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# Revision 3.21 2006/12/05 18:45:29 bruno |
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# Update of the CARD geometry |
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# Simulated also legs, table and magnetic screen |
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# |
# |
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# $Id: v_100.txt,v 3.22 2006/11/28 11:43:41 pam-ba Exp $ |
# $Id: v_100.txt,v 3.26 2007/03/30 15:24:54 cafagna Exp $ |
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# |
# |
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# $Log: v_100.txt,v $ |
# $Log: v_100.txt,v $ |
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# Revision 3.22 2006/11/28 11:43:41 pam-ba |
# Revision 3.26 2007/03/30 15:24:54 cafagna |
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# History modified |
# Calo geometry modified. X-view plane shifts in X coordinates have been swapped, i.e. they do start with X=0.05 instead of X=-0.05 |
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# |
# |
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# Revision 3.21 2006/11/28 10:26:15 pam-ba |
# Revision 3.25 2006/12/17 14:53:18 cafagna |
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# S3 positioning completed |
# Full review of the CARD geometry. S1 table added |
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# |
# |
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# Revision 3.20 2006/11/16 18:45:29 pam-ba |
# Revision 3.20 2006/11/16 18:45:29 pam-ba |
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# Simulated an aluminum container for S4 |
# Simulated an aluminum container for S4 |
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#CMZ : 1.00/03 30/04/96 12.23.59 by Francesco Cafagna |
#CMZ : 1.00/03 30/04/96 12.23.59 by Francesco Cafagna |
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#CMZ : 1.00/02 05/04/96 15.31.25 by Francesco Cafagna |
#CMZ : 1.00/02 05/04/96 15.31.25 by Francesco Cafagna |
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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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30 November 2006, Bari F. Cafagna |
Sept 2007, Bari |
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BUG FIXED |
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For some reason there was a conflict using FLUKA and the GARFILD |
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interface for the TRD. The file TRD_ATT.TXT was treated as flukaerr |
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file by the compiler. It is not clear why. The code was correct, |
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the logical units and names were not inconflict, but the compiler |
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assigned to them the same internal number. It may be a problem |
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related to the optimization phase. I did close the file just after |
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the read-out in GPDAT.F and commented out the closing in UGLAST.F |
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POWER LAW SPECTRA GENERATION: |
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It is now possible to select a power law spectra. Using the |
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datacard: PLAW, is possible to pass the spectral index and the |
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kinetic energy range. In PAWL(1) the user can pass the signed power |
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law index, i.e. PAWL -2.5, will generate a power law spectrum |
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according to exp(-2.5). Please note that the range is in kinetic |
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energy. In gukine the generated particle charateristics will be |
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retrived and the mass calculated from this infos. The KINE data |
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card assigned momentum will be overriden as well. |
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PATHLENGHT CALCULATION MODIFIED IN TOF: |
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The pathlength calulation saved in the TOF hit structure has now |
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been modified. Insted of the pathlenght inside each paddle the |
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average pathlenght from the generation vertex to the hit in the |
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paddle, is saved. In this way it will be possible to calculate the |
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beta using this variable. |
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ERROR IN MATERIAL ASSIGNMENT FOR NEUTRON DETECTOR: |
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The material assigned to the NDTU volume was wrong. It was |
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scintillator, IRON has been asigned now. |
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March 2007, Bari |
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CALO GEOMETRY: |
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An error was found in the original document describing PAMELA |
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geometry. The shift along X axis of the X view planes are swapped, |
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i.e. they don't start with X=+0.05 but with X=-0.05. The sequence |
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is: 0.05m -0.05, 0.05, -0.05 and so on. |
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MAKEFILE FIXED: |
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Option -fdebug_kludge has been discharged |
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GASATT WRNING FIXED: |
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There was a warning message from a graphic routine. The GSATT calls has been commented out. |
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December 2006, Bari |
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CARD GEOMETRY: |
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Positions, dimensions and quotes have been updated. Indeed, the aluminium table |
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under S1, legs included, and the magnetic screen between the CARD and S2 have |
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been added. |
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#------------------------------------------------------------------------- |
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November 2006, Bari |
November 2006, Bari |
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S4 GEOMETRY UPDATED: |
S4 GEOMETRY UPDATED: |
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The x and y dimensions have been corrected because they were wrong. |
The x and y dimensions have been corrected because they were wrong. |
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A container of aluminum has been added having walls of thickness equal |
A container of aluminum has been added having walls of thickness equal |
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to 0.1 cm. |
to 0.1 cm. |
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TOF POSITIONS DEFINITELY UPDATED: |
TOF POSITIONS DEFINITELY UPDATED: |
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S2 and S1 have been positioned again, after the simulation of the top plate. |
S2 and S1 have been positioned again, after the simulation of the top plate. |
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Before now, the positions were put by hand based on the positions given by |
Before now, the positions were put ad hoc based on the positions given by |
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Sergio Ricciarini in the document 'Main geometrical parameters of the PAMELA |
Sergio Ricciarini in the document 'Main geometrical parameters of the PAMELA |
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sub-detectors' released by O. Adriani, L. Bonechi, E. Mocchiutti and |
sub-detectors' released by O. Adriani, L. Bonechi, E. Mocchiutti and |
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S. Ricciarini on the 20th of December 2005.. These positions were |
S. Ricciarini on the 20th of December 2005.. These positions were |
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lightly approximated because the thicknesses of the mylar and of the glue were |
lightly approximated. |
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not considered in that document. Also the height of S3 has been modified as |
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suggested from the Naples PAMELA collaborators. |
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150 |
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ND GEOMETRY COMPLETED. |
ND GEOMETRY COMPLETED. |
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The He3 and the polyethylene (CH2) have been added to fill |
The He3 and the polyethylene (CH2) have been added to fill |
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details of these materials. |
details of these materials. |
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TOP PLATE GEOMETRY ADDED. |
TOP PLATE GEOMETRY ADDED. |
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The top plate geometry has been simulated as a rectangular window filled |
The top plate geometry has been simulated as a N2 box that has the same |
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with a mixture of titanium (90%), aluminum (6%) and vanadium (4%). It has been |
dimensions of CATA. Inside it, at the right positions, there are S2 and CATA. |
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put in a N2 box having the same planar dimensions of CATA. In this box there |
The real top plate is a rectangular window having a thickness of 0.5 cm |
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are also S2 and CATA at the right positions. Then the top plate geometry has |
(volume TPTL emptied by the volume TPCV). This volume is filled with a mixture |
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been completed with other eight small volumes of titanium positioned at the |
of titanium (90%), aluminum (6%) and vanadium (4%). Other parts of titanium |
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corners of the N2 box. Four of them are at the same height of CATA, the |
are the four volumes TPTU, which are positioned at the corners of TPTL at the |
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other four are at the same height of S2. The simulated geometry of the top |
same height of CATA, and the four volumes TPTM, which are positioned at the |
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plate is based on a simplified version of the CAD drawings. |
corners of TPTL, at the same height of S2. |
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The geometry of the top plate is based on a simplified version of the CAD |
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drawings. |
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October 2006, Bari |
October 2006, Bari |
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missing in the subroutine gpgeo.F, has been added; the meaning of the SPHE |
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: |
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 |
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. |
a flat one.Now NDET 'SPHE' eliminates the whole container of PAMELA. |
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June 2006, Bari |
June 2006, Bari |
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The center of the scintillator planes S22Y (variable ZPAMS22Y in gpdgeo.inc) |
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 |
and S12X (variable ZPAMS12X in gpdgeo.inc) has been positioned at the |
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E. Mocchiutti, S. Ricciarini, 20 December 2005). Follows that the positions |
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 |
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 |
that in GPAMELA the thickness of the mylar has been considered while in the |
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document it has been neglected. |
document it has been neglected. |
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May 2006, Bari & Tor Vergata |
May 2006, Bari & Tor Vergata |
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ntple booking have been updated. The GPDCAL routine has been fixed |
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 |
so to handle the case in wich hits stored are more than the maximum |
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number of hit. |
number of hit. |
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In this case in the ntple up to the maximum number of hits will be stored. |
In this case in the ntple up to the maximum number of hits will be stored. |
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April 2006, Bari |
April 2006, Bari |
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is set to true in GPDAT if the data card: HPAK, is set to |
is set to true in GPDAT if the data card: HPAK, is set to |
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'GCAL'. The gpkey.inc has been update accordingly. |
'GCAL'. The gpkey.inc has been update accordingly. |
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NEUTRON DETECTOR ADDED. NEW DIR: GPND |
NEUTRON DETECTOR ADDED. NEW DIR: GPND |
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The neutron detector has been added. At the moment it is just the |
The neutron detector has been added. At the moment it is just the |
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http://www.staff.uni-mainz.de/zeitnitz/Gcalor/gcalor.html |
http://www.staff.uni-mainz.de/zeitnitz/Gcalor/gcalor.html |
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This package should be distributed with the GEANT library but is |
This package should be distributed with the GEANT library but is |
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not up to date. I did download the latest release and stored into |
not up to date. I did download the latest release and stored into |
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gpcalor directory of the gpamela tree. |
gpcalor directory of the gpamela tree. |
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Then I did clean up the code substituting the explicit inclusion of |
Then I did clean up the code substituting the explicit inclusion of |
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the commons with a #include cpp directive. In parallel I did |
the commons with a #include cpp directive. In parallel I did |
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extract the commons to include files having the same common name. I |
extract the commons to include files having the same common name. I |
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NOTE: There are still problem due to different common sizes. In |
NOTE: There are still problem due to different common sizes. In |
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particular the common MICFIL is maller in the geant library |
particular the common MICFIL is maller in the geant library |
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libgeant.a . There the subroutines: gmorin, gmxsec, gmplxs, are |
libgeant.a . There the subroutines: gmorin, gmxsec, gmplxs, are |
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present and linked using a wrong version of the common. This still needs to be debuged. |
present and linked using a wrong version of the common. This still needs to be debuged. |
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NOTE2: The auxiliary files with the cross sections: chetc.dat.gz |
NOTE2: The auxiliary files with the cross sections: chetc.dat.gz |
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and xsneut.dat.gz, have been added to the aux directory and moved |
and xsneut.dat.gz, have been added to the aux directory and moved |
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to the working directory, i.e. GPAMELA_BIN. The GCALOR routine will |
to the working directory, i.e. GPAMELA_BIN. The GCALOR routine will |
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searched there at first, then in the working directory. A fool |
searched there at first, then in the working directory. A fool |
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proof policy has to be implemented to avoid problem with |
proof policy has to be implemented to avoid problem with |
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synchronization fo these files. |
synchronization fo these files. |
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The GCALOR package |
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The GCALOR package |
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June 2005, Bari |
June 2005, Bari |
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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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NEW DATA CARD ADDED: HFSF |
NEW DATA CARD ADDED: HFSF |
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To define a policy for the random number initial seeds |
To define a policy for the random number initial seeds |
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definition. Using this card is possible to override GEANT seeds |
definition. Using this card is possible to override GEANT seeds |
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defined via NRDM card. The policy is selected according to the |
defined via NRDM card. The policy is selected according to the |
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values: |
values: |
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- 1: The seeds are initialized to the initial values found in a user |
- 1: The seeds are initialized to the initial values found in a user |
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defined file or the default file: INPUTSEED.DAT |
defined file or the default file: INPUTSEED.DAT |
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- 2: The seeds are initialized to the final values found in a user defined |
- 2: The seeds are initialized to the final values found in a user defined |
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file or the default file: INPUTSEED.DAT |
file or the default file: INPUTSEED.DAT |
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The case 1 must be used in case the user needs to reproduce the |
The case 1 must be used in case the user needs to reproduce the |
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binary file and pass the filename to the program using the *FLSF |
binary file and pass the filename to the program using the *FLSF |
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data card. In case the user file is not specified the default |
data card. In case the user file is not specified the default |
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INPUTSEED.DAT will be used. |
INPUTSEED.DAT will be used. |
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The case 2 must be used in case the user needs to chain several |
The case 2 must be used in case the user needs to chain several |
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GPAMELA run and likes to be sure he is starting the random |
GPAMELA run and likes to be sure he is starting the random |
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generator using the right sequence. In this case the user must |
generator using the right sequence. In this case the user must |
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filled with his own seeds. For this purpose an utility program: |
filled with his own seeds. For this purpose an utility program: |
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writeseeds.f, has been added in the aux directory. In case the |
writeseeds.f, has been added in the aux directory. In case the |
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*FSFI card is not specified the default values: 24 and INPUTSEEDS.DAT, will |
*FSFI card is not specified the default values: 24 and INPUTSEEDS.DAT, will |
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be used as LUN and file name respectively. |
be used as LUN and file name respectively. |
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NEW DATA CARD ADDED: *LSFI |
NEW DATA CARD ADDED: *LSFI |
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Using this card the user can specify the logical unit and name of |
Using this card the user can specify the logical unit and name of |
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run. This file is a FORTRAN binary one. This file can be used as |
run. This file is a FORTRAN binary one. This file can be used as |
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input one specifying it in the *FSFI data card of the next GPAMELA |
input one specifying it in the *FSFI data card of the next GPAMELA |
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run. In case the *LSFI card is not specified the default values: 26 |
run. In case the *LSFI card is not specified the default values: 26 |
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and HBOOKFILENAME.DAT (as sepified in *HFI), will be used as LUN |
and HBOOKFILENAME.DAT (as sepified in *HFI), will be used as LUN |
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and file name respectively. |
and file name respectively. |
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NEW UTILITY PROGRAMS ADDED: writeseeds.f, readseeds.f |
NEW UTILITY PROGRAMS ADDED: writeseeds.f, readseeds.f |
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These new programs have been added in the aux directory. Using these a |
These new programs have been added in the aux directory. Using these a |
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has been revied and new sets of calibration constants calculated |
has been revied and new sets of calibration constants calculated |
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comparing the beam test data with the GPAMELA results. The new |
comparing the beam test data with the GPAMELA results. The new |
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constants are about 3% larger than the previous ones. |
constants are about 3% larger than the previous ones. |
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TRACKER GEOMETRY REVIEWED. NEW VOLUME DEFINED: THBP, TPAS, TPAI |
TRACKER GEOMETRY REVIEWED. NEW VOLUME DEFINED: THBP, TPAS, TPAI |
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Thanks to Lorenzo Bonechi for the drawings and explanations. Now the |
Thanks to Lorenzo Bonechi for the drawings and explanations. Now the |
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hybrd cards have been put into the simulation and the geometry updated |
hybrd cards have been put into the simulation and the geometry updated |
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considering the dead zones in the silicon detectors. The hybrid zone |
considering the dead zones in the silicon detectors. The hybrid zone |
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has been simulated as well. At the moment the hybrid is simulated as |
has been simulated as well. At the moment the hybrid is simulated as |
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a G10 plates. The full height of the tracker magnet has been |
a G10 plates. The full height of the tracker magnet has been |
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reviewed as well. |
reviewed as well. |
403 |
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The tracker ladder is now simulated inside a nitrogen box: TPAS, |
The tracker ladder is now simulated inside a nitrogen box: TPAS, |
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placed inside an aluminum frame: TRPB. Each silicon ladder has been |
placed inside an aluminum frame: TRPB. Each silicon ladder has been |
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smaller silicon detector: TPAI, has been placed inside the larger |
smaller silicon detector: TPAI, has been placed inside the larger |
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silicon block TRSL. In this way the subdivided silicon ladder can |
silicon block TRSL. In this way the subdivided silicon ladder can |
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be upgraded with an indipendend roto-translation for each sensor. |
be upgraded with an indipendend roto-translation for each sensor. |
410 |
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The TRPB aluminum frame has been enlarged to fit the external |
The TRPB aluminum frame has been enlarged to fit the external |
412 |
magnet canister frame. |
magnet canister frame. |
413 |
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The last plane has been flipped with a 180 degree rotation around |
The last plane has been flipped with a 180 degree rotation around |
415 |
the X axis. |
the X axis. |
416 |
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TRACKER HIT STRUCTURE REVIEWED |
TRACKER HIT STRUCTURE REVIEWED |
418 |
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Taking into account the new version of the tracker geometry, the hit |
Taking into account the new version of the tracker geometry, the hit |
420 |
structure for this detector has been revied. |
structure for this detector has been revied. |
421 |
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422 |
CALORIMETER GEOMETRY REVIEWED |
CALORIMETER GEOMETRY REVIEWED |
423 |
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424 |
Marco Albi reviewed the calorimeter dimentions and positioning. |
Marco Albi reviewed the calorimeter dimentions and positioning. |
425 |
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426 |
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29 March 2004, Bari |
29 March 2004, Bari |
435 |
the GARFIELD code for details). Follows that different runs produce |
the GARFIELD code for details). Follows that different runs produce |
436 |
different results without changing the initial seeds. To have identical |
different results without changing the initial seeds. To have identical |
437 |
results in different runs, the GARFIELD program has to start typing the |
results in different runs, the GARFIELD program has to start typing the |
438 |
noRNDM_initialisation switch. To avoid of specifying this switch |
noRNDM_initialisation switch. To avoid of specifying this switch |
439 |
by the user, |
by the user, |
440 |
the GARFIELD package has been upgraded with a patch. In this way the problem |
the GARFIELD package has been upgraded with a patch. In this way the problem |
441 |
is partially solved because, now, the initial seeds of the random generators |
is partially solved because, now, the initial seeds of the random generators |
443 |
activated by the user for changing the initial seeds in the GPAMELA program. |
activated by the user for changing the initial seeds in the GPAMELA program. |
444 |
Work is in progress for a more general correction of this problem. |
Work is in progress for a more general correction of this problem. |
445 |
Please, use the updated GARFIELD code released with the CVS version v4r1 |
Please, use the updated GARFIELD code released with the CVS version v4r1 |
446 |
to fix this problem. |
to fix this problem. |
447 |
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448 |
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449 |
RNDM ROUTINE REPLACED BY THE GRNDM ROUTINE IN GPXTR AND NPOISS. |
RNDM ROUTINE REPLACED BY THE GRNDM ROUTINE IN GPXTR AND NPOISS. |
456 |
the GPSED common when the set and the detector ZEBRA banks are filled |
the GPSED common when the set and the detector ZEBRA banks are filled |
457 |
during a run. In general the values of the set and detector addresses |
during a run. In general the values of the set and detector addresses |
458 |
depend on the number of active detectors in a given run. ISCAL=12 and |
depend on the number of active detectors in a given run. ISCAL=12 and |
459 |
IDCASI=1 are only right when all the detectors of GPAMELA are active. |
IDCASI=1 are only right when all the detectors of GPAMELA are active. |
460 |
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461 |
9 December 2003, Bari |
9 December 2003, Bari |
462 |
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500 |
-ICAPLANE(i) contains the number of hit plane; |
-ICAPLANE(i) contains the number of hit plane; |
501 |
-ICASTRIP(i) contains the number of hit strip; |
-ICASTRIP(i) contains the number of hit strip; |
502 |
-ICAMOD(i) can assume different values based on the number of times and |
-ICAMOD(i) can assume different values based on the number of times and |
503 |
positions in which a `long strip' has been hit. |
positions in which a `long strip' has been hit. |
504 |
-ENESTRIP(i) contains the deposited energy in the hit strip; |
-ENESTRIP(i) contains the deposited energy in the hit strip; |
505 |
where i is the number of hit (1<i<4224). |
where i is the number of hit (1<i<4224). |
506 |
Note that in the calorimeter each hit is filled at the end of the event and |
Note that in the calorimeter each hit is filled at the end of the event and |
526 |
The energy deposited in the calorimeter is calculated in GeV. |
The energy deposited in the calorimeter is calculated in GeV. |
527 |
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|
528 |
To store the hits in the calorimeter the subroutine GSAHIT is used instead of |
To store the hits in the calorimeter the subroutine GSAHIT is used instead of |
529 |
GSCHIT. |
GSCHIT. |
530 |
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|
531 |
To retrieve the hit structure the call to the routine GPRHIT is done instead |
To retrieve the hit structure the call to the routine GPRHIT is done instead |
532 |
of a call to the GFHITS subroutine. |
of a call to the GFHITS subroutine. |
533 |
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534 |
25 February 2003, Bari |
25 February 2003, Bari |
535 |
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536 |
BUG found: |
BUG found: |
537 |
DCUTEAER, DCUTEAL, DCUTECE, DCUTECP, DCUTEFE, DCUTEG10C, DCUTEG10, DCUTEKAP, |
DCUTEAER, DCUTEAL, DCUTECE, DCUTECP, DCUTEFE, DCUTEG10C, DCUTEG10, DCUTEKAP, |
538 |
DCUTEN2G, DCUTEROA, DCUTESCIN, DCUTESICA, DCUTETRAD, DCUTEW2, |
DCUTEN2G, DCUTEROA, DCUTESCIN, DCUTESICA, DCUTETRAD, DCUTEW2, |
556 |
Updated the relative positions of the calorimeter planes. The corrected |
Updated the relative positions of the calorimeter planes. The corrected |
557 |
shifting are: |
shifting are: |
558 |
|
|
559 |
first view: (Dxo,Dyo)=(0.10,0.05) cm |
first view: (Dxo,Dyo)=(0.10,0.05) cm |
560 |
second view: (Dxo,Dyo)=(-0.05,0.10) cm |
second view: (Dxo,Dyo)=(-0.05,0.10) cm |
561 |
third view: (Dxo,Dyo)=(-0.10,-0.05) cm |
third view: (Dxo,Dyo)=(-0.10,-0.05) cm |
562 |
fourth view: (Dxo,Dyo)=(0.05,-0.10) cm |
fourth view: (Dxo,Dyo)=(0.05,-0.10) cm |
563 |
|
|
564 |
4 November 2002, Bari |
4 November 2002, Bari |
565 |
|
|
566 |
CAS detectors distances modified |
CAS detectors distances modified |
567 |
|
|
568 |
The distances between the CAS detectors have been modified based on the |
The distances between the CAS detectors have been modified based on the |
569 |
latest CAD drawings. |
latest CAD drawings. |
570 |
|
|
571 |
2 November 2002, Bari |
2 November 2002, Bari |
572 |
|
|
583 |
CALB and CALS. CALS is an aluminum box of dimensions: 48.4*48.4*21.278 cm^3, |
CALB and CALS. CALS is an aluminum box of dimensions: 48.4*48.4*21.278 cm^3, |
584 |
having side-walls 1 cm thick and a bottom of 1 mm. The real box is more |
having side-walls 1 cm thick and a bottom of 1 mm. The real box is more |
585 |
complicated and the configuration of the bottom should be upgraded if we want |
complicated and the configuration of the bottom should be upgraded if we want |
586 |
a reliable description of the event in the S4 scintillator. |
a reliable description of the event in the S4 scintillator. |
587 |
|
|
588 |
22 October 2002, Stockholm |
22 October 2002, Stockholm |
589 |
|
|
1247 |
CAT dimension modified |
CAT dimension modified |
1248 |
CAT dimensions modified after PAOLO simulation and Tom design. Here |
CAT dimensions modified after PAOLO simulation and Tom design. Here |
1249 |
are the new dimensions: |
are the new dimensions: |
1250 |
DATA CATB/22.05,21.05,0.55/ |
DATA CATB/22.05,21.05,0.55/ |
1251 |
DATA CATL/15.75,6.675,0.55/ |
DATA CATL/15.75,6.675,0.55/ |
1252 |
DATA CATT/6.3,14.375,0.55/ |
DATA CATT/6.3,14.375,0.55/ |
1253 |
DATA ZCAT/75.75/ |
DATA ZCAT/75.75/ |