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A Monte Carlo simulation program for the radio detection of Ultra High Energy(UHE) neutrino interactions in the Antarctic ice as viewed by the AntarcticImpulsive Transient Antenna (ANITA) is described in this article. The program,icemc, provides an input spectrum of UHE neutrinos, the parametrization of theAskaryan radiation generated by their interaction in the ice, and thepropagation of the radiation through ice and air to a simulated model of thethird and fourth ANITA flights. This paper provides an overview of the icemcsimulation, descriptions of the physics models used and of the ANITAelectronics processing chain, data/simulation comparisons to validate thepredicted performance, and a summary of the impact of published results.

journal of instrumentation

The Simulation of the Sensitivity of the Antarctic Impulsive Transient  Antenna (ANITA) to Askaryan Radiation from Cosmogenic Neutrinos Interacting  in the Antarctic Ice