An Estimate of the primary mass of cosmic rays at 10<sup>18</sup> eV as inferred from Volcano Ranch data

Accurate measurements of the lateral distribution of extensive air showers produced by cosmic rays of energy greater than 10<sup>17</sup> eV were made in the 1970s by Linsley. At the time, the state of knowledge about the best hadronic interaction model to use to describe such data preve...

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Autores principales: Dova, María Teresa, Manceñido, Mónica E., Mariazzi, Analisa Gabriela, McCauley, Thomas, Watson, Alan
Formato: Objeto de conferencia
Lenguaje:Inglés
Publicado: 2003
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/81762
http://inspirehep.net/record/619085
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id I19-R120-10915-81762
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Exactas
Física
Cascada atmosférica extensa
Radiación Cósmica
QGSJET98
spellingShingle Ciencias Exactas
Física
Cascada atmosférica extensa
Radiación Cósmica
QGSJET98
Dova, María Teresa
Manceñido, Mónica E.
Mariazzi, Analisa Gabriela
McCauley, Thomas
Watson, Alan
An Estimate of the primary mass of cosmic rays at 10<sup>18</sup> eV as inferred from Volcano Ranch data
topic_facet Ciencias Exactas
Física
Cascada atmosférica extensa
Radiación Cósmica
QGSJET98
description Accurate measurements of the lateral distribution of extensive air showers produced by cosmic rays of energy greater than 10<sup>17</sup> eV were made in the 1970s by Linsley. At the time, the state of knowledge about the best hadronic interaction model to use to describe such data prevented conclusions about the cosmic ray mass from being drawn. We have used a modern model, QGSJET98, to infer the primary mass from these data, using the very careful records left by Linsley. We find that at a median energy of 10<sup>18</sup> eV, the data are well described by an iron-dominated composition (88 ± 6(stat) ± 18 (syst))%. We discuss the systematic errors in this estimate that arise from model uncertainties and from the range of energies used in the work of Linsley. These data are used with the permission of the late John Linsley to whom this work is dedicated
format Objeto de conferencia
Objeto de conferencia
author Dova, María Teresa
Manceñido, Mónica E.
Mariazzi, Analisa Gabriela
McCauley, Thomas
Watson, Alan
author_facet Dova, María Teresa
Manceñido, Mónica E.
Mariazzi, Analisa Gabriela
McCauley, Thomas
Watson, Alan
author_sort Dova, María Teresa
title An Estimate of the primary mass of cosmic rays at 10<sup>18</sup> eV as inferred from Volcano Ranch data
title_short An Estimate of the primary mass of cosmic rays at 10<sup>18</sup> eV as inferred from Volcano Ranch data
title_full An Estimate of the primary mass of cosmic rays at 10<sup>18</sup> eV as inferred from Volcano Ranch data
title_fullStr An Estimate of the primary mass of cosmic rays at 10<sup>18</sup> eV as inferred from Volcano Ranch data
title_full_unstemmed An Estimate of the primary mass of cosmic rays at 10<sup>18</sup> eV as inferred from Volcano Ranch data
title_sort estimate of the primary mass of cosmic rays at 10<sup>18</sup> ev as inferred from volcano ranch data
publishDate 2003
url http://sedici.unlp.edu.ar/handle/10915/81762
http://inspirehep.net/record/619085
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