4.7 Article

Towards radiocarbon calibration beyond 28 ka using speleothems from the Bahamas

Journal

EARTH AND PLANETARY SCIENCE LETTERS
Volume 289, Issue 1-2, Pages 1-10

Publisher

ELSEVIER
DOI: 10.1016/j.epsl.2009.10.004

Keywords

radiocarbon; U-Th dating; speleothems; MIS 3; geomagnetic intensity; earth system models

Funding

  1. NERC [NER/A/S/2001/00526]
  2. Leverhulme Trust [F/00 182/AU]
  3. NSF [EAR0223311, EAR0446861, EAR0622305]
  4. Natural Environment Research Council [ESM010002, NE/C515904/1] Funding Source: researchfish
  5. NERC [ESM010002, NE/C515904/1] Funding Source: UKRI

Ask authors/readers for more resources

We present a new speleothem record of atmospheric Delta C-14 between 28 and 44 ka that offers considerable promise for resolving some of the uncertainty associated with existing radiocarbon calibration curves for this time period. The record is based on a comprehensive suite of AMS C-14 ages, using new low-blank protocols, and U-Th ages using high precision MC-ICPMS procedures. Atmospheric Delta C-14 was calculated by correcting C-14 ages with a constant dead carbon fraction (DCF) of 22.7 +/- 5.9%, based on a comparison of stalagmite C-14 ages with the lntCal04 (Reimer et al., 2004) calibration curve between 15 and 11 ka. The new Delta C-14 speleothem record shows similar structure and amplitude to that derived from Cariaco Basin foraminifera (Hughen et al., 2004, 2006), and the match is further improved if the latter is tied to the most recent Greenland ice core chronology (Svensson et al., 2008). These data are however in conflict with a previously published C-14 data set for a stalagmite record from the Bahamas - CB-89-24-1 (Beck et al., 2001), which likely suffered from C-14 analytical blank subtraction issues in the older part of the record. The new Bahamas speleothem. Delta C-14 data do not show the extreme shifts between 44 and 40 ka reported in the previous study (Beck et al., 2001). Causes for the observed structure in derived atmospheric Delta C-14 variation based on the new speleothem data are investigated with a suite of simulations using an earth system model of intermediate complexity. Data-model comparison indicates that major fluctuations in atmospheric Delta C-14 during marine isotope stage 3 is primarily a function of changes in geomagnetic field intensity, although ocean-atmosphere system reorganisation also played a supporting role. (C) 2009 Elsevier B.V. All rights reserved.

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