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The IceCube Neutrino Observatory is a cubic-kilometer Cherenkov detector thatis deployed deep in the Antarctic ice at the South Pole. A square kilometercompanion surface detector, IceTop, located directly above in the in-ice array,measures cosmic-ray initiated extensive air showers with primary energiesbetween 100 TeV and 1 EeV. By combining the events measured by IceTop and thein-ice detectors of IceCube in coincidence, we can reconstruct the energyspectra for different primary mass groups. Therefore, we provide informationabout the origin of cosmic rays, in particular, in the transition region fromgalactic to extra-galactic origin of high-energy cosmic rays. In thiscontribution we present recent experimental results, as well as prospects bythe foreseen enhancement of the surface detectors of IceTop and the futureIceCube-Gen2 surface array.

Recent results of cosmic-ray studies with IceTop at the IceCube Neutrino