Identifying clouds over the Pierre Auger Observatory using infrared satellite data

Mostrar todas las versiones(2)

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 O...

Descripción completa

Guardado en:

Detalles Bibliográficos
Autor principal:	Multitudinario:505
Formato:	JOUR
Materias:	Atmospheric monitoring Clouds Extensive air showers Pierre Auger Observatory Satellites Ultra-high energy cosmic rays Central laser facilities Cloud identification Infrared satellites Pierre Auger observatory Space-based observatories Ultra high-energy cosmic rays Augers Cosmic rays Observatories
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_09276505_v50-52_n_p92_Multitudinario
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

id	todo:paper_09276505_v50-52_n_p92_Multitudinario
record_format	dspace
spelling	todo:paper_09276505_v50-52_n_p92_Multitudinario2023-10-03T15:47:02Z Identifying clouds over the Pierre Auger Observatory using infrared satellite data Multitudinario:505 Atmospheric monitoring Clouds Extensive air showers Pierre Auger Observatory Satellites Ultra-high energy cosmic rays Atmospheric monitoring Central laser facilities Cloud identification Extensive air showers Infrared satellites Pierre Auger observatory Space-based observatories Ultra high-energy cosmic rays Augers Clouds Cosmic rays Satellites Observatories 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 2 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. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_09276505_v50-52_n_p92_Multitudinario
institution	Universidad de Buenos Aires
institution_str	I-28
repository_str	R-134
collection	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic	Atmospheric monitoring Clouds Extensive air showers Pierre Auger Observatory Satellites Ultra-high energy cosmic rays Atmospheric monitoring Central laser facilities Cloud identification Extensive air showers Infrared satellites Pierre Auger observatory Space-based observatories Ultra high-energy cosmic rays Augers Clouds Cosmic rays Satellites Observatories
spellingShingle	Atmospheric monitoring Clouds Extensive air showers Pierre Auger Observatory Satellites Ultra-high energy cosmic rays Atmospheric monitoring Central laser facilities Cloud identification Extensive air showers Infrared satellites Pierre Auger observatory Space-based observatories Ultra high-energy cosmic rays Augers Clouds Cosmic rays Satellites Observatories Multitudinario:505 Identifying clouds over the Pierre Auger Observatory using infrared satellite data
topic_facet	Atmospheric monitoring Clouds Extensive air showers Pierre Auger Observatory Satellites Ultra-high energy cosmic rays Atmospheric monitoring Central laser facilities Cloud identification Extensive air showers Infrared satellites Pierre Auger observatory Space-based observatories Ultra high-energy cosmic rays Augers Clouds Cosmic rays Satellites Observatories
description	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 2 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.
format	JOUR
author	Multitudinario:505
author_facet	Multitudinario:505
author_sort	Multitudinario:505
title	Identifying clouds over the Pierre Auger Observatory using infrared satellite data
title_short	Identifying clouds over the Pierre Auger Observatory using infrared satellite data
title_full	Identifying clouds over the Pierre Auger Observatory using infrared satellite data
title_fullStr	Identifying clouds over the Pierre Auger Observatory using infrared satellite data
title_full_unstemmed	Identifying clouds over the Pierre Auger Observatory using infrared satellite data
title_sort	identifying clouds over the pierre auger observatory using infrared satellite data
url	http://hdl.handle.net/20.500.12110/paper_09276505_v50-52_n_p92_Multitudinario
work_keys_str_mv	AT multitudinario505 identifyingcloudsoverthepierreaugerobservatoryusinginfraredsatellitedata
_version_	1807316999405043712

Identifying clouds over the Pierre Auger Observatory using infrared satellite data

Ejemplares similares