Cosmic Ray Results from the IceTop Air Shower Array

We report on the first results obtained with the IceTop air shower array on the cosmic ray energy spectrum and mass composition in the range of 1 PeV to 80 PeV. IceTop is the surface detector of the IceCube neutrino telescope currently under construction at the South Pole. A high sensitivity to the...

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Main Author: Kolanoski, Hermann
Format: Report
Language:unknown
Published: arXiv 2008
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.0810.3409
https://arxiv.org/abs/0810.3409
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spelling ftdatacite:10.48550/arxiv.0810.3409 2023-05-15T18:22:20+02:00 Cosmic Ray Results from the IceTop Air Shower Array Kolanoski, Hermann 2008 https://dx.doi.org/10.48550/arxiv.0810.3409 https://arxiv.org/abs/0810.3409 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics astro-ph FOS Physical sciences Preprint Article article CreativeWork 2008 ftdatacite https://doi.org/10.48550/arxiv.0810.3409 2022-04-01T15:15:15Z We report on the first results obtained with the IceTop air shower array on the cosmic ray energy spectrum and mass composition in the range of 1 PeV to 80 PeV. IceTop is the surface detector of the IceCube neutrino telescope currently under construction at the South Pole. A high sensitivity to the primary mass composition was observed by reconstructing showers at different zenith angles. Assuming only protons or iron nuclei as primary particles yields significantly different energy spectra for different zenith angle ranges, while only models with mixed composition, like the poly-gonato model, lead to the expected isotropic flux. The prospects of composition measurements with different, alternative methods using the full IceCube detector are also discussed. : Presented at ICHEP08, Philadelphia, USA, July 2008. 5 pages, PDFLaTeX, 6 pdf figures Report South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics astro-ph
FOS Physical sciences
spellingShingle Astrophysics astro-ph
FOS Physical sciences
Kolanoski, Hermann
Cosmic Ray Results from the IceTop Air Shower Array
topic_facet Astrophysics astro-ph
FOS Physical sciences
description We report on the first results obtained with the IceTop air shower array on the cosmic ray energy spectrum and mass composition in the range of 1 PeV to 80 PeV. IceTop is the surface detector of the IceCube neutrino telescope currently under construction at the South Pole. A high sensitivity to the primary mass composition was observed by reconstructing showers at different zenith angles. Assuming only protons or iron nuclei as primary particles yields significantly different energy spectra for different zenith angle ranges, while only models with mixed composition, like the poly-gonato model, lead to the expected isotropic flux. The prospects of composition measurements with different, alternative methods using the full IceCube detector are also discussed. : Presented at ICHEP08, Philadelphia, USA, July 2008. 5 pages, PDFLaTeX, 6 pdf figures
format Report
author Kolanoski, Hermann
author_facet Kolanoski, Hermann
author_sort Kolanoski, Hermann
title Cosmic Ray Results from the IceTop Air Shower Array
title_short Cosmic Ray Results from the IceTop Air Shower Array
title_full Cosmic Ray Results from the IceTop Air Shower Array
title_fullStr Cosmic Ray Results from the IceTop Air Shower Array
title_full_unstemmed Cosmic Ray Results from the IceTop Air Shower Array
title_sort cosmic ray results from the icetop air shower array
publisher arXiv
publishDate 2008
url https://dx.doi.org/10.48550/arxiv.0810.3409
https://arxiv.org/abs/0810.3409
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.0810.3409
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