Performance of the surface scintillation detector for the telescope array

被引：0

作者：

Hayashi, Y. ^{[1
]}

Kawakami, S. ^{[1
]}

Matsumoto, K. ^{[1
]}

Matsumoto, Y. ^{[1
]}

Matsuyama, T. ^{[1
]}

Nonaka, T. ^{[1
]}

Okuda, T. ^{[1
]}

Oshima, A. ^{[1
]}

Tanaka, H. ^{[1
]}

机构：

[1] Osaka City Univ, Grad Sch Sci, Osaka 5588585, Japan

来源：

Proceedings of the 29th International Cosmic Ray Conference Vol 8: HE 1.5 | 2005年

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Systematic measurement on basic characteristics of surface detectors have been done in detail. These test are quite essential for reducing the systematic error in estimating the total number of charged particles in a giant air shower, so energy of primary cosmic rays. Some of those things, such as position sensitivity and temperature dependence of scintillation detector and surface sensitivity map of photo tubes were also measured. We found that all of these variation is within 10 to 15% and total performance of our scintillation systems are well inside our expectation.

引用

页码：161 / 164

页数：4

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