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The IceCube Observatory provides our highest-statistics picture of thecosmic-ray arrival directions in the Southern Hemisphere, with over 700 billioncosmic-ray-induced muon events collected between May 2011 and May 2022. Usingthe larger data volume, we find an improved significance of the PeV cosmic rayanisotropy down to scales of $6^\circ$. In addition, we observe a variation inthe angular power spectrum as a function of energy, hinting at a relativedecrease in large-scale features above 100 TeV. The data-taking period covers acomplete solar cycle, providing new insight into the time variability of thesignal. We present preliminary results using this up-to-date event sample.

Cosmic Ray Anisotropy with 11 Years of IceCube Data