用TALE混合探测器测量宇宙射线质量成分

K. Fujita
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引用次数: 0

摘要

位于美国犹他州的望远镜阵列(TA)是北半球最大的超高能量宇宙射线天文台。望远镜阵列低能延伸(TALE)探测器是为了研究宇宙射线从银河系起源到星系外起源的转变而建造的。TALE探测器由一个荧光探测器(FD)站和一个由80个闪烁计数器组成的表面探测器(SD)阵列组成,其中40个间隔400米,40个间隔600米。FD站位于TA中鼓FD站(本身由14个FD望远镜组成)。自2017年以来,我们继续使用混合模式进行稳定观测。在这篇文章中,我们介绍了利用近4年的TALE混合数据测量宇宙射线质量组成的最新结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Cosmic ray mass composition measurement with the TALE hybrid detector
The Telescope Array (TA) located in the State of Utah in the US is the largest ultra-high energy cosmic rays observatory in the northern hemisphere. The Telescope Array Low-energy Extension (TALE) detector was constructed to study the transition of cosmic rays from Galactic to extra-galactic origin. The TALE detector consists of a Fluorescence Detector (FD) station with 10 high elevation telescopes located at the TA Middle Drum FD Station (itself made up of 14 FD telescopes), and a Surface Detector (SD) array made up of 80 scintillation counters, including 40 with 400 m spacing and 40 with 600 m spacing. We have continued stable observation with hybrid mode since 2017. In this contribution, we present the latest result of the cosmic ray mass composition measurement using almost 4 years of TALE hybrid data.
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