|
|
|
1 |
# |
# |
2 |
# $Id: v_100.txt,v 3.11 2006/05/11 23:53:15 cafagna Exp $ |
# $Id: v_100.txt,v 3.13 2006/06/05 13:56:17 pamela Exp $ |
3 |
# |
# |
4 |
# $Log: v_100.txt,v $ |
# $Log: v_100.txt,v $ |
5 |
|
# Revision 3.13 2006/06/05 13:56:17 pamela |
6 |
|
# Gigantic resonance added for gamma enetering in the calorimeter absorber |
7 |
|
# |
8 |
|
# Revision 3.12 2006/05/18 10:52:32 pam-ba |
9 |
|
# TOF geometry completed and a new material, the polystyrene (density 35 g/l), added |
10 |
|
# |
11 |
# Revision 3.11 2006/05/11 23:53:15 cafagna |
# Revision 3.11 2006/05/11 23:53:15 cafagna |
12 |
# More bugs fixed in the CALO ntple structure filling |
# More bugs fixed in the CALO ntple structure filling |
13 |
# |
# |
55 |
#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 |
56 |
#-- Author : Francesco Cafagna 28/11/95 |
#-- Author : Francesco Cafagna 28/11/95 |
57 |
|
|
58 |
|
June 2006, Bari |
59 |
|
|
60 |
|
The center of the scintillator planes S22Y (variable ZPAMS22Y in gpdgeo.inc) |
61 |
|
and S12X (variable ZPAMS12X in gpdgeo.inc) has been positioned at the |
62 |
|
nominal height as measured in PAMELA (See the document: "Main geometrical |
63 |
|
parameters of the PAMELA sub-detectors" by O. Adriani, L. Bonechi, |
64 |
|
E. Mocchiutti, S. Ricciarini, 20 December 2005). Follows that the positions |
65 |
|
of S21Y and S12X are higher than those in the cited document due to the fact |
66 |
|
that in GPAMELA the thickness of the mylar has been considered while in the |
67 |
|
document it has been neglected. |
68 |
|
|
69 |
|
|
70 |
|
May 2006, Bari & Tor Vergata |
71 |
|
|
72 |
|
GIGANTIC RESONANCE FOR NEUTRON DETECTOR ADDED |
73 |
|
|
74 |
|
Routines to simulate the gigantic resonance of gammas in Tungsten |
75 |
|
have been added. The GPGIG routine is called in GUSTEP if a gamma |
76 |
|
enter the calorimeter absorber. This is the steering routine to |
77 |
|
simulate the production of neutrons from gigantic resonance. It |
78 |
|
does checks on STEP lenght. If the range is smaller than the other |
79 |
|
selected for that step, it does generate the neutron and stops the |
80 |
|
gamma. Please note that the neutron has now a new particle |
81 |
|
number. This is to tag the gigantic resonance neutrons. |
82 |
|
|
83 |
|
|
84 |
May 2006, Bari & Florence |
May 2006, Bari & Florence |
85 |
|
|
86 |
CAL HIT STRUCTURE BUGS FIXED |
CAL HIT STRUCTURE BUGS FIXED |