Clumped isotope constraints on upper tropospheric temperature changes during the last deglaciation

• Main Authors: Banerjee, A., Yeung, L., Yan, Y.
• Format: Conference Object
• Language: English
• Published: 2023
• Subjects: Antarctic; West Antarctic Ice Sheet; Antarc*; ice core; Ice Sheet
• Online Access: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5018279

The clumped-isotope composition of oxygen, denoted by Δ 36 , measures the proportional abundance of two heavy oxygen isotopes, 18 O 18 O in oxygen, and is sensitive to photochemical and thermal properties of the atmosphere. Ozone photochemistry controls Δ 36 values via isotope exchange reactions, yielding a higher abundance of 18 O 18 O than would be expected for a stochastic distribution. Colder temperatures increase this preference for 18 O 18 O formation at equilibrium by 0.013‰/K. If tropospheric ozone and stratosphere-troposphere exchange fluxes remain unchanged, Δ 36 would record changes in free-tropospheric temperatures to provide a high-resolution record of upper tropospheric (UT) temperatures on glacial-interglacial timescales. We present an ice core record of Δ 36 values measured in the West Antarctic Ice Sheet Divide ice core spanning 15–8ka BP. Measured Δ 36 values decrease to Early Holocene (EH; 8-11ka BP)/Pre-industrial (PI; 1850CE) levels at the onset of the Bølling Allerød (BA; 14.7–12.9ka BP) warm period, and continues into the Younger Dryas (YD; 12.9-11.7ka BP). Δ 36 values reach PI/EH when global-mean surface temperatures are still colder than those of PI/EH. This indicates either a change in the lapse rate feedback, or a significant increase in tropospheric ozone burden. Our investigations reveal no evidence for increased O 3 and that the decrease in Δ 36 is coeval with rapid decreases in Northern Hemisphere ice sheet elevation. Previous work highlights the influence of changing ice sheet elevation on the thermal structure of the atmosphere. A plausible explanation for our observation is that during periods of abrupt climate change the cryosphere plays a predominant role in governing UT temperatures.