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.
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SKA-Low augmented with particle detectors is well suited to measure cosmic ray mass composition in the Galactic-extragalactic transition energy range, building on LOFAR experience.
citing papers explorer
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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.
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Origins of Cosmic Rays in the Galactic-extragalactic Transition Energy Range
SKA-Low augmented with particle detectors is well suited to measure cosmic ray mass composition in the Galactic-extragalactic transition energy range, building on LOFAR experience.