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RADIOCARBON CALIBRATION: FROM BANE TO BLESSING

Published online by Cambridge University Press:  15 May 2023

Christopher Bronk Ramsey*
Affiliation:
University of Oxford, UK
*
*Corresponding author. Email: christopher.ramsey@arch.ox.ac.uk
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Abstract

Temporal and spatial variation in radiocarbon (14C) in the atmosphere has been the subject of investigation from the first pioneering work of Libby and Arnold. However, as the precision of measurements has improved, now by almost two orders of magnitude, what constitutes a significant variation has also changed. Furthermore, it has become possible to test degrees of variation over much longer timescales and with ever wider geographic coverage. As knowledge has improved, the interpretation of 14C measurements has had to be revised. These re-evaluations, and the loss of chronological precision that comes with accurate calibration, have often been seen as an unfortunate drawback in the 14C dating method. However, these problems have stimulated extensive research in global 14C records, statistical methods for dealing with complex 14C data, and measurement methods. This research has provided a wealth of information useful for other scientific challenges, most notably the quantification of the global carbon cycle, but also enabled, in the right circumstances, measurement precision an order of magnitude better than if there had been no variation in atmospheric 14C. Challenges remain but the research undertaken for 14C calibration has, through its ingenuity and innovation, provided rich scientific dividends in both chronology and broader geoscience.

Information

Type
Conference Paper
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of University of Arizona
Figure 0

Figure 1 This figure shows a comparison of the IntCal20 (Reimer et al. 2020) calibration curve (blue) with values under the assumption of a constant atmospheric radiocarbon ratio (red) as shown in Fig 1 of Arnold and Libby (1949) with an assumed uncertainty of 5% (400 radiocarbon years). It is only beyond about 5000 years that significant deviations are apparent. (Please see online version for color figures.)

Figure 1

Figure 2 Showing two places in the Holocene part of the calibration curve where the changes from IntCal13 (Reimer et al. 2013) shown in green to IntCal20 (Reimer et al. 2020) shown in blue are significant within the plotted 1σ error bands. These are examples of “unknown unknowns” (Jackson 2012) in the underlying data.

Figure 2

Figure 3 On the left it is clear that the radiocarbon date can be plotted as a function of age (data from IntCal20; Reimer et al. 2020) but that there is no inverse function. The plot also shows that much more of the age scale is taken up with plateaus than steep parts of the curve. The panel on the right shows why there is no calibration function because one radiocarbon date might be associated with multiple ages.

Figure 3

Figure 4 Annual data in the IntCal20 calibration curve (Reimer et al. 2020) surrounding the 774/5 solar event (Miyake et al. 2012) showing the high frequency components in the curve in this period.

Figure 4

Figure 5 All dating methods rely on changes in measured quantities relative to age. Purely radiometric methods, such as U-Th dating, make use of high precision measurements to track a simple decay process. Dendrochronology makes use only of the high-frequency component of the signal, and radiocarbon makes use of a much broader spectrum.