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Late pleistocene glaciations of the arid subtropical Andes and new results from the Chajnantor Plateau, northern Chile
Indexado
WoS WOS:000364884400007
Scopus SCOPUS_ID:84943657028
DOI 10.1016/J.QUASCIREV.2015.09.022
Año 2015
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



The spatiotemporal pattern of glaciation along the Andes Mountains is an important proxy record reflecting the varying influence of global and regional circulation features on South American climate. However, the timing and extent of glaciation in key parts of the orogen, particularly the deglaciated arid Andes, are poorly constrained. We present new cosmogenic Be-10 and Cl-36 exposure ages for glacial features on and near the Chajnantor Plateau (23 degrees S). The new dates, although scattered due to cosmogenic inheritance, imply that the most recent extensive glacial occupation ended before or during the global Last Glacial Maximum (LGM). We discuss this new record in the context of published glacial chronologies from glacial features in Peru, Bolivia, and northern Chile rescaled using the latest cosmogenic 10Be production rate calibration for the tropical Andes. The results imply regionally synchronous moraine stabilization ca. 25-40 ka, 15-17 ka, and 12-14 ka, with the youngest of these moraines absent in records south of similar to 20 degrees S, including in our new Chajnantor area chronology. This spatial pattern implicates easterly moisture in generating sufficient snowfall to glaciate the driest parts of the Andes, while allowing a role for westerly moisture, possibly modulated by the migration of the Southern Westerly Wind belt, in the regions near and south of the Atacama Desert. (C) 2015 Elsevier Ltd. All rights reserved.

Revista



Revista ISSN
Quaternary Science Reviews 0277-3791

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Disciplinas de Investigación



WOS
Geosciences, Multidisciplinary
Geography, Physical
Scopus
Geology
Archeology (Arts And Humanities)
Archeology
Global And Planetary Change
Ecology, Evolution, Behavior And Systematics
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 Ward, Dylan J. Hombre UNIV CINCINNATI - Estados Unidos
University of Cincinnati - Estados Unidos
2 Cesta, Jason M. Hombre UNIV CINCINNATI - Estados Unidos
University of Cincinnati - Estados Unidos
3 Galewsky, Joseph Hombre UNIV NEW MEXICO - Estados Unidos
The University of New Mexico - Estados Unidos
4 SAGREDO-TAPIA, ESTEBAN ANDRES Hombre Pontificia Universidad Católica de Chile - Chile
Núcleo Milenio Paleoclima - Chile

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 4.0 %
Citas No-identificadas: 96.0 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 4.0 %
Citas No-identificadas: 96.0 %

Financiamiento



Fuente
National Science Foundation
NSF
University of New Mexico Latin American and Iberian Institute
University of New Mexico Research Allocations Committee
New Mexico EPSCoR

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Agradecimientos



Agradecimiento
The authors would like to thank Marc Caffee, J Radler, and Susan Ma at PRIME Lab for AMS support; Bob Anderson, Miriam Duhnforth, and Kurt Refsnider for logistical support at the University of Colorado Cosmogenic Isotope Lab and Sarah Hammer for support at the University of Cincinnati Cosmogenic Isotope Labs; as well as Kimberly Samuels, Alex Lechler, Chris Sheehan, and the staffs of the Atacama Large Millimeter/Submillimeter Array and the Caltech Chajnantor Test Facility for assistance in the field. We thank Tom Lowell and Andrew Malone for discussion that helped clarify some of the ideas presented here. Funding was provided by the University of New Mexico Research Allocations Committee, the University of New Mexico Latin American and Iberian Institute, and NSF grants EPS-0918635 and EPS-0814449 (New Mexico EPSCoR) and EAR-1226611 (Geomorphology and Landuse Dynamics). We thank two anonymous referees for unusually thorough and constructive reviews.
The authors would like to thank Marc Caffee, J Radler, and Susan Ma at PRIME Lab for AMS support; Bob Anderson, Miriam Dühnforth, and Kurt Refsnider for logistical support at the University of Colorado Cosmogenic Isotope Lab and Sarah Hammer for support at the University of Cincinnati Cosmogenic Isotope Labs; as well as Kimberly Samuels, Alex Lechler, Chris Sheehan, and the staffs of the Atacama Large Millimeter/Submillimeter Array and the Caltech Chajnantor Test Facility for assistance in the field. We thank Tom Lowell and Andrew Malone for discussion that helped clarify some of the ideas presented here. Funding was provided by the University of New Mexico Research Allocations Committee , the University of New Mexico Latin American and Iberian Institute , and NSF grants EPS-0918635 and EPS-0814449 (New Mexico EPSCoR) and EAR-1226611 (Geomorphology and Landuse Dynamics). We thank two anonymous referees for unusually thorough and constructive reviews.

Muestra la fuente de financiamiento declarada en la publicación.