δ 13 C decreases in the upper western South Atlantic during Heinrich Stadials 3 and 2
Abrupt millennial-scale climate change events of the last deglaciation (i.e. Heinrich Stadial 1 and the Younger Dryas) were accompanied by marked increases in atmospheric CO 2 (CO 2atm ) and decreases in its stable carbon isotopic ratios ( δ 13 C), i.e. δ 13 CO 2atm , presumably due to outgassing fr...
| Published in: | Climate of the Past |
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| Main Authors: | , , , , , |
| Format: | Article in Journal/Newspaper |
| Language: | English |
| Published: |
Copernicus Publications
2017
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| Subjects: | |
| Online Access: | https://doi.org/10.5194/cp-13-345-2017 https://doaj.org/article/8f16a480067d45b5aea904a29c10da01 |
| Summary: | Abrupt millennial-scale climate change events of the last deglaciation (i.e. Heinrich Stadial 1 and the Younger Dryas) were accompanied by marked increases in atmospheric CO 2 (CO 2atm ) and decreases in its stable carbon isotopic ratios ( δ 13 C), i.e. δ 13 CO 2atm , presumably due to outgassing from the ocean. However, information on the preceding Heinrich Stadials during the last glacial period is scarce. Here we present δ 13 C records from two species of planktonic foraminifera from the western South Atlantic that reveal major decreases (up to 1 ‰) during Heinrich Stadials 3 and 2. These δ 13 C decreases are most likely related to millennial-scale periods of weakening of the Atlantic meridional overturning circulation and the consequent increase (decrease) in CO 2atm ( δ 13 CO 2atm ). We hypothesise two mechanisms that could account for the decreases observed in our records, namely strengthening of Southern Ocean deep-water ventilation and weakening of the biological pump. Additionally, we suggest that air–sea gas exchange could have contributed to the observed δ 13 C decreases. Together with other lines of evidence, our data are consistent with the hypothesis that the CO 2 added to the atmosphere during abrupt millennial-scale climate change events of the last glacial period also originated in the ocean and reached the atmosphere by outgassing. The temporal evolution of δ 13 C during Heinrich Stadials 3 and 2 in our records is characterized by two relative minima separated by a relative maximum. This <q>w structure</q> is also found in North Atlantic and South American records, further suggesting that such a structure is a pervasive feature of Heinrich Stadial 2 and, possibly, also Heinrich Stadial 3. |
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