Abstract
The current generation of air shower radio arrays has demonstrated that the atmospheric depth of the shower maximum Xmax can be reconstructed with high accuracy. These experiments are now contributing to mass composition studies in the energy range where a transition from galactic to extragalactic cosmic-ray sources is expected. However, we are still far away from an unambiguous interpretation of the data. Here we propose to use radio measurements to derive a new type of constraint on the mass composition, by reconstructing the shower length L. The low-frequency part of the Square Kilometer Array will have an extremely high antenna density of roughly 60.000 antennas within one square kilometer, and is the perfect site for high-resolution studies of air showers. In this contribution, we discuss the impact of being able to reconstruct L, and the unique contribution that SKA can make to cosmic-ray science.
| Original language | British English |
|---|---|
| Article number | 046 |
| Journal | Proceedings of Science |
| Volume | 424 |
| State | Published - 25 Oct 2023 |
| Event | 9th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities, ARENA 2022 - Santiago de Compostela, Spain Duration: 7 Jun 2022 → 10 Jun 2022 |