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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/3D53LQ3
Repositorydpi.inpe.br/plutao/2012/11.28.16.49.49   (restricted access)
Last Update2013:02.14.15.43.23 (UTC) marciana
Metadata Repositorydpi.inpe.br/plutao/2012/11.28.16.49.50
Metadata Last Update2018:06.05.00.02.06 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.sedgeo.2012.09.015
ISSN0037-0738
Labellattes: 0307721738107549 1 RossettiZanCohCohCre:2012:LaPlWe
Citation KeyRossettiZaniCoheCrem:2012:LaPlWe
TitleA Late Pleistocene-Holocene wetland megafan in the Brazilian Amazonia
Year2012
Access Date2024, May 04
Secondary TypePRE PI
Number of Files1
Size5963 KiB
2. Context
Author1 Rossetti, Dilce de Fátima
2 Zani, Hiran
3 Cohen, Marcelo
4 Cremon, Édipo Henrique
Resume Identifier1 8JMKD3MGP5W/3C9JGTQ
Group1 DSR-OBT-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 rossetti@dsr.inpe.br
2 hzani@dsr.inpe.br
3
4 edipocremon@yahoo.com.br
e-Mail Addressrossetti@dsr.inpe.br
JournalSedimentary Geology
Volume282
Pages276-293
Secondary MarkA1_ENGENHARIAS_III A2_GEOCIÊNCIAS
History (UTC)2012-11-28 23:06:30 :: lattes -> marciana :: 2012
2012-12-21 18:12:18 :: marciana -> administrator :: 2012
2013-01-20 15:55:03 :: administrator -> marciana :: 2012
2013-02-14 15:43:23 :: marciana -> administrator :: 2012
2018-06-05 00:02:06 :: administrator -> marciana :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordstropical wetland megafan
late Pleistocene–Holocene
facies model
residual morphology
monsoonal climate
tectonic subsidence
AbstractDespite the growing interest in megafans, definitions provided for this type of environmental setting have not yet been widely agreed upon. A record of sedimentary facies distribution in both space and time including a larger number of analogs is particularly needed for improving megafan facies models. This work focuses on a large fan-like feature from an Amazonian wetland in northern Brazil. Morphological data based on remote sensing, as well as sedimentary facies and radiocarbon analyses, were integrated to propose that this feature is related to a megafan system active during the Late Pleistocene to Holocene. The megafan displays a divergent drainage network, gently-dipping slope, and concave-up and convex-up longitudinal and transverse profiles, respectively. Near surface deposits correspond to fining and coarsening upward sands related to active channels and overbank sand sheets/terminal fan lobes. Sediments are interbedded with abandoned channel/floodplain and lake/pond muds. Morphostructural analyses and drainage anomalies revealed a geological setting affected by reactivation of pre-existing faults contemporaneous with sediment accumulation. Establishment of a megafan system in this wetland most likely occurred within a slightly tectonically subsiding basin under favorable climatic conditions. During wet seasons, high water discharge would have favored sediment transport from highlands into this depositional site. High summer temperatures and drought under a monsoonal regime kept the water levels low. The described megafan could serve as an analog for contemporary tropical wetland megafans formed under a monsoonal climate regime.
AreaSRE
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDSR > A Late Pleistocene-Holocene...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target File1-s2.0-S0037073812002758-main.pdf
User Groupadministrator
lattes
marciana
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ER446E
DisseminationWEBSCI; PORTALCAPES; COMPENDEX.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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