Future Plans of Telescope Array

被引：1
|
作者：
Ogio, Shoichi [1 ]
机构：
[1] Osaka City Univ, Grad Sch Sci, Sumiyoshi Ku, Osaka 5588585, Japan
来源：
INTERNATIONAL SYMPOSIUM ON THE RECENT PROGRESS OF ULTRA-HIGH ENERGY COSMIC RAY OBSERVATION | 2011年 / 1367卷
关键词：
ultra high energy cosmic rays; air shower array; fluorescence detectors; RAY ENERGY-SPECTRUM; COSMIC-RAYS;
D O I：
10.1063/1.3628729
中图分类号：
O59 [应用物理学];
学科分类号：
摘要：
The Telescope Array (TA) experiment is the only ultra high energy cosmic ray observatory in the northern hemisphere. In addition, it will be the world's first air shower detector to be directly calibrated by an on-site accelerator beam. For wider and deeper understanding of cosmic rays by via high precision measurements, we have undertaken the study of extension plans for TA. One extension plan will extend the sensitive energy range of TA down to 10(17) eV. A second plan would extend of the aperture area of the SD array. These plans are described in this note.
引用
收藏
页码：132 / 136
页数：5
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