Time-domain response of the ARIANNA detector

The Antarctic Ross Ice Shelf Antenna Neutrino Array (ARIANNA) is a high-energy neutrino detector designed to record the Askaryan electric field signature of cosmogenic neutrino interactions in ice. To understand the inherent radio-frequency (RF) neutrino signature, the time-domain response of the AR...

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Main Authors: Barwick, SW, Berg, EC, Besson, DZ, Duffin, T, Hanson, JC, Klein, SR, Kleinfelder, SA, Piasecki, M, Ratzlaff, K, Reed, C, Roumi, M, Stezelberger, T, Tatar, J, Walker, J, Young, R, Zou, L
Format: Article in Journal/Newspaper
Language:unknown
Published: eScholarship, University of California 2015
Subjects:
Online Access:https://escholarship.org/uc/item/5t31q0w2
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spelling ftcdlib:oai:escholarship.org/ark:/13030/qt5t31q0w2 2023-05-15T13:52:09+02:00 Time-domain response of the ARIANNA detector Barwick, SW Berg, EC Besson, DZ Duffin, T Hanson, JC Klein, SR Kleinfelder, SA Piasecki, M Ratzlaff, K Reed, C Roumi, M Stezelberger, T Tatar, J Walker, J Young, R Zou, L 2015-01-01 application/pdf https://escholarship.org/uc/item/5t31q0w2 unknown eScholarship, University of California qt5t31q0w2 https://escholarship.org/uc/item/5t31q0w2 public GZK neutrinos Askaryan effect Radio detector astro-ph.IM astro-ph.HE Astronomical and Space Sciences Atomic Molecular Nuclear Particle and Plasma Physics Nuclear & Particles Physics article 2015 ftcdlib 2021-08-16T17:10:20Z The Antarctic Ross Ice Shelf Antenna Neutrino Array (ARIANNA) is a high-energy neutrino detector designed to record the Askaryan electric field signature of cosmogenic neutrino interactions in ice. To understand the inherent radio-frequency (RF) neutrino signature, the time-domain response of the ARIANNA RF receiver must be measured. ARIANNA uses Create CLP5130-2N log-periodic dipole arrays (LPDAs). The associated effective height operator converts incident electric fields to voltage waveforms at the LDPA terminals. The effective height versus time and incident angle was measured, along with the associated response of the ARIANNA RF amplifier. The results are verified by correlating to field measurements in air and ice, using oscilloscopes. Finally, theoretical models for the Askaryan electric field are combined with the detector response to predict the neutrino signature. Article in Journal/Newspaper Antarc* Antarctic Ice Shelf Ross Ice Shelf University of California: eScholarship Antarctic Ross Ice Shelf The Antarctic
institution Open Polar
collection University of California: eScholarship
op_collection_id ftcdlib
language unknown
topic GZK neutrinos
Askaryan effect
Radio detector
astro-ph.IM
astro-ph.HE
Astronomical and Space Sciences
Atomic
Molecular
Nuclear
Particle and Plasma Physics
Nuclear & Particles Physics
spellingShingle GZK neutrinos
Askaryan effect
Radio detector
astro-ph.IM
astro-ph.HE
Astronomical and Space Sciences
Atomic
Molecular
Nuclear
Particle and Plasma Physics
Nuclear & Particles Physics
Barwick, SW
Berg, EC
Besson, DZ
Duffin, T
Hanson, JC
Klein, SR
Kleinfelder, SA
Piasecki, M
Ratzlaff, K
Reed, C
Roumi, M
Stezelberger, T
Tatar, J
Walker, J
Young, R
Zou, L
Time-domain response of the ARIANNA detector
topic_facet GZK neutrinos
Askaryan effect
Radio detector
astro-ph.IM
astro-ph.HE
Astronomical and Space Sciences
Atomic
Molecular
Nuclear
Particle and Plasma Physics
Nuclear & Particles Physics
description The Antarctic Ross Ice Shelf Antenna Neutrino Array (ARIANNA) is a high-energy neutrino detector designed to record the Askaryan electric field signature of cosmogenic neutrino interactions in ice. To understand the inherent radio-frequency (RF) neutrino signature, the time-domain response of the ARIANNA RF receiver must be measured. ARIANNA uses Create CLP5130-2N log-periodic dipole arrays (LPDAs). The associated effective height operator converts incident electric fields to voltage waveforms at the LDPA terminals. The effective height versus time and incident angle was measured, along with the associated response of the ARIANNA RF amplifier. The results are verified by correlating to field measurements in air and ice, using oscilloscopes. Finally, theoretical models for the Askaryan electric field are combined with the detector response to predict the neutrino signature.
format Article in Journal/Newspaper
author Barwick, SW
Berg, EC
Besson, DZ
Duffin, T
Hanson, JC
Klein, SR
Kleinfelder, SA
Piasecki, M
Ratzlaff, K
Reed, C
Roumi, M
Stezelberger, T
Tatar, J
Walker, J
Young, R
Zou, L
author_facet Barwick, SW
Berg, EC
Besson, DZ
Duffin, T
Hanson, JC
Klein, SR
Kleinfelder, SA
Piasecki, M
Ratzlaff, K
Reed, C
Roumi, M
Stezelberger, T
Tatar, J
Walker, J
Young, R
Zou, L
author_sort Barwick, SW
title Time-domain response of the ARIANNA detector
title_short Time-domain response of the ARIANNA detector
title_full Time-domain response of the ARIANNA detector
title_fullStr Time-domain response of the ARIANNA detector
title_full_unstemmed Time-domain response of the ARIANNA detector
title_sort time-domain response of the arianna detector
publisher eScholarship, University of California
publishDate 2015
url https://escholarship.org/uc/item/5t31q0w2
geographic Antarctic
Ross Ice Shelf
The Antarctic
geographic_facet Antarctic
Ross Ice Shelf
The Antarctic
genre Antarc*
Antarctic
Ice Shelf
Ross Ice Shelf
genre_facet Antarc*
Antarctic
Ice Shelf
Ross Ice Shelf
op_relation qt5t31q0w2
https://escholarship.org/uc/item/5t31q0w2
op_rights public
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