Southern Hemisphere westerlies as a driver of the early deglacial atmospheric CO2 rise

L. Menviel (), P. Spence, J. Yu, M. A. Chamberlain, R. J. Matear, K. J. Meissner and M. H. England
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L. Menviel: University of New South Wales
P. Spence: University of New South Wales
J. Yu: The Australian National University
M. A. Chamberlain: CSIRO Oceans and Atmosphere
R. J. Matear: CSIRO Oceans and Atmosphere
K. J. Meissner: University of New South Wales
M. H. England: University of New South Wales

Nature Communications, 2018, vol. 9, issue 1, 1-12

Abstract: Abstract The early part of the last deglaciation is characterised by a ~40 ppm atmospheric CO2 rise occurring in two abrupt phases. The underlying mechanisms driving these increases remain a subject of intense debate. Here, we successfully reproduce changes in CO2, δ13C and Δ14C as recorded by paleo-records during Heinrich stadial 1 (HS1). We show that HS1 CO2 increase can be explained by enhanced Southern Ocean upwelling of carbon-rich Pacific deep and intermediate waters, resulting from intensified Southern Ocean convection and Southern Hemisphere (SH) westerlies. While enhanced Antarctic Bottom Water formation leads to a millennial CO2 outgassing, intensified SH westerlies induce a multi-decadal atmospheric CO2 rise. A strengthening of SH westerlies in a global eddy-permitting ocean model further supports a multi-decadal CO2 outgassing from the Southern Ocean. Our results highlight the crucial role of SH westerlies in the global climate and carbon cycle system with important implications for future climate projections.

Date: 2018
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DOI: 10.1038/s41467-018-04876-4

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