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The energy spectrum of cosmic rays above 10(17.2) eV measured by the fluorescence detectors of the Telescope Array experiment in seven years

机译:望远镜阵列实验的荧光检测器在七年内测得的宇宙射线的能量谱高于10(17.2)eV

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The Telescope Array (TA) experiment is the largest detector to observe ultra-high-energy cosmic rays in the northern hemisphere. The fluorescence detectors at two stations of TA are newly constructed and have now completed seven years of steady operation. One advantage of monocular analysis of the fluorescence detectors is a lower energy threshold for cosmic rays than that of other techniques like stereoscopic observations or coincidences with the surface detector array, allowing the measurement of an energy spectrum covering three orders of magnitude in energy. Analyzing data collected during those seven years, we report the energy spectrum of cosmic rays covering a broad range of energies above 10(17.2)eV measured by the fluorescence detectors and a comparison with previously published results. (C) 2016 Elsevier B.V. All rights reserved.
机译:望远镜阵列(TA)实验是观察北半球超高能宇宙射线的最大探测器。 TA的两个站点的荧光检测器是新建的,现已完成了七年的稳定运行。荧光探测器的单眼分析的一个优点是,宇宙射线的能量阈值比其他技术(如立体观测或与表面探测器阵列的重合性)低,从而可以测量覆盖三个数量级能量的能谱。分析这七年来收集的数据,我们报告了宇宙射线的能谱,该光谱涵盖了荧光检测器测得的10(17.2)eV以上的广泛能量,并与先前发表的结果进行了比较。 (C)2016 Elsevier B.V.保留所有权利。

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