FOR THE ICECUBE COLLABORATION
See special section of these proceedings Abstract: Important information pertaining to the origin of high-energy cosmic rays can be gained by studying their mass composition in the region of the knee ( 3 PeV). Thus, air showers have been ob-served at the South Pole using the SPASE-2 detector, which...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.561.8776 2023-05-15T18:22:12+02:00 FOR THE ICECUBE COLLABORATION K. G. Andeen C. Song K. Rawlins The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.561.8776 http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc1285.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.561.8776 http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc1285.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc1285.pdf text ftciteseerx 2016-01-08T12:05:00Z See special section of these proceedings Abstract: Important information pertaining to the origin of high-energy cosmic rays can be gained by studying their mass composition in the region of the knee ( 3 PeV). Thus, air showers have been ob-served at the South Pole using the SPASE-2 detector, which measures the electronic component at the surface, and the AMANDA-II neutrino telescope, which measures the coincident muonic component in deep ice. These two components, together with a Monte Carlo simulation and a well-understood analysis method, yield the relative cosmic ray composition in the knee region. We report on the efcacy of a new neural network technique for obtaining a composition result with the SPASE-2/AMANDA-II detectors. Text South pole Unknown South Pole |
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See special section of these proceedings Abstract: Important information pertaining to the origin of high-energy cosmic rays can be gained by studying their mass composition in the region of the knee ( 3 PeV). Thus, air showers have been ob-served at the South Pole using the SPASE-2 detector, which measures the electronic component at the surface, and the AMANDA-II neutrino telescope, which measures the coincident muonic component in deep ice. These two components, together with a Monte Carlo simulation and a well-understood analysis method, yield the relative cosmic ray composition in the knee region. We report on the efcacy of a new neural network technique for obtaining a composition result with the SPASE-2/AMANDA-II detectors. |
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The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
K. G. Andeen C. Song K. Rawlins |
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K. G. Andeen C. Song K. Rawlins FOR THE ICECUBE COLLABORATION |
author_facet |
K. G. Andeen C. Song K. Rawlins |
author_sort |
K. G. Andeen |
title |
FOR THE ICECUBE COLLABORATION |
title_short |
FOR THE ICECUBE COLLABORATION |
title_full |
FOR THE ICECUBE COLLABORATION |
title_fullStr |
FOR THE ICECUBE COLLABORATION |
title_full_unstemmed |
FOR THE ICECUBE COLLABORATION |
title_sort |
for the icecube collaboration |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.561.8776 http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc1285.pdf |
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South Pole |
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South Pole |
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South pole |
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South pole |
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http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc1285.pdf |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.561.8776 http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc1285.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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