Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America
Pierre Auger Collaboration, Gabriele Curci

TL;DR
This study analyzes aerosol optical depth measurements at the Pierre Auger Observatory over several years, revealing seasonal patterns and air mass origins, with implications for atmospheric monitoring in cosmic ray research.
Contribution
It provides the first detailed analysis of aerosol optical depth and air mass trajectories at the remote Pierre Auger Observatory in South America.
Findings
Aerosol optical depth is low and seasonal, with winter minima and summer maxima.
Air masses from the Pacific Ocean correlate with low aerosol concentrations.
Biomass burning and urban pollution influence aerosol levels in certain periods.
Abstract
The Pierre Auger Observatory is making significant contributions towards understanding the nature and origin of ultra-high energy cosmic rays. One of its main challenges is the monitoring of the atmosphere, both in terms of its state variables and its optical properties. The aim of this work is to analyze aerosol optical depth values measured from 2004 to 2012 at the observatory, which is located in a remote and relatively unstudied area of the Pampa Amarilla, Argentina. The aerosol optical depth is in average quite low - annual mean - and shows a seasonal trend with a winter minimum - -, and a summer maximum - -, and an unexpected increase from August to September - ). We computed backward trajectories for the years…
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