Abstract

Abstract. The spatial patterns of global temperature and precipitation changes, as well as corresponding large-scale circulation patterns during the latter part of the 9th and 5th millennia BP (4800–4500 versus 4500–4000 BP and 9200–8800 versus 8800–8000 BP) are compared through a group of transient simulations using the Community Climate System Model version 3 (CCSM3). Both periods are characterized by significant sea surface temperature (SST) decreases over the North Atlantic, south of Iceland. Temperatures were also colder across the Northern Hemisphere but warmer in the Southern Hemisphere. Significant precipitation decreases are seen over most of the Northern Hemisphere, especially over Eurasia and the Asian monsoon regions, indicating a weaker summer monsoon. Large precipitation anomalies over northern South America and adjacent ocean regions are related to a southward displacement of the Intertropical Convergence Zone (ITCZ) in that region. Climate changes in the late 9th millennium BP (the “8.2 ka event”) are widely considered to have been caused by a large freshwater discharge into the northern Atlantic, which is confirmed in a meltwater forcing sensitivity experiment, but this was not the cause of changes occurring between the early and latter halves of the 5th millennium BP. Model simulations suggest that a combination of factors, led by long-term changes in insolation, drove a steady decline in SSTs across the North Atlantic and a reduction in the North Atlantic Meridional Overturning Circulation (AMOC), over the past 4500 years, with associated teleconnections across the globe, leading to drought in some areas. Multi-century-scale fluctuations in SSTs and AMOC strength were superimposed on this decline. This helps explain the onset of neoglaciation around 5000–4500 BP, followed by a series of neoglacial advances and retreats during recent millennia. The “4.2 ka BP Event” appears to have been one of several late Holocene multi-century fluctuations that were embedded in the long-term, low-frequency change in climate that occurred after ∼4.8 ka. Whether these multi-century fluctuations were a response to internal centennial-scale ocean–atmosphere variability or external forcing (such as explosive volcanic eruptions and associated feedbacks) or a combination of such conditions is not known and requires further study.

Highlights

  • It is well documented that the first-order driver of Holocene climate change was orbital forcing, with an overall decline in summer insolation in summer months, at high latitudes

  • The major changes in precipitation patterns were comparable but less pronounced from 4500–4000 BP. These similarities are somewhat puzzling as the meltwater forcing sensitivity experiment clearly shows that the 8.2 ka event was induced by a massive freshwater flux into the Atlantic, whereas no comparable meltwater event occurred in the late Holocene, so it seems unlikely that such forcing was a factor driving the changes seen in the model output for 4500–4000 BP

  • The Intertropical Convergence Zone (ITCZ) was displaced to the south across much of the globe, and monsoon regions of the Northern Hemisphere were generally drier

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Summary

Introduction

It is well documented that the first-order driver of Holocene climate change was orbital forcing, with an overall decline in summer insolation in summer months, at high latitudes. Wang (2009a) reviewed studies of Holocene cold events, and concluded that the most severe Holocene cold event, at ∼ 8.2 ka, was brought about by an outburst flood from proglacial Lake Agassiz This large volume of freshwater drained into the North Atlantic extremely rapidly, leading to a brief reorganization of the Atlantic Meridional Overturning Circulation (AMOC) and a southward displacement of the ITCZ, resulting in dry conditions over many regions (Barber et al, 1999; Bianchi and McCave, 1999; Risebrobakken et al, 2003; McManus et al, 2004; Clarke et al, 2004). As GCM simulations of the 4.2 ka BP Event have not received much attention, in this study, the spatial patterns and corresponding mechanisms relevant to the 4.2 ka BP Event are examined and compared to those associated with the 8.2 ka event

Data and methodology
Results
Discussion and conclusions

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