Solar Energetic Particle Spectrum on 13 December 2006 Determined by IceTop
On 13 December 2006 the IceTop air shower array at the South Pole detected a major solar particle event. By numerically simulating the response of the IceTop tanks, which are thick Cherenkov detectors with multiple thresholds deployed at high altitude with no geomagnetic cut-off, we determined the p...
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ftdatacite:10.48550/arxiv.0810.2034 2023-05-15T18:22:12+02:00 Solar Energetic Particle Spectrum on 13 December 2006 Determined by IceTop Abbasi, R. 2008 https://dx.doi.org/10.48550/arxiv.0810.2034 https://arxiv.org/abs/0810.2034 unknown arXiv https://dx.doi.org/10.1086/595679 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.0810.2034 https://doi.org/10.1086/595679 2022-04-01T15:13:49Z On 13 December 2006 the IceTop air shower array at the South Pole detected a major solar particle event. By numerically simulating the response of the IceTop tanks, which are thick Cherenkov detectors with multiple thresholds deployed at high altitude with no geomagnetic cut-off, we determined the particle energy spectrum in the energy range 0.6 to 7.6 GeV. This is the first such spectral measurement using a single instrument with a well defined viewing direction. We compare the IceTop spectrum and its time evolution with previously published results and outline plans for improved resolution of future solar particle spectra. : To appear in Astrophysical Journal Letters, 6 pages, 4 figures 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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topic |
Astrophysics astro-ph FOS Physical sciences |
spellingShingle |
Astrophysics astro-ph FOS Physical sciences Abbasi, R. Solar Energetic Particle Spectrum on 13 December 2006 Determined by IceTop |
topic_facet |
Astrophysics astro-ph FOS Physical sciences |
description |
On 13 December 2006 the IceTop air shower array at the South Pole detected a major solar particle event. By numerically simulating the response of the IceTop tanks, which are thick Cherenkov detectors with multiple thresholds deployed at high altitude with no geomagnetic cut-off, we determined the particle energy spectrum in the energy range 0.6 to 7.6 GeV. This is the first such spectral measurement using a single instrument with a well defined viewing direction. We compare the IceTop spectrum and its time evolution with previously published results and outline plans for improved resolution of future solar particle spectra. : To appear in Astrophysical Journal Letters, 6 pages, 4 figures |
format |
Text |
author |
Abbasi, R. |
author_facet |
Abbasi, R. |
author_sort |
Abbasi, R. |
title |
Solar Energetic Particle Spectrum on 13 December 2006 Determined by IceTop |
title_short |
Solar Energetic Particle Spectrum on 13 December 2006 Determined by IceTop |
title_full |
Solar Energetic Particle Spectrum on 13 December 2006 Determined by IceTop |
title_fullStr |
Solar Energetic Particle Spectrum on 13 December 2006 Determined by IceTop |
title_full_unstemmed |
Solar Energetic Particle Spectrum on 13 December 2006 Determined by IceTop |
title_sort |
solar energetic particle spectrum on 13 december 2006 determined by icetop |
publisher |
arXiv |
publishDate |
2008 |
url |
https://dx.doi.org/10.48550/arxiv.0810.2034 https://arxiv.org/abs/0810.2034 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.1086/595679 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.0810.2034 https://doi.org/10.1086/595679 |
_version_ |
1766201566839177216 |