Comparing glacial and Holocene opal fluxes in the Pacific sector of the Southern Ocean

dc.contributor.author Bradtmiller, Louisa I.
dc.contributor.author Anderson, Robert F.
dc.contributor.author Fleisher, Martin Q.
dc.contributor.author Burckle, Lloyd H.
dc.date.accessioned 2010-05-18T14:18:57Z
dc.date.available 2010-05-18T14:18:57Z
dc.date.issued 2009-06-03
dc.description Author Posting. © American Geophysical Union, 2009. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Paleoceanography 24 (2009): PA2214, doi:10.1029/2008PA001693. en_US
dc.description.abstract The silicic acid leakage hypothesis (SALH) predicts that during glacial periods excess silicic acid was transported from the Southern Ocean to lower latitudes, which favored diatom production over coccolithophorid production and caused a drawdown of atmospheric CO2. Downcore records of 230Th-normalized opal (biogenic silica) fluxes from 31 cores in the Pacific sector of the Southern Ocean were used to compare diatom productivity during the last glacial period to that of the Holocene and to examine the evidence for increased glacial Si export to the tropics. Average glacial opal fluxes south of the modern Antarctic Polar Front (APF) were less than during the Holocene, while average glacial opal fluxes north of the APF were greater than during the Holocene. However, the magnitude of the increase north of the APF was not enough to offset decreased fluxes to the south, resulting in a decrease in opal burial in the Pacific sector of the Southern Ocean during the last glacial period, equivalent to approximately 15 Gt opal ka−1. This is consistent with the work of Chase et al. (2003a), and satisfies the primary requirement of the SALH, assuming that the upwelled supply of Si was approximately equivalent during the Holocene and the glacial period. However, previous results from the equatorial oceans are inconsistent with the other predictions of the SALH, namely that either the Corg:CaCO3 ratio or the rate of opal burial should have increased during glacial periods. We compare the magnitudes of changes in the Southern Ocean and the tropics and suggest that Si escaping the glacial Southern Ocean must have had an alternate destination, possibly the continental margins. There is currently insufficient data to test this hypothesis, but the existence of this sink and its potential impact on glacial pCO2 remain interesting topics for future study. en_US
dc.description.sponsorship Funding for this research was provided in part by the U.S. NSF (grant OPP02-30268). We thank the core repository at LDEO and the Antarctic Research Facility at FSU for providing samples. en_US
dc.format.mimetype application/pdf
dc.format.mimetype image/jpeg
dc.format.mimetype text/plain
dc.identifier.citation Paleoceanography 24 (2009): PA2214 en_US
dc.identifier.doi 10.1029/2008PA001693
dc.identifier.uri https://hdl.handle.net/1912/3460
dc.language.iso en_US en_US
dc.publisher American Geophysical Union en_US
dc.relation.uri https://doi.org/10.1029/2008PA001693
dc.subject Southern Ocean en_US
dc.subject Silica cycles en_US
dc.subject Paleoceanography en_US
dc.title Comparing glacial and Holocene opal fluxes in the Pacific sector of the Southern Ocean en_US
dc.type Article en_US
dspace.entity.type Publication
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relation.isAuthorOfPublication.latestForDiscovery 68ed3000-3c93-433a-96b9-0015429c7fd8
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Figure S1: Magnetic susceptibility, % opal and % E. antarctica data for core E11-11.
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Figure S2: Opal and detrital fluxes, and 231Pa/230Th ratios (X 10) for core E11-11.
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Text S1: The text file describes the methods used to select cores for study, and methods used to create core chronologies.
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