IceTop - Cosmic Ray Physics with IceCube
The IceCube experiment at South Pole consists of two detector components - the IceTop air shower array on the surface and the neutrino telescope at depths from 1450 m to 2450 m below. Currently, 26 IceTop stations and 22 InIce strings are deployed. With the present size of the IceTop array, it is po...
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ftdatacite:10.48550/arxiv.0802.2540 2023-05-15T18:22:16+02:00 IceTop - Cosmic Ray Physics with IceCube Waldenmaier, Tilo 2008 https://dx.doi.org/10.48550/arxiv.0802.2540 https://arxiv.org/abs/0802.2540 unknown arXiv https://dx.doi.org/10.1016/j.nima.2008.01.015 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2008 ftdatacite https://doi.org/10.48550/arxiv.0802.2540 https://doi.org/10.1016/j.nima.2008.01.015 2022-04-01T15:57:26Z The IceCube experiment at South Pole consists of two detector components - the IceTop air shower array on the surface and the neutrino telescope at depths from 1450 m to 2450 m below. Currently, 26 IceTop stations and 22 InIce strings are deployed. With the present size of the IceTop array, it is possible to measure cosmic rays with energies ranging from 0.5 to 100 PeV. Coincident events between the IceTop and the InIce detector provide useful cross-checks of the detector performance and furthermore make it possible to study the cosmic-ray composition. This paper gives an overview on the current status of IceTop. : 4 pages, 6 figures. Talk at Roma International Conference on Astroparticle Physics, June 2007 Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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DataCite Metadata Store (German National Library of Science and Technology) |
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Astrophysics astro-ph FOS Physical sciences |
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Astrophysics astro-ph FOS Physical sciences Waldenmaier, Tilo IceTop - Cosmic Ray Physics with IceCube |
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Astrophysics astro-ph FOS Physical sciences |
description |
The IceCube experiment at South Pole consists of two detector components - the IceTop air shower array on the surface and the neutrino telescope at depths from 1450 m to 2450 m below. Currently, 26 IceTop stations and 22 InIce strings are deployed. With the present size of the IceTop array, it is possible to measure cosmic rays with energies ranging from 0.5 to 100 PeV. Coincident events between the IceTop and the InIce detector provide useful cross-checks of the detector performance and furthermore make it possible to study the cosmic-ray composition. This paper gives an overview on the current status of IceTop. : 4 pages, 6 figures. Talk at Roma International Conference on Astroparticle Physics, June 2007 |
format |
Text |
author |
Waldenmaier, Tilo |
author_facet |
Waldenmaier, Tilo |
author_sort |
Waldenmaier, Tilo |
title |
IceTop - Cosmic Ray Physics with IceCube |
title_short |
IceTop - Cosmic Ray Physics with IceCube |
title_full |
IceTop - Cosmic Ray Physics with IceCube |
title_fullStr |
IceTop - Cosmic Ray Physics with IceCube |
title_full_unstemmed |
IceTop - Cosmic Ray Physics with IceCube |
title_sort |
icetop - cosmic ray physics with icecube |
publisher |
arXiv |
publishDate |
2008 |
url |
https://dx.doi.org/10.48550/arxiv.0802.2540 https://arxiv.org/abs/0802.2540 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.1016/j.nima.2008.01.015 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.0802.2540 https://doi.org/10.1016/j.nima.2008.01.015 |
_version_ |
1766201650069897216 |