A scale factor derived from CoREAS radio emission simulations correlates with primary energy and enables reconstruction with ~11% error largely independent of core position.
Aab, et al., the Pierre Auger Collaboration, Energy estimation of cosmic rays with the en- gineering radio array of the pierre auger ob- servatory, Phys
2 Pith papers cite this work. Polarity classification is still indexing.
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Feasibility proposal for SKA-Low radio detection of PeV gamma-ray air showers from galactic PeVatrons.
citing papers explorer
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Energy estimation of cosmic rays by air shower radio signals
A scale factor derived from CoREAS radio emission simulations correlates with primary energy and enables reconstruction with ~11% error largely independent of core position.
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Using SKA-Low to Detect PeV Gamma-rays from Galactic Sources
Feasibility proposal for SKA-Low radio detection of PeV gamma-ray air showers from galactic PeVatrons.