Radiocarbon: A key tracer for studying Earth’s dynamo, climate system, carbon cycle, and Sun

Author:

Heaton T. J.1ORCID,Bard E.2ORCID,Bronk Ramsey C.3ORCID,Butzin M.4ORCID,Köhler P.4ORCID,Muscheler R.5ORCID,Reimer P. J.6ORCID,Wacker L.7ORCID

Affiliation:

1. School of Mathematics and Statistics, University of Sheffield, Sheffield S3 7RH, UK.

2. CEREGE, Aix-Marseille University, CNRS, IRD, INRAE, Collège de France, Technopole de l’Arbois BP 80, 13545 Aix-en-Provence Cedex 4, France.

3. Research Laboratory for Archaeology and the History of Art, University of Oxford, Oxford OX1 3TG, UK.

4. Alfred-Wegener-Institut Helmholtz-Zentrum für Polar- und Meeresforschung (AWI), D-27515 Bremerhaven, Germany.

5. Quaternary Sciences, Department of Geology, Lund University, 223 62 Lund, Sweden.

6. 14CHRONO Centre for Climate, the Environment and Chronology, School of Natural and Built Environment, Queen’s University, Belfast BT7 1NN, UK.

7. Laboratory of Ion Beam Physics, ETH Zürich, CH-8093 Zürich, Switzerland.

Abstract

Using carbon-14 Carbon-14 or radiocarbon, a radioactive isotope produced in the upper atmosphere by cosmic rays, is rapidly incorporated into the terrestrial carbon cycle and provides a way to calculate the age of carbon-bearing materials as old as 55,000 years. Heaton et al . review recent progress that has allowed the construction of better radiocarbon age calibration curves and discuss the new insights into climate processes, the Sun, Earth’s geodynamo, and the carbon cycle that have emerged from these efforts. —HJS

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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