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Influence of polystyrene scintillator strip methods of production on their main characteristics

Identifieur interne : 000239 ( PascalFrancis/Curation ); précédent : 000238; suivant : 000240

Influence of polystyrene scintillator strip methods of production on their main characteristics

Auteurs : V. Senchyshyn [Ukraine] ; B. Grynyov [Ukraine] ; S. Melnychuk [Ukraine] ; V. Lagutin [Ukraine] ; M. Dracos [France] ; A. Olchevski [Russie] ; Y. Gornushkin [Russie] ; A. Nozdrin [Russie] ; A. Sadovski [Russie]

Source :

RBID : Pascal:07-0470728

Descripteurs français

English descriptors

Abstract

The baseline option for Target Tracker of OPERA detector is plastic scintillator strips, 6.7m length, read with wavelength shifting (WLS) fiber. Usually such strips are supposed to be obtained by extrusion from pellets. Despite many advantages of extrusion process the strips extruded from pellet strips have low attenuation length (BAL = 20-40cm) and low yield (LY). The main idea of our new method was to obtain scintillator using extrusion method but from the melt of specially polymerized plastic. Pilot setup was created and pilot batch for OPERA prototype was obtained with the 10kg/h productivity. Still, for mass production there was a necessity to adapt the production scheme and to manage quality assurance and quality control system. During mass production of scintillator strips for OPERA detector we have implemented all obtained results into production process. And we have carefully studied their influence on strip quality. The achieved average light yield is 7.2 ph.el. for OPERA strips.
pA  
A01 01  1    @0 1350-4487
A03   1    @0 Radiat. meas.
A05       @2 42
A06       @2 4-5
A08 01  1  ENG  @1 Influence of polystyrene scintillator strip methods of production on their main characteristics
A09 01  1  ENG  @1 Proceedings of the 6th European Conference on Luminescent Detectors and Transformers of Ionizing Radiation (LUMDETR 2006)
A11 01  1    @1 SENCHYSHYN (V.)
A11 02  1    @1 GRYNYOV (B.)
A11 03  1    @1 MELNYCHUK (S.)
A11 04  1    @1 LAGUTIN (V.)
A11 05  1    @1 DRACOS (M.)
A11 06  1    @1 OLCHEVSKI (A.)
A11 07  1    @1 GORNUSHKIN (Y.)
A11 08  1    @1 NOZDRIN (A.)
A11 09  1    @1 SADOVSKI (A.)
A12 01  1    @1 VAKARCHUK (Ivan) @9 ed.
A12 02  1    @1 GRINYOV (Boris) @9 ed.
A14 01      @1 Institute for Scintillation Materials, STC "Institute for Single Crystals" NAS of Ukraine, Lenin Av @2 60 Kharkov @3 UKR @Z 1 aut. @Z 2 aut. @Z 3 aut. @Z 4 aut.
A14 02      @1 IReS, 23 rue du Loess @2 67037 Strasbourg @3 FRA @Z 5 aut.
A14 03      @1 JINR, 6 Joliot-Curie @2 14198, Dubna, Moscow region @3 RUS @Z 6 aut. @Z 7 aut. @Z 8 aut. @Z 9 aut.
A20       @1 911-914
A21       @1 2007
A23 01      @0 ENG
A43 01      @1 INIST @2 17536 @5 354000149759170970
A44       @0 0000 @1 © 2007 INIST-CNRS. All rights reserved.
A45       @0 1/4 p.
A47 01  1    @0 07-0470728
A60       @1 P @2 C
A61       @0 A
A64 01  1    @0 Radiation measurements
A66 01      @0 GBR
C01 01    ENG  @0 The baseline option for Target Tracker of OPERA detector is plastic scintillator strips, 6.7m length, read with wavelength shifting (WLS) fiber. Usually such strips are supposed to be obtained by extrusion from pellets. Despite many advantages of extrusion process the strips extruded from pellet strips have low attenuation length (BAL = 20-40cm) and low yield (LY). The main idea of our new method was to obtain scintillator using extrusion method but from the melt of specially polymerized plastic. Pilot setup was created and pilot batch for OPERA prototype was obtained with the 10kg/h productivity. Still, for mass production there was a necessity to adapt the production scheme and to manage quality assurance and quality control system. During mass production of scintillator strips for OPERA detector we have implemented all obtained results into production process. And we have carefully studied their influence on strip quality. The achieved average light yield is 7.2 ph.el. for OPERA strips.
C02 01  2    @0 001E01C02
C02 02  2    @0 220C02
C03 01  2  FRE  @0 Ligne base @5 01
C03 01  2  ENG  @0 baseline @5 01
C03 02  2  FRE  @0 Longueur onde @5 02
C03 02  2  ENG  @0 wavelength @5 02
C03 03  2  FRE  @0 Atténuation @5 04
C03 03  2  ENG  @0 attenuation @5 04
C03 03  2  SPA  @0 Atenuación @5 04
C03 04  2  FRE  @0 Méthode nouvelle @5 05
C03 04  2  ENG  @0 new methods @5 05
C03 04  2  SPA  @0 Método nuevo @5 05
C03 05  2  FRE  @0 Productivité @5 07
C03 05  2  ENG  @0 productivity @5 07
C03 05  2  SPA  @0 Productividad @5 07
C03 06  2  FRE  @0 Contrôle qualité @5 09
C03 06  2  ENG  @0 quality controls @5 09
C03 06  2  SPA  @0 Control calidad @5 09
C03 07  2  FRE  @0 Scintillation @5 10
C03 07  2  ENG  @0 scintillations @5 10
C03 08  2  FRE  @0 Scintillateur @4 INC @5 52
C03 09  2  FRE  @0 Polystyrène @4 INC @5 53
C03 10  2  FRE  @0 Styrène polymère @4 INC @5 54
C03 11  2  FRE  @0 Détecteur @4 INC @5 55
C03 12  2  FRE  @0 OPERA @4 INC @5 56
N21       @1 309
N44 01      @1 PSI
N82       @1 PSI
pR  
A30 01  1  ENG  @1 LUMDETR 2006 : European Conference on Luminescent Detectors and Transformers of Ionizing Radiation @2 6 @3 Lviv UKR @4 2006-06-19

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Pascal:07-0470728

Le document en format XML

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<div type="abstract" xml:lang="en">The baseline option for Target Tracker of OPERA detector is plastic scintillator strips, 6.7m length, read with wavelength shifting (WLS) fiber. Usually such strips are supposed to be obtained by extrusion from pellets. Despite many advantages of extrusion process the strips extruded from pellet strips have low attenuation length (BAL = 20-40cm) and low yield (LY). The main idea of our new method was to obtain scintillator using extrusion method but from the melt of specially polymerized plastic. Pilot setup was created and pilot batch for OPERA prototype was obtained with the 10kg/h productivity. Still, for mass production there was a necessity to adapt the production scheme and to manage quality assurance and quality control system. During mass production of scintillator strips for OPERA detector we have implemented all obtained results into production process. And we have carefully studied their influence on strip quality. The achieved average light yield is 7.2 ph.el. for OPERA strips.</div>
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<s0>1/4 p.</s0>
</fA45>
<fA47 i1="01" i2="1">
<s0>07-0470728</s0>
</fA47>
<fA60>
<s1>P</s1>
<s2>C</s2>
</fA60>
<fA61>
<s0>A</s0>
</fA61>
<fA64 i1="01" i2="1">
<s0>Radiation measurements</s0>
</fA64>
<fA66 i1="01">
<s0>GBR</s0>
</fA66>
<fC01 i1="01" l="ENG">
<s0>The baseline option for Target Tracker of OPERA detector is plastic scintillator strips, 6.7m length, read with wavelength shifting (WLS) fiber. Usually such strips are supposed to be obtained by extrusion from pellets. Despite many advantages of extrusion process the strips extruded from pellet strips have low attenuation length (BAL = 20-40cm) and low yield (LY). The main idea of our new method was to obtain scintillator using extrusion method but from the melt of specially polymerized plastic. Pilot setup was created and pilot batch for OPERA prototype was obtained with the 10kg/h productivity. Still, for mass production there was a necessity to adapt the production scheme and to manage quality assurance and quality control system. During mass production of scintillator strips for OPERA detector we have implemented all obtained results into production process. And we have carefully studied their influence on strip quality. The achieved average light yield is 7.2 ph.el. for OPERA strips.</s0>
</fC01>
<fC02 i1="01" i2="2">
<s0>001E01C02</s0>
</fC02>
<fC02 i1="02" i2="2">
<s0>220C02</s0>
</fC02>
<fC03 i1="01" i2="2" l="FRE">
<s0>Ligne base</s0>
<s5>01</s5>
</fC03>
<fC03 i1="01" i2="2" l="ENG">
<s0>baseline</s0>
<s5>01</s5>
</fC03>
<fC03 i1="02" i2="2" l="FRE">
<s0>Longueur onde</s0>
<s5>02</s5>
</fC03>
<fC03 i1="02" i2="2" l="ENG">
<s0>wavelength</s0>
<s5>02</s5>
</fC03>
<fC03 i1="03" i2="2" l="FRE">
<s0>Atténuation</s0>
<s5>04</s5>
</fC03>
<fC03 i1="03" i2="2" l="ENG">
<s0>attenuation</s0>
<s5>04</s5>
</fC03>
<fC03 i1="03" i2="2" l="SPA">
<s0>Atenuación</s0>
<s5>04</s5>
</fC03>
<fC03 i1="04" i2="2" l="FRE">
<s0>Méthode nouvelle</s0>
<s5>05</s5>
</fC03>
<fC03 i1="04" i2="2" l="ENG">
<s0>new methods</s0>
<s5>05</s5>
</fC03>
<fC03 i1="04" i2="2" l="SPA">
<s0>Método nuevo</s0>
<s5>05</s5>
</fC03>
<fC03 i1="05" i2="2" l="FRE">
<s0>Productivité</s0>
<s5>07</s5>
</fC03>
<fC03 i1="05" i2="2" l="ENG">
<s0>productivity</s0>
<s5>07</s5>
</fC03>
<fC03 i1="05" i2="2" l="SPA">
<s0>Productividad</s0>
<s5>07</s5>
</fC03>
<fC03 i1="06" i2="2" l="FRE">
<s0>Contrôle qualité</s0>
<s5>09</s5>
</fC03>
<fC03 i1="06" i2="2" l="ENG">
<s0>quality controls</s0>
<s5>09</s5>
</fC03>
<fC03 i1="06" i2="2" l="SPA">
<s0>Control calidad</s0>
<s5>09</s5>
</fC03>
<fC03 i1="07" i2="2" l="FRE">
<s0>Scintillation</s0>
<s5>10</s5>
</fC03>
<fC03 i1="07" i2="2" l="ENG">
<s0>scintillations</s0>
<s5>10</s5>
</fC03>
<fC03 i1="08" i2="2" l="FRE">
<s0>Scintillateur</s0>
<s4>INC</s4>
<s5>52</s5>
</fC03>
<fC03 i1="09" i2="2" l="FRE">
<s0>Polystyrène</s0>
<s4>INC</s4>
<s5>53</s5>
</fC03>
<fC03 i1="10" i2="2" l="FRE">
<s0>Styrène polymère</s0>
<s4>INC</s4>
<s5>54</s5>
</fC03>
<fC03 i1="11" i2="2" l="FRE">
<s0>Détecteur</s0>
<s4>INC</s4>
<s5>55</s5>
</fC03>
<fC03 i1="12" i2="2" l="FRE">
<s0>OPERA</s0>
<s4>INC</s4>
<s5>56</s5>
</fC03>
<fN21>
<s1>309</s1>
</fN21>
<fN44 i1="01">
<s1>PSI</s1>
</fN44>
<fN82>
<s1>PSI</s1>
</fN82>
</pA>
<pR>
<fA30 i1="01" i2="1" l="ENG">
<s1>LUMDETR 2006 : European Conference on Luminescent Detectors and Transformers of Ionizing Radiation</s1>
<s2>6</s2>
<s3>Lviv UKR</s3>
<s4>2006-06-19</s4>
</fA30>
</pR>
</standard>
</inist>
</record>

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