Arid
Telescope Array; Simulation and data analysis
Sakurai, N.; Yoshida, S.; Ozawa, S.; Taketa, A.; Hibino, K.; Inoue, N.; Wada, Y.; Kasahara, K.; Minagawa, R.; Iguchi, T.
通讯作者Sakurai, N.
会议名称29th International Cosmic Ray Conference
会议日期AUG 03-10, 2005
会议地点Pune, INDIA
英文摘要

Telescope Array (TA) is a EAS detector which is now building in the western desert in Utah, USA. In order to estimate the performance of TA, a detailed detector simulation is being developed in Java. The number of particles produced during the development of the EAS shower with various inclinations is calculated by COSMOS code. The detection efficiency of each detector is evaluated by using the various calibration data and the results of GEANT4 simulation. And it is taken into account in estimating the signal. The analysis methods of the EAS data are also being developed using TA simulation. This report describes the structure of our simulation code, the analysis methods and the TA performance estimation based on our simulation.


来源出版物Proceedings of the 29th International Cosmic Ray Conference Vol 8: HE 1.5
出版年2005
页码193-195
ISBN*************
出版者TATA INST FUNDAMENTAL RESEARCH
类型Proceedings Paper
语种英语
国家Japan
收录类别CPCI-S
WOS记录号WOS:000243522900049
WOS类目Astronomy & Astrophysics ; Instruments & Instrumentation ; Physics, Particles & Fields
WOS研究方向Astronomy & Astrophysics ; Instruments & Instrumentation ; Physics
资源类型会议论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/295637
作者单位(1)Chiba Univ, Inage Ku, Chiba 2638522, Japan
推荐引用方式
GB/T 7714
Sakurai, N.,Yoshida, S.,Ozawa, S.,et al. Telescope Array; Simulation and data analysis[C]:TATA INST FUNDAMENTAL RESEARCH,2005:193-195.
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