Global ocean response to orbital forcing in the Holocene

98Citations
Citations of this article
124Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

Global upper ocean evolution in the Holocene is studied in two coupled ocean-atmosphere models under orbital forcing conditions at 3, 6, 8, and 11 ka. The annual mean sea surface temperature (SST) changes in the early to mid-Holocene are found to be forced mainly by the annual mean insolation forcing with an overall symmetric response of colder equator (<0.5°C)/warmer high latitudes (<0.4°C in the Southern Ocean and >1°C in the Arctic). This SST change is consistent with a synthesis of mid-Holocene paleo-SST records. In contrast, the temperature response in the thermocline is dominated by an antisymmetric pattern with a cooling (warming) in the Northern (Southern Hemisphere midlatitudes. The thermocline response is determined predominantly by surface water subduction, and ultimately, the insolation forcing in local late winter.

Cite

CITATION STYLE

APA

Liu, Z., Brady, E., & Lynch-Stieglitz, J. (2003). Global ocean response to orbital forcing in the Holocene. Paleoceanography, 18(2). https://doi.org/10.1029/2002PA000819

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free