/[PAMELA software]/gpamela/history/v_100.txt
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revision 3.17 by pam-ba, Fri Oct 13 16:36:59 2006 UTC revision 3.28 by pamela, Tue Jan 29 18:25:18 2008 UTC
# Line 1  Line 1 
1    # Revision 3.21  2006/12/05 18:45:29  bruno
2    # Update of the CARD geometry
3    # Simulated also legs, table and magnetic screen
4  #  #
5  # $Id: v_100.txt,v 3.16 2006/10/12 11:11:21 pam-ba Exp $  # $Id: v_100.txt,v 3.27 2007/10/02 17:58:32 cafagna Exp $
6  #  #
7  # $Log: v_100.txt,v $  # $Log: v_100.txt,v $
8    # Revision 3.27  2007/10/02 17:58:32  cafagna
9    # Power law spectra introduced
10    #
11    # Revision 3.26  2007/03/30 15:24:54  cafagna
12    # 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
13    #
14    # Revision 3.25  2006/12/17 14:53:18  cafagna
15    # Full review of the CARD geometry. S1 table added
16    #
17    # Revision 3.20  2006/11/16 18:45:29  pam-ba
18    # Simulated an aluminum container for S4
19    #
20    # Revision 3.19  2006/11/16 12:01:13  pam-ba
21    # S4 dimensions corrected.
22    #
23    # Revision 3.18  2006/11/10 11:39:35  pam-ba
24    # S2 and S1 z-positions corrected, He3 and plystyrene mixture added, Top Plate geometry simulated and titanium mixture added.
25    #
26    # Revision 3.17  2006/10/13 16:36:59  pam-ba
27    # Added a new material, the cadmium, for ND
28    #
29  # Revision 3.16  2006/10/12 11:11:21  pam-ba  # Revision 3.16  2006/10/12 11:11:21  pam-ba
30  # ND geometry updated.  # ND geometry updated.
31  #  #
# Line 62  Line 86 
86  #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
87  #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
88  #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
89  #-- Author :    Francesco Cafagna   28/11/95  #-- Author :    Francesco Cafagna   28/11/95
90    
91    Jan 2008, Bari
92    
93    PRESSURIZED CONTAINER GEOMETRY:
94       Pressurized container geometry has been updated: top container TSPH
95       now has been placed at the maximum distance, quoted in the ICD,
96       from S1: 5cm. This distance corresponds to the maximum one in
97       flight due to the cover deformation due to the internal
98       pressure. Three thermal cover layers (nylon6, mylar and aluminium,
99       respectively in the new volumes COV1, COV2 and COV3) have been
100       added to the top container.
101    
102    NEW MATERIALS AND TRACKING MEDIA:
103    
104       Two new materials have been implemented: AMg6M mixture for volume
105       TSPH, and Nylon6 mixture for volume COV1.  New tracking medium have
106       been added for Nylon6 Mixture (TNYL), AMg6M Mixture (TAMG) and Iron
107       (TIRO).
108    
109    TOF GEOMETRY:
110       TOF geometry has been updated: Scintillators positions in the
111       GPAMELA reference system have been corrected shifting all
112       scintillator paddle by 23 microns.
113    
114    TRACK NUMBER RECORDED FOR TOF:
115       The TOF structure now register the stack number into the HIT
116       structure. In GUSTEP the stack number is tested, if is greater than
117       0, i.e. the particle is not the primary, the particle number is set
118       to 1000+IPART and passed to GPUTOF. Accordingly, now IPARTOF
119       variable can assume 2000 values instead of 100.
120    
121    POWER LAW SPECTRA GENERATION:
122       PLAW datacard parameters have been increased to 4. The meaning of
123       the 4th parameter is: extract random kinetic energy if PLAW(4)<0.,
124       or extract random momentum if PLAW(4)>=0..
125    
126    Sept 2007, Bari
127    
128    POWER LAW SPECTRA GENERATION:
129       It is now possible to select a power law spectra. Using the
130       datacard: PLAW, is possible to pass the spectral index and the
131       kinetic energy range. In PAWL(1) the user can pass the signed power
132       law index, i.e. PAWL -2.5, will generate a power law spectrum
133       according to exp(-2.5). Please note that the range is in kinetic
134       energy. In gukine the generated particle charateristics will be
135       retrived and the mass calculated from this infos. The KINE data
136       card assigned momentum will be overriden as well.
137    
138    PATHLENGHT CALCULATION MODIFIED IN TOF:
139       The pathlength calulation saved in the TOF hit structure has now
140       been modified. Insted of the pathlenght inside each paddle the
141       average pathlenght from the generation vertex to the hit in the
142       paddle, is saved. In this way it will be possible to calculate the
143       beta using this variable.
144    
145    ERROR IN MATERIAL ASSIGNMENT FOR NEUTRON DETECTOR:
146       The material assigned to the NDTU volume was wrong. It was
147       scintillator, IRON has been asigned now.
148    
149    March 2007, Bari
150    
151    CALO GEOMETRY:
152       An error was found in the original document describing PAMELA
153       geometry.  The shift along X axis of the X view planes are swapped,
154       i.e. they don't start with X=+0.05 but with X=-0.05.  The sequence
155       is: 0.05m -0.05, 0.05, -0.05 and so on.
156    
157    MAKEFILE FIXED:
158       Option -fdebug_kludge has been discharged
159    
160    GASATT WRNING FIXED:
161       There was a warning message from a graphic routine. The GSATT calls has been commented out.
162    
163    
164    December 2006, Bari
165    
166    CARD GEOMETRY:
167    Positions, dimensions and quotes have been updated. Indeed, the aluminium table
168    under S1, legs included, and the magnetic screen between the CARD and S2 have
169    been added.
170    
171    #-------------------------------------------------------------------------
172    
173    November 2006, Bari
174    
175    
176    S4 GEOMETRY UPDATED:
177    The x and y dimensions have been corrected because they were wrong.
178    A container of aluminum has been added having walls of thickness equal
179    to 0.1 cm.
180    
181    TOF POSITIONS DEFINITELY UPDATED:
182    S2 and S1 have been positioned again, after the simulation of the top plate.
183    Before now, the positions were put ad hoc based on the positions given by
184    Sergio Ricciarini in the document 'Main geometrical parameters of the PAMELA
185    sub-detectors' released by O. Adriani, L. Bonechi, E. Mocchiutti and
186    S. Ricciarini on the 20th of December 2005.. These positions were
187    lightly approximated.
188    
189    ND GEOMETRY COMPLETED.
190    The He3 and the polyethylene (CH2) have been added to fill
191    the volumes NDTI and NDPB in the neutron detector. Leonov gave us the
192    details of these materials.
193    
194    TOP PLATE GEOMETRY ADDED.
195    The top plate geometry has been simulated as a N2 box that has the same
196    dimensions of CATA. Inside it, at the right positions, there are S2 and CATA.
197    The real top plate is a rectangular window having a thickness of 0.5 cm
198    (volume TPTL emptied by the volume TPCV). This volume is filled with a mixture
199    of titanium (90%), aluminum (6%) and vanadium (4%). Other parts of titanium
200    are the four volumes TPTU, which are positioned at the corners of TPTL at the
201    same height of CATA, and the four volumes TPTM, which are positioned at the
202    corners of TPTL, at the same height of S2.
203    The geometry  of the top plate is based on a simplified version of the CAD
204    drawings.
205    
206  October 2006, Bari  October 2006, Bari
207    
208  The geometry of the neutron detector has been updated. Some dimensions of some  The geometry of the neutron detector has been updated. Some dimensions of some
209  volumes have been corrected while the aluminum cover and the aluminum boxes to  volumes have been corrected and the aluminum cover and the aluminum boxes to
210  put the cables have been added. A new material, the cadmium, has been also  put the cables have been added. A new material, the cadmium, has been also
211  defined.  defined.
212    
# Line 77  SPHE and ND data card bugs fixed: the de Line 216  SPHE and ND data card bugs fixed: the de
216  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
217  data card has been changed. Before the correction the data card:  data card has been changed. Before the correction the data card:
218  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
219  a flat one.Now NDET 'SPHE' eliminates the whole container of PAMELA.  a flat one.Now NDET 'SPHE' eliminates the whole container of PAMELA.
220    
221    
222  June 2006, Bari  June 2006, Bari
223    
224  The center of the scintillator planes S22Y (variable ZPAMS22Y in gpdgeo.inc)  The center of the scintillator planes S22Y (variable ZPAMS22Y in gpdgeo.inc)
225  and S12X (variable ZPAMS12X in gpdgeo.inc) has been positioned at the  and S12X (variable ZPAMS12X in gpdgeo.inc) has been positioned at the
# Line 89  parameters of the PAMELA sub-detectors" Line 228  parameters of the PAMELA sub-detectors"
228  E. Mocchiutti, S. Ricciarini, 20 December 2005). Follows that the positions  E. Mocchiutti, S. Ricciarini, 20 December 2005). Follows that the positions
229  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
230  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
231  document it has been neglected.  document it has been neglected.
232    
233    
234  May 2006, Bari & Tor Vergata  May 2006, Bari & Tor Vergata
# Line 115  CAL HIT STRUCTURE BUGS FIXED Line 254  CAL HIT STRUCTURE BUGS FIXED
254     ntple booking have been updated. The GPDCAL routine has been fixed     ntple booking have been updated. The GPDCAL routine has been fixed
255     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
256     number of hit.     number of hit.
257     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.
258    
259  April 2006, Bari  April 2006, Bari
260    
# Line 158  NEW GPKEY ADDED: GPCALOR Line 297  NEW GPKEY ADDED: GPCALOR
297     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
298     'GCAL'. The gpkey.inc has been update accordingly.     'GCAL'. The gpkey.inc has been update accordingly.
299    
300      
301  NEUTRON DETECTOR ADDED. NEW DIR: GPND  NEUTRON DETECTOR ADDED. NEW DIR: GPND
302    
303     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
# Line 175  GCALOR PACKAGE ADDED. NEW DIRs: GPCALOR, Line 314  GCALOR PACKAGE ADDED. NEW DIRs: GPCALOR,
314     http://www.staff.uni-mainz.de/zeitnitz/Gcalor/gcalor.html     http://www.staff.uni-mainz.de/zeitnitz/Gcalor/gcalor.html
315     This package should be distributed with the GEANT library but is     This package should be distributed with the GEANT library but is
316     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
317     gpcalor directory of the gpamela tree.     gpcalor directory of the gpamela tree.
318     Then I did clean up the code substituting the explicit inclusion of     Then I did clean up the code substituting the explicit inclusion of
319     the commons with a #include cpp directive. In parallel I did     the commons with a #include cpp directive. In parallel I did
320     extract the commons to include files having the same common name. I     extract the commons to include files having the same common name. I
# Line 186  GCALOR PACKAGE ADDED. NEW DIRs: GPCALOR, Line 325  GCALOR PACKAGE ADDED. NEW DIRs: GPCALOR,
325     NOTE: There are still problem due to different common sizes. In     NOTE: There are still problem due to different common sizes. In
326     particular the common MICFIL is maller in the geant library     particular the common MICFIL is maller in the geant library
327     libgeant.a . There the subroutines: gmorin, gmxsec, gmplxs, are     libgeant.a . There the subroutines: gmorin, gmxsec, gmplxs, are
328     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.
329     NOTE2: The auxiliary files with the cross sections: chetc.dat.gz     NOTE2: The auxiliary files with the cross sections: chetc.dat.gz
330     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
331     to the working directory, i.e. GPAMELA_BIN. The GCALOR routine will     to the working directory, i.e. GPAMELA_BIN. The GCALOR routine will
# Line 194  GCALOR PACKAGE ADDED. NEW DIRs: GPCALOR, Line 333  GCALOR PACKAGE ADDED. NEW DIRs: GPCALOR,
333     searched there at first, then in the working directory. A fool     searched there at first, then in the working directory. A fool
334     proof policy has to be implemented to avoid problem with     proof policy has to be implemented to avoid problem with
335     synchronization fo these files.     synchronization fo these files.
     
336    
337  The GCALOR package  
338    The GCALOR package
339    
340  June 2005, Bari  June 2005, Bari
341    
# Line 207  TOF SCINTILLATOR PADDLES UPDATED Line 346  TOF SCINTILLATOR PADDLES UPDATED
346    
347  May 2005, Bari  May 2005, Bari
348    
349  Some updates on the latest modification done in the past year.  Some updates on the latest modification done in the past year.
350    
351  NEW DATA CARD ADDED: HFSF  NEW DATA CARD ADDED: HFSF
352    
353     To define a policy for the random number initial seeds     To define a policy for the random number initial seeds
354     definition. Using this card is possible to override GEANT seeds     definition. Using this card is possible to override GEANT seeds
355     defined via NRDM card. The policy is selected according to the     defined via NRDM card. The policy is selected according to the
356     values:     values:
357    
358     - 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
359          defined file or the default file: INPUTSEED.DAT          defined file or the default file: INPUTSEED.DAT
360      
361     - 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
362          file or the default file: INPUTSEED.DAT          file or the default file: INPUTSEED.DAT
363    
364     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
# Line 228  NEW DATA CARD ADDED: HFSF Line 367  NEW DATA CARD ADDED: HFSF
367     binary file and pass the filename to the program using the *FLSF     binary file and pass the filename to the program using the *FLSF
368     data card. In case the user file is not specified the default     data card. In case the user file is not specified the default
369     INPUTSEED.DAT will be used.     INPUTSEED.DAT will be used.
370      
371     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
372     GPAMELA run and likes to be sure he is starting the random     GPAMELA run and likes to be sure he is starting the random
373     generator using the right sequence. In this case the user must     generator using the right sequence. In this case the user must
# Line 246  NEW DATA CARD ADDED: *FSFI Line 385  NEW DATA CARD ADDED: *FSFI
385     filled with his own seeds. For this purpose an utility program:     filled with his own seeds. For this purpose an utility program:
386     writeseeds.f, has been added in the aux directory.  In case the     writeseeds.f, has been added in the aux directory.  In case the
387     *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
388     be used as LUN and file name respectively.     be used as LUN and file name respectively.
389      
390  NEW DATA CARD ADDED: *LSFI  NEW DATA CARD ADDED: *LSFI
391    
392     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
# Line 255  NEW DATA CARD ADDED: *LSFI Line 394  NEW DATA CARD ADDED: *LSFI
394     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
395     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
396     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
397     and HBOOKFILENAME.DAT (as sepified in *HFI), will be used as LUN     and HBOOKFILENAME.DAT (as sepified in *HFI), will be used as LUN
398     and file name respectively.     and file name respectively.
399      
400  NEW UTILITY PROGRAMS ADDED: writeseeds.f, readseeds.f  NEW UTILITY PROGRAMS ADDED: writeseeds.f, readseeds.f
401    
402     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
# Line 290  TRD GEOMETRY AND CALIBRATION REVIEWD Line 429  TRD GEOMETRY AND CALIBRATION REVIEWD
429     has been revied and new sets of calibration constants calculated     has been revied and new sets of calibration constants calculated
430     comparing the beam test data with the GPAMELA results. The new     comparing the beam test data with the GPAMELA results. The new
431     constants are about 3% larger than the previous ones.     constants are about 3% larger than the previous ones.
432      
433  TRACKER GEOMETRY REVIEWED. NEW VOLUME DEFINED: THBP, TPAS, TPAI  TRACKER GEOMETRY REVIEWED. NEW VOLUME DEFINED: THBP, TPAS, TPAI
434      
435     Thanks to Lorenzo Bonechi for the drawings and explanations. Now the     Thanks to Lorenzo Bonechi for the drawings and explanations. Now the
436     hybrd cards have been put into the simulation and the geometry updated     hybrd cards have been put into the simulation and the geometry updated
437     considering the dead zones in the silicon detectors. The hybrid zone     considering the dead zones in the silicon detectors. The hybrid zone
438     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
439     a G10 plates. The full height of the tracker magnet has been     a G10 plates. The full height of the tracker magnet has been
440     reviewed as well.     reviewed as well.
441    
442     The tracker ladder is now simulated inside a nitrogen box: TPAS,     The tracker ladder is now simulated inside a nitrogen box: TPAS,
443     placed inside an aluminum frame: TRPB. Each silicon ladder has been     placed inside an aluminum frame: TRPB. Each silicon ladder has been
# Line 306  TRACKER GEOMETRY REVIEWED. NEW VOLUME DE Line 445  TRACKER GEOMETRY REVIEWED. NEW VOLUME DE
445     smaller silicon detector: TPAI, has been placed inside the larger     smaller silicon detector: TPAI, has been placed inside the larger
446     silicon block TRSL. In this way the subdivided silicon ladder can     silicon block TRSL. In this way the subdivided silicon ladder can
447     be upgraded with an indipendend roto-translation for each sensor.     be upgraded with an indipendend roto-translation for each sensor.
448      
449     The TRPB aluminum frame has been enlarged to fit the external     The TRPB aluminum frame has been enlarged to fit the external
450     magnet canister frame.     magnet canister frame.
451      
452     The last plane has been flipped with a 180 degree rotation around     The last plane has been flipped with a 180 degree rotation around
453     the X axis.     the X axis.
454      
455  TRACKER HIT STRUCTURE REVIEWED  TRACKER HIT STRUCTURE REVIEWED
456    
457     Taking into account the new version of the tracker geometry, the hit     Taking into account the new version of the tracker geometry, the hit
458     structure for this detector has been revied.     structure for this detector has been revied.
459    
460  CALORIMETER GEOMETRY REVIEWED  CALORIMETER GEOMETRY REVIEWED
461    
462     Marco Albi reviewed the calorimeter dimentions and positioning.     Marco Albi reviewed the calorimeter dimentions and positioning.
463    
464    
465  29 March 2004, Bari  29 March 2004, Bari
# Line 334  NON-REPRODUCIBILITY PROBLEM OF A GPAMELA Line 473  NON-REPRODUCIBILITY PROBLEM OF A GPAMELA
473     the GARFIELD code for details). Follows that different runs produce     the GARFIELD code for details). Follows that different runs produce
474     different results without changing the initial seeds. To have identical     different results without changing the initial seeds. To have identical
475     results in different runs, the GARFIELD program has to start typing the     results in different runs, the GARFIELD program has to start typing the
476     noRNDM_initialisation switch. To avoid of specifying this switch     noRNDM_initialisation switch. To avoid of specifying this switch
477     by the user,     by the user,
478     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
479     is partially solved because, now, the initial seeds of the random generators     is partially solved because, now, the initial seeds of the random generators
# Line 342  NON-REPRODUCIBILITY PROBLEM OF A GPAMELA Line 481  NON-REPRODUCIBILITY PROBLEM OF A GPAMELA
481     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.
482     Work is in progress for a more general correction of this problem.     Work is in progress for a more general correction of this problem.
483     Please, use the updated GARFIELD code released with the CVS version v4r1     Please, use the updated GARFIELD code released with the CVS version v4r1
484     to fix this problem.       to fix this problem.
485    
486    
487  RNDM ROUTINE REPLACED BY THE GRNDM ROUTINE IN GPXTR AND NPOISS.  RNDM ROUTINE REPLACED BY THE GRNDM ROUTINE IN GPXTR AND NPOISS.
# Line 355  BUG FOUND AND FIXED: the set and detecto Line 494  BUG FOUND AND FIXED: the set and detecto
494     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
495     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
496     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
497     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.
498    
499  9 December 2003, Bari  9 December 2003, Bari
500    
# Line 399  BUG FOUND AND FIXED: the set and detecto Line 538  BUG FOUND AND FIXED: the set and detecto
538     -ICAPLANE(i) contains the number of hit plane;     -ICAPLANE(i) contains the number of hit plane;
539     -ICASTRIP(i) contains the number of hit strip;     -ICASTRIP(i) contains the number of hit strip;
540     -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
541                positions in which a `long strip' has been hit.            positions in which a `long strip' has been hit.
542     -ENESTRIP(i) contains the deposited energy in the hit strip;     -ENESTRIP(i) contains the deposited energy in the hit strip;
543     where i is the number of hit (1<i<4224).     where i is the number of hit (1<i<4224).
544     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
# Line 425  BUG FOUND AND FIXED: the set and detecto Line 564  BUG FOUND AND FIXED: the set and detecto
564     The energy deposited in the calorimeter is calculated in GeV.     The energy deposited in the calorimeter is calculated in GeV.
565    
566     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
567     GSCHIT.     GSCHIT.
568    
569     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
570     of a call to the GFHITS subroutine.     of a call to the GFHITS subroutine.
571    
572  25 February 2003, Bari  25 February 2003, Bari
573    
574  BUG found:  BUG found:
575     DCUTEAER, DCUTEAL, DCUTECE, DCUTECP, DCUTEFE, DCUTEG10C, DCUTEG10, DCUTEKAP,     DCUTEAER, DCUTEAL, DCUTECE, DCUTECP, DCUTEFE, DCUTEG10C, DCUTEG10, DCUTEKAP,
576     DCUTEN2G, DCUTEROA, DCUTESCIN, DCUTESICA, DCUTETRAD, DCUTEW2,     DCUTEN2G, DCUTEROA, DCUTESCIN, DCUTESICA, DCUTETRAD, DCUTEW2,
# Line 455  BUG found: Line 594  BUG found:
594     Updated the relative positions of the calorimeter planes. The corrected     Updated the relative positions of the calorimeter planes. The corrected
595     shifting are:     shifting are:
596    
597     first view: (Dxo,Dyo)=(0.10,0.05) cm     first view: (Dxo,Dyo)=(0.10,0.05) cm
598     second view: (Dxo,Dyo)=(-0.05,0.10) cm     second view: (Dxo,Dyo)=(-0.05,0.10) cm
599     third view: (Dxo,Dyo)=(-0.10,-0.05) cm     third view: (Dxo,Dyo)=(-0.10,-0.05) cm
600     fourth view: (Dxo,Dyo)=(0.05,-0.10) cm     fourth view: (Dxo,Dyo)=(0.05,-0.10) cm
601    
602  4 November 2002, Bari  4 November 2002, Bari
603    
604  CAS detectors distances modified  CAS detectors distances modified
605    
606     The distances between the CAS detectors have been modified based on the     The distances between the CAS detectors have been modified based on the
607     latest CAD drawings.     latest CAD drawings.
608    
609  2 November 2002, Bari  2 November 2002, Bari
610    
# Line 482  CALORIMETER geometry upgrade Line 621  CALORIMETER geometry upgrade
621     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,
622     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
623     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
624     a reliable description of the event in the S4 scintillator.     a reliable description of the event in the S4 scintillator.
625    
626  22 October 2002, Stockholm  22 October 2002, Stockholm
627    
# Line 1146  CAS dimensions and positions modified Line 1285  CAS dimensions and positions modified
1285  CAT dimension modified  CAT dimension modified
1286     CAT dimensions modified after PAOLO simulation and Tom design. Here     CAT dimensions modified after PAOLO simulation and Tom design. Here
1287     are the new dimensions:     are the new dimensions:
1288          DATA CATB/22.05,21.05,0.55/      DATA CATB/22.05,21.05,0.55/
1289          DATA CATL/15.75,6.675,0.55/          DATA CATL/15.75,6.675,0.55/
1290          DATA CATT/6.3,14.375,0.55/          DATA CATT/6.3,14.375,0.55/
1291          DATA ZCAT/75.75/          DATA ZCAT/75.75/

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