PoS - Proceedings of Science
Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Neutrino. NU-instrumentation
Interferometric Neutrino Event Reconstruction in Inhomogeneous Media with the Askaryan Radio Array
J. Kelley*, M. Beheler-Amass, M. Beydler, A. Karle, M.Y. Lu and  for the ARA Collaboration
Full text: pdf
Pre-published on: August 16, 2017
Published on: August 03, 2018
The Askaryan Radio Array (ARA) is an ultra-high-energy (UHE) neutrino detector under construction at the South Pole. Using antennas deployed up to 200m deep in the ice, ARA searches for the impulsive Askaryan radio signals from UHE neutrino interactions. Directional reconstruction of these events is complicated by the inhomogeneity of the polar ice cap, causing the radio waves to bend as they travel through less dense regions close to the surface. To deal with the computational challenges involved, we have developed a spline-based scheme for fast lookup of pre-calculated raytracing results in the ice and air, combined with a parallelized interferometric directional reconstruction. Using these techniques, we demonstrate an angular resolution of $O(1^\circ)$ for neutrino event reconstruction as well as a fast online event filter based on the cross-correlation of antenna signals.
DOI: https://doi.org/10.22323/1.301.1054
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.