Performance and simulation of the RICE detector
The Radio Ice Cherenkov Experiment at the South Pole, co-deployed with the AMANDA experiment, seeks to detect ultra-high energy electron neutrinos interacting in cold polar ice. Such interactions produce electromagnetic showers, which emit radio-frequency Cherenkov radiation. We describe the experim...
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| Veröffentlicht in: | Astroparticle physics 2003-04, Vol.19 (1), p.15-36 |
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| container_title | Astroparticle physics |
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| creator | Kravchenko, I Frichter, G.M Seckel, D Spiczak, G.M Adams, J Seunarine, S Allen, C Bean, A Besson, D Box, D.J Buniy, R Drees, J McKay, D Meyers, J Perry, L Ralston, J Razzaque, S Schmitz, D.W |
| description | The Radio Ice Cherenkov Experiment at the South Pole, co-deployed with the AMANDA experiment, seeks to detect ultra-high energy electron neutrinos interacting in cold polar ice. Such interactions produce electromagnetic showers, which emit radio-frequency Cherenkov radiation. We describe the experimental apparatus and the procedures used to measure the neutrino flux. |
| doi_str_mv | 10.1016/S0927-6505(02)00194-9 |
| format | Article |
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| issn | 0927-6505 1873-2852 |
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| source | ScienceDirect Journals (5 years ago - present) |
| title | Performance and simulation of the RICE detector |
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