Authors

J. Abraham, Consejo Nacional de Investigaciones Científicas y TécnicasFollow
P. Abreu, Instituto Superior TécnicoFollow
M. Aglietta, Università degli Studi di TorinoFollow
C. Aguirre, Universidad Catolica de BoliviaFollow
E. J. Ahn, Fermi National Accelerator LaboratoryFollow
D. Allard, APC - AstroParticule et CosmologieFollow
I. Allekotte, Instituto BalseiroFollow
J. Allen, New York UniversityFollow
P. Allison, The Ohio State UniversityFollow
J. Alvarez-Muñiz, Universidad de Santiago de CompostelaFollow
M. Ambrosio, Università degli Studi di Napoli Federico IIFollow
L. Anchordoqui, University of Wisconsin-MilwaukeeFollow
S. Andringa, Instituto Superior TécnicoFollow
A. Anzalone, INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
C. Aramo, Università degli Studi di Napoli Federico II
E. Arganda, Universidad Complutense de Madrid
S. Argirò, Università degli Studi di Torino
K. Arisaka, University of California, Los Angeles
F. Arneodo, Laboratori Nazionali del Gran Sasso
F. Arqueros, Universidad Complutense de Madrid
T. Asch, Karlsruher Institut für Technologie, Campus Nord
H. Asorey, Instituto Balseiro
P. Assis, Instituto Superior Técnico
J. Aublin, Laboratoire de Physique Nucléaire et de Hautes Energies
M. Ave, The Enrico Fermi Institute
G. Avila, Pierre Auger Observatory
T. Bäcker, Universität Siegen
D. Badagnani, Universidad Nacional de La Plata
K. B. Barber, The University of Adelaide
A. F. Barbosa, Centro Brasileiro de Pesquisas Físicas
S. L.C. Barroso, Universidade Estadual do Sudoeste da Bahia
B. Baughman, The Ohio State University
P. Bauleo, Colorado State University

Document Type

Article

Publication Date

1-1-2009

Abstract

Atmospheric parameters, such as pressure (P), temperature (T) and density (ρ ∝ P / T), affect the development of extensive air showers initiated by energetic cosmic rays. We have studied the impact of atmospheric variations on extensive air showers by means of the surface detector of the Pierre Auger Observatory. The rate of events shows a ∼ 10 % seasonal modulation and ∼ 2 % diurnal one. We find that the observed behaviour is explained by a model including the effects associated with the variations of P and ρ. The former affects the longitudinal development of air showers while the latter influences the Molière radius and hence the lateral distribution of the shower particles. The model is validated with full simulations of extensive air showers using atmospheric profiles measured at the site of the Pierre Auger Observatory. © 2009 Elsevier B.V. All rights reserved.

Publication Source (Journal or Book title)

Astroparticle Physics

First Page

89

Last Page

99

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