Resolving electrons from protons in ATIC
文献类型:期刊论文
作者 | Chang, J.1,2; Adams, J. H., Jr.3; Ahn, H. S.4; Bashindzhagyan, G. L.5; Batkov, K. E.5; Christl, M.; Fazely, A. R.6; Ganel, O.4; Gunashingha, R. M.6; Guzik, T. G.7 |
刊名 | ADVANCES IN SPACE RESEARCH |
出版日期 | 2008-08-05 |
卷号 | 42期号:3页码:431-436 |
ISSN号 | 0273-1177 |
关键词 | electron simulation beam test balloon flight |
英文摘要 | The Advanced Thin Ionization Calorimeter (ATIC) experiment is designed for high energy cosmic ray ion detection. The possibility to identify high energy primary cosmic ray electrons in the presence of the 'background' of cosmic ray protons has been studied by simulating nuclear-electromagnetic cascade showers using the FLUKA Monte Carlo simulation code. The ATIC design, consisting of a graphite target and an energy detection device, a totally active calorimeter built up of 2.5 cm x 2.5 cm x 25.0 cm BGO scintillator bars, gives sufficient information to distinguish electrons from protons. While identifying about 80% of electrons as such, only about 2 in 10,000 protons (@ 150 GeV) will mimic electrons. In September of 1999 ATIC was exposed to high-energy electron and proton beams at the CERN H2 beam line, and this data confirmed the electron detection capabilities of ATIC. From 2000-12-28 to 2001-01-13 ATIC was flown as a long duration balloon test flight from McMurdo, Antarctica, recording over 360 h of data and allowing electron separation to be confirmed in the flight data. In addition, ATIC electron detection capabilities can be checked by atmospheric gamma-ray observations. (c) 2007 COSPAR. Published by Elsevier Ltd. All rights reserved. |
学科主题 | Engineering; Astronomy & Astrophysics; Geology; Meteorology & Atmospheric Sciences |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics ; Geosciences, Multidisciplinary ; Meteorology & Atmospheric Sciences |
研究领域[WOS] | Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000257684300005 |
公开日期 | 2011-12-29 |
源URL | [http://159.226.72.40/handle/332002/1773] |
专题 | 紫金山天文台_暗物质和空间天文实验室 |
作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Space Astron Div, Jiangsu 210008, Peoples R China 2.Max Planck Inst Solar Syst Res, Katlenburg Lindau, Germany 3.NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA 4.Univ Maryland, Inst Phys Sci & Technol, College Pk, MD 20742 USA 5.Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow, Russia 6.So Univ, Dept Phys, Baton Rouge, LA USA 7.Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA 8.Univ Alabama, Huntsville, AL 35899 USA |
推荐引用方式 GB/T 7714 | Chang, J.,Adams, J. H., Jr.,Ahn, H. S.,et al. Resolving electrons from protons in ATIC[J]. ADVANCES IN SPACE RESEARCH,2008,42(3):431-436. |
APA | Chang, J..,Adams, J. H., Jr..,Ahn, H. S..,Bashindzhagyan, G. L..,Batkov, K. E..,...&Zatsepin, V. I..(2008).Resolving electrons from protons in ATIC.ADVANCES IN SPACE RESEARCH,42(3),431-436. |
MLA | Chang, J.,et al."Resolving electrons from protons in ATIC".ADVANCES IN SPACE RESEARCH 42.3(2008):431-436. |
入库方式: OAI收割
来源:紫金山天文台
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