Paleogeographic controls on the evolution of Late Cretaceous ocean circulation
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Published:2020-06-09
Issue:3
Volume:16
Page:973-1006
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ISSN:1814-9332
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Container-title:Climate of the Past
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language:en
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Short-container-title:Clim. Past
Author:
Ladant Jean-BaptisteORCID, Poulsen Christopher J.ORCID, Fluteau FrédéricORCID, Tabor Clay R., MacLeod Kenneth G.ORCID, Martin Ellen E., Haynes Shannon J.ORCID, Rostami Masoud A.
Abstract
Abstract. Understanding of the role of ocean circulation on climate during the Late
Cretaceous is contingent on the ability to reconstruct its modes and
evolution. Geochemical proxies used to infer modes of past circulation
provide conflicting interpretations for the reorganization of the ocean
circulation through the Late Cretaceous. Here, we present climate model
simulations of the Cenomanian (100.5–93.9 Ma) and Maastrichtian (72.1–66.1 Ma) stages of the Cretaceous with the CCSM4 earth system model. We
focus on intermediate (500–1500 m) and deep (> 1500 m) ocean
circulation and show that while there is continuous deep-water production
in the southwestern Pacific, major circulation changes occur between the
Cenomanian and Maastrichtian. Opening of the Atlantic and Southern Ocean, in
particular, drives a transition from a mostly zonal circulation to enhanced
meridional exchange. Using additional experiments to test the effect of
deepening of major ocean gateways in the Maastrichtian, we demonstrate that
the geometry of these gateways likely had a considerable impact on ocean
circulation. We further compare simulated circulation results with
compilations of εNd records and show that simulated
changes in Late Cretaceous ocean circulation are reasonably consistent with
proxy-based inferences. In our simulations, consistency with the geologic
history of major ocean gateways and absence of shift in areas of deep-water
formation suggest that Late Cretaceous trends in εNd
values in the Atlantic and southern Indian oceans were caused by the
subsidence of volcanic provinces and opening of the Atlantic and Southern
oceans rather than changes in deep-water formation areas and/or reversal of
deep-water fluxes. However, the complexity in interpreting Late Cretaceous
εNd values underscores the need for new records as well as
specific εNd modeling to better discriminate between the
various plausible theories of ocean circulation change during this period.
Publisher
Copernicus GmbH
Subject
Paleontology,Stratigraphy,Global and Planetary Change
Reference133 articles.
1. Andjić, G., Baumgartner, P. O., and Baumgartner-Mora, C.: Collision of
the Caribbean Large Igneous Province with the Americas: Earliest evidence
from the forearc of Costa Rica, Geological Society of America Bulletin,
2019. 2. Ando, A., Woodard, S. C., Evans, H. F., Littler, K., Herrmann, S., MacLeod,
K. G., Kim, S., Khim, B. K., Robinson, S. A., and Huber, B. T.: An emerging
palaeoceanographic “missing link”: multidisciplinary study of rarely
recovered parts of deep-sea Santonian–Campanian transition from Shatsky
Rise, J. Geol. Soc., 170, 381–384, 2013. 3. Arsouze, T., Dutay, J. C., Lacan, F., and Jeandel, C.: Modeling the
neodymium isotopic composition with a global ocean circulation model,
Chem. Geol., 239, 165–177, 2007. 4. Ayache, M., Dutay, J.-C., Arsouze, T., Révillon, S., Beuvier, J., and Jeandel, C.: High-resolution neodymium characterization along the Mediterranean margins and modelling of εNd distribution in the Mediterranean basins, Biogeosciences, 13, 5259–5276, https://doi.org/10.5194/bg-13-5259-2016, 2016. 5. Bardin, A., Primeau, F., and Lindsay, K.: An offline implicit solver for
simulating prebomb radiocarbon, Ocean Model., 73, 45–58, 2014.
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