Reconstruction of Cenozoic δ11Bsw Using a Gaussian Process

Author:

Whiteford Ross1ORCID,Heaton Timothy J.2ORCID,Henehan Michael J.3ORCID,Anagnostou Eleni4ORCID,Jurikova Hana1,Foster Gavin L.5,Rae James W. B.1ORCID

Affiliation:

1. School of Earth and Environmental Sciences University of St Andrews St Andrews UK

2. Department of Statistics School of Mathematics University of Leeds Leeds UK

3. School of Earth Sciences University of Bristol Bristol UK

4. GEOMAR Helmholtz Centre for Ocean Research Kiel Kiel Germany

5. School of Ocean Earth Science University of Southampton Southampton UK

Abstract

AbstractThe boron isotope ratio of seawater (δ11Bsw) is a parameter which must be known to reconstruct palaeo pH and CO2 from boron isotope measurements of marine carbonates. Beyond a few million years ago, δ11Bsw is likely to have been different to modern. Palaeo δ11Bsw can be estimated by simultaneously constraining the vertical gradients in foraminiferal δ11B (Δδ11B) and pH (ΔpH). A number of subtly different techniques have been used to estimate ΔpH in the past, all broadly based on assumptions about vertical gradients in oxygen, and/or carbon, or other carbonate system constraints. In this work we pull together existing data from previous studies, alongside a constraint on the rate of change of δ11Bsw from modeling. We combine this information in an overarching statistical framework called a Gaussian Process. The Gaussian Process technique allows us to bring together data and constraints on the rate of change in δ11Bsw to generate random plausible evolutions of δ11Bsw. We reconstruct δ11Bsw, and by extension palaeo pH, across the last 65Myr using this novel methodology. Reconstructed δ11Bsw is compared to other seawater isotope ratios, namely , , and δ7Li, which we also reconstruct with Gaussian Processes. Our method provides a template for incorporation of future δ11Bsw constraints, and a mechanism for propagation of uncertainty in δ11Bsw into future studies.

Publisher

American Geophysical Union (AGU)

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