Retrofitted Digital Optical Modules for the Radio Detection of Neutrinos in Ice

Details Retrofitted Digital Optical Modules for the Radio Detection of Neutrinos in Ice Retrofitted Digital Optical Modules for the Radio Detection of Neutrinos in Ice

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jphcs..81a2024w&link_type=abstract

Journal of Physics: Conference Series, Volume 81, Issue 1, pp. 012024 (2007).

Physics

Scientific paper

The Askaryan Underice Radio Array (AURA) is a proposed next-generation radio neutrino detector for the South Pole, which succeeds the existing Radio Ice Cherenkov Experiment (RICE). In the 2006/7 IceCube deployment season, AURA will co-deploy new radio antennas. I describe the Digital Optical Module (DRM), which will incorporate triggering and data-handling in-ice, using both IceCube and radio technology.

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