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Digital radio arrays have become an effective tool to measure air showers atenergies around and above 100 PeV. Compared to optical techniques, the radiotechnique is not restricted to clear nights. Thanks to recent progress oncomputational analysis techniques, radio arrays can provide an equally accuratemeasurement of the energy and the depth of the shower maximum. Stand-aloneradio arrays offer an economic way towards huge apertures, e.g., for the searchfor ultra-high-energy neutrinos, but still require technical demonstration onlarge scales. Hybrid arrays combining radio antennas and particle detectorshave already started to contribute to cosmic-ray physics in the energy range ofthe presumed Galactic-to-extragalactic transition. In particular, thecombination of radio and muon detectors can pave a path to unprecedentedaccuracy for the mass composition of cosmic rays. This proceeding reviewsrecent developments regarding the radio technique and highlights selectedrunning and planned antennas arrays, such as GCOS, GRAND, the SKA, theAugerPrime Upgrade of the Pierre Auger Observatory, and IceCube-Gen2.

Digital Radio Arrays for the Detection of Air Showers Initiated by Ultra-High-Energy Particles (Epiphany 2022)