Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/88389
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Type: Journal article
Title: Identifying clouds over the Pierre Auger Observatory using infrared satellite data
Author: Abreu, P.
Aglietta, M.
Ahlers, M.
Ahn, E.
Albuquerque, I.
Allekotte, I.
Allen, J.
Allison, P.
Almela, A.
Alvarez Castillo, J.
Alvarez-Muñiz, J.
Alves Batista, R.
Ambrosio, M.
Aminaei, A.
Anchordoqui, L.
Andringa, S.
Antičić, T.
Aramo, C.
Arqueros, F.
Asorey, H.
et al.
Citation: Astroparticle Physics, 2013; 50-52:92-101
Publisher: Elsevier Science BV
Issue Date: 2013
ISSN: 0927-6505
1873-2852
Statement of
Responsibility: 
P. Abreu ... K.B. Barber ... J.A. Bellido ... R.W. Clay ... M.J. Cooper ... B.R. Dawson ... T.D. Grubb ... T.A. Harrison ... A.E. Herve ... G.C. Hill ... V.C. Holmes ... M. Malacari ... S.J. Saffi ... J. Sorokin ... P. Wahrlich ... et al.
Abstract: We describe a new method of identifying night-time clouds over the Pierre Auger Observatory using infrared data from the Imager instruments on the GOES-12 and GOES-13 satellites. We compare cloud identifications resulting from our method to those obtained by the Central Laser Facility of the Auger Observatory. Using our new method we can now develop cloud probability maps for the 3000 km2 of the Pierre Auger Observatory twice per hour with a spatial resolution of ∼2.4 km by ∼5.5 km. Our method could also be applied to monitor cloud cover for other ground-based observatories and for space-based observatories. © 2013 Elsevier B.V. All rights reserved.
Keywords: Ultra-high energy cosmic rays; Pierre Auger Observatory; Extensive air showers; Atmospheric monitoring; Clouds; Satellites
Rights: © 2013 Elsevier B.V. All rights reserved.
DOI: 10.1016/j.astropartphys.2013.09.004
Published version: http://dx.doi.org/10.1016/j.astropartphys.2013.09.004
Appears in Collections:Aurora harvest 7
Chemistry and Physics publications

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