Affordable Access

Access to the full text

Time Domain Response of the ARIANNA Detector

Authors
  • Barwick, S. W.
  • Berg, E. C.
  • Besson, D. Z.
  • Hanson, J. C.
  • Klein, S. R.
  • Kleinfelder, S. A.
  • Piasecki, M.
  • Ratzlaff, K.
  • Reed, C.
  • Roumi, M.
  • Stezelberger, T.
  • Tatar, J.
  • Walker, J.
  • Young, R.
  • Zou, L.
Type
Published Article
Publication Date
Oct 20, 2014
Submission Date
Jun 03, 2014
Identifiers
DOI: 10.1016/j.astropartphys.2014.09.002
Source
arXiv
License
Yellow
External links

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.

Report this publication

Statistics

Seen <100 times