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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Main Authors: Allen, C, Bean, A, Besson, D, Frichter, G, Kotov, S A, Kravchenko, I V, McKay, D, Miller, T, Piccirillo, L, Ralston, J P, Seckel, D, Seunarine, S, Spiczak, G M
Language:English
Published: 1997
Subjects:
Astrophysics and Astronomy
Austral
South Pole
South pole
Online Access:http://cds.cern.ch/record/334536
id ftcern:oai:cds.cern.ch:334536
record_format openpolar
spelling ftcern:oai:cds.cern.ch:334536 2023-05-15T18:22:03+02:00 Status of Radio Ice Cherenkov Experiment (RICE) Allen, C Bean, A Besson, D Frichter, G Kotov, S A Kravchenko, I V McKay, D Miller, T Piccirillo, L Ralston, J P Seckel, D Seunarine, S Spiczak, G M 1997-09-24 http://cds.cern.ch/record/334536 eng eng http://cds.cern.ch/record/334536 astro-ph/9709223 oai:cds.cern.ch:334536 Astrophysics and Astronomy 1997 ftcern 2018-07-28T03:25:56Z 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. Other/Unknown Material South pole CERN Document Server (CDS) Austral South Pole
institution Open Polar
collection CERN Document Server (CDS)
op_collection_id ftcern
language English
topic Astrophysics and Astronomy
spellingShingle Astrophysics and Astronomy
Allen, C
Bean, A
Besson, D
Frichter, G
Kotov, S A
Kravchenko, I V
McKay, D
Miller, T
Piccirillo, L
Ralston, J P
Seckel, D
Seunarine, S
Spiczak, G M
Status of Radio Ice Cherenkov Experiment (RICE)
topic_facet Astrophysics and Astronomy
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.
author Allen, C
Bean, A
Besson, D
Frichter, G
Kotov, S A
Kravchenko, I V
McKay, D
Miller, T
Piccirillo, L
Ralston, J P
Seckel, D
Seunarine, S
Spiczak, G M
author_facet Allen, C
Bean, A
Besson, D
Frichter, G
Kotov, S A
Kravchenko, I V
McKay, D
Miller, T
Piccirillo, L
Ralston, J P
Seckel, D
Seunarine, S
Spiczak, G M
author_sort Allen, C
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)
publishDate 1997
url http://cds.cern.ch/record/334536
geographic Austral
South Pole
geographic_facet Austral
South Pole
genre South pole
genre_facet South pole
op_relation http://cds.cern.ch/record/334536
astro-ph/9709223
oai:cds.cern.ch:334536
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