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# $Id: v_100.txt,v 3.11 2006/05/11 23:53:15 cafagna Exp $ |
# $Id: v_100.txt,v 3.15 2006/10/02 11:17:30 pam-ba Exp $ |
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# $Log: v_100.txt,v $ |
# $Log: v_100.txt,v $ |
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# Revision 3.15 2006/10/02 11:17:30 pam-ba |
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# NDET 'SPHE' data card meaning changed. Now it eliminates the whole PAMELA container. |
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# |
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# Revision 3.14 2006/06/30 15:38:16 pam-ba |
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# S22 and S12 heights positioned in GPAMELA at the nominal heights in PAMELA (see document: Main geometrical parameters of the PAMELA sub-detectors, 20 December 2005) |
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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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# |
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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 |
# Revision 3.11 2006/05/11 23:53:15 cafagna |
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# More bugs fixed in the CALO ntple structure filling |
# More bugs fixed in the CALO ntple structure filling |
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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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October 2006, Bari |
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The geometry of the neutron detector has been updated. Some dimensions of some |
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volumes have been corrected while the aluminum cover and the aluminum boxes to |
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put the cables have been added. |
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September 2006, Bari |
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SPHE and ND data card bugs fixed: the definition of the ND data card, |
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missing in the subroutine gpgeo.F, has been added; the meaning of the SPHE |
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data card has been changed. Before the correction the data card: |
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NDET 'SPHE' was used to delete the spherical top shell to substitute it with |
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a flat one.Now NDET 'SPHE' eliminates the whole container of PAMELA. |
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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 |
May 2006, Bari & Florence |
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CAL HIT STRUCTURE BUGS FIXED |
CAL HIT STRUCTURE BUGS FIXED |
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