Status of Radio Ice Cherenkov Experiment (RICE)
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 bo...
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ftdatacite:10.48550/arxiv.astro-ph/9709223 2023-05-15T18:22:05+02:00 Status of Radio Ice Cherenkov Experiment (RICE) RICE Collaboration Allen, C. Bean, A. Besson, D. Frichter, G. Kotov, S. Kravchenko, I. McKay, D. Miller, T. Piccirillo, L. Ralston, J. Seckel, D. Seunarine, S. Spiczak, G. 1997 https://dx.doi.org/10.48550/arxiv.astro-ph/9709223 https://arxiv.org/abs/astro-ph/9709223 unknown arXiv Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences Preprint Article article CreativeWork 1997 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/9709223 2022-04-01T17:14:35Z 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. : 4 pages, LaTeX, epsfig.sty, wrapfig.sty Report South pole DataCite Metadata Store (German National Library of Science and Technology) Austral South Pole |
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topic |
Astrophysics astro-ph FOS Physical sciences |
spellingShingle |
Astrophysics astro-ph FOS Physical sciences RICE Collaboration Allen, C. Bean, A. Besson, D. Frichter, G. Kotov, S. Kravchenko, I. McKay, D. Miller, T. Piccirillo, L. Ralston, J. Seckel, D. Seunarine, S. Spiczak, G. Status of Radio Ice Cherenkov Experiment (RICE) |
topic_facet |
Astrophysics astro-ph FOS Physical sciences |
description |
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. : 4 pages, LaTeX, epsfig.sty, wrapfig.sty |
format |
Report |
author |
RICE Collaboration Allen, C. Bean, A. Besson, D. Frichter, G. Kotov, S. Kravchenko, I. McKay, D. Miller, T. Piccirillo, L. Ralston, J. Seckel, D. Seunarine, S. Spiczak, G. |
author_facet |
RICE Collaboration Allen, C. Bean, A. Besson, D. Frichter, G. Kotov, S. Kravchenko, I. McKay, D. Miller, T. Piccirillo, L. Ralston, J. Seckel, D. Seunarine, S. Spiczak, G. |
author_sort |
RICE Collaboration |
title |
Status of Radio Ice Cherenkov Experiment (RICE) |
title_short |
Status of Radio Ice Cherenkov Experiment (RICE) |
title_full |
Status of Radio Ice Cherenkov Experiment (RICE) |
title_fullStr |
Status of Radio Ice Cherenkov Experiment (RICE) |
title_full_unstemmed |
Status of Radio Ice Cherenkov Experiment (RICE) |
title_sort |
status of radio ice cherenkov experiment (rice) |
publisher |
arXiv |
publishDate |
1997 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/9709223 https://arxiv.org/abs/astro-ph/9709223 |
geographic |
Austral South Pole |
geographic_facet |
Austral South Pole |
genre |
South pole |
genre_facet |
South pole |
op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
op_doi |
https://doi.org/10.48550/arxiv.astro-ph/9709223 |
_version_ |
1766201437340041216 |