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...
Main Authors: | , , , , , , , , , , , , , , , |
---|---|
Format: | Article in Journal/Newspaper |
Language: | unknown |
Published: |
eScholarship, University of California
2015
|
Subjects: | |
Online Access: | https://escholarship.org/uc/item/5t31q0w2 |
id |
ftcdlib:oai:escholarship.org/ark:/13030/qt5t31q0w2 |
---|---|
record_format |
openpolar |
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 |
_version_ |
1766256403732758528 |