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revision 3.5 by pamela, Tue Apr 6 10:33:46 2004 UTC revision 3.12 by pam-ba, Thu May 18 10:52:32 2006 UTC
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1    
2  #  #
3  # $Id: v_100.txt,v 3.4 2003/12/17 11:32:50 pamela Exp $  # $Id: v_100.txt,v 3.11 2006/05/11 23:53:15 cafagna Exp $
4  #  #
5  # $Log: v_100.txt,v $  # $Log: v_100.txt,v $
6    # Revision 3.11  2006/05/11 23:53:15  cafagna
7    # More bugs fixed in the CALO ntple structure filling
8    #
9    # Revision 3.10  2006/04/10 11:07:43  cafagna
10    # GEN data card updated, ZDGEN added
11    #
12    # Revision 3.9  2005/12/14 03:34:40  cafagna
13    # An update of the history and inform readme files.
14    #
15    # Revision 3.8  2005/12/14 03:16:08  cafagna
16    # Neutron detector added. Geometry and GPCALOR package
17    #
18    # Revision 3.7  2005/10/18 08:24:35  cafagna
19    # History updated
20    #
21    # Revision 3.6  2005/07/25 11:53:21  cafagna
22    # Several updates. See history for details
23    #
24    # Revision 3.5  2004/04/06 10:33:46  pamela
25    # NON-REPRODUCIBILITY problem of a GPAMELA RUN fixed; bug found and fixed filling in the hit structure of the calorimeter
26    #
27  # Revision 3.4  2003/12/17 11:32:50  pamela  # Revision 3.4  2003/12/17 11:32:50  pamela
28  # CALO SIMULATION COMPLETED: geometry and special tracking parameters updated and simulation checked by a comparison with the Trieste's standalone Monte Carlo simulation  # CALO SIMULATION COMPLETED: geometry and special tracking parameters updated and simulation checked by a comparison with the Trieste's standalone Monte Carlo simulation
29  #  #
# Line 28  Line 50 
50  #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
51  #-- Author :    Francesco Cafagna   28/11/95  #-- Author :    Francesco Cafagna   28/11/95
52    
53    May 2006, Bari & Florence
54    
55    CAL HIT STRUCTURE BUGS FIXED
56    
57       The maximum number of hit is now different for the two hit
58       structures: CALST and CALI. Vectors inizialization and HBOOK
59       ntple booking have been updated. The GPDCAL routine has been fixed
60       so to handle the case in wich hits stored are more than the maximum
61       number of hit.
62       In this case in the ntple up to the maximum number of hits will be stored.
63    
64    April 2006, Bari
65    
66    TOF GEOMETRY AND POSITIONS UPDATED AND NEW MIXTURES ADDED
67    
68       The TOF geometry has been modified. The following boxes have been
69       added: POL1, POL2 and POLY made of polystyrene, S11M, S12M, S21M,
70       S22M, S31M and S32M made of mylar, S1A, S2A and S3 made of air and
71       S1 and S2 made of aluminum. Each scintillator paddle has been put
72       in his mylar box and the other materials: air, polystyrene, and
73       aluminum have been added at their nominal positions.  According to
74       Naples people the araldite glue has been simulated has an air
75       gap. For this work two new materials: the Mylar (MYLAR) and the
76       polystyrene (POLYSTYRENE) with a density of 35 g/l have been
77       defined as a mixture.  The positions of the three bottom
78       scintillator planes that contain respectively the S12X, S22Y and
79       S32X paddles have been regulated according on their official
80       positions in PAMELA.
81    
82    Mar 2006, Bari
83    
84    GEN DATA CARD UPDATED
85    
86       To enable generation on a surface perpendicular to the XY plane,
87       GEN gata card has been updated addingh a new parameter: ZDGEN. This is
88       the dimension, along Z axis , of the generation surface. The Z
89       position will be randomply chosen according to: Z= ZDGEN*RNDM_NUMBER +
90       ZGEN, i.e. Z= GEN(6)*RNDM_NOMBER + GEN(3).
91    
92    Nov 2005, Bari
93    
94    GUHADR AND GUPHAD UPDATED
95    
96       To use GCALOR package the hadronic routines have been updated. The
97       inizialization routine call CALSIG, while the other calls GCALOR.
98    
99    NEW GPKEY ADDED: GPCALOR
100    
101       This logical has been added to enable the GCALOR package. This flag
102       is set to true in GPDAT if the data card: HPAK, is set to
103       'GCAL'. The gpkey.inc has been update accordingly.
104    
105      
106    NEUTRON DETECTOR ADDED. NEW DIR: GPND
107    
108       The neutron detector has been added. At the moment it is just the
109       geometry. The directory structure of the repository has been
110       updated as well. Dimensions has been taken from picture and
111       literature. A full upgrade to the drawing is needed.
112    
113    GCALOR PACKAGE ADDED. NEW DIRs: GPCALOR, GPCALORDES
114    
115       GCALOR package contins the CALOR simulation code and an interface
116       to use it in GEANT. The important feature for us is the usage of
117       the MICAP code. This is facused on the low energy neutron
118       simulation. for details see:
119       http://www.staff.uni-mainz.de/zeitnitz/Gcalor/gcalor.html
120       This package should be distributed with the GEANT library but is
121       not up to date. I did download the latest release and stored into
122       gpcalor directory of the gpamela tree.
123       Then I did clean up the code substituting the explicit inclusion of
124       the commons with a #include cpp directive. In parallel I did
125       extract the commons to include files having the same common name. I
126       did store the include files into a newly created directory:
127       gpcalordes.
128       The Makefile has been updated accordingly.
129       Please note that to avoid conflict with CRENLIB distribution the gcalor source file has been named gpcalor.F
130       NOTE: There are still problem due to different common sizes. In
131       particular the common MICFIL is maller in the geant library
132       libgeant.a . There the subroutines: gmorin, gmxsec, gmplxs, are
133       present and linked using a wrong version of the common. This still needs to be debuged.
134       NOTE2: The auxiliary files with the cross sections: chetc.dat.gz
135       and xsneut.dat.gz, have been added to the aux directory and moved
136       to the working directory, i.e. GPAMELA_BIN. The GCALOR routine will
137       look for CERN_ROOT environment variable. If found files are
138       searched there at first, then in the working directory. A fool
139       proof policy has to be implemented to avoid problem with
140       synchronization fo these files.
141      
142    
143    The GCALOR package
144    
145    June 2005, Bari
146    
147    TOF SCINTILLATOR PADDLES UPDATED
148    
149       The dimensions and the number of the scintillator paddles for each
150       TOF planes have been updated.
151    
152    May 2005, Bari
153    
154    Some updates on the latest modification done in the past year.
155    
156    NEW DATA CARD ADDED: HFSF
157    
158       To define a policy for the random number initial seeds
159       definition. Using this card is possible to override GEANT seeds
160       defined via NRDM card. The policy is selected according to the
161       values:
162    
163       - 1: The seeds are initialized to the initial values found in a user
164            defined file or the default file: INPUTSEED.DAT
165      
166       - 2: The seeds are initialized to the final values found in a user defined
167            file or the default file: INPUTSEED.DAT
168    
169       The case 1 must be used in case the user needs to reproduce the
170       random chain of a previous run. In this case the user can save the
171       initial seeds, used in the run he would like to reproduce, in a
172       binary file and pass the filename to the program using the *FLSF
173       data card. In case the user file is not specified the default
174       INPUTSEED.DAT will be used.
175      
176       The case 2 must be used in case the user needs to chain several
177       GPAMELA run and likes to be sure he is starting the random
178       generator using the right sequence. In this case the user must
179       specify an input binary file using the *FLSF data card, otherwise
180       the INPUTSEED.DAT file will be used.
181    
182    NEW DATA CARD ADDED: *FSFI
183    
184       Using this card the user can specify the logical unit and name of
185       the file storing the initial seeds to be used to initialize the
186       random number generator. This file must be a FORTRAN binary one
187       storing four integer numbers. The first two are the number to be
188       used in the case: HFSF=1, the other two will be used in the case:
189       HFSF=2. This file can be one created by GPAMELA or by the user
190       filled with his own seeds. For this purpose an utility program:
191       writeseeds.f, has been added in the aux directory.  In case the
192       *FSFI card is not specified the default values: 24 and INPUTSEEDS.DAT, will
193       be used as LUN and file name respectively.
194      
195    NEW DATA CARD ADDED: *LSFI
196    
197       Using this card the user can specify the logical unit and name of
198       the file storing the first and last seeds used in the GPAMELA
199       run. This file is a FORTRAN binary one. This file can be used as
200       input one specifying it in the *FSFI data card of the next GPAMELA
201       run.  In case the *LSFI card is not specified the default values: 26
202       and HBOOKFILENAME.DAT (as sepified in *HFI), will be used as LUN
203       and file name respectively.
204      
205    NEW UTILITY PROGRAMS ADDED: writeseeds.f, readseeds.f
206    
207       These new programs have been added in the aux directory. Using these a
208       user defined seed file can be created and re-read.
209    
210    NEW VOLUMES ADDED: MSHE, BSPH; PRESSURIZED CONTAINER ADDED
211    
212       Alexey Bakaldin, in MEPHI, did add the PAMELA pressurized container to
213       the simulation. He did defined new volumes filled with aluminum and
214       placed inside the mother volume. Positions have been fine tuned by
215       Marialuigia Ambriola and compared to the CAD drawings.
216       Two new volumes have been added to simulate the container:
217       - MSHE, a tube simulating the middle part of the container
218       - BSPH, the spherical bottom part of the container
219    
220       To better simulate the upper part the SHEL volume has been modified
221       into a cone. Dimentions of the top cover: TSPH, have been modified
222       accordingly.
223    
224    DETECTOR POSITIONS REVIEWED
225    
226       All detector Z positions have been reviewd to fit into the
227       simulated pressurized container.
228    
229    TRD GEOMETRY AND CALIBRATION REVIEWD
230    
231       The TRD geometry has been deeply reviewed. Using the CAD drawings
232       the carbon fiber frames have been simulated and radiator dimentions
233       corrected. For this reason the calibration done on the beam tests
234       has been revied and new sets of calibration constants calculated
235       comparing the beam test data with the GPAMELA results. The new
236       constants are about 3% larger than the previous ones.
237      
238    TRACKER GEOMETRY REVIEWED. NEW VOLUME DEFINED: THBP, TPAS, TPAI
239      
240       Thanks to Lorenzo Bonechi for the drawings and explanations. Now the
241       hybrd cards have been put into the simulation and the geometry updated
242       considering the dead zones in the silicon detectors. The hybrid zone
243       has been simulated as well. At the moment the hybrid is simulated as
244       a G10 plates. The full height of the tracker magnet has been
245       reviewed as well.
246    
247       The tracker ladder is now simulated inside a nitrogen box: TPAS,
248       placed inside an aluminum frame: TRPB. Each silicon ladder has been
249       simulated using two silicon blocks: TRSL, into each of this block a
250       smaller silicon detector: TPAI, has been placed inside the larger
251       silicon block TRSL. In this way the subdivided silicon ladder can
252       be upgraded with an indipendend roto-translation for each sensor.
253      
254       The TRPB aluminum frame has been enlarged to fit the external
255       magnet canister frame.
256      
257       The last plane has been flipped with a 180 degree rotation around
258       the X axis.
259      
260    TRACKER HIT STRUCTURE REVIEWED
261    
262       Taking into account the new version of the tracker geometry, the hit
263       structure for this detector has been revied.
264    
265    CALORIMETER GEOMETRY REVIEWED
266    
267       Marco Albi reviewed the calorimeter dimentions and positioning.
268    
269    
270  29 March 2004, Bari  29 March 2004, Bari
271    
272  NON-REPRODUCIBILITY PROBLEM OF A GPAMELA RUN FIXED.  NON-REPRODUCIBILITY PROBLEM OF A GPAMELA RUN FIXED.
273  The non-reproducibility of a GPAMELA run was due to the random number     The non-reproducibility of a GPAMELA run was due to the random number
274  initialization in the GARFIELD code. In GARFIELD by default, the initial     initialization in the GARFIELD code. In GARFIELD by default, the initial
275  seeds of the random number generators are always the same while the random     seeds of the random number generators are always the same while the random
276  number generators are called a given number of times (determined by the     number generators are called a given number of times (determined by the
277  hour of the day) during the initialization phase (see init.f subroutine in     hour of the day) during the initialization phase (see init.f subroutine in
278  the GARFIELD code for details). Follows that different runs produce     the GARFIELD code for details). Follows that different runs produce
279  different results without changing the initial seeds. To have identical     different results without changing the initial seeds. To have identical
280  results in different runs, the GARFIELD program has to start typing the     results in different runs, the GARFIELD program has to start typing the
281  noRNDM_initialisation switch. To avoid of specifying this switch by the user,     noRNDM_initialisation switch. To avoid of specifying this switch
282  the GARFIELD package has been upgraded with a patch. In this way the problem     by the user,
283  is partially solved because, now, the initial seeds of the random generators     the GARFIELD package has been upgraded with a patch. In this way the problem
284  in GARFIELD will be always the same even if the RNDM GEANT data card is     is partially solved because, now, the initial seeds of the random generators
285  activated by the user for changing the initial seeds in the GPAMELA program.     in GARFIELD will be always the same even if the RNDM GEANT data card is
286  Work is in progress for a more general correction of this problem.     activated by the user for changing the initial seeds in the GPAMELA program.
287  Please, use the updated GARFIELD code released with the CVS version v4r1     Work is in progress for a more general correction of this problem.
288  to fix this problem.       Please, use the updated GARFIELD code released with the CVS version v4r1
289       to fix this problem.  
290    
291    
292  RNDM ROUTINE REPLACED BY THE GRNDM ROUTINE IN GPXTR AND NPOISS.  RNDM ROUTINE REPLACED BY THE GRNDM ROUTINE IN GPXTR AND NPOISS.
293  The obsolete RNDM random number generator has been replaced by the GEANT     The obsolete RNDM random number generator has been replaced by the GEANT
294  GRNDN routine in the gpxtr.F subroutine and in the npoiss.F function.     GRNDN routine in the gpxtr.F subroutine and in the npoiss.F function.
295    
296  BUG FOUND AND FIXED: the set and detector calorimeter addresses (ISCAL  BUG FOUND AND FIXED: the set and detector calorimeter addresses (ISCAL
297  and IDCASI variables) used in GUTREV were respectively set to a fixed     and IDCASI variables) used in GUTREV were respectively set to a fixed
298  values of 12 and 1. The correct values of these variables are stored in     values of 12 and 1. The correct values of these variables are stored in
299  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
300  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
301  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
302  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.
303    
304  9 December 2003, Bari  9 December 2003, Bari
305    
306  CALORIMETER SIMULATION completed! The update of the geometry and of the     CALORIMETER SIMULATION completed! The update of the geometry and of the
307  special tracking parameters and the tuning of the calorimeter have been     special tracking parameters and the tuning of the calorimeter have been
308  successfully done. A great quantity of simulated data have been produced     successfully done. A great quantity of simulated data have been produced
309  in the calorimeter for different particles (muons, electrons and pions)     in the calorimeter for different particles (muons, electrons and pions)
310  and momenta (5 and 40 GeV/c) and the output data have been analyzed. The     and momenta (5 and 40 GeV/c) and the output data have been analyzed. The
311  distributions of the total energy deposited in the calorimeter and the     distributions of the total energy deposited in the calorimeter and the
312  total number of strips hit have been compared with the respective     total number of strips hit have been compared with the respective
313  distributions produced by the Trieste's tuned standalone Monte Carlo     distributions produced by the Trieste's tuned standalone Monte Carlo
314  simulation program of the PAMELA calorimeter. The accord between the     simulation program of the PAMELA calorimeter. The accord between the
315  two simulations is excellent. Many thanks to Mirko for his collaboration.     two simulations is excellent. Many thanks to Mirko for his collaboration.
316    
317  Working in progress on TRD. The GARFIELD interface to the HEED program is not     Working in progress on TRD. The GARFIELD interface to the HEED program is not
318  optimized to track particle with a charge greater than one and photons. The     optimized to track particle with a charge greater than one and photons. The
319  program print a warning message to advise the user when it is the case.     program print a warning message to advise the user when it is the case.
320    
321  18 April 2003, Bari  18 April 2003, Bari
322    
323  The buffer size of each column of the GPAMELA Ntuple has been increased to     The buffer size of each column of the GPAMELA Ntuple has been increased to
324  4096 and set equal to the record length, defined by a call to the HROPEN     4096 and set equal to the record length, defined by a call to the HROPEN
325  routine.     routine.
326  Also the length of the common /PAWC/ (parameter NWPAW) has been increased     Also the length of the common /PAWC/ (parameter NWPAW) has been increased
327  to 1.34E8, according to the rule that it has to be larger than the number     to 1.34E8, according to the rule that it has to be larger than the number
328  of columns times the buffer size.     of columns times the buffer size.
329    
330  10 April 2003, Bari  10 April 2003, Bari
331    
332  The variables in the HIT STRUCTURE of the CALORIMETER and their way to be     The variables in the HIT STRUCTURE of the CALORIMETER and their way to be
333  filled have been changed according to the electronics system of the real     filled have been changed according to the electronics system of the real
334  detector. In fact, because each silicon detector (module) consists of     detector. In fact, because each silicon detector (module) consists of
335  32 strips and each strip is connected to those belonging to the two detectors     32 strips and each strip is connected to those belonging to the two detectors
336  of the same row (or column) for forming 24 cm long strips, the sum of the     of the same row (or column) for forming 24 cm long strips, the sum of the
337  deposited energies in the strips forming a `long strip' is now calculated for     deposited energies in the strips forming a `long strip' is now calculated for
338  each event (gpucal.F subroutine) and it is stored in a hit only at the     each event (gpucal.F subroutine) and it is stored in a hit only at the
339  end of the event (gutrev.F subroutine).     end of the event (gutrev.F subroutine).
340  The output variables of the GPAMELA en-tuple are then filled in the vectors     The output variables of the GPAMELA en-tuple are then filled in the vectors
341  ICAPLANE(NTHCAL), ICASTRIP(NTHCAL), ENESTRIP(NTHCAL) and ICAMOD(NTHCAL),     ICAPLANE(NTHCAL), ICASTRIP(NTHCAL), ENESTRIP(NTHCAL) and ICAMOD(NTHCAL),
342  by a call to the GPDCAL subroutine:     by a call to the GPDCAL subroutine:
343  -ICAPLANE(i) contains the number of hit plane;     -ICAPLANE(i) contains the number of hit plane;
344  -ICASTRIP(i) contains the number of hit strip;     -ICASTRIP(i) contains the number of hit strip;
345  -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
346             positions in which a `long strip' has been hit.                positions in which a `long strip' has been hit.
347  -ENESTRIP(i) contains the deposited energy in the hit strip;     -ENESTRIP(i) contains the deposited energy in the hit strip;
348  where i is the number of hit (1<i<4224).     where i is the number of hit (1<i<4224).
349  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
350  that there is a hit for each `long strip' hit from     that there is a hit for each `long strip' hit from
351  the particle. This use of the hit structure is different for the other     the particle. This use of the hit structure is different for the other
352  detectors and it has been considered to avoid a too big number of hit in the     detectors and it has been considered to avoid a too big number of hit in the
353  calorimeter due to the showers. Follows that NTHCAL, which is the     calorimeter due to the showers. Follows that NTHCAL, which is the
354  max number of hit in the calorimeter, is equal to 4224, the total     max number of hit in the calorimeter, is equal to 4224, the total
355  number of `long strips'. So, for each event, the real number of hit will     number of `long strips'. So, for each event, the real number of hit will
356  be less or equal to 4224.     be less or equal to 4224.
357  ICAMOD(i) is an additional information that does not exist in the real     ICAMOD(i) is an additional information that does not exist in the real
358  detector: if the strip i (i=1,32) of the module 1 or 2 or 3     detector: if the strip i (i=1,32) of the module 1 or 2 or 3
359  is hit, the value of ICAMOD(i) is respectively incremented of 1, 100, 10000.     is hit, the value of ICAMOD(i) is respectively incremented of 1, 100, 10000.
360  Analogously it is done, if it is the strip j (j=33,64) of the modules 4, 5     Analogously it is done, if it is the strip j (j=33,64) of the modules 4, 5
361  and 6 or if it is the strip k (k=65,96) of the modules 7, 8 and 9.     and 6 or if it is the strip k (k=65,96) of the modules 7, 8 and 9.
362  For example if we consider the hit 1 of an event, we could read:     For example if we consider the hit 1 of an event, we could read:
363  ICASTRIP(1)=30, ICAPLANE(1)=21, ENESTRIP(1)=0.5E-03 and ICAMOD(1)=10001.     ICASTRIP(1)=30, ICAPLANE(1)=21, ENESTRIP(1)=0.5E-03 and ICAMOD(1)=10001.
364  It means that the hit 1 contains the information that in the strip 30 of the     It means that the hit 1 contains the information that in the strip 30 of the
365  plane 21 has been deposited a total energy of 0.5E-03 GeV. In addition the     plane 21 has been deposited a total energy of 0.5E-03 GeV. In addition the
366  `long strip 30' has been hit two times, one in the first module and the     `long strip 30' has been hit two times, one in the first module and the
367  other in the third one.     other in the third one.
368    
369  The energy deposited in the calorimeter is calculated in GeV.     The energy deposited in the calorimeter is calculated in GeV.
370    
371  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
372  GSCHIT.     GSCHIT.
373    
374  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
375  of a call to the GFHITS subroutine.     of a call to the GFHITS subroutine.
376    
377  25 February 2003, Bari  25 February 2003, Bari
378    
379  BUG found:  BUG found:
380  DCUTEAER, DCUTEAL, DCUTECE, DCUTECP, DCUTEFE, DCUTEG10C, DCUTEG10, DCUTEKAP,     DCUTEAER, DCUTEAL, DCUTECE, DCUTECP, DCUTEFE, DCUTEG10C, DCUTEG10, DCUTEKAP,
381  DCUTEN2G, DCUTEROA, DCUTESCIN, DCUTESICA, DCUTETRAD, DCUTEW2,     DCUTEN2G, DCUTEROA, DCUTESCIN, DCUTESICA, DCUTETRAD, DCUTEW2,
382  DCUTEW, DCUTEXE variables missed in the commons: gpaer.inc, gpal.inc, gpce.inc,     DCUTEW, DCUTEXE variables missed in the commons: gpaer.inc, gpal.inc, gpce.inc,
383  gpcp.inc, gpfe.inc, gpg10c.inc, gpg10.inc, gpkap.inc, gpn2g.inc, gproa.inc,     gpcp.inc, gpfe.inc, gpg10c.inc, gpg10.inc, gpkap.inc, gpn2g.inc, gproa.inc,
384  gpscin.inc (obsolete), gpscint.inc, gpsica.inc, gptrad.inc, gpw2.inc, gpw.inc,     gpscin.inc (obsolete), gpscint.inc, gpsica.inc, gptrad.inc, gpw2.inc, gpw.inc,
385  gpxe.inc, gpdaer.inc, gpdal.inc, gpdce.inc, gpdcp.inc, gpdfe.inc, gpdg10c.inc,     gpxe.inc, gpdaer.inc, gpdal.inc, gpdce.inc, gpdcp.inc, gpdfe.inc, gpdg10c.inc,
386  gpdg10.inc, gpdkap.inc, gpdn2g.inc, gpdroa.inc, gpdscin.inc, gpdsica.inc,     gpdg10.inc, gpdkap.inc, gpdn2g.inc, gpdroa.inc, gpdscin.inc, gpdsica.inc,
387  gpdtrad.inc, gpdw2.inc, gpdw.inc, gpdxe.inc.     gpdtrad.inc, gpdw2.inc, gpdw.inc, gpdxe.inc.
388  They have been added in these commons and they have been initialized in the     They have been added in these commons and they have been initialized in the
389  GPSTM subroutine.     GPSTM subroutine.
390    
391  Updated the special tracking parameters SICALO, TUNGA, KAOLINITE and G10C     Updated the special tracking parameters SICALO, TUNGA, KAOLINITE and G10C
392  in the subroutines gpsica.F, gpw2.F, gpw.F, gpce.F and gpg10c.F. They were     in the subroutines gpsica.F, gpw2.F, gpw.F, gpce.F and gpg10c.F. They were
393  suggested by Mirko Boezio.     suggested by Mirko Boezio.
394    
395  Updated the value of the absorption length for silicon in the calorimeter     Updated the value of the absorption length for silicon in the calorimeter
396  and tracker although this parameter is ignored by GEANT. For this reason     and tracker although this parameter is ignored by GEANT. For this reason
397  it was equal to the radiation length.     it was equal to the radiation length.
398    
399  Updated the relative positions of the calorimeter planes. The corrected     Updated the relative positions of the calorimeter planes. The corrected
400  shifting are:     shifting are:
401    
402  first view: (Dxo,Dyo)=(0.10,0.05) cm     first view: (Dxo,Dyo)=(0.10,0.05) cm
403  second view: (Dxo,Dyo)=(-0.05,0.10) cm     second view: (Dxo,Dyo)=(-0.05,0.10) cm
404  third view: (Dxo,Dyo)=(-0.10,-0.05) cm     third view: (Dxo,Dyo)=(-0.10,-0.05) cm
405  fourth view: (Dxo,Dyo)=(0.05,-0.10) cm     fourth view: (Dxo,Dyo)=(0.05,-0.10) cm
406    
407  4 November 2002, Bari  4 November 2002, Bari
408    
409  CAS detectors distances modified  CAS detectors distances modified
410    
411  The distances between the CAS detectors have been modified based on the     The distances between the CAS detectors have been modified based on the
412  latest CAD drawings.     latest CAD drawings.
413    
414  2 November 2002, Bari  2 November 2002, Bari
415    
416  CALORIMETER geometry upgrade  CALORIMETER geometry upgrade
417    
418  The volumes CAPD and CAAD have been taken off from the calorimeter.     The volumes CAPD and CAAD have been taken off from the calorimeter.
419  In addition the logical tree has been slightly changed to make the shifts of     In addition the logical tree has been slightly changed to make the shifts of
420  the silicon planes into the calorimeter box easier, i.e. the CAPL volume,     the silicon planes into the calorimeter box easier, i.e. the CAPL volume,
421  which was made of the CASI, CAKP, CAGL, C10C and CAKA volumes, has     which was made of the CASI, CAKP, CAGL, C10C and CAKA volumes, has
422  been split up in the volumes CANS and CAPL. Now CANS is made of the CAKP,     been split up in the volumes CANS and CAPL. Now CANS is made of the CAKP,
423  CAGL, C10C and CAKA volumes while CAPL contains the CASI volume, that has to     CAGL, C10C and CAKA volumes while CAPL contains the CASI volume, that has to
424  be shifted as a function of the vertical position in the calorimeter. Also the     be shifted as a function of the vertical position in the calorimeter. Also the
425  dimensions of some volumes have been upgraded, including the external ones:     dimensions of some volumes have been upgraded, including the external ones:
426  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,
427  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
428  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
429  a reliable description of the event in the S4 scintillator.     a reliable description of the event in the S4 scintillator.
430    
431  22 October 2002, Stockholm  22 October 2002, Stockholm
432    

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