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dc.contributor.author
Varela, Antonia M.  
dc.contributor.author
Vázquez Ramió, Héctor  
dc.contributor.author
Vernin, Jean  
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Muñoz Tuñon, Casiana  
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Sarazin, Marc  
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Trinquet, Hervé  
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Delgado, José Miguel  
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Jiménez Fuensalida, Jesús  
dc.contributor.author
Reyes, Marcos  
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Benhida, Abdelmajid  
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Benkhaldoun, Zouhair  
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Garcia Lambas, Diego Rodolfo  
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Hach, Youssef  
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Lazrek, Mohamed  
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Lombardi, Gianluca  
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Navarrete, Julio  
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Recabarren, Pablo Genaro Antonio  
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Renzi, Victor Alberto  
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Sabil, Mohammed  
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Vrech, Ruben Hector  
dc.date.available
2024-12-20T13:51:40Z  
dc.date.issued
2014-04  
dc.identifier.citation
Varela, Antonia M.; Vázquez Ramió, Héctor; Vernin, Jean; Muñoz Tuñon, Casiana; Sarazin, Marc; et al.; European Extremely Large Telescope Site Characterization III: Ground Meteorology; University of Chicago Press; Publications of the Astronomical Society of the Pacific; 126; 938; 4-2014; 412-431  
dc.identifier.issn
0004-6280  
dc.identifier.uri
http://hdl.handle.net/11336/250909  
dc.description.abstract
Both meteorology and optical conditions are crucial for selecting the best site to host extremely large telescopes such as the Thirty Meter Telescope (TMT) and the European project (E-ELT). For the E-ELT, a year-long meteorological campaign was performed at our two reference sites, the Observatorio del Roque de los Muchachos (ORM) and Cerro Ventarrones (very close to the VLT site at Paranal), and at other sites also considered as alternatives to the reference sites: Aklim, Macón, and Izaña (Observatorio del Teide; OT). In this article, we present a statistical analysis of the ground meteorological properties recorded at these sites, making use of automatic weather stations (AWSs) equipped with standard meteorological sensors providing the air temperature, relative humidity, barometric pressure, wind speed, and wind direction, using standard procedures across all sites. Meteorology offers but one discriminant in the complicated question of where to site such a major facility as the E-ELT (other factors being seeing, local geology, the economics of the logistics, etc.), both for determining the feasibility of telescope and instrumentation design and construction and for determining the useful observing time. However, the final decision of where to locate a major telescope depends in part on all these—and other—considerations and not on any one criterion alone. In summary, for 90% of the nighttime, the wind speed is lower than 18 m s 1, the telescope operational limit at all the sites except Macón. For this reason, Macón was discarded in the final site selection as, for 25% of the time, the wind speed is greater than 17 m s 1. The smallest nighttime temperature gradient is at ORM, whereas the lowest mean relative humidity value is reached at the Ventarrones site. Izaña was discarded in the site selection study from the very beginning due to lack of funding to install further site-testing equipement (e.g., MultiAperture Scintillation Sensor-Differential Image Motion Monitor (MASS-DIMM)). We investigate the statistical distributions of annual and monthly meteorological conditions for day and night separately. This is the third paper in a series discussing the E-ELT FP6 site characterization project.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
University of Chicago Press  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
EXTREMELY  
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TELESCOPE  
dc.subject
CHARACTERIZATION  
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METEOROLOGY  
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Astronomía  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
European Extremely Large Telescope Site Characterization III: Ground Meteorology  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2024-10-23T17:33:46Z  
dc.journal.volume
126  
dc.journal.number
938  
dc.journal.pagination
412-431  
dc.journal.pais
Estados Unidos  
dc.journal.ciudad
Chicago  
dc.description.fil
Fil: Varela, Antonia M.. Instituto de Astrofísica de Canarias; España  
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Fil: Vázquez Ramió, Héctor. Centro de Estudios de Física del Cosmos de Aragón; España  
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Fil: Vernin, Jean. Université de Nice-Sophia Antipolis, Observatoire de la Côte d’Azur; Francia  
dc.description.fil
Fil: Muñoz Tuñon, Casiana. Instituto de Astrofísica de Canarias; España  
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Fil: Sarazin, Marc. European Southern Observatory; Alemania  
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Fil: Trinquet, Hervé. Direction Générale de l'Armement; Francia  
dc.description.fil
Fil: Delgado, José Miguel. Instituto de Astrofísica de Canarias; España  
dc.description.fil
Fil: Jiménez Fuensalida, Jesús. Instituto de Astrofísica de Canarias; España  
dc.description.fil
Fil: Reyes, Marcos. Instituto de Astrofísica de Canarias; España  
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Fil: Benhida, Abdelmajid. Université Cadi Ayyad; Marruecos  
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Fil: Benkhaldoun, Zouhair. Université Cadi Ayyad; Marruecos  
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Fil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina  
dc.description.fil
Fil: Hach, Youssef. Université Cadi Ayyad; Marruecos  
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Fil: Lazrek, Mohamed. Université Cadi Ayyad; Marruecos  
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Fil: Lombardi, Gianluca. European Southern Observatory; Alemania  
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Fil: Navarrete, Julio. European Southern Observatory; Alemania  
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Fil: Recabarren, Pablo Genaro Antonio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina  
dc.description.fil
Fil: Renzi, Victor Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina  
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Fil: Sabil, Mohammed. Université Cadi Ayyad; Marruecos  
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Fil: Vrech, Ruben Hector. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina  
dc.journal.title
Publications of the Astronomical Society of the Pacific  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/676135  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1086/676135