PER OLOF HULTH FOR THE ICECUBE COLLABORATION a
The success of the AMANDA neutrino telescope has shown that the ice sheet at the geographical South Pole is a suitable medium for optical Cherenkov detection of high energy neutrino interactions. Several thousands of atmospheric neutrinos have been recorded by AMANDA and the sensitivity for cosmic n...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.256.667 2023-05-15T16:40:37+02:00 PER OLOF HULTH FOR THE ICECUBE COLLABORATION a From Amanda To Icecube The Pennsylvania State University CiteSeerX Archives 2006 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.667 http://arxiv.org/pdf/astro-ph/0604374v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.667 http://arxiv.org/pdf/astro-ph/0604374v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/0604374v1.pdf text 2006 ftciteseerx 2016-01-07T19:58:22Z The success of the AMANDA neutrino telescope has shown that the ice sheet at the geographical South Pole is a suitable medium for optical Cherenkov detection of high energy neutrino interactions. Several thousands of atmospheric neutrinos have been recorded by AMANDA and the sensitivity for cosmic neutrinos has continuously improved. So far no cosmic neutrino signals have been detected. The deployment of the much larger and more sensitive IceCube neutrino observatory has started and nine out of 80 strings have been installed. This paper summarizes some of the results obtained by the AMANDA telescope and presents the status of the IceCube project. 1. Text Ice Sheet South pole Unknown Hulth ENVELOPE(-64.183,-64.183,-66.683,-66.683) South Pole |
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ftciteseerx |
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English |
description |
The success of the AMANDA neutrino telescope has shown that the ice sheet at the geographical South Pole is a suitable medium for optical Cherenkov detection of high energy neutrino interactions. Several thousands of atmospheric neutrinos have been recorded by AMANDA and the sensitivity for cosmic neutrinos has continuously improved. So far no cosmic neutrino signals have been detected. The deployment of the much larger and more sensitive IceCube neutrino observatory has started and nine out of 80 strings have been installed. This paper summarizes some of the results obtained by the AMANDA telescope and presents the status of the IceCube project. 1. |
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The Pennsylvania State University CiteSeerX Archives |
format |
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author |
From Amanda To Icecube |
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From Amanda To Icecube PER OLOF HULTH FOR THE ICECUBE COLLABORATION a |
author_facet |
From Amanda To Icecube |
author_sort |
From Amanda To Icecube |
title |
PER OLOF HULTH FOR THE ICECUBE COLLABORATION a |
title_short |
PER OLOF HULTH FOR THE ICECUBE COLLABORATION a |
title_full |
PER OLOF HULTH FOR THE ICECUBE COLLABORATION a |
title_fullStr |
PER OLOF HULTH FOR THE ICECUBE COLLABORATION a |
title_full_unstemmed |
PER OLOF HULTH FOR THE ICECUBE COLLABORATION a |
title_sort |
per olof hulth for the icecube collaboration a |
publishDate |
2006 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.667 http://arxiv.org/pdf/astro-ph/0604374v1.pdf |
long_lat |
ENVELOPE(-64.183,-64.183,-66.683,-66.683) |
geographic |
Hulth South Pole |
geographic_facet |
Hulth South Pole |
genre |
Ice Sheet South pole |
genre_facet |
Ice Sheet South pole |
op_source |
http://arxiv.org/pdf/astro-ph/0604374v1.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.667 http://arxiv.org/pdf/astro-ph/0604374v1.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766031024227090432 |