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Short radio pulses can be measured from showers of both high-energy cosmicrays and neutrinos. While commonly several antenna stations are needed toreconstruct the energy of an air shower, we describe a novel method that relieson the radio signal measured in one antenna station only. Exploiting a broadfrequency bandwidth of $80-300$ MHz, we obtain a statistical energy resolutionof better than 15\% on a realistic Monte Carlo set. This method is both a steptowards energy reconstruction from the radio signal of neutrino inducedshowers, as well as a promising tool for cosmic-ray radio arrays. Especiallyfor hybrid arrays where the air shower geometry is provided by an independentdetector, this method provides a precise handle on the energy of the showereven with a sparse array.

Reconstructing the cosmic-ray energy from the radio signal measured in one single station