A Novel Approach Using Time-Depth Distortions to Assess Multicentennial Variability in Deep-Sea Oxygen Deficiency in the Eastern Mediterranean Sea During Sapropel S5

Jan Pieter Dirksen*, Rick Hennekam, Esmee Geerken, Gert-Jan Reichart

*Corresponding author for this work

Research output: Contribution to journalArticleAcademicpeer-review

Abstract

Reconstructing millennial- to centennial-scale climate variability for the Eemian—an interval with estimated sea surface temperatures ~0.5 °C warmer than “preindustrial”—requires records with high temporal resolution. Sapropel S5 sediments, deposited under anoxic conditions in the Eastern Mediterranean Sea, offer the rare opportunity to assess multicentennial climate variability during this time. Here we present high-resolution S5 piston core data from the Nile delta region. Specifically, we focus on Ba/Ti, Br/Ti, and Mo/Ti, as they are proxies for paleo-productivity, marine organic carbon, and sediment anoxia, respectively. A high correlation between our Ba/Ti values in core 64PE-406-E1 and well-dated Ba records of nearby cores (LC21 and ODP967) was found. We, therefore, tuned our data to these cores obtaining an initial age model. A time-frequency analyses indicated significant frequency content in the multicentennial band, although the frequency components drifted over time. Assuming spectral simplicity, we corrected for sedimentation rate changes on a multicentennial time scale. This novel approach grants a higher-resolution age model. The resulting variability in sedimentation rate is similar to records of monsoon variability, indicating a possible link between sedimentation at the core location and low-latitude monsoon variability, linked via the River Nile. Moreover, the periodicities found in the sapropel time series are similar to the frequency content of total solar irradiance and sunspot records known for the Holocene, at least at high frequencies (~50–150 years). Hence, our data suggest cyclic intrasapropel variability, at least during the deposition of sapropel S5, may be linked to solar cycles.

Original languageEnglish
Pages (from-to)774-786
Number of pages13
JournalPaleoceanography and Paleoclimatology
Volume34
Issue number5
DOIs
Publication statusPublished - May 2019

Funding

The authors would like to thank Rineke Gielens for helping with the XRF measurements. We acknowledge chief Scientist Marcel van der Meer and the crew of the R/V Pelagia for their extensive help during the first NESSC Mediterranean cruise. We would like to thank the editor (professor Stephen Barker), reviewer Gianluca Marino, and another anonymous reviewer for their constructive comments and recommendations. This work was carried out under the program of the Netherlands Earth System Science Centre (NESSC), financially supported by the Ministry of Education, Culture and Science (OCW; Grant 024.002.001) This research is made possible by financial support to the SCANALOGUE‐project (ALWOP.2015.113) by the Netherlands Organization for Scientific Research (NWO) and The Netherlands Research Centre for Integrated Solid Earth Science (ISES 2017‐UU‐23). The pub lished data are archived in the PANGAEA data repository (https://doi. pangaea.de/10.1594/ PANGAEA.899596).

Keywords

  • anoxia
  • Eastern Mediterranean Sea
  • Eemian
  • sapropel S5
  • solar cycles
  • X-ray fluorescence core scanning

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