SKA-Low can resolve double-bump air shower profiles to constrain hadronic interaction properties and cosmic-ray mass composition between 10^16 and 10^18 eV.
The Forward Physics Facility at the HL-LHC and its Synergies with Astroparticle Physics
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Anomalous Air Showers and What They Reveal About Hadronic Interactions and Cosmic-ray Masses
SKA-Low can resolve double-bump air shower profiles to constrain hadronic interaction properties and cosmic-ray mass composition between 10^16 and 10^18 eV.