1. Identificação | |
Tipo de Referência | Artigo em Revista Científica (Journal Article) |
Site | plutao.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | J8LNKAN8RW/3D53MH6 |
Repositório | dpi.inpe.br/plutao/2012/11.28.16.58.52 (acesso restrito) |
Última Atualização | 2013:01.28.12.20.06 (UTC) administrator |
Repositório de Metadados | dpi.inpe.br/plutao/2012/11.28.16.58.53 |
Última Atualização dos Metadados | 2018:06.05.00.02.07 (UTC) administrator |
Chave Secundária | INPE--PRE/ |
DOI | 10.1016/j.palaeo.2012.04.003 |
ISSN | 0031-0182 |
Rótulo | lattes: 7888258901938956 3 LatrubesseSCMTHBA:2012:LaQuMe |
Chave de Citação | LatrubesseSCMTHBA:2012:LaQuMe |
Título | Late Quaternary megafans, fans and fluvio-aeolian interactions in the Bolivian Chaco, tropical South America |
Ano | 2012 |
Mês | Oct. |
Data de Acesso | 21 maio 2024 |
Tipo Secundário | PRE PI |
Número de Arquivos | 1 |
Tamanho | 3331 KiB |
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2. Contextualização | |
Autor | 1 Latrubesse, Edgardo Manuel 2 Stevaux, José Cândido 3 Cremon, Édipo Henrique 4 May, Jan-Hendrik 5 Tatumi, Sonia Hatsue 6 Hurtado, Martín A. 7 Bezada, Maximiliano 8 Argollo, Jaime B. |
Grupo | 1 2 3 DSR-OBT-INPE-MCTI-GOV-BR |
Afiliação | 1 2 3 Instituto Nacional de Pesquisas Espaciais (INPE) |
Endereço de e-Mail do Autor | 1 2 3 edipocremon@yahoo.com.br |
Endereço de e-Mail | edipocremon@yahoo.com.br |
Revista | Palaeogeography, Palaeoclimatology, Palaeoecology |
Volume | 356-357 |
Páginas | 75-88 |
Nota Secundária | A1_CIÊNCIAS_BIOLÓGICAS_I A2_ECOLOGIA_E_MEIO_AMBIENTE A1_FILOSOFIA_/_TEOLOGIA:subcomissão_FILOSOFIA A2_GEOCIÊNCIAS A1_GEOGRAFIA A1_INTERDISCIPLINAR A2_SAÚDE_COLETIVA |
Histórico (UTC) | 2012-11-28 23:06:30 :: lattes -> marciana :: 2012 2013-01-28 12:20:07 :: marciana -> administrator :: 2012 2018-06-05 00:02:07 :: administrator -> marciana :: 2012 |
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3. Conteúdo e estrutura | |
É a matriz ou uma cópia? | é a matriz |
Estágio do Conteúdo | concluido |
Transferível | 1 |
Tipo do Conteúdo | External Contribution |
Palavras-Chave | air mass alluvial fan biome deflation dune field eolian deposit fluvial deposit orography rainfall subtropical region Bolivia Gran Chaco South America chaco fluvio-aeolian megafans paleogeography quaternary tropical South America |
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. |
Área | SRE |
Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDSR > Late Quaternary megafans,... |
Conteúdo da Pasta doc | acessar |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | não têm arquivos |
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4. Condições de acesso e uso | |
Idioma | en |
Grupo de Usuários | administrator lattes marciana |
Visibilidade | shown |
Política de Arquivamento | denypublisher denyfinaldraft24 |
Permissão de Leitura | deny from all and allow from 150.163 |
Permissão de Atualização | não transferida |
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5. Fontes relacionadas | |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ER446E |
Divulgação | WEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX. |
Acervo Hospedeiro | dpi.inpe.br/plutao@80/2008/08.19.15.01 |
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6. Notas | |
Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url versiontype |
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7. Controle da descrição | |
e-Mail (login) | marciana |
atualizar | |
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