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Southern Hemisphere Climate Forcing Mechanisms during the Last Glacial-Interglacial Transition

This study focuses on the first-order local forcing mechanisms in the Southern Hemisphere, specifically between 50°-90°S, during the last glacial-interglacial transition. The study examines the relationship between austral spring insolation changes, sea salt flux, and Antarctic climate. Results suggest that spring insolation changes contribute to the deglacial temperature rise and sea ice reduction. This study also highlights the importance of Northern Hemispheric warming and its impact on the Laurentide ice sheet.

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Southern Hemisphere Climate Forcing Mechanisms during the Last Glacial-Interglacial Transition

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  1. Aim: study the first order local forcing mechanisms Focusing on 50°-90°S (regional features will average out)

  2. Introduction In Antarctic sites • 20-17.5ka BP → 9-10ka BP • Temperature rose • Atmospheric CO2 concentration rose about 80 ppmv • Sea salt flux indicate that Antarctic sea ice started to retreat around 20-17ka ago.

  3. Introduction • Northern Hemispheric summer insolation leads Antarctic temperature. (Augustinet al.) • Local spring insolation changes in the Southern Hemisphere was recently suggested in Stott et al. • The length of the austral summerseason may provide an important climate forcingfor Southern Hemispheric climate. (Huybers and Denton)

  4. Austral spring insolation and sea salt flux correlate well.

  5. Spring insolation changes of up to 15–30 Wm-2 could have contributed to the Southern Hemispheric deglacial temperature rise between 20 and 10 ka BP. Blue:fixed angle season Black:fixed length season local spring mimumum insolation Blue:δD Black:CO2 variations

  6. *Model description • ECBilt-Clio • spectral T21, three-level quasigeostrophic model that is extended by diagnostic estimates of the neglected ageostrophic terms. • contains a full hydrological cycle • Synoptic variability associated with weather patterns is explicitly computed. • Diabatic heating due to radiative fluxes, the release of latent heat, and the exchange of sensible heat with the surface are parameterized, and cloudiness is prescribed. • The sea ice– ocean component CLIO consists of a free-surface primitive equation model with 3*3 resolution coupled to a thermodynamic–dynamic sea ice model.

  7. ECBilt , ERA40 and Observed Sea ice area Precip. Temp. 2m agree well with each other

  8. CO2 forcing starts to rise at 17 ka BP, which is basically consistent with Monnin et al. (2001). ORBonly incorporated the time-varying orbital forcing. GHGonly, only the observed temporal evolution of the atmospheric greenhouse gas concentrations was prescribed. TOPOonly is forced only by the time varying orographic and ice-sheet albedo effects in both the Northern and Southern Hemispheres.

  9. Results Austral spring 18-17ka rose AMOC(17ka) Summer Menviel et al. (2008) simulated a 20-ppmv increase of atmospheric CO2 in response to a complete shutdown of the AMOC.

  10. TS • First significant increase in the CO2 concentration occurring around 17 ka BP leads to a rapid warming of about 18C about 1–2 ka later than in the ORBonly experiment. • The CO2 forcing accounts for about 80% of the glacial–interglacial annual mean warming in ALL between 20 and 10 ka BP. GHGonly ORBonly

  11. Albedo • With only small seasonal variations. GHGonly TOPOonly

  12. TS Albedo ORBonly • Only orbital forcing leads to significant differences in the seasonal response. • Austral spring with a maximum temperature anomaly of about 4℃ occurring around 9 ka BP. • The sea ice evolution (Fig. 6f) does not directly follow the simulated temperature evolution. For example, strong summer sea ice response is not directly matched by a similarly strong summer temperature change. • (6f) sea ice start to retreat around 18 ka, about 1 ka earlier than in the GHGonly simulation.

  13. Temp. 2m Sea ice area Under present-day conditions, there is a typical phase lag of about 6–8 weeks between sea ice area and area averaged surface temperature (see Fig. 3). Temperature anomalies lead the sea ice anomalies by about 50–60 days, but eventually the resulting changes in sea ice albedo will also affect the temperature evolution, thereby providing a positive feedback. Temperature Positive feedback Sea ice albedo

  14. 13Wm-2 • In Fig. 8a, insolation variations in spring and summer oppose one another over the deglaciation. • The simulated albedo changes illustrated in Fig. 6f lead to large seasonal anomalies in absorbed shortwave radiation. Summer and spring are the dominant terms because they constitute the largest climatological incoming shortwave radiation changes. • The sum of the shortwave contributions shown in Fig. 8c closely matches the temperature evolution in Fig. 6e.

  15. feedbacks

  16. More longwave radiation is emitted from the surface. About ~ 0.5 Wm-2 Less than 0.5 Wm-2

  17. Conclusion • Spring solar insolation forcing increases substantially between 20 and 10 ka BP, leading to a reduction in sea ice area, and increased absorption of shortwave radiation. This warms the surface and leads to further sea ice reduction. • Recent paleoreconstructions of sea ice area changes (Shemesh et al. 2002; Bianchi and Gersonde 2004; Wolff et al. 2006) around Antarctica are consistent with the idea that spring insolation forcing is an important pacemaker for glacial–interglacial Southern Hemispheric climate change, as is further illustrated in Stott et al. (2007).

  18. * • In addition, the Northern Hemispheric warming between 21 and 18 ka BP may have destabilized the Laurentide ice sheet, resulting in a major freshwater discharge into the North Atlantic (Heinrich event I) and a subsequent weakening of the Atlantic Meridional Overturning Circulation. • A weakened overturning circulation may further increase the atmospheric CO2 due to oceanic or terrestrial processes

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