Abstract

Here we present an overview of speleothem δ18O records from South America, most of which are available in the Speleothem Isotopes Synthesis and Analysis (SISAL_v1) database. South American tropical and subtropical speleothem δ18O time series are primarily interpreted to reflect changes in precipitation amount, the amount effect, and consequently history of convection intensity variability of convergence zones such as the Intertropical Convergence Zone (ITCZ) and the South America Monsoon System (SAMS). We investigate past hydroclimate scenarios in South America related to the South American Monsoon System in three different time periods: Late Pleistocene, Holocene, and the last two millennia. Precession driven summertime insolation is the main driver of convective variability over the continent during the last 120 kyrs (from present day to 120 kyrs BP), including the Holocene. However, there is a dipole between speleothem δ18O records from western and eastern South America. Records located in the central region of Brazil are weakly affected by insolation-driven variability, and instead are more susceptible to the variability associated with the South Atlantic Convergence Zone (SACZ). Cold episodic events in the Northern Hemisphere, such as Heinrich and Bond Events, and the Little Ice Age, increase the convective activity of the SAMS, resulting in increased precipitation amount in South America.

Highlights

  • Rainfall variability in South America is primarily driven by the Intertropical Convergence Zone (ITCZ) [1], the South American Monsoon System (SAMS) [2], and to a lesser extent, other forcings such as South Atlantic cyclones (SACs), the Southern Hemisphere westerly winds (SHWW), and past

  • We have identified 75 individual speleothem isotope records from South America from the speleothem records identified in the literature but not yet in SISAL_v1 (Section 2)

  • Only a few studies report speleothem δ18 O time series on orbital time-scales in regions where the precipitation pattern is dominantly influenced by SAMS variability

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Summary

Introduction

Rainfall variability in South America is primarily driven by the Intertropical Convergence Zone (ITCZ) [1], the South American Monsoon System (SAMS) [2], and to a lesser extent, other forcings such as South Atlantic cyclones (SACs), the Southern Hemisphere westerly winds (SHWW), and past. Marcelo Arévalo Cave (MA Cave), and Panama (Chilibrillo Cave) are the only records available in (3.1) focuses on SAMS variations associated with changes in insolation due to variations in Earth’s the literature that are outside the SAMS region. We have identified 75 individual speleothem isotope records from South America from the literature (Table 1). SISAL_v1 database suitable for characterization of SAMS variability over the past 30 kyrs, but again, the need tothe increase spatio-temporal coverage ofcoverage speleothem records. From about 20 to 15 kyrs BP, the available speleothem isotope time series show a clear peak

Insolation Forced Changes of the SAMS
Orbital changes in South
Wavelet of analyses of the BT2
Millennial-Scale
Insolation Driven Holocene δ18 O Records
Dipole of Holocene δ18 O Values
Holocene Variations of the South Atlantic Convergence Zone
Summary on South American Monsoon System Variability
Outlook and Potentials for Future Speleothem-Based Empirical Research
Next Steps and Potentials for SISAL-Based Research
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