Status of Radio Ice Cherenkov Experiment (RICE)

RICE Collaboration; C. Allen; A. Bean; D. Besson; G. Frichter; S. Kotov; I. Kravchenko; D. McKay; T. Miller; L. Piccirillo; J. Ralston; D. Seckel; S. Seunarine; G. Spiczak

arXiv · astro-ph/9709223

Status of Radio Ice Cherenkov Experiment (RICE)

RICE Collaboration·C. Allen·A. Bean·D. Besson·G. Frichter·S. Kotov·I. Kravchenko·D. McKay·T. Miller·L. Piccirillo·J. Ralston·D. Seckel·S. Seunarine·G. Spiczak

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Abstract

RICE is designed to detect ultrahigh energy (>100 TeV) neutrinos from astrophysical sources. It will consist of an array of compact radio (100 to 1000 MHz) receivers buried in ice at the South Pole. During the 1995-96 and 1996-97 austral summers, several receivers transmitters were deployed in bore holes drilled for the AMANDA project, at depths of 141 to 260 m. This was the first in situ test of radio receivers in deep ice for neutrino astronomy.

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RICE Collaboration, C. Allen, A. Bean, D. Besson, G. Frichter, S. Kotov, I. Kravchenko, D. McKay, T. Miller, L. Piccirillo, J. Ralston, D. Seckel, S. Seunarine, G. Spiczak. 1997-09-23. Status of Radio Ice Cherenkov Experiment (RICE). https://arxiv.org/abs/astro-ph/9709223

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