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The lunar Cherenkov technique, which aims to detect the coherent Cherenkovradiation produced when UHE particles interact in the lunar regolith, was firstattempted with the Parkes radio-telescope in 1995, though the theory was notsufficiently developed at this time to calculate a limit on the UHE neutrinoflux from the non-observation. Since then, the technique has evolved to includeexperiments utilising lower frequencies, wider bandwidths, and entire arrays ofantenna. We develop a simulation to analyse the full range of experiments, andcalculate the UHE neutrino flux limit from the Parkes experiment, including thedirectional dependence. Our results suggest a methodology for planning futureobservations, and demonstrate how to utilise all available information on thenature of radio pulses from the Moon for the detection of UHE particles.

The Lunar Cherenkov Technique: From Parkes Onwards