1 |
# |
# |
2 |
# $Id: v_100.txt,v 3.3 2002/12/05 17:27:59 pamela Exp $ |
# $Id: v_100.txt,v 3.6 2005/07/25 11:53:21 cafagna Exp $ |
3 |
# |
# |
4 |
# $Log: v_100.txt,v $ |
# $Log: v_100.txt,v $ |
5 |
|
# Revision 3.6 2005/07/25 11:53:21 cafagna |
6 |
|
# Several updates. See history for details |
7 |
|
# |
8 |
|
# Revision 3.5 2004/04/06 10:33:46 pamela |
9 |
|
# NON-REPRODUCIBILITY problem of a GPAMELA RUN fixed; bug found and fixed filling in the hit structure of the calorimeter |
10 |
|
# |
11 |
|
# Revision 3.4 2003/12/17 11:32:50 pamela |
12 |
|
# CALO SIMULATION COMPLETED: geometry and special tracking parameters updated and simulation checked by a comparison with the Trieste's standalone Monte Carlo simulation |
13 |
|
# |
14 |
# Revision 3.3 2002/12/05 17:27:59 pamela |
# Revision 3.3 2002/12/05 17:27:59 pamela |
15 |
# New GARFIELD.GAR file added and GPAMELA.FFR cleaned and updated |
# New GARFIELD.GAR file added and GPAMELA.FFR cleaned and updated |
16 |
# |
# |
32 |
#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 |
33 |
#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 |
34 |
#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 |
35 |
#-- Author : Francesco Cafagna 28/11/95 |
#-- Author : Francesco Cafagna 28/11/95 |
36 |
|
|
37 |
|
May 2005, Bari |
38 |
|
|
39 |
|
Some updates on the latest modification done in the past year. |
40 |
|
|
41 |
|
NEW DATA CARD ADDED: HFSF |
42 |
|
|
43 |
|
To define a policy for the random number initial seeds |
44 |
|
definition. Using this card is possible to override GEANT seeds |
45 |
|
defined via NRDM card. The policy is selected according to the |
46 |
|
values: |
47 |
|
|
48 |
|
- 1: The seeds are initialized to the initial values found in a user |
49 |
|
defined file or the default file: INPUTSEED.DAT |
50 |
|
|
51 |
|
- 2: The seeds are initialized to the final values found in a user defined |
52 |
|
file or the default file: INPUTSEED.DAT |
53 |
|
|
54 |
|
The case 1 must be used in case the user needs to reproduce the |
55 |
|
random chain of a previous run. In this case the user can save the |
56 |
|
initial seeds, used in the run he would like to reproduce, in a |
57 |
|
binary file and pass the filename to the program using the *FLSF |
58 |
|
data card. In case the user file is not specified the default |
59 |
|
INPUTSEED.DAT will be used. |
60 |
|
|
61 |
|
The case 2 must be used in case the user needs to chain several |
62 |
|
GPAMELA run and likes to be sure he is starting the random |
63 |
|
generator using the right sequence. In this case the user must |
64 |
|
specify an input binary file using the *FLSF data card, otherwise |
65 |
|
the INPUTSEED.DAT file will be used. |
66 |
|
|
67 |
|
NEW DATA CARD ADDED: *FSFI |
68 |
|
|
69 |
|
Using this card the user can specify the logical unit and name of |
70 |
|
the file storing the initial seeds to be used to initialize the |
71 |
|
random number generator. This file must be a FORTRAN binary one |
72 |
|
storing four integer numbers. The first two are the number to be |
73 |
|
used in the case: HFSF=1, the other two will be used in the case: |
74 |
|
HFSF=2. This file can be one created by GPAMELA or by the user |
75 |
|
filled with his own seeds. For this purpose an utility program: |
76 |
|
writeseeds.f, has been added in the aux directory. In case the |
77 |
|
*FSFI card is not specified the default values: 24 and INPUTSEEDS.DAT, will |
78 |
|
be used as LUN and file name respectively. |
79 |
|
|
80 |
|
NEW DATA CARD ADDED: *LSFI |
81 |
|
|
82 |
|
Using this card the user can specify the logical unit and name of |
83 |
|
the file storing the first and last seeds used in the GPAMELA |
84 |
|
run. This file is a FORTRAN binary one. This file can be used as |
85 |
|
input one specifying it in the *FSFI data card of the next GPAMELA |
86 |
|
run. In case the *LSFI card is not specified the default values: 26 |
87 |
|
and HBOOKFILENAME.DAT (as sepified in *HFI), will be used as LUN |
88 |
|
and file name respectively. |
89 |
|
|
90 |
|
NEW UTILITY PROGRAMS ADDED: writeseeds.f, readseeds.f |
91 |
|
|
92 |
|
These new programs have been added in the aux directory. Using these a |
93 |
|
user defined seed file can be created and re-read. |
94 |
|
|
95 |
|
NEW VOLUMES ADDED: MSHE, BSPH; PRESSURIZED CONTAINER ADDED |
96 |
|
|
97 |
|
Alexey Bakaldin, in MEPHI, did add the PAMELA pressurized container to |
98 |
|
the simulation. He did defined new volumes filled with aluminum and |
99 |
|
placed inside the mother volume. Positions have been fine tuned by |
100 |
|
Marialuigia Ambriola and compared to the CAD drawings. |
101 |
|
Two new volumes have been added to simulate the container: |
102 |
|
- MSHE, a tube simulating the middle part of the container |
103 |
|
- BSPH, the spherical bottom part of the container |
104 |
|
|
105 |
|
To better simulate the upper part the SHEL volume has been modified |
106 |
|
into a cone. Dimentions of the top cover: TSPH, have been modified |
107 |
|
accordingly. |
108 |
|
|
109 |
|
DETECTOR POSITIONS REVIEWED |
110 |
|
|
111 |
|
All detector Z positions have been reviewd to fit into the |
112 |
|
simulated pressurized container. |
113 |
|
|
114 |
|
TRD GEOMETRY AND CALIBRATION REVIEWD |
115 |
|
|
116 |
|
The TRD geometry has been deeply reviewed. Using the CAD drawings |
117 |
|
the carbon fiber frames have been simulated and radiator dimentions |
118 |
|
corrected. For this reason the calibration done on the beam tests |
119 |
|
has been revied and new sets of calibration constants calculated |
120 |
|
comparing the beam test data with the GPAMELA results. The new |
121 |
|
constants are about 3% larger than the previous ones. |
122 |
|
|
123 |
|
TRACKER GEOMETRY REVIEWED. NEW VOLUME DEFINED: THBP, TPAS, TPAI |
124 |
|
|
125 |
|
Thanks to Lorenzo Bonechi for the drawings and explanations. Now the |
126 |
|
hybrd cards have been put into the simulation and the geometry updated |
127 |
|
considering the dead zones in the silicon detectors. The hybrid zone |
128 |
|
has been simulated as well. At the moment the hybrid is simulated as |
129 |
|
a G10 plates. The full height of the tracker magnet has been |
130 |
|
reviewed as well. |
131 |
|
|
132 |
|
The tracker ladder is now simulated inside a nitrogen box: TPAS, |
133 |
|
placed inside an aluminum frame: TRPB. Each silicon ladder has been |
134 |
|
simulated using two silicon blocks: TRSL, into each of this block a |
135 |
|
smaller silicon detector: TPAI, has been placed inside the larger |
136 |
|
silicon block TRSL. In this way the subdivided silicon ladder can |
137 |
|
be upgraded with an indipendend roto-translation for each sensor. |
138 |
|
|
139 |
|
The TRPB aluminum frame has been enlarged to fit the external |
140 |
|
magnet canister frame. |
141 |
|
|
142 |
|
The last plane has been flipped with a 180 degree rotation around |
143 |
|
the X axis. |
144 |
|
|
145 |
|
TRACKER HIT STRUCTURE REVIEWED |
146 |
|
|
147 |
|
Taking into account the new version of the tracker geometry, the hit |
148 |
|
structure for this detector has been revied. |
149 |
|
|
150 |
|
CALORIMETER GEOMETRY REVIEWED |
151 |
|
|
152 |
|
Marco Albi reviewed the calorimeter dimentions and positioning. |
153 |
|
|
154 |
|
|
155 |
|
29 March 2004, Bari |
156 |
|
|
157 |
|
NON-REPRODUCIBILITY PROBLEM OF A GPAMELA RUN FIXED. |
158 |
|
The non-reproducibility of a GPAMELA run was due to the random number |
159 |
|
initialization in the GARFIELD code. In GARFIELD by default, the initial |
160 |
|
seeds of the random number generators are always the same while the random |
161 |
|
number generators are called a given number of times (determined by the |
162 |
|
hour of the day) during the initialization phase (see init.f subroutine in |
163 |
|
the GARFIELD code for details). Follows that different runs produce |
164 |
|
different results without changing the initial seeds. To have identical |
165 |
|
results in different runs, the GARFIELD program has to start typing the |
166 |
|
noRNDM_initialisation switch. To avoid of specifying this switch |
167 |
|
by the user, |
168 |
|
the GARFIELD package has been upgraded with a patch. In this way the problem |
169 |
|
is partially solved because, now, the initial seeds of the random generators |
170 |
|
in GARFIELD will be always the same even if the RNDM GEANT data card is |
171 |
|
activated by the user for changing the initial seeds in the GPAMELA program. |
172 |
|
Work is in progress for a more general correction of this problem. |
173 |
|
Please, use the updated GARFIELD code released with the CVS version v4r1 |
174 |
|
to fix this problem. |
175 |
|
|
176 |
|
|
177 |
|
RNDM ROUTINE REPLACED BY THE GRNDM ROUTINE IN GPXTR AND NPOISS. |
178 |
|
The obsolete RNDM random number generator has been replaced by the GEANT |
179 |
|
GRNDN routine in the gpxtr.F subroutine and in the npoiss.F function. |
180 |
|
|
181 |
|
BUG FOUND AND FIXED: the set and detector calorimeter addresses (ISCAL |
182 |
|
and IDCASI variables) used in GUTREV were respectively set to a fixed |
183 |
|
values of 12 and 1. The correct values of these variables are stored in |
184 |
|
the GPSED common when the set and the detector ZEBRA banks are filled |
185 |
|
during a run. In general the values of the set and detector addresses |
186 |
|
depend on the number of active detectors in a given run. ISCAL=12 and |
187 |
|
IDCASI=1 are only right when all the detectors of GPAMELA are active. |
188 |
|
|
189 |
9 December 2003, Bari |
9 December 2003, Bari |
190 |
|
|
191 |
CALORIMETER SIMULATION completed! The update of the geometry and of the |
CALORIMETER SIMULATION completed! The update of the geometry and of the |
192 |
special tracking parameters and the tuning of the calorimeter have been |
special tracking parameters and the tuning of the calorimeter have been |
193 |
successfully done. A great quantity of simulated data have been produced |
successfully done. A great quantity of simulated data have been produced |
194 |
in the calorimeter for different particles (muons, electrons and pions) |
in the calorimeter for different particles (muons, electrons and pions) |
195 |
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 |
196 |
distributions of the total energy deposited in the calorimeter and the |
distributions of the total energy deposited in the calorimeter and the |
197 |
total number of strips hit have been compared with the respective |
total number of strips hit have been compared with the respective |
198 |
distributions produced by the Trieste's tuned standalone Monte Carlo |
distributions produced by the Trieste's tuned standalone Monte Carlo |
199 |
simulation program of the PAMELA calorimeter. The accord between the |
simulation program of the PAMELA calorimeter. The accord between the |
200 |
two simulations is excellent. Many thanks to Mirko for his collaboration. |
two simulations is excellent. Many thanks to Mirko for his collaboration. |
201 |
|
|
202 |
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 |
203 |
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 |
204 |
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. |
205 |
|
|
206 |
18 April 2003, Bari |
18 April 2003, Bari |
207 |
|
|
208 |
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 |
209 |
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 |
210 |
routine. |
routine. |
211 |
Also the length of the common /PAWC/ (parameter NWPAW) has been increased |
Also the length of the common /PAWC/ (parameter NWPAW) has been increased |
212 |
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 |
213 |
of columns times the buffer size. |
of columns times the buffer size. |
214 |
|
|
215 |
10 April 2003, Bari |
10 April 2003, Bari |
216 |
|
|
217 |
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 |
218 |
filled have been changed according to the electronics system of the real |
filled have been changed according to the electronics system of the real |
219 |
detector. In fact, because each silicon detector (module) consists of |
detector. In fact, because each silicon detector (module) consists of |
220 |
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 |
221 |
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 |
222 |
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 |
223 |
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 |
224 |
end of the event (gutrev.F subroutine). |
end of the event (gutrev.F subroutine). |
225 |
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 |
226 |
ICAPLANE(NTHCAL), ICASTRIP(NTHCAL), ENESTRIP(NTHCAL) and ICAMOD(NTHCAL), |
ICAPLANE(NTHCAL), ICASTRIP(NTHCAL), ENESTRIP(NTHCAL) and ICAMOD(NTHCAL), |
227 |
by a call to the GPDCAL subroutine: |
by a call to the GPDCAL subroutine: |
228 |
-ICAPLANE(i) contains the number of hit plane; |
-ICAPLANE(i) contains the number of hit plane; |
229 |
-ICASTRIP(i) contains the number of hit strip; |
-ICASTRIP(i) contains the number of hit strip; |
230 |
-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 |
231 |
positions in which a `long strip' has been hit. |
positions in which a `long strip' has been hit. |
232 |
-ENESTRIP(i) contains the deposited energy in the hit strip; |
-ENESTRIP(i) contains the deposited energy in the hit strip; |
233 |
where i is the number of hit (1<i<4224). |
where i is the number of hit (1<i<4224). |
234 |
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 |
235 |
that there is a hit for each `long strip' hit from |
that there is a hit for each `long strip' hit from |
236 |
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 |
237 |
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 |
238 |
calorimeter due to the showers. Follows that NTHCAL, which is the |
calorimeter due to the showers. Follows that NTHCAL, which is the |
239 |
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 |
240 |
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 |
241 |
be less or equal to 4224. |
be less or equal to 4224. |
242 |
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 |
243 |
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 |
244 |
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. |
245 |
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 |
246 |
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. |
247 |
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: |
248 |
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. |
249 |
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 |
250 |
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 |
251 |
`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 |
252 |
other in the third one. |
other in the third one. |
253 |
|
|
254 |
The energy deposited in the calorimeter is calculated in GeV. |
The energy deposited in the calorimeter is calculated in GeV. |
255 |
|
|
256 |
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 |
257 |
GSCHIT. |
GSCHIT. |
258 |
|
|
259 |
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 |
260 |
of a call to the GFHITS subroutine. |
of a call to the GFHITS subroutine. |
261 |
|
|
262 |
25 February 2003, Bari |
25 February 2003, Bari |
263 |
|
|
264 |
BUG found: |
BUG found: |
265 |
DCUTEAER, DCUTEAL, DCUTECE, DCUTECP, DCUTEFE, DCUTEG10C, DCUTEG10, DCUTEKAP, |
DCUTEAER, DCUTEAL, DCUTECE, DCUTECP, DCUTEFE, DCUTEG10C, DCUTEG10, DCUTEKAP, |
266 |
DCUTEN2G, DCUTEROA, DCUTESCIN, DCUTESICA, DCUTETRAD, DCUTEW2, |
DCUTEN2G, DCUTEROA, DCUTESCIN, DCUTESICA, DCUTETRAD, DCUTEW2, |
267 |
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, |
268 |
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, |
269 |
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, |
270 |
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, |
271 |
gpdg10.inc, gpdkap.inc, gpdn2g.inc, gpdroa.inc, gpdscin.inc, gpdsica.inc, |
gpdg10.inc, gpdkap.inc, gpdn2g.inc, gpdroa.inc, gpdscin.inc, gpdsica.inc, |
272 |
gpdtrad.inc, gpdw2.inc, gpdw.inc, gpdxe.inc. |
gpdtrad.inc, gpdw2.inc, gpdw.inc, gpdxe.inc. |
273 |
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 |
274 |
GPSTM subroutine. |
GPSTM subroutine. |
275 |
|
|
276 |
Updated the special tracking parameters SICALO, TUNGA, KAOLINITE and G10C |
Updated the special tracking parameters SICALO, TUNGA, KAOLINITE and G10C |
277 |
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 |
278 |
suggested by Mirko Boezio. |
suggested by Mirko Boezio. |
279 |
|
|
280 |
Updated the value of the absorption length for silicon in the calorimeter |
Updated the value of the absorption length for silicon in the calorimeter |
281 |
and tracker although this parameter is ignored by GEANT. For this reason |
and tracker although this parameter is ignored by GEANT. For this reason |
282 |
it was equal to the radiation length. |
it was equal to the radiation length. |
283 |
|
|
284 |
Updated the relative positions of the calorimeter planes. The corrected |
Updated the relative positions of the calorimeter planes. The corrected |
285 |
shifting are: |
shifting are: |
286 |
|
|
287 |
first view: (Dxo,Dyo)=(0.10,0.05) cm |
first view: (Dxo,Dyo)=(0.10,0.05) cm |
288 |
second view: (Dxo,Dyo)=(-0.05,0.10) cm |
second view: (Dxo,Dyo)=(-0.05,0.10) cm |
289 |
third view: (Dxo,Dyo)=(-0.10,-0.05) cm |
third view: (Dxo,Dyo)=(-0.10,-0.05) cm |
290 |
fourth view: (Dxo,Dyo)=(0.05,-0.10) cm |
fourth view: (Dxo,Dyo)=(0.05,-0.10) cm |
291 |
|
|
292 |
4 November 2002, Bari |
4 November 2002, Bari |
293 |
|
|
294 |
CAS detectors distances modified |
CAS detectors distances modified |
295 |
|
|
296 |
The distances between the CAS detectors have been modified based on the |
The distances between the CAS detectors have been modified based on the |
297 |
latest CAD drawings. |
latest CAD drawings. |
298 |
|
|
299 |
2 November 2002, Bari |
2 November 2002, Bari |
300 |
|
|
301 |
CALORIMETER geometry upgrade |
CALORIMETER geometry upgrade |
302 |
|
|
303 |
The volumes CAPD and CAAD have been taken off from the calorimeter. |
The volumes CAPD and CAAD have been taken off from the calorimeter. |
304 |
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 |
305 |
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, |
306 |
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 |
307 |
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, |
308 |
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 |
309 |
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 |
310 |
dimensions of some volumes have been upgraded, including the external ones: |
dimensions of some volumes have been upgraded, including the external ones: |
311 |
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, |
312 |
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 |
313 |
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 |
314 |
a reliable description of the event in the S4 scintillator. |
a reliable description of the event in the S4 scintillator. |
315 |
|
|
316 |
22 October 2002, Stockholm |
22 October 2002, Stockholm |
317 |
|
|