Measurement of the depth of maximum of extensive air showers above 1018eV

We describe the measurement of the depth of maximum, Xmax, of the longitudinal development of air showers induced by cosmic rays. Almost 4000 events above 1018eV observed by the fluorescence detector of the Pierre Auger Observatory in coincidence with at least one surface detector station are select...

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spelling todo:paper_00319007_v104_n9_p_Multitudinario2023-10-03T14:42:07Z Measurement of the depth of maximum of extensive air showers above 1018eV Multitudinario:476 Cosmic ray measurement Cosmology Fluorescence Air showers Extensive air showers Fluorescence detector Mass composition Pierre Auger observatory Surface detectors Cosmic rays We describe the measurement of the depth of maximum, Xmax, of the longitudinal development of air showers induced by cosmic rays. Almost 4000 events above 1018eV observed by the fluorescence detector of the Pierre Auger Observatory in coincidence with at least one surface detector station are selected for the analysis. The average shower maximum was found to evolve with energy at a rate of (106-21+35)g/cm2/decade below 1018.24 ± 0. 05eV, and (24±3)g/cm2/decade above this energy. The measured shower-to-shower fluctuations decrease from about 55 to 26g/cm2. The interpretation of these results in terms of the cosmic ray mass composition is briefly discussed. © 2010 The American Physical Society. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00319007_v104_n9_p_Multitudinario
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Cosmic ray measurement
Cosmology
Fluorescence
Air showers
Extensive air showers
Fluorescence detector
Mass composition
Pierre Auger observatory
Surface detectors
Cosmic rays
spellingShingle Cosmic ray measurement
Cosmology
Fluorescence
Air showers
Extensive air showers
Fluorescence detector
Mass composition
Pierre Auger observatory
Surface detectors
Cosmic rays
Multitudinario:476
Measurement of the depth of maximum of extensive air showers above 1018eV
topic_facet Cosmic ray measurement
Cosmology
Fluorescence
Air showers
Extensive air showers
Fluorescence detector
Mass composition
Pierre Auger observatory
Surface detectors
Cosmic rays
description We describe the measurement of the depth of maximum, Xmax, of the longitudinal development of air showers induced by cosmic rays. Almost 4000 events above 1018eV observed by the fluorescence detector of the Pierre Auger Observatory in coincidence with at least one surface detector station are selected for the analysis. The average shower maximum was found to evolve with energy at a rate of (106-21+35)g/cm2/decade below 1018.24 ± 0. 05eV, and (24±3)g/cm2/decade above this energy. The measured shower-to-shower fluctuations decrease from about 55 to 26g/cm2. The interpretation of these results in terms of the cosmic ray mass composition is briefly discussed. © 2010 The American Physical Society.
format JOUR
author Multitudinario:476
author_facet Multitudinario:476
author_sort Multitudinario:476
title Measurement of the depth of maximum of extensive air showers above 1018eV
title_short Measurement of the depth of maximum of extensive air showers above 1018eV
title_full Measurement of the depth of maximum of extensive air showers above 1018eV
title_fullStr Measurement of the depth of maximum of extensive air showers above 1018eV
title_full_unstemmed Measurement of the depth of maximum of extensive air showers above 1018eV
title_sort measurement of the depth of maximum of extensive air showers above 1018ev
url http://hdl.handle.net/20.500.12110/paper_00319007_v104_n9_p_Multitudinario
work_keys_str_mv AT multitudinario476 measurementofthedepthofmaximumofextensiveairshowersabove1018ev
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