12–23 Jul 2021
Online
Europe/Berlin timezone

On the need for unbiasing azimuthal asymmetries in signals measured by surface detector arrays

16 Jul 2021, 18:00
1h 30m
TBA

TBA

Talk CRI | Cosmic Ray Indirect Discussion

Speaker

Dr Quentin Luce (IAP, Karlsruhe Institute of Technology (KIT))

Description

A surface detector array samples the lateral distribution of an extensive air-shower (EAS) at the ground, i.e. the density of particles as a function of the distance from the axis of the shower. The azimuthal symmetry of this measured lateral distribution is broken for EAS with a non-zero zenith angle. The resulting asymmetry, caused by atmospheric attenuation and geometrical effects, increases with the inclination of the shower and introduces a bias in the reconstruction of the shower parameters.
Using simulated sets of air-showers, we present a model to correct the azimuthal asymmetry in signals measured by water-Cherenkov detectors and exemplified using the geometry and detector response of the Pierre Auger Observatory. Testing showers initiated by proton and iron primaries using EPOS-LHC and QGSJetII-04 as hadronic models, we developed a fine-tuned model of the amplitude of the asymmetry as a function of the zenith angle, shower size and distance of a detector from the shower axis. The improvements resulting from the application of the correction are quantified in terms of the biases and resolutions in the impact-point and arrival direction.

Keywords

asymmetry, lateral distribution function, energy estimation, models of hadronic interactions, simulation of extensive air showers

Subcategory Theoretical Methods

Primary authors

Dr Quentin Luce (IAP, Karlsruhe Institute of Technology (KIT)) Dr Markus Roth (KIT) David Schmidt (Karlsruhe Institute of Technology) Dr Darko Veberic (IAP, Karlsruhe Institute of Technology)

Presentation materials