Further development of data acquisition system of the Akeno Giant Air Shower Array

被引：30

作者：

Ohoka, H

Takeda, M

Hayashida, N

Honda, K

Honda, M

Inoue, N

Kadota, K

Kakimoto, F

Kamata, K

Kawaguchi, S

Kawasumi, N

Matsubara, Y

Murakami, K

Nagano, M

Teshima, M

Tsushima, I

Uchihori, Y

Yoshida, S

Yoshii, H

机构：

[1] TOKYO INST TECHNOL,DEPT PHYS,TOKYO 152,JAPAN

[2] UNIV TOKYO,INST COSM RAY RES,TANASHI,TOKYO 188,JAPAN

[3] YAMANASHI UNIV,FAC EDUC,KOFU,YAMANASHI 400,JAPAN

[4] SAITAMA UNIV,DEPT PHYS,URAWA,SAITAMA 338,JAPAN

[5] NISHINA MEM FDN,KOMAGOME,TOKYO 188,JAPAN

[6] HIROSAKI UNIV,FAC GEN EDUC,HIROSAKI,AOMORI 036,JAPAN

[7] NAGOYA UNIV,SOLAR TERR ENVIRONM LAB,NAGOYA,AICHI 46401,JAPAN

[8] NAGOYA UNIV FOREIGN STUDIES,AICHI 47001,JAPAN

[9] EHIME UNIV,FAC GEN EDUC,MATSUYAMA,EHIME 790,JAPAN

来源：

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 1997年 / 385卷 / 02期

关键词：

extremely high energy cosmic rays; data acquisition; air shower array;

D O I：

10.1016/S0168-9002(96)01027-3

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

The data acquisition system of the Akeno Giant Air Shower Array (AGASA) is described, The AGASA array covers an area of about 100 km(2) and has been operated since 1990 to study the origin of extremely high energy cosmic rays. In the early stage of our experiment, AGASA was divided into four sub-arrays called branches for topographical reasons so that air showers were observed independently at each branch. In December 1995, we have improved the data acquisition system and unified the four branches into a single detection system. By this unification, the effective detection area of the AGASA increases by about 1.7 times in the early stage.

引用

页码：268 / 276

页数：9

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