Identifying clouds over the Pierre Auger Observatory using infrared satellite data

Date

2013

Authors

Abreu, P.
Aglietta, M.
Ahlers, M.
Ahn, E.
Albuquerque, I.
Allekotte, I.
Allen, J.
Allison, P.
Almela, A.
Alvarez Castillo, J.

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Journal article

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Astroparticle Physics, 2013; 50-52:92-101

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.

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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 km<sup>2</sup> 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.

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© 2013 Elsevier B.V. All rights reserved.

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