  We simulate three-dimensional, horizontally periodic Rayleigh-B\'enard
convection between free-slip horizontal plates, rotating about a distant
horizontal axis. When both the temperature difference between the plates and
the rotation rate are sufficiently large, a strong horizontal wind is generated
that is perpendicular to both the rotation vector and the gravity vector. The
wind is turbulent, large-scale, and vertically sheared. Horizontal anisotropy,
engendered here by rotation, appears necessary for such wind generation. Most
of the kinetic energy of the flow resides in the wind, and the vertical
turbulent heat flux is much lower on average than when there is no wind.
