2 + > (SQRT(1 - UEMIS**2 - VEMIS**2)* > (-CTPARS(NCT,YCT) + YG) - > VEMIS*(-CTPARS(NCT,ZCT) + ZG))**2) IF ( DIST2 .LT. (CTPARS(NCT,CTDIAM)/2.) ) GOTO 102 c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> 101 CONTINUE GOTO 7001 C BUNCH FALLS ON A DETECTOR, CALCULATE ARRIVAL TIME (NSEC) 102 CARTIM = ((ETADSN*(THCKOB(NOBSLV)-THICK(DBLE(ZEMIS))) * /WEMIS+PATHCR-VCOR/BETACR)/C(25)+TPART)*1.E9 c CALL OUTPT2(INT(CURPAR(1)),I) CALL OUTPT2(NCT,I) c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> call jctime(cartim) c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> GOTO 1000 7001 CONTINUE 1000 CONTINUE c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> RETURN END C======================================================================= SUBROUTINE GETBUS( IPARTI,ENERGY,THETA,CERSZE ) C----------------------------------------------------------------------- C GET BU(NCH) S(IZE) C C CALCULATES OPTIMAL BUNCH SIZE FOR CERENKOV PHOTONS. CERENKOV PHOTONS C ARE GROUPED IN BUNCHES IN ORDER TO ACCELERATE COMPUTING TIME. C HOWEVER, WE SET A MAXIMAL VALUE FOR THE GROUPING OF CERENKOV PHOTONS C SO THAT WE GET AT LEAST 100 BUNCHES/M**2 AT A CERENKOV FLUX OF 3000 C PHOTONS/M**2. THIS IS THE MINIMUM CERENKOV FLUX WHICH CAN BE C DISTINGUISHED FROM THE NIGHT SKY LIGHT BACKGROUND IN THE HEGRA C EXPERIMENT AT THE ISLAND LA PALMA. SO THE PARAMETRIZATION OF THE C CERENKOV BUNCH AS CALCULATED IN THIS SUBROUTINE IS VALID FOR C OBSERVATION LEVELS SIMILAR TO THAT OF THE HEGRA EXPERIMENT. C FOR A GIVEN PRIMARY PARTICLE, INCIDENT ENERGY AND ANGLE, AN C OPTIMAL BUNCH SIZE IS CALCULATED BY INTERPOLATION IN A TABLE, C WHERE WE HAVE CHOSEN AN ENERGY RANGE UP TO 1000 TEV, INCIDENT C ANGLES 0 AND 40 DEGREES, AND 4 TYPES OF PRIMARIS: GAMMAS, C PROTONS, NITROGEN, AND IRON. C THIS SUBROUTINE IS CALLED FROM MAIN C ARGUMENTS: C IPARTI = TYPE OF PRIMARY PARTICLE C ENERGY (R4) = PARTICLES ENERGY IN GEV C THETA (R4) = ANGLE IN RAD C CERSZE (R4) = SIZE OF CERENKOV BUNCH C C AUTHORS : S. MARTINEZ UNIVERSITY OF MADRID C F. ARQUEROS UNIVERSITY OF MADRID C----------------------------------------------------------------------- IMPLICIT NONE *KEEP,CONST. COMMON /CONST/ PI,PI2,OB3,TB3,ENEPER DOUBLE PRECISION PI,PI2,OB3,TB3,ENEPER *KEEP,RUNPAR. COMMON /RUNPAR/ FIXHEI,THICK0,HILOECM,HILOELB, * STEPFC,NRRUN,NSHOW,PATAPE,MONIIN, * MONIOU,MDEBUG,NUCNUC, * CETAPE, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE, * DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG COMMON /RUNPAC/ DSN,HOST,USER DOUBLE PRECISION FIXHEI,THICK0,HILOECM,HILOELB REAL STEPFC INTEGER NRRUN,NSHOW,PATAPE,MONIIN,MONIOU,MDEBUG,NUCNUC, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE INTEGER CETAPE CHARACTER*79 DSN CHARACTER*20 HOST,USER LOGICAL DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG *KEND. REAL ANGLE(2),ENGAM(3),ENHAD(3),ENNIT(2), * SIFE(3,2),SIGAM(3,2),SINIT(2),SIPRO(3,2) REAL CERS1F,CERS1P,ENERGY,CERSZE,S1,S2,THETA INTEGER I,IANFE,IANP,IATNUM,IPARTI,I1,I2 DATA ANGLE / 0., 40. / DATA ENGAM / 100., 200., 500. / DATA ENHAD / 100., 200., 1000. / DATA ENNIT / 200., 1000. / DATA ( SIFE (I,1),I=1,3 ) / 30., 30., 140. / DATA ( SIFE (I,2),I=1,3 ) / 30., 30., 110. / DATA ( SIGAM(I,1),I=1,3 ) / 30., 45., 100. / DATA ( SIGAM(I,2),I=1,3 ) / 30., 40., 100. / DATA SINIT / 30., 150. / DATA ( SIPRO(I,1),I=1,3 ) / 30., 30., 120. / DATA ( SIPRO(I,2),I=1,3 ) / 30., 30., 160. / DATA IANP / 1 /, IANFE / 26 / C----------------------------------------------------------------------- c IF ( DEBUG ) WRITE(MDEBUG,100) IPARTI,SNGL(ENERGY),SNGL(THETA) c 100 FORMAT(' GETBUS: INPUT PARTICLE = ',I5,1P,2E10.3) C DEFAULT VALUE CERSZE = 100. ENERGY = ENERGY / 1000. IF ( ENERGY .LE. 100. ) THEN CERSZE = 30. IF ( DEBUG ) WRITE(MDEBUG,101) CERSZE RETURN ENDIF THETA = THETA / PI * 180. C----------------------------------------------------------------------- C PHOTON, ELECTRON OR POSITRON AS PRIMARY PARTICLE IF ( IPARTI .LE. 3 ) THEN C FIND ENERGY BIN FOR INTERPOLATION IF ( ENERGY .LE. ENGAM(2) ) THEN I1 = 1 I2 = 2 ELSE I1 = 2 I2 = 3 ENDIF S1 = SIGAM(I1,1) + (ENERGY - ENGAM(I1)) * / (ENGAM(I2) - ENGAM(I1)) * * (SIGAM(I2,1) - SIGAM(I1,1)) S2 = SIGAM(I1,2) + (ENERGY - ENGAM(I1)) * / (ENGAM(I2) - ENGAM(I1)) * * (SIGAM(I2,2) - SIGAM(I1,2)) CERSZE = S1 + (THETA-ANGLE(1))/(ANGLE(2)-ANGLE(1)) * (S2-S1) IF ( DEBUG ) WRITE(MDEBUG,101) CERSZE RETURN ENDIF C----------------------------------------------------------------------- C NITROGEN AS PRIMARY PARTICLE AND VERTICAL INCIDENCE CJOK WHY SPECIAL TREATMENT FOR NITROGEN ???? CJOK WHY ONLY VERTICAL INCIDENCE ???? IF ( IPARTI .EQ. 1407 .AND. ABS(THETA) .LT. 1.E-1 ) THEN IF ( ENERGY .LT. 200. ) THEN CERSZE = 30. ELSE CERSZE = SINIT(1) + (ENERGY-ENNIT(1)) * / (ENNIT(2)-ENNIT(1)) * (SINIT(2)-SINIT(1)) ENDIF IF ( DEBUG ) WRITE(MDEBUG,101) CERSZE RETURN ENDIF C----------------------------------------------------------------------- C GET THE ATOMIC NUMBER OF THE NUCLEUS C Z IS 1, IF PROTON IF ( IPARTI .EQ. 14 ) THEN IATNUM = 1 C REST OF POSSIBLE NUCLEI ELSEIF ( IPARTI .GT. 100 ) THEN IATNUM = MOD(IPARTI,100) IF ( IATNUM .GT. 26 ) THEN WRITE(MONIOU,*) 'GETBUS: UNEXPECTED PARTICLE CODE' RETURN ENDIF ELSE WRITE(MONIOU,*) 'GETBUS: UNEXPECTED PARTICLE CODE' RETURN ENDIF C FIND ENERGY BIN FOR INTERPOLATION IN CASE OF HADRONIC PRIMARY IF ( ENERGY .LE. ENHAD(2) ) THEN I1 = 1 I2 = 2 ELSE I1 = 2 I2 = 3 ENDIF C INTERPOLATION FOR HADRONS S1 = SIPRO(I1,1) + (ENERGY-ENHAD(I1)) * / (ENHAD(I2)-ENHAD(I1)) * (SIPRO(I2,1)-SIPRO(I1,1)) S2 = SIPRO(I1,2) + (ENERGY-ENHAD(I1)) * / (ENHAD(I2)-ENHAD(I1)) * (SIPRO(I2,2)-SIPRO(I1,2)) CERS1P = S1 + (THETA-ANGLE(1)) / (ANGLE(2)-ANGLE(1)) * (S2-S1) S1 = SIFE(I1,1) + (ENERGY-ENHAD(I1)) / (ENHAD(I2)-ENHAD(I1)) * * (SIFE(I2,1)-SIFE(I1,1)) S2 = SIFE(I1,2) + (ENERGY-ENHAD(I1)) / (ENHAD(I2)-ENHAD(I1)) * * (SIFE(I2,2)-SIFE(I1,2)) CERS1F = S1 + (THETA-ANGLE(1)) / (ANGLE(2)-ANGLE(1)) * (S2-S1) CERSZE = CERS1P + (IATNUM-IANP) * (CERS1F-CERS1P) / (IANFE-IANP) IF ( DEBUG ) WRITE(MDEBUG,101) CERSZE 101 FORMAT(' GETBUS: BUNCH SIZE = ',1P,1E10.3) RETURN END C======================================================================= SUBROUTINE OUTND2 C----------------------------------------------------------------------- C OUT(PUT AT E)ND (OF SHOWER) C C WRITE REST OF PARTICLES TO OUTPUT BUFFER C OUTND2 IS CALLED FROM MAIN C C AUTHORS : S. MARTINEZ, UNIVERSITY OF MADRID C F. ARQUEROS, UNIVERSITY OF MADRID C----------------------------------------------------------------------- IMPLICIT NONE *KEEP,RUNPAR. COMMON /RUNPAR/ FIXHEI,THICK0,HILOECM,HILOELB, * STEPFC,NRRUN,NSHOW,PATAPE,MONIIN, * MONIOU,MDEBUG,NUCNUC, * CETAPE, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE, * DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG COMMON /RUNPAC/ DSN,HOST,USER DOUBLE PRECISION FIXHEI,THICK0,HILOECM,HILOELB REAL STEPFC INTEGER NRRUN,NSHOW,PATAPE,MONIIN,MONIOU,MDEBUG,NUCNUC, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE INTEGER CETAPE CHARACTER*79 DSN CHARACTER*20 HOST,USER LOGICAL DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG *KEEP,CEREN2. COMMON /CEREN2/ PHOTCM,XCER,YCER,UEMIS,VEMIS,CARTIM,ZEMIS, * DCERX,DCERY,ACERX,ACERY, * XCMAX,YCMAX,EPSX,EPSY, * DCERXI,DCERYI,FCERX,FCERY, * XSCATT,YSCATT,CERXOS,CERYOS, * NCERX,NCERY,ICERML REAL PHOTCM,XCER,YCER,UEMIS,VEMIS,CARTIM,ZEMIS, * DCERX,DCERY,ACERX,ACERY, * XCMAX,YCMAX,EPSX,EPSY, * DCERXI,DCERYI,FCERX,FCERY, * XSCATT,YSCATT,CERXOS(20),CERYOS(20) INTEGER NCERX,NCERY,ICERML *KEEP,CEREN3. COMMON /CEREN3/ CERCNT,DATAB2,LHCER INTEGER MAXBF2 PARAMETER (MAXBF2 = 39 * 7) DOUBLE PRECISION CERCNT REAL DATAB2(MAXBF2) INTEGER LHCER *KEND. INTEGER I C----------------------------------------------------------------------- IF ( LHCER .GT. 0 ) THEN CALL TOBUFC( DATAB2,1 ) DO 2 I = 1,MAXBF2 DATAB2(I) = 0. 2 CONTINUE ELSE CALL TOBUFC( DATAB2,2 ) ENDIF WRITE(MONIOU,*) 'CERCNT = ',SNGL( CERCNT ) CERCNT = 0.D0 LHCER = 0 RETURN END C======================================================================= SUBROUTINE OUTPT2(J,IMOV) C----------------------------------------------------------------------- C (WRITE CERENKOV RADIATION) OUTP(U)T C C OUTPUT ROUTINE FOR CERENKOV PHOTONS C THIS SUBROUTINE IS CALLED FROM CERENE AND CERENH C C AUTHORS : S. MARTINEZ, UNIVERSITY OF MADRID C F. ARQUEROS, UNIVERSITY OF MADRID C----------------------------------------------------------------------- IMPLICIT NONE *KEEP,BUFFS. COMMON /BUFFS/ RUNH,RUNE,EVTH,EVTE,DATAB,LH INTEGER MAXBUF,MAXLEN PARAMETER (MAXBUF=39*7) PARAMETER (MAXLEN=12) REAL RUNH(MAXBUF),EVTH(MAXBUF),EVTE(MAXBUF), * RUNE(MAXBUF),DATAB(MAXBUF) INTEGER LH CHARACTER*4 CRUNH,CRUNE,CEVTH,CEVTE EQUIVALENCE (RUNH(1),CRUNH), (RUNE(1),CRUNE) EQUIVALENCE (EVTH(1),CEVTH), (EVTE(1),CEVTE) *KEEP,RUNPAR. COMMON /RUNPAR/ FIXHEI,THICK0,HILOECM,HILOELB, * STEPFC,NRRUN,NSHOW,PATAPE,MONIIN, * MONIOU,MDEBUG,NUCNUC, * CETAPE, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE, * DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG COMMON /RUNPAC/ DSN,HOST,USER DOUBLE PRECISION FIXHEI,THICK0,HILOECM,HILOELB REAL STEPFC INTEGER NRRUN,NSHOW,PATAPE,MONIIN,MONIOU,MDEBUG,NUCNUC, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE INTEGER CETAPE CHARACTER*79 DSN CHARACTER*20 HOST,USER LOGICAL DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG *KEEP,CEREN1. COMMON /CEREN1/ CERELE,CERHAD,ETADSN,WAVLGL,WAVLGU,CYIELD, * CERSIZ,LCERFI DOUBLE PRECISION CERELE,CERHAD,ETADSN,WAVLGL,WAVLGU,CYIELD REAL CERSIZ LOGICAL LCERFI *KEEP,CEREN2. COMMON /CEREN2/ PHOTCM,XCER,YCER,UEMIS,VEMIS,CARTIM,ZEMIS, * DCERX,DCERY,ACERX,ACERY, * XCMAX,YCMAX,EPSX,EPSY, * DCERXI,DCERYI,FCERX,FCERY, * XSCATT,YSCATT,CERXOS,CERYOS, * NCERX,NCERY,ICERML REAL PHOTCM,XCER,YCER,UEMIS,VEMIS,CARTIM,ZEMIS, * DCERX,DCERY,ACERX,ACERY, * XCMAX,YCMAX,EPSX,EPSY, * DCERXI,DCERYI,FCERX,FCERY, * XSCATT,YSCATT,CERXOS(20),CERYOS(20) INTEGER NCERX,NCERY,ICERML *KEEP,CEREN3. COMMON /CEREN3/ CERCNT,DATAB2,LHCER INTEGER MAXBF2 PARAMETER (MAXBF2 = 39 * 7) DOUBLE PRECISION CERCNT REAL DATAB2(MAXBF2) INTEGER LHCER c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> COMMON /GRAAL1/ WAVELENGTH ! (NM) REAL WAVELENGTH c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> *KEND. INTEGER I,J,IMOV C----------------------------------------------------------------------- IF(DEBUG)WRITE(MDEBUG,3)PHOTCM,XCER,YCER,UEMIS,VEMIS,CARTIM,ZEMIS 3 FORMAT(' OUTPT2: ',1P,8E10.3) C WRITE A BLOCK OF 39 PARTICLES TO THE CERENKOV OUTPUT BUFFER AND C CLEAR FIELD IF ( LCERFI ) THEN c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c DATAB2(LHCER+1) = PHOTCM cc DATAB2(LHCER+1) = WAVELENGTH + J*1000. DATAB2(LHCER+1) = J*100000. + IMOV*1000. + WAVELENGTH c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> DATAB2(LHCER+2) = XCER DATAB2(LHCER+3) = YCER DATAB2(LHCER+4) = UEMIS DATAB2(LHCER+5) = VEMIS DATAB2(LHCER+6) = CARTIM DATAB2(LHCER+7) = ZEMIS c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c CERCNT = CERCNT + DBLE( PHOTCM ) CERCNT = CERCNT + 1 c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> LHCER = LHCER + 7 IF ( LHCER .GE. MAXBF2 ) THEN CALL TOBUFC( DATAB2,0 ) DO 1 I = 1,MAXBF2 DATAB2(I) = 0. 1 CONTINUE LHCER = 0 ENDIF ELSE C WRITE A BLOCK OF 39 PARTICLES TO THE PARTICLE OUTPUT BUFFER AND C CLEAR FIELD DATAB(LH+1) = 99.E5 + NINT(PHOTCM)*10. + 1. DATAB(LH+2) = XCER DATAB(LH+3) = YCER DATAB(LH+4) = UEMIS DATAB(LH+5) = VEMIS DATAB(LH+6) = CARTIM DATAB(LH+7) = ZEMIS LH = LH + 7 NOPART = NOPART + 1 c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c CERCNT = CERCNT + DBLE( PHOTCM ) CERCNT = CERCNT + 1 c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> IF ( LH .GE. MAXBUF ) THEN CALL TOBUF( DATAB,0 ) DO 2 I = 1,MAXBUF DATAB(I) = 0. 2 CONTINUE LH = 0 ENDIF ENDIF RETURN END C======================================================================= SUBROUTINE TOBUFC( A,IFL ) C----------------------------------------------------------------------- C (WRITE) TO BUF(FER) C(ERENKOV DATA) C C COPY TO BUFFER CERENKOV DATA C THIS SUBROUTINE IS CALLED FROM MAIN, INPRM, ELECTR, PHOTON, OUTND2, C AND OUTPT2 C ARGUMENTS: C A = ARRAY TO BE WRITTEN TO TAPE C IFL = STARTING OF FINAL OUTPUT C = 0 NORMAL BLOCK C = 1 NORMAL BLOCK WITH END OF OUTPUT C = 2 ONLY END OF OUTPUT C----------------------------------------------------------------------- IMPLICIT NONE *KEEP,BUFFS. COMMON /BUFFS/ RUNH,RUNE,EVTH,EVTE,DATAB,LH INTEGER MAXBUF,MAXLEN PARAMETER (MAXBUF=39*7) PARAMETER (MAXLEN=12) REAL RUNH(MAXBUF),EVTH(MAXBUF),EVTE(MAXBUF), * RUNE(MAXBUF),DATAB(MAXBUF) INTEGER LH CHARACTER*4 CRUNH,CRUNE,CEVTH,CEVTE EQUIVALENCE (RUNH(1),CRUNH), (RUNE(1),CRUNE) EQUIVALENCE (EVTH(1),CEVTH), (EVTE(1),CEVTE) *KEEP,RECORD. COMMON /RECORD/ IRECOR INTEGER IRECOR *KEEP,RUNPAR. COMMON /RUNPAR/ FIXHEI,THICK0,HILOECM,HILOELB, * STEPFC,NRRUN,NSHOW,PATAPE,MONIIN, * MONIOU,MDEBUG,NUCNUC, * CETAPE, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE, * DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG COMMON /RUNPAC/ DSN,HOST,USER DOUBLE PRECISION FIXHEI,THICK0,HILOECM,HILOELB REAL STEPFC INTEGER NRRUN,NSHOW,PATAPE,MONIIN,MONIOU,MDEBUG,NUCNUC, * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL, * N1STTR,MDBASE INTEGER CETAPE CHARACTER*79 DSN CHARACTER*20 HOST,USER LOGICAL DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR, * FIX1I,FMUADD,FNKG,FPRINT,FDBASE * ,GHEISH,GHESIG *KEEP,CEREN3. COMMON /CEREN3/ CERCNT,DATAB2,LHCER INTEGER MAXBF2 PARAMETER (MAXBF2 = 39 * 7) DOUBLE PRECISION CERCNT REAL DATAB2(MAXBF2) INTEGER LHCER *KEEP,CEREN4. COMMON /CEREN4/ NRECER INTEGER NRECER *KEND. INTEGER NSUBBL PARAMETER (NSUBBL=21) REAL A(*) C NSUBBL IS NUMBER OF SUBBLOCKS IN ONE OUTPUT RECORD C (OUTPUT RECORD LENGTH = NSUBBL * 39 * 7 * 4 BYTES <= 22932 ) C IBLK2 IS COUNTER FOR SUBBLOCKS OF CERENKOV OUTPUT C OUTPUT BUFFER FOR CERENKOV OUTPUT REAL OUTBF2(MAXBF2,NSUBBL) SAVE OUTBF2 INTEGER I,IBLK2,IFL,K DATA IBLK2 / 0 / C----------------------------------------------------------------------- IF ( IFL .LE. 1 ) THEN IBLK2 = IBLK2 + 1 DO 3 I = 1,MAXBF2 OUTBF2(I,IBLK2) = A(I) 3 CONTINUE ENDIF C WRITE TO TAPE IF BLOCK IS FULL OR IF IFL IS 1 IF ( IFL .GE. 1 .OR. IBLK2 .EQ. NSUBBL ) THEN NRECER = NRECER + 1 c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> c WRITE(CETAPE) ((OUTBF2(I,K),I=1,MAXBF2),K=1,NSUBBL) call jccersave(outbf2) c>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>> IBLK2 = 0 DO 4 K = 1,NSUBBL DO 4 I = 1,MAXBF2 OUTBF2(I,K) = 0.0 4 CONTINUE ENDIF RETURN END