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Please use this identifier to cite or link to this item: http://apo.ansto.gov.au/dspace/handle/10238/3041

Title: Atmospheric c-14 variations derived from tree rings during the early Younger Dryas.
Authors: Hua, Q
Barbetti, M
Fink, D
Kaiser, KF
Friedrich, M
Kromer, B
Levchenko, VA
Zoppi, U
Smith, AM
Bertuch, F
Keywords: Tree Rings
Carbon 14
Tasmania
Isotope Dating
Water Currents
Atmospheric Circulation
Issue Date: Dec-2009
Publisher: Elsevier
Citation: Hua, Q., Barbetti, M., Fink, D., Kaiser, K. F., Friedrich, M., Kromer, B., et al. (2009). Atmospheric c-14 variations derived from tree rings during the early Younger Dryas. Quaternary Science Reviews, 28(25-26), 2982-2990.
Abstract: Atmospheric radiocarbon variations over the Younger Dryas interval, from ~13,000 to 11,600 cal yr BP, are of immense scientific interest because they reveal crucial information about the linkages between climate, ocean circulation and the carbon cycle. However, no direct and reliable atmospheric 14C records based on tree rings for the entire Younger Dryas have been available. In this paper, we present (1) high-precision 14C measurements on the extension of absolute tree-ring chronology from 12,400 to 12,560 cal yr BP and (2) high-precision, high-resolution atmospheric 14C record derived from a 617-yr-long tree-ring chronology of Huon pine from Tasmania, Australia, spanning the early Younger Dryas. The new tree-ring 14C records bridge the current gap in European tree-ring radiocarbon chronologies during the early Younger Dryas, linking the floating Lateglacial Pine record to the absolute tree-ring timescale. A continuous and reliable atmospheric 14C record for the past 14,000 cal yr BP including the Younger Dryas is now available. The new records indicate that the abrupt rise in atmospheric Δ14C associated with the Younger Dryas onset occurs at ~12,760 cal yr BP, ~240 yrs later than that recorded in Cariaco varves, with a smaller magnitude of ~40‰ followed by several centennial Δ14C variations of 20–25‰. Comparing the tree-ring Δ14C to marine-derived Δ14C and modelled Δ14C based on ice-core 10Be fluxes, we conclude that changes in ocean circulation were mainly responsible for the Younger Dryas onset, while a combination of changes in ocean circulation and 14C production rate were responsible for atmospheric Δ14C variations for the remainder of the Younger Dryas. © 2009, Elsevier Ltd.
URI: http://dx.doi.org/10.1016/j.quascirev.2009.08.013
http://apo.ansto.gov.au/dspace/handle/10238/3041
ISSN: 0277-3791
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