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