Arid
DOI10.1007/s13538-014-0253-3
Highlights from the Telescope Array Experiment
Sagawa, H.
通讯作者Sagawa, H.
会议名称33rd International Cosmic Ray Conference (ICRC)
会议日期2013
会议地点Rio de Janeiro, BRAZIL
英文摘要

The Telescope Array (TA) is the largest experiment in the Northern Hemisphere currently studying the origin and nature of ultra-high-energy cosmic rays above similar to 10(18) eV by measuring their energy spectrum, mass composition, and arrival directions. It is located in the western desert of central Utah, USA. The TA detector consists of a surface array of 507 scintillation counters, deployed on a square grid of 1.2-km spacing that covers approximately 700 km(2), and 38 fluorescence telescopes located at three sites looking over the surface array. The TA commenced hybrid observation with both sets of detectors in 2008. Here, we present recent results from these 5 years of data and outline our ongoing and near future plans.


英文关键词Ultra-high-energy cosmic rays Telescope array experiment Spectrum Composition Anisotropy
来源出版物BRAZILIAN JOURNAL OF PHYSICS
ISSN0103-9733
EISSN1678-4448
出版年2014
卷号44
期号5
页码589-599
出版者SPRINGER
类型Article;Proceedings Paper
语种英语
国家Japan
收录类别SCI-E ; CPCI-S
WOS记录号WOS:000342165000018
WOS关键词ACTIVE GALACTIC NUCLEI ; AIR-SHOWER ARRAY ; COSMIC-RAYS ; FLUORESCENCE YIELD ; SURFACE DETECTOR ; ENERGY-SPECTRUM
WOS类目Physics, Multidisciplinary
WOS研究方向Physics
资源类型会议论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/302553
作者单位Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba, Japan
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GB/T 7714
Sagawa, H.. Highlights from the Telescope Array Experiment[C]:SPRINGER,2014:589-599.
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