Identifying clouds over the Pierre Auger Observatory using infrared satellite data


Autoria(s): Abreu, P.; Albuquerque, Ivone Freire da Mota e; Souza, Vitor de; Gouffon, Philippe; Peixoto, C. J. Todero; Tridapalli, D. B.; et al.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

17/06/2014

17/06/2014

01/12/2013

Resumo

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.

CNPq

FINEP

FAPERJ

FAPESP

MCTI

Entre outras

Identificador

Astroparticle Physics, Amsterdam : Elsevier BV, v. 50-52, p. 92-101, Dec. 2013

0927-6505

http://www.producao.usp.br/handle/BDPI/45436

10.1016/j.astropartphys.2013.09.004

Idioma(s)

eng

Publicador

Elsevier BV

Amsterdam

Relação

Astroparticle Physics

Direitos

restrictedAccess

Copyright Elsevier B.V.

Palavras-Chave #Ultra-high energy cosmic rays #Pierre Auger Observatory #Extensive air showers #Atmospheric monitoring #Clouds #Satellites #SATÉLITES #ATMOSFERA (MONITORAMENTO) #FÍSICA DE ALTA ENERGIA #INFRAVERMELHO
Tipo

article

original article

publishedVersion