Knowledge Resource Center for Ecological Environment in Arid Area
DOI | 10.1007/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 |
ISSN | 0103-9733 |
EISSN | 1678-4448 |
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/2XILL650/302782 |
作者单位 | Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba, Japan |
推荐引用方式 GB/T 7714 | Sagawa, H.. Highlights from the Telescope Array Experiment[C]:SPRINGER,2014:589-599. |
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