An investigation of carbon cycle dynamics since the Last Glacial Maximum: Complex interactions between the terrestrial biosphere, weathering, ocean alkalinity, and CO2 radiative warming in an Earth system model of intermediate complexity
| Autor: | Lawrence A. Mysak, H. D. Matthews, C. T. Simmons |
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| Rok vydání: | 2016 |
| Předmět: |
010506 paleontology
geography geography.geographical_feature_category Milankovitch cycles 010504 meteorology & atmospheric sciences Last Glacial Maximum 15. Life on land Radiative forcing 01 natural sciences Carbon cycle 13. Climate action Climatology Paleoclimatology Deglaciation Climate model Ice sheet Geology 0105 earth and related environmental sciences |
| DOI: | 10.5194/cp-2016-24 |
| Popis: | Proxy reconstructions and modeling studies of the glacial-interglacial changes in the global carbon cycle have led to a stimulating debate in the paleoclimate literature about the mechanisms leading to a 90–100 ppmv increase in atmospheric CO2. In this paper, we used the University of Victoria Earth System Climate Model v. 2.9 to simulate the carbon cycle response to ice sheet retreat and Milankovitch (insolation) forcing from the Last Glacial Maximum (LGM) to the present. In addition, we conducted sensitivity studies to address the contributions of CO2 radiative forcing, atmospheric carbon content, and weathering rates to climate and carbon cycle changes since 21 kyr BP. The simulations show that ice sheet and orbital changes by themselves do not lead to a notable increase in atmospheric CO2 over the course of deglaciation. However, with the application of CO2 radiative forcing and different weathering rates, the simulated atmospheric CO2 variations ranged over ~ 35 ppmv. Virtually all of the simulated net global vegetation carbon uptake since the LGM is attributable to CO2 fertilization rather than greater land availability or warmer temperatures. Furthermore, the ‘greening’ from CO2 fertilization significantly enhances total deglacial warming (by 0.14°C) and contributes to warmer intermediate and deep ocean temperatures during the interglacial period. We also found that CO2 radiative forcing was the dominant factor allowing for greater outgassing at the ocean surface and an earlier ventilation of deep-ocean DIC. The downwelling of high-alkalinity surface waters stimulated by a stronger, earlier overturning circulation led to greater deep sedimentation (alkalinity removal), which, in turn, permitted CO2 to continue to increase through much of the simulation period. |
| Databáze: | OpenAIRE |
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