Inverse response of 231Pa/230Th to variations of the Atlantic meridional overturning circulation in the North Atlantic intermediate water

• Main Authors: Süfke, Finn, Schulz, Hartmut, Scheen, Jeemijn, Szidat, Sönke, Regelous, Marcel, Blaser, Patrick, Pöppelmeier, Frerk, Goepfert, Tyler J., Stocker, Thomas F., Lippold, Jörg
• Format: Text
• Language: English
• Published: Springer
• Subjects: 530 Physics; 540 Chemistry; 550 Earth sciences & geology; North Atlantic
• Online Access: https://dx.doi.org/10.7892/boris.141787; https://boris.unibe.ch/141787/

This study aims to provide a more detailed understanding of the behavior of ²³¹Pa/²³⁰Th under varying ocean circulation regimes. The North Atlantic provides a unique sedimentary setting with its ice-rafted detritus (IRD) layers deposited during glacial times. These layers have been found north of 40° N (Ruddiman Belt) and are most pronounced during Heinrich Stadials. Most of these sediments have been recovered from the deep North Atlantic basin typically below 3000 m water depth. This study reports sedimentological and sediment geochemical data from one of the few sites at intermediate depth of the open North Atlantic (core SU90-I02, 45° N 39° W, 1965 m water depth) within the Ruddiman Belt. The time periods of Heinrich Stadials 1 and 2 of this core were identified with the help of the major element composition by XRF scanning and by IRD counting. Along the core profile, the sedimentary ²³¹Pa/²³⁰Th activity ratio has been measured as a kinematic proxy for the circulation strength. The ²³¹Pa/²³⁰Th record shows highest values during the Holocene and Last Glacial Maximum, above the natural production ratio of these isotopes. During Heinrich Stadials 1 and 2, when Atlantic meridional overturning circulation was most reduced, the ²³¹Pa/²³⁰Th record shows overall lowest values below the production ratio. This behavior is contrary to classical findings of ²³¹Pa/²³⁰Th from the northwestern Atlantic where a strong Holocene circulation is associated with low values. However, this behavior at the presented location is in agreement with results from simulations of the ²³¹Pa/²³⁰Th-enabled Bern3D Earth system model.