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Energy Spectrum Measured by Telescope Array Surface Detector

机译:通过望远镜阵列表面检测器测量的能谱

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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。俯视SD的507闪烁计数器和三个荧光检测器(FD)站的表面检测器(SD)的itconsistis。我们正在使用新技术分析TA SD收集的数据,该数据包括使用数据的所有特征生成Montecarlo(MC)模拟,将MC与数据进行比较以验证HIMC的有效性,以及SD光圈的计算MC信息。在本文中,我们描述了我们的基本分析,仅基于数据,我们在没有通过减少的情况下产生的核心座淋浴的方法,我们的MC与数据的比较,以及最新的TA SD能量谱结果。

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