Design and Performance of the ARIANNA Hexagonal Radio Array Systems

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 la...

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Main Authors: Barwick, S. W., Berg, E. C., Besson, D. Z., Cheim, E., Duffin, T., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Prakash, T., Piasecki, M., Ratzlaff, K., Reed, C., Roumi, M., Samanta, A., Stezelberger, T., Tatar, J., Walker, J., Young, R., Zou, L.
Format: Report
Language:unknown
Published: arXiv 2014
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.1410.7369
https://arxiv.org/abs/1410.7369
id ftdatacite:10.48550/arxiv.1410.7369
record_format openpolar
spelling ftdatacite:10.48550/arxiv.1410.7369 2023-05-15T14:02:26+02:00 Design and Performance of the ARIANNA Hexagonal Radio Array Systems Barwick, S. W. Berg, E. C. Besson, D. Z. Cheim, E. Duffin, T. Hanson, J. C. Klein, S. R. Kleinfelder, S. A. Prakash, T. Piasecki, M. Ratzlaff, K. Reed, C. Roumi, M. Samanta, A. Stezelberger, T. Tatar, J. Walker, J. Young, R. Zou, L. 2014 https://dx.doi.org/10.48550/arxiv.1410.7369 https://arxiv.org/abs/1410.7369 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Instrumentation and Methods for Astrophysics astro-ph.IM Instrumentation and Detectors physics.ins-det FOS Physical sciences Preprint Article article CreativeWork 2014 ftdatacite https://doi.org/10.48550/arxiv.1410.7369 2022-04-01T12:49:34Z 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 station's pattern-trigger capabilities reduce the trigger rates to a few milli-Hertz with 4-sigma thresholds while retaining good stability and high efficiency for neutrino signals. The timing resolution of the station has been found to be 0.049 ps, RMS, and the angular precision of event reconstructions of signals bounced off of the sea-ice interface of the Ross Ice Shelf ranged from 0.14 to 0.17 degrees. A new fully-synchronous 2+ G-sample/s, 1.5 GHz bandwidth 4-channel signal acquisition chip with deeper memory and flexible >600 MHz, <1 mV RMS sensitivity triggering has been designed and incorporated into a single-board data acquisition and control system that uses an average of only 1.7W of power. Along with updated amplifiers, these new systems are expected to be deployed during the 2014-2015 Austral summer to complete the Hexagonal Radio Array. : 17 Page, 27 Figures, 1 Table Report Antarc* Antarctica Ice Shelf Ross Ice Shelf Sea ice DataCite Metadata Store (German National Library of Science and Technology) Austral Ross Ice Shelf
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Instrumentation and Methods for Astrophysics astro-ph.IM
Instrumentation and Detectors physics.ins-det
FOS Physical sciences
spellingShingle Instrumentation and Methods for Astrophysics astro-ph.IM
Instrumentation and Detectors physics.ins-det
FOS Physical sciences
Barwick, S. W.
Berg, E. C.
Besson, D. Z.
Cheim, E.
Duffin, T.
Hanson, J. C.
Klein, S. R.
Kleinfelder, S. A.
Prakash, T.
Piasecki, M.
Ratzlaff, K.
Reed, C.
Roumi, M.
Samanta, A.
Stezelberger, T.
Tatar, J.
Walker, J.
Young, R.
Zou, L.
Design and Performance of the ARIANNA Hexagonal Radio Array Systems
topic_facet Instrumentation and Methods for Astrophysics astro-ph.IM
Instrumentation and Detectors physics.ins-det
FOS Physical sciences
description 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 station's pattern-trigger capabilities reduce the trigger rates to a few milli-Hertz with 4-sigma thresholds while retaining good stability and high efficiency for neutrino signals. The timing resolution of the station has been found to be 0.049 ps, RMS, and the angular precision of event reconstructions of signals bounced off of the sea-ice interface of the Ross Ice Shelf ranged from 0.14 to 0.17 degrees. A new fully-synchronous 2+ G-sample/s, 1.5 GHz bandwidth 4-channel signal acquisition chip with deeper memory and flexible >600 MHz, <1 mV RMS sensitivity triggering has been designed and incorporated into a single-board data acquisition and control system that uses an average of only 1.7W of power. Along with updated amplifiers, these new systems are expected to be deployed during the 2014-2015 Austral summer to complete the Hexagonal Radio Array. : 17 Page, 27 Figures, 1 Table
format Report
author Barwick, S. W.
Berg, E. C.
Besson, D. Z.
Cheim, E.
Duffin, T.
Hanson, J. C.
Klein, S. R.
Kleinfelder, S. A.
Prakash, T.
Piasecki, M.
Ratzlaff, K.
Reed, C.
Roumi, M.
Samanta, A.
Stezelberger, T.
Tatar, J.
Walker, J.
Young, R.
Zou, L.
author_facet Barwick, S. W.
Berg, E. C.
Besson, D. Z.
Cheim, E.
Duffin, T.
Hanson, J. C.
Klein, S. R.
Kleinfelder, S. A.
Prakash, T.
Piasecki, M.
Ratzlaff, K.
Reed, C.
Roumi, M.
Samanta, A.
Stezelberger, T.
Tatar, J.
Walker, J.
Young, R.
Zou, L.
author_sort Barwick, S. W.
title Design and Performance of the ARIANNA Hexagonal Radio Array Systems
title_short Design and Performance of the ARIANNA Hexagonal Radio Array Systems
title_full Design and Performance of the ARIANNA Hexagonal Radio Array Systems
title_fullStr Design and Performance of the ARIANNA Hexagonal Radio Array Systems
title_full_unstemmed Design and Performance of the ARIANNA Hexagonal Radio Array Systems
title_sort design and performance of the arianna hexagonal radio array systems
publisher arXiv
publishDate 2014
url https://dx.doi.org/10.48550/arxiv.1410.7369
https://arxiv.org/abs/1410.7369
geographic Austral
Ross Ice Shelf
geographic_facet Austral
Ross Ice Shelf
genre Antarc*
Antarctica
Ice Shelf
Ross Ice Shelf
Sea ice
genre_facet Antarc*
Antarctica
Ice Shelf
Ross Ice Shelf
Sea ice
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1410.7369
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