Sea surface temperature reconstruction for sediment core KH-10-7 COR1GC from the Conrad Rise, Southern Ocean

• Main Authors: Orme, Lisa C, Crosta, Xavier, Miettinen, Arto, Divine, Dmitry V, Husum, Katrine, Isaksson, Elisabeth, Wacker, Lukas, Mohan, Rahul, Ther, Oliver, Ikehara, Minoru
• Format: Dataset
• Language: English
• Published: PANGAEA 2020
• Subjects: AGE; calibrated; Calculated; Conrad Rise; Deglaciation; DEPTH; sediment/rock; diatoms; GC; Gravity corer; Holocene; KH-10-7_COR1GC; Sea ice concentration; Sea surface temperature; Southern Ocean; Temperature; water; maximum; minimum; Indian; ice core; Sea ice
• Online Access: https://doi.pangaea.de/10.1594/PANGAEA.913621; https://doi.org/10.1594/PANGAEA.913621

Centennial and millennial scale variability of Southern Ocean temperature is poorly known, due to both short instrumental records and sparsely distributed high-resolution temperature reconstructions, with evidence for past temperature variability instead coming mainly from ice core records. Here we present a high-resolution (~ 60 year), diatom-based sea-surface temperature (SST) reconstruction from the western Indian sector of the Southern Ocean that spans the interval 14.2 to 1.0 ka BP (calibrated kiloyears before present). During the late deglaciation, the new SST record shows cool temperatures at 14.2–12.9 ka BP and gradual warming between 12.9–11.6 ka BP in phase with atmospheric temperature evolution. This supports that the temperature of the Southern Ocean during the deglaciation was linked with a complex combination of processes and drivers associated with reorganisations of atmospheric and oceanic circulation patterns. Specifically, we suggest that Southern Ocean surface warming coincided, within the dating uncertainties, with the reconstructed slowdown of the Atlantic Meridional Overturning Circulation (AMOC), rising atmospheric CO2 levels, changes in the southern westerly winds and enhanced upwelling. During the Holocene the record shows warm and stable temperatures from 11.6–8.7 ka BP followed by a slight cooling and greater variability from 8.7 to 1 ka BP, with a quasi-periodic variability of 200–260 years as identified by spectral analysis. We suggest that the increased variability during the mid to late Holocene may reflect the establishment of centennial variability in SST connected with changes in the high latitude atmospheric circulation and Southern Ocean convection, as identified in models.