Ventilation of the Deep Southern Ocean and Deglacial CO 2 Rise

Author:

Skinner L. C.1,Fallon S.2,Waelbroeck C.3,Michel E.3,Barker S.4

Affiliation:

1. Godwin Laboratory for Palaeoclimate Research, Department of Earth Sciences, University of Cambridge, Downing Street, Cambridge CB2 3EQ, UK.

2. Research School of Earth Sciences, Australian National University (ANU), Canberra ACT 0200, Australia.

3. Laboratoire des Sciences du Climat et l'Environnement/Institut Pierre-Simon Laplace, Laboratoire CNRS-CEA-UVSQ, Bâtiment 12, Avenue de la Terrasse, F-91198, Gif-sur-Yvette Cedex, France.

4. School of Earth and Ocean Sciences, Cardiff University, Cardiff CF10 3YE, UK.

Abstract

Telling Up from Down It is generally believed that carbon dioxide accumulates in the deep ocean during cold periods and that it is released rapidly and in huge quantities during deglaciation, but evidence of deep ocean carbon dioxide storage has been elusive. Now Skinner et al. (p. 1147 ; see the Perspective by Anderson and Carr ) present radiocarbon data from the Southern Ocean that indicate that the deep water circulating around Antarctica was about twice as old relative to the atmosphere as it is today, a condition considered indicative of carbon dioxide accumulation and storage.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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