Time-domain response of the ARIANNA detector.

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Title: Time-domain response of the ARIANNA detector.
Authors: Barwick, S.W.1, Berg, E.C.1, Besson, D.Z.2,3, Duffin, T.1, Hanson, J.C.1,2 j529h838@ku.edu, Klein, S.R.4, Kleinfelder, S.A.5, Piasecki, M.6, Ratzlaff, K.6, Reed, C.1, Roumi, M.5, Stezelberger, T.4, Tatar, J.1,7, Walker, J.1, Young, R.6, Zou, L.5
Source: Astroparticle Physics. Mar2015, Vol. 62, p139-151. 13p.
Subjects: Neutrino detectors, Neutrino astrophysics, Oscilloscopes, Cosmogenic nuclides, Time-domain analysis
Abstract: 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. [ABSTRACT FROM AUTHOR]
Copyright of Astroparticle Physics is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: Time-domain response of the ARIANNA detector.
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  Data: 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. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of Astroparticle Physics is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1016/j.astropartphys.2014.09.002
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      – Code: eng
        Text: English
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        PageCount: 13
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      – SubjectFull: Neutrino detectors
        Type: general
      – SubjectFull: Neutrino astrophysics
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      – SubjectFull: Oscilloscopes
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      – SubjectFull: Cosmogenic nuclides
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      – SubjectFull: Time-domain analysis
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      – TitleFull: Time-domain response of the ARIANNA detector.
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