A reconstruction of atmospheric carbon dioxide and its stable carbon isotopic composition from the penultimate glacial maximum to the last glacial inception

• Published in: Climate of the Past
• Main Authors: Schneider, R., Schmitt, J., Köhler, P., Joos, F., Fischer, H.
• Format: Text
• Language: English
• Published: 2018
• Subjects: Antarctic; East Antarctica; Talos Dome; Antarc*; Antarctica; EPICA
• Online Access: https://doi.org/10.5194/cp-9-2507-2013; https://cp.copernicus.org/articles/9/2507/2013/

The reconstruction of the stable carbon isotope evolution in atmospheric CO 2 (δ 13 C atm ), as archived in Antarctic ice cores, bears the potential to disentangle the contributions of the different carbon cycle fluxes causing past CO 2 variations. Here we present a new record of δ 13 C atm before, during and after the Marine Isotope Stage 5.5 (155 000 to 105 000 yr BP). The dataset is archived on the data repository PANGEA® ( www.pangea.de ) under 10.1594/PANGAEA.817041 . The record was derived with a well established sublimation method using ice from the EPICA Dome C (EDC) and the Talos Dome ice cores in East Antarctica. We find a 0.4‰ shift to heavier values between the mean δ 13 C atm level in the Penultimate (~ 140 000 yr BP) and Last Glacial Maximum (~ 22 000 yr BP), which can be explained by either (i) changes in the isotopic composition or (ii) intensity of the carbon input fluxes to the combined ocean/atmosphere carbon reservoir or (iii) by long-term peat buildup. Our isotopic data suggest that the carbon cycle evolution along Termination II and the subsequent interglacial was controlled by essentially the same processes as during the last 24 000 yr, but with different phasing and magnitudes. Furthermore, a 5000 yr lag in the CO 2 decline relative to EDC temperatures is confirmed during the glacial inception at the end of MIS5.5 (120 000 yr BP). Based on our isotopic data this lag can be explained by terrestrial carbon release and carbonate compensation.