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As of 2023, the low-frequency part of the Square Kilometre Array will goonline in Australia. It will constitute the largest and most powerfullow-frequency radio-astronomical observatory to date, and will facilitate arich science programme in astronomy and astrophysics. With modest engineeringchanges, it will also be able to measure cosmic rays via the radio emissionfrom extensive air showers. The extreme antenna density and the homogeneouscoverage provided by more than 60,000 antennas within an area of one km$^2$will push radio detection of cosmic rays in the energy range around 10$^{17}$eV to ultimate precision, with superior capabilities in the reconstruction ofarrival direction, energy, and an expected depth-of-shower-maximum resolutionof 6~g/cm${^2}$.

Ultimate precision in cosmic-ray radio detection --- the SKA