A global glacial ocean state estimate constrained by upper-ocean temperature proxies

dc.contributor.author Amrhein, Daniel E.
dc.contributor.author Wunsch, Carl
dc.contributor.author Marchal, Olivier
dc.contributor.author Forget, Gael
dc.date.accessioned 2018-09-17T17:13:48Z
dc.date.available 2018-09-17T17:13:48Z
dc.date.issued 2018-08-28
dc.description Author Posting. © American Meteorological Society, 2018. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Climate 31 (2018): 8059-8079, doi:10.1175/JCLI-D-17-0769.1. en_US
dc.description.abstract We use the method of least squares with Lagrange multipliers to fit an ocean general circulation model to the Multiproxy Approach for the Reconstruction of the Glacial Ocean Surface (MARGO) estimate of near sea surface temperature (NSST) at the Last Glacial Maximum (LGM; circa 23–19 thousand years ago). Compared to a modern simulation, the resulting global, last-glacial ocean state estimate, which fits the MARGO data within uncertainties in a free-running coupled ocean–sea ice simulation, has global-mean NSSTs that are 2°C lower and greater sea ice extent in all seasons in both the Northern and Southern Hemispheres. Increased brine rejection by sea ice formation in the Southern Ocean contributes to a stronger abyssal stratification set principally by salinity, qualitatively consistent with pore fluid measurements. The upper cell of the glacial Atlantic overturning circulation is deeper and stronger. Dye release experiments show similar distributions of Southern Ocean source waters in the glacial and modern western Atlantic, suggesting that LGM NSST data do not require a major reorganization of abyssal water masses. Outstanding challenges in reconstructing LGM ocean conditions include reducing effects from model biases and finding computationally efficient ways to incorporate abyssal tracers in global circulation inversions. Progress will be aided by the development of coupled ocean–atmosphere–ice inverse models, by improving high-latitude model processes that connect the upper and abyssal oceans, and by the collection of additional paleoclimate observations. en_US
dc.description.sponsorship DEA was supported by a NSF Graduate Research Fellowship and NSF Grant OCE-1060735. OM acknowledges support from the NSF. GF was supported by NASA Award 1553749 and Simons Foundation Award 549931. en_US
dc.identifier.citation Journal of Climate 31 (2018): 8059-8079 en_US
dc.identifier.doi 10.1175/JCLI-D-17-0769.1
dc.identifier.uri https://hdl.handle.net/1912/10576
dc.language.iso en_US en_US
dc.publisher American Meteorological Society en_US
dc.relation.uri https://doi.org/10.1175/JCLI-D-17-0769.1
dc.subject Ocean en_US
dc.subject Abyssal circulation en_US
dc.subject Sea surface temperature en_US
dc.subject Paleoclimate en_US
dc.subject Inverse methods en_US
dc.subject Ocean models en_US
dc.title A global glacial ocean state estimate constrained by upper-ocean temperature proxies en_US
dc.type Article en_US
dspace.entity.type Publication
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