Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America
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 a...
Autores principales: | , , , , , , , , |
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Formato: | Articulo |
Lenguaje: | Inglés |
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2014
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Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/75390 |
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I19-R120-10915-75390 |
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institution |
Universidad Nacional de La Plata |
institution_str |
I-19 |
repository_str |
R-120 |
collection |
SEDICI (UNLP) |
language |
Inglés |
topic |
Ciencias Exactas Física Atmósfera cosmic rays aerosol air masses atmospheric effect HYSPLIT GDAS |
spellingShingle |
Ciencias Exactas Física Atmósfera cosmic rays aerosol air masses atmospheric effect HYSPLIT GDAS Dova, María Teresa Gómez Albarracín, Flavia Alejandra Hansen, Patricia María Jarne, Cecilia Gisele Mariazzi, Analisa Gabriela Moreno, Juan Cruz Sciutto, Sergio Juan Wahlberg, Hernán Pablo The Pierre Auger Collaboration Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America |
topic_facet |
Ciencias Exactas Física Atmósfera cosmic rays aerosol air masses atmospheric effect HYSPLIT GDAS |
description |
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 analyse aerosol optical depth τa(z) values measured from 2004 to 2012 at the observatory, which is located in a remote and relatively unstudied area of Pampa Amarilla, Argentina. The aerosol optical depth is in average quite low – annual mean τa(3.5 km) ∼ 0.04 – and shows a seasonal trend with a winter minimum – τa(3.5 km) ∼ 0.03 –, and a summer maximum – τa(3.5 km) ∼ 0.06 –, and an unexpected increase from August to September — τa(3.5 km) ∼ 0.055. We computed backward trajectories for the years 2005 to 2012 to interpret the air mass origin. Winter nights with low aerosol concentrations show air masses originating from the Pacific Ocean. Average concentrations are affected by continental sources (wind-blown dust and urban pollution), whilst the peak observed in September and October could be linked to biomass burning in the northern part of Argentina or air pollution coming from surrounding urban areas. |
format |
Articulo Articulo |
author |
Dova, María Teresa Gómez Albarracín, Flavia Alejandra Hansen, Patricia María Jarne, Cecilia Gisele Mariazzi, Analisa Gabriela Moreno, Juan Cruz Sciutto, Sergio Juan Wahlberg, Hernán Pablo The Pierre Auger Collaboration |
author_facet |
Dova, María Teresa Gómez Albarracín, Flavia Alejandra Hansen, Patricia María Jarne, Cecilia Gisele Mariazzi, Analisa Gabriela Moreno, Juan Cruz Sciutto, Sergio Juan Wahlberg, Hernán Pablo The Pierre Auger Collaboration |
author_sort |
Dova, María Teresa |
title |
Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America |
title_short |
Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America |
title_full |
Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America |
title_fullStr |
Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America |
title_full_unstemmed |
Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America |
title_sort |
origin of atmospheric aerosols at the pierre auger observatory using studies of air mass trajectories in south america |
publishDate |
2014 |
url |
http://sedici.unlp.edu.ar/handle/10915/75390 |
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