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Reconstructing the cosmic-ray energy from the radio signal measured in one single station
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abstract
Short radio pulses can be measured from showers of both high-energy cosmic rays and neutrinos. While commonly several antenna stations are needed to reconstruct the energy of an air shower, we describe a novel method that relies on the radio signal measured in one antenna station only. Exploiting a broad frequency bandwidth of $80-300$ MHz, we obtain a statistical energy resolution of better than 15\% on a realistic Monte Carlo set. This method is both a step towards energy reconstruction from the radio signal of neutrino induced showers, as well as a promising tool for cosmic-ray radio arrays. Especially for hybrid arrays where the air shower geometry is provided by an independent detector, this method provides a precise handle on the energy of the shower even with a sparse array.
Forward citations
Cited by 3 Pith papers
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Likelihood Reconstruction for Radio Detectors of Neutrinos and Cosmic Rays
A multivariate-normal likelihood with a circulant noise covariance, derived from the noise spectrum, improves radio-detector reconstruction of neutrino and cosmic-ray parameters and yields correctly covered event-by-e...
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Universality and template synthesis of cosmic ray air shower radio emission
Air shower radio pulses can be synthesized from template simulations by slicing the cascade in atmospheric depth and rescaling each slice's amplitude spectrum via fits against shower maximum.
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A search for cosmogenic neutrinos with the ARIANNA test bed using 4.5 years of data
After 4.5 years of operation, the ARIANNA test bed found no neutrino candidates and set a 90% confidence upper limit of E^2 Phi = 1.7e-6 GeV cm^-2 s^-1 sr^-1 at 10^18 eV.
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