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IceCube is a cubic-kilometer Cherenkov detector located in the deep ice atthe geographic South Pole. The dominant event yield in the deep ice detectorconsists of penetrating atmospheric muons produced in cosmic ray air showerswith energies above several 100 GeV. In addition, the surface array, IceTop,deployed above the IceCube deep ice detector, measures the electromagneticsignal and low-energy muons of the air shower. Hence, IceCube and IceTop yieldunique opportunities to study cosmic rays with large statistics in greatdetail. We discuss the latest results of air shower measurements from IceCubeand IceTop, including the energy spectrum of cosmic rays from 250 TeV up to theEeV range. We will also report a measurement of the cosmic ray mass compositionin the PeV to EeV range and show recent results from searches for PeV gamma raysources in the Southern Hemisphere. In addition, results from a full-skyanalysis of the cosmic ray anisotropy, using combined data from the IceCube andHAWC observatories, will be reported. Finally, we will present a measurement ofthe density of muons in the GeV range and discuss its consistency withpredictions from hadronic interaction models.

Recent Results of Cosmic Ray Measurements from IceCube and IceTop