European Extremely Large Telescope Site Characterization III: Ground Meteorology
- Autores
- Varela, Antonia M.; Vázquez Ramió, Héctor; Vernin, Jean; Muñoz Tuñon, Casiana; Sarazin, Marc; Trinquet, Hervé; Delgado, José Miguel; Jiménez Fuensalida, Jesús; Reyes, Marcos; Benhida, Abdelmajid; Benkhaldoun, Zouhair; Garcia Lambas, Diego Rodolfo; Hach, Youssef; Lazrek, Mohamed; Lombardi, Gianluca; Navarrete, Julio; Recabarren, Pablo Genaro Antonio; Renzi, Victor Alberto; Sabil, Mohammed; Vrech, Ruben Hector
- Año de publicación
- 2014
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 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.
Fil: Varela, Antonia M.. Instituto de Astrofísica de Canarias; España
Fil: Vázquez Ramió, Héctor. Centro de Estudios de Física del Cosmos de Aragón; España
Fil: Vernin, Jean. Université de Nice-Sophia Antipolis, Observatoire de la Côte d’Azur; Francia
Fil: Muñoz Tuñon, Casiana. Instituto de Astrofísica de Canarias; España
Fil: Sarazin, Marc. European Southern Observatory; Alemania
Fil: Trinquet, Hervé. Direction Générale de l'Armement; Francia
Fil: Delgado, José Miguel. Instituto de Astrofísica de Canarias; España
Fil: Jiménez Fuensalida, Jesús. Instituto de Astrofísica de Canarias; España
Fil: Reyes, Marcos. Instituto de Astrofísica de Canarias; España
Fil: Benhida, Abdelmajid. Université Cadi Ayyad; Marruecos
Fil: Benkhaldoun, Zouhair. Université Cadi Ayyad; Marruecos
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
Fil: Hach, Youssef. Université Cadi Ayyad; Marruecos
Fil: Lazrek, Mohamed. Université Cadi Ayyad; Marruecos
Fil: Lombardi, Gianluca. European Southern Observatory; Alemania
Fil: Navarrete, Julio. European Southern Observatory; Alemania
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
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
Fil: Sabil, Mohammed. Université Cadi Ayyad; Marruecos
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 - Materia
-
EXTREMELY
TELESCOPE
CHARACTERIZATION
METEOROLOGY - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/250909
Ver los metadatos del registro completo
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European Extremely Large Telescope Site Characterization III: Ground MeteorologyVarela, Antonia M.Vázquez Ramió, HéctorVernin, JeanMuñoz Tuñon, CasianaSarazin, MarcTrinquet, HervéDelgado, José MiguelJiménez Fuensalida, JesúsReyes, MarcosBenhida, AbdelmajidBenkhaldoun, ZouhairGarcia Lambas, Diego RodolfoHach, YoussefLazrek, MohamedLombardi, GianlucaNavarrete, JulioRecabarren, Pablo Genaro AntonioRenzi, Victor AlbertoSabil, MohammedVrech, Ruben HectorEXTREMELYTELESCOPECHARACTERIZATIONMETEOROLOGYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Both 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.Fil: Varela, Antonia M.. Instituto de Astrofísica de Canarias; EspañaFil: Vázquez Ramió, Héctor. Centro de Estudios de Física del Cosmos de Aragón; EspañaFil: Vernin, Jean. Université de Nice-Sophia Antipolis, Observatoire de la Côte d’Azur; FranciaFil: Muñoz Tuñon, Casiana. Instituto de Astrofísica de Canarias; EspañaFil: Sarazin, Marc. European Southern Observatory; AlemaniaFil: Trinquet, Hervé. Direction Générale de l'Armement; FranciaFil: Delgado, José Miguel. Instituto de Astrofísica de Canarias; EspañaFil: Jiménez Fuensalida, Jesús. Instituto de Astrofísica de Canarias; EspañaFil: Reyes, Marcos. Instituto de Astrofísica de Canarias; EspañaFil: Benhida, Abdelmajid. Université Cadi Ayyad; MarruecosFil: Benkhaldoun, Zouhair. Université Cadi Ayyad; MarruecosFil: 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; ArgentinaFil: Hach, Youssef. Université Cadi Ayyad; MarruecosFil: Lazrek, Mohamed. Université Cadi Ayyad; MarruecosFil: Lombardi, Gianluca. European Southern Observatory; AlemaniaFil: Navarrete, Julio. European Southern Observatory; AlemaniaFil: 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; ArgentinaFil: 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; ArgentinaFil: Sabil, Mohammed. Université Cadi Ayyad; MarruecosFil: 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; ArgentinaUniversity of Chicago Press2014-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/250909Varela, 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; 412-4310004-6280CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/676135info:eu-repo/semantics/altIdentifier/doi/10.1086/676135info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:39:02Zoai:ri.conicet.gov.ar:11336/250909instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:39:02.461CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
European Extremely Large Telescope Site Characterization III: Ground Meteorology |
| title |
European Extremely Large Telescope Site Characterization III: Ground Meteorology |
| spellingShingle |
European Extremely Large Telescope Site Characterization III: Ground Meteorology Varela, Antonia M. EXTREMELY TELESCOPE CHARACTERIZATION METEOROLOGY |
| title_short |
European Extremely Large Telescope Site Characterization III: Ground Meteorology |
| title_full |
European Extremely Large Telescope Site Characterization III: Ground Meteorology |
| title_fullStr |
European Extremely Large Telescope Site Characterization III: Ground Meteorology |
| title_full_unstemmed |
European Extremely Large Telescope Site Characterization III: Ground Meteorology |
| title_sort |
European Extremely Large Telescope Site Characterization III: Ground Meteorology |
| dc.creator.none.fl_str_mv |
Varela, Antonia M. Vázquez Ramió, Héctor Vernin, Jean Muñoz Tuñon, Casiana Sarazin, Marc Trinquet, Hervé Delgado, José Miguel Jiménez Fuensalida, Jesús Reyes, Marcos Benhida, Abdelmajid Benkhaldoun, Zouhair Garcia Lambas, Diego Rodolfo Hach, Youssef Lazrek, Mohamed Lombardi, Gianluca Navarrete, Julio Recabarren, Pablo Genaro Antonio Renzi, Victor Alberto Sabil, Mohammed Vrech, Ruben Hector |
| author |
Varela, Antonia M. |
| author_facet |
Varela, Antonia M. Vázquez Ramió, Héctor Vernin, Jean Muñoz Tuñon, Casiana Sarazin, Marc Trinquet, Hervé Delgado, José Miguel Jiménez Fuensalida, Jesús Reyes, Marcos Benhida, Abdelmajid Benkhaldoun, Zouhair Garcia Lambas, Diego Rodolfo Hach, Youssef Lazrek, Mohamed Lombardi, Gianluca Navarrete, Julio Recabarren, Pablo Genaro Antonio Renzi, Victor Alberto Sabil, Mohammed Vrech, Ruben Hector |
| author_role |
author |
| author2 |
Vázquez Ramió, Héctor Vernin, Jean Muñoz Tuñon, Casiana Sarazin, Marc Trinquet, Hervé Delgado, José Miguel Jiménez Fuensalida, Jesús Reyes, Marcos Benhida, Abdelmajid Benkhaldoun, Zouhair Garcia Lambas, Diego Rodolfo Hach, Youssef Lazrek, Mohamed Lombardi, Gianluca Navarrete, Julio Recabarren, Pablo Genaro Antonio Renzi, Victor Alberto Sabil, Mohammed Vrech, Ruben Hector |
| author2_role |
author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
EXTREMELY TELESCOPE CHARACTERIZATION METEOROLOGY |
| topic |
EXTREMELY TELESCOPE CHARACTERIZATION METEOROLOGY |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
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. Fil: Varela, Antonia M.. Instituto de Astrofísica de Canarias; España Fil: Vázquez Ramió, Héctor. Centro de Estudios de Física del Cosmos de Aragón; España Fil: Vernin, Jean. Université de Nice-Sophia Antipolis, Observatoire de la Côte d’Azur; Francia Fil: Muñoz Tuñon, Casiana. Instituto de Astrofísica de Canarias; España Fil: Sarazin, Marc. European Southern Observatory; Alemania Fil: Trinquet, Hervé. Direction Générale de l'Armement; Francia Fil: Delgado, José Miguel. Instituto de Astrofísica de Canarias; España Fil: Jiménez Fuensalida, Jesús. Instituto de Astrofísica de Canarias; España Fil: Reyes, Marcos. Instituto de Astrofísica de Canarias; España Fil: Benhida, Abdelmajid. Université Cadi Ayyad; Marruecos Fil: Benkhaldoun, Zouhair. Université Cadi Ayyad; Marruecos 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 Fil: Hach, Youssef. Université Cadi Ayyad; Marruecos Fil: Lazrek, Mohamed. Université Cadi Ayyad; Marruecos Fil: Lombardi, Gianluca. European Southern Observatory; Alemania Fil: Navarrete, Julio. European Southern Observatory; Alemania 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 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 Fil: Sabil, Mohammed. Université Cadi Ayyad; Marruecos 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 |
| description |
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. |
| publishDate |
2014 |
| dc.date.none.fl_str_mv |
2014-04 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
| status_str |
publishedVersion |
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http://hdl.handle.net/11336/250909 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 0004-6280 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/250909 |
| identifier_str_mv |
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 0004-6280 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
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eng |
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info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/676135 info:eu-repo/semantics/altIdentifier/doi/10.1086/676135 |
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University of Chicago Press |
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University of Chicago Press |
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