Authors

A. Aab, Radboud Universiteit
P. Abreu, Instituto Superior TécnicoFollow
M. Aglietta, Istituto Nazionale di Fisica Nucleare, Sezione di TorinoFollow
I. Al Samarai, Laboratoire de Physique Nucléaire et de Hautes EnergiesFollow
I. F.M. Albuquerque, Universidade de São PauloFollow
I. Allekotte, Centro Atomico BarilocheFollow
A. Almela, Universidad Nacional de San Martín
J. Alvarez Castillo, Universidad Nacional Autónoma de MéxicoFollow
J. Alvarez-Muñiz, Universidad de Santiago de CompostelaFollow
G. A. Anastasi, Gran Sasso Science InstituteFollow
L. Anchordoqui, Lehman CollegeFollow
B. Andrada, Universidad Nacional de San MartínFollow
S. Andringa, Instituto Superior TécnicoFollow
C. Aramo, Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
F. Arqueros, Universidad Complutense de Madrid
N. Arsene, Universitatea din Bucuresti
H. Asorey, Centro Atomico Bariloche
P. Assis, Instituto Superior Técnico
J. Aublin, Laboratoire de Physique Nucléaire et de Hautes Energies
G. Avila, Pierre Auger Observatory
A. M. Badescu, University Politehnica of Bucharest
A. Balaceanu, Horia Hulubei National Institute of Physics and Nuclear Engineering
R. J. Barreira Luz, Instituto Superior Técnico
C. Baus, Karlsruher Institut für Technologie
J. J. Beatty, The Ohio State University
K. H. Becker, Bergische Universität Wuppertal
J. A. Bellido, The University of Adelaide
C. Berat, Universite Grenoble Alpes
M. E. Bertaina, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
X. Bertou, Centro Atomico Bariloche
P. L. Biermann, Max Planck Institute for Radio Astronomy
P. Billoir, Laboratoire de Physique Nucléaire et de Hautes Energies
J. Biteau, Institut de Physique Nucléaire d’Orsay

Document Type

Conference Proceeding

Publication Date

2-7-2017

Abstract

Atmospheric conditions, such as the pressure (P), temperature (T) or air density (-/ P=T), affect the development of extended air showers initiated by energetic cosmic rays. We study the impact of the atmospheric variations on the reconstruction of air showers with data from the arrays of surface detectors of the Pierre Auger Observatory, considering separately the one with detector spacings of 1500m and the one with 750m spacing. We observe modulations in the event rates that are due to the influence of the air density and pressure variations on the measured signals, from which the energy estimators are obtained. We show how the energy assignment can be corrected to account for such atmospheric effects.

Publication Source (Journal or Book title)

Journal of Instrumentation

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