/[PAMELA software]/gpamela/history/v_100.txt
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revision 3.12 by pam-ba, Thu May 18 10:52:32 2006 UTC revision 3.13 by pamela, Mon Jun 5 13:56:17 2006 UTC
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1  #  #
2  # $Id: v_100.txt,v 3.11 2006/05/11 23:53:15 cafagna Exp $  # $Id: v_100.txt,v 3.12 2006/05/18 10:52:32 pam-ba Exp $
3  #  #
4  # $Log: v_100.txt,v $  # $Log: v_100.txt,v $
5    # Revision 3.12  2006/05/18 10:52:32  pam-ba
6    # TOF geometry completed and a new material, the polystyrene (density 35 g/l), added
7    #
8  # Revision 3.11  2006/05/11 23:53:15  cafagna  # Revision 3.11  2006/05/11 23:53:15  cafagna
9  # More bugs fixed in the CALO ntple structure filling  # More bugs fixed in the CALO ntple structure filling
10  #  #
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52  #CMZ :  1.00/01 28/11/95  18.51.23  by  Francesco Cafagna  #CMZ :  1.00/01 28/11/95  18.51.23  by  Francesco Cafagna
53  #-- Author :    Francesco Cafagna   28/11/95  #-- Author :    Francesco Cafagna   28/11/95
54    
55    May 2006, Bari & Tor Vergata
56    
57    GIGANTIC RESONANCE FOR NEUTRON DETECTOR ADDED
58    
59       Routines to simulate the gigantic resonance of gammas in Tungsten
60       have been added.  The GPGIG routine is called in GUSTEP if a gamma
61       enter the calorimeter absorber.  This is the steering routine to
62       simulate the production of neutrons from gigantic resonance.  It
63       does checks on STEP lenght. If the range is smaller than the other
64       selected for that step, it does generate the neutron and stops the
65       gamma. Please note that the neutron has now a new particle
66       number. This is to tag the gigantic resonance neutrons.
67    
68    
69  May 2006, Bari & Florence  May 2006, Bari & Florence
70    
71  CAL HIT STRUCTURE BUGS FIXED  CAL HIT STRUCTURE BUGS FIXED
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