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Near collapse of the meridional SST gradient in the eastern equatorial Pacific during Heinrich Stadial 1

Journal

PALEOCEANOGRAPHY
Volume 28, Issue 4, Pages 663-674

Publisher

AMER GEOPHYSICAL UNION
DOI: 10.1002/2013PA002499

Keywords

meridional SST gradient; eastern equatorial Pacific; Heinrich Stadial 1

Funding

  1. NSF [OCE97-12024, OCE-9102410, 1010869]
  2. Canadian Foundation for Climate and Atmospheric Sciences (CFCAS)
  3. Canadian Institute for Advanced Research (CIFAR)
  4. Natural Sciences and Engineering Research Council (NSERC), Canada
  5. National Science Foundation (NSF), USA
  6. Directorate For Geosciences
  7. Div Atmospheric & Geospace Sciences [1010869] Funding Source: National Science Foundation

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Sea surface temperatures (SST) and inorganic continental input over the last 25,000years (25ka) are reconstructed in the far eastern equatorial Pacific (EEP) based on three cores stretching from the equatorial front (similar to 0.01 degrees N, ME0005-24JC) into the cold tongue region (similar to 3.6 degrees S; TR163-31P and V19-30). We revisit previously published alkenone-derived SST records for these sites and present a revised chronology for V19-30. Inorganic continental input is quantified at all three sites based on Th-230-normalized fluxes of the long-lived continental isotope thorium-232 and interpreted to be largely dust. Our data show a very weak meridional (cross-equatorial) SST gradient during Heinrich Stadial 1 (HS1, 18-15kaB.P.) and high dust input along with peak export production at and north of the equator. These findings are corroborated by an Earth system model experiment for HS1 that simulates intensified northeasterly trade winds in the EEP, stronger equatorial upwelling, and surface cooling. Furthermore, the related southward shift of the Intertropical Convergence Zone (ITCZ) during HS1 is also indicative of drier conditions in the typical source regions for dust.

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