Status of the AMANDA South Pole Neutrino Detector

Initial deployment of optical modules near 1 and 2 kilometer depth indicate that deep polar ice is the most transparent known natural solid. Experience with early data has revealed that a detector, conceived to measure muons tracks, can also measure energy of high energy neutrinos as well as bursts...

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Bibliographic Details
Main Author: Halzen, Francis
Language:English
Published: 1996
Subjects:
Online Access:http://cds.cern.ch/record/315211
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spelling ftcern:oai:cds.cern.ch:315211 2023-05-15T18:22:12+02:00 Status of the AMANDA South Pole Neutrino Detector Halzen, Francis 1996-11-19 http://cds.cern.ch/record/315211 eng eng http://cds.cern.ch/record/315211 hep-ex/9611014 MAD-PH-977 oai:cds.cern.ch:315211 Particle Physics - Experiment 1996 ftcern 2018-07-28T03:11:39Z Initial deployment of optical modules near 1 and 2 kilometer depth indicate that deep polar ice is the most transparent known natural solid. Experience with early data has revealed that a detector, conceived to measure muons tracks, can also measure energy of high energy neutrinos as well as bursts of MeV neutrinos, e.g. produced by supernovae and gamma ray bursts. We plan to complete AMANDA this austral summer to form a detector of 11 deep strings instrumented over 400 meters height with 300 optical modules. We will argue that ice is the ideal medium to deploy a future kilometer-scale detector and discuss the first deployment of 10 strings of kilometer length. 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 Particle Physics - Experiment
spellingShingle Particle Physics - Experiment
Halzen, Francis
Status of the AMANDA South Pole Neutrino Detector
topic_facet Particle Physics - Experiment
description Initial deployment of optical modules near 1 and 2 kilometer depth indicate that deep polar ice is the most transparent known natural solid. Experience with early data has revealed that a detector, conceived to measure muons tracks, can also measure energy of high energy neutrinos as well as bursts of MeV neutrinos, e.g. produced by supernovae and gamma ray bursts. We plan to complete AMANDA this austral summer to form a detector of 11 deep strings instrumented over 400 meters height with 300 optical modules. We will argue that ice is the ideal medium to deploy a future kilometer-scale detector and discuss the first deployment of 10 strings of kilometer length.
author Halzen, Francis
author_facet Halzen, Francis
author_sort Halzen, Francis
title Status of the AMANDA South Pole Neutrino Detector
title_short Status of the AMANDA South Pole Neutrino Detector
title_full Status of the AMANDA South Pole Neutrino Detector
title_fullStr Status of the AMANDA South Pole Neutrino Detector
title_full_unstemmed Status of the AMANDA South Pole Neutrino Detector
title_sort status of the amanda south pole neutrino detector
publishDate 1996
url http://cds.cern.ch/record/315211
geographic Austral
South Pole
geographic_facet Austral
South Pole
genre South pole
genre_facet South pole
op_relation http://cds.cern.ch/record/315211
hep-ex/9611014
MAD-PH-977
oai:cds.cern.ch:315211
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