Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/18325
Share/Export:
logo share SHARE logo core CORE BASE
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE
Title

A dynamic explanation for the origin of the western Mediterranean organic-rich layers

AuthorsRogerson, M.; Cacho, Isabel; Jiménez Espejo, Francisco J.; Reguera, I.; Sierro, Francisco Javier; Martínez Ruíz, Francisca C. CSIC ORCID; Frigola, Jaime
Issue Date8-Jul-2008
PublisherAmerican Geophysical Union
AbstractThe eastern Mediterranean sapropels are amongst the most intensively investigated phenomena in the palaeoceanographic record , but relatively little has been written regarding the origin of the equivalent of the sapropels in the western Mediterranean, the Organic Rich Layers (ORL's). ORL's are recognised as sediment layers containing enhanced Total Organic Carbon that extend throughout the deep basins of the Western Mediterranean, and are associated with enhanced total barium concentration and a reduced diversity (dysoxic but not anoxic) benthic foraminiferal assemblage. Consequently, it has been suggested that ORL's represent periods of enhanced productivity coupled with reduced deep ventilation, presumably related to increased continental runoff, in close analogy to the sapropels. We demonstrate that despite their superficial similarity, the timing of the deposition of the most recent ORL in the Alboran Sea is different to that of the approximately coincident sapropel, indicating that there are important differences between their modes of formation. We go on to demonstrate, through physical arguments, that a likely explanation for the origin of the Alboran ORLs lies in the response of the Western Mediterranean basin to a strong reduction in surface water density and a shoaling of the interface between intermediate and deep water during the deglacial period. This moves the emphasis for forcing deep convection collapse in the western basins away from atmospheric forcing and towards changes in the residence time of water in the Mediterranean Sea (i.e. oceanic forcing). Furthermore, we provide evidence that deep convection had already slowed by the time of Heinrich Event 1, and explore this event as a potential agent for preconditioning deep convection collapse. Important differences between Heinrich-like and deglacial-like influences are highlighted, giving insight into the response of the western Mediterranean system to external forcing.
Publisher version (URL)http://dx.doi.org/10.1029/2007GC001936
URIhttp://hdl.handle.net/10261/18325
DOI10.1029/2007GC001936
Appears in Collections:(IACT) Artículos

Show full item record
Review this work

SCOPUSTM   
Citations

63
checked on May 25, 2022

WEB OF SCIENCETM
Citations

42
checked on May 24, 2022

Page view(s)

371
checked on May 26, 2022

Google ScholarTM

Check

Altmetric

Dimensions


WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.