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cafagna |
3.1 |
* |
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cafagna |
3.5 |
* $Id: gpdcal.F,v 3.4 2005/07/25 11:53:20 cafagna Exp $ |
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pamela |
3.2 |
* |
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* $Log: gpdcal.F,v $ |
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cafagna |
3.5 |
* Revision 3.4 2005/07/25 11:53:20 cafagna |
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* Several updates. See history for details |
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* |
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3.4 |
* Revision 3.3 2005/06/21 02:42:03 cafagna |
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* Major modification to the geometry and to the random number chain |
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* |
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cafagna |
3.3 |
* Revision 3.2 2003/12/17 11:32:48 pamela |
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* CALO SIMULATION COMPLETED: geometry and special tracking parameters updated and simulation checked by a comparison with the Trieste's standalone Monte Carlo simulation |
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* |
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pamela |
3.2 |
* Revision 3.1.1.1 2002/07/11 16:02:14 cafagna |
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* First GPAMELA release on CVS |
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cafagna |
3.1 |
* |
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* |
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*CMZ : 2.03/00 31/10/2000 11.18.51 by Francesco Cafagna |
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*CMZ : 2.02/00 10/10/2000 14.09.00 by Francesco Cafagna |
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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 29/02/2000 17.39.10 by Francesco Cafagna |
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*CMZ : 1.02/00 10/02/2000 17.28.08 by Francesco Cafagna |
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*CMZ : 1.01/00 21/05/96 17.33.38 by Francesco Cafagna |
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*CMZ : 1.00/02 05/04/96 11.26.03 by Francesco Cafagna |
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*-- Author : Francesco Cafagna 23/02/96 |
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SUBROUTINE GPDCAL |
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************************************************************************ |
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* * |
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* To perform CAL 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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cafagna |
3.5 |
#include "gcflag.inc" |
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cafagna |
3.1 |
#include "gpphit.inc" |
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cafagna |
3.5 |
PARAMETER (NH1=NHCALI,NHM1=NHMCALI,NVOL1=2) |
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PARAMETER (NH=NHCAL,NHM=NHMCAL,NVOL=3) |
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cafagna |
3.1 |
#include "gprhit.inc" |
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#include "gpcal.inc" |
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#include "gpsed.inc" |
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#include "gpkey.inc" |
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#include "gpgeo.inc" |
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pamela |
3.2 |
*ml:21/02/02 |
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#include "gpencal.inc" |
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*end ml. |
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cafagna |
3.1 |
* |
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INTEGER IS,ID,NV,NVM,NNHM |
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CHARACTER*4 CSET |
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cafagna |
3.5 |
INTEGER ITRA1(NHM1),NUMD1(NVOL1),NUMBV1(NVOL1,NHM1) |
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REAL VHITS1(NH1,NHM1) |
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cafagna |
3.1 |
* |
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* Vector zeroed |
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* |
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CALL VZERO(ICAPL ,NHMCAL) |
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CALL VZERO(ICASI ,NHMCAL) |
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CALL VZERO(ICAST ,NHMCAL) |
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CALL VZERO(XCASI,NHMCAL) |
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CALL VZERO(YCASI,NHMCAL) |
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CALL VZERO(ZCASI,NHMCAL) |
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CALL VZERO(IPARCAL,NHMCAL) |
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CALL VZERO(ERCASI,NHMCAL) |
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CALL VZERO(NUMD ,NVOL) |
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CALL VZERO(NUMD1 ,NVOL1) |
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pamela |
3.2 |
c ml:16/4/2003 |
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cafagna |
3.5 |
CALL VZERO(ICASTRIP,NHMCALI) |
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CALL VZERO(ICAPLANE,NHMCALI) |
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CALL VZERO(ICAMOD,NHMCALI) |
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CALL VZERO(ENESTRIP,NHMCALI) |
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pamela |
3.2 |
c end 16/4/2003 |
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cafagna |
3.1 |
* |
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* |
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* The tungsten plane case |
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* |
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cafagna |
3.5 |
NV = NVOL |
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NVM= NVMAX |
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cafagna |
3.1 |
IS = ISCAL |
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cafagna |
3.3 |
ID = IDCAST |
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cafagna |
3.1 |
IT = -1 |
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CSET = 'CAL ' |
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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 10 |
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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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NHITS = -1 |
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* |
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* Update the max number of hits to be retrived |
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* |
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NNHM = NHM |
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cafagna |
3.5 |
c$$$ IF(NNHM.LE.0) THEN |
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c$$$ WRITE(CHMAIL,10100) CSET,CNSED(IS,ID),NTHCAL,NHM, |
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c$$$ + IDRUN,IDEVT |
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c$$$ CALL GMAIL(1,0) |
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c$$$ GO TO 10 |
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c$$$ ENDIF |
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cafagna |
3.1 |
CALL VZERO(NUMBV,NVOL*NHM) |
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CALL GPRHIT(CSET,CNSED(IS,ID),IS,ID,NVOL,NH,NNHM,1, |
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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) THEN |
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WRITE(CHMAIL,10200) 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 10 |
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ENDIF |
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* |
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* >>>>>>>>>>>>>>>>>>>>>> DIGI action |
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* |
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* |
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* Fill the CWN common |
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* |
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pamela |
3.2 |
NTHCAL=0 |
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cafagna |
3.1 |
DO I=1,NHITS |
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cafagna |
3.3 |
NTHCAL = NTHCAL + 1 |
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ICAPL(NTHCAL) = NUMBV((NVCAL-2),I) |
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ICASI(NTHCAL) = NUMBV((NVCAL-1),I) |
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ICAST(NTHCAL) = NUMBV((NVCAL),I) |
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XINCAL(NTHCAL) = VHITS(1,I) |
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YINCAL(NTHCAL) = VHITS(2,I) |
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ZINCAL(NTHCAL) = VHITS(3,I) |
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ERELCAL(NTHCAL) = VHITS(4,I) |
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cafagna |
3.1 |
c IPARCAL(NTHCAL) = VHITS(5,I) |
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c P0CAL(NTHCAL) = VHITS(6,I) |
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cafagna |
3.3 |
ENDDO |
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C |
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C The energy released per strip |
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C |
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NV = NVOL1 |
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NVM= NVMAX |
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* |
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* The tungsten plane case |
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* |
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IS = ISCAL |
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ID = IDCASI |
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IT = -1 |
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CSET = 'CAL ' |
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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 10 |
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ENDIF |
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cafagna |
3.5 |
CALL VZERO(VHITS1,NH1*NHM1) |
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CALL VZERO(ITRA1 ,NHM1) |
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cafagna |
3.3 |
NHITS = -1 |
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* |
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* Update the max number of hits to be retrived |
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* |
162 |
cafagna |
3.5 |
NNHM = NHM1 |
163 |
cafagna |
3.3 |
IF(NNHM.LE.0) THEN |
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WRITE(CHMAIL,10100) CSET,CNSED(IS,ID),NTHCALI,NHM, |
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+ IDRUN,IDEVT |
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CALL GMAIL(1,0) |
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GO TO 10 |
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ENDIF |
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cafagna |
3.5 |
CALL VZERO(NUMBV1,NVOL1*NHM1) |
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CALL GPRHIT(CSET,CNSED(IS,ID),IS,ID,NVOL1,NH1,NNHM,1, |
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+ IT,NUMD1,ITRA1,NUMBV1,VHITS1,NHITS) |
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cafagna |
3.3 |
* |
173 |
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* If there was a problem in GPRHIT then exit |
174 |
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* |
175 |
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IF(NHITS.LT.0) THEN |
176 |
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WRITE(CHMAIL,10200) 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 10 |
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ENDIF |
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* |
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* >>>>>>>>>>>>>>>>>>>>>> DIGI action |
183 |
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* |
184 |
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* |
185 |
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* Fill the CWN common |
186 |
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* |
187 |
pamela |
3.2 |
c |
188 |
cafagna |
3.4 |
NTHCALI=0 |
189 |
cafagna |
3.3 |
DO I=1,NHITS |
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NTHCALI=NTHCALI+1 |
191 |
cafagna |
3.5 |
ICASTRIP(NTHCALI)=NUMBV1(NVCALI,I) |
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ICAPLANE(NTHCALI)=NUMBV1((NVCALI-1),I) |
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ICAMOD(NTHCALI)=VHITS1(1,I) |
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ENESTRIP(NTHCALI)=VHITS1(2,I) |
195 |
cafagna |
3.3 |
ENDDO |
196 |
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c |
197 |
pamela |
3.2 |
10000 FORMAT(' GPDCAL: VOLUME level too big: SET=',A4,', DET=',A4,', |
198 |
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+ NVOL=',I3,', NVMAX=',I3,', RUN=',I5,', EVT=',I8) |
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10100 FORMAT(' GPDCAL: MAX number of hits retrived: SET=',A4, |
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+ ', DET=',A4,',NHREAD=',I5,', NHMAX=',I5, |
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+ ', RUN=',I5,', EVT=',I8) |
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10200 FORMAT(' GPDCAL: 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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10 RETURN |
206 |
cafagna |
3.1 |
END |