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.
Title resolution pending
5 Pith papers cite this work. Polarity classification is still indexing.
5
Pith papers citing it
years
2026 5verdicts
UNVERDICTED 5representative citing papers
SKA-Low is projected to reconstruct cosmic-ray air-shower depth of maximum with better than 8 g/cm² resolution and enable full reconstruction down to PeV energies via radio detection.
Feasibility proposal for SKA-Low radio detection of PeV gamma-ray air showers from galactic PeVatrons.
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.
Information Field Theory is presented as a framework for full-information reconstruction and near-field interferometry of air-shower radio emission.
citing papers explorer
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Interferometric Analysis of Air-shower Radio Emission in the Near Field with an Information Field Theory Approach
Information Field Theory is presented as a framework for full-information reconstruction and near-field interferometry of air-shower radio emission.