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The LUNASKA (Lunar UHE Neutrino Astrophysics with the Square Kilometre Array)project is a theoretical and experimental project developing the lunarCherenkov technique for the next generation of giant radio-telescope arrays.This contribution presents our simulation results on the directional dependenceof the technique for UHE neutrino detection. In particular, these indicate thatboth the instantaneous sensitivities and time-integrated limits from lunarCherenkov experiments such as those at Parkes, Goldstone, Kalyazin and ATCA arehighly anisotropic. We study the regions of the sky which have not been probedby either these or other experiments, and present the expected sky coverage offuture experiments with the SKA. Our results show how the sensitivity of LunarCherenkov observations to potential astrophysical sources of UHE particles maybe maximised by choosing appropriate observations dates and antenna-beampointing positions.

The Directional Dependence of the Lunar Cherenkov Technique for UHE Neutrino Detection