We combine our previous ice-sheet and climate models to address abrupt climate changes pertaining to Heinrich (H) and Dansgaard-Oeschger (DO) cycles as well as last deglaciation punctuated by Younger Dryas (YD). We posit their common origin in the calving of the ice sheet but differentiate thermal triggers by geothermal-heat/surface-melt in calving inland/marginal ice, the respective sources of H/DO-cycles. The thermal switches would produce step-like freshwater fluxes to endow abruptness to the resulting climate signals characterized by millennial timescale due to the internal ice dynamics. For an eddying ocean, its response to the freshwater perturbation entails millennial adjustment to maximum entropy production, which would cause sudden post-H warming followed by gradual cooling to form the H-cycles, and the above-freezing warmth (hence surface-melt) would calve the marginal ice to generate DO-cycles anchored on the cooling trend to form the Bond cycle. Since there is already ablation of the Holocene icecap, there would be self-sustained DO-cycles, which thus retain the same pacing as their glacial counterparts to resolve this seeming puzzle. This millennial pacing also transcends the deglaciation to account for its observed sequence although the occurrence of YD requires a boost of the freshwater flux by the rerouted continental meltwater. It is seen that by differentiating thermal triggers of the ice calving and incorporating MEP adjustment of the ocean, the theory has provided an integrated account of the genesis of the abrupt climate changes and their deduced anatomies bear strong resemblance to the observed ones, in support of the theory.

Tongya Liu

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Most of the classic wind-driven circulation theories based on the Sverdrup balance have neglected the profound influence of eddy mixing on the large-scale distribution of the potential vorticity (PV), thus failing to explain some prominent features of the observed circulation. In this study, using a series of numerical experiments based on the MITgcm, we diagnose the PV balance to quantify the effect of eddy mixing on the subtropical gyre. Four grid-spacings of 1, 1/3.2, 1/10, and 1/32 degrees are selected to compare the structure of the upper-ocean circulation. In the 1° grid case, the structure of the thermocline is as predicted by the Sverdrup dynamics, with its maximum depth located in the subtropical interior where the wind stress curl is strongest. With increasing resolution, however, this maximum depth is displaced toward the subtropical front, which more closely resembles the observed thermocline. From 1° to 1/32°, the enhanced eddy mixing tends to homogenize the macroscopic PV in the subtropical gyre and reduces the latitudinal PV range to about 25% of the non-eddy solution; and the region where the Sverdrup balance holds is relegated to isolated patches, with its area reduced by about 60%. Furthermore, sensitivity experiments show that the observed thermocline structure is well reproduced in eddy-resolving runs, indicating that the PV mixing provides a better explanation of the subtropical circulation than the Sverdrup dynamics. Our results suggest that the Sverdrup relationship should be treated carefully in the eddy-rich region, even in the subtropical interior.