Atmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatory

作者:Abraham J; Abreu P; Aglietta M; Aguirre C; Ahn E J; Allard D; Allekotte I; Allen J; Allison P; Alvarez Muniz J; Ambrosio M; Anchordoqui L; Andringa S; Anzalone A; Aramo C; Arganda E; Argiro S; Arisaka K; Arneodo F; Arqueros F; Asch T; Asorey H; Assis P; Aublin J; Ave M; Avila G; Baecker T; Badagnani D; Barber K B; Barbosa A F; Barroso S L C; Baughman B; Bauleo P; Beatty J J; Beau T; Becker B R; Becker K H
来源:Astroparticle Physics, 2009, 32(2): 89-99.
DOI:10.1016/j.astropartphys.2009.06.004

摘要

Atmospheric parameters, Such as pressure (P), temperature (T) and density (rho proportional to 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 similar to 10% seasonal modulation and similar to 2% diurnal one. We find that the observed behaviour is explained by a model including the effects associated with the variations of P and rho. The former affects the longitudinal development of air showers while the latter influences the Moliere 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.