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* |
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* $Id: gpdspe.F,v 3.2 2005/07/25 11:53:21 cafagna Exp $ |
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* |
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* $Log: gpdspe.F,v $ |
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* Revision 3.2 2005/07/25 11:53:21 cafagna |
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* Several updates. See history for details |
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* |
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* Revision 3.1.1.1 2002/07/11 16:02:13 cafagna |
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* First GPAMELA release on CVS |
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* |
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* |
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*CMZ : 2.01/00 05/04/2000 14.35.18 by Marialuigia Ambriola |
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*CMZ : 2.00/00 03/03/2000 15.39.06 by Francesco Cafagna |
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*CMZ : 1.02/00 19/01/2000 15.50.14 by Francesco Cafagna |
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*CMZ : 1.01/00 16/05/96 17.38.13 by Francesco Cafagna |
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*CMZ : 1.00/02 27/03/96 18.35.42 by Francesco Cafagna |
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*-- Author : Francesco Cafagna 23/02/96 |
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SUBROUTINE GPDSPE |
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************************************************************************ |
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* * |
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* To perform SPE digitization * |
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* * |
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* Called by: GUDIGI * |
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* Author: Francesco Cafagna, 23/02/96 12.50.38 * |
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* * |
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************************************************************************ |
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#include "gcunit.inc" |
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#include "gpphit.inc" |
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PARAMETER (RADDEG=57.295779) |
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PARAMETER (NH=NHSPE,NHM=NHMSPE,NVOL=3) |
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#include "gppdigi.inc" |
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c +SEQ,GPDSPE. |
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#include "gprhit.inc" |
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#include "gpspe.inc" |
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#include "gpsed.inc" |
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* |
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INTEGER IS,ID,NV,NVM,GPNHIT,NTHIT,NHFRST |
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CHARACTER*4 CSET |
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LOGICAL CONT,HF |
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* |
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* Data block for digitalization |
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* |
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INTEGER NTRA,IDIG,LTRA,NPLANE,LKDN,NTDIGI,JJ |
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INTEGER KDIGI(4),NUMBVD(NVOL) |
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REAL XI,YI,XO,YO,PATH,DE,GPGAUS |
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REAL VPOS(3),BMAGNET(3),ANGLEX,ANGLEY,XMULT,YMULT,DXPOS,DYPOS |
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* |
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DATA NTRA,LTRA/1,1/ |
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* |
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* |
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* Vector zeroed |
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* |
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CALL VZERO(ITRPB ,NHM) |
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CALL VZERO(ITRSL ,NHM) |
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CALL VZERO(ITSPA ,NHM) |
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CALL VZERO(XTSPA,NHM) |
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CALL VZERO(YTSPA,NHM) |
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CALL VZERO(ZTSPA,NHM) |
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CALL VZERO(XOTSPA,NHM) |
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CALL VZERO(YOTSPA,NHM) |
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CALL VZERO(ZOTSPA,NHM) |
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CALL VZERO(ERTSPA,NHM) |
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CALL VZERO(PATSPA,NHM) |
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CALL VZERO(NUMD ,NVOL) |
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CALL VZERO(NDPLAN,NDMSPE) |
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CALL VZERO(NDSIL ,NDMSPE) |
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CALL VZERO(NDISTR,NDMSPE) |
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CALL VZERO(NDIADC,NDMSPE) |
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* |
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CONT = .FALSE. |
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HF = .TRUE. |
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NTDIGI = 0 |
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NDISPE = 0 |
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NV = NVOL |
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NVM= NVMAX |
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IS = ISSPE |
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ID = IDTSPA |
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CSET = 'SPE ' |
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IT = -1 |
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* |
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* Get the total number of hits stored for TSPA detector |
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* |
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NTHIT = GPNHIT(CSET,CNSED(IS,ID) ) |
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IF (NTHIT.GT.NHM) CONT=.TRUE. |
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* |
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* Check on the volume level |
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* |
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IF (NV.GT.NVM) THEN |
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WRITE(CHMAIL,10000) CSET,CNSED(IS,ID),NVOL,NVMAX, |
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+ IDRUN,IDEVT |
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CALL GMAIL(1,0) |
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GO TO 20 |
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ENDIF |
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CALL VZERO(VHITS,NH*NHM) |
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CALL VZERO(ITRA ,NHM) |
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CALL VZERO(NUMBV,NVOL*NHM) |
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NHITS = -1 |
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NHFRST = 1 |
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LKDN = 0 |
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10 CALL GPRHIT(CSET,CNSED(IS,ID),IS,ID,NVOL,NH,NHM,NHFRST, |
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+ IT,NUMD,ITRA,NUMBV,VHITS,NHITS) |
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* |
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* If there was a problem in GPRHIT then exit |
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* |
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IF(NHITS.LT.0.AND.(NHITS.NE.-(NHM+1)) ) THEN |
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WRITE(CHMAIL,10100) CSET,CNSED(IS,ID),NHITS,NHM, |
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+ IDRUN,IDEVT |
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CALL GMAIL(1,0) |
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GO TO 20 |
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ENDIF |
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IF( NHITS.EQ. -(NHM+1) ) NHITS = NHM |
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* |
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* Fill CWN entuple |
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* |
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NTHSPE = NHITS |
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DO I=1,NHITS |
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ITRPB(I) = NUMBV(1,I) |
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ITRSL(I) = NUMBV(2,I) |
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ITSPA(I) = NUMBV(3,I) |
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#if defined(GPAMELA_INTER) |
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XAVSPE(I) = VHITS(1,I) |
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YAVSPE(I) = VHITS(2,I) |
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ZAVSPE(I) = VHITS(3,I) |
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XOUTSPE(I) = VHITS(4,I) |
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YOUTSPE(I) = VHITS(5,I) |
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ZOUTSPE(I) = VHITS(6,I) |
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XINSPE(I) = 2*XAVSPE(I) - XOUTSPE(I) |
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YINSPE(I) = 2*YAVSPE(I) - YOUTSPE(I) |
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ZINSPE(I) = 2*ZAVSPE(I) - ZOUTSPE(I) |
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#endif |
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#if !defined(GPAMELA_INTER) |
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XINSPE(I) = VHITS(1,I) |
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YINSPE(I) = VHITS(2,I) |
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ZINSPE(I) = VHITS(3,I) |
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XOUTSPE(I) = VHITS(4,I) |
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YOUTSPE(I) = VHITS(5,I) |
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ZOUTSPE(I) = VHITS(6,I) |
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XAVSPE(I) = (XINSPE(I)+XOUTSPE(I))/2. |
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YAVSPE(I) = (YINSPE(I)+YOUTSPE(I))/2. |
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ZAVSPE(I) = (ZINSPE(I)+ZOUTSPE(I))/2. |
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#endif |
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ERELSPE(I) = VHITS(7,I) |
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PATHSPE(I) = VHITS(8,I) |
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IPARSPE(I) = VHITS(9,I) |
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P0SPE (I) = VHITS(10,I) |
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C |
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C ADD RESOLUTION SIMULATION TO XAVSPE |
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C |
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ANGLEX=0. |
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ANGLEY=0. |
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IF(ZOUTSPE(I).NE.ZINSPE(I)) THEN |
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ANGLEX=RADDEG*ATAN( ABS(XOUTSPE(I)-XINSPE(I) )/ |
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+ ABS(ZOUTSPE(I)-ZINSPE(I) ) ) |
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ANGLEY=RADDEG*ATAN( ABS(YOUTSPE(I)-YINSPE(I) )/ |
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+ ABS(ZOUTSPE(I)-ZINSPE(I) ) ) |
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ENDIF |
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VPOS(1)=XAVSPE(I) |
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VPOS(2)=YAVSPE(I) |
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VPOS(3)=ZAVSPE(I) |
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CALL GUFLD(VPOS,BMAGNET) |
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|
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CALL GPRSPE(ANGLEX,ANGLEY,BMAGNET,XMULT,YMULT,DXPOS,DYPOS) |
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|
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XAVSPE(I) = XAVSPE(I) + DXPOS |
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YAVSPE(I) = YAVSPE(I) + DYPOS |
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|
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C |
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C ADD RESOLUTION OF THE SHIFT INDUCED BY THE MAG. FIELD |
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C |
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|
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IF(ITRPB(I).LT.6) THEN |
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XAVSPE(I) = XAVSPE(I) - 2.64e-4/4.5*BMAGNET(2) |
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ELSE IF(ITRPB(I).EQ.6) THEN |
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XAVSPE(I) = XAVSPE(I) + 2.64e-4/4.5*BMAGNET(2) |
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ENDIF |
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|
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ENDDO |
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* |
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* Loop on the hits retrived to fill the CWN common and the DIGI bank |
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* |
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C fc IF (HF) NTHSPE = NHITS |
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C fc DO I=1,NHITS |
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C fc * |
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C fc * Start DIGI action |
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C fc * |
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C fc NPLANE=NUMBV(3,I) |
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C fc XI=VHITS(1,I) |
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C fc YI=VHITS(2,I) |
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C fc ZI=VHITS(3,I) |
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C fc XO=VHITS(4,I) |
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C fc YO=VHITS(5,I) |
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C fc ZO=VHITS(6,I) |
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C fc +SELF,IF=INTER |
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C fc * interactive case: we need the track edges |
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C fc XI=2.*XI-XO |
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C fc YI=2.*YI-YO |
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C fc ZI=2.*ZI-ZO |
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C fc +SELF. |
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C fc PATH=VHITS(8,I) |
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C fc DE=VHITS(7,I) |
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C fc IF(DE.GT.0.) THEN |
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C fc DO J=1,6 |
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C fc NUMBVD(J)=NUMBV(J,I) |
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C fc ENDDO |
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C fc c+SELF,IF=PAOLO |
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C fc c CALL GPSPEHD(I,NPLANE,XI,YI,ZI,XO,YO,ZO,PATH,DE,LKDN) |
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C fc c+SELF |
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C fc c+SELF,IF=-PAOLO |
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C fc c CALL GPSPEHD(I,NUMBVD,NVSPE,XI,YI,ZI,XO,YO,ZO,PATH,DE,LKDN) |
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C fc c+SELF. |
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C fc NTDIGI = LKDN |
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C fc ENDIF |
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C fc * |
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C fc * Fill CWN common |
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C fc * |
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C fc IF(HF) THEN |
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C fc ITRPB(I) = NUMBV((NVSPE-3),I) |
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C fc ITRSL(I) = NUMBV((NVSPE-1),I) |
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C fc ITSPA(I) = NUMBV(NVSPE,I) |
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C fc XTSPA(I) = VHITS(1,I) |
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C fc YTSPA(I) = VHITS(2,I) |
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C fc ZTSPA(I) = VHITS(3,I) |
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C fc XOTSPA(I) = VHITS(4,I) |
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C fc YOTSPA(I) = VHITS(5,I) |
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C fc ZOTSPA(I) = VHITS(6,I) |
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C fc ERTSPA(I) = VHITS(7,I) |
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C fc PATSPA(I) = VHITS(8,I) |
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C fc ENDIF |
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C fc IF(CONT) HF = .FALSE. |
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C fc ENDDO |
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C fc IF(CONT) THEN |
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C fc NHFRST = NHFRST + NHM |
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C fc IF( (NTHIT-NHFRST).LE.NHM) CONT=.FALSE. |
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C fc GO TO 10 |
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C fc ENDIF |
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C fc * |
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C fc * fill digits with noise included |
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C fc * |
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C fc IF(LKDN.GE.1) THEN |
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C fc DO II=1,LKDN |
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C fc * plane=0 if the signal is lesser than 1 ADC |
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C fc IF(INT(RLKD4(II)*ADCX).LE.0.AND.LKD2(II).GE.1. |
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C fc + AND.LKD2(II).LE.3) LKD1(II)=0 |
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C fc IF(INT(RLKD4(II)*ADCY).LE.0.AND.LKD2(II).GE.4. |
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C fc + AND.LKD2(II).LE.5) LKD1(II)=0 |
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C fc * |
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C fc JJ=LKDH(II)+(NHFRST-1) |
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C fc * KDIGI(1)=LKD1(II) |
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C fc * KDIGI(2)=LKD2(II) |
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C fc KDIGI(1)=LKD2(II) |
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C fc KDIGI(2)=LKD3(II) |
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C fc * R1=RAN(IR) |
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C fc * R2=RAN(IR) |
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C fc * GRNDM0=SIN(2.*3.14159*R1)*SQRT(-2.*LOG(R2)) |
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C fc GRNDM0 = GPGAUS(0.) |
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C fc IF(LKD2(II).GE.1.AND.LKD2(II).LE.3) THEN |
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C fc RLKD4(II)=RLKD4(II)+GRNDM0*ENOISX+PIEDX |
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C fc KDIGI(3)=INT(RLKD4(II)*ADCX) |
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C fc ENDIF |
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C fc IF(LKD2(II).GE.4.AND.LKD2(II).LE.5) THEN |
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C fc RLKD4(II)=RLKD4(II)+GRNDM0*ENOISY+PIEDY |
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C fc KDIGI(3)=INT(RLKD4(II)*ADCY) |
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C fc ENDIF |
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C fc C+SELF,IF=PAOLO |
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C fc DO J=1,NVOL |
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C fc NUMBVD(J)=NUMBV(J,JJ) |
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C fc ENDDO |
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C fc C+SELF |
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C fc LTRA=ITRA(JJ) |
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C fc IF(KDIGI(3).LT.0) KDIGI(3)=0 |
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C fc IF(KDIGI(3).GE.1024) KDIGI(3)=1023 |
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C fc IF(KDIGI(3).GT.0.AND.LKD1(II).GT.0) THEN |
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C fc CALL GSDIGI(IS,ID,LTRA,NTRA,NUMBVD,KDIGI,IDIG) |
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C fc IF (IDIG.EQ.0) THEN |
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C fc WRITE(CHMAIL,10200) CSET,CNSED(IS,ID),NVOL,KDIGI |
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C fc CALL GMAIL(1,0) |
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C fc GO TO 20 |
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C fc ENDIF |
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C fc ENDIF |
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C fc * |
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C fc * Fills CWN |
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C fc * |
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C fc IF(HF) THEN |
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C fc IF(LKD2(II).GE.1.AND.LKD2(II).LE.3) KDIGIT=INT(RLKD4(II)* |
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C fc + ADCX) |
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C fc IF(LKD2(II).GE.4.AND.LKD2(II).LE.5) KDIGIT=INT(RLKD4(II)* |
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C fc + ADCY) |
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C fc IF(KDIGIT.GT.0.AND.LKD1(II).GT.0) THEN |
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C fc NDISPE=NDISPE+1 |
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C fc IF (NDISPE.LE.NDMSPE) THEN |
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C fc NDPLAN(NDISPE)=LKD1(II) |
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C fc NDSIL (NDISPE)=LKD2(II) |
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C fc NDISTR(NDISPE)=LKD3(II) |
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C fc IF(KDIGIT.LT.1024) THEN |
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C fc NDIADC(NDISPE)=KDIGIT |
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C fc ELSE |
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C fc NDIADC(NDISPE)=1023 |
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C fc ENDIF |
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C fc ENDIF |
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C fc ENDIF |
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C fc ENDIF |
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C fc ENDDO |
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C fc ENDIF |
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* |
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10000 FORMAT(' GPDSPE: VOLUME level too big: SET=',A4,', DET=',A4,', |
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+ NVOL=',I3,', NVMAX=',I3,', RUN=',I5,', EVT=',I8) |
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10100 FORMAT(' GPDSPE: Error in GPRHIT: SET=',A4, |
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+ ', DET=',A4,',NHITS=',I5,', NHMAX=',I5, |
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+ ', RUN=',I5,', EVT=',I8) |
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10200 FORMAT(' GPDSPE: digitization ERROR: SET=',A4,', DET=',A4,', |
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+ NVOL=',I3,', KDIGI=',4I4) |
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20 RETURN |
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END |
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