Prototype of the Scintillation Time-of-Flight Hodoscope
The results of studies of the characteristics of the prototype of the scintillation time-of-flight hodoscope 71 cm long are presented. Prototype testing using a 90 Sr + 90 Y radioactive source showed that the coordinate resolution and detection efficiency depend on the source position on the work su...
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| Veröffentlicht in: | Bulletin of the Lebedev Physics Institute 2023-08, Vol.50 (8), p.354-359 |
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| container_title | Bulletin of the Lebedev Physics Institute |
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| creator | Alekseev, V. I. Baskov, V. A. Dronov, V. A. L’vov, A. I. Kolzov, A. V. Krechetov, Yu. F. Poliansky, V. V. Sidorin, S. S. Varfolomeeva, E. A. |
| description | The results of studies of the characteristics of the prototype of the scintillation time-of-flight hodoscope 71 cm long are presented. Prototype testing using a
90
Sr +
90
Y radioactive source showed that the coordinate resolution and detection efficiency depend on the source position on the work surface. The best coordinate resolution and the highest detection efficiency were found at the module center as σ
x
≈ 1.2 cm and ε ≈ 9%, respectively. |
| doi_str_mv | 10.3103/S1068335623080031 |
| format | Article |
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90
Sr +
90
Y radioactive source showed that the coordinate resolution and detection efficiency depend on the source position on the work surface. The best coordinate resolution and the highest detection efficiency were found at the module center as σ
x
≈ 1.2 cm and ε ≈ 9%, respectively.</description><identifier>ISSN: 1068-3356</identifier><identifier>EISSN: 1934-838X</identifier><identifier>DOI: 10.3103/S1068335623080031</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Physics ; Physics and Astronomy ; Prototype tests ; Scintillation ; Strontium 90</subject><ispartof>Bulletin of the Lebedev Physics Institute, 2023-08, Vol.50 (8), p.354-359</ispartof><rights>Allerton Press, Inc. 2023. ISSN 1068-3356, Bulletin of the Lebedev Physics Institute, 2023, Vol. 50, No. 8, pp. 354–359. © Allerton Press, Inc., 2023. Russian Text © The Author(s), 2023, published in Kratkie Soobshcheniya po Fizike, 2023, Vol. 50, No. 8, pp. 49–57.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c268t-b06930a83bff542eb34b94ffe78d61d91e2e7cca4df9d24adb80517c1463ebcc3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.3103/S1068335623080031$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.3103/S1068335623080031$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Alekseev, V. I.</creatorcontrib><creatorcontrib>Baskov, V. A.</creatorcontrib><creatorcontrib>Dronov, V. A.</creatorcontrib><creatorcontrib>L’vov, A. I.</creatorcontrib><creatorcontrib>Kolzov, A. V.</creatorcontrib><creatorcontrib>Krechetov, Yu. F.</creatorcontrib><creatorcontrib>Poliansky, V. V.</creatorcontrib><creatorcontrib>Sidorin, S. S.</creatorcontrib><creatorcontrib>Varfolomeeva, E. A.</creatorcontrib><title>Prototype of the Scintillation Time-of-Flight Hodoscope</title><title>Bulletin of the Lebedev Physics Institute</title><addtitle>Bull. Lebedev Phys. Inst</addtitle><description>The results of studies of the characteristics of the prototype of the scintillation time-of-flight hodoscope 71 cm long are presented. Prototype testing using a
90
Sr +
90
Y radioactive source showed that the coordinate resolution and detection efficiency depend on the source position on the work surface. The best coordinate resolution and the highest detection efficiency were found at the module center as σ
x
≈ 1.2 cm and ε ≈ 9%, respectively.</description><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Prototype tests</subject><subject>Scintillation</subject><subject>Strontium 90</subject><issn>1068-3356</issn><issn>1934-838X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><recordid>eNp1kFFLwzAUhYMoOKs_wLeCz9EkN2nTRxnODQYKm-BbadObraNrapI97N_bMcEH8eleOOc7l3MJuefsETiDpxVnmQZQmQCmGQN-QSa8AEk16M_LcR9letKvyU0IO8aU0oWakPzdu-jiccDU2TRuMV2Zto9t11WxdX26bvdInaWzrt1sYzp3jQvGDXhLrmzVBbz7mQn5mL2sp3O6fHtdTJ-X1IhMR1qzrABWaaitVVJgDbIupLWY6ybjTcFRYG5MJRtbNEJWTa2Z4rnhMgOsjYGEPJxzB---DhhiuXMH348nS6FzBkqc6ieEn13GuxA82nLw7b7yx5Kz8mQo__xnZMSZCaO336D_Tf4f-ga9lWal</recordid><startdate>20230801</startdate><enddate>20230801</enddate><creator>Alekseev, V. I.</creator><creator>Baskov, V. A.</creator><creator>Dronov, V. A.</creator><creator>L’vov, A. I.</creator><creator>Kolzov, A. V.</creator><creator>Krechetov, Yu. F.</creator><creator>Poliansky, V. V.</creator><creator>Sidorin, S. S.</creator><creator>Varfolomeeva, E. A.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20230801</creationdate><title>Prototype of the Scintillation Time-of-Flight Hodoscope</title><author>Alekseev, V. I. ; Baskov, V. A. ; Dronov, V. A. ; L’vov, A. I. ; Kolzov, A. V. ; Krechetov, Yu. F. ; Poliansky, V. V. ; Sidorin, S. S. ; Varfolomeeva, E. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c268t-b06930a83bff542eb34b94ffe78d61d91e2e7cca4df9d24adb80517c1463ebcc3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Prototype tests</topic><topic>Scintillation</topic><topic>Strontium 90</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Alekseev, V. I.</creatorcontrib><creatorcontrib>Baskov, V. A.</creatorcontrib><creatorcontrib>Dronov, V. A.</creatorcontrib><creatorcontrib>L’vov, A. I.</creatorcontrib><creatorcontrib>Kolzov, A. V.</creatorcontrib><creatorcontrib>Krechetov, Yu. F.</creatorcontrib><creatorcontrib>Poliansky, V. V.</creatorcontrib><creatorcontrib>Sidorin, S. S.</creatorcontrib><creatorcontrib>Varfolomeeva, E. A.</creatorcontrib><collection>CrossRef</collection><jtitle>Bulletin of the Lebedev Physics Institute</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Alekseev, V. I.</au><au>Baskov, V. A.</au><au>Dronov, V. A.</au><au>L’vov, A. I.</au><au>Kolzov, A. V.</au><au>Krechetov, Yu. F.</au><au>Poliansky, V. V.</au><au>Sidorin, S. S.</au><au>Varfolomeeva, E. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Prototype of the Scintillation Time-of-Flight Hodoscope</atitle><jtitle>Bulletin of the Lebedev Physics Institute</jtitle><stitle>Bull. Lebedev Phys. Inst</stitle><date>2023-08-01</date><risdate>2023</risdate><volume>50</volume><issue>8</issue><spage>354</spage><epage>359</epage><pages>354-359</pages><issn>1068-3356</issn><eissn>1934-838X</eissn><abstract>The results of studies of the characteristics of the prototype of the scintillation time-of-flight hodoscope 71 cm long are presented. Prototype testing using a
90
Sr +
90
Y radioactive source showed that the coordinate resolution and detection efficiency depend on the source position on the work surface. The best coordinate resolution and the highest detection efficiency were found at the module center as σ
x
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| ispartof | Bulletin of the Lebedev Physics Institute, 2023-08, Vol.50 (8), p.354-359 |
| issn | 1068-3356 1934-838X |
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| subjects | Physics Physics and Astronomy Prototype tests Scintillation Strontium 90 |
| title | Prototype of the Scintillation Time-of-Flight Hodoscope |
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