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. 2019 Nov 28;9:17829. doi: 10.1038/s41598-019-53583-7

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© The Author(s) 2019

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

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RMD1 proxies vs. age. From bottom: δ¹⁸O; δ¹³C, growth rate; [²³⁰Th/²³²Th] for the dated points; filtered mass magnetic susceptibility (χ) series representing the background magnetic flux (BMF, see text for details), light-blue bars are the χ peaks >12 m³ kg⁻¹ indicating the spikes of coarser material. Rectangles indicate the spikes in BMF, yellow: spikes characterized by a similar behaviour of δ¹³C and δ¹⁸O; blue: intervals where δ¹³C and δ¹⁸O show an opposite pattern.