Detection of ultra-high energy cosmic ray air showers by Cosmic Ray Air Fluorescence Fresnel lens Telescope for next generation

被引：1

作者：

Tameda, Yuichiro ^{[1
]}

Yamamoto, Mashu ^{[2
]}

Tomida, Takayuki ^{[2
]}

Ikeda, Daisuke ^{[3
]}

Yamazaki, Katsuya ^{[4
]}

Iwakura, Hirokazu ^{[2
]}

Nakamura, Yuya ^{[2
]}

Saito, Yasunori ^{[2
]}

机构：

[1] Osaka Electrocommun Univ, Neyagawa, Osaka, Japan

[2] Shinshu Univ, Nagano, Nagano, Japan

[3] Univ Tokyo, Earthquake Res Inst, Bunkyo Ku, Tokyo, Japan

[4] Kanagawa Univ, Yokohama, Kanagawa, Japan

来源：

ULTRA HIGH ENERGY COSMIC RAYS 2018 (UHECR 2018) | 2019年 / 210卷

关键词：

ARRAY;

D O I：

10.1051/epjconf/201921006004

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In the future, ultra-high energy cosmic ray (UHECR) observatory will be expanded due to the small flux. Then, cost reduction is useful strategy to realize a huge scale observatory. For this purpose, we are developing a simple structure cosmic ray detector named as Cosmic Ray Air Fluorescence Fresnel-lens Telescope (CRAFFT). We deployed CRAFFT detectors at the Telescope Array site and performed a test observation. We have successfully observed UHECR air showers. We will report the status and the result of the test observation.

引用

页数：7

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