Particulate organic matter and ballast fluxes measured using time-series and settling velocity sediment traps in the northwestern Mediterranean Sea |
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| Authors: | Cindy Lee Michael L Peterson Stuart G Wakeham Robert A Armstrong J Kirk Cochran Juan Carlos Miquel Scott W Fowler David Hirschberg Aaron Beck Jianhong Xue |
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| Institution: | aMarine Sciences Research Center, Stony Brook University, Stony Brook, NY 11794-5000, USA;bSchool of Oceanography, University of Washington, Box 357940, Seattle, WA 98195-7940, USA;cSkidaway Institute of Oceanography, 10 Ocean Science Circle, Savannah, GA 31411, USA;dInternational Atomic Energy Agency, Marine Environment Laboratories, 4 Quai Antoine 1er, MC98000 Monaco |
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| Abstract: | Prompted by recent data analyses suggesting that the flux of particulate organic carbon sinking into deep waters is determined by fluxes of mineral ballasts, we undertook a study of the relationships among organic matter (OM), calcium carbonate, opal, lithogenic material, and excess aluminum fluxes as part of the MedFlux project. We measured fluxes of particulate components during Spring and Summer of 2003, and Spring of 2005, using a swimmer-excluding sediment trap design capable of measuring fluxes both in a time-series (TS) mode and in a configuration for obtaining particle settling velocity (SV) profiles. On the basis of these studies, we suggest that distinct OM–ballast associations observed in particles sinking at a depth of  200 m imply that the mechanistic basis of the organic matter–ballast association is set in the upper water column above the Twilight Zone, and that the importance of different ballast types follows the seasonal succession of phytoplankton. As in other studies, carbonate appears to enhance the flux of organic matter over opal. Particles must be at least half organic matter before their settling velocity is affected by ballast concentration. This lack of change in ballast composition with SV in particles with <40% OM content suggests that particle SV reaches a maximum because of the increasing importance of inertial drag. Relative amounts of OM and opal decrease with depth due to decomposition and dissolution; carbonates and lithogenic material contribute about the same amount to total mass, or increase slightly, throughout the water column. The high proportion of excess Al cannot be explained by its incorporation into diatom opal or reverse weathering, so Al is most likely adsorbed to particulate oxides. On shorter time scales, dust appears to increase particle flux through its role in aggregation rather than by nutrient inputs enhancing productivity. We suggest that the role of dust as a catalyst in particle formation may be a central mechanism in flux formation in this region, particularly when zooplankton fecal pellet production is low. |
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| Keywords: | MedFlux Organic carbon flux Opal flux Carbonate flux Ballast ratio hypothesis Mediterranean Sea biogeochemistry |
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