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# $Id: v_100.txt,v 3.9 2005/12/14 03:34:40 cafagna Exp $ |
# $Id: v_100.txt,v 3.13 2006/06/05 13:56:17 pamela Exp $ |
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# $Log: v_100.txt,v $ |
# $Log: v_100.txt,v $ |
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# Revision 3.13 2006/06/05 13:56:17 pamela |
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# Gigantic resonance added for gamma enetering in the calorimeter absorber |
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# Revision 3.12 2006/05/18 10:52:32 pam-ba |
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# TOF geometry completed and a new material, the polystyrene (density 35 g/l), added |
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# Revision 3.11 2006/05/11 23:53:15 cafagna |
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# More bugs fixed in the CALO ntple structure filling |
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# Revision 3.10 2006/04/10 11:07:43 cafagna |
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# GEN data card updated, ZDGEN added |
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# Revision 3.9 2005/12/14 03:34:40 cafagna |
# Revision 3.9 2005/12/14 03:34:40 cafagna |
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# An update of the history and inform readme files. |
# An update of the history and inform readme files. |
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#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 |
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#-- Author : Francesco Cafagna 28/11/95 |
#-- Author : Francesco Cafagna 28/11/95 |
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June 2006, Bari |
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The center of the scintillator planes S22Y (variable ZPAMS22Y in gpdgeo.inc) |
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and S12X (variable ZPAMS12X in gpdgeo.inc) has been positioned at the |
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nominal height as measured in PAMELA (See the document: "Main geometrical |
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parameters of the PAMELA sub-detectors" by O. Adriani, L. Bonechi, |
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E. Mocchiutti, S. Ricciarini, 20 December 2005). Follows that the positions |
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of S21Y and S12X are higher than those in the cited document due to the fact |
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that in GPAMELA the thickness of the mylar has been considered while in the |
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document it has been neglected. |
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May 2006, Bari & Tor Vergata |
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GIGANTIC RESONANCE FOR NEUTRON DETECTOR ADDED |
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Routines to simulate the gigantic resonance of gammas in Tungsten |
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have been added. The GPGIG routine is called in GUSTEP if a gamma |
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enter the calorimeter absorber. This is the steering routine to |
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simulate the production of neutrons from gigantic resonance. It |
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does checks on STEP lenght. If the range is smaller than the other |
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selected for that step, it does generate the neutron and stops the |
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gamma. Please note that the neutron has now a new particle |
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number. This is to tag the gigantic resonance neutrons. |
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May 2006, Bari & Florence |
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CAL HIT STRUCTURE BUGS FIXED |
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The maximum number of hit is now different for the two hit |
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structures: CALST and CALI. Vectors inizialization and HBOOK |
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ntple booking have been updated. The GPDCAL routine has been fixed |
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so to handle the case in wich hits stored are more than the maximum |
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number of hit. |
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In this case in the ntple up to the maximum number of hits will be stored. |
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April 2006, Bari |
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TOF GEOMETRY AND POSITIONS UPDATED AND NEW MIXTURES ADDED |
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The TOF geometry has been modified. The following boxes have been |
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added: POL1, POL2 and POLY made of polystyrene, S11M, S12M, S21M, |
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S22M, S31M and S32M made of mylar, S1A, S2A and S3 made of air and |
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S1 and S2 made of aluminum. Each scintillator paddle has been put |
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in his mylar box and the other materials: air, polystyrene, and |
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aluminum have been added at their nominal positions. According to |
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Naples people the araldite glue has been simulated has an air |
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gap. For this work two new materials: the Mylar (MYLAR) and the |
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polystyrene (POLYSTYRENE) with a density of 35 g/l have been |
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defined as a mixture. The positions of the three bottom |
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scintillator planes that contain respectively the S12X, S22Y and |
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S32X paddles have been regulated according on their official |
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positions in PAMELA. |
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Mar 2006, Bari |
Mar 2006, Bari |
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GEN DATA CARD UPDATED |
GEN DATA CARD UPDATED |
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The GCALOR package |
The GCALOR package |
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June 2005, Bari |
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TOF SCINTILLATOR PADDLES UPDATED |
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The dimensions and the number of the scintillator paddles for each |
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TOF planes have been updated. |
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May 2005, Bari |
May 2005, Bari |
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Some updates on the latest modification done in the past year. |
Some updates on the latest modification done in the past year. |
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