  In-ice radio detectors are a promising tool for the discovery of EeV
neutrinos. For astrophysics, the implications of such a discovery will rely on
the reconstruction of the neutrino arrival direction. This paper describes a
first complete neutrino arrival direction reconstruction for detectors
employing deep antennas such as RNO-G or planning to employ them like
IceCube-Gen2. We will didactically introduce the challenges of neutrino
direction reconstruction using radio emission in ice, elaborate on the detail
of the algorithm used, and describe the obtainable performance based on a
simulation study and discuss its implication for astrophysics.
