dc.creatorDova, María Teresa
dc.creatorGómez Albarracín, Flavia Alejandra
dc.creatorHansen, Patricia María
dc.creatorJarne, Cecilia Gisele
dc.creatorMariazzi, Analisa Gabriela
dc.creatorMoreno, Juan Cruz
dc.creatorSciutto, Sergio Juan
dc.creatorWahlberg, Hernán Pablo
dc.creatorThe Pierre Auger Collaboration
dc.date2013-12
dc.date2019-07-16T16:27:13Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/78252
dc.identifierissn:0927-6505
dc.descriptionWe 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.
dc.descriptionFacultad de Ciencias Exactas
dc.formatapplication/pdf
dc.format92-101
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Exactas
dc.subjectUltra-high energy cosmic rays
dc.subjectPierre Auger observatory
dc.subjectExtensive air showers
dc.subjectAtmospheric monitoring
dc.subjectClouds
dc.subjectSatellites
dc.subjectFísica
dc.titleIdentifying clouds over the Pierre Auger Observatory using infrared satellite data
dc.typeArticulo
dc.typeArticulo


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