A scale factor derived from CoREAS radio emission simulations correlates with primary energy and enables reconstruction with ~11% error largely independent of core position.
Schoorlemmer, et al., Energy and flux measurements of ultra-high energy cos- mic rays observed during the first anita flight, Astropart
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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.