Research ArticleEvidence of Southern Ocean influence into the far Northwest Pacific (Northern Emperor Rise) since the Bølling–Allerød warming
Introduction
The concentration of carbon dioxide (CO2) in the atmosphere is largely determined by the interplay between primary productivity, which regulates the uptake of CO2 into the deep oceanic carbon reservoir (biological carbon pump), and ocean circulation, which determines organic respiration in water and escape of CO2 into the atmosphere (Sigman and Boyle, 2000) The atmospheric CO2 content during the Last Glacial Maximum (LGM, ~23–19 ka) was ~80 ppmv lower than its preindustrial level, but the exact mechanisms responsible for this change remain elusive. During Heinrich Stadial 1 (HS1, 17.5–14.7 ka), a millennial-scale cold event in the Northern Hemisphere, there was a first pulse in the rise in atmospheric CO2, a drop in atmospheric 14C accompanied by rapid deposition of opal in the Southern Ocean, and a dramatic decrease in the Atlantic Meridional Overturning Circulation (AMOC) (Anderson et al., 2009; Marchitto et al., 2007; McManus et al., 2004; Monnin et al., 2001). The Southern Ocean may have been a main driver in controlling atmospheric CO2 levels, by accumulating CO2 in the deep oceans during glacials, then releasing it into the atmosphere through upwelling of deep waters around Antarctica during deglaciation (Anderson et al., 2009; Burke and Robinson, 2012; Jansen and Nadeau, 2016; Marshall and Speer, 2012; Sigman et al., 2010). However, the potential mechanisms by which changes in meridional overturning circulation may control ocean–atmosphere CO2 exchange are not clear, and especially the role of the Pacific Ocean, the largest ocean and thus the main reservoir of CO2, is not known (Marshall and Speer, 2012). Paleoceanographers have been studying the subarctic North Pacific extensively during the last decades, because this region is the last link of the global meridional overturning circulation (Du et al., 2018; Galbraith et al., 2007; Gebhardt et al., 2008; Gong et al., 2019; Jaccard et al., 2005; Jaccard and Galbraith, 2013; Keigwin, 1998; Okazaki et al., 2010). Radiocarbon data of paired benthic (BF) and planktic foraminifera (PF), the δ13C of BF and other proxies suggest that North Pacific Intermediate Water (NPIW) was well ventilated during HS1 (Ahagon et al., 2003; Max et al., 2014; Okazaki et al., 2012), while deep oceans remained poorly ventilated (Galbraith et al., 2007; Jaccard and Galbraith, 2013; Max et al., 2014). Deep water ventilation of the western and eastern subarctic Pacific may have been significantly different (Okazaki et al., 2012, Okazaki et al., 2010). There is considerable evidence for increased deep water ventilation in the northeastern (NE) Pacific during the last deglaciation (Du et al., 2018; Marchitto et al., 2007; Okazaki et al., 2010). A large drop in radiocarbon activity in intermediate waters during HS1 and Younger Dryas (YD, 12.9–11.8 ka), as measured in BF in a core from the continental margin of southern Baja California, requires an injection of old waters from a previously isolated deep-ocean carbon reservoir (Marchitto et al., 2007). Based on changes in neodymium isotope values in a core from the NE Pacific (Gulf of Alaska), Du et al. (2018) inferred that acceleration of NE Pacific abyssal circulation during HS1 was mostly controlled by flushing of Antarctic Bottom Water, triggered by Southern Hemisphere warming and sea ice retreat in the Southern Ocean.
The history of western subarctic Pacific deep ventilation during the last deglaciation is controversial (Galbraith et al., 2007; Gebhardt et al., 2008; Keigwin, 1998; Max et al., 2014; Okazaki et al., 2010). Based on BF stable isotope data from more than 30 cores from the Northern Emperor Rise (NER) and the Okhotsk Sea from depths of 1000–4000 m, Keigwin (1998) suggested that an intermediate water mass in the far northwestern (NW) Pacific was better ventilated during the LGM than during the Holocene, but deep waters were as nutrient-rich as today. Compiling radiocarbon ages from the NW Pacific, Okazaki et al. (2010) concluded that the average ventilation rate of intermediate-to-deep waters (900 to 2800 m) during the LGM was ~1500 years, then decreased to nearly 950 years during HS1, and increased again to ~1550 years during the Bølling/Allerød (B/A) warming (14.7–12.9 ka). Galbraith et al. (2007) concluded that abrupt and strong NW Pacific deep water ventilation since 14.6 ka was caused by an increase in deep water formation in the North Atlantic, but Jaccard and Galbraith (2013) combined redox-sensitive trace metal data from core PC13 (2393 m depth, NW Pacific; Fig. 1) with previously published data and did not find changes in ventilation at intermediate water depths during the early deglaciation. They suggested that the deepest core showing evidence for enhanced ventilation during HS1 was from 1366 m water depth, reflecting intensified intermediate water formation. Simulation of North Pacific ventilation by Earth System Modeling shows enhanced intermediate-to-deep ocean stratification due to intensified NPIW formation during HS1, relative to the LGM period (Gong et al., 2019). Increased input of nutrient- and CO2-rich water into this region, caused by wind-driven upwelling within the subpolar North Pacific and the collapse of NPIW formation, may have led to enhanced productivity during the B/A warming, based on boron isotope data of PF in a NW Pacific core and climate model simulations (Gray et al., 2018).
Here we present records of several productivity proxies, sea ice influence, δ18O and δ13C in BF and PF, redox-sensitive trace metals from six sediment cores from the NER (new data from three cores and previously published data from other three cores) and BF abundance and species composition for core MD-16 over the last 20 kyr. Age models of the sediment cores were based on accelerator mass spectrometry (AMS) 14C dating and robust regional indicators for correlation with the well-dated core MD-16 by atmospheric 14C plateau tuning (Sarnthein et al., 2015; Sarnthein, personal communication, 2019). In the results we provide new evidence of environmental evolution and deep water ventilation in the NER area since the LGM with abrupt input of Southern Ocean origin water into the deep water of NER at 14.5 ka, near the onset of B/A warming.
Section snippets
Oceanographic setting
The surface circulation of the subarctic North Pacific is characterized by a large-scale cyclonic pattern of surface currents with two counterclockwise circulating systems: the Alaskan Gyre in the NE Pacific and the Western Subarctic Gyre in the NW Pacific (Fig. 1). Today, the upper waters of the subarctic North Pacific have a strong, permanent halocline because the freshwater input is substantially higher than the evaporation rate. This halocline prevents deep water formation (Emile-Geay et
Core material
We present new data on three cores, LV63-4-2 (LV63-4), LV76-18-1 (LV76-18) and AV19/4 GC-36 (GC-36), combined with published data from other three cores: RAMA 44PC (R-44), GGC-37 (GC-37) and MD01–2416 (MD-16) (Table 1). Cores LV63-4 and LV76-18 were recovered by a gravity corer on the R/V “Akademik M.A. Lavrentyev” during Russian–Chinese expeditions in 2014 and 2016, respectively. Core GC-36 was recovered by a gravity corer during a Russian–American expedition in 1991, Leg 19/4 on the Russian
Age control
Age control for the cores is based on AMS 14C data on the PF N. pachyderma sin. In order to convert conventional AMS 14C data to calendar years, we used the plateau-tuning technique, i.e., we compared a suite of 14C atmosphere plateaus as recorded in Lake Suigetsu (Sarnthein et al., 2015), where AMS 14C ages of terrestrial macrofossils are placed in a varve-counted age model, thus showing the calendar ages of all 14C atmospheric plateaus (Bronk Ramsey et al., 2012, revised by Schlolaut, 2018).
Results
Fig. 2 shows records for productivity proxies (TOC, CaCO3, chlorin, and opal), δ18O and δ13C of PF and BF, and IRD of the three new cores, compared to published records for cores R-44 and MD-16 versus core depth and versus age for core GC-37 (Gebhardt et al., 2008; Keigwin, 1998; Keigwin et al., 1992). All proxies in all cores show a common pattern of variability over the last 20 kyr, consistent with the hypothesis of synchronicity of common environmental and hydrological changes occurring over
A precise age of the AICC as a milestone of NER hydrology
The PF N. pachyderma sin. and Globigerina bulloides which provided the more significant input into the CaCO3 content of regional sediments mostly dwell and calcify their shells in subsurface water close to the thermocline and surface water, respectively (Bauch et al., 1997; Kiefer et al., 2001; Riethdorf et al., 2013; Simstich et al., 2003). Therefore, their production as heterotrophic organisms is mostly determined by primary and bacterial productivity (Be, 1977). However, accumulation of PF
Conclusions
We present records of productivity proxies (CaCO3, opal, TOC and chlorin content), δ18O and δ13C of BF and PF, and IRD content over the last 20 kyr in six cores (three new and three previously published, all from 2300 to 3300 m depth) from the NER region, including the Meiji, Detroit and Tenji Seamounts. In addition, new data of redox-sensitive elemental content, and BF abundance and species composition for core MD-16 are presented. Age models for the cores were constructed using AMS 14C data
Declaration of Competing Interest
The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.
Acknowledgments
We are grateful to Dr. Lloyd Keigwin for the opportunity to measure the δ18O and δ13C of foraminifera in core GC-36 sediments in his lab, and to Dr. John Southon for kindly measuring AMS 14C data in the same core. We greatly appreciate Dr. Ellen Thomas and an anonymous reviewer for their valuable comments and editing. We thank Dr. Selvaraj Kandasamy (Xiamen University) for manuscript correction. This work was supported by the Russian Foundation for Basic Research (19–05–00663a), Ministry
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