Late Quaternary megafans, fans and fluvio-aeolian interactions in the Bolivian Chaco, Tropical South America

Detalhes bibliográficos
Autor(a) principal: Latrubesse, Edgardo M.
Data de Publicação: 2012
Outros Autores: Stevaux, Jose C., Cremon, Edipo H., May, Jan-Hendrik, Tatumi, Sonia H. [UNESP], Hurtado, Martín A., Bezada, Maximiliano, Argollo, Jaime B.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1016/j.palaeo.2012.04.003
http://hdl.handle.net/11449/219834
Resumo: The Chaco is a huge plain and a main biogeographic biome of South America dominated by subtropical semi-deciduous vegetation that spreads on the Andes footslope on more than 800,000km 2 through Bolivia, Argentina and Paraguay. The climate is tropical wet-dry and the South American Summer Monsoon (SASM) leads to intensive convective rainfall during the summer season. Some of the world's largest river-fans such as the Parapeti and Grande rivers megafans developed in the Bolivian Chaco. Our research was based on morpho-sedimentary information and sustained by 25 OSL dating of fluvial and aeolian sediments. We demonstrate that these megafans are bigger than previously postulated by some authors. Morphostratigraphic analysis, geochronological data and regional correlations suggest that the Chaco megafans and large piedmont fans were generated and reached maximum development during the middle pleniglacial and early pleniglacial (ca. 60 to 28ka) because of the presence of colder and more seasonal conditions (dry-wet intense contrasting seasons) than those existing today in the Amazon and the Bolivian plains. We suggest that a main mechanism triggering the megafan development was the presence of an intense monsoonal effect on the Eastern flank of the Andes that enhanced rainfall by orographic excitation during MIS 3 and the early part of MIS 2 that produced an increase in discharge and sediment supply. Concomitantly to fluvial processes the deflation of fluvial belts occurred and big sand dune fields developed by winds blowing out from North to South following the same pattern the South American lower level jet follows presently. Maximum aridity was reached during MIS 2 with the deposition of loess deposits on the piedmont areas and megafan surfaces, the continuous generation of aeolian dunes and a remarkable decrease in the fluvial activity. Cold air mass related to the polar advection (friagens or surazos) probably affected the area with more intensity and frequency. The Lateglacial was also arid but probably less extreme than the LGM. During a good part of the Holocene the climatic conditions were still arid to semiarid but became more similar to the present sub-humid climate since ~1.5ka. During the Holocene, the megafans and aeolian systems didn't reach Late Pleistocene size and level of activity. © 2012 Elsevier B.V.
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spelling Late Quaternary megafans, fans and fluvio-aeolian interactions in the Bolivian Chaco, Tropical South AmericaChacoFluvio-aeolianMegafansPaleogeographyQuaternaryTropical South AmericaThe Chaco is a huge plain and a main biogeographic biome of South America dominated by subtropical semi-deciduous vegetation that spreads on the Andes footslope on more than 800,000km 2 through Bolivia, Argentina and Paraguay. The climate is tropical wet-dry and the South American Summer Monsoon (SASM) leads to intensive convective rainfall during the summer season. Some of the world's largest river-fans such as the Parapeti and Grande rivers megafans developed in the Bolivian Chaco. Our research was based on morpho-sedimentary information and sustained by 25 OSL dating of fluvial and aeolian sediments. We demonstrate that these megafans are bigger than previously postulated by some authors. Morphostratigraphic analysis, geochronological data and regional correlations suggest that the Chaco megafans and large piedmont fans were generated and reached maximum development during the middle pleniglacial and early pleniglacial (ca. 60 to 28ka) because of the presence of colder and more seasonal conditions (dry-wet intense contrasting seasons) than those existing today in the Amazon and the Bolivian plains. We suggest that a main mechanism triggering the megafan development was the presence of an intense monsoonal effect on the Eastern flank of the Andes that enhanced rainfall by orographic excitation during MIS 3 and the early part of MIS 2 that produced an increase in discharge and sediment supply. Concomitantly to fluvial processes the deflation of fluvial belts occurred and big sand dune fields developed by winds blowing out from North to South following the same pattern the South American lower level jet follows presently. Maximum aridity was reached during MIS 2 with the deposition of loess deposits on the piedmont areas and megafan surfaces, the continuous generation of aeolian dunes and a remarkable decrease in the fluvial activity. Cold air mass related to the polar advection (friagens or surazos) probably affected the area with more intensity and frequency. The Lateglacial was also arid but probably less extreme than the LGM. During a good part of the Holocene the climatic conditions were still arid to semiarid but became more similar to the present sub-humid climate since ~1.5ka. During the Holocene, the megafans and aeolian systems didn't reach Late Pleistocene size and level of activity. © 2012 Elsevier B.V.Department of Geography and the Environment The University of Texas at Austin, Austin, TX, 78712GEMA- Department of Geography Universidade Estadual de Maringa, Maringa, PR 87020-900National Institute for Space Research (INPE) - Remote Sensing Division (DSR) São José dos Campos-SP, CEP 12227-010School of Earth and Environmental Sciences University of Wollongong, Wollongong, NSW 2500Laboratório de Vidros e Datacões FATEC, Faculdade de Tecnologia Universidade Estadual de São Paulo, São Paulo, SP, 01124-060Institute of Geomorphology and Soils Universidad Nacional de La Plata, La Plata, 1900Department of Geosciences Universidad Pedagógica El Libertador, CaracasDepartment of Geology Universidad Mayor de San Andres, La PazLaboratório de Vidros e Datacões FATEC, Faculdade de Tecnologia Universidade Estadual de São Paulo, São Paulo, SP, 01124-060The University of Texas at AustinUniversidade Estadual de Maringá (UEM)São José dos Campos-SPUniversity of WollongongUniversidade Estadual Paulista (UNESP)Universidad Nacional de La PlataUniversidad Pedagógica El LibertadorUniversidad Mayor de San AndresLatrubesse, Edgardo M.Stevaux, Jose C.Cremon, Edipo H.May, Jan-HendrikTatumi, Sonia H. [UNESP]Hurtado, Martín A.Bezada, MaximilianoArgollo, Jaime B.2022-04-28T18:58:01Z2022-04-28T18:58:01Z2012-10-15info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article75-88http://dx.doi.org/10.1016/j.palaeo.2012.04.003Palaeogeography, Palaeoclimatology, Palaeoecology, v. 356-357, p. 75-88.0031-0182http://hdl.handle.net/11449/21983410.1016/j.palaeo.2012.04.0032-s2.0-84865860860Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPalaeogeography, Palaeoclimatology, Palaeoecologyinfo:eu-repo/semantics/openAccess2022-04-28T18:58:01Zoai:repositorio.unesp.br:11449/219834Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-05-23T11:26:56.365166Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Late Quaternary megafans, fans and fluvio-aeolian interactions in the Bolivian Chaco, Tropical South America
title Late Quaternary megafans, fans and fluvio-aeolian interactions in the Bolivian Chaco, Tropical South America
spellingShingle Late Quaternary megafans, fans and fluvio-aeolian interactions in the Bolivian Chaco, Tropical South America
Latrubesse, Edgardo M.
Chaco
Fluvio-aeolian
Megafans
Paleogeography
Quaternary
Tropical South America
title_short Late Quaternary megafans, fans and fluvio-aeolian interactions in the Bolivian Chaco, Tropical South America
title_full Late Quaternary megafans, fans and fluvio-aeolian interactions in the Bolivian Chaco, Tropical South America
title_fullStr Late Quaternary megafans, fans and fluvio-aeolian interactions in the Bolivian Chaco, Tropical South America
title_full_unstemmed Late Quaternary megafans, fans and fluvio-aeolian interactions in the Bolivian Chaco, Tropical South America
title_sort Late Quaternary megafans, fans and fluvio-aeolian interactions in the Bolivian Chaco, Tropical South America
author Latrubesse, Edgardo M.
author_facet Latrubesse, Edgardo M.
Stevaux, Jose C.
Cremon, Edipo H.
May, Jan-Hendrik
Tatumi, Sonia H. [UNESP]
Hurtado, Martín A.
Bezada, Maximiliano
Argollo, Jaime B.
author_role author
author2 Stevaux, Jose C.
Cremon, Edipo H.
May, Jan-Hendrik
Tatumi, Sonia H. [UNESP]
Hurtado, Martín A.
Bezada, Maximiliano
Argollo, Jaime B.
author2_role author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv The University of Texas at Austin
Universidade Estadual de Maringá (UEM)
São José dos Campos-SP
University of Wollongong
Universidade Estadual Paulista (UNESP)
Universidad Nacional de La Plata
Universidad Pedagógica El Libertador
Universidad Mayor de San Andres
dc.contributor.author.fl_str_mv Latrubesse, Edgardo M.
Stevaux, Jose C.
Cremon, Edipo H.
May, Jan-Hendrik
Tatumi, Sonia H. [UNESP]
Hurtado, Martín A.
Bezada, Maximiliano
Argollo, Jaime B.
dc.subject.por.fl_str_mv Chaco
Fluvio-aeolian
Megafans
Paleogeography
Quaternary
Tropical South America
topic Chaco
Fluvio-aeolian
Megafans
Paleogeography
Quaternary
Tropical South America
description The Chaco is a huge plain and a main biogeographic biome of South America dominated by subtropical semi-deciduous vegetation that spreads on the Andes footslope on more than 800,000km 2 through Bolivia, Argentina and Paraguay. The climate is tropical wet-dry and the South American Summer Monsoon (SASM) leads to intensive convective rainfall during the summer season. Some of the world's largest river-fans such as the Parapeti and Grande rivers megafans developed in the Bolivian Chaco. Our research was based on morpho-sedimentary information and sustained by 25 OSL dating of fluvial and aeolian sediments. We demonstrate that these megafans are bigger than previously postulated by some authors. Morphostratigraphic analysis, geochronological data and regional correlations suggest that the Chaco megafans and large piedmont fans were generated and reached maximum development during the middle pleniglacial and early pleniglacial (ca. 60 to 28ka) because of the presence of colder and more seasonal conditions (dry-wet intense contrasting seasons) than those existing today in the Amazon and the Bolivian plains. We suggest that a main mechanism triggering the megafan development was the presence of an intense monsoonal effect on the Eastern flank of the Andes that enhanced rainfall by orographic excitation during MIS 3 and the early part of MIS 2 that produced an increase in discharge and sediment supply. Concomitantly to fluvial processes the deflation of fluvial belts occurred and big sand dune fields developed by winds blowing out from North to South following the same pattern the South American lower level jet follows presently. Maximum aridity was reached during MIS 2 with the deposition of loess deposits on the piedmont areas and megafan surfaces, the continuous generation of aeolian dunes and a remarkable decrease in the fluvial activity. Cold air mass related to the polar advection (friagens or surazos) probably affected the area with more intensity and frequency. The Lateglacial was also arid but probably less extreme than the LGM. During a good part of the Holocene the climatic conditions were still arid to semiarid but became more similar to the present sub-humid climate since ~1.5ka. During the Holocene, the megafans and aeolian systems didn't reach Late Pleistocene size and level of activity. © 2012 Elsevier B.V.
publishDate 2012
dc.date.none.fl_str_mv 2012-10-15
2022-04-28T18:58:01Z
2022-04-28T18:58:01Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1016/j.palaeo.2012.04.003
Palaeogeography, Palaeoclimatology, Palaeoecology, v. 356-357, p. 75-88.
0031-0182
http://hdl.handle.net/11449/219834
10.1016/j.palaeo.2012.04.003
2-s2.0-84865860860
url http://dx.doi.org/10.1016/j.palaeo.2012.04.003
http://hdl.handle.net/11449/219834
identifier_str_mv Palaeogeography, Palaeoclimatology, Palaeoecology, v. 356-357, p. 75-88.
0031-0182
10.1016/j.palaeo.2012.04.003
2-s2.0-84865860860
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Palaeogeography, Palaeoclimatology, Palaeoecology
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 75-88
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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