Abstract

The deglacial history of CO2 release from the deep North Pacific remains unresolved. This is due to conflicting indications about subarctic Pacific ventilation changes based on various marine proxies, especially for Heinrich Stadial 1 (HS-1) when a rapid atmospheric CO2 rise occurs. Here, we use a complex Earth System Model to investigate the deglacial North Pacific overturning and its control on ocean stratification. Our results show an enhanced intermediate-to-deep ocean stratification coeval with intensified North Pacific Intermediate Water (NPIW) formation during HS-1, compared to the Last Glacial Maximum. The stronger NPIW formation causes lower salinities and higher temperatures at intermediate depths. By lowering NPIW densities, this enlarges vertical density gradient and thus enhances intermediate-to-deep ocean stratification during HS-1. Physically, this process prevents the North Pacific deep waters from a better communication with the upper oceans, thus prolongs the existing isolation of glacial Pacific abyssal carbons during HS-1.

Highlights

  • The deglacial history of CO2 release from the deep North Pacific remains unresolved

  • The rapid atmospheric CO2 rise during the Atlantic Meridional Overturning Circulation (AMOC) offmode in Heinrich Stadial 1 (HS-1, 17.5-14.9 ka) is thought to be mainly induced by the CO2 outgassing from the Southern Ocean[2,3,4,5] and a lower efficiency of the biological carbon pump globally[6,7]

  • Our work aims to complement the limitations of currently available proxy evidence in identifying the paleo-physical mechanisms of the HS-1 intensified North Pacific ventilation and development of North Pacific deep-ocean stratification

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Summary

Introduction

The deglacial history of CO2 release from the deep North Pacific remains unresolved. This is due to conflicting indications about subarctic Pacific ventilation changes based on various marine proxies, especially for Heinrich Stadial 1 (HS-1) when a rapid atmospheric CO2 rise occurs. Paleoceanographic studies have hypothesized a role of potential sea ice expansion in causing a deeper ventilation (Fig. 1a–c) and probably stronger NPIW formation in HS-1 than during the LGM15,18–20, besides a direct control of a colder surface ocean[21].

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