EGU24-19442, updated on 31 Mar 2024
https://doi.org/10.5194/egusphere-egu24-19442
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Strength variability of the Mediterranean Outflow Water during late Quaternary: Preliminary results from IODP Site U1588

Jiawang Wu1,2, Xinyang Chen1, Zongxian He1, Qin Deng1, Lifeng Zhong2, Xiaolei Pang3, David Hodell4, Fatima Abrantes5, Carlos Alvarez Zarikian6, and the Expedition 397 Scientific Party*
Jiawang Wu et al.
  • 1School of Marine Sciences, Sun Yat-Sen University, Guangdong, China
  • 2Southern Marine Science and Engineering Guangdong Laboratory (Zhuhai), Guangdong, China
  • 3Institute of Ocean Research, Peking University, Beijing, China
  • 4Department of Earth Sciences, University of Cambridge, Cambridge, UK
  • 5Portuguese Institute of the Sea and Atmosphere (IPMA), Lisbon, Portugal
  • 6International Ocean Discovery Program, Texas A&M University, College Station, Texas, USA
  • *A full list of authors appears at the end of the abstract

The Mediterranean Sea is thought to play a role in changing past ocean circulation and North Atlantic climate, through the outflow of warm, saline intermediate waters (Mediterranean Outflow Water; MOW) into the North Atlantic. Previous studies mostly focused on the Gulf of Cádiz, immediately after the MOW existing the Mediterranean, but how the MOW varied along the northward transport is still unclear. Fine grain-size parameters have been widely employed to infer paleo-flow speeds of near-bottom currents in the deep sea, in particular the terrigenous non-cohesive “sortable silt” (denoted as SS) controlled by selective deposition. Here we present terrigenous sediment grain size results on IODP Site U1588 (37°57.61′N, 9°30.99′W, 1339 m water depth), which was retrieved from the Iberian Margin during the IODP Expedition 397. Our aim is to reconstruct strength variations in the lower branch of the MOW over the past ~250,000 years. After removing organic matter (leached with 10% H2O2 at 85 ℃) and marine carbonates (leached with 0.5 M HCl), the terrigenous detrital component of about 100 samples were measured on a Malvern Mastersizer 3000 instrument. Our grain-size results show a bimodal distribution, with a small peak near 1 μm and the main mode between 5–8 μm. The correlation between the percentage and mean of the sortable silt fraction (10–63 μm) is significant (R2=0.43, P<0.01), permitting the use of SS-mean as a reliable indicator of the deep-sea current strength. The calculated SS-mean is from ~14.2 to 18.2 μm, corresponding to the flow speed of ~3.3 to 10.2 cm/s. Based on the shipboard age model, our results show a persistent low-latitude forcing of MOW flow speed over the past 250,000 years, with strong precessional and glacial cycles.

Expedition 397 Scientific Party:

David A. Hodell, Fatima F. Guedes Abrantes, Carlos A. Alvarez Zarikian, Hannah L. Brooks, William B. Clark, Louise F.B. Dauchy-Tric, Viviane dos Santos Rocha, José-Abel Flores Villarejo, Timothy D. Herbert, Sophia K.V. Hines, Huai-Hsuan May Huang, Hisashi Ikeda, Stefanie Kaboth-Bahr, Junichiro Kuroda, Jasmin M. Link, Jerry F. McManus, Bryce A. Mitsunaga, Lucien Nana Yobo, Celeste T. Pallone, Xiaolei Pang, Marion Y. Peral, Saray Sanchez, Komal Verma, Jiawang Wu, Chuang Xuan, Jimin Yu.

How to cite: Wu, J., Chen, X., He, Z., Deng, Q., Zhong, L., Pang, X., Hodell, D., Abrantes, F., and Zarikian, C. A. and the Expedition 397 Scientific Party: Strength variability of the Mediterranean Outflow Water during late Quaternary: Preliminary results from IODP Site U1588, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-19442, https://doi.org/10.5194/egusphere-egu24-19442, 2024.