Design and Performance of the ARIANNA Hexagonal Radio Array Systems
S. W. Barwick, E. C. Berg, D. Z. Besson, E. Cheim, T. Duffin, J. C., Hanson, S. R. Klein, S. A. Kleinfelder, T. Prakash, M. Piasecki, K. Ratzlaff,, C. Reed, M. Roumi, A. Samanta, T. Stezelberger, J. Tatar, J. Walker, R., Young, and L. Zou

TL;DR
The paper details the development, deployment, and performance evaluation of the ARIANNA Hexagonal Radio Array stations in Antarctica, aimed at detecting ultra-high energy neutrinos through radio signals with high precision and low power consumption.
Contribution
It introduces a new fully-synchronous high-speed signal acquisition chip and demonstrates the operational performance of the first stations in a large neutrino detection array.
Findings
Stations operate with >=58% live-time annually.
Trigger system reduces rates to a few milli-Hertz.
Timing resolution of 0.049 ps RMS and angular precision of 0.14-0.17 degrees.
Abstract
We report on the development, installation and operation of the first three of seven stations deployed at the ARIANNA site's pilot Hexagonal Radio Array in Antarctica. The primary goal of the ARIANNA project is to observe ultra-high energy (>100 PeV) cosmogenic neutrino signatures using a large array of autonomous stations each dispersed 1 km apart on the surface of the Ross Ice Shelf. Sensing radio emissions of 100 MHz to 1 GHz, each station in the array contains RF antennas, amplifiers, 1.92 G-sample/s, 850 MHz bandwidth signal acquisition circuitry, pattern-matching trigger capabilities, an embedded CPU, 32 GB of solid-state data storage, and long-distance wireless and satellite communications. Power is provided by the sun and LiFePO4 storage batteries, and the stations consume an average of 7W of power. Operation on solar power has resulted in >=58% per calendar-year live-time. The…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Neutrino Physics Research
