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dc.contributor.author김항배-
dc.date.accessioned2018-04-16T00:55:48Z-
dc.date.available2018-04-16T00:55:48Z-
dc.date.issued2012-07-
dc.identifier.citationNuclear Inst. and Methods in Physics Research, 2012, 689, P.87-97en_US
dc.identifier.issn0168-9002-
dc.identifier.issn1872-9576-
dc.identifier.urihttp://apps.webofknowledge.com/InboundService.do?customersID=LinksAMR&mode=FullRecord&IsProductCode=Yes&product=WOS&Init=Yes&Func=Frame&DestFail=http%3A%2F%2Fwww.webofknowledge.com&action=retrieve&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&SID=D6b9phXB7a8rOqHzzua&UT=WOS%3A000307797500014-
dc.identifier.urihttp://hdl.handle.net/20.500.11754/67197-
dc.description.abstractThe Telescope Array (TA) experiment, located in the western desert of Utah, USA, is designed for the observation of extensive air showers from extremely high energy cosmic rays. The experiment has a surface detector array surrounded by three fluorescence detectors to enable simultaneous detection of shower particles at ground level and fluorescence photons along the shower track. The TA surface detectors and fluorescence detectors started full hybrid observation in March, 2008. In this article we describe the design and technical features of the TA surface detector.en_US
dc.description.sponsorshipThe Telescope Array experiment is supported by the Japan Society for the Promotion of Science through Grants-in-Aid for Scientific Research on Specially Promoted Research (21000002) "Extreme Phenomena in the Universe Explored by Highest Energy Cosmic Rays", and the Inter-University Research Program of the Institute for Cosmic Ray Research; by the U.S. National Science Foundation awards PHY-0307098, PHY-0601915, PHY-0703893, PHY-0758342, and PHY-0848320 (Utah) and PHY-0649681 (Rutgers); by the National Research Foundation of Korea (2006-0050031, 2007-0056005, 2007-0093860, 2010-0011378, 2010-0028071, R32-10130, 2011-0002617); by the Russian Academy of Sciences, RFBR Grants 10-02-01406a and 11-02-01528a (INR), IISN project No. 4.4509.10 and Belgian Science Policy under IUAP VI/11 (ULB). The foundations of Dr. Ezekiel R. and Edna Wattis Dumke, Willard L Eccles and the George S. and Dolores Dore Eccles all helped with generous donations. The State of Utah supported the project through its Economic Development Board, and the University of Utah through the Office of the Vice President for Research. The experimental site became available through the cooperation of the Utah School and Institutional Trust Lands Administration (SITLA), U.S. Bureau of Land Management and the U.S. Air Force. We also wish to thank the people and the officials of Millard County, Utah, for their steadfast and warm support. We gratefully acknowledge the contributions from the technical staffs of our home institutions and the University of Utah Center for High Performance Computing (CHPC).en_US
dc.language.isoenen_US
dc.publisherElsevier Science B.Ven_US
dc.subjectUltra-high energy cosmic raysen_US
dc.subjectTelescope Array experimenten_US
dc.subjectExtensive air shower arrayen_US
dc.titleThe surface detector array of the Telescope Array experimenten_US
dc.typeArticleen_US
dc.relation.volume689-
dc.identifier.doi10.1016/j.nima.2012.05.079-
dc.relation.page87-97-
dc.relation.journalNUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT-
dc.contributor.googleauthorAbu-Zayyad, T.-
dc.contributor.googleauthorAida, R.-
dc.contributor.googleauthorAllen, M.-
dc.contributor.googleauthorAnderson, R.-
dc.contributor.googleauthorAzuma, R.-
dc.contributor.googleauthorBarcikowski, E.-
dc.contributor.googleauthorBelz, J. W.-
dc.contributor.googleauthorBergman, D. R.-
dc.contributor.googleauthorBlake, S. A.-
dc.contributor.googleauthorCady, R.-
dc.relation.code2012214156-
dc.sector.campusS-
dc.sector.daehakCOLLEGE OF NATURAL SCIENCES[S]-
dc.sector.departmentDEPARTMENT OF PHYSICS-
dc.identifier.pidhbkim-
Appears in Collections:
COLLEGE OF NATURAL SCIENCES[S](자연과학대학) > PHYSICS(물리학과) > Articles
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