Radio-interferometric Neutrino Reconstruction for the Askaryan Radio Array
The Askaryan Radio Array (ARA) is a neutrino telescope array under phased deployment near the South Pole. The array aims to discover and determine the ultra-high energy neutrino flux via detection of the Askaryan signal from neutrino-induced showers. This novel detection channel makes ARA the most c...
Main Author: | Lu Ming-Yuan |
---|---|
Format: | Article |
Language: | English |
Published: |
EDP Sciences
2017-01-01
|
Series: | EPJ Web of Conferences |
Online Access: | https://doi.org/10.1051/epjconf/201713505003 |
Similar Items
-
A search for cosmogenic neutrinos with the Askaryan Radio Array
by: Davies, J. P.
Published: (2014) -
Simulation of the Event Reconstruction ofUltra High Energy Neutrino with Askaryan Radio Array
by: Shang-Yu Sun, et al.
Published: (2010) -
Simulation of Askaryan Radio Array Neutrino Events for the Identification of Flavor Ratios
by: Shi-Hao Wang, et al.
Published: (2012) -
Optimization of the Configuration of Askaryan Radio Array Observatory
by: Hsin-Yi Tu, et al.
Published: (2012) -
Searching for Ultra-high Energy Neutrinos with Data from a Prototype Station of the Askaryan Radio Array
by: Hong, Eugene S.
Published: (2014)