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A Satellite Survey of Cloud Cover and Water Vapor in the Southwestern USA and Northern Mexico
Indexado
WoS WOS:000423187500001
Scopus SCOPUS_ID:85014131787
DOI 10.1088/1538-3873/129/973/035005
Año 2017
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



Cloud cover and water vapor conditions in the southwestern USA and northern Mexico were surveyed as a preparatory work for the Thirty Meter Telescope (TMT) in situ site testing program. Although the telescope site is already selected, the TMT site testing team decided to make public these results for its usefulness for the community. Using 58 months of meteorological satellite observations between 1993 July and 1999 September, different atmospheric parameters were quantified from data of the 10.7 mu m and of 6.7 mu m windows. In particular, cloud cover and water vapor conditions were identified in preferred areas. As a result of the aerial analysis, 15 sites of existing and potential telescope were selected, compared, and ranked in terms of their observing quality. The clearest sites are located along the spine of the Baja peninsula and into southern California on mountain peaks above the temperature inversion layer. A steep gradient of cloudiness was observed along the coast where coastal cloud and fog are trapped below the inversion layer. Moving from west to east over the continent, a significant increase in cloudiness was observed. The analysis shows that San Pedro Martir, San Gorgonio Mountain and San Jacinto Peak have the largest fraction of clear sky conditions (similar to 74%). The site with the optimal combination of clear skies and low precipitable water vapor is Boundary Peak, Nevada. An approach based in satellite data provided a reliable method for sites comparison.

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 CARRASCO-LICEA, ESPERANZA Mujer Inst Nacl Astrofis Opt & Electr - México
Instituto Nacional de Astrofisica Optica y Electronica - México
2 AVILA-RUBIO, RICARDO FELIX Hombre Univ Nacl Autonoma Mexico - México
Universidad Nacional Autónoma de México - México
UNAM campus Juriquilla - México
3 Erasmus, A. - South African Astron Observ - República de Sudáfrica
South African Astronomical Observatory - República de Sudáfrica
4 Djorgovski, S. G. - CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos
5 WALKER, ALISTAIR Hombre Natl Opt Astron Observ - Chile
Cerro Tololo Inter American Observatory - Chile
National Optical Astronomy Observatory - Chile
6 Blum, Robert Hombre Natl Opt Astron Observ - Estados Unidos
National Optical Astronomy Observatory - Estados Unidos

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Financiamiento



Fuente
Universidad Nacional Autónoma de México
University of Tokyo
European Southern Observatory
South African Astronomical Observatory
Instituto de Astronomia (Universidad Nacional Autonoma de Mexico)
CELT project (University of California)
Mt. Graham International Observatory (University of Arizona)
CELT project (California Institute of Technology)
Observatorio Astronomico Nacional de San Pedro Martir
Instituto de Astronom?a
Universidad Nacional Aut?noma de M?xico
University of California and California Institute of Technology
Instituto de Astronomía
Direct For Mathematical & Physical Scien; Division Of Astronomical Sciences

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
The results presented in this paper were based in a study funded by the CELT project (University of California and California Institute of Technology). The data were purchased by Cerro Tololo Inter-American Observatory, the University of Tokyo, and the European Southern Observatory. Mt. Graham International Observatory (University of Arizona); the Observatorio Astronomico Nacional de San Pedro Martir and the Instituto de Astronomia (Universidad Nacional Autonoma de Mexico); and the South African Astronomical Observatory are also acknowledged for their support.
The results presented in this paper were based in a study funded by the CELT project (University of California and California Institute of Technology). The data were purchased by Cerro Tololo Inter-American Observatory, the University of Tokyo, and the European Southern Observatory. Mt. Graham International Observatory (University of Arizona); the Observatorio Astrónomico Nacional de San Pedro Mártir and the Instituto de Astronomía (Universidad Nacional Autónoma de México); and the South African Astronomical Observatory are also acknowledged for their support.

Muestra la fuente de financiamiento declarada en la publicación.