Gamma-ray families featuring halos are predominantly (>96%) produced by protons and helium nuclei according to simulation comparisons, enabling estimation of their fraction in primary cosmic radiation.
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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.
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Origin of gamma-ray families accompanied by halos and detected in experiments with x-ray emulsion chambers
Gamma-ray families featuring halos are predominantly (>96%) produced by protons and helium nuclei according to simulation comparisons, enabling estimation of their fraction in primary cosmic radiation.
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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.