Measurement of horizontal air showers with the Auger Engineering Radio Array

Abstract

The Auger Engineering Radio Array (AERA), at the Pierre Auger Observatory in Argentina, measures the radio emission of extensive air showers in the 30-80 MHz frequency range. AERA consists of more than 150 antenna stations distributed over 17 km${}^2$. Together with the Auger surface detector, the fluorescence detector and the under-ground muon detector (AMIGA), AERA is able to measure cosmic rays with energies above 10${}^{17}$ eV in a hybrid detection mode. AERA is optimized for the detection of air showers up to 60${}^{\circ }$ zenith angle, however, using the reconstruction of horizontal air showers with the Auger surface array, very inclined showers can also be measured. In this contribution an analysis of the AERA data in the zenith angle range from 62${}^{\circ }$ to 80${}^{\circ }$ will be presented. CoREAS simulations predict radio emission footprints of several km${}^2$ for horizontal air showers, which are now confirmed by AERA measurements. This can lead to radio-based composition measurements and energy determination of horizontal showers in the future and the radio detection of neutrino induced showers is possible.

To be published in the Proceedings of the ARENA2016 conference, Groningen, The Netherlands

References in corpus (1)

• Radio detection of cosmic ray air showers in the digital era

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