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Energy Spectrum Measured by Telescope Array Surface Detector

机译:望远镜阵列表面探测器测量能谱

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The Telescope Array experiment (TA) is the largest cosmic ray experiment in the northern hemisphere. Itconsists of a surface detector (SD) of 507 scintillation counters and three fluorescence detector (FD) stations overlookingthe SD. We are analyzing the data collected by TA SD using a new technique which consists of generating a MonteCarlo (MC) simulation with all characteristics of the data, comparing the MC with the data to verify the validity of theMC, and calculation of the SD aperture from the MC information. In this paper, we describe our basic analysis, whichis based solely upon the data, our method of generating CORSIKA showers without the problems caused by thinning,comparisons of our MC with the data, and the latest TA SD energy spectrum result.
机译:望远镜阵列实验(TA)是北半球最大的宇宙射线实验。它由507个闪烁计数器的表面检测器(SD)和俯瞰SD的三个荧光检测器(FD)站组成。我们正在使用一种新技术来分析TA SD收集的数据,该技术包括生成具有数据所有特征的MonteCarlo(MC)仿真,将MC与数据进行比较以验证MC的有效性,以及从中计算SD孔径MC信息。在本文中,我们描述了仅基于数据的基础分析,不存在因变薄而产生问题的CORSIKA阵雨的生成方法,MC与数据的比较以及最新的TA SD能谱结果。

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