Gamma-quanta and charged particles recognition by the counting and triggers signals formation system of GAMMA-400 space gamma-telescope

Registered events identification procedures details in three apertures of gamma-telescope GAMMA-400 are discussed in the presented article for gammas, electrons/positrons and protons both in low and high energy bands. Gamma-telescope GAMMA-400 consists of the converter-tracker (C) surrounded by anti...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Journal of physics. Conference series 2017-01, Vol.798 (1), p.12016
Hauptverfasser: Arkhangelskaja, I V, Arkhangelskiy, A I, Chasovikov, E N, Kheymits, M D, Yurkin, Y T, Galper, A M, Suchkov, S I, Topchiev, N P, Murchenko, A E
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 1
container_start_page 12016
container_title Journal of physics. Conference series
container_volume 798
creator Arkhangelskaja, I V
Arkhangelskiy, A I
Chasovikov, E N
Kheymits, M D
Yurkin, Y T
Galper, A M
Suchkov, S I
Topchiev, N P
Murchenko, A E
description Registered events identification procedures details in three apertures of gamma-telescope GAMMA-400 are discussed in the presented article for gammas, electrons/positrons and protons both in low and high energy bands. Gamma-telescope GAMMA-400 consists of the converter-tracker (C) surrounded by anticoincidence system, time-of-flight system (2 sections S1 and S2) and calorimeter. Anticoincidence system will make of top and lateral sections - ACtop and AClat, time-of-flight system TOF contain 2 segments S1 and S2. Calorimeter consists of position-sensitive calorimeter CC1 makes of 2 strips layers and 2 layers of CsI(Tl) detectors and electromagnetic calorimeter CC2 composed of CsI(Tl) crystals surrounded by plastic lateral detectors LD. Scintillation detectors of the calorimeter S3 and S4 placed correspondingly between CC1 and CC2 and after electromagnetic calorimeter. All segments of detector systems ACtop, AClat, S1-S4, LD composed of two BC-408 based sensitive layers thickness of 1 cm each. Events registration both from upper and lateral directions provides due three apertures: main, additional and lateral. GAMMA-400 parameters are optimized for detection of gamma-quanta with the energy ∼ 100 GeV in the main aperture. Gammas, electrons/positrons and protons recognition in main aperture provides due energy deposition analysis in individual detectors of ACtop, AClat, S1-S3 and CC1 individual scintillator detectors discriminators. Particles identification in the additional aperture supplied by study of energy deposition in the individual detectors S2, S3 and position-sensitive calorimeter individual scintillator detectors discriminators. In the lateral aperture low energy (0.2 - 100 MeV) photons classified by using simple anticoincidence signals from the individual detectors of LD and CC2. Higher energies γ-quanta (E>100 MeV) recognized using energy deposition analysis in the individual detectors of S3, S4, LD and CC2.
doi_str_mv 10.1088/1742-6596/798/1/012016
format Article
fullrecord <record><control><sourceid>proquest_iop_j</sourceid><recordid>TN_cdi_proquest_journals_2573779659</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2573779659</sourcerecordid><originalsourceid>FETCH-LOGICAL-c355t-783c61cefa4cd0985b4f8566197ff0457d02cae90f0bc12968646863ba993b383</originalsourceid><addsrcrecordid>eNqFkN9KwzAUh4soOKevIAGvvKhLmjZ_LsfQqWwoqNchTZOuY226JLvYE_jaZptMBMFAyAn5feeEL0muEbxDkLERonmWkoKTEeXxNoIog4icJIPjw-mxZuw8ufB-CSGOiw6Sz6lsW5muN7ILEsiuAmohXa0r0EsXGrXSHjitbN01obEdKLcgLDRQdtOFpqv3RHBNXWvngW_qTq48MNa1ch_3Wx90C6wB0_F8Pk5zCIHvpdKg3s8NOg5QtteXyZmJqL76PofJx8P9--Qxnb1MnybjWapwUYSUMqwIUtrIXFWQs6LMDSsIQZwaA_OCVjBTUnNoYKlQxgkjedy4lJzjEjM8TG4OfXtn1xvtg1jajdv9WmQFxZTyKCymyCGlnPXeaSN617TSbQWCYidd7HyKnVsRpQskDtIjmB3AxvY_nf-Fbv-Anl8nb79yoq8M_gLzM5Hh</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2573779659</pqid></control><display><type>article</type><title>Gamma-quanta and charged particles recognition by the counting and triggers signals formation system of GAMMA-400 space gamma-telescope</title><source>Institute of Physics Open Access Journal Titles</source><source>Institute of Physics IOPscience extra</source><source>EZB-FREE-00999 freely available EZB journals</source><source>Alma/SFX Local Collection</source><source>Free Full-Text Journals in Chemistry</source><creator>Arkhangelskaja, I V ; Arkhangelskiy, A I ; Chasovikov, E N ; Kheymits, M D ; Yurkin, Y T ; Galper, A M ; Suchkov, S I ; Topchiev, N P ; Murchenko, A E</creator><creatorcontrib>Arkhangelskaja, I V ; Arkhangelskiy, A I ; Chasovikov, E N ; Kheymits, M D ; Yurkin, Y T ; Galper, A M ; Suchkov, S I ; Topchiev, N P ; Murchenko, A E</creatorcontrib><description>Registered events identification procedures details in three apertures of gamma-telescope GAMMA-400 are discussed in the presented article for gammas, electrons/positrons and protons both in low and high energy bands. Gamma-telescope GAMMA-400 consists of the converter-tracker (C) surrounded by anticoincidence system, time-of-flight system (2 sections S1 and S2) and calorimeter. Anticoincidence system will make of top and lateral sections - ACtop and AClat, time-of-flight system TOF contain 2 segments S1 and S2. Calorimeter consists of position-sensitive calorimeter CC1 makes of 2 strips layers and 2 layers of CsI(Tl) detectors and electromagnetic calorimeter CC2 composed of CsI(Tl) crystals surrounded by plastic lateral detectors LD. Scintillation detectors of the calorimeter S3 and S4 placed correspondingly between CC1 and CC2 and after electromagnetic calorimeter. All segments of detector systems ACtop, AClat, S1-S4, LD composed of two BC-408 based sensitive layers thickness of 1 cm each. Events registration both from upper and lateral directions provides due three apertures: main, additional and lateral. GAMMA-400 parameters are optimized for detection of gamma-quanta with the energy ∼ 100 GeV in the main aperture. Gammas, electrons/positrons and protons recognition in main aperture provides due energy deposition analysis in individual detectors of ACtop, AClat, S1-S3 and CC1 individual scintillator detectors discriminators. Particles identification in the additional aperture supplied by study of energy deposition in the individual detectors S2, S3 and position-sensitive calorimeter individual scintillator detectors discriminators. In the lateral aperture low energy (0.2 - 100 MeV) photons classified by using simple anticoincidence signals from the individual detectors of LD and CC2. Higher energies γ-quanta (E&gt;100 MeV) recognized using energy deposition analysis in the individual detectors of S3, S4, LD and CC2.</description><identifier>ISSN: 1742-6588</identifier><identifier>EISSN: 1742-6596</identifier><identifier>DOI: 10.1088/1742-6596/798/1/012016</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Apertures ; Charged particles ; Converters ; Deposition ; Detectors ; Discriminators ; Electrons ; Energy ; Energy bands ; Particle physics ; Physics ; Position sensing ; Positrons ; Protons ; Recognition ; Scintillation counters ; Segments ; Sensors ; Telescopes ; Thickness</subject><ispartof>Journal of physics. Conference series, 2017-01, Vol.798 (1), p.12016</ispartof><rights>Published under licence by IOP Publishing Ltd</rights><rights>2017. This work is published under http://creativecommons.org/licenses/by/3.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c355t-783c61cefa4cd0985b4f8566197ff0457d02cae90f0bc12968646863ba993b383</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/1742-6596/798/1/012016/pdf$$EPDF$$P50$$Giop$$Hfree_for_read</linktopdf><link.rule.ids>314,780,784,27924,27925,38868,38890,53840,53867</link.rule.ids></links><search><creatorcontrib>Arkhangelskaja, I V</creatorcontrib><creatorcontrib>Arkhangelskiy, A I</creatorcontrib><creatorcontrib>Chasovikov, E N</creatorcontrib><creatorcontrib>Kheymits, M D</creatorcontrib><creatorcontrib>Yurkin, Y T</creatorcontrib><creatorcontrib>Galper, A M</creatorcontrib><creatorcontrib>Suchkov, S I</creatorcontrib><creatorcontrib>Topchiev, N P</creatorcontrib><creatorcontrib>Murchenko, A E</creatorcontrib><title>Gamma-quanta and charged particles recognition by the counting and triggers signals formation system of GAMMA-400 space gamma-telescope</title><title>Journal of physics. Conference series</title><addtitle>J. Phys.: Conf. Ser</addtitle><description>Registered events identification procedures details in three apertures of gamma-telescope GAMMA-400 are discussed in the presented article for gammas, electrons/positrons and protons both in low and high energy bands. Gamma-telescope GAMMA-400 consists of the converter-tracker (C) surrounded by anticoincidence system, time-of-flight system (2 sections S1 and S2) and calorimeter. Anticoincidence system will make of top and lateral sections - ACtop and AClat, time-of-flight system TOF contain 2 segments S1 and S2. Calorimeter consists of position-sensitive calorimeter CC1 makes of 2 strips layers and 2 layers of CsI(Tl) detectors and electromagnetic calorimeter CC2 composed of CsI(Tl) crystals surrounded by plastic lateral detectors LD. Scintillation detectors of the calorimeter S3 and S4 placed correspondingly between CC1 and CC2 and after electromagnetic calorimeter. All segments of detector systems ACtop, AClat, S1-S4, LD composed of two BC-408 based sensitive layers thickness of 1 cm each. Events registration both from upper and lateral directions provides due three apertures: main, additional and lateral. GAMMA-400 parameters are optimized for detection of gamma-quanta with the energy ∼ 100 GeV in the main aperture. Gammas, electrons/positrons and protons recognition in main aperture provides due energy deposition analysis in individual detectors of ACtop, AClat, S1-S3 and CC1 individual scintillator detectors discriminators. Particles identification in the additional aperture supplied by study of energy deposition in the individual detectors S2, S3 and position-sensitive calorimeter individual scintillator detectors discriminators. In the lateral aperture low energy (0.2 - 100 MeV) photons classified by using simple anticoincidence signals from the individual detectors of LD and CC2. Higher energies γ-quanta (E&gt;100 MeV) recognized using energy deposition analysis in the individual detectors of S3, S4, LD and CC2.</description><subject>Apertures</subject><subject>Charged particles</subject><subject>Converters</subject><subject>Deposition</subject><subject>Detectors</subject><subject>Discriminators</subject><subject>Electrons</subject><subject>Energy</subject><subject>Energy bands</subject><subject>Particle physics</subject><subject>Physics</subject><subject>Position sensing</subject><subject>Positrons</subject><subject>Protons</subject><subject>Recognition</subject><subject>Scintillation counters</subject><subject>Segments</subject><subject>Sensors</subject><subject>Telescopes</subject><subject>Thickness</subject><issn>1742-6588</issn><issn>1742-6596</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><sourceid>O3W</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNqFkN9KwzAUh4soOKevIAGvvKhLmjZ_LsfQqWwoqNchTZOuY226JLvYE_jaZptMBMFAyAn5feeEL0muEbxDkLERonmWkoKTEeXxNoIog4icJIPjw-mxZuw8ufB-CSGOiw6Sz6lsW5muN7ILEsiuAmohXa0r0EsXGrXSHjitbN01obEdKLcgLDRQdtOFpqv3RHBNXWvngW_qTq48MNa1ch_3Wx90C6wB0_F8Pk5zCIHvpdKg3s8NOg5QtteXyZmJqL76PofJx8P9--Qxnb1MnybjWapwUYSUMqwIUtrIXFWQs6LMDSsIQZwaA_OCVjBTUnNoYKlQxgkjedy4lJzjEjM8TG4OfXtn1xvtg1jajdv9WmQFxZTyKCymyCGlnPXeaSN617TSbQWCYidd7HyKnVsRpQskDtIjmB3AxvY_nf-Fbv-Anl8nb79yoq8M_gLzM5Hh</recordid><startdate>20170101</startdate><enddate>20170101</enddate><creator>Arkhangelskaja, I V</creator><creator>Arkhangelskiy, A I</creator><creator>Chasovikov, E N</creator><creator>Kheymits, M D</creator><creator>Yurkin, Y T</creator><creator>Galper, A M</creator><creator>Suchkov, S I</creator><creator>Topchiev, N P</creator><creator>Murchenko, A E</creator><general>IOP Publishing</general><scope>O3W</scope><scope>TSCCA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope></search><sort><creationdate>20170101</creationdate><title>Gamma-quanta and charged particles recognition by the counting and triggers signals formation system of GAMMA-400 space gamma-telescope</title><author>Arkhangelskaja, I V ; Arkhangelskiy, A I ; Chasovikov, E N ; Kheymits, M D ; Yurkin, Y T ; Galper, A M ; Suchkov, S I ; Topchiev, N P ; Murchenko, A E</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c355t-783c61cefa4cd0985b4f8566197ff0457d02cae90f0bc12968646863ba993b383</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Apertures</topic><topic>Charged particles</topic><topic>Converters</topic><topic>Deposition</topic><topic>Detectors</topic><topic>Discriminators</topic><topic>Electrons</topic><topic>Energy</topic><topic>Energy bands</topic><topic>Particle physics</topic><topic>Physics</topic><topic>Position sensing</topic><topic>Positrons</topic><topic>Protons</topic><topic>Recognition</topic><topic>Scintillation counters</topic><topic>Segments</topic><topic>Sensors</topic><topic>Telescopes</topic><topic>Thickness</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Arkhangelskaja, I V</creatorcontrib><creatorcontrib>Arkhangelskiy, A I</creatorcontrib><creatorcontrib>Chasovikov, E N</creatorcontrib><creatorcontrib>Kheymits, M D</creatorcontrib><creatorcontrib>Yurkin, Y T</creatorcontrib><creatorcontrib>Galper, A M</creatorcontrib><creatorcontrib>Suchkov, S I</creatorcontrib><creatorcontrib>Topchiev, N P</creatorcontrib><creatorcontrib>Murchenko, A E</creatorcontrib><collection>Institute of Physics Open Access Journal Titles</collection><collection>IOPscience (Open Access)</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Advanced Technologies &amp; Aerospace Database</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>Access via ProQuest (Open Access)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><jtitle>Journal of physics. Conference series</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Arkhangelskaja, I V</au><au>Arkhangelskiy, A I</au><au>Chasovikov, E N</au><au>Kheymits, M D</au><au>Yurkin, Y T</au><au>Galper, A M</au><au>Suchkov, S I</au><au>Topchiev, N P</au><au>Murchenko, A E</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Gamma-quanta and charged particles recognition by the counting and triggers signals formation system of GAMMA-400 space gamma-telescope</atitle><jtitle>Journal of physics. Conference series</jtitle><addtitle>J. Phys.: Conf. Ser</addtitle><date>2017-01-01</date><risdate>2017</risdate><volume>798</volume><issue>1</issue><spage>12016</spage><pages>12016-</pages><issn>1742-6588</issn><eissn>1742-6596</eissn><abstract>Registered events identification procedures details in three apertures of gamma-telescope GAMMA-400 are discussed in the presented article for gammas, electrons/positrons and protons both in low and high energy bands. Gamma-telescope GAMMA-400 consists of the converter-tracker (C) surrounded by anticoincidence system, time-of-flight system (2 sections S1 and S2) and calorimeter. Anticoincidence system will make of top and lateral sections - ACtop and AClat, time-of-flight system TOF contain 2 segments S1 and S2. Calorimeter consists of position-sensitive calorimeter CC1 makes of 2 strips layers and 2 layers of CsI(Tl) detectors and electromagnetic calorimeter CC2 composed of CsI(Tl) crystals surrounded by plastic lateral detectors LD. Scintillation detectors of the calorimeter S3 and S4 placed correspondingly between CC1 and CC2 and after electromagnetic calorimeter. All segments of detector systems ACtop, AClat, S1-S4, LD composed of two BC-408 based sensitive layers thickness of 1 cm each. Events registration both from upper and lateral directions provides due three apertures: main, additional and lateral. GAMMA-400 parameters are optimized for detection of gamma-quanta with the energy ∼ 100 GeV in the main aperture. Gammas, electrons/positrons and protons recognition in main aperture provides due energy deposition analysis in individual detectors of ACtop, AClat, S1-S3 and CC1 individual scintillator detectors discriminators. Particles identification in the additional aperture supplied by study of energy deposition in the individual detectors S2, S3 and position-sensitive calorimeter individual scintillator detectors discriminators. In the lateral aperture low energy (0.2 - 100 MeV) photons classified by using simple anticoincidence signals from the individual detectors of LD and CC2. Higher energies γ-quanta (E&gt;100 MeV) recognized using energy deposition analysis in the individual detectors of S3, S4, LD and CC2.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/1742-6596/798/1/012016</doi><tpages>5</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 1742-6588
ispartof Journal of physics. Conference series, 2017-01, Vol.798 (1), p.12016
issn 1742-6588
1742-6596
language eng
recordid cdi_proquest_journals_2573779659
source Institute of Physics Open Access Journal Titles; Institute of Physics IOPscience extra; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection; Free Full-Text Journals in Chemistry
subjects Apertures
Charged particles
Converters
Deposition
Detectors
Discriminators
Electrons
Energy
Energy bands
Particle physics
Physics
Position sensing
Positrons
Protons
Recognition
Scintillation counters
Segments
Sensors
Telescopes
Thickness
title Gamma-quanta and charged particles recognition by the counting and triggers signals formation system of GAMMA-400 space gamma-telescope
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-01T11%3A48%3A42IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_iop_j&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Gamma-quanta%20and%20charged%20particles%20recognition%20by%20the%20counting%20and%20triggers%20signals%20formation%20system%20of%20GAMMA-400%20space%20gamma-telescope&rft.jtitle=Journal%20of%20physics.%20Conference%20series&rft.au=Arkhangelskaja,%20I%20V&rft.date=2017-01-01&rft.volume=798&rft.issue=1&rft.spage=12016&rft.pages=12016-&rft.issn=1742-6588&rft.eissn=1742-6596&rft_id=info:doi/10.1088/1742-6596/798/1/012016&rft_dat=%3Cproquest_iop_j%3E2573779659%3C/proquest_iop_j%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2573779659&rft_id=info:pmid/&rfr_iscdi=true