Implementing a Low-Threshold Analysis with the Askaryan Radio Array (ARA)

the ARA Collaboration

研究成果: Conference article同行評審

摘要

The Askaryan Radio Array (ARA) is a ground-based radio detector at the South Pole designed to capture Askaryan emission from ultra-high energy neutrinos interacting within the Antarctic ice. The newest ARA station has been equipped with a phased array trigger, in which radio signals in multiple antennas are summed in predetermined directions prior to the trigger. In this way, impulsive signals add coherently, while noise likely does not, allowing the trigger threshold to be lower than a traditional ARA station. Early results on just a fraction of available data from this new system prove the feasibility of a low-threshold analysis.

原文English
文章編號1153
期刊Proceedings of Science
395
出版狀態Published - 18 3月 2022
事件37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, 德國
持續時間: 12 7月 202123 7月 2021

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