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A. Anker et al., Advances in Space Research (in press) (2019) [ 1903.01609 ]
Original
1903
Earlier work this paper cites.
C. Glaser et al., The European Physical Journal C 79 (2019) [ 1903.07023 ]
Original
1903
Earlier work this paper cites.
C. Welling, C. Glaser and A. Nelles, JCAP10(2019)075 [ 1905.11185 ]
Original
1905
Earlier work this paper cites.

Similar

C. Glaser et al., submitted to EPJ-C (2019) [ 1906.01670 ]
Original
1906
Cited alongside, same era.
C. Glaser et al. (ARIANNA collaboration), submitted to JCAP (2019) [ 1909.02677 ]
Original
1909
Cited alongside, same era.
G. Gaswint for the ARIANNA collaboration, PoS(ICRC2019)897 (2019)
2019
Cited alongside, same era.

Then

A. Nelles for the ARIANNA collaboration, PoS(ICRC2019)366 (2019)
2019
Closest in time.
P. Allison et al., Astroparticle Physics 108 (2019) 63
2019
Closest in time.

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2019

Neutrino direction and energy resolution of Askaryan detectors

Glaser, Christian

Understand

Detection of high-energy neutrinos via the radio technique allows for an exploration of the neutrino energy range from $\sim10^{16}$\~eV to $\sim10^{20}$\~eV with unprecedented precision.

These Askaryan detectors have matured in two pilot arrays (ARA and ARIANNA) and the construction of a large-scale detector is actively discussed in the community.
In this contribution, we present reconstruction techniques to determine the neutrino direction and energy from the observed few-nanoseconds short radio flashes and quantify the resolution of one of such detectors.
The reconstruction of the neutrino direction requires a precise measurement of both the signal direction as well as the signal polarization.