Response of Iberian Margin sediments to orbital and suborbital forcing over the past 420 ka

Here we report 420 kyr long records of sediment geochemical and color variations from the southwestern Iberian Margin. We synchronized the Iberian Margin sediment record to Antarctic ice cores and speleothem records on millennial time scales and investigated the phase responses relative to orbital f...

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Published in:Paleoceanography
Main Authors: Hodell, David, Crowhurst, Simon, Skinner, Luke, Tzedakis, Polychronis C., Margari, Vasiliki, Channell, James E.T., Kamenov, George, Maclachlan, Suzanne, Rothwell, Guy
Format: Article in Journal/Newspaper
Language:English
Published: 2013
Subjects:
Online Access:http://nora.nerc.ac.uk/id/eprint/502220/
https://nora.nerc.ac.uk/id/eprint/502220/1/palo20017_Hodell.pdf
https://doi.org/10.1002/palo.20017
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spelling ftnerc:oai:nora.nerc.ac.uk:502220 2023-05-15T13:48:07+02:00 Response of Iberian Margin sediments to orbital and suborbital forcing over the past 420 ka Hodell, David Crowhurst, Simon Skinner, Luke Tzedakis, Polychronis C. Margari, Vasiliki Channell, James E.T. Kamenov, George Maclachlan, Suzanne Rothwell, Guy 2013-03 text http://nora.nerc.ac.uk/id/eprint/502220/ https://nora.nerc.ac.uk/id/eprint/502220/1/palo20017_Hodell.pdf https://doi.org/10.1002/palo.20017 en eng https://nora.nerc.ac.uk/id/eprint/502220/1/palo20017_Hodell.pdf Hodell, David; Crowhurst, Simon; Skinner, Luke; Tzedakis, Polychronis C.; Margari, Vasiliki; Channell, James E.T.; Kamenov, George; Maclachlan, Suzanne; Rothwell, Guy. 2013 Response of Iberian Margin sediments to orbital and suborbital forcing over the past 420 ka. Paleoceanography, 28 (1). 185-199. https://doi.org/10.1002/palo.20017 <https://doi.org/10.1002/palo.20017> Publication - Article PeerReviewed 2013 ftnerc https://doi.org/10.1002/palo.20017 2023-02-04T19:37:08Z Here we report 420 kyr long records of sediment geochemical and color variations from the southwestern Iberian Margin. We synchronized the Iberian Margin sediment record to Antarctic ice cores and speleothem records on millennial time scales and investigated the phase responses relative to orbital forcing of multiple proxy records available from these cores. Iberian Margin sediments contain strong precession power. Sediment “redness” (a* and 570–560 nm) and the ratio of long-chain alcohols to n-alkanes (C26OH/(C26OH + C29)) are highly coherent and in-phase with precession. Redder layers and more oxidizing conditions (low alcohol ratio) occur near precession minima (summer insolation maxima). We suggest these proxies respond rapidly to low-latitude insolation forcing by wind-driven processes (e.g., dust transport, upwelling, precipitation). Most Iberian Margin sediment parameters lag obliquity maxima by 7–8 ka, indicating a consistent linear response to insolation forcing at obliquity frequencies driven mainly by high-latitude processes. Although the lengths of the time series are short (420 ka) for detecting 100 kyr eccentricity cycles, the phase relationships support those obtained by Shackleton []. Antarctic temperature and the Iberian Margin alcohol ratios (C26OH/(C26OH + C29)) lead eccentricity maxima by 6 kyr, with lower ratios (increased oxygenation) occurring at eccentricity maxima. CO2, CH4, and Iberian SST are nearly in phase with eccentricity, and minimum ice volume (as inferred from Pacific δ18Oseawater) lags eccentricity maxima by 10 kyr. The phase relationships derived in this study continue to support a potential role of the Earth's carbon cycle in contributing to the 100 kyr cycle. Article in Journal/Newspaper Antarc* Antarctic Natural Environment Research Council: NERC Open Research Archive Antarctic Shackleton Pacific Paleoceanography 28 1 185 199
institution Open Polar
collection Natural Environment Research Council: NERC Open Research Archive
op_collection_id ftnerc
language English
description Here we report 420 kyr long records of sediment geochemical and color variations from the southwestern Iberian Margin. We synchronized the Iberian Margin sediment record to Antarctic ice cores and speleothem records on millennial time scales and investigated the phase responses relative to orbital forcing of multiple proxy records available from these cores. Iberian Margin sediments contain strong precession power. Sediment “redness” (a* and 570–560 nm) and the ratio of long-chain alcohols to n-alkanes (C26OH/(C26OH + C29)) are highly coherent and in-phase with precession. Redder layers and more oxidizing conditions (low alcohol ratio) occur near precession minima (summer insolation maxima). We suggest these proxies respond rapidly to low-latitude insolation forcing by wind-driven processes (e.g., dust transport, upwelling, precipitation). Most Iberian Margin sediment parameters lag obliquity maxima by 7–8 ka, indicating a consistent linear response to insolation forcing at obliquity frequencies driven mainly by high-latitude processes. Although the lengths of the time series are short (420 ka) for detecting 100 kyr eccentricity cycles, the phase relationships support those obtained by Shackleton []. Antarctic temperature and the Iberian Margin alcohol ratios (C26OH/(C26OH + C29)) lead eccentricity maxima by 6 kyr, with lower ratios (increased oxygenation) occurring at eccentricity maxima. CO2, CH4, and Iberian SST are nearly in phase with eccentricity, and minimum ice volume (as inferred from Pacific δ18Oseawater) lags eccentricity maxima by 10 kyr. The phase relationships derived in this study continue to support a potential role of the Earth's carbon cycle in contributing to the 100 kyr cycle.
format Article in Journal/Newspaper
author Hodell, David
Crowhurst, Simon
Skinner, Luke
Tzedakis, Polychronis C.
Margari, Vasiliki
Channell, James E.T.
Kamenov, George
Maclachlan, Suzanne
Rothwell, Guy
spellingShingle Hodell, David
Crowhurst, Simon
Skinner, Luke
Tzedakis, Polychronis C.
Margari, Vasiliki
Channell, James E.T.
Kamenov, George
Maclachlan, Suzanne
Rothwell, Guy
Response of Iberian Margin sediments to orbital and suborbital forcing over the past 420 ka
author_facet Hodell, David
Crowhurst, Simon
Skinner, Luke
Tzedakis, Polychronis C.
Margari, Vasiliki
Channell, James E.T.
Kamenov, George
Maclachlan, Suzanne
Rothwell, Guy
author_sort Hodell, David
title Response of Iberian Margin sediments to orbital and suborbital forcing over the past 420 ka
title_short Response of Iberian Margin sediments to orbital and suborbital forcing over the past 420 ka
title_full Response of Iberian Margin sediments to orbital and suborbital forcing over the past 420 ka
title_fullStr Response of Iberian Margin sediments to orbital and suborbital forcing over the past 420 ka
title_full_unstemmed Response of Iberian Margin sediments to orbital and suborbital forcing over the past 420 ka
title_sort response of iberian margin sediments to orbital and suborbital forcing over the past 420 ka
publishDate 2013
url http://nora.nerc.ac.uk/id/eprint/502220/
https://nora.nerc.ac.uk/id/eprint/502220/1/palo20017_Hodell.pdf
https://doi.org/10.1002/palo.20017
geographic Antarctic
Shackleton
Pacific
geographic_facet Antarctic
Shackleton
Pacific
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Antarctic
genre_facet Antarc*
Antarctic
op_relation https://nora.nerc.ac.uk/id/eprint/502220/1/palo20017_Hodell.pdf
Hodell, David; Crowhurst, Simon; Skinner, Luke; Tzedakis, Polychronis C.; Margari, Vasiliki; Channell, James E.T.; Kamenov, George; Maclachlan, Suzanne; Rothwell, Guy. 2013 Response of Iberian Margin sediments to orbital and suborbital forcing over the past 420 ka. Paleoceanography, 28 (1). 185-199. https://doi.org/10.1002/palo.20017 <https://doi.org/10.1002/palo.20017>
op_doi https://doi.org/10.1002/palo.20017
container_title Paleoceanography
container_volume 28
container_issue 1
container_start_page 185
op_container_end_page 199
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