  The High-Altitude Water Cherenkov (HAWC) Observatory is sensitive to gamma
rays and charged cosmic rays at TeV energies. The detector is still under
construction, but data acquisition with the partially deployed detector started
in 2013. An analysis of the cosmic-ray arrival direction distribution based on
$4.9\times 10^{10}$ events recorded between June 2013 and February 2014 shows
anisotropy at the $10^{-4}$ level on angular scales of about $10^\circ$. The
HAWC cosmic-ray sky map exhibits three regions of significantly enhanced
cosmic-ray flux; two of these regions were first reported by the Milagro
experiment. A third region coincides with an excess recently reported by the
ARGO-YBJ experiment. An angular power spectrum analysis of the sky shows that
all terms up to $\ell=15$ contribute significantly to the excesses.
