Tune In, Turn On, Drop Down or Catching Neutrinos in the Antarctic Icecap Among the most energetic cosmic rays incident on the earth are those, which may be produced by either massive black holes, which could exist at the centers of some galaxies (aka `Active Galactic Nuclei', or `AGN'), or perhaps Gamma-Ray Bursts (GRB). Additional ultra-high energy neutrinos may be produced by the (as-yet-unidentified) process responsible for the ultra-high energy cosmic rays observed in present Extensive Air Shower experiments, and anticipated for the future Auger Project. The Fly's Eye and Akeno Experiments have confirmed that particles of energy as high as 1020 eV are, indeed, present in the cosmic ray flux, suggesting an enormously energetic, yet mysteriously invisible source close to earth. We describe a new experimental effort to detect ultra high energy electron neutrinos through their interactions with ice molecules in the Antarctic icecap, based on the principle of `radio coherence'. Experimentally, we measure a long-wavelength (radio-frequency) pulse resulting from this interaction. A prototype experiment (Radio Ice Cerenkov Experiment, or `RICE') presently operating as part of the larger AMANDA effort at the South Pole is described.