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Main Authors: Woodard, Stella C, Thomas, Deborah J, Marcantonio, Franco
Format: Dataset Open Access
Language:en
Published: PANGAEA 2012
Subjects:
Online Access:https://doi.org/10.1594/PANGAEA.813592
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author Woodard, Stella C
Thomas, Deborah J
Marcantonio, Franco
author_facet Woodard, Stella C
Thomas, Deborah J
Marcantonio, Franco
collection Datos científicos de ciencias marinas y ambientales
contents Eolian dust in pelagic deep sea sediments can be used to reconstruct ancient wind patterns and paleoenvironmental response to climate change. Traditional methods to determine dust accumulation involve isolating the non-dissolvable aluminosilicate minerals from deep sea sediments through a series of chemical leaches, but cannot differentiate between minerals from eolian, authigenic and volcanogenic sources. Other geochemical proxies, such as sedimentary 232Th and crustal 4He content, have been used to construct high-resolution records of atmospheric dust fluxes to the deep sea during the Quaternary. Here we use sedimentary Th content as a proxy for terrigenous material (eolian dust) in ~58 Myr-old sediments from the Shatsky Rise (ODP Site 1209) and compare our results with previous dust estimates generated using the traditional chemical extraction method and sedimentary 4He(crustal) concentrations. We find excellent agreement between Th-based dust estimates and those generated using the traditional method. In addition our results show a correlation between sedimentary Th and 4He(crustal) content, which suggests a source older than present day Asian loess supplied dust to the central subtropical Pacific Ocean during the early Paleogene.
format Dataset Open Access
id pangaea_https___doi_org_10_1594_PANGAEA_813592
institution PANGAEA
language en
publishDate 2012
publisher PANGAEA
record_format pangaea
spellingShingle Reconstruction of dust flux of ODP Hole 198-1209C
Woodard, Stella C
Thomas, Deborah J
Marcantonio, Franco
198-1209C; DRILL; Drilling/drill rig; Joides Resolution; Leg198; North Pacific Ocean; Ocean Drilling Program; ODP
Eolian dust in pelagic deep sea sediments can be used to reconstruct ancient wind patterns and paleoenvironmental response to climate change. Traditional methods to determine dust accumulation involve isolating the non-dissolvable aluminosilicate minerals from deep sea sediments through a series of chemical leaches, but cannot differentiate between minerals from eolian, authigenic and volcanogenic sources. Other geochemical proxies, such as sedimentary 232Th and crustal 4He content, have been used to construct high-resolution records of atmospheric dust fluxes to the deep sea during the Quaternary. Here we use sedimentary Th content as a proxy for terrigenous material (eolian dust) in ~58 Myr-old sediments from the Shatsky Rise (ODP Site 1209) and compare our results with previous dust estimates generated using the traditional chemical extraction method and sedimentary 4He(crustal) concentrations. We find excellent agreement between Th-based dust estimates and those generated using the traditional method. In addition our results show a correlation between sedimentary Th and 4He(crustal) content, which suggests a source older than present day Asian loess supplied dust to the central subtropical Pacific Ocean during the early Paleogene.
title Reconstruction of dust flux of ODP Hole 198-1209C
topic 198-1209C; DRILL; Drilling/drill rig; Joides Resolution; Leg198; North Pacific Ocean; Ocean Drilling Program; ODP
url https://doi.org/10.1594/PANGAEA.813592