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Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf

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arxiv 1612.04473 v2 pith:EONPGO33 submitted 2016-12-14 astro-ph.IM astro-ph.HE

S. W. Barwick , D. Z. Besson , A. Burgman , E. Chiem , A. Hallgren , J. C. Hanson , S. R. Klein , S. Kleinfelder
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A. Nelles C. Persichilli S. Phillips T. Prakash C. Reed S. R. Shively J. Tatar E. Unger J. Walker G. Yodh
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keywords radiosignalsariannashowerscosmicdetectionenergyexperiment
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abstract

The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 10^16 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of \unit[100-500]{MHz} and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of $6.5^{+1.2}_{-1.0}\times10^{17}$ eV is measured to be $1.1^{+1.0}_{-0.7}\times10^{-16}$ eV$^{-1}$km$^{-2}$sr$^{-1}$yr$^{-1}$ and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Simulation of combined radio and radar signals at the Radar Echo Telescope for Cosmic Rays

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    Combined FAERIE+MARES simulations show RET-CR radar echoes can exceed in-ice Askaryan power near 182 MHz for many geometries at 136–544 W, separable by timing and narrowband filtering.

  2. Instrument design and performance of the first seven stations of RNO-G

    astro-ph.IM 2024-11 conditional novelty 6.0 of 10

    The first seven RNO-G stations are commissioned and performing to design expectations, with 10-20 ps timing resolution and trigger thresholds near design targets.

  3. Complex Analysis of Askaryan Radiation: UHECR Reconstruction

    astro-ph.HE 2026-06 unverdicted novelty 5.0 of 10

    An analytical model of Askaryan radiation plus detector response is shown to match 13 ARA UHECR candidate waveforms with correlations 0.69-0.86.

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